Q91490687
star in the constellation Serpens
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Q91490687
Summary
Q91490687 is a star[1].
Key Facts
- Q91490687's instance of is recorded as star[2].
- Q91490687's constellation is recorded as Serpens[3].
- Q91490687's spectral class is recorded as K0[4].
- Q91490687's catalog code is recorded as AG+10 1796[5].
- Q91490687's catalog code is recorded as BD+10 2817[6].
- Q91490687's catalog code is recorded as GSC 00920-00722[7].
- Q91490687's catalog code is recorded as PPM 161411[8].
- Q91490687's catalog code is recorded as SAO 101470[9].
- Q91490687's catalog code is recorded as TYC 920-722-1[10].
- Q91490687's catalog code is recorded as YZ 10 5352[11].
- Q91490687's catalog code is recorded as 2MASS J15162541+0955512[12].
- Q91490687's catalog code is recorded as Gaia DR2 1167439185557980032[13].
- Q91490687's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.236'}[14].
- Q91490687's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.737'}[15].
- Q91490687's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.606'}[16].
- Q91490687's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.97'}[17].
- Q91490687's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.96'}[18].
- Q91490687's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7010'}[19].
- Q91490687's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2861'}[20].
- Q91490687's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-17.85'}[21].
- Q91490687's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+437.4262'}[22].
- Q91490687's SIMBAD ID is recorded as BD+10 2817[23].
- Q91490687's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+229.10591465585350'}[24].
- Q91490687's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+9.93092764159110'}[25].
- Q91490687's epoch is recorded as J2000.0[26].