Q90337308
star in the constellation Gemini
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Q90337308
Summary
Q90337308 is a star[1].
Key Facts
- Q90337308's instance of is recorded as star[2].
- Q90337308's constellation is recorded as Gemini[3].
- Q90337308's spectral class is recorded as F5[4].
- Q90337308's catalog code is recorded as AG+15 857[5].
- Q90337308's catalog code is recorded as BD+15 1701[6].
- Q90337308's catalog code is recorded as GSC 01363-00304[7].
- Q90337308's catalog code is recorded as PPM 124583[8].
- Q90337308's catalog code is recorded as SAO 97358[9].
- Q90337308's catalog code is recorded as TYC 1363-304-1[10].
- Q90337308's catalog code is recorded as YZ 15 3096[11].
- Q90337308's catalog code is recorded as 2MASS J07544833+1502573[12].
- Q90337308's catalog code is recorded as Gaia DR2 666577794766692480[13].
- Q90337308's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.96'}[14].
- Q90337308's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.009'}[15].
- Q90337308's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.821'}[16].
- Q90337308's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.775'}[17].
- Q90337308's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.39'}[18].
- Q90337308's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.8404'}[19].
- Q90337308's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.2387'}[20].
- Q90337308's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-8.75'}[21].
- Q90337308's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+235.9214'}[22].
- Q90337308's SIMBAD ID is recorded as BD+15 1701[23].
- Q90337308's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+118.70141038777260'}[24].
- Q90337308's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+15.04923730488160'}[25].
- Q90337308's epoch is recorded as J2000.0[26].