Q85905183
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Q85905183
Summary
Q85905183 is an exoplanet[1].
Key Facts
- Q85905183's instance of is recorded as exoplanet[2].
- Q85905183's constellation is recorded as Lyra[3].
- Q85905183's parent astronomical body is recorded as Q90113355[4].
- Q85905183's catalog code is recorded as KOI-2527.01[5].
- Q85905183's catalog code is recorded as Kepler-1850b[6].
- Q85905183's catalog code is recorded as KOI-2527b[7].
- Q85905183's time of discovery or invention is recorded as +2017-00-00T00:00:00Z[8].
- Q85905183's time of discovery or invention is recorded as +2022-02-00T00:00:00Z[9].
- Q85905183's discovery method is recorded as transit method[10].
- Q85905183's orbital inclination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+86.72'}[11].
- Q85905183's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+0.729096625'}[12].
- Q85905183's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+1.385800004'}[13].
- Q85905183's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.9680'}[14].
- Q85905183's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.0206'}[15].
- Q85905183's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+8130'}[16].
- Q85905183's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+287.1428295'}[17].
- Q85905183's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+43.6161177'}[18].
- Q85905183's epoch is recorded as J2000.0[19].
- Q85905183's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+13.305'}[20].
- Q85905183's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+17.300'}[21].
Body
Definition and Type
Q85905183's instance of is recorded as exoplanet[2].