Q78792273
star in the constellation Orion
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Q78792273
Summary
Q78792273 is a star[1].
Key Facts
- Q78792273's instance of is recorded as star[2].
- Q78792273's constellation is recorded as Orion[3].
- Q78792273's spectral class is recorded as G5IV[4].
- Q78792273's catalog code is recorded as BD+14 1198[5].
- Q78792273's catalog code is recorded as GSC 00742-02182[6].
- Q78792273's catalog code is recorded as LF 8 +14 136[7].
- Q78792273's catalog code is recorded as 2MASS J06132343+1406273[8].
- Q78792273's catalog code is recorded as Gaia DR2 3344786428365326848[9].
- Q78792273's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.0'}[10].
- Q78792273's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.998'}[11].
- Q78792273's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.520'}[12].
- Q78792273's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.351'}[13].
- Q78792273's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.6523'}[14].
- Q78792273's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.6668'}[15].
- Q78792273's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-44.10'}[16].
- Q78792273's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+599.9520'}[17].
- Q78792273's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+93.34767145372660'}[18].
- Q78792273's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+14.10754081726770'}[19].
- Q78792273's epoch is recorded as J2000.0[20].
- Q78792273's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-12.759'}[21].
- Q78792273's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+10.821'}[22].
Body
Definition and Type
Q78792273's instance of is recorded as star[2].