Q76553519
emission-line star in the constellation Scorpius
Press Enter · cited answer in seconds
0 sources
Q76553519
Summary
Q76553519 is an emission-line star[1].
Key Facts
- Q76553519's instance of is recorded as emission-line star[2].
- Q76553519's constellation is recorded as Scorpius[3].
- Q76553519's spectral class is recorded as K7[4].
- Q76553519's catalog code is recorded as CD-36 11382[5].
- Q76553519's catalog code is recorded as CPC 18 8614[6].
- Q76553519's catalog code is recorded as CPD-36 7222[7].
- Q76553519's catalog code is recorded as GSC 07374-00413[8].
- Q76553519's catalog code is recorded as HD 319637[9].
- Q76553519's catalog code is recorded as PPM 296133[10].
- Q76553519's catalog code is recorded as SAO 208622[11].
- Q76553519's catalog code is recorded as THA 10-10[12].
- Q76553519's catalog code is recorded as TYC 7374-413-1[13].
- Q76553519's catalog code is recorded as UCAC2 16438788[14].
- Q76553519's catalog code is recorded as 2MASS J17170500-3612182[15].
- Q76553519's catalog code is recorded as SSTGLMC G350.6297+01.0334[16].
- Q76553519's catalog code is recorded as Gaia DR1 5975449975856984064[17].
- Q76553519's catalog code is recorded as Gaia DR2 5975449980158859648[18].
- Q76553519's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.154'}[19].
- Q76553519's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.411'}[20].
- Q76553519's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.153'}[21].
- Q76553519's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.43'}[22].
- Q76553519's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.17'}[23].
- Q76553519's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.7027'}[24].
- Q76553519's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+2.5693'}[25].
- Q76553519's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+8.07'}[26].
Body
Definition and Type
Q76553519's instance of is recorded as emission-line star[2].