Q86851281
Mira variable star in the constellation Aquila
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Q86851281
Summary
Q86851281 is a Mira variable[1].
Key Facts
- Q86851281's instance of is recorded as Mira variable[2].
- Q86851281's instance of is recorded as infrared source[3].
- Q86851281's instance of is recorded as long-period variable star[4].
- Q86851281's instance of is recorded as near-infrared source[5].
- Q86851281's constellation is recorded as Aquila[6].
- Q86851281's spectral class is recorded as M6[7].
- Q86851281's catalog code is recorded as IRAS 20141-0716[8].
- Q86851281's catalog code is recorded as IRC -10532[9].
- Q86851281's catalog code is recorded as RAFGL 5489S[10].
- Q86851281's catalog code is recorded as 2MASS J20165004-0706578[11].
- Q86851281's catalog code is recorded as Gaia DR2 4216300816744655744[12].
- Q86851281's catalog code is recorded as V499 Aql[13].
- Q86851281's catalog code is recorded as TYC 5174-160-1[14].
- Q86851281's catalog code is recorded as TIC 205443385[15].
- Q86851281's catalog code is recorded as Gaia DR3 4216300816742250112[16].
- Q86851281's type of variable star is recorded as SRa semi-regular variable star[17].
- Q86851281's type of variable star is recorded as long-period variable star[18].
- Q86851281's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.76'}[19].
- Q86851281's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.69'}[20].
- Q86851281's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.954'}[21].
- Q86851281's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.954'}[22].
- Q86851281's apparent magnitude is recorded as {'unit': '1', 'amount': '+2.592'}[23].
- Q86851281's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.914546'}[24].
- Q86851281's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.5'}[25].
- Q86851281's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2157'}[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].