Q84191303
rotating variable star in the constellation Andromeda
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Q84191303
Summary
Q84191303 is a rotating variable star[1].
Key Facts
- Q84191303's instance of is recorded as rotating variable star[2].
- Q84191303's constellation is recorded as Andromeda[3].
- Q84191303's spectral class is recorded as sdK7.5-[4].
- Q84191303's catalog code is recorded as HAT 163-04964[5].
- Q84191303's catalog code is recorded as 2MASS J00420408+4012040[6].
- Q84191303's catalog code is recorded as LAMOST J004204.08+401204.0[7].
- Q84191303's catalog code is recorded as Gaia DR2 369095642443866368[8].
- Q84191303's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.027'}[9].
- Q84191303's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.380'}[10].
- Q84191303's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.203'}[11].
- Q84191303's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.985'}[12].
- Q84191303's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.1118'}[13].
- Q84191303's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+8.8357'}[14].
- Q84191303's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.58'}[15].
- Q84191303's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+113.1772'}[16].
- Q84191303's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+10.51703630656130'}[17].
- Q84191303's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+40.20110824672580'}[18].
- Q84191303's epoch is recorded as J2000.0[19].
- Q84191303's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-49.562'}[20].
- Q84191303's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-18.039'}[21].
Body
Definition and Type
Q84191303's instance of is recorded as rotating variable star[2].