Q91184051
high proper-motion star in the constellation Gemini
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Q91184051
Summary
Q91184051 is a high proper-motion star[1].
Key Facts
- Q91184051's instance of is recorded as high proper-motion star[2].
- Q91184051's constellation is recorded as Gemini[3].
- Q91184051's spectral class is recorded as MV:e[4].
- Q91184051's catalog code is recorded as PM J06587+2843[5].
- Q91184051's catalog code is recorded as 2E 1751[6].
- Q91184051's catalog code is recorded as 1E 0655.6+2847[7].
- Q91184051's catalog code is recorded as 1E 0655+28.7[8].
- Q91184051's catalog code is recorded as 1RXS J065846.9+284302[9].
- Q91184051's catalog code is recorded as 2E 0655.6+2847[10].
- Q91184051's catalog code is recorded as 2MASS J06584690+2843004[11].
- Q91184051's catalog code is recorded as HAT 220-01181[12].
- Q91184051's catalog code is recorded as ASAS J065847+2843.0[13].
- Q91184051's catalog code is recorded as UCAC3 238-80252[14].
- Q91184051's catalog code is recorded as UCAC4 594-036158[15].
- Q91184051's catalog code is recorded as Gaia DR2 887456864602391552[16].
- Q91184051's type of variable star is recorded as rotating variable star[17].
- Q91184051's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.642'}[18].
- Q91184051's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.995'}[19].
- Q91184051's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.776'}[20].
- Q91184051's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.70'}[21].
- Q91184051's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.63'}[22].
- Q91184051's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.14'}[23].
- Q91184051's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.2256'}[24].
- Q91184051's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+23.9494'}[25].
- Q91184051's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+41.7547'}[26].
Body
Definition and Type
Q91184051's instance of is recorded as high proper-motion star[2].