Kepler-90h
Exoplanet | List of exoplanets | |
---|---|---|
| ||
Parent star | ||
Star | Kepler-90 | |
Constellation | Draco | |
Right ascension | (α) | 18h 57m 44.04s |
Declination | (δ) | +49° 18′ 18.6″ |
Apparent magnitude | (mV) | 14[1] |
Distance | 2500 ly (765 pc) | |
Spectral type | G or F | |
Mass | (m) | 1.13[1] M☉ |
Radius | (r) | 1.14[1] R☉ |
Temperature | (T) | 5930 ± 320[1] K |
Orbital elements | ||
Semi-major axis | (a) | 1.01 ± 0.11[1] AU |
Eccentricity | (e) | 0.0 ≤ 0.001[1] |
Orbital period | (P) | 331.60059 ± 0.00037[1] d |
Inclination | (i) | 89.6 ± 1.3[2]° |
Physical characteristics | ||
Mass | (m) | ≤ 5.0[1] MJ |
Radius | (r) | 1.008 ± 0.089[1] RJ |
Temperature | (T) | 292[2]K |
Discovery information | ||
Discovery date | November 12, 2013[1] | |
Discoverer(s) | Kepler Science Team | |
Discovery method | Transit[2] | |
Discovery site | Kepler telescope | |
Discovery status | Published | |
Other designations | ||
KOI-351.01[3] | ||
Database references | ||
Extrasolar Planets Encyclopaedia | data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
Kepler-90h is a planet orbiting Kepler-90 in the constellation Draco.
Characteristics
Kepler-90h is a gas giant with a radius that is 1.008 times that of Jupiter.[1] With an equilibrium temperature of 292 K (19°C), it is near the inner edge of the habitable zone. It is orbiting the late-F or early-G-type star Kepler-90.
References
- 1 2 3 4 5 6 7 8 9 10 11 "TEPcat: Kepler-90h". www.astro.keele.ac.uk. December 31, 2013. Retrieved January 3, 2013.
- 1 2 3 "Planet Kepler-90 h". exoplanet.eu. Retrieved January 3, 2014.
- ↑ Schmitt, Joseph R.; Wang, Ji; Fischer, Debra A.; Jek, Kian J.; Moriarty, John C.; Boyajian, Tabetha S.; Schwamb, Megan E.; Lintott, Chris; Smith, Arfon M.; Parrish, Michael; Schawinski, Kevin; Lynn, Stuart; Simpson, Robert; Omohundro, Mark; Winarski, Troy; Goodman, Samuel J.; Jebson, Tony; Lacourse, Daryll (2013). "Planet Hunters VI: The First Kepler Seven Planet Candidate System and 13 Other Planet Candidates from the Kepler Archival Data", Astrophysical Journal, p. 23.
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