Q87057495
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Q87057495
Summary
Q87057495 is a high proper-motion star[1].
Key Facts
- Q87057495's instance of is recorded as high proper-motion star[2].
- Q87057495's instance of is recorded as BY Draconis variable[3].
- Q87057495's instance of is recorded as near-infrared source[4].
- Q87057495's instance of is recorded as variable star[5].
- Q87057495's instance of is recorded as astrophysical X-ray source[6].
- Q87057495's constellation is recorded as Pegasus[7].
- Q87057495's spectral class is recorded as K4V[8].
- Q87057495's catalog code is recorded as 1RXS J230725.0+315012[9].
- Q87057495's catalog code is recorded as GSC 02751-00009[10].
- Q87057495's catalog code is recorded as 2MASS J23072487+3150141[11].
- Q87057495's catalog code is recorded as Gaia DR1 1886707939755266176[12].
- Q87057495's catalog code is recorded as Gaia DR2 1886707944052138752[13].
- Q87057495's catalog code is recorded as V567 Peg[14].
- Q87057495's catalog code is recorded as Gaia DR3 1886707944052532608[15].
- Q87057495's catalog code is recorded as TIC 305978886[16].
- Q87057495's catalog code is recorded as TYC 2751-9-1[17].
- Q87057495's type of variable star is recorded as BY Draconis variable[18].
- Q87057495's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.48'}[19].
- Q87057495's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.73'}[20].
- Q87057495's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.538'}[21].
- Q87057495's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.995'}[22].
- Q87057495's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.874'}[23].
- Q87057495's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.80'}[24].
- Q87057495's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.382854'}[25].
- Q87057495's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+20.4203'}[26].
Body
Definition and Type
Recorded instance of include high proper-motion star[2], BY Draconis variable[3], near-infrared source[4], variable star[5], and astrophysical X-ray source[6].