Kepler-285c
extrasolar planet
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Kepler-285c
Summary
Kepler-285c is an exoplanet[1].
Key Facts
- Kepler-285c is credited with the discovery of Kepler Space Telescope[2].
- Kepler-285c's instance of is recorded as exoplanet[3].
- Kepler-285c's constellation is recorded as Cygnus[4].
- Kepler-285c's parent astronomical body is recorded as Q87706442[5].
- Kepler-285c's catalog code is recorded as Kepler-285c[6].
- Kepler-285c's catalog code is recorded as KOI-1305.02[7].
- Kepler-285c's catalog code is recorded as KOI-1305c[8].
- Kepler-285c's catalog code is recorded as TIC 26416742c[9].
- Kepler-285c's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-285c's discovery method is recorded as transit method[11].
- Kepler-285c's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+1.187'}[12].
- Kepler-285c's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+6.1866965315'}[13].
- Kepler-285c's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1846'}[14].
- Kepler-285c's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.064'}[15].
- Kepler-285c's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+17900'}[16].
- Kepler-285c's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.39089647525043'}[17].
- Kepler-285c's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.06558931223667'}[18].
- Kepler-285c's epoch is recorded as J2000.0[19].
- Kepler-285c's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-11.639'}[20].
- Kepler-285c's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-7.693'}[21].
Body
Definition and Type
Kepler-285c's instance of is recorded as exoplanet[3].