Q86916951
star in the constellation Hydra
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Q86916951
Summary
Q86916951 is a star[1].
Key Facts
- Q86916951's instance of is recorded as star[2].
- Q86916951's constellation is recorded as Hydra[3].
- Q86916951's spectral class is recorded as G5[4].
- Q86916951's catalog code is recorded as AG+04 1198[5].
- Q86916951's catalog code is recorded as BD+05 2008[6].
- Q86916951's catalog code is recorded as GSC 00218-00888[7].
- Q86916951's catalog code is recorded as PPM 154729[8].
- Q86916951's catalog code is recorded as SAO 116940[9].
- Q86916951's catalog code is recorded as TYC 218-888-1[10].
- Q86916951's catalog code is recorded as YZ 4 4680[11].
- Q86916951's catalog code is recorded as 2MASS J08363607+0445152[12].
- Q86916951's catalog code is recorded as Gaia DR2 3092473759899394048[13].
- Q86916951's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.090'}[14].
- Q86916951's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.862'}[15].
- Q86916951's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.827'}[16].
- Q86916951's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.82'}[17].
- Q86916951's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.35'}[18].
- Q86916951's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.8780'}[19].
- Q86916951's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.6566'}[20].
- Q86916951's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-2.51'}[21].
- Q86916951's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+273.4781'}[22].
- Q86916951's SIMBAD ID is recorded as BD+05 2008[23].
- Q86916951's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+129.15032305264270'}[24].
- Q86916951's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+4.75423298011800'}[25].
- Q86916951's epoch is recorded as J2000.0[26].