Q88149752
long period variable
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Q88149752
Summary
Q88149752 is a long-period variable star[1].
Key Facts
- Q88149752's instance of is recorded as long-period variable star[2].
- Q88149752's constellation is recorded as Ursa Minor[3].
- Q88149752's spectral class is recorded as M3/4[4].
- Q88149752's catalog code is recorded as FBS 1522+834[5].
- Q88149752's catalog code is recorded as FBS L 8-56[6].
- Q88149752's catalog code is recorded as IRAS F15225+8324[7].
- Q88149752's catalog code is recorded as [WWV2004] J1517464+831345[8].
- Q88149752's catalog code is recorded as 2MASS J15174650+8313469[9].
- Q88149752's catalog code is recorded as Gaia DR2 1722341847736375936[10].
- Q88149752's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.711'}[11].
- Q88149752's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.796'}[12].
- Q88149752's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.526'}[13].
- Q88149752's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.6254'}[14].
- Q88149752's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.3276'}[15].
- Q88149752's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-9.33'}[16].
- Q88149752's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+3052.5031'}[17].
- Q88149752's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+229.44369597396340'}[18].
- Q88149752's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+83.22971028369140'}[19].
- Q88149752's epoch is recorded as J2000.0[20].
- Q88149752's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+1.307'}[21].
- Q88149752's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-6.311'}[22].
Body
Definition and Type
Q88149752's instance of is recorded as long-period variable star[2].