Q84283010
Mira variable star in the constellation Sagittarius
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Q84283010
Summary
Q84283010 is a Mira variable[1].
Key Facts
- Q84283010's instance of is recorded as Mira variable[2].
- Q84283010's instance of is recorded as infrared source[3].
- Q84283010's instance of is recorded as long-period variable star[4].
- Q84283010's instance of is recorded as near-infrared source[5].
- Q84283010's constellation is recorded as Sagittarius[6].
- Q84283010's spectral class is recorded as M7[7].
- Q84283010's catalog code is recorded as [GGA99] NGC 6522 245[8].
- Q84283010's catalog code is recorded as 2MASS J18031146-2957471[9].
- Q84283010's catalog code is recorded as MSX6C G001.0464-03.8196[10].
- Q84283010's catalog code is recorded as Gaia DR2 4050202474231521280[11].
- Q84283010's catalog code is recorded as V4002 Sgr[12].
- Q84283010's catalog code is recorded as OGLE BUL-SC45 101285[13].
- Q84283010's catalog code is recorded as OGLE BLG190.6 117634[14].
- Q84283010's catalog code is recorded as OGLE BLG513.12 60218[15].
- Q84283010's catalog code is recorded as Gaia DR3 4050202474231521280[16].
- Q84283010's catalog code is recorded as TIC 406401351[17].
- Q84283010's catalog code is recorded as OGLE BLG-LPV-192148[18].
- Q84283010's type of variable star is recorded as Mira variable[19].
- Q84283010's type of variable star is recorded as long-period variable star[20].
- Q84283010's type of variable star is recorded as semiregular variable star[21].
- Q84283010's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.564'}[22].
- Q84283010's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.353'}[23].
- Q84283010's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.20'}[24].
- Q84283010's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.535'}[25].
- Q84283010's apparent magnitude is recorded as {'unit': '1', 'amount': '+18.058'}[26].
Body
Definition and Type
Recorded instance of include Mira variable[2], infrared source[3], long-period variable star[4], and near-infrared source[5].