Q90472810
Algol variable in the constellation Aquila
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Q90472810
Summary
Q90472810 is an Algol variable[1].
Key Facts
- Q90472810's instance of is recorded as Algol variable[2].
- Q90472810's constellation is recorded as Aquila[3].
- Q90472810's spectral class is recorded as F5[4].
- Q90472810's catalog code is recorded as HD 231630[5].
- Q90472810's catalog code is recorded as AN 117.1935[6].
- Q90472810's catalog code is recorded as GSC 01067-00962[7].
- Q90472810's catalog code is recorded as SV* P 5042[8].
- Q90472810's catalog code is recorded as TYC 1067-962-1[9].
- Q90472810's catalog code is recorded as 2MASS J19304372+1340208[10].
- Q90472810's catalog code is recorded as ASAS J193044+1340.3[11].
- Q90472810's catalog code is recorded as Gaia DR2 4316576758263867136[12].
- Q90472810's catalog code is recorded as V415 Aql[13].
- Q90472810's type of variable star is recorded as eclipsing binary star[14].
- Q90472810's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.18'}[15].
- Q90472810's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.55'}[16].
- Q90472810's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.546'}[17].
- Q90472810's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.269'}[18].
- Q90472810's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.183'}[19].
- Q90472810's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.2369'}[20].
- Q90472810's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.0606'}[21].
- Q90472810's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+485.2955'}[22].
- Q90472810's SIMBAD ID is recorded as V* V415 Aql[23].
- Q90472810's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+292.68220097422660'}[24].
- Q90472810's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+13.67244714303510'}[25].
- Q90472810's epoch is recorded as J2000.0[26].