Q86189802
star in the constellation Virgo
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Q86189802
Summary
Q86189802 is a star[1].
Key Facts
- Q86189802's instance of is recorded as star[2].
- Q86189802's constellation is recorded as Virgo[3].
- Q86189802's spectral class is recorded as G5[4].
- Q86189802's catalog code is recorded as AG+07 1610[5].
- Q86189802's catalog code is recorded as BD+08 2575[6].
- Q86189802's catalog code is recorded as GSC 00287-00008[7].
- Q86189802's catalog code is recorded as HD 105867[8].
- Q86189802's catalog code is recorded as PPM 158591[9].
- Q86189802's catalog code is recorded as TYC 287-8-1[10].
- Q86189802's catalog code is recorded as Gaia DR1 3904622388759096576[11].
- Q86189802's catalog code is recorded as Gaia DR2 3904622393055114624[12].
- Q86189802's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.15'}[13].
- Q86189802's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.94'}[14].
- Q86189802's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.0229'}[15].
- Q86189802's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.6792'}[16].
- Q86189802's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+36.87'}[17].
- Q86189802's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+213.7117'}[18].
- Q86189802's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+182.77797629248440'}[19].
- Q86189802's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+7.26490989546410'}[20].
- Q86189802's epoch is recorded as J2000.0[21].
- Q86189802's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+0.060'}[22].
- Q86189802's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.278'}[23].
Body
Definition and Type
Q86189802's instance of is recorded as star[2].