119 Tauri

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119 Tauri
119 Tauri(english)new.png
The sky position of 119 Tauri
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Taurus
Right ascension 05h 32m 12.75251s[1]
Declination +18° 35′ 39.2436″[1]
Apparent magnitude (V) 4.33[2] (4.23-4.54[3])
Characteristics
Spectral type M2Iab-Ib[3]
U−B color index +2.23[2]
B−V color index +2.08[2]
Variable type SRc[3]
Astrometry
Radial velocity (Rv) +23.75[4] km/s
Proper motion (μ) RA: 1.86[1] mas/yr
Dec.: −4.48[1] mas/yr
Parallax (π) 1.82 ± 0.26[1] mas
Distance approx. 1,800 ly
(approx. 550 pc)
Absolute magnitude (MV) −5.20[5]
Details
Mass 8.0[6] M
Radius 601[6] R
Luminosity 43,000[6] L
Surface gravity (log g) -0.21[6] cgs
Temperature 3,400[6] K
Metallicity 0.0[6]
Other designations
CE Tauri, HR 1845, HD 36389, BD+18°875, HIP 25945, SAO 94628, GC 6841, AAVSO 0526+18
Database references
SIMBAD data

119 Tauri (CE Tau) is a star in the constellation Taurus. It is one of the largest stars known, having a diameter about 600 times that of the Sun. CE Tau is close enough that its distance can be determined accurately by parallax and so the actual diameter can be determined directly from the angular diameter.

119 Tauri is a M-type red supergiant with a mean apparent magnitude of +4.32. It is approximately 1,800 light years from Earth. The star is classified as a semiregular variable star and its brightness varies from magnitude +4.23 to +4.54 with a period of 165 days.[3] With a colour index of +2.07, it is one of the reddest naked eye stars in the night sky.[2] CE Tauri lies 4.6 degrees off the ecliptic. This makes it a candidate for occultations by the Moon and (extremely rarely) by one of the bright planets. The star's angular diameter and a linear radius of 450 Solar radii have been measured in three colors by lunar occultation.[7] The diameter has also been measured directly by VLTI, leading to a measurement of the radius with a margin of error of 83 R.[6]

Notes

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