82 Cancri

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Template:Short description Template:Other stars by Bayer designation

82 Cancri
Template:Location mark
Location of 82 Cancri (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Cancer[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) +5.33[3]
Characteristics
Spectral type K1 III[4]
U−B Template:Engvar +1.31[3]
B−V Template:Engvar +1.32[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: −41.018 mas/yr[2]
Dec.: −11.304 mas/yr[2]
Parallax (π)5.6869±0.0902 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−0.98[1]
Details
MassScript error: No such module "val".[6] Template:Solar mass
RadiusScript error: No such module "val".[2] Template:Solar radius
LuminosityScript error: No such module "val".[2] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[2] cgs
TemperatureScript error: No such module "val".[2] K
Metallicity [Fe/H]Script error: No such module "val".[7] dex
Rotational velocity (v sin i)Script error: No such module "val".[8] km/s
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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82 Cancri is a solitary,[4] orange-hued star in the zodiac constellation of Cancer. It has the Bayer designation Pi2 Cancri, which is Latinized from π2 Cancri; 82 Cancri is the star's Flamsteed designation. The star lies just a degree to the south of the ecliptic.[10] With an apparent visual magnitude of +5.33,[3] it is dimly visible to the naked eye on a dark night. This star is located at a distance of approximately Script error: No such module "convert". from the Sun based on parallax measurements. At that range, the visual magnitude is diminished by an extinction of 0.10 magnitudes due to interstellar dust.[11] It is drifting further away with a radial velocity of +27.5 km/s.[5]

This is an evolved K-type giant star with a stellar classification of K1 III,[4] having exhausted the supply of hydrogen at its core then cooled and expanded off the main sequence. The star 2.6[6] times the Sun's mass and has expanded to 31[2] times the girth of the Sun. It is spinning slowly with a projected rotational velocity. This star is radiating 435 times the Sun's luminosity from its enlarged photosphere at an effective temperature of 4,703 K.[2] Based on its abundance of iron, the star has a lower abundances of heavier elements than the Sun.[7]

References

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  2. a b c d e f g h i j Template:Cite Gaia DR3
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Template:Stars of Cancer