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| naked eye star | ||||
| subject | fact | |||
| naked eye star | has been observed for many centuries | ![]() |
| is usually part of asterism | ![]() | |
| is a part of celestial sphere | ![]() | |
| is a part of Milky Way | ![]() | |
| has apparent magnitude brighter than 5 | ![]() | |
| has definition A star visible without visual aids | ![]() | |
| is a kind of star | ![]() | |
| is a kind of naked eye object | ![]() | |
| star | has star surface temperature | ![]() |
| has spectral type | ![]() | |
| has V magnitude | ![]() | |
| has B magnitude | ![]() | |
| has U magnitude | ![]() | |
| has position on celestial sphere from the point of view of Earth | ![]() | |
| has parallax from the point of view of Earth's orbit | ![]() | |
| has proper motion | ![]() | |
| has radiation at surface which is diffused out from the hotter core | ![]() | |
| has energy source gravitational contraction and or fusion | ![]() | |
| has energy production which takes place primarily within the core | ![]() | |
| has surface density which depends on luminosity class | ![]() | |
| has surface temperature greater than 1000 Kelvin | ![]() | |
| has absolute magnitude | ![]() | |
| has age | ![]() | |
| has catalog star catalog | ![]() | |
| has material hydrogen, helium | ![]() | |
| has velocity determined from proper motion and radial velocity | ![]() | |
| has mass greater than 0.08 the sun's mass | ![]() | |
| celestial body | has spectra | ![]() |
| physical object | has location or center of gravity | ![]() |
| has angular momentum | ![]() | |
| has momentum | ![]() | |
| has temperature | ![]() | |
| has volume | ![]() | |
| has extent | ![]() |
Kinds of naked eye star :
(15 facts) (omicron Cet) - A red giant that varies in brightness as it pulsates. When brightest, Mira is visible to the naked eye; when dimmest, Mira can be viewed only with optical aid. Mira is the prototype of all pulsating red giants, which are called Miras in its honor., A irregular long-period intrinsic variable. It was named Mira ("wonderful") in 1596 by Fabricius, who made the first recorded observations of its brightness fluctuations. Mira is a double star with a faint B companion which is itself variable.
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