HD 203949

HD 203949 is a K-type giant star 257 light-years away in the constellation of Microscopium. Its surface temperature is 4618±113 K. It is either on the red giant branch fusing hydrogen in a shell around a helium core, or more likely a red clump star currently fusing helium in its core. HD 203949 is enriched in heavy elements relative to the Sun, with a metallicity ([Fe/H]) of 0.17±0.07 dex. As is common for red giants, HD 203949 has an enhanced concentration of sodium and aluminium compared to iron.

HD 203949
Observation data
Epoch J2000      Equinox J2000
Constellation Microscopium
Right ascension 21h 26m 22.8745s
Declination −37° 49 45.950
Apparent magnitude (V) 5.62±0.01
Characteristics
Evolutionary stage giant
Spectral type K2III
Astrometry
Radial velocity (Rv)−83.50±0.16 km/s
Proper motion (μ) RA: 168.257 mas/yr
Dec.: −11.075 mas/yr
Parallax (π)12.6806 ± 0.0577 mas
Distance257 ± 1 ly
(78.9 ± 0.4 pc)
Absolute magnitude (MV)+1.10
Details
Mass1.00±0.16 M
Radius10.30±0.51 R
Luminosity (bolometric)43.34±4.27 L
Surface gravity (log g)2.415±0.044 cgs
Temperature4618±113 K
Metallicity [Fe/H]0.17±0.07 dex
Age7.29±3.06 Gyr
Other designations
CD−38 14551, Gaia DR2 6583094222249556224, HIP 105854, HR 8200, TYC 7979-47-1, GSC 07979-00047, 2MASS J21262286-3749458
Database references
SIMBADdata

Multiplicity surveys did not find any stellar companions around HD 203949 as of 2019.

This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.