Q85698049
star in the constellation Serpens
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Q85698049
Summary
Q85698049 is a star[1].
Key Facts
- Q85698049's instance of is recorded as star[2].
- Q85698049's constellation is recorded as Serpens[3].
- Q85698049's spectral class is recorded as G5[4].
- Q85698049's catalog code is recorded as BD-06 4731[5].
- Q85698049's catalog code is recorded as GSC 05110-00364[6].
- Q85698049's catalog code is recorded as PPM 201547[7].
- Q85698049's catalog code is recorded as SAO 142181[8].
- Q85698049's catalog code is recorded as TYC 5110-364-1[9].
- Q85698049's catalog code is recorded as YZ 0 4371[10].
- Q85698049's catalog code is recorded as YZ 95 6130[11].
- Q85698049's catalog code is recorded as 2MASS J18152956-0558053[12].
- Q85698049's catalog code is recorded as Gaia DR2 4172787369222255616[13].
- Q85698049's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.92'}[14].
- Q85698049's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.78'}[15].
- Q85698049's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.316'}[16].
- Q85698049's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.950'}[17].
- Q85698049's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.780'}[18].
- Q85698049's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.6908'}[19].
- Q85698049's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+6.5810'}[20].
- Q85698049's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-2.75'}[21].
- Q85698049's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+151.9526'}[22].
- Q85698049's SIMBAD ID is recorded as BD-06 4731[23].
- Q85698049's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+273.87314723135110'}[24].
- Q85698049's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-5.96812845803150'}[25].
- Q85698049's epoch is recorded as J2000.0[26].