Q88915305
Algol variable in the constellation Lacerta
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Q88915305
Summary
Q88915305 is a spectroscopic binary[1].
Key Facts
- Q88915305's instance of is recorded as spectroscopic binary[2].
- Q88915305's instance of is recorded as eclipsing binary star[3].
- Q88915305's instance of is recorded as near-infrared source[4].
- Q88915305's constellation is recorded as Lacerta[5].
- Q88915305's spectral class is recorded as F0(N)[6].
- Q88915305's catalog code is recorded as AG+38 2360[7].
- Q88915305's catalog code is recorded as BD+37 4662[8].
- Q88915305's catalog code is recorded as GSC 03214-01295[9].
- Q88915305's catalog code is recorded as PPM 88077[10].
- Q88915305's catalog code is recorded as SAO 72615[11].
- Q88915305's catalog code is recorded as 2MASS J22410056+3819200[12].
- Q88915305's catalog code is recorded as Gaia DR1 1905008280007897984[13].
- Q88915305's catalog code is recorded as Gaia DR2 1905008284306000128[14].
- Q88915305's catalog code is recorded as VX Lac[15].
- Q88915305's catalog code is recorded as TYC 3214-1295-1[16].
- Q88915305's catalog code is recorded as TIC 128785705[17].
- Q88915305's catalog code is recorded as Gaia DR3 1905008284306000128[18].
- Q88915305's type of variable star is recorded as eclipsing binary star[19].
- Q88915305's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.950'}[20].
- Q88915305's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.753'}[21].
- Q88915305's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.670'}[22].
- Q88915305's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.51'}[23].
- Q88915305's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.87'}[24].
- Q88915305's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.593241'}[25].
- Q88915305's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.2832'}[26].
Body
Definition and Type
Recorded instance of include spectroscopic binary[2], eclipsing binary star[3], and near-infrared source[4].