Kepler-87
Kepler-87 is a star slightly more massive than the Sun and it is nearing the end of its main-sequence period.[1]
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Cygnus |
| Right ascension | 19h 51m 40.04s |
| Declination | +46° 57′ 54.41″ |
| Apparent magnitude (V) | 15 |
| Characteristics | |
| Spectral type | G4IV |
| Variable type | planetary transit |
| Astrometry | |
| Proper motion (μ) | RA: -4.43279 ±0.0341821 mas/yr Dec.: -0.932606 ±0.0402233 mas/yr |
| Parallax (π) | 0.782544 ± 0.0176347 mas |
| Details | |
| Mass | 1.01 M☉ |
| Radius | 1.49669 R☉ |
| Luminosity | 0.3260445 L☉ |
| Temperature | 5692 ± 60.7121 K |
| Metallicity [Fe/H] | 0.0562149±0.0587866 dex |
| Age | 7.24+1.50 −1.56 years |
| Other designations | |
Planetary system
Kepler-87 hosts four planets, two confirmed (Kepler-87b,[2] Kepler-87c[3] and two unconfirmed (Kepler-87d, Kepler-87e). It is the farthest system from the Sun with two unconfirmed planet candidates at 4021 light-years.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | 1.02+0.16 −0.16 MJ |
0.481+0.026 −0.028 |
114.73635+0.00015 −0.00015 |
0.036±0.009 | — | — |
| c | 0.02+0.003 −0.003 MJ |
0.676+0.037 −0.04 |
191.2318+0.0015 −0.0015 |
0.039±0.012 | — | — |
| d (unconfirmed) | — | 0.0628 | 5.83393857±2.241 | 0 | — | — |
| e (unconfirmed) | — | 0.0836 | 8.9772888±0.0001451 | 0 | — | — |
References
- "Kepler-87 | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 10 September 2023.
- "The Extrasolar Planet Encyclopaedia — Kepler-87b". exoplanet.eu. Retrieved 10 September 2023.
- "The Extrasolar Planet Encyclopaedia — Kepler-87c". exoplanet.eu. Retrieved 10 September 2023.
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