K2-288 is a binary star system consisting of two red dwarfs. The companion star, K2-288B, is known to host a single planet, K2-288Bb.

K2-288
Observation data
Epoch J2000      Equinox J2000
Constellation Taurus
Right ascension 03h 41m 46.43s[1]
Declination +18° 16′ 08.0″[1]
Characteristics
Spectral type M2 V[1] + M3 V[1]
Orbit[1]
PrimaryK2-288 A
CompanionK2-288 B
Semi-major axis (a)55 AU
Details[1]
K2-288 A
Mass0.52±0.02 M
Radius0.45±0.03 R
Surface gravity (log g)4.85±0.03 cgs
Temperature3584±205 K
Metallicity [Fe/H]−0.29±0.09 dex
K2-288 B
Mass0.33±0.02 M
Radius0.32±0.03 R
Surface gravity (log g)4.96±0.02 cgs
Temperature3341±276 K
Metallicity [Fe/H]−0.21±0.09 dex
Database references
SIMBADdata

Planetary System

edit

In January 2019, it was announced that a team of citizen scientists had discovered a planet in orbit of K2-288B.[1]

The K2-288 planetary system[1]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b .164 ± 0.03 31.393463+0.000067
−0.000069
89.81+0.13
−0.17
°
1.90 ± 0.3 R🜨


See also

edit

Kepler 296, similar red dwarf binary with exoplanets

References

edit
  1. ^ a b c d e f g h Feinstein, Adina D.; et al. (7 January 2019). "K2-288Bb: A Small Temperate Planet in a Low-mass Binary System Discovered by Citizen Scientists" (PDF). The Astronomical Journal. 157 (2): 40. arXiv:1902.02789. Bibcode:2019AJ....157...40F. doi:10.3847/1538-3881/aafa70. hdl:1721.1/121222.