HD 240210

HD 240210
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cassiopeia
Right ascension 23h 10m 29.22633s
Declination +57° 01 46.0277
Apparent magnitude (V) 8.33
Characteristics
Evolutionary stage giant
Spectral type K3III
B−V color index 1.63
Astrometry
Radial velocity (Rv)+8.57±0.05 km/s
Proper motion (μ) RA: 18.492 mas/yr
Dec.: 6.883 mas/yr
Parallax (π)2.6570±0.0349 mas
Distance1,230 ± 20 ly
(376 ± 5 pc)
Absolute bolometric
magnitude
 (Mbol)
+0.38
Details
Mass1.25±0.25 M
Radius25.46+1.16
−0.75
 R
Luminosity152±3 L
Surface gravity (log g)2.31±0.11 cgs
Temperature4,019+60
−90
 K
Metallicity [Fe/H]−0.18±0.12 dex
Rotation> 654 days
Rotational velocity (v sin i)< 1.0 km/s
Age3.0+2.9
−1.5
 Gyr
Other designations
BD+56°2959, HD 240210, SAO 35195, PPM 41549
Database references
SIMBADdata
Exoplanet Archivedata

HD 240210 is a star in the northern constellation of Cassiopeia. It has an orange hue but is too faint to be viewed with the naked eye, having an apparent visual magnitude of 8.33. Parallax measurements provide an estimate of its distance from the Sun as approximately 1,230 light years. It is drifting further away with a radial velocity of +8.6 km/s.

This is an aging giant star with a class of K3, which has exhausted the supply of hydrogen at its core and expanded to 25 times the radius of the Sun. It is around three billion years old with 1.3 times the Sun's mass. The star is radiating 152 times the luminosity of the Sun from its enlarged photosphere at an effective temperature of 4,019 K. It is spinning slowly, with each rotation taking at least 1.8 years.

On June 10, 2009 a planet orbiting the star was discovered by Niedzielski et al. This exoplanet is a 6.9 or greater Jupiter mass planet. Evidence for additional planetary companions has been found.

The HD 240210 planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b  6.90 MJ 1.33 501.75±2.33 0.15±0.02