Kepler-356b
extrasolar planet
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Kepler-356b
Summary
Kepler-356b is an exoplanet[1].
Key Facts
- Kepler-356b is credited with the discovery of Kepler Space Telescope[2].
- Kepler-356b's instance of is recorded as exoplanet[3].
- Kepler-356b's constellation is recorded as Cygnus[4].
- Kepler-356b's parent astronomical body is recorded as Q86174952[5].
- Kepler-356b's catalog code is recorded as Kepler-356b[6].
- Kepler-356b's catalog code is recorded as KOI-2053.02[7].
- Kepler-356b's catalog code is recorded as KOI-2053b[8].
- Kepler-356b's catalog code is recorded as TIC 137636895b[9].
- Kepler-356b's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-356b's discovery method is recorded as transit method[11].
- Kepler-356b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+1.803'}[12].
- Kepler-356b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+4.6126505733'}[13].
- Kepler-356b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.3848'}[14].
- Kepler-356b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.057'}[15].
- Kepler-356b's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+18000'}[16].
- Kepler-356b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.42107650841916'}[17].
- Kepler-356b's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.68280800362500'}[18].
- Kepler-356b's epoch is recorded as J2000.0[19].
- Kepler-356b's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.729'}[20].
- Kepler-356b's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.287'}[21].
Body
Definition and Type
Kepler-356b's instance of is recorded as exoplanet[3].