Kepler-292f
extrasolar planet
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Kepler-292f
Summary
Kepler-292f is an exoplanet[1].
Key Facts
- Kepler-292f is credited with the discovery of Kepler Space Telescope[2].
- Kepler-292f's instance of is recorded as exoplanet[3].
- Kepler-292f's constellation is recorded as Cygnus[4].
- Kepler-292f's parent astronomical body is recorded as Kepler-292[5].
- Kepler-292f's catalog code is recorded as Kepler-292f[6].
- Kepler-292f's catalog code is recorded as KOI-1364.01[7].
- Kepler-292f's catalog code is recorded as KOI-1364f[8].
- Kepler-292f's catalog code is recorded as TIC 271960465f[9].
- Kepler-292f's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-292f's discovery method is recorded as transit method[11].
- Kepler-292f's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+2.324'}[12].
- Kepler-292f's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+20.8343328525'}[13].
- Kepler-292f's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9198'}[14].
- Kepler-292f's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.141'}[15].
- Kepler-292f's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+43600'}[16].
- Kepler-292f's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.76615670460120'}[17].
- Kepler-292f's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+42.42429173205889'}[18].
- Kepler-292f's epoch is recorded as J2000.0[19].
- Kepler-292f's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.211'}[20].
- Kepler-292f's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+7.063'}[21].
Body
Definition and Type
Kepler-292f's instance of is recorded as exoplanet[3].