Q93189328
star
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Q93189328
Summary
Q93189328 is a star[1].
Key Facts
- Q93189328's instance of is recorded as star[2].
- Q93189328's constellation is recorded as Virgo[3].
- Q93189328's spectral class is recorded as K4/5III[4].
- Q93189328's catalog code is recorded as BD-15 3792[5].
- Q93189328's catalog code is recorded as GSC 06137-00810[6].
- Q93189328's catalog code is recorded as HD 122487[7].
- Q93189328's catalog code is recorded as HIC 68606[8].
- Q93189328's catalog code is recorded as HIP 68606[9].
- Q93189328's catalog code is recorded as PPM 228194[10].
- Q93189328's catalog code is recorded as SAO 158301[11].
- Q93189328's catalog code is recorded as TYC 6137-810-1[12].
- Q93189328's catalog code is recorded as YZ 105 5248[13].
- Q93189328's catalog code is recorded as 2MASS J14023500-1553286[14].
- Q93189328's catalog code is recorded as EPIC 212359316[15].
- Q93189328's catalog code is recorded as Gaia DR2 6300855875230740608[16].
- Q93189328's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.252'}[17].
- Q93189328's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.467'}[18].
- Q93189328's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.285'}[19].
- Q93189328's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.11'}[20].
- Q93189328's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.66'}[21].
- Q93189328's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.4686'}[22].
- Q93189328's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.4624'}[23].
- Q93189328's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-26.24'}[24].
- Q93189328's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+683.8074'}[25].
- Q93189328's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+210.64586524175830'}[26].
Body
Definition and Type
Q93189328's instance of is recorded as star[2].