Q88083966
star in the constellation Scorpius
Press Enter · cited answer in seconds
0 sources
Q88083966
Summary
Q88083966 is a star[1].
Key Facts
- Q88083966's instance of is recorded as star[2].
- Q88083966's constellation is recorded as Scorpius[3].
- Q88083966's spectral class is recorded as K5[4].
- Q88083966's catalog code is recorded as GSC 07385-00013[5].
- Q88083966's catalog code is recorded as TYC 7385-13-1[6].
- Q88083966's catalog code is recorded as CD-34 11978[7].
- Q88083966's catalog code is recorded as CPD-34 6989[8].
- Q88083966's catalog code is recorded as HD 320431[9].
- Q88083966's catalog code is recorded as Gaia DR1 4053427406246266624[10].
- Q88083966's catalog code is recorded as Gaia DR2 4053427410643655040[11].
- Q88083966's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.08'}[12].
- Q88083966's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.84'}[13].
- Q88083966's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.3780'}[14].
- Q88083966's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.2260'}[15].
- Q88083966's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+32.37'}[16].
- Q88083966's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+815.6607'}[17].
- Q88083966's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+265.70746612237360'}[18].
- Q88083966's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-34.23899374942920'}[19].
- Q88083966's epoch is recorded as J2000.0[20].
- Q88083966's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.206'}[21].
- Q88083966's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+4.851'}[22].
Body
Definition and Type
Q88083966's instance of is recorded as star[2].