Tau Geminorum

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Template:Short description

Tau Geminorum
Template:Location mark
Location of τ Geminorum (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Gemini
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +4.42[2]
Characteristics
Spectral type K2 III[3]
U−B Template:Engvar +1.41[2]
B−V Template:Engvar +1.261[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[3] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[1]
Dec.: Script error: No such module "val". mas/yr[1]
Parallax (π)8.3261±0.1591 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Script error: No such module "val".[3]
Details
MassScript error: No such module "val".[3] Template:Solar mass
RadiusScript error: No such module "val".[4] Template:Solar radius
LuminosityScript error: No such module "val".[4] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[3] cgs
TemperatureScript error: No such module "val".[4] K
Metallicity [Fe/H]Script error: No such module "val".[3] dex
Rotational velocity (v sin i)5.8[5] km/s
AgeScript error: No such module "val".[3] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBADdata

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Tau Geminorum, Latinized from τ Geminorum, is a star in the northern zodiac constellation of Gemini. It has the apparent visual magnitude of +4.42,[2] making it visible to the naked eye under suitably good seeing conditions. This star is close enough to the Earth that its distance can be measured using the parallax technique, which yields a value of roughly Script error: No such module "convert"..[1]

File:Tau Geminorum and brown dwarf.png
Artist's illustration of the giant star Tau Geminorum (left) and its brown dwarf companion—the dark disk at right.

It is an evolved giant star of the spectral type K2 III. It has double[6] the mass of the Sun and has expanded to 30 times the Sun's radius. Tau Geminorum is radiating 364[4] times as much radiation as the Sun from its expanded outer atmosphere at an effective temperature of 4,583 K,[4] giving it the characteristic orange-hued glow of a K-type star. It appears to be rotating slowly with a projected rotational velocity of Script error: No such module "val"..[5]

Substellar companion

This star has a brown dwarf companion designated Tau Geminorum b, whose mass is at least 20.6 Jupiter masses.[3] It was discovered in 2004 by Mitchell and colleagues, who also discovered Nu Ophiuchi b at the same time.[7] This brown dwarf takes Script error: No such module "convert". to revolve around Tau Gem. It may also have a stellar companion; a magnitude 11, K0 dwarf at a projected separation of about Script error: No such module "val"..[3]

The Tau Geminorum system [3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b Script error: No such module "val". 1.17 Script error: No such module "val". Script error: No such module "val".

References

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  1. a b c d e Template:Cite Gaia DR3
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  4. a b c d e Script error: No such module "Citation/CS1".
  5. a b Script error: No such module "citation/CS1".
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Template:Stars of Gemini