| 10 ton asteroid impact | has average interval time 1 year |  |
| is a kind of asteroid impact |  |
| 100 ton asteroid impact | has average interval time 10 years |  |
| is a kind of asteroid impact |  |
| 1000 ton asteroid impact | has average interval time 100 years |  |
| is a kind of asteroid impact |  |
| 16th century scientist | has definition a scientist born between 1500 and 1600 AD |  |
| is a kind of dead person |  |
| is a kind of scientist |  |
| 17 Leporis | has companion M1 III | ![has source: [H76], 2001-09-19 14:35:30.0](facet.gif) |
| has definition A close binary system (A0 V, M1 III) with a shell-like spectrum indicating that mass transfer may be occurring from the late-type companion onto the A0 primary. | ![has source: [H76], 2001-09-19 14:35:30.0](facet.gif) |
| has primary A0 V | ![has source: [H76], 2001-09-19 14:35:30.0](facet.gif) |
| is a part of Lepus | ![has source: [H76], 2001-09-19 14:35:30.0](facet.gif) |
| is an instance of binary star |  |
| is an instance of shell star |  |
| 17th century scientist | has definition a scientist born between 1600 and 1700 AD |  |
| is a kind of dead person |  |
| is a kind of scientist |  |
| 18th century scientist | has definition a scientist born between 1700 and 1800 AD |  |
| is a kind of dead person |  |
| is a kind of scientist |  |
| 19th century scientist | has definition a scientist born between 1800 and 1900 AD |  |
| is a kind of dead person |  |
| is a kind of scientist |  |
| 2-meter Telescope | has altitude 331 m |  |
| has aperture 1.34 m |  |
| has comment can also be used in Cassegrain and coude modes |  |
| has creation date 1960 |  |
| has focal ratio f/3.00 |  |
| has has mirror diameter 2 m |  |
| has latitude 50° 59' N |  |
| has location Tautenberg, Germany |  |
| has longitude 11° 43'E |  |
| has mirror maker Zeiss (Jena) |  |
| has mirror type Schott ZK-7 glass |  |
| has mounting manufacturer Zeiss (Jena) |  |
| has owner Karl Schwarzschild Observatorium |  |
| has synonym Tautenberg Schmidt |  |
| is an instance of Fork equatorial telescope |  |
| is an instance of Schmidt |  |
| 2.3-meter Telescope | has altitude 725 m |  |
| has aperture 2.33 m |  |
| has creation date 1985 |  |
| has focal ratio f/3.25, 13, 43 |  |
| has latitude 12° 35' N |  |
| has location Kavalur, Tamil Nadu, India |  |
| has longitude 78° 50' E |  |
| has mirror maker Indian Inst. Astrophys. |  |
| has mirror type Zerodur |  |
| has mounting manufacturer Walchandnagar Industries |  |
| has owner Vainu Bappu Observatory |  |
| has synonym Vainu Bappu 2.3 m |  |
| is an instance of Horseshoe equatorial telescope |  |
| is an instance of optical telescope |  |
| is an instance of reflector |  |
| 20th century scientist | has definition a scientist born between 1900 and 2000 AD |  |
| is a kind of scientist |  |
| 26-inch Equatorial | has altitude 92 m |  |
| has aperture 0.66 m |  |
| has creation date 1873 |  |
| has focal ratio f/15.0 |  |
| has latitude 38° 55' N |  |
| has lens maker Alvan Clark & Sons |  |
| has location Washington, DC, US |  |
| has longitude 77° 04' W |  |
| has mounting manufacturer Warner and Swasey |  |
| has owner US Naval Observatory |  |
| is an instance of German equatorial telescope |  |
| is an instance of refractor |  |
| 28-inch Visual Refractor | has altitude 47 m |  |
| has aperture 0.711 m |  |
| has comment Dome under repair in 1992 |  |
| has creation date 1894 |  |
| has focal ratio f/11.9 |  |
| has latitude 51° 29' N |  |
| has lens maker Gmbh |  |
| has location Greenwich, London, England |  |
| has longitude 00° 00' |  |
| has mounting manufacturer Ransomes and Sims |  |
| has owner Old Royal Observatory |  |
| has synonym Greenwich refractor |  |
| is an instance of English equatorial telescope |  |
| is an instance of refractor |  |
| 2U 1543-47 | is an instance of transient X-ray source | ![has source: [H76], 2001-09-19 14:35:23.0](facet.gif) |
| 3 alpha process | has definition A nuclear reaction (3 4He → 12C + γ + 7 MeV) by which helium is transformed into carbon. The process is dominant in red giants. At a temperature of about 2 × 108 K and a density of 105 g cm-3, after core hydrogen is exhausted, three α-particles can fuse to form an excited nucleus of carbon 12, which occasionally decays into a stable carbon 12 nucleus. The overall process can be looked upon as an equilibrium between three helium nuclei and the excited 12C*, with occasional irreversible leakage out of the equilibrium into the ground state of carbon 12. Further capture of α-particles by carbon 12 nuclei produces oxygen 16 and neon 20. (also called the triple-α process) | ![has source: [H76], 2001-09-19 14:34:40.0](facet.gif) |
| is a kind of nucleosynthetic reaction |  |
| 3-kpc arm | has definition A component of the Sagittarius arm with noncircular gas motions. It is seen in absorption against Sgr A with a velocity of -53 km s-1, implying that at least part of the arm is expanding away from the galactic center. The nearest "edge" is presently at a radius of 4 kpc from the Galactic center. | ![has source: [H76], 2001-09-19 14:37:14.0](facet.gif) |
| is a part of Sagittarius arm | ![has source: [H76], 2001-09-19 14:37:14.0](facet.gif) |
| 3.5-meter Telescope | has altitude 2168 m |  |
| has aperture 3.50 m |  |
| has creation date 1984 |  |
| has focal ratio f/3.5, 3.9, 10, 35 |  |
| has latitude 37° 13' N |  |
| has location Calar Alto, Spain |  |
| has longitude 2° 32' W |  |
| has mirror maker Zeiss (Ober.) |  |
| has mirror type Zerodur |  |
| has mounting manufacturer Voith, Heidenheim; Zeiss (Ober.) |  |
| has operator German-Spanish Astronomical Center |  |
| has owner Calar Alto Observatory |  |
| is an instance of Horseshoe equatorial telescope |  |
| is an instance of optical telescope |  |
| is an instance of Ritchey-Chrétien |  |
| 30 Doradus Nebula | has absolute magnitude Mv = - 19 |  |
| has definition A giant H II region, at least 300 pc across - one of the largest known. It is larger and more luminous than any known in the Galaxy. It is the brightest object in the Large Magellanic Cloud at both optical and radio wavelengths, and contains the densest concentration of W-R stars. (The brightest object near the center is a O+ WN star of Mv = - 10.2.) It is characterized by very rapid, disordered, and complex motions. | ![has source: [H76], 2001-09-19 14:35:20.0](facet.gif) |
| has distance 170000 light years |  |
has image  |  |
| has synonym Great Looped Nebula | ![has source: [H76], 2001-09-19 14:35:20.0](facet.gif) |
| has synonym NGC 2070 |  |
| has synonym Tarantula Nebula | ![has source: [H76], 2001-09-19 14:35:20.0](facet.gif) |
| is a part of Large Magellanic Cloud |  |
| is an instance of gaseous nebula |  |
| 36-inch Refractor | has altitude 1290 m |  |
| has aperture 0.895 m |  |
| has comment Front surface of crown element refigured in 1987 |  |
| has creation date 1888 |  |
| has focal ratio f/19.7 |  |
| has latitude 37° 20' N |  |
| has lens maker Alvan Clark & Sons |  |
| has location Mount Hamilton, Calif., US |  |
| has longitude 121° 39' W |  |
| has mounting manufacturer Warner and Swasey |  |
| has owner Lick Observatory |  |
| has synonym 36 inch |  |
| is an instance of German equatorial telescope |  |
| is an instance of refractor |  |
| 3TA-10 Schmidt Telescope | has altitude 1450 m |  |
| has aperture 1.00 m |  |
| has comment three 1 m diameter objective prisms |  |
| has creation date 1961 |  |
| has focal ratio f/2.13 |  |
| has latitude 40° 20' N |  |
| has location Mount Aragatz, Armenia |  |
| has longitude 44° 30' E |  |
| has mirror diameter 1.5 m |  |
| has mirror maker LOMO |  |
| has mounting manufacturer LOMO |  |
| has owner Byurakan Astrophysical Observatory |  |
| has synonym Byurakan Schmidt |  |
| is an instance of Schmidt |  |
| 4-kpc arm | has definition A component of the Sagittarius arm with noncircular gas motions. | ![has source: [H76], 2001-09-19 14:37:14.0](facet.gif) |
| is a part of Sagittarius arm |  |
| 40 Eridani | has definition A nearby triple system, 5 pc distant. Component A is K0 V; component B is a DA white dwarf; component C is M5e V. | ![has source: [H76], 2001-09-19 14:35:32.0](facet.gif) |
| is a part of Eridanus |  |
| is an instance of triple star |  |
| 47 Tucanae | has definition A metal-rich globular cluster. It has roughly one-quarter the solar metal abundance. It has a high galactic latitude and low reddening. It is a member of the thick-disk population. | ![has source: [H76], 2001-09-19 14:36:06.0](facet.gif) |
| has distance 15000 light years |  |
has image  |  |
| is a part of halo |  |
| is a part of Tucana |  |
| is an instance of unclassified globular cluster |  |
| 4N nucleus | has definition Nuclei possessing equal and even numbers of neutrons and protons. 4N nuclei are formed in supernova envelopes at temperatures of at least 2 × 109 K and are very stable. | ![has source: [H76], 2001-09-19 14:33:17.0](facet.gif) |
| has synonym even-even nucleus |  |
| is a kind of Bose-Einstein nucleus |  |
| 53 Arietis | has definition Runaway star which diverges from a comparatively small area in Orion. | ![has source: [H76], 2001-09-19 14:35:45.0](facet.gif) |
| is a part of Aries | ![has source: [H76], 2001-09-19 14:35:45.0](facet.gif) |
| is an instance of runaway star | ![has source: [H76], 2001-09-19 14:35:45.0](facet.gif) |
| 61 Cygni | has definition The first star other than the Sun to have its parallax, and hence distance, measured. The star is a double orange dwarf. | ![has source: [C95], 2001-09-19 14:35:26.0](facet.gif) |
| has distance 11.4 light-years | ![has source: [C95], 2001-09-19 14:35:26.0](facet.gif) |
| is a part of Cygnus | ![has source: [C95], 2001-09-19 14:35:26.0](facet.gif) |
| is an instance of high proper motion star |  |
| [O III] line | is a kind of forbidden line |  |
| [WR] star | has definition WR star that is the central object of a planetary nebula. | ![has source: [JJ95], 2001-09-19 14:35:31.0](facet.gif) |
| is a kind of Wolf-Rayet |  |
| A band | has definition One of about a dozen of the strongest Fraunhofer lines seen in the Solar spectrum, the A band at 7600 angstoms is due to telluric lines of molecular oxygen in the Earth's atmosphere. (originally thought to originate in the Sun by Fraunhofer) |  |
| has species O2 |  |
| has wavelength 7600 Å |  |
| is a kind of Fraunhofer line |  |
| is a kind of molecular band |  |
| occurs in Earth's atmosphere |  |
| A ring | is a kind of ring |  |
| is a part of Saturn ring system |  |
| A star | has absorption line H I |  |
| has color white |  |
| has definition Star with spectral type A in which the spectrum of the Balmer lines of hydrogen attain their greatest strength. Helium lines can no longer be seen. Some metallic lines are present; in late A stars the H and K lines of ionized calcium appear. A0 stars have a color index of zero. | ![has source: [H76], 2001-09-19 14:35:46.0](facet.gif) |
| has surface temperature 10000 K |  |
| is a kind of early star |  |
| ablation | has definition Removal of material from a solid by heating, vaporization or collisions | ![has source: [T01], 2001-09-19 14:34:39.0](facet.gif) |
| has example Erosion of a meteorite by the friction generated when it passes through the Earth's atmosphere. The material passes from solid to gas phase. | ![has source: [H76], 2001-09-19 14:34:39.0](facet.gif) |
| has final phase gas |  |
| has initial phase solid |  |
| has inverse process condensation |  |
| is a kind of first order phase transition |  |
| absolute magnitude | has definition A measure of the intrinsic brightness of a star or galaxy. Absolute magnitude is defined as the apparent magnitude the star or galaxy would have if it were 32.6 light-years (10 parsecs) from Earth. The lower an object's absolute magnitude, the greater its intrinsic brightness. For example, the Sun has an absolute magnitude of +4.83, while Sirius, whose intrinsic brightness is greater, has an absolute magnitude of +1.43. A star that is one absolute magnitude brighter than another (e.g., +4 versus +5) is 2.5 times intrinsically brighter; a star that is 5 absolute magnitudes brighter is 100 times intrinsically brighter; and a star that is 10 absolute magnitudes brighter is 10000 times intrinsically brighter. | ![has source: [C95], 2001-09-19 14:38:08.0](facet.gif) |
| has definition The absolute magnitude (g) of a solar-system body such as an asteroid is defined as the brightness at zero phase angle when the object is 1 AU from the Sun and 1 AU from the observer. | ![has source: [H76], 2001-09-19 14:38:08.0](facet.gif) |
| is a kind of magnitude |  |
| absolute temperature | has definition Temperature measured on the Kelvin scale: 0 Kelvin = -273.15 ° Celsius. Absolute temperature is directly related to (kinetic) energy via the equation E = kBT, where kB is Boltzmann's constant. So, a temperature of 0 K corresponds to zero energy, and room temperature, 300 K = 27 °C, corresponds to an energy of 0.025 eV. | ![has source: [CD99], 2001-09-19 14:38:04.0](facet.gif) |
| is a kind of temperature |  |
| absolute zero | has definition The lowest possible temperature, attained when a system is at its minimum possible energy. The Kelvin temperature scale sets its zero point at absolute zero (-273.15° on the Celsius scale, and -434.07° on the Fahrenheit scale). | ![has source: [HH98], 2001-09-19 14:38:04.0](facet.gif) |
| is an instance of temperature |  |
| absorption | has definition Decrease in the intensity of radiation, representing energy converted into excitation or ionization of electrons in the region through which the radiation travels. As contrasted with monochromatic scattering (in which reemission occurs in all directions at the same frequency), the inverse process of emission refers to radiation that is reemitted in general in all directions and at all frequencies. | ![has source: [H76], 2001-09-19 14:34:44.0](facet.gif) |
| has inverse process emission |  |
| is a kind of radiation intensity modification |  |
| absorption edge | has definition Sudden rises superposed on the smooth decrease of the curve of the attenuation coefficient, which cause the curve to have a typical sawtooth aspect. They generally occur at the limit of spectral lines. | ![has source: [H76], 2001-09-19 14:38:12.0](facet.gif) |
| is a kind of spectral feature |  |
| absorption line | has antonym emission line |  |
| has definition Dark line in a spectrum, produced when light or other electromagnetic radiation coming from a distant source passes through a gas cloud or similar object closer to the observer. Like emission lines, absorption lines betray the chemical composition and velocity of the material that produces them. | ![has source: [F88], 2001-09-19 14:38:15.0](facet.gif) |
| has definition Dark line superposed on a continuous spectrum, caused by the absorption of light passing through a gas of lower temperature than the continuum light source. | ![has source: [H76], 2001-09-19 14:38:15.0](facet.gif) |
| is a kind of spectral line |  |
| abstraction | has definition a general concept formed by extracting common features from specific examples |  |
| is a kind of kbTop |  |
| acceleration unit | has definition meter per second squared |  |
| has symbol m·s-2 |  |
| is a kind of derived SI unit |  |
| accretion | has definition A process by which a star accumulates matter as it moves through a dense cloud of interstellar gas; or, more generally, whereby matter surrounding a star flows toward it (as in close binaries). | ![has source: [H76], 2001-09-19 14:34:53.0](facet.gif) |
| has definition Collection of material together, generally to form a single body. | ![has source: [A84], 2001-09-19 14:34:53.0](facet.gif) |
| is a kind of contraction |  |
| accumulating oceanic element | has ocean concentration depth indenpendent |  |
| has ocean residence time 105 years or greater |  |
| is a kind of oceanic element |  |
| accumulation theory | has definition The theory by which planetesimals are assumed to collide with one another and coalesce, eventually sweeping up enough material to form the planets. | ![has source: [Silk90], 2001-09-19 14:38:55.0](facet.gif) |
| is a kind of planetary theory |  |
| acetaldehyde | has symbol CH3CHO |  |
| is an instance of interstellar molecule |  |
| Achernar | has B-V magnitude -0.16 |  |
| has declination -57 14 12 |  |
| has distance 35 pc | ![has source: [H76], 2001-09-19 14:36:32.0](facet.gif) |
| has right ascension 1 37 42.9 |  |
| has spectral type B3Vpe |  |
| has spectral type B5 | ![has source: [H76], 2001-09-19 14:36:31.0](facet.gif) |
| has synonym alpha Eridani | ![has source: [H76], 2001-09-19 14:36:31.0](facet.gif) |
| has synonym HR 472 |  |
| has V magnitude 0.46 |  |
is a part of Eridanus  |  |
| is an instance of B star | ![has source: [H76], 2001-09-19 14:36:31.0](facet.gif) |
| is an instance of naked eye star |  |
| is an instance of subgiant | ![has source: [H76], 2001-09-19 14:36:31.0](facet.gif) |
| Achilles | has asteroid number 588 |  |
| has definition Trojan asteroid (60°) ahead of Jupiter. It was the first Trojan to be discovered. | ![has source: [H76], 2001-09-19 14:37:08.0](facet.gif) |
| has discovery date 1906 | ![has source: [H76], 2001-09-19 14:37:08.0](facet.gif) |
| has eccentricity e = 0.15 | ![has source: [H76], 2001-09-19 14:37:08.0](facet.gif) |
| has inclination i = 10°.3 | ![has source: [H76], 2001-09-19 14:37:08.0](facet.gif) |
| has orbital period P = 11.98 yr | ![has source: [H76], 2001-09-19 14:37:08.0](facet.gif) |
| has semi-major axis a = 5.2 AU | ![has source: [H76], 2001-09-19 14:37:08.0](facet.gif) |
| is a part of Trojan asteroid |  |
| is an instance of Trojan asteroid | ![has source: [H76], 2001-09-19 14:37:08.0](facet.gif) |
| achromatic lens | has definition Lens (or combination of lenses) that brings different wavelenghts within a ray of light to a single focus, thus overcoming chromatic aberration. It was first successfully made by Joseph von Fraunhofer. | ![has source: [A84], 2001-09-19 14:32:33.0](facet.gif) |
| is a kind of lens |  |
| achromatic objective | has definition A lens of two or more components with different refraction indices (e.g., crown glass and flint glass), used to correct for chromatic aberration. | ![has source: [H76], 2001-09-19 14:32:33.0](facet.gif) |
| is a kind of achromatic lens |  |
| actinide | has atomic number 89 to 103 |  |
| has definition Element with atomic number between 89 (Actinium) and 103 | ![has source: [NASA/SP-2000-7501/Vol1], 2001-09-19 14:33:24.0](facet.gif) |
| has filling orbital 5f |  |
| is a kind of inner transition metal |  |
| is a kind of inner transition metal |  |
| is a kind of metal | ![has source: [NASA/SP-2000-7501/Vol1], 2001-09-19 14:33:23.0](facet.gif) |
| actinium | has abundance minute traces in Earth's crust |  |
| has abundance n.a. in Sun relative to H = 1 × 1012 |  |
| has abundance nil in seawater |  |
| has atomic emission line 383.312 nm for Ac II |  |
| has atomic emission line 408.844 nm for Ac II |  |
| has atomic emission line 450.720 nm for Ac II |  |
| has atomic emission line 591.085 nm for Ac II |  |
| has atomic emission line 416.840 nm for Ac II (strong) |  |
| has atomic emission line 438.641 nm for Ac II (strong) |  |
| has atomic number 89 |  |
| has atomic radii 188 pm |  |
| has biological role none |  |
| has boiling point 3470 ± 300 K |  |
| has chief source uranium ore contain 0.2 p.p.m. |  |
| has crystal cell dimension a = 531.1 pm |  |
| has crystal type f.c.c. |  |
| has daily dietary intake nil |  |
| has definition soft, silvery-white, radioactive metal which glows in the dark |  |
| has density 10060 kg m-3 for solid at 293 K |  |
| has discoverer Andre Debierne |  |
| has discovery date 1899 |  |
| has discovery location Paris, France |  |
| has electron configuration [Rn]6d17s2 in ground state |  |
| has electronegativity 1.1 Pauling |  |
| has hazard never encountered normally, dangerous because it is a powerful source of α-radiation, element found only inside nuclear facilities or research laboratories |  |
| has heat capacity 20.84 J K-1 mol-1 for gas at constant pressure 0.1 MPa at 298.15 K |  |
| has heat capacity 27.2 J K-1 mol-1 for solid at constant pressure 0.1 MPa at 298.15 K |  |
| has heat of fusion 14.2 kJ mol-1 |  |
| has heat of sublimation 51.9 ± 0.5 kJ mol-1 |  |
| has heat of vaporization 418 kJ mol-1 |  |
has image  |  |
| has ionic radii 118 pm for Ac3+ |  |
| has isotope mass range 209 to 232 |  |
| has level in humans nil |  |
| has linear expansion coefficient 14.9 K-1 |  |
| has longest lived isotope actinium 227 |  |
| has mass absorption coefficient cm2 g-1 for CuKα X-ray diffraction |  |
| has mass absorption coefficient cm2 g-1 for MoKα X-ray diffraction |  |
| has mass of element in person nil for a 70 kg average person |  |
| has melting point 1320 ± 50 K |  |
| has molar volume 22.6 cm3 |  |
| has name origin aktinos from Greek word for 'ray' |  |
has number of isotopes 26  |  |
| has number of protons 89 |  |
| has pronunciation ak-tin-iuhm |  |
has registry number 7440-34-8 for Chemical Abstracts System database  |  |
| has relative atomic mass 227.0728 for 227Ac in units of 12C = 12.000 |  |
| has space group Fm3m |  |
| has specimen not commerecially available |  |
| has symbol Ac |  |
| has symbol Ac |  |
| has synthesis mechanism bombardment of radium 236 with neutrons |  |
| has synthesis mechanism decay of uranium 235 |  |
| has term symbol 2D3/2 in ground state |  |
| has thermal conductivity 12 W m-1 K-1 at 300 K |  |
| has world production probably less than a gram |  |
| is a kind of actinide |  |
| is a kind of radioactive element |  |
| reacts with water to release hydrogen gas |  |
| actinium 224 | has atomic mass 224.021685 |  |
| has decay mode α (6.323 MeV) 9.1% |  |
| has decay mode γ |  |
| has decay mode EC (1.397 MeV) 90.9% |  |
| has half life 2.9 hours |  |
| has nuclear spin I = |  |
| has number of neutrons 135 |  |
| has number of nucleons 224 |  |
| has symbol 224Ac |  |
is an instance of actinium  |  |
| actinium 225 | has atomic mass 225.023205 |  |
| has decay mode α (5.935 MeV) |  |
| has decay mode γ |  |
| has half life 10.0 days |  |
| has nuclear spin I = 3/2+ |  |
| has number of neutrons 136 |  |
| has number of nucleons 225 |  |
| has symbol 225Ac |  |
| has uses tracer |  |
is an instance of actinium  |  |
| actinium 226 | has atomic mass 226.026084 |  |
| has decay mode α 6 × 10-3% |  |
| has decay mode β- (1.117) 83 % |  |
| has decay mode γ |  |
| has decay mode EC (0.635 MeV) 17% |  |
| has half life 29 hours |  |
| has nuclear spin I = 1- |  |
| has number of neutrons 137 |  |
| has number of nucleons 226 |  |
| has symbol 226Ac |  |
is an instance of actinium  |  |
| actinium 227 | has atomic mass 227.027750 |  |
| has decay mode α (5.043 Mev) 1.380% |  |
| has decay mode β- (0.0410 Mev) 98.620% |  |
| has decay mode γ |  |
| has decay products radium 223 |  |
| has decay products thorium 227 |  |
| has half life 21.773 years |  |
| has magnetogyric ratio 3.5 × 107 rad T-1 s-1 |  |
| has NMR frequency 13.1 MHz where 1H = 100 MHz; 2.3488 T |  |
| has NMR receptivity where 13C = 1.00 |  |
| has nuclear magnetic moment μ = +1.1 |  |
| has nuclear quadrupole moment 1.7 × 10-28 m2 |  |
| has nuclear spin I = 3/2- |  |
| has number of neutrons 138 |  |
| has number of nucleons 227 |  |
| has relative NMR sensitivity where 1H = 1.00 |  |
| has symbol 227Ac |  |
| has thermal neutron capture cross section 515 barns |  |
| has uses Nuclear Magnetic Resonance |  |
is an instance of actinium  |  |
| actinium 228 | has atomic mass 228.031015 |  |
has decay mode β- (2.142 MeV)  |  |
| has decay mode γ |  |
| has half life 6.15 hours |  |
| has nuclear spin I = 3+ |  |
| has number of neutrons 139 |  |
| has number of nucleons 228 |  |
| has symbol 228Ac |  |
is an instance of actinium  |  |
| actinium 229 | has atomic mass 229.032980 |  |
| has decay mode β- (0.0410 MeV) 99% |  |
| has decay mode γ |  |
| has half life 62.7 minutes |  |
| has nuclear spin I = 3/2+ |  |
| has number of neutrons 140 |  |
| has number of nucleons 229 |  |
| has symbol 229Ac |  |
is an instance of actinium  |  |
| active galaxy | has definition Active galactic nuclei are very luminous. Their energy output is in two forms: nonthermal continuum and thermal emission line. | ![has source: [H76], 2001-09-19 14:36:17.0](facet.gif) |
| has definition Any galaxy which is emitting large quantities of non-thermal radiation. | ![has source: [C97], 2001-09-19 14:36:17.0](facet.gif) |
| has luminosity 1043 to 1046 ergs s-1 | ![has source: [H76], 2001-09-19 14:36:17.0](facet.gif) |
| is a kind of galaxy |  |
| active optics | has definition Controlling the shape of a telescope mirror at a relatively slow rate. | ![has source: [McL97], 2001-09-19 14:32:34.0](facet.gif) |
| is a kind of mirror |  |
| active satellite | is a kind of artificial satellite |  |
| active Sun | has definition The Sun during its 11-year cycle of activity when spots, flares, prominences, and variations in radiofrequency radiation are at a maximum. | ![has source: [H76], 2001-09-19 14:35:01.0](facet.gif) |
| has period 11 years | ![has source: [H76], 2001-09-19 14:35:01.0](facet.gif) |
| is an instance of periodic celestial event |  |
| is an instance of solar event |  |
| adaptive optics | has definition Compensating for atmospheric distortions in a wavefront by high-speed changes in the shape of a small, thin mirror. | ![has source: [McL97], 2001-09-19 14:32:34.0](facet.gif) |
| is a kind of mirror |  |
| advance of the perihelion | has definition The slow rotation of the major axis of a planet's orbit in the same direction as the revolution of the planet itself, due to gravitational interactions with other planets and/or other effects (such as those due to general relativity). | ![has source: [H76], 2001-09-19 14:34:52.0](facet.gif) |
| is a kind of motion |  |
| AE Aurigae | has definition Runaway star which diverges from a comparatively small area in Orion. | ![has source: [H76], 2001-09-19 14:35:45.0](facet.gif) |
| has spectral type O9.5 V | ![has source: [H76], 2001-09-19 14:35:45.0](facet.gif) |
| is a part of Auriga | ![has source: [H76], 2001-09-19 14:35:45.0](facet.gif) |
| is an instance of dwarf |  |
| is an instance of O star |  |
| is an instance of runaway star | ![has source: [H76], 2001-09-19 14:35:45.0](facet.gif) |
| Ae star | has definition A-type star with emission in one or several Balmer lines. | ![has source: [JJ95], 2001-09-19 14:35:28.0](facet.gif) |
| has emission line one or several Balmer lines |  |
| is a kind of A star |  |
| is a kind of emission line star |  |
| aeon | has definition In astronomical terms, 1000 million years. | ![has source: [A84], 2001-09-19 14:37:47.0](facet.gif) |
| has synonym eon |  |
| is an instance of time unit |  |
| aether | has definition In Aristotelian physics, the fifth element, of which the stars and planets are made. |  |
| has definition In Classical physics, an invisible medium that was thought to suffuse all space. | ![has source: [F88], 2001-09-19 14:38:56.0](facet.gif) |
| is a kind of outdated belief |  |
| AI Velorum star | has definition A class of dwarf Cepheids. They are all RR Lyrae stars with periods shorter than 0.25 days. | ![has source: [H76], 2001-09-19 14:35:39.0](facet.gif) |
| is a kind of dwarf Cepheid |  |
| airborne telescope | is a kind of telescope |  |
| airglow | has definition Light in the nighttime sky caused by the collision of atoms and molecules (primarily oxygen, OH, and Ne) in Earth's geocorona with charged particles and X-rays from the Sun or outer space. The airglow varies with time of night, latitude, and season. It is a minimum at zenith and maximum about 10° above the horizon. | ![has source: [H76], 2001-09-19 14:36:54.0](facet.gif) |
| has synonym nightglow |  |
| is a part of geocorona |  |
| alchemy | has definition Art of bringing parts of the universe to the perfect state toward which they were thought to aspire - e.g., gold for metals, immortality for human beings. | ![has source: [F88], 2001-09-19 14:38:56.0](facet.gif) |
| is a kind of outdated belief |  |
| Aldebaran | has B-V magnitude 1.54 |  |
| has declination +16 30 33 |  |
| has definition A K5 III subgiant (a foreground star in the Hyades). It has a faint M2 V companion. It is now known to be slowly and irregularly variable. | ![has source: [H76], 2001-09-19 14:36:24.0](facet.gif) |
| has distance 21 parsecs | ![has source: [H76], 2001-09-19 14:36:24.0](facet.gif) |
| has right ascension 4 35 55.2 |  |
| has spectral type K5III |  |
| has synonym alpha Tau | ![has source: [H76], 2001-09-19 14:36:24.0](facet.gif) |
| has synonym HR 1457 |  |
| has V magnitude 0.85 |  |
is a part of Taurus  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Algol | has definition An eclipsing system of at least three components (B8 V, K0, Am). Period of components A and B is about 68.8 hours; period of components A, B, and C is about 1.9 years. Long term observations also indicate a massive, unseen fourth component with a period of about 190 years. Algol is also an erratic radio source of about 0.5 AU diameter. | ![has source: [H76], 2001-09-19 14:35:36.0](facet.gif) |
| has definition The most famous eclipsing binary, Algol was probably the first variable star discovered. It lies in the constellation Perseus and consists of two stars that orbit each other every 2.87 days. When one star passes in front of the other, the light of the system dims. | ![has source: [C95], 2001-09-19 14:35:36.0](facet.gif) |
| has distance 25 pc |  |
| has synonym beta Per |  |
| has synonym Demon star | ![has source: [H76], 2001-09-19 14:35:36.0](facet.gif) |
| is a part of Perseus |  |
| is an instance of beta Persei star |  |
| alkali earth metal | has definition Element in the second column of the periodic table (from the left) |  |
| alkali Earth metal | has group 2 |  |
| alkali earth metal | has hardness malleable, extrudable and machinable |  |
| alkali Earth metal | has synonym group II element |  |
| is a kind of column grouped element |  |
| alkali earth metal | is a kind of metallic element |  |
| alkali metal | has appearancee silvery except for francium |  |
| has definition Metal in the first column of the periodic table | ![has source: [NASA/SP-2000-7501/Vol1], 2001-09-19 14:33:21.0](facet.gif) |
| has group 1 |  |
| has hardness soft |  |
| has synonym group I element |  |
| is a kind of column grouped element |  |
| is a kind of metallic element |  |
| reacts with water vigorously |  |
| Alpha Andromedae | has B-V magnitude -0.11 |  |
| has declination +29 05 26 |  |
| has right ascension 00 08 23.2 |  |
| has spectral type B8IVpMnHg |  |
| has synonym HR 15 |  |
| has V magnitude 2.06 |  |
is a part of Andromeda  |  |
| is an instance of B star |  |
| is an instance of naked eye star |  |
| is an instance of subgiant |  |
| Alpha Antliae | has B-V magnitude 1.45 |  |
| has declination -31 04 04 |  |
| has right ascension 10 27 09.1 |  |
| has spectral type K4III |  |
| has synonym HR 4104 |  |
| has V magnitude 4.25 |  |
is a part of Antlia  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Apodis | has B-V magnitude 1.43 |  |
| has declination -79 02 41 |  |
| has right ascension 14 47 51.6 |  |
| has spectral type K2.5III |  |
| has synonym HR 5470 |  |
| has V magnitude 3.83 |  |
is a part of Apus  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Arietis | has B-V magnitude 1.15 |  |
| has declination +23 27 45 |  |
| has right ascension 02 07 10.3 |  |
| has spectral type K2IIIabCa-I |  |
| has synonym HR 617 |  |
| has V magnitude 2.00 |  |
is a part of Aries  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Caeli | has B-V magnitude 0.34 |  |
| has declination -41 51 50 |  |
| has right ascension 4 40 33.6 |  |
| has spectral type F2V |  |
| has synonym HR 1502 |  |
| has V magnitude 4.45 |  |
is a part of Caelum  |  |
| is an instance of dwarf |  |
| is an instance of F star |  |
| is an instance of naked eye star |  |
| Alpha Cassiopeiae | has B-V magnitude 1.17 |  |
| has declination +56 32 15 |  |
| has right ascension 0 40 30.4 |  |
| has spectral type K0III |  |
| has synonym HR 168 |  |
| has V magnitude 2.23 |  |
is a part of Cassiopeia  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| alpha Centauri | has B-V magnitude 0.71 |  |
| has declination -60 50 07 |  |
| has definition A binary star whose components have G2 V and K5 V spectral types. The nearest star system to the Sun and the third brightest star in the night sky. | ![has source: [H76], 2001-09-19 14:36:28.0](facet.gif) |
| has distance 4.35 light-years | ![has source: [C95], 2001-09-19 14:36:28.0](facet.gif) |
| has period 80 years | ![has source: [C95], 2001-09-19 14:36:28.0](facet.gif) |
| has proper motion 3'.68 per year | ![has source: [H76], 2001-09-19 14:36:28.0](facet.gif) |
| has right ascension 14 39 36.2 |  |
| has spectral type G2V |  |
| has synonym HR 5459 |  |
| has synonym Rigil Kent | ![has source: [H76], 2001-09-19 14:36:28.0](facet.gif) |
| has V magnitude -0.01 |  |
is a part of Centaurus  |  |
| is an instance of binary star |  |
| is an instance of dwarf |  |
| is an instance of G star |  |
| is an instance of naked eye star |  |
| Alpha Cephei | has B-V magnitude 0.22 |  |
| has declination +62 35 08 |  |
| has right ascension 21 18 34.7 |  |
| has spectral type A7V |  |
| has synonym HR 8162 |  |
| has V magnitude 2.44 |  |
is a part of Cepheus  |  |
| is an instance of A star |  |
| is an instance of dwarf |  |
| is an instance of naked eye star |  |
| Alpha Chamaeleontis | has B-V magnitude 0.39 |  |
| has declination -76 55 11 |  |
| has right ascension 08 18 31.7 |  |
| has spectral type F5III |  |
| has synonym HR 3318 |  |
| has V magnitude 4.07 |  |
is a part of Chamaeleon  |  |
| is an instance of F star |  |
| is an instance of giant |  |
| is an instance of naked eye star |  |
| Alpha Circini | has B-V magnitude 0.24 |  |
| has declination -64 58 31 |  |
| has right ascension 14 42 30.3 |  |
| has spectral type ApSrEuCr: |  |
| has synonym HR 5463 |  |
| has V magnitude 3.19 |  |
is a part of Circinus  |  |
| is an instance of A star |  |
| is an instance of naked eye star |  |
| Alpha Columbae | has B-V magnitude -0.12 |  |
| has declination -34 04 27 |  |
| has right ascension 05 39 38.9 |  |
| has spectral type B7IVe |  |
| has synonym HR 1956 |  |
| has V magnitude 2.64 |  |
is a part of Columba  |  |
| is an instance of B star |  |
| is an instance of naked eye star |  |
| is an instance of subgiant |  |
| Alpha Comae Berenices | has B-V magnitude 0.00 |  |
| has declination +17 31 46 |  |
| has right ascension 13 09 59.2 |  |
| has spectral type F5V |  |
| has synonym HR 4969 |  |
| has V magnitude 5.22 |  |
is a part of Coma Berenices  |  |
| is an instance of dwarf |  |
| is an instance of F star |  |
| Alpha Coronae Autralis | has B-V magnitude 0.04 |  |
| has declination -37 54 16 |  |
| has right ascension 19 09 28.2 |  |
| has spectral type A2V |  |
| has synonym HR 7254 |  |
| has V magnitude 4.11 |  |
is a part of Corona Australis  |  |
| is an instance of A star |  |
| is an instance of dwarf |  |
| is an instance of naked eye star |  |
| Alpha Coronae Borealis | has B-V magnitude -0.02 |  |
| has declination +26 42 53 |  |
| has right ascension 15 34 41.2 |  |
| has spectral type A0V |  |
| has synonym HR 5793 |  |
| has V magnitude 2.23 |  |
is a part of Corona Borealis  |  |
| is an instance of A star |  |
| is an instance of dwarf |  |
| is an instance of naked eye star |  |
| alpha decay | has definition Spontaneous emission by a heavier element (such as uranium) of positively charged helium nuclei - alpha particles - comprising 2 protons and 2 neutrons. The result of this radioactive decay is that the original element is very gradually converted into another element, with a decreased atomic number and mass. Alpha particle emission may be simultaneous with beta particle decay. | ![has source: [A84], 2001-09-19 14:34:40.0](facet.gif) |
| has definition The disintegration of an atomic nucleus, in which the final products are an alpha particle and a nucleus with two fewer protons and two fewer neutrons than the original. | ![has source: [G97], 2001-09-19 14:34:40.0](facet.gif) |
| is a kind of nuclear decay |  |
| Alpha Doradus | has B-V magnitude -0.10 |  |
| has declination -55 2 42 |  |
| has right ascension 4 33 59.8 |  |
| has spectral type A0IIISi |  |
| has synonym HR 1465 |  |
| has V magnitude 3.27 |  |
is a part of Dorado  |  |
| is an instance of A star |  |
| is an instance of giant |  |
| is an instance of naked eye star |  |
| Alpha Equulei | has B-V magnitude 0.53 |  |
| has declination + 5 14 52 |  |
| has right ascension 21 15 49.3 |  |
| has spectral type G0III+A5V |  |
| has synonym HR 8131 |  |
| has V magnitude 3.92 |  |
is a part of Equuleus  |  |
| is an instance of G star |  |
| is an instance of giant |  |
| is an instance of naked eye star |  |
| Alpha Fornacis | has B-V magnitude 0.52 |  |
| has declination -28 59 14 |  |
| has right ascension 03 12 04.2 |  |
| has spectral type F8V |  |
| has synonym HR 963 |  |
| has V magnitude 3.87 |  |
is a part of Fornax  |  |
| is an instance of dwarf |  |
| is an instance of F star |  |
| is an instance of naked eye star |  |
| Alpha Gruis | has B-V magnitude -0.13 |  |
| has declination -46 57 40 |  |
| has right ascension 22 8 13.9 |  |
| has spectral type B7IV |  |
| has synonym HR 8425 |  |
| has V magnitude 1.74 |  |
is a part of Grus  |  |
| is an instance of B star |  |
| is an instance of naked eye star |  |
| is an instance of subgiant |  |
| Alpha Horologii | has B-V magnitude 1.10 |  |
| has declination -42 17 40 |  |
| has right ascension 04 14 00.1 |  |
| has spectral type K1III |  |
| has synonym HR 1326 |  |
| has V magnitude 3.86 |  |
is a part of Horologium  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Hydrae | has B-V magnitude 1.44 |  |
| has declination -8 39 31 |  |
| has right ascension 9 27 35.2 |  |
| has spectral type K3II-III |  |
| has synonym Alphard |  |
| has synonym HR 3748 |  |
| has V magnitude 1.98 |  |
is a part of Hydra  |  |
| is an instance of bright giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Indi | has B-V magnitude 1.00 |  |
| has declination -47 17 29 |  |
| has right ascension 20 37 34.0 |  |
| has spectral type K0IIICNIII-IV |  |
| has synonym HR 7869 |  |
| has V magnitude 3.11 |  |
is a part of Indus  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Lacertae | has B-V magnitude 0.01 |  |
| has declination +50 16 57 |  |
| has right ascension 22 31 17.4 |  |
| has spectral type A1V |  |
| has synonym HR 8585 |  |
| has V magnitude 3.77 |  |
is a part of Lacerta  |  |
| is an instance of A star |  |
| is an instance of dwarf |  |
| is an instance of naked eye star |  |
| Alpha Leonis | has B-V magnitude -0.11 |  |
| has declination +11 58 2 |  |
| has right ascension 10 8 22.3 |  |
| has spectral type B7V |  |
| has synonym HR 3982 |  |
| has V magnitude 1.35 |  |
is a part of Leo  |  |
| is an instance of B star |  |
| is an instance of dwarf |  |
| is an instance of naked eye star |  |
| Alpha Leporis | has B-V magnitude 0.21 |  |
| has declination -17 49 20 |  |
| has right ascension 05 32 43.7 |  |
| has spectral type F0Ib |  |
| has synonym HR 1865 |  |
| has V magnitude 2.58 |  |
is a part of Lepus  |  |
| is an instance of F star |  |
| is an instance of naked eye star |  |
| Alpha Lupi | has B-V magnitude -0.20 |  |
| has declination -47 23 17 |  |
| has right ascension 14 41 55.7 |  |
| has spectral type B1.5III |  |
| has synonym HR 5469 |  |
| has V magnitude 2.30 |  |
is a part of Lupus  |  |
| is an instance of B star |  |
| is an instance of giant |  |
| is an instance of naked eye star |  |
| Alpha Lyncis | has B-V magnitude 1.55 |  |
| has declination +34 23 33 |  |
| has right ascension 9 21 3.2 |  |
| has spectral type K7IIIab |  |
| has synonym HR 3705 |  |
| has V magnitude 3.13 |  |
is a part of Lynx  |  |
| is an instance of bright giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Mensae | has B-V magnitude 0.72 |  |
| has declination -74 45 11 |  |
| has right ascension 06 10 14.6 |  |
| has spectral type G6V |  |
| has synonym HR 2261 |  |
| has V magnitude 5.09 |  |
is a part of Mensa  |  |
| is an instance of dwarf |  |
| is an instance of G star |  |
| Alpha Monocerotis | has B-V magnitude 1.02 |  |
| has declination -09 33 04 |  |
| has right ascension 07 41 14.8 |  |
| has spectral type K0III |  |
| has synonym HR 2970 |  |
| has V magnitude 3.93 |  |
is a part of Monoceros  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Muscae | has B-V magnitude -0.20 |  |
| has declination -69 08 08 |  |
| has right ascension 12 37 11.0 |  |
| has spectral type B2IV-V |  |
| has synonym HR 4798 |  |
| has V magnitude 2.69 |  |
is a part of Musca  |  |
| is an instance of B star |  |
| is an instance of naked eye star |  |
| is an instance of subgiant |  |
| Alpha Ophiuchi | has B-V magnitude 0.15 |  |
| has declination +12 33 36 |  |
| has right ascension 17 34 56.0 |  |
| has spectral type A5III |  |
| has synonym HR 6556 |  |
| has V magnitude 2.08 |  |
is a part of Ophiuchus  |  |
| is an instance of A star |  |
| is an instance of giant |  |
| is an instance of naked eye star |  |
| alpha particle mass | applies to particle alpha particle |  |
| has symbol mα |  |
| has uncertainty 0.00000052 × 10-27 kg |  |
has value 6.64465598 × 10-27 kg  |  |
| is an instance of particle mass |  |
| Alpha Pavonis | has B-V magnitude -0.20 |  |
| has declination -56 44 07 |  |
| has right ascension 20 25 38.8 |  |
| has spectral type B2IV |  |
| has synonym HR 7790 |  |
| has V magnitude 1.94 |  |
is a part of Pavo  |  |
| is an instance of B star |  |
| is an instance of naked eye star |  |
| is an instance of subgiant |  |
| Alpha Persei | has B-V magnitude 0.48 |  |
| has declination +49 51 41 |  |
| has right ascension 3 24 19.3 |  |
| has spectral type F5Ib |  |
| has synonym HR 1017 |  |
| has V magnitude 1.79 |  |
is a part of Perseus  |  |
| is an instance of F star |  |
| is an instance of naked eye star |  |
| is an instance of supergiant |  |
| alpha Persei cluster | has definition A young open cluster with a high mean rotational velocity. | ![has source: [H76], 2001-09-19 14:35:55.0](facet.gif) |
| is a part of Perseus |  |
| is an instance of open cluster |  |
| Alpha Phoenicis | has B-V magnitude 1.09 |  |
| has declination -42 18 22 |  |
| has right ascension 0 26 17.0 |  |
| has spectral type K0III |  |
| has synonym HR 99 |  |
| has V magnitude 2.39 |  |
is a part of Phoenix  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Pictoris | has B-V magnitude 0.21 |  |
| has declination -61 56 29 |  |
| has right ascension 06 48 11.4 |  |
| has spectral type A7IV |  |
| has synonym HR 2550 |  |
| has V magnitude 3.27 |  |
is a part of Pictor  |  |
| is an instance of A star |  |
| is an instance of naked eye star |  |
| is an instance of subgiant |  |
| Alpha Pyxidis | has B-V magnitude -0.18 |  |
| has declination -33 11 11 |  |
| has right ascension 08 43 35.5 |  |
| has spectral type B1.5III |  |
| has synonym HR 3468 |  |
| has V magnitude 3.68 |  |
is a part of Pyxis  |  |
| is an instance of B star |  |
| is an instance of giant |  |
| is an instance of naked eye star |  |
| Alpha Reticuli | has B-V magnitude 0.91 |  |
| has declination -62 28 26 |  |
| has right ascension 04 14 25.5 |  |
| has spectral type G8II-III |  |
| has synonym HR 1336 |  |
| has V magnitude 3.35 |  |
is a part of Reticulum  |  |
| is an instance of bright giant |  |
| is an instance of G star |  |
| is an instance of naked eye star |  |
| Alpha Sculptoris | has B-V magnitude -0.16 |  |
| has declination -29 21 28 |  |
| has right ascension 0 58 36.3 |  |
| has spectral type B7IIIp |  |
| has synonym HR 280 |  |
| has V magnitude 4.31 |  |
is a part of Sculptor  |  |
| is an instance of B star |  |
| is an instance of bright giant |  |
| is an instance of naked eye star |  |
| Alpha Scuti | has B-V magnitude 1.33 |  |
| has declination -08 14 39 |  |
| has right ascension 18 35 12.3 |  |
| has spectral type K3III-IIIb |  |
| has synonym HR 6973 |  |
| has V magnitude 3.85 |  |
is a part of Scutum  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Serpentis | has B-V magnitude 1.17 |  |
| has declination +6 25 32 |  |
| has right ascension 15 44 16.0 |  |
| has spectral type K2IIIbCN1Fe414 |  |
| has synonym HR 5854 |  |
| has V magnitude 2.65 |  |
is a part of Serpens  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Sextantis | has B-V magnitude -0.04 |  |
| has declination -0 22 18 |  |
| has right ascension 10 7 56.2 |  |
| has spectral type A0III |  |
| has synonym HR 3981 |  |
| has V magnitude 4.49 |  |
is a part of Sextans  |  |
| is an instance of A star |  |
| is an instance of giant |  |
| is an instance of naked eye star |  |
| Alpha Telescopii | has B-V magnitude -0.17 |  |
| has declination -45 58 06 |  |
| has right ascension 18 26 58.3 |  |
| has spectral type B3IV |  |
| has synonym HR 6897 |  |
| has V magnitude 3.51 |  |
is a part of Telescopium  |  |
| is an instance of B star |  |
| is an instance of naked eye star |  |
| is an instance of subgiant |  |
| Alpha Trianguli Australis | has B-V magnitude 1.44 |  |
| has declination -69 01 40 |  |
| has right ascension 16 48 39.9 |  |
| has spectral type K2IIb-IIIa |  |
| has synonym HR 6217 |  |
| has V magnitude 1.92 |  |
is a part of Triangulum Australe  |  |
| is an instance of bright giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Tucanae | has B-V magnitude 1.39 |  |
| has declination -60 15 35 |  |
| has right ascension 22 18 30.1 |  |
| has spectral type K3III |  |
| has synonym HR 8502 |  |
| has V magnitude 2.86 |  |
is a part of Tucana  |  |
| is an instance of giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| Alpha Vulpeculae | has B-V magnitude 1.50 |  |
| has declination +24 39 54 |  |
| has right ascension 19 28 42.2 |  |
| has spectral type M0III |  |
| has synonym HR 7405 |  |
| has V magnitude 4.44 |  |
is a part of Vulpecula  |  |
| is an instance of giant |  |
| is an instance of M star |  |
| is an instance of naked eye star |  |
| alpha-particle | has definition Nucleus formed by the α-process (q.v.) (see even-even nuclei). | ![has source: [H76], 2001-09-19 14:33:17.0](facet.gif) |
| has definition Particle first discovered in radioactive α decay, and later identified as helium nuclei (two protons and two neutrons bound together). | ![has source: [CD99], 2001-09-19 14:33:17.0](facet.gif) |
| has definition The nucleus of a 4He atom, consisting of two protons and two neutrons. Mass of α-particle 4.00260 amu. | ![has source: [H76], 2001-09-19 14:33:17.0](facet.gif) |
| is an instance of 4N nucleus |  |
| alpha-process | has definition A hypothetical process of nucleosynthesis, which consisted of redistributing α-particles in the region from neon 20 to iron 56 (and perhaps slightly higher). The α-process has been replaced by explosive and nonexplosive C, O, and Si burning occurring in rapidly evolving or even explosive stages of stellar evolution which at higher temperatures and densities becomes the e-process. | ![has source: [H76], 2001-09-19 14:34:40.0](facet.gif) |
| is a kind of nucleosynthetic reaction |  |
| alpha2 CVn | has definition A spectrum variable with spectrum showing strong, profuse lines of rare earths, iron-peak elements, and Si. | ![has source: [H76], 2001-09-19 14:35:35.0](facet.gif) |
| has period 5.469 days | ![has source: [H76], 2001-09-19 14:35:35.0](facet.gif) |
| is a part of Canes Venatici |  |
| is an instance of spectrum variable |  |
| Altair | has apparent magnitude mv = 0.78 |  |
| has B-V magnitude 0.22 |  |
| has declination +08 52 06 |  |
| has definition A bright A7 V star. | ![has source: [H76], 2001-09-19 14:36:25.0](facet.gif) |
| has distance 4.8 pc | ![has source: [H76], 2001-09-19 14:36:25.0](facet.gif) |
| has right ascension 19 50 46.9 |  |
| has spectral type A7 V | ![has source: [H76], 2001-09-19 14:36:25.0](facet.gif) |
| has synonym alpha Aql |  |
| has synonym HR 7557 |  |
| has V magnitude 0.77 |  |
is a part of Aquila  |  |
| is an instance of A star |  |
| is an instance of dwarf |  |
| is an instance of naked eye star |  |
| altazimuth telescope | has definition A form of mounting similar to that of a radar which allows the telescope tube to be moved horizontally (by rotation in azimuth or compass direction) and vertically (by rotation in altitude or elevation). To follow a star the telescope must be adjusted simultaneously in both axes. (also called alt-az) | ![has source: [McL97], 2001-09-19 14:32:43.0](facet.gif) |
| has mounting altazimuth | ![has source: [McL97], 2001-09-19 14:32:43.0](facet.gif) |
| is a kind of Earth based telescope |  |
| aluminium | has abundance 0.13 × 10-4 p.p.m. in deep Pacific seawater |  |
| has abundance 1.3 × 10-4 p.p.m. in Pacific surface seawater |  |
| has abundance 3.3 × 106 in Sun relative to H = 1 × 1012 |  |
| has abundance 5.2 × 10-4 p.p.m. in deep Atlantic seawater |  |
| has abundance 82000 p.p.m. in Earth's crust |  |
| has abundance 9.7 × 10-4 p.p.m. in Atlantic surface seawater |  |
| has atomic emission line 308.215 nm for Al I |  |
| has atomic emission line 309.271 nm for Al I (used in atom absorption spectrometry) |  |
| has atomic emission line 309.281 nm for Al I (used in atom absorption spectrometry) |  |
| has atomic emission line 394.401 nm for Al I |  |
| has atomic emission line 396.152 nm for Al I (strong) |  |
| has atomic number 13 |  |
| has atomic radii 143 pm |  |
| has biological role none |  |
| has boiling point 2740 K |  |
| has bulk modulus 75.2 GPa |  |
| has chief source bauxite |  |
| has covalent radii 125 pm |  |
| has crystal cell dimension a = 404.959 pm |  |
| has crystal type f.c.c. |  |
| has daily dietary intake 2.45 mg |  |
| has definition soft and malleable metal |  |
| has density 2390 kg m-3 for liquid at 933.52 K melting point |  |
| has density 2698 kg m-3 for solid at 293 K |  |
| has discoverer Oersted |  |
| has discovery date 1825 |  |
| has discovery location Copenhagen, Denmark |  |
| has electrical resistivity 2.6548 × 108 Ω m at 293 K |  |
| has electron affinity 44 kJ mol-1 from Al to Al- |  |
| has electron configuration [Ne]3s23p1 in ground state |  |
| has electronegativity 1.61 Pauling |  |
| has hazard accumulates in the body from daily intake, compounds are used as food additives and in indigestion tablets |  |
| has heat capacity 21.38 J K-1 mol-1 for gas at constant pressure 0.1 MPa at 298.15 K |  |
| has heat capacity 24.35 J K-1 mol-1 for solid at constant pressure 0.1 MPa at 298.15 K |  |
| has heat of fusion 10.67 kJ mol-1 |  |
| has heat of vaporization 293.72 kJ mol-1 |  |
has image  |  |
| has ionic radii 57 pm for Al3+ |  |
| has isotope mass range 22 to 31 |  |
| has level in human blood 0.39 mg dm-3 |  |
| has level in human bone 4 - 27 p.p.m. |  |
| has level in human liver 3 - 23 p.p.m. |  |
| has level in human muscle 0.7 - 28 p.p.m. |  |
| has linear expansion coefficient 23.03 K-1 |  |
| has longest lived isotope aluminium 27 which is stable |  |
| has main mining area Surinam, Jamaica, Ghana, Indonesia, Russia |  |
| has mass absorption coefficient 48.6 cm2 g-1 for CuKα X-ray diffraction |  |
| has mass absorption coefficient 5.16 cm2 g-1 for MoKα X-ray diffraction |  |
| has mass magnetic susceptibility 7.7 × 109 kg-1 m3 for solid |  |
| has mass of element in person 60 mg for a 70 kg average person |  |
| has melting point 933.52 K |  |
| has mineral bauxite, boehmite, diaspore, gibbsite, andalusite, corundum, sillimanite, topaz |  |
| has molar volume 10.00 cm3 |  |
| has name origin alumen = alum from latin |  |
| has neutron scattering length 0.3449 × 10-12 cm |  |
has number of isotopes 11  |  |
| has number of protons 13 |  |
| has ocean oxidation state III |  |
| has ocean residence time 150 years |  |
| has poisson's ratio 0.345 GPa |  |
| has pronunciation al-oo-min-iuhm |  |
has registry number 7429-90-5 for Chemical Abstracts System database  |  |
| has relative atomic mass 26.981539 in units of 12C = 12.000 |  |
| has reserves 6 × 106 tonnes |  |
| has rigidity modulus 26.2 GPa |  |
| has space group Fm3m |  |
| has specimen foil, granules, ingots, pellets, powder, rod, shot or wire. Safe. Aluminum powder can react dangerously with other materials. |  |
| has symbol Al |  |
| has term symbol 2P1/2 in ground state |  |
| has thermal conductivity 237 W m-1 K-1 at 300 K |  |
| has toxic intake 5 g |  |
| has uses vehicle, aircraft and construction industries |  |
| has van der Waals radii 205 pm |  |
| has world production 15 × 106 tonnes per year |  |
| has young's modulus 70.6 GPa |  |
| is a kind of accumulating oceanic element |  |
| is a kind of group III element |  |
| is a kind of metallic element |  |
| reacts with air to produce a thin protective oxide layer |  |
| stable isotope aluminium 27 |  |
| aluminium 26 | has atomic mass 25.986892 |  |
| has decay mode β+ (4.005 Mev) 82% |  |
| has decay mode γ |  |
| has decay mode EC 18% |  |
| has decay product magnesium 26 |  |
| has diagnostic role if decay products found in a solid then solid must have condensed within the first million years after the creation of Al 26 |  |
| has half life 7.2 × 105 years |  |
| has nuclear spin I = 5+ |  |
| has number of neutrons 13 |  |
| has number of nucleons 26 |  |
| has symbol 26Al |  |
| has uses research |  |
is an instance of aluminium  |  |
| is an instance of supernova produced radioactive element |  |
| aluminium 27 | has atomic mass 26.9885386 |  |
| has magnetogyric ratio 6.9704 × 107 rad T-1 s-1 |  |
| has NMR frequency 26.057 MHz where 1H = 100 MHz; 2.3488 T |  |
| has NMR receptivity 1.17 × 103 where 13C = 1.00 |  |
| has nuclear magnetic moment μ = 3.641504 |  |
| has nuclear quadrupole moment 0.1403 × 10-28 m2 |  |
| has nuclear spin I = 5/2+ |  |
| has number of neutrons 14 |  |
| has number of nucleons 27 |  |
| has relative NMR sensitivity 0.21 where 1H = 1.00 |  |
| has symbol 27Al |  |
| has thermal neutron capture cross section 0.231 barns |  |
| has uses Nuclear Magnetic Resonance |  |
is an instance of aluminium  |  |
| aluminium 28 | has atomic mass 27.981910 |  |
| has decay mode β- (4.642 Mev) |  |
| has decay mode γ |  |
| has half life 2.25 minutes |  |
| has nuclear magnetic moment μ = 3.24 |  |
| has nuclear spin I = 3+ |  |
| has number of neutrons 15 |  |
| has number of nucleons 28 |  |
| has symbol 28Al |  |
is an instance of aluminium  |  |
| aluminium 29 | has atomic mass 28.980446 |  |
| has decay mode β- (3.68 Mev) % |  |
| has decay mode γ |  |
| has half life 6.5 minutes |  |
| has nuclear spin I = 5/2+ |  |
| has number of neutrons 16 |  |
| has number of nucleons 29 |  |
| has symbol 29Al |  |
is an instance of aluminium  |  |
| Am star | has definition A-type or F-type object to which no unique spectral type can be assigned. Usually the classifier provides a classification according to the hydrogen, metallic and calcium lines. Also call metallic-line stars. | ![has source: [JJ95], 2001-09-19 14:35:47.0](facet.gif) |
| has definition Peculiar star whose metallic lines are as strong as those of the F stars but whose hydrogen lines are so strong as to require that they be classed with the A stars. They are generally short-period (<300d) spectroscopic binaries with high atmospheric turbulence and variable spectra, and are slower rotators than normal A stars. | ![has source: [H76], 2001-09-19 14:35:47.0](facet.gif) |
| is a kind of A star |  |
| is a kind of peculiar star |  |
| Amalthea | has definition The innermost satellite of Jupiter. | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has diameter 140 km | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has discoverer Barnard | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has discovery date 1892 | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has eccentricity e = 0.0028 | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has inclination i = 0°.4 | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has orbital period 0.498 days | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has synonym Barnard's satellite | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| has synonym Jupiter V | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| is a part of Jupiter | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| is an instance of natural satellite | ![has source: [H76], 2001-09-19 14:36:57.0](facet.gif) |
| americium | has abundance nil in Earth's crust |  |
| has abundance nil in seawater |  |
| has atomic emission line 367.312 nm for Am I |  |
| has atomic emission line 377.750 nm for Am II |  |
| has atomic emission line 392.625 nm for Am II |  |
| has atomic emission line 408.929 nm for Am II |  |
| has atomic emission line 428.926 nm for Am I |  |
| has atomic emission line 450.945 nm for Am II |  |
| has atomic emission line 457.559 nm for Am II |  |
| has atomic emission line 466.279 nm for Am II |  |
| has atomic emission line 605.464 nm for Am I (strong) |  |
| has atomic number 95 |  |
| has atomic radii 173 pm |  |
| has biological role none |  |
| has boiling point 2880 K |  |
| has crystal cell dimension a = 346.80 pm for α phase |  |
| has crystal cell dimension a = 489.4 pm for β phase |  |
| has crystal type f.c.c. for β phase |  |
| has crystal type h.c.p. for α phase |  |
| has daily dietary intake nil |  |
| has definition radioactive silvery metal which does not occur naturally |  |
| has density 13670 kg m-3 for solid at 293 K |  |
| has discoverer Glen T. Seaborg, R.A. James, L.O. Morgan, and A. Ghiorso |  |
| has discovery date 1944 |  |
| has discovery location Chicago, Illinois, US |  |
| has electrical resistivity 68 × 10-8 Ω m |  |
| has electron configuration [Rn]5f77s2 in ground state |  |
| has electronegativity 1.3 Pauling |  |
| has hazard intense α-radiation, maximum permissible body burden of 241Am is 0.03 μCi - it targets bone. γ radiation is a problem in gram amounts. |  |
| has heat of fusion 14.4 kJ mol-1 |  |
| has heat of sublimation 34.2 kJ mol-1 |  |
| has heat of vaporization 284 kJ mol-1 |  |
has image  |  |
| has ionic radii 107 pm for Am3+ |  |
| has ionic radii 80 pm for Am6+ |  |
| has ionic radii 86 pm for Am5+ |  |
| has ionic radii 92 pm for Am4+ |  |
| has isotope mass range 227 to 247 |  |
| has level in humans nil |  |
| has longest lived isotope americium 243 |  |
| has mass magnetic susceptibility +5 × 10-8 kg-1 m3 |  |
| has mass of element in person nil for a 70 kg average person |  |
| has melting point 1445 K |  |
| has mineral none |  |
| has molar volume 17.78 cm3 |  |
| has name origin america from English |  |
| has neutron scattering length 0.83 in 10-12 cm units |  |
| has number of isotopes 23 including nuclear isomers |  |
| has number of protons 95 |  |
| has phase changed temperature 1347 K at α to β phase crystal transition |  |
| has pronunciation amer-is-iuhm |  |
has registry number 7440-35-9 for Chemical Abstracts System database  |  |
| has relative atomic mass 243.0614 for americium 243 in units of 12C = 12.000 |  |
| has space group Fm3m for β phase |  |
| has space group P63/mmc for α phase |  |
| has symbol Am |  |
| has term symbol 8S7/2 in ground state |  |
| has thermal conductivity 10 W m-1 K-1 at 300 K |  |
| has thermal neutron capture cross section 75.3 barns |  |
| has uses source of radiation for γ-radiotherapy |  |
| has world production probably a few kilograms per year |  |
| is a kind of radioactive element |  |
| is a kind of transuranium element |  |
| reacts with air, steam and acids, but not alkalis |  |
| americium 237 | has atomic mass 237.050050 |  |
| has decay mode α (6.20 Mev) 0.02% |  |
| has decay mode γ |  |
| has decay mode EC (1.6 Mev) 99.98% |  |
| has half life 1.22 hours |  |
| has nuclear spin I = 5/2- |  |
| has number of neutrons 142 |  |
| has number of nucleons 237 |  |
| has symbol 237Am |  |
is an instance of americium  |  |
| americium 238 | has atomic mass 238.051980 |  |
| has decay mode α (6.04 Mev) < 0.1% |  |
| has decay mode γ |  |
| has decay mode EC (2.26 MeV) |  |
| has half life 1.63 hours |  |
| has nuclear spin I = 1+ |  |
| has number of neutrons 143 |  |
| has number of nucleons 238 |  |
| has symbol 238Am |  |
is an instance of americium  |  |
| americium 239 | has atomic mass 239.053016 |  |
| has decay mode α (5.924 Mev) 0.01% |  |
| has decay mode γ |  |
| has decay mode EC (0.800 MeV) 99.99% |  |
| has half life 11.9 hours |  |
| has nuclear spin I = 5/2- |  |
| has number of neutrons 144 |  |
| has number of nucleons 239 |  |
| has symbol 239Am |  |
is an instance of americium  |  |
| americium 240 | has atomic mass 240.055278 |  |
| has decay mode α (5.592 Mev) |  |
| has decay mode γ |  |
| has decay mode EC (1.38 MeV) |  |
| has half life 2.12 days |  |
| has nuclear spin I = 3- |  |
| has number of neutrons 145 |  |
| has number of nucleons 240 |  |
| has symbol 240Am |  |
is an instance of americium  |  |
| americium 241 | has atomic mass 241.056823 |  |
| has decay mode α (5.637 Mev) % |  |
| has decay mode γ |  |
| has half life 432.2 years |  |
| has nuclear magnetic moment μ = 1.61 |  |
| has nuclear spin I = 5/2- |  |
| has number of neutrons 146 |  |
| has number of nucleons 241 |  |
| has specimen commercially available, under licence |  |
| has symbol 241Am |  |
| has synthesis mechanism 241Pu subjected to neutron bombardment over a period of years |  |
| has uses research, medical therapy, medical diagnosis |  |
is an instance of americium  |  |
| americium 242 | has atomic mass 242.056541 |  |
| has decay mode β- (0.663 Mev) 83% |  |
| has decay mode γ |  |
| has decay mode EC (0.750 Mev) 17% |  |
| has half life |  |
| has nuclear magnetic moment μ = +0.388 |  |
| has nuclear spin I = 1- |  |
| has number of neutrons 147 |  |
| has number of nucleons 242 |  |
| has symbol 242Am |  |
is an instance of americium  |  |
| americium 242m | has decay mode α (5.62 Mev) 0.5% |  |
| has decay mode γ |  |
| has decay mode IT (0.48 Mev) 99.5% |  |
| has half life 141 years |  |
| has nuclear magnetic moment μ = 1.0 |  |
| has nuclear spin I = 5- |  |
| has number of neutrons 147 |  |
| has number of nucleons 242 |  |
| has symbol 242mAm |  |
is an instance of americium  |  |
| americium 243 | has atomic mass 243.061375 |  |
| has decay mode α (5.438 Mev) |  |
| has decay mode γ |  |
| has half life 7370 years |  |
| has magnetogyric ratio 1.54 × 107 rad T-1 s-1 |  |
| has NMR frequency 5.76 MHz where 1H = 100 MHz; 2.3488 T |  |
| has nuclear magnetic moment μ = 1.61 |  |
| has nuclear quadrupole moment +4.210 × 10-28 m2 |  |
| has nuclear spin I = 5/2- |  |
| has number of neutrons 148 |  |
| has number of nucleons 243 |  |
| has specimen commercially available, under licence |  |
| has symbol 243Am |  |
| has synthesis mechanism 239Pu subjected to neutron bombardment |  |
| has uses research, Nuclear Magnetic Resonance |  |
is an instance of americium  |  |
| americium 244 | has atomic mass 244.064279 |  |
| has decay mode β- (1.427 Mev) |  |
| has decay mode γ |  |
| has half life 10.0 hours |  |
| has number of neutrons 149 |  |
| has number of nucleons 244 |  |
| has symbol 244Am |  |
is an instance of americium  |  |
| americium 245 | has atomic mass 245.066444 |  |
| has decay mode β- (0.894 Mev) |  |
| has decay mode γ |  |
| has half life 2.05 hours |  |
| has nuclear spin I = 5/2+ |  |
| has number of neutrons 150 |  |
| has number of nucleons 245 |  |
| has symbol 245Am |  |
is an instance of americium  |  |
| ammonia | has symbol NH3 |  |
| is an instance of interstellar molecule |  |
| is an instance of neutral particle |  |
| amount of substance unit | is a kind of unit |  |
| is a unit of amount of substance |  |
| amount-of-substance concentration unit | has definition mole per cubic meter |  |
| has symbol mol·m-3 |  |
| is a kind of derived SI unit |  |
| ampere | has consequence fixes the magnetic constant (permeability of vacuum) at exactly 4 × 10-7 H · m-1 |  |
| has definition constant current which, if maintained in two straight parallel conductors of infinite length, of negligible circular cross-section, and placed 1 meter apart in vacuum, would produce between these conductors a force equal to 2 × 10-7 newton per meter of length |  |
| has definition Unit of electric current. "The ampere is that constant current which, if maintained in two straight parallel conductors of infinite length, of negligible circular cross-section, and placed 1 meter apart in vacuum, would produce between these conductors a force equal to 2 × 10-7 newton per meter of length" (CIPM | ![has source: [1946], Resolution 2, approved by the 9th CGPM 1948). A current of 1 A is equivalent to the passage along the filament of a light bulb of about 6 × 10<sup>18</sup> electronic charges per second., 2001-09-19 14:39:00.0](facet.gif) |
| has symbol A |  |
| is an instance of base SI unit |  |
| is an instance of current unit |  |
| Andromeda | has acronym And |  |
has boundary  |  |
| has genitive Andromedae |  |
has historical image  |  |
| has synonym Chained Lady |  |
| has synonym Princess of Ethiopia |  |
| is a part of celestial sphere |  |
is an instance of constellation  |  |
| Andromeda galaxy | has definition A spiral galaxy (kS5 in Morgan's classification) in the Local Group, about 650-700 kpc distant (MV = -21), visible to the naked eye as a fuzzy patch in the constellation of Andromeda. Total mass about 3.1 × 1011 Msun ; i = 77°, heliocentric velocity - 180 km s-1. Its nucleus exhibits noncircular gas motions. It is similar to but slightly larger than our Galaxy. | ![has source: [H76], 2001-09-19 14:36:20.0](facet.gif) |
| has definition Major spiral galaxy, 2.2 million light-years from Earth. Gravitationally bound to the Milky Way with which it shares membership in the Local Group, it is currently approaching us, rather than receding as is the case for most galaxies. | ![has source: [F88], 2001-09-19 14:36:20.0](facet.gif) |
| has definition The largest galaxy in the Local Group. Also known as the Great Spiral and M31. It is about one and a half times the size of our own galaxy, and contains at least 300 globular clusters. Two smaller, elliptical galaxies (M32 and NGC 205) lie close to it. | ![has source: [A84], 2001-09-19 14:36:20.0](facet.gif) |
| has definition The largest member of the local group. It is a giant spiral galaxy that lies 2.4 million light-years away. | ![has source: [C95], 2001-09-19 14:36:20.0](facet.gif) |
has image  |  |
has NED data  |  |
| has synonym M 31 |  |
| is a part of Local Group |  |
| is an instance of galaxy containing Cepheids |  |
| is an instance of hypergalaxy | ![has source: [Silk90], 2001-09-19 14:36:20.0](facet.gif) |
| is an instance of Messier object |  |
| is an instance of naked eye object |  |
| is an instance of Sb spiral | ![has source: [H76], 2001-09-19 14:36:20.0](facet.gif) |
| Andromeda I | has definition Dwarf spheroidal galaxy in the Andromeda subgroup of the Local Group. It is among the intrinsically faintest members of the Local Group. | ![has source: [H76], 2001-09-19 14:36:12.0](facet.gif) |
| has discoverer van den Bergh | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| has discovery date 1972 | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| is a part of Local Group |  |
| is an instance of satellite galaxy |  |
| orbits Andromeda galaxy | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| Andromeda II | has definition Dwarf spheroidal galaxy in the Andromeda subgroup of the Local Group. It is among the intrinsically faintest members of the Local Group. | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| has discoverer van den Bergh | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| has discovery date 1972 | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| is a part of Local Group |  |
| is an instance of satellite galaxy | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| orbits Andromeda galaxy | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| Andromeda III | has definition Dwarf spheroidal galaxy in the Andromeda subgroup of the Local Group. It is among the intrinsically faintest members of the Local Group. | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| has discoverer van den Bergh | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| has discovery date 1972 | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| is a part of Local Group |  |
| is an instance of satellite galaxy | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| orbits Andromeda galaxy | ![has source: [H76], 2001-09-19 14:36:13.0](facet.gif) |
| angle | has unit angle unit |  |
| is a kind of quantity |  |
| angle unit | is a kind of unit |  |
| is a unit of angle |  |
| Anglo-Australian Telescope | has acronym AAT |  |
| has altitude 1149 m |  |
| has aperture 3.893 m |  |
| has creation date 1975 |  |
| has focal ratio t/3.3. 8, 15. 36 |  |
| has latitude 31° 17' S |  |
| has location Siding Spring Mtn., Australia |  |
| has longitude 149° 04' E |  |
| has mirror maker Grubb-Parsons |  |
| has mirror type Cer-Vit |  |
| has mounting manufacturer Mitsubishi |  |
has owner Anglo-Australian Observatory  |  |
| is an instance of Horseshoe equatorial telescope |  |
| is an instance of optical telescope |  |
is an instance of reflector  |  |
| angstrom | has definition A unit of length used when expressing wavelengths. | ![has source: [McL97], 2001-09-19 14:37:39.0](facet.gif) |
| has equivalent 10-10 meters | ![has source: [McL97], 2001-09-19 14:37:39.0](facet.gif) |
| has symbol Å | ![has source: [McL97], 2001-09-19 14:37:39.0](facet.gif) |
| is an instance of length unit |  |
| is an instance of non SI unit |  |
| is named after Anders Jonas Angstrom (1814-1874) | ![has source: [McL97], 2001-09-19 14:37:39.0](facet.gif) |
| angular momentum | has definition The angular momentum of a system about a specified origin is the sum over all the particles in the system (or an integral over the different elements of the system if it is continuous) of the vector products of the radius vector joining each particle to the origin and the momentum of the particle. For a closed system it is conserved by virtue of the isotropy of space. | ![has source: [H76], 2001-09-19 14:38:20.0](facet.gif) |
| has definition The product of mass and angular velocity for an object in rotation; similar to linear momentum. In quantum mechanics, angular momentum is quantized, i.e., is measured in indivisible units equivalent to Planck's constant divided by 2 pi. This corresponds classically to only certain frequencies of rotation being allowed. | ![has source: [F88], 2001-09-19 14:38:20.0](facet.gif) |
| has symbol L |  |
| is a kind of quantity |  |
| angular size | has definition The angle subtended by an object on the sky. For example, the angular size of the moon is 30 arcminutes. | ![has source: [HH98], 2001-09-19 14:38:23.0](facet.gif) |
| is a kind of angle |  |
| ANIK 1 | is an instance of ANIK satellite |  |
| ANIK 2 | is an instance of ANIK satellite |  |
| ANIK 3 | is an instance of ANIK satellite |  |
| ANIK satellite | is a kind of geosynchronous satellite |  |
| anisotropy | breaks isotropy |  |
| has definition The characteristic of being dependent upon direction. (Light coming with equal intensity from all directions is isotropic; a spotlight's beam is anisotropic.) The cosmic background radiation is generally isotropic - i.e., its intensity is the same in all parts of the sky - but small anisotropies have been detected which are thought to reflect the earth's proper motion relative to the framework of the universe as a whole. | ![has source: [F88], 2001-09-19 14:37:27.0](facet.gif) |
| has definition The condition in which the universe appears different in different directions. | ![has source: [LB90], 2001-09-19 14:37:27.0](facet.gif) |
| is a kind of symmetry breaking |  |
| Annie Jump Cannon | has career Havard College Observatory  |  |
has greatest achievement the Henry Draper Catalog of spectral types  |  |
| is an instance of 19th century scientist |  |
| is an instance of astronomer |  |
| annular eclipse | has definition A solar eclipse in which the solar disk is never completely covered but is seen as an annulus or ring at maximum eclipse. An annular eclipse occurs when the apparent disk of the Moon is smaller than that of the Sun. | ![has source: [S92], 2001-09-19 14:35:00.0](facet.gif) |
| has definition An eclipse of the Sun in which the Moon is too far from Earth to block out the Sun completely, so that a ring of sunlight appears around the Moon. | ![has source: [H76], 2001-09-19 14:35:00.0](facet.gif) |
| is an instance of solar eclipse |  |
| anomalistic month | has definition The interval between two successive perigee passages of the Moon. | ![has source: [H76], 2001-09-19 14:37:46.0](facet.gif) |
| has value 27.555 days | ![has source: [H76], 2001-09-19 14:37:46.0](facet.gif) |
| is an instance of month |  |
| anomalistic year | has definition A period of time based on the revolution of the Earth around the Sun, where a year is defined as the mean interval between successive passages of the Earth through perihelion. | ![has source: [S92], 2001-09-19 14:37:45.0](facet.gif) |
| has definition The interval between two successive perihelion passages of Earth. | ![has source: [H76], 2001-09-19 14:37:45.0](facet.gif) |
| has value 365.2596 ephemeris days | ![has source: [H76], 2001-09-19 14:37:46.0](facet.gif) |
| is an instance of year |  |
| anomalous Zeeman effect | has cause the influence of magnetic fields on both the orbital angular momentum and the spin angular momentum of electrons in atoms or ions | ![has source: [H76], 2001-09-19 14:34:44.0](facet.gif) |
| has definition Zeeman effet in which spectral lines are split into several components, in contrast to the normal Zeeman effect which results in only two distinct components. | ![has source: [H76], 2001-09-19 14:34:44.0](facet.gif) |
| has effect splitting of spectral lines into more than two components | ![has source: [H76], 2001-09-19 14:34:44.0](facet.gif) |
| is a kind of Zeeman effect |  |
| antapex | has definition The direction in the sky away from which the Sun seems to be moving (at a speed of 19.4 km s-1) relative to general field stars in the Galaxy. | ![has source: [H76], 2001-09-19 14:37:32.0](facet.gif) |
| is a part of Columba | ![has source: [H76], 2001-09-19 14:37:32.0](facet.gif) |
| is an instance of equatorial coordinate |  |
| is opposite of solar apex |  |
| Antares | has B-V magnitude 1.83 |  |
| has declination -26 25 55 |  |
| has definition A red M1 Ib supergiant. It has a B3 V companion, which is a radio source. | ![has source: [H76], 2001-09-19 14:36:24.0](facet.gif) |
| has distance 125 parsecs | ![has source: [H76], 2001-09-19 14:36:24.0](facet.gif) |
| has location inner edge of the Orion spiral arm | ![has source: [C95], 2001-09-19 14:36:24.0](facet.gif) |
| has right ascension 16 29 24.4 |  |
| has spectral type M1.5Iab-Ib+B4V |  |
| has synonym alpha Sco |  |
| has synonym HR 6134 |  |
| has V magnitude 0.96 |  |
is a part of Scorpius  |  |
| is an instance of naked eye star |  |
| is an instance of red supergiant |  |
| anthropic principle | has definition The doctrine that the value of certain fundamental constants of nature can be explained by demonstrating that, were they otherwise, the universe could not support life and therefore would contain nobody capable of worrying about why they are as they are. Were the strong nuclear force slightly different in strength, for instance, the stars could not shine and life as we know it would be impossible. | ![has source: [F88], 2001-09-19 14:38:56.0](facet.gif) |
| has definition The weak form of the anthropic principle states that life can exist only during a brief period of the history of our universe. The strong form of the principle states that out of all possible values for the fundamental constants of nature and the initial conditions of the universe, only a small fraction could allow life to form at all, at anytime. (See boundary conditions; fundamental constants of nature.) | ![has source: [LB90], 2001-09-19 14:38:56.0](facet.gif) |
| is a kind of outdated belief |  |
| anthropocentrism | has definition The belief that humans are central to the universe. | ![has source: [HH98], 2001-09-19 14:38:56.0](facet.gif) |
| is a kind of outdated belief |  |
| anthropomorphism | has definition The projection of human attributes onto nonhuman entities such as animals, the planets, or the universe as a whole. | ![has source: [HH98], 2001-09-19 14:38:56.0](facet.gif) |
| is a kind of outdated belief |  |
| anti-reflection coating | has definition Also AR coating. A layer of material of lower refractive index of just the right thickness (1/4 wave) is deposited on the optical surface to be coated. More complex coatings are possible which cover a large wavelength range. | ![has source: [McL97], 2001-09-19 14:32:36.0](facet.gif) |
| is a kind of coating |  |
| anticenter | has definition The direction of the sky opposite to that of the galactic center. | ![has source: [H76], 2001-09-19 14:37:33.0](facet.gif) |
| has definition The point in the galactic plane that lies directly opposite the galactic center. Here we gaze toward the edge of the Galactic disk. The nearest bright star to the anticenter is El Nath, in the constellation Taurus. | ![has source: [C95], 2001-09-19 14:37:33.0](facet.gif) |
| has galactic latitude 0 |  |
| has galactic longitude 180 degrees |  |
| is a part of Auriga | ![has source: [H76], 2001-09-19 14:37:33.0](facet.gif) |
| is an instance of galactic coordinate |  |
| is opposite of galactic center |  |
| antimony | has abundance 0.2 p.p.m. in Earth's crust |  |
| has abundance 10 in Sun relative to H = 1 × 1012 |  |
| has abundance 3 × 10-4 p.p.m. in seawater |  |
| has atomic emission line 206.833 nm for Sb I |  |
| has atomic emission line 217.581 nm for Sb I |  |
| has atomic emission line 252.852 nm for Sb I |  |
| has atomic emission line 259.805 nm for Sb I |  |
| has atomic emission line 231.147 nm for Sb I (strong) |  |
| has atomic number 51 |  |
| has atomic radii 182 pm |  |
| has biological role none |  |
| has boiling point 1908 K |  |
| has chief source stibnite, tetrahedrite although mainly a copper ore yields antimony as a by-product |  |
| has covalent radii 141 pm |  |
| has crystal cell dimension a = 298.6 pm for grey cubic form |  |
| has crystal cell dimension a = 336.9 pm for metal form |  |
| has crystal cell dimension a = 430.84 pm for grey rhombohedral form |  |
| has crystal cell dimension c = 1124.7 pm for grey rhombohedral form |  |
| has crystal cell dimension c = 533 pm for metal form |  |
| has crystal type cubic for grey cubic form |  |
| has crystal type h.c.p. for metal form |  |
| has crystal type rhombohedral for grey rhombohedral form |  |
| has daily dietary intake 0.002 to 1.3 mg |  |
| has definition metalloid element with three forms. The metallic form is the more stable and is bright, silvery, hard and brittle |  |
| has density 6483 kg m-3 for liquid at 903.89 K melting point |  |
| has density 6691 kg m-3 for solid at 293 K |  |
| has discovery date 1600 BC probably known to the ancients and certainly to the alchemists |  |
| has electrical resistivity 39.0 × 10-8 Ω m at 273 K |  |
| has electron affinity 101 kJ mol-1 from Sb to Sb- |  |
| has electron configuration [Kr]4d105s25p3 in ground state |  |
| has electronegativity 2.05 Pauling |  |
| has hazard small doses stimulate metabolism, large doses cause liver damage |  |
| has heat capacity 20.79 J K-1 mol-1 for gas at constant pressure 0.1 MPa at 298.15 K |  |
| has heat capacity 25.23 J K-1 mol-1 for solid at constant pressure 0.1 MPa at 298.15 K |  |
| has heat of fusion 20.9 kJ mol-1 |  |
| has heat of vaporization 67.91 kJ mol-1 |  |
has image  |  |
| has ionic radii 245 pm for Sb2- |  |
| has ionic radii 62 pm for Sb5+ |  |
| has ionic radii 89 pm for Sb3+ |  |
| has isotope mass range 108 to 136 |  |
| has lethal intake 140 mg for antimony potassium tartrate (oral) for LD50 |  |
| has level in humans 0.0033 mg dm-3 in blood |  |
| has level in humans 0.01 to 0.6 p.p.m. in bone |  |
| has level in humans 0.011 to 0.42 p.p.m. in liver |  |
| has level in humans 0.042 to 0.191 p.p.m. in muscle |  |
| has linear expansion coefficient 8.5 × 10-6 K-1 |  |
| has main mining area China, Italy, Peru, Mexico, Bolivia, France |  |
| has mass absorption coefficient 270 cm2 g-1 for CuKα X-ray diffraction |  |
| has mass absorption coefficient 33.1 cm2 g-1 for MoKα X-ray diffraction |  |
| has mass magnetic susceptibility -1.0 × 10-8 kg-1 m3 for solid |  |
| has mass of element in person 2 mg for a 70 kg average person |  |
| has melting point 903.89 K |  |
| has mineral sibiconite, stibnite, tetrahedrite, ullmannite |  |
| has molar volume 18.20 cm3 |  |
| has name origin anti + monos = not alone from greek |  |
| has neutron scattering length 0.557 × 10-12 cm |  |
| has number of isotopes 40 |  |
| has number of protons 51 |  |
| has ocean oxidation state III |  |
| has ocean residence time 3.5 × 105 years |  |
| has poisson's ratio 0.25 to 0.33 GPa |  |
| has pronunciation anti-moni |  |
has registry number 7440-36-0 for Chemical Abstracts System database  |  |
| has relative atomic mass 112.760 in units of 12C = 12.000 |  |
| has reserves 2.5 × 106 tonnes |  |
| has rigidity modulus 20.7 GPa |  |
| has space group P63/mmc for metal form |  |
| has space group Pm3m for grey cubic form |  |
| has space group R3m for grey rhombohedral form |  |
| has specimen available as pieces, powder or shot. Care ! |  |
| has stable isotope antimony 121 |  |
| has stable isotope antimony 123 |  |
| has symbol Sb |  |
| has symbol origin stibium from latin |  |
| has term symbol 4S3/2 in ground state |  |
| has thermal conductivity 24.3 W m-1 K-1 at 300 K |  |
| has thermal neutron capture cross section 4.91 barns |  |
| has toxic intake 100 mg |  |
| has uses hardenning other metals, stotage batteries, bearings |  |
| has van der Waals radii 220 pm |  |
| has world production 53000 tonnes per year |  |
| has young's modulus 54.7 GPa |  |
| is a kind of accumulating oceanic element |  |
| is a kind of group V element |  |
| is a kind of metallic metalloid |  |
| reacts with stable in dry air, not attacked by dilute acids or alkalis |  |
| antimony 119 | has atomic mass 118.903948 |  |
| has decay mode γ |  |
| has decay mode EC (0.59 Mev) |  |
| has half life 38.1 hours |  |
| has nuclear magnetic moment μ = +3.45 |  |
| has nuclear spin I = 5/2+ |  |
| has number of neutrons 68 |  |
| has number of nucleons 119 |  |
| has symbol 119Sb |  |
is an instance of antimony  |  |
| antimony 120 | has atomic mass 119.903821 |  |
| has decay mode β+ (2.68 Mev) 41% |  |
| has decay mode γ |  |
| has decay mode EC 59% |  |
| has half life 15.89 minutes |  |
| has nuclear magnetic moment μ = +2.3 |  |
| has nuclear spin I = 1+ |  |
| has number of neutrons 69 |  |
| has number of nucleons 120 |  |
| has symbol 120Sb |  |
is an instance of antimony  |  |
| antimony 120m | has atomic mass 119.903821 |  |
| has decay mode γ |  |
| has decay mode EC |  |
| has half life 5.76 days |  |
| has nuclear magnetic moment μ = 2.34 |  |
| has nuclear spin I = 8- |  |
| has number of neutrons 69 |  |
| has number of nucleons 120 |  |
| has symbol 120mSb |  |
is an instance of antimony  |  |
| antimony 121 | has atomic mass 120.9038212 |  |
| has magnetogyric ratio 6.4016 × 107 rad T-1 s-1 |  |
| has natural abundance 57.3 % |  |
| has NMR frequency 23.930 MHz where 1H = 100 MHz; 2.3488 T |  |
| has NMR receptivity 520 where 13C = 1.00 |  |
| has nuclear magnetic moment μ = +3.3634 |  |
| has nuclear quadrupole moment -0.360 × 10-28 m2 |  |
| has nuclear spin I = 5/2+ |  |
| has number of neutrons 70 |  |
| has number of nucleons 121 |  |
| has relative NMR sensitivity 0.16 where 1H = 1.00 |  |
| has symbol 121Sb |  |
| has uses experimental, Nuclear Magnetic Resonance |  |
is an instance of antimony  |  |
| antimony 122 | has atomic mass 121.905179 |  |
| has decay mode β+ (0.619 Mev) 2% |  |
| has decay mode β- (1.9820 Mev) 98% |  |
| has decay mode γ |  |
| has half life 2.73 days |  |
| has nuclear magnetic moment μ = -1.90 |  |
| has nuclear spin I = 2- |  |
| has number of neutrons 71 |  |
| has number of nucleons 122 |  |
| has symbol 122Sb |  |
is an instance of antimony  |  |
| antimony 123 | has atomic mass 122.9042160 |  |
| has magnetogyric ratio 3.4668 × 107 rad T-1 s-1 |  |
| has natural abundance 42.7 % |  |
| has NMR frequency 12.959 MHz where 1H = 100 MHz; 2.3488 T |  |
| has NMR receptivity 111 where 13C = 1.00 |  |
| has nuclear magnetic moment μ = 2.5498 |  |
| has nuclear quadrupole moment -0.490 × 10-28 m2 |  |
| has nuclear spin I = 7/2+ |  |
| has number of neutrons 72 |  |
| has number of nucleons 123 |  |
| has relative NMR sensitivity 4.57 × 10-2 where 1H = 1.00 |  |
| has symbol 123Sb |  |
| has uses experimental, Nuclear Magnetic Resonance |  |
is an instance of antimony  |  |
| antimony 124 | has atomic mass 123.905038 |  |
| has decay mode β- (2.905 Mev) |  |
| has decay mode γ |  |
| has half life 60.30 days |  |
| has nuclear magnetic moment μ = 1.2 |  |
| has nuclear spin I = 3- |  |
| has number of neutrons 73 |  |
| has number of nucleons 124 |  |
| has symbol 124Sb |  |
| has uses research |  |
is an instance of antimony  |  |
| antimony 125 | has atomic mass 124.905252 |  |
| has decay mode β- (0.767 Mev) |  |
| has decay mode γ |  |
| has half life 2.758 years |  |
| has nuclear magnetic moment μ = +2.63 |  |
| has nuclear spin I = 7/2+ |  |
| has number of neutrons 74 |  |
| has number of nucleons 125 |  |
| has symbol 125Sb |  |
is an instance of antimony  |  |
| antimony 126 | has atomic mass 125.907250 |  |
| has decay mode β- (3.67 Mev) % |  |
| has decay mode γ |  |
| has half life 12.4 days |  |
| has nuclear magnetic moment μ = 1.3 |  |
| has nuclear spin I = 8- |  |
| has number of neutrons 75 |  |
| has number of nucleons 126 |  |
| has symbol 126Sb |  |
is an instance of antimony  |  |
| antimony 127 | has atomic mass 126.906919 |  |
| has decay mode β- (1.58 Mev) |  |
| has decay mode γ |  |
| has half life 3.84 days |  |
| has nuclear magnetic moment μ = 2.6 |  |
| has nuclear spin I = 7/2+ |  |
| has number of neutrons 76 |  |
| has number of nucleons 127 |  |
| has symbol 127Sb |  |
is an instance of antimony  |  |
| antineutrino | has antiparticle neutrino |  |
| has definition The antiparticle of a neutrino. | ![has source: [Silk90], 2001-09-19 14:33:13.0](facet.gif) |
| is a kind of antiparticle |  |
| is a kind of lepton |  |
| is a kind of neutral particle |  |
| antineutron | has antiparticle neutron |  |
| has definition The antiparticle of a neutron. A neutron and antineutron both have the same mass and zero electric charge, but can be differentiated by their interactions: a neutron and an antineutron can annihilate into gamma rays, while two neutrons cannot. | ![has source: [G97], 2001-09-19 14:33:13.0](facet.gif) |
| is an instance of antiparticle |  |
| is an instance of baryon |  |
| is an instance of neutral particle |  |
| is an instance of radioactive particle |  |
| antiparticle | has definition An elementary particle of opposite charge but otherwise identical to its partner. Most of the observable universe consists of particles and matter, as opposed to antiparticles and antimatter. | ![has source: [Silk90], 2001-09-19 14:33:13.0](facet.gif) |
| has definition Atomic particles that have the same mass as, but opposite charge and orbital direction to, an ordinary particle. Thus, instead of negatively charged electrons, atoms of antimatter have positrons. A quantity of antimatter coming into contact with matter would "cancel out" - annihilate, with total conversion of mass to energy - an exact proportion of matter corresponding to the original quantity of antimatter, provided that the elements in the matter also corresponded with the "elements" in the antimatter, i.e., that the atoms were equivalent but opposite. | ![has source: [A84], 2001-09-19 14:33:13.0](facet.gif) |
| has definition For every known type of particle, there exists an antiparticle with exactly the same mass, but with the opposite electric charge. When a particle and its antiparticle come together, they can always annihilate to form gamma rays. The antiparticle of an electrically neutral particle is sometimes the same as the original particle (e.g., photons) and sometimes it is distinct (e.g., neutrons). | ![has source: [G97], 2001-09-19 14:33:13.0](facet.gif) |
| has definition Particles predicted by combining the theories of special relativity and quantum mechanics. For each particle, there must exist an antiparticle with the opposite charge, magnetic moment and other internal quantum numbers (e.g., lepton number, baryon number, strangeness, charm, etc.), but with the same mass, spin and lifetime. Note that certain neutral particles (such as the photon and π0) are their own antiparticles. | ![has source: [CD99], 2001-09-19 14:33:13.0](facet.gif) |
| has definition Particles with identical mass and spin as those of ordinary matter, but with opposite charge. Antimatter has been produced experimentally, but little of it is found in nature. Why this should be so is one of the questions that must be answered by any adequate theory of the early universe. | ![has source: [F88], 2001-09-19 14:33:13.0](facet.gif) |
| is a kind of particle |  |
| antiproton | has antiparticle proton |  |
| has charge -1 |  |
| has definition The antiparticle of a proton, identical in mass and spin but of opposite (negative) charge. | ![has source: [Silk90], 2001-09-19 14:33:13.0](facet.gif) |
| is an instance of antiparticle |  |
| is an instance of baryon |  |
| is an instance of charged particle |  |
| is an instance of radioactive particle |  |
| antiquark | has antiparticle quark |  |
| has definition The antiparticle of the quark. | ![has source: [G97], 2001-09-19 14:33:14.0](facet.gif) |
| is a kind of antiparticle |  |
| is a kind of charged particle |  |
| is a kind of parton | ![has source: [CD99], 2001-09-19 14:33:14.0](facet.gif) |
| Antlia | has acronym Ant |  |
has boundary  |  |
| has genitive Antliae |  |
| has synonym Air Pump |  |
| is a part of celestial sphere |  |
is an instance of constellation named by de Lacaille  |  |
| Antonia Maury | has career Havard College Observatory  |  |
| is an instance of 19th century scientist |  |
| is an instance of astronomer |  |
| Ap star | has definition Peculiar A-type stars ("magnetic" A stars) that show abnormally strong lines, sometimes of varying intensity, of certain ionized metals. Recent evidence indicates that all Ap stars are slow rotators compared with normal A stars. | ![has source: [H76], 2001-09-19 14:35:47.0](facet.gif) |
| has definition Star with spectral type A in which the lines of one or several elements are abnormally enhanced. Traditionally the most important subgroups are Si λ4200, Hg-Mn and Cr-Eu-Sr stars. The latest objects of the latter group correspond to early F-type. | ![has source: [JJ95], 2001-09-19 14:35:47.0](facet.gif) |
| has definition Stars can be classified according to their surface temperatures, which determine, in large part, the spectrum of radiation they emit. A stars have surface temperatures between about 7,500 and 11,000 degrees centigrade. Peculiar A stars are A stars whose emitted radiation spectra have many of the characteristics of A stars but are peculiar in certain ways. | ![has source: [LB90], 2001-09-19 14:35:47.0](facet.gif) |
| is a kind of A star |  |
| is a kind of peculiar star |  |
| apastron | has antonym periastron |  |
| has definition The point in the orbit of one component of a binary system where it is farthest from the other. | ![has source: [H76], 2001-09-19 14:35:03.0](facet.gif) |
| has participants binary star |  |
| is an instance of binary star orbital event |  |
| aphelion | has antonym perihelion |  |
| has definition The point in a planetary orbit that is at the greatest distance from the Sun. | ![has source: [S92], 2001-09-19 14:35:04.0](facet.gif) |
| is an instance of Sun orbital event |  |
| aplanatic system | has definition A system of three lenses which, taken together, correct for spherical aberration, chromatic aberration, and coma. | ![has source: [H76], 2001-09-19 14:32:33.0](facet.gif) |
| is a kind of lens |  |
| apocenter | has antonym pericenter |  |
| has definition The point in the orbit of one component of a binary system which is farthest from the center of mass of the system. | ![has source: [H76], 2001-09-19 14:35:03.0](facet.gif) |
| has participants binary star |  |
| is an instance of binary star orbital event |  |
| apogalacticon | has antonym perigalacticon |  |
| has definition The point in a star's orbit farthest from the Galactic center. | ![has source: [C95], 2001-09-19 14:35:04.0](facet.gif) |
| is an instance of galaxy orbital event |  |
| apogee | has antonym perigee |  |
| has definition The point at which a body in orbit around the Earth reaches its farthest distance from the Earth. | ![has source: [S92], 2001-09-19 14:35:03.0](facet.gif) |
| is an instance of Earth orbital event |  |
| Apollo | has definition Prototype of a small group of asteroids whose orbits intersect that of Earth. | ![has source: [H76], 2001-09-19 14:37:09.0](facet.gif) |
| has eccentricity e = 0.57 | ![has source: [H76], 2001-09-19 14:37:09.0](facet.gif) |
| has inclination i = 6°.4 | ![has source: [H76], 2001-09-19 14:37:09.0](facet.gif) |
| has orbital period P = 622d | ![has source: [H76], 2001-09-19 14:37:09.0](facet.gif) |
| has semi-major axis a = 1.486 AU | ![has source: [H76], 2001-09-19 14:37:09.0](facet.gif) |
| is a part of Apollo asteroid |  |
| is an instance of Apollo asteroid |  |
| Apollo asteroid | has definition One of a small group of asteroids whose orbits intersect that of Earth. They are named for the prototype, Apollo. | ![has source: [H76], 2001-09-19 14:37:09.0](facet.gif) |
| is a kind of Earth-crossing asteroid |  |
| is a part of Earth-crossing asteroid |  |
| Apollo space program | has definition Successful US lunar exploration program in which the Apollo spacecraft 1 to 6 were unmanned; 7 to 10 were manned but did not land; and 11, 12 and 14 to 17 landed and returned safely. (Apollo 13 was an aborted mission.) The first men to land on the Moon were Neil Armstrong and Edwin Aldrin, from Apollo 11, on 20 July 1969. The final Apollo flight (17) lasted from 7 to 19 December 1972, and left a considerable quantity of exploratory devices on the lunar surface. | ![has source: [A84], 2001-09-19 14:37:21.0](facet.gif) |
| is an instance of space science institution |  |
| apparent magnitude | has definition A measure of how bright a star looks in the sky. The brighter the star, the smaller the apparent magnitude. A star that is one magnitude brighter than another (e.g., +1 versus +2) looks 2.5 times brighter. The brightest star of all, of course, is the Sun, whose apparent magnitude is -26.74, followed by Sirius, whose apparent magnitude is -1.46, Canopus (-0.72), Alpha Centauri (-0.27), Arcturus (-0.04), and Vega (+0.03). Stars of the Big Dipper are fainter, most of them around magnitude +2. On a clear, dark night, the unaided eye can see stars as faint as apparent magnitude +6, and the largest telescopes penetrate to apparent magnitude +30. | ![has source: [C95], 2001-09-19 14:38:09.0](facet.gif) |
| has definition Measure of the observed brightness of a celestial object as seen from the Earth. It is a function of the star's intrinsic brightness, its distance from the observer, and the amount of absorption by interstellar matter between the star and the observer. The mv, of Sun, -26.5 mag. A sixth-magnitude star is just barely visible to the naked eye. | ![has source: [H76], 2001-09-19 14:38:09.0](facet.gif) |
| is a kind of magnitude |  |
| apsidal motion | has definition Rotation of the line of apsides in the plane of the orbit; (in a binary) precession of the line of apsides due to mutual tidal distortion. | ![has source: [H76], 2001-09-19 14:34:51.0](facet.gif) |
| is an instance of precession |  |
| Apus | has acronym Aps |  |
has boundary  |  |
| has genitive Apodis |  |
| has synonym Bird of Paradise |  |
| is a part of celestial sphere |  |
is an instance of constellation named by Bayer  |  |
| Aquarius | has acronym Aqr |  |
has boundary  |  |
| has genitive Aquarii |  |
has historical image  |  |
| has synonym Water Bearer |  |
| is a part of Zodiac |  |
is an instance of zodiacal constellation  |  |
| Aquila | has acronym Aql |  |
has boundary  |  |
| has genitive Aquilae |  |
has historical image  |  |
| has historical origin the eagle that belonged to Zeus. Aquila's most famous task was carrying the mortal Ganymede to the heavens to serve as Zeus' cup bearer |  |
| has synonym Eagle |  |
| is a part of celestial sphere |  |
is an instance of constellation  |  |
| Ara | has acronym Ara |  |
has boundary  |  |
| has genitive Arae |  |
| has historical origin the altar of the centaur Chiron or the altar that Noah built after the great flood |  |
| has synonym Altar |  |
| is a part of celestial sphere |  |
is an instance of constellation  |  |
| arcminute | has definition A unit of angle equal to 1/60 of a degree. | ![has source: [LB90], 2001-09-19 14:37:40.0](facet.gif) |
| has equivalent 1/60 degree | ![has source: [LB90], 2001-09-19 14:37:40.0](facet.gif) |
| is an instance of angle unit |  |
| arcsecond | has definition One sixtieth of an arcminute, or 1/3600 of a degree. | ![has source: [C95], 2001-09-19 14:37:40.0](facet.gif) |
| has equivalent 1/3600 degree | ![has source: [C95], 2001-09-19 14:37:40.0](facet.gif) |
| has equivalent 1/60 arcminute | ![has source: [C95], 2001-09-19 14:37:40.0](facet.gif) |
| is an instance of angle unit |  |
| Arcturus | has B-V magnitude 1.23 |  |
| has declination +19 10 57 |  |
| has definition A beautiful orange star that is the brightest in the constellation Bootes and the fourth brightest in the night sky. It lies 34 light-years away and is a member of the thick-disk population. Historically, Arcturus is famous because it was one of the first stars to have its proper motion measured. | ![has source: [C95], 2001-09-19 14:36:26.0](facet.gif) |
| has definition An old subgiant disk star (K2 IIIp, mv = 0.06) about 11 pc distant. | ![has source: [H76], 2001-09-19 14:36:26.0](facet.gif) |
| has right ascension 14 15 39.6 |  |
| has spectral type K1IIIbCN-1 |  |
| has synonym Alpha Boötis | ![has source: [H76], 2001-09-19 14:36:26.0](facet.gif) |
| has synonym HR 5340 |  |
| has V magnitude -0.04 |  |
is a part of Boötes  |  |
| is an instance of bright giant |  |
| is an instance of K star |  |
| is an instance of naked eye star |  |
| area | is a kind of quantity |  |
| area unit | has definition square meter |  |
| has symbol m2 |  |
| is a kind of derived SI unit |  |
| Arecibo | has angular resolving power 5 arcminute |  |
| has effective diameter 300 meters |  |
| has position Puerto Rico |  |
has reference NAIC Arecibo Observatory  |  |
| is an instance of radio telescope |  |
| argon | has abundance 1 × 106 in Sun relative to H = 1 × 1012 |  |
| has abundance 1.2 p.p.m. in Earth's crust |  |
| has abundance 9300 p.p.m. in atmopshere |  |
| has atomic emission line 695.5431 nm for Ar I |  |
| has atomic emission line 706.7218 nm for Ar I |  |
| has atomic emission line 750.3869 nm for Ar I |  |
| has atomic emission line 801.4786 nm for Ar I |  |
| has atomic emission line 912.2967 nm for Ar I |  |
| has atomic emission line 965.7786 nm for Ar I |  |
| has atomic emission line 811.5311 nm for Ar I (strong) |  |
| has atomic number 18 |  |
| has atomic radii 174 pm |  |
| has biological role none |  |
| has boiling point 87.29 K |  |
| has chief source lquid air |  |
| has critical pressure 4862 kPa |  |
| has critical temperature 150.87 K |  |
| has crystal cell dimension a = 531.088 pm |  |
| has crystal type f.c.c |  |
| has daily dietary intake very low |  |
| has definition colourless, odourless gas comprising 1% of the atmosphere |  |
| has density 1.784 kg m-3 for gas at 273 K |  |
| has density 1380 kg m-3 for liquid at 87.29 K boiling point |  |
| has density 1656 kg m-3 for solid at 40 K |  |
| has discoverer Lord Rayleigh and Sir William Ramsay |  |
| has discovery date 1894 |  |
| has discovery location London and Bristol, England |  |
| has electron affinity -35 kJ mol-1 from Ar to Ar- |  |
| has electron configuration [Ne]3s23p6 in ground state |  |
| has hazard can asphyxiate if it excludes oxygen from the lungs |  |
| has heat capacity 20.786 J K-1 mol-1 for gas at constant pressure 0.1 MPa at 298.15 K |  |
| has heat of fusion 2.21 kJ mol-1 |  |
| has heat of vaporization 6.53 kJ mol-1 |  |
has image  |  |
| has isotope mass range 32 to 46 |  |
| has lethal intake non-toxic |  |
| has level in humans trace amounts in blood |  |
| has mass absorption coefficient 123 cm2 g-1 for CuKα X-ray diffraction |  |
| has mass absorption coefficient 13.5 cm2 g-1 for MoKα X-ray diffraction |  |
| has mass magnetic susceptibility -6.16 × 10-9 kg-1 m3 for gas |  |
| has mass of element in person very small for a 70 kg average person |  |
| has melting point 83.78 K |  |
| has mineral none |  |
| has molar volume 24.12 cm3 at 40 K |  |
| has name origin argos = inactive from Greek |  |
| has neutron scattering length 0.1909 × 10-12 cm |  |
| has number of isotopes 15 |  |
| has number of protons 18 |  |
| has ocean oxidation state 0 |  |
| has ocean residence time 28000 years |  |
| has pronunciation ar-gon |  |
has registry number 7440-37-1 for Chemical Abstracts System database  |  |
| has relative atomic mass 39.948 in units of 12C = 12.000 |  |
| has reserves 6.6 × 1013 tonnes in atmosphere |  |
| has space group Fm3m |  |
| has specimen available in small pressurized canisters. Safe. |  |
| has stable isotope argon 36 |  |
| has stable isotope argon 38 |  |
| has stable isotope argon 40 |  |
| has symbol Ar |  |
| has synthesis mechanism extracted from the atmosphere by liquefaction |  |
| has term symbol 1S0 in ground state |  |
| has thermal conductivity 0.0177 W m-1 K-1 at 300 K for gas |  |
| has thermal neutron capture cross section 0.675 barns |  |
| has toxic intake non-toxic |  |
| has uses inert atmosphere in lamps and high temperature metallurgy |  |
| has van der Waals radii 191 pm |  |
| has world production 700000 tonnes per year |  |
| is a kind of inert gas |  |
| is a kind of unclassified oceanic element |  |
| reacts with nothing |  |
| argon 36 | has atomic mass 35.96754552 |  |
| has natural abundance 0.337 % |  |
| has nuclear magnetic moment μ = 0 |  |
| has nuclear spin I = 0+ |  |
| has number of neutrons 18 |  |
| has number of nucleons 36 |  |
| has symbol 36Ar |  |
is an instance of argon  |  |
| argon 37 | has atomic mass 36.966776 |  |
| has decay mode EC (0.814 Mev) |  |
| has decay mode no γ |  |
| has half life 35.0 days |  |
| has nuclear magnetic moment μ = +1.15 |  |
| has nuclear spin I = 3/2+ |  |
| has number of neutrons 19 |  |
| has number of nucleons 37 |  |
| has symbol 37Ar |  |
| has uses research |  |
is an instance of argon  |  |
| argon 38 | has atomic mass 37.9627325 |  |
| has natural abundance 0.063 % |  |
| has nuclear magnetic moment μ = 0 |  |
| has nuclear spin I = 0+ |  |
| has number of neutrons 20 |  |
| has number of nucleons 38 |  |
| has symbol 38Ar |  |
is an instance of argon  |  |
| argon 39 | has atomic mass 38.962 |  |
| has decay mode β- (0.565 Mev) |  |
| has decay mode no γ |  |
| has half life 268 years |  |
| has nuclear magnetic moment μ = -1.3 |  |
| has nuclear spin I = 7/2- |  |
| has number of neutrons 21 |  |
| has number of nucleons 39 |  |
| has symbol 39Ar |  |
is an instance of argon  |  |
| argon 40 | has atomic mass 39.9623837 |  |
| has natural abundance 99.600 % |  |
| has nuclear magnetic moment μ = 0 |  |
| has nuclear spin I = 0+ |  |
| has number of neutrons 22 |  |
| has number of nucleons 40 |  |
| has symbol 40Ar |  |
is an instance of argon  |  |
| argon 41 | has atomic mass 40.964501 |  |
| has decay mode β- (2.492 Mev) |  |
| has decay mode γ |  |
| has half life 1.82 hours |  |
| has nuclear spin I = 7/2- |  |
| has number of neutrons 23 |  |
| has number of nucleons 41 |  |
| has symbol 41Ar |  |
is an instance of argon  |  |
| argon 42 | has atomic mass 41.963050 |  |
| has decay mode β- (0.60 Mev) % |  |
| has decay mode no γ |  |
| has half life 33 years |  |
| has nuclear spin I = 0+ |  |
| has number of neutrons 24 |  |
| has number of nucleons 42 |  |
| has symbol 42Ar |  |
is an instance of argon  |  |
| argon 44 | has atomic mass 43.963650 |  |
| has decay mode β- (3.54 Mev) |  |
| has decay mode γ |  |
| has half life 11.87 minutes |  |
| has nuclear spin I = 0+ |  |
| has number of neutrons 26 |  |
| has number of nucleons 44 |  |
| has symbol 44Ar |  |
is an instance of argon  |  |
| argument of the perihelion | has definition An orbital element representing the longitude of the ascending node plus the angle along the orbit from the ascending node to the perihelion point. | ![has source: [H76], 2001-09-19 14:38:26.0](facet.gif) |
| has definition Angular distance (measured in the plane of the object's orbit and in the direction of its motion) from the ascending node to the perihelion point. | ![has source: [H76], 2001-09-19 14:38:26.0](facet.gif) |
| has symbol ω | ![has source: [H76], 2001-09-19 14:38:26.0](facet.gif) |
| has synonym longitude of the perihelion | ![has source: [H76], 2001-09-19 14:38:26.0](facet.gif) |
| is an instance of angle |  |
| is an instance of orbital element |  |
| Ariel | has definition Second satellite of Uranus. | ![has source: [H76], 2001-09-19 14:37:05.0](facet.gif) |
| has diameter 1600 km | ![has source: [H76], 2001-09-19 14:37:05.0](facet.gif) |
| has discoverer Lassell | ![has source: [H76], 2001-09-19 14:37:05.0](facet.gif) |
| has discovery date 1851 | ![has source: [H76], 2001-09-19 14:37:05.0](facet.gif) |
| has period 2.52 days | ![has source: [H76], 2001-09-19 14:37:05.0](facet.gif) |
| is a part of Uranus |  |
| is an instance of natural satellite |  |
| Aries | has acronym Ari |  |
| has genitive Arietis |  |
has historical image  |  |
| has historical origin the ram sent by Hermes to carry the abused children of the King of Thessaly to safety |  |
| has synonym Ram |  |
| is a part of Zodiac |  |
is an instance of zodiacal constellation  |  |
| Arietids | is an instance of meteor shower |  |
| Aristotelian physics | has definition Physics as promulgated by Aristotle; includes the hypothesis that our world is comprised of four elements, and that the universe beyond the moon is made of a fifth element and so is fundamentally different from the mundane realm. | ![has source: [F88], 2001-09-19 14:38:56.0](facet.gif) |
| is a kind of outdated belief |  |
| array telescope | has definition a telescope composed of an array of separete individual elements acting in concert |  |
| has element aperture |  |
| has element separation |  |
| has number of elements |  |
| is a kind of electromagnetic telescope |  |
| arsenic | has abundance 1.45 × 10-3 p.p.m. in Atlantic surface seawater |  |
| has abundance 1.45 × 10-3 p.p.m. in Pacific surface seawater |  |
| has abundance 1.5 p.p.m. in Earth's crust |  |
| has abundance 1.53 × 10-3 p.p.m. in deep Atlantic seawater |  |
| has abundance 1.75 × 10-3 p.p.m. in deep Pacific seawater |  |
| has abundance see list in Sun relative to H = 1 × 1012 |  |
| has appearance metallic for α form |  |
| has atomic emission line 419.008 nm for As II |  |
| has atomic emission line 445.847 nm for As II |  |
| has atomic emission line 446.635 nm for As II |  |
| has atomic emission line 449.423 nm for As II |  |
| has atomic emission line 450.766 nm for As II |  |
| has atomic emission line 454.348 nm for As II |  |
| has atomic emission line 193.759 nm for As I (Strong, used in atom absorption spectrometry) |  |
| has atomic number 33 |  |
| has atomic radii 125 pm |  |
| has biological role essential to some species including humans |  |
| has boiling point 889 K sublimes |  |
| has chief source arsenopyrite, realgar and orpiment |  |
| has covalent radii 121 pm |  |
| has crystal cell dimension a = 376.0 pm for β form |  |
| has crystal cell dimension a = 413.18 pm for α form |  |
| has crystal cell dimension alpha angle = 54 deg 10' for α form |  |
| has crystal cell dimension c = 10.548 pm for β form |  |
| has crystal type hexagonal for β form |  |
| has crystal type rhombohedral for α form |  |
| has daily dietary intake 0.04 to 1.4 mg |  |
| has definition a metalloid element with two main forms, grey α arsenic and β arsenic |  |
| has density 4700 kg m-3 for solid at 293 K (β form) |  |
| has density 5780 kg m-3 for solid at 293 K (α form) |  |
| has discoverer Albertus Magnus |  |
| has discovery date 1250 |  |
| has discovery location Germany |  |
| has electrical resistivity 26 × 10-8 Ω m at 273 K |  |
| has electron affinity 78 kJ mol-1 from As to As- |  |
| has electron configuration [Ar]3d104s24p3 in ground state |  |
| has electronegativity 2.18 Pauling |  |
| has hardness brittle for α form |  |
| has hazard salts and arsine gases are very poisonous. Stimulates metabolism in small doses, but it is carcinogenic and possibly teratogenic |  |
| has heat capacity 20.786 J K-1 mol-1 for gas at constant pressure of 0.1 MPa at 298.15 K |  |
| has heat capacity 24.64 J K-1 mol-1 for solid at constant pressure of 0.1 MPa at 298.15 K |  |
| has heat of fusion 27.7 kJ mol-1 |  |
| has heat of vaporization 31.9 kJ mol-1 |  |
has image  |  |
| has ionic radii 46 pm for As5+ |  |
| has ionic radii 69 pm for As3+ |  |
| has isotope mass range 67 to 87 |  |
| has lethal intake 50 to 300 mg |  |
| has level in humans 0.0017 to 0.09 mg dm-3 in blood |  |
| has level in humans 0.009 to 0.65 p.p.m. in muscle |  |
| has level in humans 0.023 to 1.61 p.p.m. in liver |  |
| has level in humans 0.08 to 1.6 p.p.m. in bone |  |
| has linear expansion coefficient 4.6 × 10-6 K-1 |  |
| has main mining area not much mined as such because more than required is produced as a by-product of refining certain sulfide ores |  |
| has mass absorption coefficient 69.7 cm2 g-1 for MoKα X-ray diffraction |  |
| has mass absorption coefficient 83.4 cm2 g-1 for CuKα X-ray diffraction |  |
| has mass magnetic susceptibility -3.97 × 10-9 kg-1 m3 for β form |  |
| has mass magnetic susceptibility -9.17 × 10-10 kg-1 m3 for α form |  |
| has mass of element in person 0.5 to 15 mg for a 70 kg average person depending on diet |  |
| has melting point 1090 K for α form under pressure |  |
| has mineral arsenopyrite, conichalcite, enargite, lollingite, olivenite, orpiment and realgar |  |
| has molar volume 12.95 cm3 for α form |  |
| has molar volume 15.9 cm3 for β form |  |
| has name origin arsenikon = yellow orpiment from Greek |  |
| has neutron scattering length 0.658 × 10-12 cm |  |
| has number of isotopes 22 |  |
| has number of protons 33 |  |
| has ocean oxidation state V |  |
| has ocean residence time 90000 years |  |
| has pronunciation ahrs-nik |  |
has registry number 7440-38-2 for Chemical Abstracts System database  |  |
| has relative atomic mass 74.92159 in units of 12C = 12.000 |  |
| has space group R3m for α form |  |
| has specimen available as powder. Danger ! |  |
| has symbol As |  |
| has term symbol 4S3/2 in ground state |  |
| has thermal conductivity 50.0 W m-1 K-1 at 300 K for α form |  |
| has thermal neutron capture cross section 4.30 barns |  |
| has toxic intake 5 to 50 mg |  |
| has uses alloys, semiconductors, pesticides, wood preservatives and glass |  |
| has van der Waals radii 200 pm |  |
| has world production 47000 tonnes per year for As2O3 |  |
| is a kind of group V element |  |
| is a kind of nonmetallic metalloid |  |
| is a kind of recycled oceanic element |  |
| reacts with hot acids and molten NaOH, tarnishes burns in oxygen |  |
| arsenic 71 | has atomic mass 70.927114 |  |
| has decay mode β+ (2.013 Mev) 32% |  |
| has decay mode γ |  |
| has decay mode EC 68% |  |
| has half life 2.72 days |  |
| has nuclear magnetic moment μ = +1.6735 |  |
| has nuclear spin I = 5/2- |  |
| has number of neutrons 38 |  |
| has number of nucleons 71 |  |
| has symbol 71As |  |
is an instance of arsenic  |  |
| arsenic 72 | has atomic mass 71.926755 |  |
| has decay mode β+ (4.355 Mev) 77% |  |
| has decay mode γ |  |
| has half life 26.0 hours |  |
| has nuclear magnetic moment μ = -2.1566 |  |
| has nuclear spin I = 2- |  |
| has number of neutrons 39 |  |
| has number of nucleons 72 |  |
| has symbol 72As |  |
is an instance of arsenic  |  |
| arsenic 73 | has atomic mass 72.923827 |  |
| has decay mode γ |  |
| has decay mode EC (0.346 Mev) |  |
| has half life 80.3 days |  |
| has nuclear spin I = 3/2- |  |
| has number of neutrons 40 |  |
| has number of nucleons 73 |  |
| has symbol 73As |  |
| has uses research |  |
is an instance of arsenic  |  |
| arsenic 74 | has atomic mass 73.923827 |  |
| has decay mode β- (1.354 Mev) |  |
| has decay mode β- (2.562 Mev) 31% |  |
| has decay mode γ |  |
| has decay mode EC 37% |  |
| has nuclear magnetic moment μ = -1.597 |  |
| has nuclear spin I = 2- |  |
| has number of neutrons 41 |  |
| has number of nucleons 74 |  |
| has symbol 74As |  |
is an instance of arsenic  |  |
| arsenic 75 | has atomic mass 74.9215942 |  |
| has magnetogyric ratio 4.5804 × 107 rad T-1 s-1 |  |
| has natural abundance 100% |  |
| has NMR frequency 17.126 MHz where 1H = 100 MHz; 2.3488 T |  |
| has NMR receptivity 143 where 13C = 1.00 |  |
| has nuclear magnetic moment μ = +1.43947 |  |
| has nuclear quadrupole moment 0.314 × 10-28 m2 |  |
| has nuclear spin I = 3/2- |  |
| has number of neutrons 42 |  |
| has number of nucleons 75 |  |
| has relative NMR sensitivity 0.0251 where 1H = 1.00 |  |
| has symbol 75As |  |
| has uses Nuclear Magnetic Resonance |  |
is an instance of arsenic  |  |
| arsenic 76 | has atomic mass 75.922393 |  |
| has decay mode β- (2.97 Mev) |  |
| has decay mode γ |  |
| has half life 26.3 hours |  |
| has nuclear magnetic moment μ = -0.906 |  |
| has nuclear spin I = 2- |  |
| has number of neutrons 43 |  |
| has number of nucleons 76 |  |
| has symbol 76As |  |
is an instance of arsenic  |  |
| arsenic 77 | has atomic mass 76.920646 |  |
| has decay mode β- (0.6904 Mev) |  |
| has decay mode γ |  |
| has half life 38.8h |  |
| has nuclear spin I = 3/2- |  |
| has number of neutrons 44 |  |
| has number of nucleons 77 |  |
| has symbol 77As |  |
is an instance of arsenic  |  |
| artifact | has creation date |  |
| has creator |  |
| has definition an object made by humans |  |
| has owner |  |
| has purpose |  |
| is a kind of physical object |  |
| artificial satellite | has attitude control |  |
| has definition a satellite made by humans which is gravitationaly bound and in orbit of a larger physical object |  |
| has ground communication station |  |
| has launch date |  |
| has launch location |  |
| has launch vehicle |  |
| is a kind of instrument |  |
| is a kind of satellite |  |
| can have orbit decay date |  |
| AS Eri | has definition An eclipsing binary whose secondary is close to its Roche limit. | ![has source: [H76], 2001-09-19 14:35:36.0](facet.gif) |
| is an instance of eclipsing binary |  |
| ascending node | has definition In the orbit of a solar-system body, the point where the body crosses the ecliptic from south to north: for a star, out of the plane of the sky toward the observer. | ![has source: [H76], 2001-09-19 14:35:04.0](facet.gif) |
| is a kind of Sun orbital event |  |
| aspheric | has definition An optical surface with departures in shape from a perfect sphere in order to cancel optical imperfections or aberrations. | ![has source: [McL97], 2001-09-19 14:32:35.0](facet.gif) |
| has wavefront modification shape |  |
| is a kind of wavefront modifier |  |
| association | has definition A sparsely populated grouping (mass range 102-103 Msun) of very young, massive stars lying along a spiral arm of the Milky Way, whose spectral types or motions in the sky indicate a common origin. The star density is insufficient for gravitation to hold the group together against shear by differential galactic rotation, but the stars have not yet had time to disperse completely. OB associations are composed of stars of spectral types O-B2; T associations have many young T Tauri stars. The internationally approved designation for associations is the name of the constellation followed by an arabic numeral - e.g., Perseus OB2. | ![has source: [H76], 2001-09-19 14:35:54.0](facet.gif) |
| has most luminous member |  |
| is a kind of collection of stars |  |
| astatine | has image  |  |
| is a kind of halogen |  |
| asterism | has definition a group of bright stars which form a conspicuous pattern on the celestial sphere |  |
| has purpose to easily recognize a part of the sky |  |
| is a part of constellation |  |
| is an instance of equatorial sky area |  |
| asteroid | has asteroid number |  |
| has definition A small planet-like body of the solar system, <e> ≃ 0.15, <i> ≃ 9°.7 . More than 1800 have been catalogued, and probably millions of smaller ones exist, but their total mass would probably be less than 3 percent that of the Moon. Their densities are poorly known (about 2.6 g cm-3), but they suggest a composition similar to carbonaceous chondrite. The bright asteroids are presumably original condensations and those fainter than about 14-15 mag are collision fragments. Asteroids and short-period comets have some orbital similarities. Also called minor planet | ![has source: [H76], 2001-09-19 14:37:07.0](facet.gif) |
| has definition A small rocky body that orbits a star. In the solar system, most asteroids lie between the orbits of Mars and Jupiter. The largest asteroid is Ceres, about 900 kilometers in diameter. | ![has source: [C95], 2001-09-19 14:37:07.0](facet.gif) |
| has definition Also called planetoids or minor planets, the asteroids are tiny planets most of which orbit the Sun between Mars and Jupiter. The largest - and the first discovered - is Ceres, with a diameter of 1,003 km. It is estimated that there may altogether be no fewer than 40000. A few have very elliptical orbits and cross the orbits of several other (major) planets. One or two even have their own satellites (moons). | ![has source: [A84], 2001-09-19 14:37:07.0](facet.gif) |
| has synonym minor planet | ![has source: [H76], 2001-09-19 14:37:07.0](facet.gif) |
| has synonym planetoid | ![has source: [A84], 2001-09-19 14:37:07.0](facet.gif) |
| is a kind of celestial body |  |
| is a part of our solar system |  |
| asteroid belt | has definition A region of space lying between Mars (1.5 AU) and Jupiter (5.2 AU), where the great majority of the asteroids are found. None of the belt asteroids have retrograde motion. | ![has source: [H76], 2001-09-19 14:36:49.0](facet.gif) |
| has mean distance from Sun 1.5 to 5.2 AU |  |
| is a kind of celestial body |  |
| is a part of our solar system |  |
| asteroid impact | is a kind of impact event |  |
| astrology | has definition Divination using the positions of the planets, the Sun and the Moon as seen against the stars in the constellations of the zodiac - a "science" almost as old as homo sapiens. Although at one stage in history astrology and astronomy were almost synonymous- the latter has advanced so far during the last three centuries that the two now bear little relation to each other. | ![has source: [A84], 2001-09-19 14:38:56.0](facet.gif) |
| has definition The belief that human affairs and people's personalities and characters are influenced by (or encoded in) the positions of the planets. | ![has source: [F88], 2001-09-19 14:38:56.0](facet.gif) |
| is a kind of outdated belief |  |
| astrometric binary | is a kind of binary star |  |
| astrometry | has definition The branch of astronomy that deals with measuring the positions of celestial objects, especially stars. Astrometrists measure parallaxes and proper motions, which allow astronomers to determine the distances and velocities of the stars. | ![has source: [C95], 2001-09-19 14:37:25.0](facet.gif) |
| is a kind of galactic astronomy |  |
| astronomer | has definition a scientist specializing in astronomy |  |
| has domain astronomy |  |
| is a kind of scientist |  |
| astronomical catalog | is a kind of data collection |  |
| astronomical constant | is a kind of constant |  |
| astronomical horizon event | has definition The time and azimuth at which a celestial body crosses the astronomical horizon of an oberver. | ![has source: [T01], 2001-09-19 14:35:02.0](facet.gif) |
| is a kind of location dependent periodic celestial event |  |
| Astronomical Image Processing System | has acronym AIPS | ![has source: [McL97], 2001-09-19 14:37:21.0](facet.gif) |
has definition Developed by the National Radio Astronomy Observatory.  | ![has source: [McL97], 2001-09-19 14:37:21.0](facet.gif) |
| is a kind of astronomical software |  |
| astronomical institution | is a kind of institution |  |
| astronomical refraction | has definition The change in direction of travel (bending) of a light ray as it passes obliquely through the atmosphere. As a result of refraction, the observed altitude of a celestial object is greater than its geometric altitude. The amount of refraction depends on the altitude of the object and on atmospheric conditions. | ![has source: [S92], 2001-09-19 14:34:45.0](facet.gif) |
| is a kind of refraction |  |
| astronomical software | is a kind of abstraction |  |
| astronomical unit | has definition Mean distance between the Earth and the Sun: 1.495985 × 1011 m. | ![has source: [A84], 2001-09-19 14:37:39.0](facet.gif) |
| has definition The AU is the preferred unit for distances within the solar system. Mercury, the innermost planet, lies on average 0.39 AU from the Sun; Pluto, normally the farthest planet, lies on average 39.5 AU from the Sun. | ![has source: [C95], 2001-09-19 14:37:39.0](facet.gif) |
| has definition The mean distance between the Earth and the Sun. The astronomical unit is defined as the length of the radius of the unperturbed circular orbit of a body of negligible mass moving around the Sun with a sidereal angular velocity of 0.017202098950 radian per day of 86400 ephemeris seconds. AU = 1.496 × 1013 cm ≈ 500 lt-sec. | ![has source: [H76], 2001-09-19 14:37:39.0](facet.gif) |
| has definition The mean distance from the earth to the sun, equal to 92.81 million miles or 499.012 light-seconds. | ![has source: [F88], 2001-09-19 14:37:39.0](facet.gif) |
| has definition The radius of a circular orbit in which a body of negligible mass, and free of perturbations, would revolve around the Sun in 2π / k days, where k is the Gaussian gravitational constant. This is slightly less than the semi-major axis of the Earth's orbit. | ![has source: [S92], 2001-09-19 14:37:39.0](facet.gif) |
| has symbol AU | ![has source: [H76], 2001-09-19 14:37:39.0](facet.gif) |
| has value in SI unit 1 au = 1.49598 × 1011 m, approximately |  |
| is an instance of length unit |  |
| is an instance of non SI unit |  |
| astronomy | has definition The science that studies the natural world beyond the earth. | ![has source: [F88], 2001-09-19 14:37:25.0](facet.gif) |
| is a kind of science |  |
| astronomy theory | has domain astronomy |  |
| is a kind of theory |  |
| Astrophysical Data Facility | has acronym ADF |  |
has definition Is responsible for designing, developing, and operating data systems that support the processing, management, archiving and distribution of NASA mission data. The ADF serves three broadly-defined astrophysics disciplines: high-energy astrophysics, UV/optical astrophysics, and infrared/submillimeter/radio astrophysics. The ADF collaborates with the GSFC Laboratory for High Energy Astrophysics (LHEA) and the Laboratory for Astronomy and Solar Physics (LASP) in managing data for specific missions. The ADF staff also support the astrophysics community's access to multi-mission and multi-spectral data archives in the National Space Science Data Center (NSSDC).  |  |
| has location Goddard Space Flight Center |  |
| is an instance of database |  |
| Astrophysical Research Consortium Telescope | has altitude 2800 m |  |
| has aperture 3.5 m |  |
| has creation date 1994 |  |
| has focal ratio f/1.75 |  |
| has latitude 32° 47' N |  |
| has location New Mexico, US |  |
| has longitude 105° 49' W |  |
| has mirror maker R. Angel, B. Martin |  |
| has mirror type spin-cast borosilicate honey-comb |  |
| has owner Apache Point |  |
| has synonym ARC 3.5 m |  |
| is an instance of altazimuth telescope |  |
| is an instance of optical telescope |  |
| is an instance of reflector |  |
| astrophysics | has definition The science that studies the physics and chemistry of extraterrestrial objects. The alliance of physics and astronomy, which began with the advent of spectroscopy, made it possible to investigate what celestial objects are and not just where they are. | ![has source: [F88], 2001-09-19 14:37:25.0](facet.gif) |
| is a kind of physics |  |
| Astroweb | is an instance of database  |  |
| asymptotic branch star | has definition Globular cluster stars, which are found in that part of the HR diagram that connects the top pf the giant tip with the horizontal branch stars. | ![has source: [JJ95], 2001-09-19 14:35:25.0](facet.gif) |
| is a kind of star |  |
| atmophile element | has definition volatile element that tends to be found in the atmosphere of a planet or asteroid |  |
| has occurrence atmosphere of a planet or asteroid |  |
| is a kind of planetary element |  |
| atmosphere | has composition 78% nitrogen and 21% oxygen (with 1% of other gases) by volume | ![has source: [A84], 2001-09-19 14:36:53.0](facet.gif) |
| has definition A unit of pressure. | ![has source: [JM92], 2001-09-19 14:37:37.0](facet.gif) |
| has definition Mantle of gases round a star planet or moon, sometimes even forming the apparent surface of the body. For a body to retain an atmosphere depends on the body's gravity, and the temperature and composition of the gases. Mean atmospheric pressure at the surface is 10330 kg/m2, and is also referred to as atmosphere. | ![has source: [A84], 2001-09-19 14:36:53.0](facet.gif) |
| has equivalent 1.013 bars | ![has source: [H76], 2001-09-19 14:37:37.0](facet.gif) |
| has equivalent 101325 pascals | ![has source: [JM92], 2001-09-19 14:37:37.0](facet.gif) |
| has equivalent 14.07 lb in-2 | ![has source: [JM92], 2001-09-19 14:37:37.0](facet.gif) |
| has equivalent 760 torr | ![has source: [JM92], 2001-09-19 14:37:37.0](facet.gif) |
| is a part of Earth |  |
| is an instance of pressure unit |  |
| atmospheric dispersion corrector | has definition An optical device usually comprising two thin prisms which can rotate to compensate for the elongation of a star image caused by the wavelength dependence of the refractive index of air. | ![has source: [McL97], 2001-09-19 14:32:35.0](facet.gif) |
| has wavefront modification wavelength |  |
| is a kind of wavefront modifier |  |
| atmospheric extinction | has definition Decrease in the intensity of light from a celestial body due to absorption and scattering by the Earth's atmosphere. The extinction increases from the zenith to the horizon and affects short wavelengths more than long wavelengths, so that objects near the horizon appear redder than they are at the zenith. | ![has source: [H76], 2001-09-19 14:34:45.0](facet.gif) |
| is a kind of selective absorption |  |
| atomic constant | is a kind of fundamental physical constant |  |
| atomic mass constant | has approval date 1961 | ![has source: [H76], 2001-09-19 14:38:02.0](facet.gif) |
| has definition One-twelfth the mean |