Q88036086
high proper-motion star in the constellation Cetus
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Q88036086
Summary
Q88036086 is a high proper-motion star[1].
Key Facts
- Q88036086's instance of is recorded as high proper-motion star[2].
- Q88036086's constellation is recorded as Cetus[3].
- Q88036086's spectral class is recorded as M4.5[4].
- Q88036086's catalog code is recorded as LSPM J0322+0256[5].
- Q88036086's catalog code is recorded as NLTT 10715[6].
- Q88036086's catalog code is recorded as 2MASS J03220410+0256346[7].
- Q88036086's catalog code is recorded as USNO-B1.0 0929-00046069[8].
- Q88036086's catalog code is recorded as G 77-48[9].
- Q88036086's catalog code is recorded as GJ 1058[10].
- Q88036086's catalog code is recorded as LHS 1540[11].
- Q88036086's catalog code is recorded as PM 03195+0246[12].
- Q88036086's catalog code is recorded as USNO 410[13].
- Q88036086's catalog code is recorded as [RHG95] 603[14].
- Q88036086's catalog code is recorded as PLX 705.03[15].
- Q88036086's catalog code is recorded as WISEA J032204.33+025626.9[16].
- Q88036086's catalog code is recorded as Gaia DR2 3269132022551595264[17].
- Q88036086's type of variable star is recorded as rotating variable star[18].
- Q88036086's apparent magnitude is recorded as {'unit': '1', 'amount': '+16.54'}[19].
- Q88036086's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.9'}[20].
- Q88036086's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.314'}[21].
- Q88036086's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.806'}[22].
- Q88036086's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.508'}[23].
- Q88036086's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.3361'}[24].
- Q88036086's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+61.1393'}[25].
- Q88036086's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+16.3561'}[26].
Body
Definition and Type
Q88036086's instance of is recorded as high proper-motion star[2].