Q88693569
Mira variable star in the constellation Sagittarius
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Q88693569
Summary
Q88693569 is a Mira variable[1].
Key Facts
- Q88693569's instance of is recorded as Mira variable[2].
- Q88693569's instance of is recorded as infrared source[3].
- Q88693569's instance of is recorded as long-period variable star[4].
- Q88693569's instance of is recorded as near-infrared source[5].
- Q88693569's constellation is recorded as Sagittarius[6].
- Q88693569's spectral class is recorded as M3[7].
- Q88693569's catalog code is recorded as IRAS 17540-1919[8].
- Q88693569's catalog code is recorded as IRC -20403[9].
- Q88693569's catalog code is recorded as ASAS J175703-1920.2[10].
- Q88693569's catalog code is recorded as RAFGL 2036[11].
- Q88693569's catalog code is recorded as [TVH89] 232[12].
- Q88693569's catalog code is recorded as 2MASS J17570307-1920159[13].
- Q88693569's catalog code is recorded as Gaia DR2 4119356086312854144[14].
- Q88693569's catalog code is recorded as VV Sgr[15].
- Q88693569's catalog code is recorded as TIC 105604187[16].
- Q88693569's catalog code is recorded as Gaia DR3 4119356086312854272[17].
- Q88693569's type of variable star is recorded as long-period variable star[18].
- Q88693569's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.8'}[19].
- Q88693569's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.326'}[20].
- Q88693569's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.210'}[21].
- Q88693569's apparent magnitude is recorded as {'unit': '1', 'amount': '+1.617'}[22].
- Q88693569's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.073892'}[23].
- Q88693569's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1746'}[24].
- Q88693569's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+44'}[25].
- Q88693569's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+851.354'}[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].