18 Tauri

Star in the constellation Taurus From Wikipedia, the free encyclopedia

18 Tauri is a single[9] star in the zodiac constellation of Taurus, located 452 light years away from the Sun. It is visible to the naked eye as a faint, blue-white hued star with an apparent visual magnitude of 5.66.[2] The star is moving further from the Earth with a heliocentric radial velocity of +4.8 km/s.[5] It is a member of the Pleiades[10] open cluster, which is positioned near the ecliptic and thus is subject to lunar occultations.[11]

Right ascension03h 45m 09.74013s[1]
Declination+24° 50 21.3432[1]
Quick facts Constellation, Right ascension ...
18 Tauri
Image of the Pleiades star cluster
18 Tauri in the Pleiades, circled in red
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 03h 45m 09.74013s[1]
Declination +24° 50 21.3432[1]
Apparent magnitude (V) 5.66[2]
Characteristics
Evolutionary stage main sequence[3]
Spectral type B8 V[4]
B−V color index −0.064±0.012[2]
Astrometry
Radial velocity (Rv)+4.8±0.8[5] km/s
Proper motion (μ) RA: +20.218[1] mas/yr
Dec.: −46.124[1] mas/yr
Parallax (π)7.2222±0.0551 mas[1]
Distance452 ± 3 ly
(138 ± 1 pc)
Absolute magnitude (MV)0.19[2]
Details
Mass3.34±0.06[3] M
Radius2.89[6] R
Luminosity160+18
−15
[3] L
Surface gravity (log g)4.126±0.113[7] cgs
Temperature13,748±223[7] K
Rotational velocity (v sin i)212[3] km/s
Age204[1] Myr
Other designations
18 Tau, BD+24°546, GC 4485, HD 23324, HIP 17527, HR 1144, SAO 76137[8]
Database references
SIMBADdata
Close

This is a B-type main-sequence star with a stellar classification of B8 V,[4] and is about halfway through its main sequence lifetime.[3] It displays an infrared excess, suggesting the presence of an orbiting debris disk with a black body temperature of 75 K at a separation of 137.8 AU from the host star.[6] The star has 3.34[3] times the mass of the Sun and 2.89[6] times the Sun's radius. It is radiating 160[3] times the Sun's luminosity from its photosphere at an effective temperature of 13,748 K.[7] 18 Tauri has a high rate of spin, showing a projected rotational velocity of 212 km/s.[3]

References

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