Q80424735
long period variable
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Q80424735
Summary
Q80424735 is a long-period variable star[1].
Key Facts
- Q80424735's instance of is recorded as long-period variable star[2].
- Q80424735's instance of is recorded as infrared source[3].
- Q80424735's instance of is recorded as near-infrared source[4].
- Q80424735's constellation is recorded as Pegasus[5].
- Q80424735's spectral class is recorded as M6[6].
- Q80424735's catalog code is recorded as BD+24 4655[7].
- Q80424735's catalog code is recorded as GSC 02225-00449[8].
- Q80424735's catalog code is recorded as IRAS 22443+2504[9].
- Q80424735's catalog code is recorded as IRC +30501[10].
- Q80424735's catalog code is recorded as 2MASS J22464652+2520156[11].
- Q80424735's catalog code is recorded as Gaia DR2 1876840342588179840[12].
- Q80424735's catalog code is recorded as EW Peg[13].
- Q80424735's catalog code is recorded as TYC 2225-449-1[14].
- Q80424735's catalog code is recorded as TIC 239543615[15].
- Q80424735's catalog code is recorded as Gaia DR3 1876840342588179840[16].
- Q80424735's type of variable star is recorded as slow irregular variables of late spectral types[17].
- Q80424735's type of variable star is recorded as long-period variable star[18].
- Q80424735's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.50'}[19].
- Q80424735's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.82'}[20].
- Q80424735's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.502'}[21].
- Q80424735's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.689'}[22].
- Q80424735's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.140'}[23].
- Q80424735's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.750532'}[24].
- Q80424735's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1628'}[25].
- Q80424735's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+859.993'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].