Q83954009
star in the constellation Sagittarius
Press Enter · cited answer in seconds
0 sources
Q83954009
Summary
Q83954009 is a star[1].
Key Facts
- Q83954009's instance of is recorded as star[2].
- Q83954009's constellation is recorded as Sagittarius[3].
- Q83954009's spectral class is recorded as K2III[4].
- Q83954009's catalog code is recorded as BD-20 5034[5].
- Q83954009's catalog code is recorded as CPD-20 6875[6].
- Q83954009's catalog code is recorded as GEN# +1.00166788[7].
- Q83954009's catalog code is recorded as GSC 06276-00987[8].
- Q83954009's catalog code is recorded as HD 166788[9].
- Q83954009's catalog code is recorded as PPM 733779[10].
- Q83954009's catalog code is recorded as TYC 6276-987-1[11].
- Q83954009's catalog code is recorded as UBV M 22723[12].
- Q83954009's catalog code is recorded as 2MASS J18130244-2041053[13].
- Q83954009's catalog code is recorded as RAVE J181302.4-204105[14].
- Q83954009's catalog code is recorded as Gaia DR1 4093998457596418688[15].
- Q83954009's catalog code is recorded as Gaia DR2 4093998457596418688[16].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.477'}[17].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.664'}[18].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.454'}[19].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.014'}[20].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.473'}[21].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.358'}[22].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.070'}[23].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.137'}[24].
- Q83954009's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7752'}[25].
- Q83954009's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.1245'}[26].
Body
Definition and Type
Q83954009's instance of is recorded as star[2].