Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Serpens |
Right ascension | 15h 48m 44.37720s[1] |
Declination | +18° 08′ 29.6337″[1] |
Apparent magnitude (V) | 4.09[2] |
Characteristics | |
Spectral type | M0.5III[3] |
U−B color index | +1.95[2] |
B−V color index | +1.62[2] |
Astrometry | |
Radial velocity (Rv) | −38.48[4] km/s |
Proper motion (μ) | RA: −52.407 mas/yr[1] Dec.: −88.419 mas/yr[1] |
Parallax (π) | 8.5231 ± 0.1657 mas[1] |
Distance | 383 ± 7 ly (117 ± 2 pc) |
Absolute magnitude (MV) | −1.25[5] |
Details | |
Radius | 71.31+1.42 −1.48[6] R☉ |
Luminosity | 1,021±57[6] L☉ |
Temperature | 3,863±39[6] K |
Other designations | |
Database references | |
SIMBAD | data |
Kappa Serpentis, Latinised from κ Serpentis, is a single,[8] red-hued star in the constellation Serpens, in its head (Serpens Caput). It has the proper name Gudja /ˈɡuːdʒə/[9] and the Flamsteed designation 35 Serpentis.[7] This star is visible to the naked eye with an apparent visual magnitude of +4.09.[2] It is located approximately 383 light years from the Sun, based on parallax,[1] and is drifting closer with a radial velocity of −38 km/s.[4]
This object is an aging red giant star with a stellar classification of M0.5III.[3] After exhausting the supply of hydrogen at its core, the star cooled and expanded off the main sequence, and now has around 71 times the Sun's radius. It is radiating nearly 1,000 times the luminosity of the Sun from its photosphere at an effective temperature of 3,863 K.[6] This is a suspected variable star.[10]
DR3
was invoked but never defined (see the help page).Ducati2002
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was invoked but never defined (see the help page).Eggleton2008
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was invoked but never defined (see the help page).Samus2017
was invoked but never defined (see the help page).