Kepler-250d
extrasolar planet
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Kepler-250d
Summary
Kepler-250d is an exoplanet[1].
Key Facts
- Kepler-250d is credited with the discovery of Kepler Space Telescope[2].
- Kepler-250d's instance of is recorded as exoplanet[3].
- Kepler-250d's constellation is recorded as Cygnus[4].
- Kepler-250d's parent astronomical body is recorded as Q86843941[5].
- Kepler-250d's catalog code is recorded as KOI-906.02[6].
- Kepler-250d's catalog code is recorded as Kepler-250d[7].
- Kepler-250d's catalog code is recorded as KOI-906d[8].
- Kepler-250d's catalog code is recorded as TIC 159098652d[9].
- Kepler-250d's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-250d's discovery method is recorded as transit method[11].
- Kepler-250d's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+2.205'}[12].
- Kepler-250d's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+17.6482492968'}[13].
- Kepler-250d's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2865'}[14].
- Kepler-250d's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.127'}[15].
- Kepler-250d's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+33900'}[16].
- Kepler-250d's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+289.59475989414500'}[17].
- Kepler-250d's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+44.14193397865417'}[18].
- Kepler-250d's epoch is recorded as J2000.0[19].
- Kepler-250d's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-28.478'}[20].
- Kepler-250d's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.570'}[21].
Body
Definition and Type
Kepler-250d's instance of is recorded as exoplanet[3].