Q86297427
high proper-motion star in the constellation Hydrus
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Q86297427
Summary
Q86297427 is a high proper-motion star[1].
Key Facts
- Q86297427's instance of is recorded as high proper-motion star[2].
- Q86297427's instance of is recorded as near-infrared source[3].
- Q86297427's instance of is recorded as eclipsing binary star[4].
- Q86297427's constellation is recorded as Hydrus[5].
- Q86297427's spectral class is recorded as G2[6].
- Q86297427's child astronomical body is recorded as WASP-126b[7].
- Q86297427's child astronomical body is recorded as WASP-126 c[8].
- Q86297427's catalog code is recorded as 2MASS J04132972-6913365[9].
- Q86297427's catalog code is recorded as GSC 09153-00833[10].
- Q86297427's catalog code is recorded as Gaia DR2 4666498154837086208[11].
- Q86297427's catalog code is recorded as RAVE J041329.7-691337[12].
- Q86297427's catalog code is recorded as Gaia DR1 4666498150540773504[13].
- Q86297427's catalog code is recorded as TOI-114[14].
- Q86297427's catalog code is recorded as Gaia DR3 4666498154837086208[15].
- Q86297427's catalog code is recorded as TYC 9153-833-1[16].
- Q86297427's catalog code is recorded as TIC 25155310[17].
- Q86297427's type of variable star is recorded as eclipsing binary star[18].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.962'}[19].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.659'}[20].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.598'}[21].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.904'}[22].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.203'}[23].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.514'}[24].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.023'}[25].
- Q86297427's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.857'}[26].
Body
Definition and Type
Recorded instance of include high proper-motion star[2], near-infrared source[3], and eclipsing binary star[4].