Q84502207
star in the constellation Crux
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Q84502207
Summary
Q84502207 is a star[1].
Key Facts
- Q84502207's instance of is recorded as star[2].
- Q84502207's constellation is recorded as Crux[3].
- Q84502207's spectral class is recorded as K4[4].
- Q84502207's catalog code is recorded as GSC 08988-00106[5].
- Q84502207's catalog code is recorded as [PF96] 5[6].
- Q84502207's catalog code is recorded as UCAC4 150-114204[7].
- Q84502207's catalog code is recorded as 2MASS J12483236-6002439[8].
- Q84502207's catalog code is recorded as Gaia DR2 6056649738547007616[9].
- Q84502207's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.99'}[10].
- Q84502207's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.542'}[11].
- Q84502207's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.912'}[12].
- Q84502207's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.685'}[13].
- Q84502207's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.8586'}[14].
- Q84502207's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4982'}[15].
- Q84502207's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-18.86'}[16].
- Q84502207's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2007.2260'}[17].
- Q84502207's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+192.13487716600280'}[18].
- Q84502207's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-60.04553719448540'}[19].
- Q84502207's epoch is recorded as J2000.0[20].
- Q84502207's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.122'}[21].
- Q84502207's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.939'}[22].
Body
Definition and Type
Q84502207's instance of is recorded as star[2].