Q89424391
long period variable
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Q89424391
Summary
Q89424391 is a long-period variable star[1].
Key Facts
- Q89424391's instance of is recorded as long-period variable star[2].
- Q89424391's constellation is recorded as Aquila[3].
- Q89424391's spectral class is recorded as M2-5e[4].
- Q89424391's spectral class is recorded as M2e[5].
- Q89424391's spectral class is recorded as M5e[6].
- Q89424391's catalog code is recorded as AN 81.1940[7].
- Q89424391's catalog code is recorded as 2MASS J19434376+0600049[8].
- Q89424391's catalog code is recorded as [NSC64] 1-35[9].
- Q89424391's catalog code is recorded as Gaia DR2 4291591284225289984[10].
- Q89424391's catalog code is recorded as V660 Aql[11].
- Q89424391's type of variable star is recorded as slow irregular variables of late spectral types[12].
- Q89424391's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.418'}[13].
- Q89424391's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.529'}[14].
- Q89424391's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.218'}[15].
- Q89424391's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.3857'}[16].
- Q89424391's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.2392'}[17].
- Q89424391's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+64.82'}[18].
- Q89424391's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+295.93235069293870'}[19].
- Q89424391's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+6.00140200652590'}[20].
- Q89424391's epoch is recorded as J2000.0[21].
- Q89424391's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-5.920'}[22].
- Q89424391's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.999'}[23].
Body
Definition and Type
Q89424391's instance of is recorded as long-period variable star[2].