Q91073347
rotating variable star in the constellation Cygnus
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Q91073347
Summary
Q91073347 is a rotating variable star[1].
Key Facts
- Q91073347's instance of is recorded as rotating variable star[2].
- Q91073347's constellation is recorded as Cygnus[3].
- Q91073347's spectral class is recorded as F3V[4].
- Q91073347's spectral class is recorded as F5/F6IV/V[5].
- Q91073347's catalog code is recorded as AG+39 2008[6].
- Q91073347's catalog code is recorded as BD+39 3907[7].
- Q91073347's catalog code is recorded as GSC 03140-00011[8].
- Q91073347's catalog code is recorded as HD 225754[9].
- Q91073347's catalog code is recorded as 2MASS J19463128+3923362[10].
- Q91073347's catalog code is recorded as PPM 83519[11].
- Q91073347's catalog code is recorded as SAO 68837[12].
- Q91073347's catalog code is recorded as TYC 3140-11-1[13].
- Q91073347's catalog code is recorded as KIC 4284968[14].
- Q91073347's catalog code is recorded as Gaia DR1 2073285407905120128[15].
- Q91073347's catalog code is recorded as Gaia DR2 2073285412215224832[16].
- Q91073347's type of variable star is recorded as rotating variable star[17].
- Q91073347's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.238'}[18].
- Q91073347's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.199'}[19].
- Q91073347's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.199'}[20].
- Q91073347's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.61'}[21].
- Q91073347's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.1090'}[22].
- Q91073347's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+5.4619'}[23].
- Q91073347's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+7.10'}[24].
- Q91073347's metallicity is recorded as {'unit': '1', 'amount': '-0.01'}[25].
- Q91073347's metallicity is recorded as {'unit': '1', 'amount': '-0.12'}[26].
Body
Definition and Type
Q91073347's instance of is recorded as rotating variable star[2].