HR 3082

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Template:Short description

HR 3082
Observation data
Epoch J2000      Equinox J2000
Constellation Camelopardalis[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 5.39[1]
Characteristics
Evolutionary stage main sequence[2]
Spectral type A0p Si[3] or B9.5 IVs[4]
B−V Template:Engvar Script error: No such module "val".[1]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[5] km/s
Proper motion (μ) RA: Script error: No such module "val". mas/yr[2]
Dec.: Script error: No such module "val". mas/yr[2]
Parallax (π)9.5700±0.0876 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Script error: No such module "val".[6]
Details
MassScript error: No such module "val".[6] Template:Solar mass
Radius2.89[7] Template:Solar radius
LuminosityScript error: No such module "val".[6] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val".[8] cgs
TemperatureScript error: No such module "val".[8] K
Rotational velocity (v sin i)30[8] km/s
Age36[8] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[9]
Database references
SIMBADdata

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HR 3082 is a double star in the northern circumpolar constellation of Camelopardalis. It is faintly visible to the naked eye with an apparent visual magnitude of 5.39.[1] The system is moving closer to the Sun with a heliocentric radial velocity of +2.7 km/s.[5] It is currently at a distance of around 341 light years, based upon an annual parallax shift of Script error: No such module "val"..[2]

The brighter component is a magnetic,[7] mild Ap star that displays an overabundance of silicon in its spectrum.[10] Cowley et al. (1969) listed a stellar classification of A0p Si,[3] while Abt and Morrell (1995) have it pegged as a subgiant star with a class of B9.5 IVs.[4] It has an estimated 2.65[6] times the mass of the Sun and 2.89[7] times the Sun's radius. The star is radiating 74[6] times the Sun's luminosity from its photosphere at an effective temperature of 10,795 K.[8]

The fainter component is a magnitude 9.6 star at an angular separation of Script error: No such module "val". along a position angle (PA) of 84°, as of 2009.[11] This is most likely a visual companion located along the same line of sight.[12] There is a magnitude 13.6 visual companion at a separation of Script error: No such module "val". along a PA of 169°, as of 2016.[11]

References

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  1. a b c d Template:Cite XHIP
  2. a b c d e f Template:Cite Gaia DR3
  3. a b Script error: No such module "citation/CS1".
  4. a b Script error: No such module "citation/CS1".
  5. a b Script error: No such module "citation/CS1".
  6. a b c d e Script error: No such module "citation/CS1".
  7. a b c Script error: No such module "citation/CS1".
  8. a b c d e Script error: No such module "citation/CS1".
  9. Template:Cite simbad
  10. Script error: No such module "citation/CS1".
  11. a b Script error: No such module "citation/CS1".
  12. Script error: No such module "citation/CS1".

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Template:Stars of Camelopardalis