Q83202248
long period variable
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Q83202248
Summary
Q83202248 is a long-period variable star[1].
Key Facts
- Q83202248's instance of is recorded as long-period variable star[2].
- Q83202248's instance of is recorded as infrared source[3].
- Q83202248's instance of is recorded as near-infrared source[4].
- Q83202248's constellation is recorded as Aquila[5].
- Q83202248's spectral class is recorded as M2[6].
- Q83202248's catalog code is recorded as GSC 01615-03862[7].
- Q83202248's catalog code is recorded as IRAS 19450+1556[8].
- Q83202248's catalog code is recorded as RAFGL 5429S[9].
- Q83202248's catalog code is recorded as 2MASS J19472024+1603575[10].
- Q83202248's catalog code is recorded as Gaia DR1 1820595164573233408[11].
- Q83202248's catalog code is recorded as Gaia DR2 1820595168911166720[12].
- Q83202248's catalog code is recorded as V446 Aql[13].
- Q83202248's catalog code is recorded as TYC 1615-3862-1[14].
- Q83202248's catalog code is recorded as TIC 345164327[15].
- Q83202248's catalog code is recorded as Gaia DR3 1820595168911166720[16].
- Q83202248's type of variable star is recorded as semiregular variable star[17].
- Q83202248's type of variable star is recorded as long-period variable star[18].
- Q83202248's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.53'}[19].
- Q83202248's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.655'}[20].
- Q83202248's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.889'}[21].
- Q83202248's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.537'}[22].
- Q83202248's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.66'}[23].
- Q83202248's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.101359'}[24].
- Q83202248's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.1029'}[25].
- Q83202248's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+54.82'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].