Q83755044
star in the constellation Centaurus
Press Enter · cited answer in seconds
0 sources
Q83755044
Summary
Q83755044 is a star[1].
Key Facts
- Q83755044's instance of is recorded as star[2].
- Q83755044's constellation is recorded as Centaurus[3].
- Q83755044's spectral class is recorded as K1III[4].
- Q83755044's catalog code is recorded as CD-35 8726[5].
- Q83755044's catalog code is recorded as CPC 18 6470[6].
- Q83755044's catalog code is recorded as CPD-35 5777[7].
- Q83755044's catalog code is recorded as GSC 07276-00441[8].
- Q83755044's catalog code is recorded as HD 117085[9].
- Q83755044's catalog code is recorded as HIC 65738[10].
- Q83755044's catalog code is recorded as HIP 65738[11].
- Q83755044's catalog code is recorded as PPM 291428[12].
- Q83755044's catalog code is recorded as SAO 204504[13].
- Q83755044's catalog code is recorded as SRS 11652[14].
- Q83755044's catalog code is recorded as TYC 7276-441-1[15].
- Q83755044's catalog code is recorded as 2MASS J13283219-3542554[16].
- Q83755044's catalog code is recorded as Gaia DR2 6166175493354583040[17].
- Q83755044's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.968'}[18].
- Q83755044's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.412'}[19].
- Q83755044's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.264'}[20].
- Q83755044's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.92'}[21].
- Q83755044's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.15'}[22].
- Q83755044's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.6109'}[23].
- Q83755044's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.6394'}[24].
- Q83755044's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-5.41'}[25].
- Q83755044's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+378.8740'}[26].
Body
Definition and Type
Q83755044's instance of is recorded as star[2].