Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Volans |
Right ascension | 07h 05m 36.2081s[2] |
Declination | −73° 00′ 52.0345″[2] |
Apparent magnitude (V) | 8.78 - 11.50[3] |
Characteristics | |
Evolutionary stage | AGB[4] |
Spectral type | Ce[5] |
Variable type | Mira[6] |
Astrometry | |
Radial velocity (Rv) | −4.7[7] km/s |
Proper motion (μ) | RA: −14.298 mas/yr[2] Dec.: +19.462 mas/yr[2] |
Parallax (π) | 1.3931 ± 0.0631 mas[2] |
Distance | 2,317+97 −96 ly (710.7+29.9 −29.5 pc)[8] |
Details | |
Mass | 0.75[9] M☉ |
Radius | 687[10][a] R☉ |
Luminosity | 6,800[10] L☉ |
Temperature | 2,000[10] K |
Other designations | |
Database references | |
SIMBAD | data |
R Volantis is a single variable star in the southern circumpolar constellation Volans. It has an average apparent magnitude of 8.7,[11] making it readily visible in amateur telescopes but not to the naked eye. The object is relatively far at a distance of about 2,300 light years but is drifting closer with a radial velocity of −5 km/s.
R Volantis' peculiarity was first observed in 1954 when it was found to have emission lines in its spectrum.[12] Observations from 1955 to 1967 reveal that the star was a probable Mira variable[13] and was given its current designation. However, its nature as a carbon star wasn't discovered until 1968 by Pik-Sin The. In the paper, R Volantis and V1163 Centauri (HD 114586) had their spectrums studied and revealed that the former is a carbon star while the latter is an S-type star.[14]
R Volantis has a stellar classification of Ce,[5] indicating that it is a carbon star with emission lines. It is a giant star on the asymptotic giant branch,[4] meaning that it is generating energy via hydrogen and helium shells around an inert carbon core. As a result, it has expanded to 687 times the radius of the Sun and now radiates a luminosity of 6800 L☉.[10] R Vol has an effective temperature of 2,000 K, giving a deep red hue.[10]
It fluctuates between magnitude 8.7 and 15.4 and has a period of 445 days.[3]
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