Q92411908
star in the constellation Gemini
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Q92411908
Summary
Q92411908 is a star[1].
Key Facts
- Q92411908's instance of is recorded as star[2].
- Q92411908's constellation is recorded as Gemini[3].
- Q92411908's spectral class is recorded as K0[4].
- Q92411908's catalog code is recorded as 2MASS J07092921+2154031[5].
- Q92411908's catalog code is recorded as AG+21 781[6].
- Q92411908's catalog code is recorded as BD+22 1594[7].
- Q92411908's catalog code is recorded as GSC 01357-00138[8].
- Q92411908's catalog code is recorded as PPM 97114[9].
- Q92411908's catalog code is recorded as SAO 79120[10].
- Q92411908's catalog code is recorded as TYC 1357-138-1[11].
- Q92411908's catalog code is recorded as YZ 21 2808[12].
- Q92411908's catalog code is recorded as Gaia DR2 3367364659121929088[13].
- Q92411908's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.360'}[14].
- Q92411908's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.854'}[15].
- Q92411908's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.762'}[16].
- Q92411908's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.07'}[17].
- Q92411908's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.07'}[18].
- Q92411908's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8249'}[19].
- Q92411908's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5724'}[20].
- Q92411908's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.57'}[21].
- Q92411908's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+635.9705'}[22].
- Q92411908's SIMBAD ID is recorded as BD+22 1594[23].
- Q92411908's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+107.37178298185210'}[24].
- Q92411908's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+21.90082437578060'}[25].
- Q92411908's epoch is recorded as J2000.0[26].