Kepler-249b
extrasolar planet
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Kepler-249b
Summary
Kepler-249b is an exoplanet[1].
Key Facts
- Kepler-249b is credited with the discovery of Kepler Space Telescope[2].
- Kepler-249b's instance of is recorded as exoplanet[3].
- Kepler-249b's constellation is recorded as Cygnus[4].
- Kepler-249b's parent astronomical body is recorded as Q86844259[5].
- Kepler-249b's catalog code is recorded as Kepler-249b[6].
- Kepler-249b's catalog code is recorded as KOI-899.02[7].
- Kepler-249b's catalog code is recorded as KOI-899b[8].
- Kepler-249b's catalog code is recorded as TIC 272942100b[9].
- Kepler-249b's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-249b's discovery method is recorded as transit method[11].
- Kepler-249b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+1.134'}[12].
- Kepler-249b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+3.3065702702'}[13].
- Kepler-249b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.2235'}[14].
- Kepler-249b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.035'}[15].
- Kepler-249b's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+13300'}[16].
- Kepler-249b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+296.98510064975335'}[17].
- Kepler-249b's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.65852884469389'}[18].
- Kepler-249b's epoch is recorded as J2000.0[19].
- Kepler-249b's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+17.518'}[20].
- Kepler-249b's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+33.524'}[21].
Body
Definition and Type
Kepler-249b's instance of is recorded as exoplanet[3].