Kepler-251d
extrasolar planet
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Kepler-251d
Summary
Kepler-251d is an exoplanet[1].
Key Facts
- Kepler-251d is credited with the discovery of Kepler Space Telescope[2].
- Kepler-251d's instance of is recorded as exoplanet[3].
- Kepler-251d's constellation is recorded as Cygnus[4].
- Kepler-251d's parent astronomical body is recorded as Q86844097[5].
- Kepler-251d's catalog code is recorded as Kepler-251d[6].
- Kepler-251d's catalog code is recorded as KOI-907.02[7].
- Kepler-251d's catalog code is recorded as KOI-907d[8].
- Kepler-251d's catalog code is recorded as TIC 272489533d[9].
- Kepler-251d's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-251d's discovery method is recorded as transit method[11].
- Kepler-251d's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+3.003'}[12].
- Kepler-251d's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+30.1328857684'}[13].
- Kepler-251d's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0538'}[14].
- Kepler-251d's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.182'}[15].
- Kepler-251d's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+48000'}[16].
- Kepler-251d's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+296.56623619141874'}[17].
- Kepler-251d's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.10586628196945'}[18].
- Kepler-251d's epoch is recorded as J2000.0[19].
- Kepler-251d's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-13.601'}[20].
- Kepler-251d's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.181'}[21].
Body
Definition and Type
Kepler-251d's instance of is recorded as exoplanet[3].