Q74743370
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Q74743370
Summary
Q74743370 is a rotating variable star[1].
Key Facts
- Q74743370's instance of is recorded as rotating variable star[2].
- Q74743370's spectral class is recorded as K2[3].
- Q74743370's catalog code is recorded as KIC 10922428[4].
- Q74743370's catalog code is recorded as 2MASS J19314999+4820596[5].
- Q74743370's catalog code is recorded as Gaia DR2 2128895171283452416[6].
- Q74743370's type of variable star is recorded as rotating variable star[7].
- Q74743370's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.692'}[8].
- Q74743370's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.210'}[9].
- Q74743370's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.109'}[10].
- Q74743370's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.1295'}[11].
- Q74743370's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.3125'}[12].
- Q74743370's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-28.1'}[13].
- Q74743370's metallicity is recorded as {'unit': '1', 'amount': '+0.12'}[14].
- Q74743370's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+432.4324'}[15].
- Q74743370's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.95829121289850'}[16].
- Q74743370's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+48.34986379623310'}[17].
- Q74743370's epoch is recorded as J2000.0[18].
- Q74743370's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5040'}[19].
- Q74743370's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-2.036'}[20].
- Q74743370's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-11.353'}[21].
Body
Definition and Type
Q74743370's instance of is recorded as rotating variable star[2].