Kepler-32b
Template:Expansion needed
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | Kepler-32 | |
Constellation | Cygnus | |
Right ascension | (α) | 19h 51m 22.18s |
Declination | (δ) | +46° 34′ 27.41″ |
Apparent magnitude | (mV) | 15.801 |
Mass | (m) | 0.54 M☉ |
Radius | (r) | 0.53 R☉ |
Temperature | (T) | 3793 K |
Metallicity | [Fe/H] | -0.01 |
Physical characteristics | ||
Radius | (r) | 2.2 R⊕ |
Temperature | (T) | 569 |
Orbital elements | ||
Semi-major axis | (a) | 0.0519 AU |
Orbital period | (P) | 5.9012 d |
Inclination | (i) | 87.660° |
Discovery information | ||
Discovery date | 2013 | |
Discoverer(s) | ||
Discovery method | Transit (Kepler Mission) | |
Other detection methods | Transit timing variations | |
Discovery status | Published refereed article | |
Other designations | ||
952.01
|
Kepler-32b (alt. name KOI 952.01) is an extrasolar planet in orbit around its M-dwarf-type star in the Kepler-32 system, constellation of Cygnus.[1] Discovered by planetary transit methods with the Kepler space telescope in January 2012, it presents a semi-major axis of 0.0519 AU and temperature of 559.9 K. 2.2 Earth-radius, a mass of 4.1 MJ, and an orbital period of 5.9012 days.[1][2]
See also
References
- 1 2 Swift, Jonathan J. (2012). "Characterizing the Cool KOIs IV: Kepler-32 as a prototype for the formation of compact planetary systems throughout the Galaxy". The Astrophysical Journal. 764: 105. arXiv:1301.0023. Bibcode:2013ApJ...764..105S. doi:10.1088/0004-637X/764/1/105.
- ↑ Fabrycky, Dan (2 Feb 2012). "Kepler-32b". NASA. Retrieved 2 Mar 2013.
This article is issued from Wikipedia - version of the 11/9/2016. The text is available under the Creative Commons Attribution/Share Alike but additional terms may apply for the media files.