Q85930774
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Q85930774
Summary
Q85930774 is an exoplanet[1].
Key Facts
- Q85930774's instance of is recorded as exoplanet[2].
- Q85930774's constellation is recorded as Cygnus[3].
- Q85930774's parent astronomical body is recorded as Q90560522[4].
- Q85930774's catalog code is recorded as KOI-2043.01[5].
- Q85930774's catalog code is recorded as Kepler-1786b[6].
- Q85930774's catalog code is recorded as KOI-2043b[7].
- Q85930774's time of discovery or invention is recorded as +2017-00-00T00:00:00Z[8].
- Q85930774's time of discovery or invention is recorded as +2022-02-00T00:00:00Z[9].
- Q85930774's discovery method is recorded as transit method[10].
- Q85930774's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+89.96'}[11].
- Q85930774's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+3.163058277'}[12].
- Q85930774's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+78.5460968'}[13].
- Q85930774's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1289'}[14].
- Q85930774's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.3659'}[15].
- Q85930774's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+33900'}[16].
- Q85930774's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.5877743'}[17].
- Q85930774's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+38.5219827'}[18].
- Q85930774's epoch is recorded as J2000.0[19].
- Q85930774's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.752'}[20].
- Q85930774's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.574'}[21].
Body
Definition and Type
Q85930774's instance of is recorded as exoplanet[2].