Q85687361
rotating variable star in the constellation Lyra
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Q85687361
Summary
Q85687361 is a rotating variable star[1].
Key Facts
- Q85687361's instance of is recorded as rotating variable star[2].
- Q85687361's instance of is recorded as star[3].
- Q85687361's instance of is recorded as near-infrared source[4].
- Q85687361's constellation is recorded as Lyra[5].
- Q85687361's child astronomical body is recorded as Q28855483[6].
- Q85687361's child astronomical body is recorded as Q28855484[7].
- Q85687361's child astronomical body is recorded as Q28855485[8].
- Q85687361's catalog code is recorded as Gaia DR2 2053457644144430848[9].
- Q85687361's catalog code is recorded as KIC 5185897[10].
- Q85687361's catalog code is recorded as 2MASS J19255247+4020378[11].
- Q85687361's catalog code is recorded as KOI-2693[12].
- Q85687361's catalog code is recorded as Kepler-398[13].
- Q85687361's catalog code is recorded as Gaia DR3 2053457644144430848[14].
- Q85687361's catalog code is recorded as TIC 137155210[15].
- Q85687361's type of variable star is recorded as rotating variable star[16].
- Q85687361's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.514'}[17].
- Q85687361's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.932'}[18].
- Q85687361's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.794'}[19].
- Q85687361's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.222908'}[20].
- Q85687361's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+0.15100943'}[21].
- Q85687361's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.62371653'}[22].
- Q85687361's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.6335'}[23].
- Q85687361's metallicity is recorded as {'unit': '1', 'amount': '-0.04'}[24].
- Q85687361's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+177.51'}[25].
- Q85687361's SIMBAD ID is recorded as Kepler-398[26].