Q93767684
star in the constellation Perseus
Press Enter · cited answer in seconds
0 sources
Q93767684
Summary
Q93767684 is a star[1].
Key Facts
- Q93767684's instance of is recorded as star[2].
- Q93767684's constellation is recorded as Perseus[3].
- Q93767684's spectral class is recorded as B[4].
- Q93767684's catalog code is recorded as 2MASS J02274481+5851475[5].
- Q93767684's catalog code is recorded as GSC 03699-00274[6].
- Q93767684's catalog code is recorded as [VGK85] IC 1805 +58 33[7].
- Q93767684's catalog code is recorded as Gaia DR2 459023839486023040[8].
- Q93767684's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.9'}[9].
- Q93767684's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.598'}[10].
- Q93767684's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.245'}[11].
- Q93767684's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.175'}[12].
- Q93767684's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.7067'}[13].
- Q93767684's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.7130'}[14].
- Q93767684's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+6.41'}[15].
- Q93767684's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+212.1791'}[16].
- Q93767684's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+36.93675795310490'}[17].
- Q93767684's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+58.86318346474330'}[18].
- Q93767684's epoch is recorded as J2000.0[19].
- Q93767684's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-9.307'}[20].
- Q93767684's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '+17.490'}[21].
Body
Definition and Type
Q93767684's instance of is recorded as star[2].