Q89445912
Algol variable in the constellation Antlia
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Q89445912
Summary
Q89445912 is a spectroscopic binary[1].
Key Facts
- Q89445912's instance of is recorded as spectroscopic binary[2].
- Q89445912's instance of is recorded as star[3].
- Q89445912's instance of is recorded as eclipsing binary star[4].
- Q89445912's instance of is recorded as near-infrared source[5].
- Q89445912's constellation is recorded as Antlia[6].
- Q89445912's spectral class is recorded as G2[7].
- Q89445912's catalog code is recorded as CPC 18 5065[8].
- Q89445912's catalog code is recorded as GSC 07211-01165[9].
- Q89445912's catalog code is recorded as PPM 288225[10].
- Q89445912's catalog code is recorded as SAO 201848[11].
- Q89445912's catalog code is recorded as 2MASS J10522138-3618104[12].
- Q89445912's catalog code is recorded as Gaia DR2 5395278719703723776[13].
- Q89445912's catalog code is recorded as CF Ant[14].
- Q89445912's catalog code is recorded as TYC 7211-1165-1[15].
- Q89445912's catalog code is recorded as TIC 158329676[16].
- Q89445912's catalog code is recorded as Gaia DR3 5395278719705226624[17].
- Q89445912's type of variable star is recorded as eclipsing binary star[18].
- Q89445912's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.984'}[19].
- Q89445912's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.736'}[20].
- Q89445912's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.587'}[21].
- Q89445912's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.16'}[22].
- Q89445912's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.77'}[23].
- Q89445912's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.975741'}[24].
- Q89445912's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.5538'}[25].
- Q89445912's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+219.597'}[26].
Body
Definition and Type
Recorded instance of include spectroscopic binary[2], star[3], eclipsing binary star[4], and near-infrared source[5].