Kepler-285b
extrasolar planet
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Kepler-285b
Summary
Kepler-285b is an exoplanet[1].
Key Facts
- Kepler-285b is credited with the discovery of Kepler Space Telescope[2].
- Kepler-285b's instance of is recorded as exoplanet[3].
- Kepler-285b's constellation is recorded as Cygnus[4].
- Kepler-285b's parent astronomical body is recorded as Q87706442[5].
- Kepler-285b's catalog code is recorded as Kepler-285b[6].
- Kepler-285b's catalog code is recorded as KOI-1305.01[7].
- Kepler-285b's catalog code is recorded as KOI-1305b[8].
- Kepler-285b's catalog code is recorded as TIC 26416742b[9].
- Kepler-285b's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-285b's discovery method is recorded as transit method[11].
- Kepler-285b's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+1.354'}[12].
- Kepler-285b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+2.6338653606'}[13].
- Kepler-285b's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1846'}[14].
- Kepler-285b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.036'}[15].
- Kepler-285b's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+20000'}[16].
- Kepler-285b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.39089647525043'}[17].
- Kepler-285b's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.06558931223667'}[18].
- Kepler-285b's epoch is recorded as J2000.0[19].
- Kepler-285b's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-11.639'}[20].
- Kepler-285b'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-285b's instance of is recorded as exoplanet[3].