Q94645519
star in the constellation Serpens
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Q94645519
Summary
Q94645519 is a star[1].
Key Facts
- Q94645519's instance of is recorded as star[2].
- Q94645519's constellation is recorded as Serpens[3].
- Q94645519's catalog code is recorded as [KSC2011] FM5-43204[4].
- Q94645519's catalog code is recorded as 2MASS J15240484+0128128[5].
- Q94645519's catalog code is recorded as Gaia DR2 4420552418908966912[6].
- Q94645519's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.595'}[7].
- Q94645519's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.007'}[8].
- Q94645519's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.39'}[9].
- Q94645519's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.28'}[10].
- Q94645519's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.944'}[11].
- Q94645519's apparent magnitude is recorded as {'unit': '1', 'amount': '+17.0928'}[12].
- Q94645519's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.0228'}[13].
- Q94645519's metallicity is recorded as {'unit': '1', 'amount': '-1.62'}[14].
- Q94645519's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+231.02021410106970'}[15].
- Q94645519's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+1.47022653617520'}[16].
- Q94645519's epoch is recorded as J2000.0[17].
- Q94645519's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+4729'}[18].
- Q94645519's surface gravity is recorded as {'unit': 'http://www.wikidata.org/entity/Q39699418', 'amount': '+38'}[19].
- Q94645519's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.560'}[20].
- Q94645519's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.664'}[21].
Body
Definition and Type
Q94645519's instance of is recorded as star[2].