Q87826435
star in the constellation Lyra
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Q87826435
Summary
Q87826435 is a star[1].
Key Facts
- Q87826435's instance of is recorded as star[2].
- Q87826435's instance of is recorded as near-infrared source[3].
- Q87826435's constellation is recorded as Lyra[4].
- Q87826435's spectral class is recorded as F9[5].
- Q87826435's child astronomical body is recorded as KIC 8540376c[6].
- Q87826435's child astronomical body is recorded as KIC 8540376b[7].
- Q87826435's child astronomical body is recorded as Kepler-457 d[8].
- Q87826435's catalog code is recorded as Gaia DR2 2105414310196331264[9].
- Q87826435's catalog code is recorded as 2MASS J18493060+4441405[10].
- Q87826435's catalog code is recorded as KIC 8540376[11].
- Q87826435's catalog code is recorded as Kepler-457[12].
- Q87826435's catalog code is recorded as Kepler-1803[13].
- Q87826435's catalog code is recorded as Gaia DR3 2105414310196331264[14].
- Q87826435's catalog code is recorded as TIC 123449386[15].
- Q87826435's catalog code is recorded as KOI-7892[16].
- Q87826435's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.260'}[17].
- Q87826435's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.014'}[18].
- Q87826435's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.966'}[19].
- Q87826435's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.203927'}[20].
- Q87826435's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.841219'}[21].
- Q87826435's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+1.15'}[22].
- Q87826435's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+1.1489118'}[23].
- Q87826435's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.9303'}[24].
- Q87826435's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-60.71'}[25].
- Q87826435's metallicity is recorded as {'unit': '1', 'amount': '-0.051'}[26].