Q87706513
rotating variable star in the constellation Cygnus
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Q87706513
Summary
Q87706513 is a rotating variable star[1].
Key Facts
- Q87706513's instance of is recorded as rotating variable star[2].
- Q87706513's instance of is recorded as star[3].
- Q87706513's instance of is recorded as near-infrared source[4].
- Q87706513's constellation is recorded as Cygnus[5].
- Q87706513's spectral class is recorded as G5[6].
- Q87706513's child astronomical body is recorded as Q28503931[7].
- Q87706513's child astronomical body is recorded as Q28503932[8].
- Q87706513's catalog code is recorded as Gaia DR2 2129509381668153984[9].
- Q87706513's catalog code is recorded as KIC 10973814[10].
- Q87706513's catalog code is recorded as 2MASS J19234258+4826367[11].
- Q87706513's catalog code is recorded as KOI-1307[12].
- Q87706513's catalog code is recorded as Kepler-287[13].
- Q87706513's catalog code is recorded as Gaia DR3 2129509381668153984[14].
- Q87706513's catalog code is recorded as TIC 417660580[15].
- Q87706513's catalog code is recorded as SPOCS 4158[16].
- Q87706513's type of variable star is recorded as rotating variable star[17].
- Q87706513's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.542'}[18].
- Q87706513's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.73246'}[19].
- Q87706513's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.2'}[20].
- Q87706513's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.13'}[21].
- Q87706513's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.71260566'}[22].
- Q87706513's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.9568379'}[23].
- Q87706513's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2209'}[24].
- Q87706513's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-23.03'}[25].
- Q87706513's metallicity is recorded as {'unit': '1', 'amount': '+0.117'}[26].