Q84365575
Algol variable in the constellation Microscopium
Press Enter · cited answer in seconds
0 sources
Q84365575
Summary
Q84365575 is an eclipsing binary star[1].
Key Facts
- Q84365575's instance of is recorded as eclipsing binary star[2].
- Q84365575's instance of is recorded as near-infrared source[3].
- Q84365575's instance of is recorded as Delta Scuti variable[4].
- Q84365575's constellation is recorded as Microscopium[5].
- Q84365575's spectral class is recorded as A5[6].
- Q84365575's catalog code is recorded as CSV 5281[7].
- Q84365575's catalog code is recorded as GSC 07972-00014[8].
- Q84365575's catalog code is recorded as 2MASS J20501638-4213046[9].
- Q84365575's catalog code is recorded as Gaia DR1 6677454065330598400[10].
- Q84365575's catalog code is recorded as Gaia DR2 6677454069627686144[11].
- Q84365575's catalog code is recorded as RZ Mic[12].
- Q84365575's catalog code is recorded as Gaia DR3 6677454069627686144[13].
- Q84365575's catalog code is recorded as UBV M 52936[14].
- Q84365575's catalog code is recorded as TYC 7972-14-1[15].
- Q84365575's catalog code is recorded as TIC 91369561[16].
- Q84365575's type of variable star is recorded as Algol variable[17].
- Q84365575's type of variable star is recorded as eclipsing binary star[18].
- Q84365575's type of variable star is recorded as Delta Scuti variable[19].
- Q84365575's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.35'}[20].
- Q84365575's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.72'}[21].
- Q84365575's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.683'}[22].
- Q84365575's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.268'}[23].
- Q84365575's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.205'}[24].
- Q84365575's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.243546'}[25].
- Q84365575's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.0769'}[26].
Body
Definition and Type
Recorded instance of include eclipsing binary star[2], near-infrared source[3], and Delta Scuti variable[4].