Q88659457
long period variable
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Q88659457
Summary
Q88659457 is a long-period variable star[1].
Key Facts
- Q88659457's instance of is recorded as long-period variable star[2].
- Q88659457's instance of is recorded as infrared source[3].
- Q88659457's instance of is recorded as near-infrared source[4].
- Q88659457's constellation is recorded as Apus[5].
- Q88659457's catalog code is recorded as CSV 7306[6].
- Q88659457's catalog code is recorded as GSC 09286-01707[7].
- Q88659457's catalog code is recorded as PPM 786862[8].
- Q88659457's catalog code is recorded as IRAS 16192-7330[9].
- Q88659457's catalog code is recorded as 2MASS J16251348-7337202[10].
- Q88659457's catalog code is recorded as Gaia DR1 5805525298508714880[11].
- Q88659457's catalog code is recorded as Gaia DR2 5805525302808129152[12].
- Q88659457's catalog code is recorded as HY Aps[13].
- Q88659457's catalog code is recorded as TYC 9286-1707-1[14].
- Q88659457's catalog code is recorded as TIC 324776317[15].
- Q88659457's catalog code is recorded as Gaia DR3 5805525302809488000[16].
- Q88659457's type of variable star is recorded as long-period variable star[17].
- Q88659457's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.63'}[18].
- Q88659457's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.24'}[19].
- Q88659457's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.458'}[20].
- Q88659457's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.575'}[21].
- Q88659457's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.118'}[22].
- Q88659457's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.227074'}[23].
- Q88659457's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.7807'}[24].
- Q88659457's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-61.62'}[25].
- Q88659457's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1280.902'}[26].
Body
Definition and Type
Recorded instance of include long-period variable star[2], infrared source[3], and near-infrared source[4].