Tau6 Eridani

Tau6 Eridani, Latinized from τ6 Eridani, is a single star in the equatorial constellation of Eridanus, located near the constellation border with Fornax. It has a yellow-white hue with an apparent visual magnitude of 4.22, which is bright enough to be seen with the naked eye. Based upon parallax measurements, the distance to this star is around 57.5 light years. It is drifting further away with a radial velocity of +8 km/s.

τ6 Eridani
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Eridanus
Right ascension 03h 46m 50.88819s
Declination −23° 14 59.0046
Apparent magnitude (V) 4.22
Characteristics
Spectral type F5IV-V
U−B color index −0.03
B−V color index +0.43
Astrometry
Radial velocity (Rv)8.0±0.8 km/s
Proper motion (μ) RA: −158.84 mas/yr
Dec.: −528.95 mas/yr
Parallax (π)56.73 ± 0.19 mas
Distance57.5 ± 0.2 ly
(17.63 ± 0.06 pc)
Absolute magnitude (MV)2.98
Details
Mass1.35 M
Radius1.80+0.08
−0.03
 R
Luminosity5.47±0.06 L
Surface gravity (log g)4.21±0.13 cgs
Temperature6,584+47
−144
 K
Metallicity [Fe/H]−0.03±0.11 dex
Rotational velocity (v sin i)16.25 km/s
Age2.0 Gyr
Other designations
τ6 Eri, 27 Eridani, CD−23°1565, FK5 140, GC 168827, HD 23754, HIP 17651, HR 1173, SAO 101600
Database references
SIMBADdata

The spectrum of Tau6 Eridani matches a stellar classification of F5IV-V, indicating it is an F-type star that shows traits of both a main sequence star and a subgiant. It has an estimated 135% of the Sun's mass and about 1.8 time the radius of the Sun. The star is radiating 5.5 times the luminosity of the Sun at an effective temperature of 6,508 K, and it does not display any surface magnetic activity. The star has been examined for infrared excess emission that could indicate the presence of circumstellar matter, but none has been detected.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.