Q85408106
long period variable
Press Enter · cited answer in seconds
0 sources
Q85408106
Summary
Q85408106 is a long-period variable star[1].
Key Facts
- Q85408106's instance of is recorded as long-period variable star[2].
- Q85408106's constellation is recorded as Vulpecula[3].
- Q85408106's catalog code is recorded as AN 133.1905[4].
- Q85408106's catalog code is recorded as 2MASS J19545276+2004346[5].
- Q85408106's catalog code is recorded as Gaia DR2 1826256210686941184[6].
- Q85408106's catalog code is recorded as CY Vul[7].
- Q85408106's type of variable star is recorded as slow irregular variables of late spectral types[8].
- Q85408106's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.756'}[9].
- Q85408106's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.906'}[10].
- Q85408106's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.626'}[11].
- Q85408106's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.6146'}[12].
- Q85408106's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4689'}[13].
- Q85408106's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-12.63'}[14].
- Q85408106's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2132.6509'}[15].
- Q85408106's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+298.71984700624820'}[16].
- Q85408106's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+20.07631602767390'}[17].
- Q85408106's epoch is recorded as J2000.0[18].
- Q85408106's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-10.364'}[19].
- Q85408106's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-4.451'}[20].
Body
Definition and Type
Q85408106's instance of is recorded as long-period variable star[2].