Kepler-9 b

Kepler-9 b Image

Description: Kepler-9b is one of the first planets discovered outside the solar system (exoplanets) by NASA's Kepler Mission. It revolves around the star Kepler-9 within the constellation Lyra. Kepler-9b is the largest of three planets detected in the Kepler system by transit method; its mass is roughly half that of the planet Saturn, and it is the largest planet in its system. Kepler-9b and Kepler-9c display a phenomenon called orbital resonance, in which gravitational pull from each planet alters and stabilizes the orbit of the other. The planet's discovery was announced on August 26, 2010.

Physical Properties

Mass (Jupiter mass): 0.136550986376365 MJ

Radius (Jupiter radius): 0.74 RJ

Density: 0.42 g/cm³

Equilibrium Temperature: 661.0 K

Orbital Parameters

Orbital Period: 19.23891 days

Semi-major Axis: 0.143 AU

Eccentricity: 0.0609

Inclination: 88.982°

Host Star Properties

Host Star: Kepler-9

Spectral Type: Unknown

Temperature: 5774.0 K

Stellar Mass: 1.02 M

Stellar Radius: 0.96 R

Discovery Information

Planet Letter: b

Object ID: 3.388

Host ID: 2.425688

Discovery Date: 2010-10

Discovery Year: 2010

Discovery Method: Transit

Discovery Locale: Space

Discovery Facility: Kepler

Discovery Instrument: Kepler CCD Array

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