YY Orionis star Comparison Table

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physical object > natural object > celestial body > star > emission line star > T Tauri star > YY Orionis star

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YY Orionis star comparison table

Subject has spectral type is part of has extent has age has surface temperature is an instance of has velocity has surface density has star surface temperature has optical brightness variation has V magnitude has parallax has observational problem has light curve has position on celestial sphere has location has angular momentum has radiation at surface has B magnitude has temperature has spectra has proper motion has amplitude has energy source has energy production has catalog has absolute magnitude has U magnitude has volume has momentum has apparent magnitude has material has mass has name designated with has emission line has observable variation time scale has synonym has definition has spectra peculiarity

YY Orionis cooler than G2 Orion greater than 1000 Kelvin YY Orionis star determined from proper motion and radial velocity which depends on luminosity class 0.2 magnitudes or greater from the point of view of Earth's orbit some difficulty in distinguishing between various kinds from the point of view of Earth or center of gravity which is diffused out from the hotter core gravitational contraction and or fusion which takes place primarily within the core star catalog hydrogen, helium greater than 0.08 the sun's mass
R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name
RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted
AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted
V 335, V 336, etc., when the double letter designations are exhausted
within a period of decades nebular variable An extremely young star (younger than T Tauri) in the Orion Nebula. inverse P Cyg type emission profiles in the Ca II HK lines

Next T Tauri star: FU Ori star Up: T Tauri star Previous T Tauri star: RW Aurigae

Subject	has spectral type	is part of	has extent	has age	has surface temperature	is an instance of	has velocity	has surface density	has star surface temperature	has optical brightness variation	has V magnitude	has parallax	has observational problem	has light curve	has position on celestial sphere	has location	has angular momentum	has radiation at surface	has B magnitude	has temperature	has spectra	has proper motion	has amplitude	has energy source	has energy production	has catalog	has absolute magnitude	has U magnitude	has volume	has momentum	has apparent magnitude	has material	has mass	has name designated with	has emission line	has observable variation time scale	has synonym	has definition	has spectra peculiarity
YY Orionis	cooler than G2	Orion			greater than 1000 Kelvin	YY Orionis star	determined from proper motion and radial velocity	which depends on luminosity class		0.2 magnitudes or greater		from the point of view of Earth's orbit	some difficulty in distinguishing between various kinds		from the point of view of Earth	or center of gravity		which is diffused out from the hotter core						gravitational contraction and or fusion	which takes place primarily within the core	star catalog						hydrogen, helium	greater than 0.08 the sun's mass	R, S, T, U, V, W, X, Y, or Z and the genitive of the latin constellation name RR, RS, RT, RU, RV, RW, RX, RY, or RZ and the genitive of the latin constellation name when the single letter designations are exhausted AA...AZ, BB...BZ, etc. (omitting J), which ends with QQ...QZ and the genitive of the latin constellation namewhen the RR...RZ designations are exhausted V 335, V 336, etc., when the double letter designations are exhausted		within a period of decades	nebular variable	An extremely young star (younger than T Tauri) in the Orion Nebula.	inverse P Cyg type emission profiles in the Ca II HK lines