Q86844151
rotating variable star in the constellation Lyra
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Q86844151
Summary
Q86844151 is a rotating variable star[1].
Key Facts
- Q86844151's instance of is recorded as rotating variable star[2].
- Q86844151's instance of is recorded as high proper-motion star[3].
- Q86844151's instance of is recorded as near-infrared source[4].
- Q86844151's instance of is recorded as eruptive variable star[5].
- Q86844151's constellation is recorded as Lyra[6].
- Q86844151's spectral class is recorded as M2V[7].
- Q86844151's child astronomical body is recorded as Q28855926[8].
- Q86844151's child astronomical body is recorded as Q28855927[9].
- Q86844151's catalog code is recorded as Gaia DR2 2107406178588473728[10].
- Q86844151's catalog code is recorded as 2MASS J18545568+4557315[11].
- Q86844151's catalog code is recorded as KIC 9388479[12].
- Q86844151's catalog code is recorded as Kepler-732[13].
- Q86844151's catalog code is recorded as KOI-936[14].
- Q86844151's catalog code is recorded as UCAC4 680-065588[15].
- Q86844151's catalog code is recorded as Gaia DR3 2107406178588473728[16].
- Q86844151's catalog code is recorded as TIC 164555597[17].
- Q86844151's type of variable star is recorded as rotating variable star[18].
- Q86844151's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.596'}[19].
- Q86844151's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.952'}[20].
- Q86844151's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.721'}[21].
- Q86844151's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.033778'}[22].
- Q86844151's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.624'}[23].
- Q86844151's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.49'}[24].
- Q86844151's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.46'}[25].
- Q86844151's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.7682'}[26].
Body
Definition and Type
Recorded instance of include rotating variable star[2], high proper-motion star[3], near-infrared source[4], and eruptive variable star[5].