Delta Monocerotis

Delta Monocerotis
Location of δ Monocerotis (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Monoceros
Right ascension 07h 11m 51.860s
Declination −00° 29 33.96
Apparent magnitude (V) 4.15
Characteristics
Spectral type A2V or A0IV
U−B color index +0.04
B−V color index +0.00
Astrometry
Radial velocity (Rv)+15.0±4.1 km/s
Proper motion (μ) RA: +0.79 mas/yr
Dec.: +4.52 mas/yr
Parallax (π)8.49±0.17 mas
Distance384 ± 8 ly
(118 ± 2 pc)
Absolute magnitude (MV)−1.20
Details
Mass2.4+0.43
−0.38
 M
Luminosity350 L
Surface gravity (log g)3.5±0.25 cgs
Temperature9,462 K
Metallicity [Fe/H]0.00 dex
Rotational velocity (v sin i)175.5±1.3 km/s
Age405+135
−207
 Myr
Other designations
δ Mon, 22 Monocerotis, BD−00°1636, FK5 1187, GC 9518, HD 55185, HIP 34769, HR 2714, SAO 134330, CCDM J07119-0030A, WDS J07119-0030A
Database references
SIMBADdata

Delta Monocerotis, which is Latinized from δ Monocerotis, is a single star in the constellation of Monoceros, positioned about a half degree south of the celestial equator. It has a white hue and is faintly visible to the naked eye with an apparent visual magnitude of 4.15. The distance to this star is approximately 384 light years based on parallax. It is drifting further away from the Sun with a radial velocity of about +15 km/s, having come to within 88 light-years some 7.3 million years ago. The star has an absolute magnitude of −1.20.

The Bright Star Catalogue assigns this star a stellar classification of A2V, suggesting this is an A-type main-sequence star. However, Houk and Swift (1999) found a more evolved subgiant class of A0IV. It has around 2.4 times the mass of the Sun and is an estimated 405 million years old. The star has a high rate of spin with a projected rotational velocity of 175.5 km/s, giving it an equatorial bulge that is 5% larger than the polar radius. It is radiating 350 times the luminosity of the Sun from its photosphere at an effective temperature of 9,462 K.

It has one reported visual companion, designated component B, at an angular separation of 32.0 and visual magnitude 13.0.