Q90947618
Algol variable in the constellation Aries
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Q90947618
Summary
Q90947618 is an eclipsing binary star[1].
Key Facts
- Q90947618's instance of is recorded as eclipsing binary star[2].
- Q90947618's instance of is recorded as near-infrared source[3].
- Q90947618's constellation is recorded as Aries[4].
- Q90947618's spectral class is recorded as F0[5].
- Q90947618's catalog code is recorded as 2MASS J02152078+2234108[6].
- Q90947618's catalog code is recorded as AG+22 206[7].
- Q90947618's catalog code is recorded as BD+21 306[8].
- Q90947618's catalog code is recorded as GSC 01765-00910[9].
- Q90947618's catalog code is recorded as PPM 91483[10].
- Q90947618's catalog code is recorded as Gaia DR1 100798759268550016[11].
- Q90947618's catalog code is recorded as Gaia DR2 100798797923874816[12].
- Q90947618's catalog code is recorded as RX Ari[13].
- Q90947618's catalog code is recorded as TYC 1765-910-1[14].
- Q90947618's catalog code is recorded as TIC 246931732[15].
- Q90947618's catalog code is recorded as Gaia DR3 100798797923874816[16].
- Q90947618's type of variable star is recorded as eclipsing binary star[17].
- Q90947618's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.93'}[18].
- Q90947618's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.649'}[19].
- Q90947618's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.361'}[20].
- Q90947618's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.285'}[21].
- Q90947618's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.41'}[22].
- Q90947618's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.331212'}[23].
- Q90947618's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+3.7261'}[24].
- Q90947618's metallicity is recorded as {'unit': '1', 'amount': '+0.01'}[25].
- Q90947618's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+268.377'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2] and near-infrared source[3].