HD 24040

Source: Wikipedia, the free encyclopedia.
HD 24040
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Taurus
Right ascension 03h 50m 22.9678s[1]
Declination +17° 28′ 34.9254″[1]
Apparent magnitude (V) 7.50[2]
Characteristics
Evolutionary stage Main sequence
Spectral type G2V[3]
B−V color index 0.653±0.003[2]
Distance
151.9 ± 0.2 ly
(46.57 ± 0.05 pc)
Absolute magnitude (MV)4.16[2]
Details
Gyr
NLTT 11955[6]
Database references
SIMBADdata

HD 24040 is a

light years. However, it is drifting closer to the Sun with a radial velocity of −9.4 km/s.[2]

This is a

Planetary system

A long period planet was discovered in 2006 based on observations made at the W. M. Keck Observatory in Hawaii. However because the observations covered less than one complete orbit there were only weak constraints on the period and mass.[5] The first reliable orbit for HD 24040b was obtained by astronomers at Haute-Provence Observatory in 2012 who combined the keck measurements with ones from the SOPHIE and ELODIE spectrographs.[7] The most recent orbit published in 2015 added additional keck measurements and refined the orbital parameters.[8]

A linear trend in the

HD 24040 c.[9]

Planet c is in the

habitable zone, with an ecc of <0.2, and may have a habitable moon
.

The HD 24040 planetary system[8][9]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
c
≥0.201±0.027 MJ 1.3±0.021 515.4+2.2
−2.5
0.11+0.120
−0.079
b >4.10±0.12 MJ 4.637±0.067 3490±25 0.047±0.020

See also

References

External links