HD 44219

HD 44219 is an 8th magnitude G-type main sequence star located approximately 164 light years away in the constellation Monoceros. This star is larger, cooler, brighter, and about the same mass as our Sun. Also its metal content is one-fifteenth more than the Sun. In 2009, a gas giant planet was found in orbit around the star.[3]

The HD 44219 planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.58+0.06
−0.04
 MJ
1.19±0.02 472.3+6.3
−5.0
0.61+0.07
−0.09
HD 44219
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Monoceros
Right ascension 06h 20m 14.32s[1]
Declination –10° 43 30.0[1]
Apparent magnitude (V) 7.705
Characteristics
Spectral type G5
Apparent magnitude (B) 8.345
Apparent magnitude (J) 6.509
Apparent magnitude (H) 6.215
Apparent magnitude (K) 6.115
B−V color index 0.640
Astrometry
Radial velocity (Rv)–12.4 km/s
Proper motion (μ) RA: 73.05±0.84[1] mas/yr
Dec.: −17.95±0.66[1] mas/yr
Parallax (π)19.83 ± 0.78[1] mas
Distance164 ± 6 ly
(50 ± 2 pc)
Absolute magnitude (MV)4.192
Details
Mass1.01 ± 0.01[2] M
Radius1.37 ± 0.03[2] R
Luminosity1.83 ± 0.01[2] L
Surface gravity (log g)4.17 ± 0.02[2] cgs
Temperature5749 ± 45[2] K
Metallicity [Fe/H]0.03 dex
Age9.6 ± 0.7[2] Gyr
Other designations
BD–10°1479, HIP 30114, PPM 217031, SAO 151367
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia
data

See also

  • List of extrasolar planets

References


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