Q87468779
hot subdwarf star in the constellation Capricornus
Press Enter · cited answer in seconds
0 sources
Q87468779
Summary
Q87468779 is a hot subdwarf star[1].
Key Facts
- Q87468779's instance of is recorded as hot subdwarf star[2].
- Q87468779's constellation is recorded as Capricornus[3].
- Q87468779's spectral class is recorded as sdOHe[4].
- Q87468779's catalog code is recorded as BPS CS 22950-0048[5].
- Q87468779's catalog code is recorded as 2MASS J20202771-1308374[6].
- Q87468779's catalog code is recorded as Gaia DR2 6879812999968424320[7].
- Q87468779's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.433'}[8].
- Q87468779's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.348'}[9].
- Q87468779's apparent magnitude is recorded as {'unit': '1', 'amount': '+15.684'}[10].
- Q87468779's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.9'}[11].
- Q87468779's apparent magnitude is recorded as {'unit': '1', 'amount': '+14.8431'}[12].
- Q87468779's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6110'}[13].
- Q87468779's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+150'}[14].
- Q87468779's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+1636.6612'}[15].
- Q87468779's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+305.11545856949400'}[16].
- Q87468779's declination is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '-13.14375510964390'}[17].
- Q87468779's epoch is recorded as J2000.0[18].
- Q87468779's declination component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-13.097'}[19].
- Q87468779's right ascension component of proper motion is recorded as {'unit': 'http://www.wikidata.org/entity/Q22137107', 'amount': '-8.697'}[20].
Body
Definition and Type
Q87468779's instance of is recorded as hot subdwarf star[2].