Kepler-325d
extrasolar planet
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Kepler-325d
Summary
Kepler-325d is an exoplanet[1].
Key Facts
- Kepler-325d is credited with the discovery of Kepler Space Telescope[2].
- Kepler-325d's instance of is recorded as exoplanet[3].
- Kepler-325d's constellation is recorded as Cygnus[4].
- Kepler-325d's parent astronomical body is recorded as Q89860933[5].
- Kepler-325d's catalog code is recorded as Kepler-325d[6].
- Kepler-325d's catalog code is recorded as KOI-1832.03[7].
- Kepler-325d's catalog code is recorded as KOI-1832d[8].
- Kepler-325d's catalog code is recorded as TIC 267671250d[9].
- Kepler-325d's time of discovery or invention is recorded as +2014-03-00T00:00:00Z[10].
- Kepler-325d's discovery method is recorded as transit method[11].
- Kepler-325d's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q1155470', 'amount': '+2.306'}[12].
- Kepler-325d's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+38.7147972585'}[13].
- Kepler-325d's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1861'}[14].
- Kepler-325d's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+0.22'}[15].
- Kepler-325d's diameter is recorded as {'unit': 'http://www.wikidata.org/entity/Q828224', 'amount': '+35600'}[16].
- Kepler-325d's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+289.83543994039246'}[17].
- Kepler-325d's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.82560118846001'}[18].
- Kepler-325d's epoch is recorded as J2000.0[19].
- Kepler-325d's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.361'}[20].
- Kepler-325d's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.696'}[21].
Body
Definition and Type
Kepler-325d's instance of is recorded as exoplanet[3].