Q83592446
Delta Scuti variable star in the constellation Lyra
Press Enter · cited answer in seconds
0 sources
Q83592446
Summary
Q83592446 is a Delta Scuti variable[1].
Key Facts
- Q83592446's instance of is recorded as Delta Scuti variable[2].
- Q83592446's constellation is recorded as Lyra[3].
- Q83592446's spectral class is recorded as F1V[4].
- Q83592446's catalog code is recorded as AG+37 1781[5].
- Q83592446's catalog code is recorded as BD+36 3535[6].
- Q83592446's catalog code is recorded as GSC 02666-00829[7].
- Q83592446's catalog code is recorded as PPM 82823[8].
- Q83592446's catalog code is recorded as SAO 68243[9].
- Q83592446's catalog code is recorded as TYC 2666-829-1[10].
- Q83592446's catalog code is recorded as 2MASS J19234056+3709547[11].
- Q83592446's catalog code is recorded as WDS J19237+3710AB[12].
- Q83592446's catalog code is recorded as KIC 1571152[13].
- Q83592446's catalog code is recorded as Gaia DR2 2051013567227950080[14].
- Q83592446's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.547'}[15].
- Q83592446's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.414'}[16].
- Q83592446's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.381'}[17].
- Q83592446's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.31'}[18].
- Q83592446's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.68'}[19].
- Q83592446's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.2242'}[20].
- Q83592446's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-23.0'}[21].
- Q83592446's metallicity is recorded as {'unit': '1', 'amount': '-0.07'}[22].
- Q83592446's SIMBAD ID is recorded as BD+36 3535[23].
- Q83592446's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+290.91908725803030'}[24].
- Q83592446's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+37.16524973295230'}[25].
- Q83592446's epoch is recorded as J2000.0[26].