Q93099941
high proper-motion star in the constellation Capricornus
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Q93099941
Summary
Q93099941 is a high proper-motion star[1].
Key Facts
- Q93099941's instance of is recorded as high proper-motion star[2].
- Q93099941's constellation is recorded as Capricornus[3].
- Q93099941's spectral class is recorded as M6.5[4].
- Q93099941's catalog code is recorded as 2MASS J21481595-1401059[5].
- Q93099941's catalog code is recorded as Gaia DR2 6840258408458749184[6].
- Q93099941's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.68'}[7].
- Q93099941's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.11'}[8].
- Q93099941's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.65'}[9].
- Q93099941's apparent magnitude is recorded as {'unit': '1', 'amount': '+20.20'}[10].
- Q93099941's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.15'}[11].
- Q93099941's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.7225'}[12].
- Q93099941's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+10.8251'}[13].
- Q93099941's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+92.3779'}[14].
- Q93099941's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+327.06642583848680'}[15].
- Q93099941's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-14.01833812440370'}[16].
- Q93099941's epoch is recorded as J2000.0[17].
- Q93099941's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+2700'}[18].
- Q93099941's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-155.478'}[19].
- Q93099941's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-173.173'}[20].
Body
Definition and Type
Q93099941's instance of is recorded as high proper-motion star[2].