Q90616601
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Q90616601
Summary
Q90616601 is a near-infrared source[1].
Key Facts
- Q90616601's instance of is recorded as near-infrared source[2].
- Q90616601's instance of is recorded as variable star[3].
- Q90616601's constellation is recorded as Cepheus[4].
- Q90616601's spectral class is recorded as OB[5].
- Q90616601's catalog code is recorded as CSV 5748[6].
- Q90616601's catalog code is recorded as GSC 04288-01103[7].
- Q90616601's catalog code is recorded as 2MASS J23320546+6400534[8].
- Q90616601's catalog code is recorded as Gaia DR1 2016941209418011136[9].
- Q90616601's catalog code is recorded as Gaia DR2 2016941213716159744[10].
- Q90616601's catalog code is recorded as DY Cep[11].
- Q90616601's catalog code is recorded as Gaia DR3 2016941213716159744[12].
- Q90616601's catalog code is recorded as TYC 4288-1103-1[13].
- Q90616601's catalog code is recorded as ALS 12997[14].
- Q90616601's catalog code is recorded as TIC 270665642[15].
- Q90616601's type of variable star is recorded as eclipsing binary star[16].
- Q90616601's type of variable star is recorded as Beta Lyrae variable[17].
- Q90616601's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.18'}[18].
- Q90616601's apparent magnitude is recorded as {'unit': '1', 'amount': '+12.86'}[19].
- Q90616601's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.348'}[20].
- Q90616601's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.13'}[21].
- Q90616601's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.983'}[22].
- Q90616601's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.726711'}[23].
- Q90616601's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.4572'}[24].
- Q90616601's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+2187.227'}[25].
- Q90616601's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+353.02279404472'}[26].
Body
Definition and Type
Recorded instance of include near-infrared source[2] and variable star[3].