Q74742053
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Q74742053
Summary
Q74742053 is a rotating variable star[1].
Key Facts
- Q74742053's instance of is recorded as rotating variable star[2].
- Q74742053's spectral class is recorded as G5[3].
- Q74742053's catalog code is recorded as KIC 11390690[4].
- Q74742053's catalog code is recorded as 2MASS J18583534+4917000[5].
- Q74742053's catalog code is recorded as Gaia DR2 2132183776199616768[6].
- Q74742053's type of variable star is recorded as rotating variable star[7].
- Q74742053's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.129'}[8].
- Q74742053's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.744'}[9].
- Q74742053's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.708'}[10].
- Q74742053's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2858'}[11].
- Q74742053's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.8357'}[12].
- Q74742053's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-4.5'}[13].
- Q74742053's metallicity is recorded as {'unit': '1', 'amount': '+0.05'}[14].
- Q74742053's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+544.7513'}[15].
- Q74742053's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+284.64727548016480'}[16].
- Q74742053's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+49.28333265495160'}[17].
- Q74742053's epoch is recorded as J2000.0[18].
- Q74742053's effective temperature is recorded as {'unit': 'http://www.wikidata.org/entity/Q11579', 'amount': '+5566'}[19].
- Q74742053's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.413'}[20].
- Q74742053's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.941'}[21].
Body
Definition and Type
Q74742053's instance of is recorded as rotating variable star[2].