Kepler-385
rotating variable star in the constellation Cygnus
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Kepler-385
Summary
Kepler-385 is a rotating variable star[1].
Key Facts
- Kepler-385's instance of is recorded as rotating variable star[2].
- Kepler-385's instance of is recorded as star[3].
- Kepler-385's instance of is recorded as near-infrared source[4].
- Kepler-385's instance of is recorded as eruptive variable star[5].
- Kepler-385's constellation is recorded as Cygnus[6].
- Kepler-385's child astronomical body is recorded as Q28855456[7].
- Kepler-385's child astronomical body is recorded as Q28855457[8].
- Kepler-385's child astronomical body is recorded as Q75151212[9].
- Kepler-385's child astronomical body is recorded as Kepler-385 h[10].
- Kepler-385's catalog code is recorded as Gaia DR2 2135203000771400320[11].
- Kepler-385's catalog code is recorded as 2MASS J19372123+5020115[12].
- Kepler-385's catalog code is recorded as KIC 11968463[13].
- Kepler-385's catalog code is recorded as Kepler-385[14].
- Kepler-385's catalog code is recorded as KOI-2433[15].
- Kepler-385's catalog code is recorded as UCAC4 702-066659[16].
- Kepler-385's catalog code is recorded as Gaia DR3 2135203000771400320[17].
- Kepler-385's catalog code is recorded as TIC 27082352[18].
- Kepler-385's catalog code is recorded as SPOCS 4271[19].
- Kepler-385's type of variable star is recorded as rotating variable star[20].
- Kepler-385's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.156'}[21].
- Kepler-385's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.851'}[22].
- Kepler-385's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.819'}[23].
- Kepler-385's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.180347'}[24].
- Kepler-385's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.354'}[25].
- Kepler-385's luminosity is recorded as {'unit': 'http://www.wikidata.org/entity/Q843877', 'amount': '+1.3927022'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], star[3], near-infrared source[4], and eruptive variable star[5].