Psi7 Aurigae

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Psi7 Aurigae
Template:Location mark
Location of ψ7 Aurigae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Auriga[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 5.02[3]
Characteristics
Spectral type K3 III[4]
U−B Template:Engvar +1.35[3]
B−V Template:Engvar +1.27[3]
R−I Template:Engvar 0.46Script error: No such module "Unsubst".
Astrometry
Radial velocity (Rv)+59.53±0.25[5] km/s
Proper motion (μ) RA: −25.542 mas/yr[2]
Dec.: −137.253 mas/yr[2]
Parallax (π)9.6073±0.1274 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.33[1]
Details
Mass1.72Script error: No such module "Su".[6] Template:Solar mass
Radius19.680[7] Template:Solar radius
Luminosity162Script error: No such module "Su".[6] Template:Solar luminosity
Surface gravity (log g)2.35[8] cgs
Temperature4,340±90[6] K
Metallicity [Fe/H]0.00[8] dex
Rotational velocity (v sin i)10[9] km/s
Age700±200[6] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[10]
Database references
SIMBADdata

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File:Psi7 Aurigae.jpg
ψ7 Aurigae in optical light

Psi7 Aurigae, is a star in the northern constellation of Auriga. Its name is a Bayer designation that is Latinized from ψ7 Aurigae, and abbreviated Psi7 Aur or ψ7 Aur. This is a dim, naked eye star with an apparent visual magnitude of 5.02. Based upon parallax measurements, it is approximately Script error: No such module "convert". distant from Earth. It is receding from the Sun with a radial velocity of +60 km/s.[5] Psi7 Aur is a probable member of the Hercules stream of co-moving stars.[11]

ψ7 Aur is an evolved giant star with a stellar classification of K3 III.[4] With 1.7[6] times the mass of the Sun, at an age of about 700 million[11] it has expanded to almost 20 times the Sun's radius.[7] The outer envelope has an effective temperature of 4,340,[6] giving it an orange colour and a classification as a K-type star.[12] Although cooler than the sun, its larger size means that it is more luminous, emitting in total 162 times as much electromagnetic radiation.[6]

It was also known to be part of a much bigger constellation named Telescopium Herschelii before it was unrecognized by the International Astronomical Union (IAU).Script error: No such module "Unsubst".

References

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External links

Template:Stars of Auriga