HD 82205
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Antlia[1] |
| Right ascension | Template:RA[2] |
| Declination | Template:DEC[2] |
| Apparent magnitude (V) | 5.48±0.01[3] |
| Characteristics | |
| Spectral type | K3 III[4] |
| B−V Template:Engvar | +1.36[5] |
| Astrometry | |
| Radial velocity (Rv) | 12±2[6] km/s |
| Proper motion (μ) | RA: −21.883 mas/yr[2] Dec.: +0.761 mas/yr[2] |
| Parallax (π) | 4.0447±0.0731 mas[2] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | −1.42[1] |
| Details | |
| Mass | 4.46[7] Template:Solar mass |
| Radius | 38.86[8] Template:Solar radius |
| Luminosity | 552[9] Template:Solar luminosity |
| Surface gravity (log g) | 1.61±0.01[10] cgs |
| Temperature | 4,413±122[8] K |
| Metallicity [Fe/H] | +0.09[11] dex |
| Rotational velocity (v sin i) | <1[12] km/s |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| Template:Odlist[13] | |
| Database references | |
| SIMBAD | data |
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HD 82205 (HR 3770) is a solitary star[14] in the southern constellation Antlia. It is faintly visible to the naked eye with an apparent magnitude of 5.48[3] and is estimated to be 810 light years[2] distant based on parallax measurements. However, it is receding with a heliocentric radial velocity of Script error: No such module "val"..[6]
HD 82205 has a general stellar classification of K3 III, indicating that it is a red giant. However, Houk and Cowley (1982) found a slightly warmer class of K2 III CNII,[15] which also suggests a strong overabundance of cyano radicals in the stellar atmosphere. At present it has 4.46 times the mass of the Sun[7] but has expanded to 38.9 times its girth.[8] It shines with a luminosity of Script error: No such module "val".[9] from its enlarged photosphere at an effective temperature of Script error: No such module "val".,[8] giving an orange hue. HD 82205 has a metallicity 123% that of the Sun and is believed to be a member of the thin disk population.[11] Currently, it spins with a projected rotational velocity lower than Script error: No such module "val"..[12]
There is a 14th magnitude optical companion separated Script error: No such module "val". away along a position angle of Script error: No such module "val"..[16] The object was first noticed by T.J.J See in 1897.[17]
References
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