Q94488484
rotating variable star in the constellation Cygnus
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Q94488484
Summary
Q94488484 is a rotating variable star[1].
Key Facts
- Q94488484's instance of is recorded as rotating variable star[2].
- Q94488484's instance of is recorded as star[3].
- Q94488484's instance of is recorded as near-infrared source[4].
- Q94488484's constellation is recorded as Cygnus[5].
- Q94488484's child astronomical body is recorded as Q28855416[6].
- Q94488484's child astronomical body is recorded as Q28855414[7].
- Q94488484's child astronomical body is recorded as Q75152117[8].
- Q94488484's catalog code is recorded as Gaia DR2 2053578521704124160[9].
- Q94488484's catalog code is recorded as KIC 5706595[10].
- Q94488484's catalog code is recorded as 2MASS J19284107+4054587[11].
- Q94488484's catalog code is recorded as KOI-2183[12].
- Q94488484's catalog code is recorded as Gaia DR3 2053578521704124160[13].
- Q94488484's catalog code is recorded as TIC 137411225[14].
- Q94488484's catalog code is recorded as SPOCS 3508[15].
- Q94488484's catalog code is recorded as Kepler-370[16].
- Q94488484's type of variable star is recorded as rotating variable star[17].
- Q94488484's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.977'}[18].
- Q94488484's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.65'}[19].
- Q94488484's apparent magnitude is recorded as {'unit': '1', 'amount': '+13.550'}[20].
- Q94488484's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.146945'}[21].
- Q94488484's mass is recorded as {'unit': 'http://www.wikidata.org/entity/Q180892', 'amount': '+0.968'}[22].
- Q94488484's radius is recorded as {'unit': 'http://www.wikidata.org/entity/Q48440', 'amount': '+0.9'}[23].
- Q94488484's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.873'}[24].
- Q94488484's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-35.2523'}[25].
- Q94488484's metallicity is recorded as {'unit': '1', 'amount': '+0.054'}[26].