Q66630765
long-period variable star in the constellation Sagittarius
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Q66630765
Summary
Q66630765 is a long-period variable star[1].
Key Facts
- Q66630765's instance of is recorded as long-period variable star[2].
- Q66630765's instance of is recorded as near-infrared source[3].
- Q66630765's constellation is recorded as Sagittarius[4].
- Q66630765's spectral class is recorded as M2III[5].
- Q66630765's catalog code is recorded as CPC 18 10603[6].
- Q66630765's catalog code is recorded as GSC 07949-01307[7].
- Q66630765's catalog code is recorded as HD 194476[8].
- Q66630765's catalog code is recorded as HIC 100868[9].
- Q66630765's catalog code is recorded as HIP 100868[10].
- Q66630765's catalog code is recorded as IRAS 20238-3909[11].
- Q66630765's catalog code is recorded as 2MASS J20270795-3859348[12].
- Q66630765's catalog code is recorded as PPM 300199[13].
- Q66630765's catalog code is recorded as Gaia DR2 6681070844407557248[14].
- Q66630765's catalog code is recorded as V4443 Sgr[15].
- Q66630765's catalog code is recorded as Gaia DR3 6681070844407557248[16].
- Q66630765's catalog code is recorded as TYC 7949-1307-1[17].
- Q66630765's catalog code is recorded as TIC 290597544[18].
- Q66630765's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.39'}[19].
- Q66630765's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.86'}[20].
- Q66630765's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.914'}[21].
- Q66630765's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.936'}[22].
- Q66630765's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.638'}[23].
- Q66630765's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.688344'}[24].
- Q66630765's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.796'}[25].
- Q66630765's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+14.42'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2] and near-infrared source[3].