Q83593262

Summary

Q83593262 is a spectroscopic binary^[1].

Key Facts

• Q83593262's instance of is recorded as spectroscopic binary^[2].
• Q83593262's instance of is recorded as eclipsing binary star^[3].
• Q83593262's instance of is recorded as near-infrared source^[4].
• Q83593262's constellation is recorded as Cygnus^[5].
• Q83593262's spectral class is recorded as A0^[6].
• Q83593262's catalog code is recorded as BD+30 4051^[7].
• Q83593262's catalog code is recorded as GSC 02685-00451^[8].
• Q83593262's catalog code is recorded as HD 332329^[9].
• Q83593262's catalog code is recorded as 2MASS J20291287+3123120^[10].
• Q83593262's catalog code is recorded as Gaia DR1 1861874816806713472^[11].
• Q83593262's catalog code is recorded as Gaia DR2 1861874821120509056^[12].
• Q83593262's catalog code is recorded as V388 Cyg^[13].
• Q83593262's catalog code is recorded as TYC 2685-451-1^[14].
• Q83593262's catalog code is recorded as TIC 408213143^[15].
• Q83593262's catalog code is recorded as Gaia DR3 1861874821120509056^[16].
• Q83593262's type of variable star is recorded as eclipsing binary star^[17].
• Q83593262's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.917'}^[18].
• Q83593262's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.844'}^[19].
• Q83593262's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.798'}^[20].
• Q83593262's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.59'}^[21].
• Q83593262's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.82'}^[22].
• Q83593262's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.635899'}^[23].
• Q83593262's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.0154'}^[24].
• Q83593262's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+496.179'}^[25].
• Q83593262's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+307.30367999962'}^[26].

Body

Definition and Type

Recorded instance of include spectroscopic binary^[2], eclipsing binary star^[3], and near-infrared source^[4].