Kepler 32c

Kepler-32 c is a Confirmed extrasolar planet exoplanet that orbits the star Kepler 32 in the constellation of Cygnus

Kepler-32c alt. name KOI 952.02 is an extrasolar planet in orbit around its M-dwarf-type star in the Kepler-32 system, in the constellation of Cygnus.1 Discovered by planetary transit methods with the Kepler space telescope in January 2012, it presents a semi-major axis of 0.033 AU and temperature of 417.3 K. It has a radius of 2.2 Earth-radius and an orbital period of 8.7522 days.amp912amp93

Kepler-32 c is a Neptune-like exoplanet that orbits a K-type star. Its mass is 0.5 Jupiters, it takes 8.8 days to complete one orbit of its star, and is 0.09 AU from its star. Its discovery was announced in 2011.

Kepler-32c alt. name KOI 952.02 is an extrasolar planet in orbit around its M-dwarf-type star in the Kepler-32 system, in the constellation of Cygnus. 1 Discovered by planetary transit methods with the Kepler space telescope in January 2012, it presents a semi-major axis of 0.033 AU and temperature of 417.3 K.

Exoplanet Kepler-32 c Exoplanet Kepler-32 c orbits star Kepler-32 that lies 1053 light years away from the Sun. It has about 250px of Earth radius and orbits its star much closer than Earth orbits Sun.

Related publications There might be giants unseen Jupiter-mass planets as sculptors of tightly-packed planetary systems 2016 HANDS T. amp ALEXANDER R. MNRAS , 456 , 4121 paper arxiv ADS. Gravitational quantization of exoplanet orbits in HD 10180, Kepler-32, Kepler-33, Kepler-102, and Kepler-186

Kepler-32c -- Extra-solar Confirmed Planet The astronomical object called Kepler-32c is a Extra-solar Confirmed Planet Origin of the objects types Ref Object type as listed in the reference quotRefquot acronym Object type linked to the acronym according to the original reference Anterior to 2007, before we can link the objet type to a

Kepler-32c does not have an entry in the catalogue of orbital obliquity measurements. Page generated on 20250324 John Southworth Keele University, UK

Kepler-32 c Kepler-32 c Kepler-32 c Kepler-32 c Exoplanet Archive Disposition CONFIRMED CONFIRMED CONFIRMED CONFIRMED CONFIRMED CONFIRMED CONFIRMED Vetting Status Done Done Done Done Done Done Done Date of Last Parameter Update 2018-08-16 2017-08-31 2015-09-24 2014-12-18 2014-12-04 2014-01-07 2013-02-12 Disposition Using Kepler Data CANDIDATE

The centroids during transit for Kepler-32b and Kepler-32c differ from those out-of-transit by only 2, roughly consistent with measurement uncertainties. The 3 radii of confusion Rc are 0 5 for Kepler-32b and 0 8 for Kepler-32c. For KOI-952.03, .04, and .05, the transits are too shallow for a constraining centroid analysis.