Q76562800
star in the constellation Scorpius
Press Enter · cited answer in seconds
0 sources
Q76562800
Summary
Q76562800 is a star[1].
Key Facts
- Q76562800's instance of is recorded as star[2].
- Q76562800's constellation is recorded as Scorpius[3].
- Q76562800's spectral class is recorded as G0[4].
- Q76562800's catalog code is recorded as GSC 07885-00638[5].
- Q76562800's catalog code is recorded as TYC 7885-638-1[6].
- Q76562800's catalog code is recorded as CD-39 11808[7].
- Q76562800's catalog code is recorded as CPD-39 7572[8].
- Q76562800's catalog code is recorded as HD 324282[9].
- Q76562800's catalog code is recorded as Gaia DR1 5961238135233811200[10].
- Q76562800's catalog code is recorded as Gaia DR2 5961238139598598016[11].
- Q76562800's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.73'}[12].
- Q76562800's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.95'}[13].
- Q76562800's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4049'}[14].
- Q76562800's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.9802'}[15].
- Q76562800's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-11.64'}[16].
- Q76562800's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+504.9995'}[17].
- Q76562800's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+266.43982275444190'}[18].
- Q76562800's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-39.09058522994020'}[19].
- Q76562800's epoch is recorded as J2000.0[20].
- Q76562800's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-0.003'}[21].
- Q76562800's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-3.837'}[22].
Body
Definition and Type
Q76562800's instance of is recorded as star[2].