Gamma Monocerotis

Star in the constellation of Monoceros From Wikipedia, the free encyclopedia

γ Monocerotis, Latinised as Gamma Monocerotis, is a binary star[9] system in the equatorial constellation of Monoceros. Based upon an annual parallax shift of 6.55 mas,[1] it is located roughly 500 light years from the Sun. It can be viewed with the naked eye, having an apparent visual magnitude of 3.96.[2] Gamma Monocerotis is moving away from the Sun with a radial velocity of −5 km/s.[4]

Right ascension06h 14m 51.33367s[1]
Declination06° 16 29.1880[1]
Quick facts Constellation, Right ascension ...
γ Monocerotis
Location of γ Monocerotis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Monoceros
Right ascension 06h 14m 51.33367s[1]
Declination 06° 16 29.1880[1]
Apparent magnitude (V) 3.96[2]
Characteristics
Spectral type K1.5IIIBa0.3[3]
U−B color index +1.42[2]
B−V color index +1.31[2]
Astrometry
Radial velocity (Rv)−4.8±0.7[4] km/s
Proper motion (μ) RA: 4.69[1] mas/yr
Dec.: 19.30[1] mas/yr
Parallax (π)6.55±0.19 mas[1]
Distance500 ± 10 ly
(153 ± 4 pc)
Absolute magnitude (MV)-1.93[5]
Details[6]
Mass4.09±0.14 M
Radius50.8+1.5
−1.6
 R
Luminosity1,247±96 L
Surface gravity (log g)1.61[7] cgs
Temperature4,810±66 K
Metallicity [Fe/H]−0.15[7] dex
Rotational velocity (v sin i)4.0[8] km/s
Age170±20 Myr
Other designations
γ Mon, 5 Monocerotis, BD−06°1469, FK5 2475, GC 7986, HD 43232, HIP 29651, HR 2227, SAO 133012, CCDM J06149-0616A, WDS J06149-0617A
Database references
SIMBADdata
Close

This is an evolved K-type giant star with a stellar classification of K1.5 III Ba0.3.[3] The Ba0.3 suffix indicates this is a mild barium star, which means the spectrum displays abnormal abundance of s-process elements, including barium. These were deposited by an orbiting companion as it passed through the asymptotic giant branch stage. The companion is now a white dwarf star.[10]

It has reported companions B, at separation 53.7" and magnitude 13.1, and C, at separation 47.9" and magnitude 13.6.[11]

References

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