Skip to content
Kepler-9 b

Comparing TRAPPIST-1 to the Solar System · NASA · NASA — public domain

EntityQ47519· pop 16· linked from 128 articles

Kepler-9 b

Sign in to save

__NOTOC__

Astronomical data · SIMBAD

Object type
Pl
Distance
2,061 light-years
Coordinates
RA 285.5740° · Dec 38.4009°
View on SIMBAD →

via SIMBAD · CDS Strasbourg

Key facts

Planet.name
Kepler-9b
Planet.image
Exoplanet Comparison Kepler-9 b.png
Planet.caption
Size comparison of Kepler-9b (left) with Jupiter (right)
Planet.discoverer
Kepler Mission team
Planet.discovery_site
Kepler space telescope
Planet.discovered
26 August 2010
Planet.discovery_method
Transit
Planet.apsis
astron
Planet.eccentricity
0
Planet.period
19.24 d
Planet.inclination
88.55
Planet.star
Kepler-9
Planet.mean_radius
0.842 ± 0.069
Planet.density
g cm−3

via Wikipedia infobox

Exoplanet data

Host star
Kepler-9
Discovered
2010
Discovered by
Kepler
Orbital period
19.24 days
Radius
8.29 × Earth
Mass
43.40 × Earth
Equilibrium temp
661 K
Distance
628.26 pc

via NASA Exoplanet Archive

Wikidata facts

Diameter
114000
Radius
0.74
Mass
0.13655
Orbital period
19.23891
Image
Kepler-9b, Jupiter size comparison.jpg
Show 13 more facts
catalog code
Kepler-9b
semi-major axis of an orbit
0.143
time of discovery or invention
2010-10-00
Commons category
Kepler-9 b
right ascension
285.57397671045170
declination
38.40088256864889
argument of periapsis
357
orbital eccentricity
0
orbital inclination
88.982
right ascension component of proper motion
2.491
declination component of proper motion
-14.713
parallax
1.5629
M sin i
0.08149941185
Sources (1)

via Wikidata · CC0

~3 min read

Article

5 sections
Contents
  • Nomenclature and history
  • Characteristics
  • Other planets in the Kepler-9 system
  • References
  • External links

__NOTOC__

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.

Gallery (2)

Connections

Categories