HD 32518

HD 32518
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Camelopardalis
Right ascension 05h 09m 36.72s[1]
Declination +69° 38 21.9[1]
Apparent magnitude (V) 6.436
Characteristics
Spectral type K1III
Apparent magnitude (B) 7.537
Apparent magnitude (J) 4.531
Apparent magnitude (H) 3.992
Apparent magnitude (K) 3.911
B−V color index 1.101
Astrometry
Radial velocity (Rv)–7.02 km/s
Proper motion (μ) RA: 60.26 ± 0.28[1] mas/yr
Dec.: -62.81 ± 0.52[1] mas/yr
Parallax (π)8.29 ± 0.58[1] mas
Distance390 ± 30 ly
(121 ± 8 pc)
Absolute magnitude (MV)1.09
Details
Mass1.2 ± 0.1[2] M
Radius10.8 ± 0.3[2] R
Luminosity46.4 ± 0.9[2] L
Surface gravity (log g)2.4 ± 0.1[2] cgs
Temperature4599 ± 41[2] K
Metallicity [Fe/H]−0.15 ± 0.04 dex
Age6.4 ± 1.5[2] Gyr
Other designations
BD+69°302, GC 6245, GCRV 3027, HIP 24003, HR 1636, PPM 15168, SAO 13382
Database references
SIMBADdata
Exoplanet Archivedata
Extrasolar Planets
Encyclopaedia
data

HD 32518 is a 6th magnitude K-type giant star located approximately 390 light years away in the constellation of Camelopardalis. It is 1.13 times more massive, 10.22 times larger, and 41.2 times more luminous than the Sun. However, it has a lower amount of metals than our Sun and the age is older. In August 2009, it was found that this giant star has a giant planet.[3]

The HD 32518 planetary system[3]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥3.04 ± 0.69 MJ 0.59 ± 0.03 157.54 ± 0.38 0.01 ± 0.03

See also

References

Coordinates: 05h 09m 36.7193s, +69° 38′ 21.844″


This article is issued from Wikipedia - version of the 11/17/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.