Q88867656
long period variable
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Q88867656
Summary
Q88867656 is a long-period variable star[1].
Key Facts
- Q88867656's instance of is recorded as long-period variable star[2].
- Q88867656's instance of is recorded as near-infrared source[3].
- Q88867656's constellation is recorded as Aquila[4].
- Q88867656's spectral class is recorded as K0/2e[5].
- Q88867656's catalog code is recorded as GSC 05160-00016[6].
- Q88867656's catalog code is recorded as 2MASS J20055278-0110015[7].
- Q88867656's catalog code is recorded as Gaia DR2 4235862056321253504[8].
- Q88867656's catalog code is recorded as V576 Aql[9].
- Q88867656's catalog code is recorded as TIC 243670971[10].
- Q88867656's catalog code is recorded as Gaia DR3 4235862056321253504[11].
- Q88867656's type of variable star is recorded as long-period variable star[12].
- Q88867656's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.821'}[13].
- Q88867656's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.234'}[14].
- Q88867656's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.965'}[15].
- Q88867656's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.274135'}[16].
- Q88867656's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1128'}[17].
- Q88867656's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-84.53'}[18].
- Q88867656's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+301.46990342325'}[19].
- Q88867656's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-1.16712286856'}[20].
- Q88867656's epoch is recorded as J2000.0[21].
- Q88867656's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-1.042'}[22].
- Q88867656's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.482'}[23].
Body
Definition and Type
Recorded instance of include long-period variable star[2] and near-infrared source[3].