HD 27969 b
exoplanet in the constellation Perseus
Press Enter · cited answer in seconds
0 sources
HD 27969 b
Summary
HD 27969 b is an exoplanet[1].
Key Facts
- HD 27969 b's instance of is recorded as exoplanet[2].
- HD 27969 b's constellation is recorded as Perseus[3].
- HD 27969 b's parent astronomical body is recorded as Q66649653[4].
- HD 27969 b's catalog code is recorded as TIC 27828749b[5].
- HD 27969 b's time of discovery or invention is recorded as +2021-09-00T00:00:00Z[6].
- HD 27969 b's discovery method is recorded as Doppler spectroscopy[7].
- HD 27969 b's orbital eccentricity is recorded as {'unit': '1', 'amount': '+0.182'}[8].
- HD 27969 b's M sin i is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+4.8'}[9].
- HD 27969 b's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q651336', 'amount': '+4.8'}[10].
- HD 27969 b's orbital period is recorded as {'unit': 'http://www.wikidata.org/entity/Q573', 'amount': '+654.5'}[11].
- HD 27969 b's semi-major axis of an orbit is recorded as {'unit': 'http://www.wikidata.org/entity/Q1811', 'amount': '+1.552'}[12].
- HD 27969 b's argument of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+106.6'}[13].
- HD 27969 b's SIMBAD ID is recorded as HD 27969b[14].
- HD 27969 b's Extrasolar Planets Encyclopaedia exoplanet ID is recorded as hd_27969_b--7932[15].
- HD 27969 b's NASA Exoplanet Archive ID is recorded as HD 27969 b[16].
- HD 27969 b's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+66.7068364'}[17].
- HD 27969 b's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+42.90872'}[18].
- HD 27969 b's epoch is recorded as J2000.0[19].
- HD 27969 b's time of periapsis is recorded as {'unit': 'http://www.wikidata.org/entity/Q14267', 'amount': '+2457020.8'}[20].
Body
Designation and Status
HD 27969 b's instance of is recorded as exoplanet[2].
History and Context
HD 27969 b's catalog code is recorded as TIC 27828749b[5].