Q93535295
star in the constellation Orion
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Q93535295
Summary
Q93535295 is a star[1].
Key Facts
- Q93535295's instance of is recorded as star[2].
- Q93535295's constellation is recorded as Orion[3].
- Q93535295's spectral class is recorded as K7[4].
- Q93535295's catalog code is recorded as 2MASS J05075837+1414598[5].
- Q93535295's catalog code is recorded as AG+14 470[6].
- Q93535295's catalog code is recorded as BD+14 835[7].
- Q93535295's catalog code is recorded as GSC 00710-00596[8].
- Q93535295's catalog code is recorded as HD 240907[9].
- Q93535295's catalog code is recorded as IRAS 05051+1411[10].
- Q93535295's catalog code is recorded as PPM 120632[11].
- Q93535295's catalog code is recorded as TYC 710-596-1[12].
- Q93535295's catalog code is recorded as Gaia DR2 3392091782275695104[13].
- Q93535295's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.665'}[14].
- Q93535295's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.897'}[15].
- Q93535295's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.594'}[16].
- Q93535295's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.03'}[17].
- Q93535295's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.72'}[18].
- Q93535295's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.2505'}[19].
- Q93535295's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.8057'}[20].
- Q93535295's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-54.73'}[21].
- Q93535295's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+553.8018'}[22].
- Q93535295's SIMBAD ID is recorded as HD 240907[23].
- Q93535295's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+76.99327884360700'}[24].
- Q93535295's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+14.24996218035290'}[25].
- Q93535295's epoch is recorded as J2000.0[26].