Q90198779
star in the constellation Corvus
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Q90198779
Summary
Q90198779 is a star[1].
Key Facts
- Q90198779's instance of is recorded as star[2].
- Q90198779's constellation is recorded as Corvus[3].
- Q90198779's spectral class is recorded as F8IV[4].
- Q90198779's catalog code is recorded as BD-16 3560[5].
- Q90198779's catalog code is recorded as GSC 06111-00385[6].
- Q90198779's catalog code is recorded as HD 112051[7].
- Q90198779's catalog code is recorded as PPM 226497[8].
- Q90198779's catalog code is recorded as SAO 157578[9].
- Q90198779's catalog code is recorded as TYC 6111-385-1[10].
- Q90198779's catalog code is recorded as YZ 106 4925[11].
- Q90198779's catalog code is recorded as 2MASS J12534539-1711504[12].
- Q90198779's catalog code is recorded as Gaia DR2 3522545710175148928[13].
- Q90198779's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.008'}[14].
- Q90198779's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.781'}[15].
- Q90198779's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.735'}[16].
- Q90198779's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.97'}[17].
- Q90198779's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.56'}[18].
- Q90198779's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9040'}[19].
- Q90198779's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.7183'}[20].
- Q90198779's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+3.28'}[21].
- Q90198779's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+174.8771'}[22].
- Q90198779's SIMBAD ID is recorded as HD 112051[23].
- Q90198779's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+193.43919092490910'}[24].
- Q90198779's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-17.19733628099240'}[25].
- Q90198779's epoch is recorded as J2000.0[26].