Q85616936
star in the constellation Draco
Press Enter · cited answer in seconds
0 sources
Q85616936
Summary
Q85616936 is a star[1].
Key Facts
- Q85616936's instance of is recorded as star[2].
- Q85616936's constellation is recorded as Draco[3].
- Q85616936's spectral class is recorded as G5[4].
- Q85616936's catalog code is recorded as AG+74 342[5].
- Q85616936's catalog code is recorded as AGKR 11494[6].
- Q85616936's catalog code is recorded as BD+75 486[7].
- Q85616936's catalog code is recorded as GSC 04407-00090[8].
- Q85616936's catalog code is recorded as HD 111716[9].
- Q85616936's catalog code is recorded as HIC 62598[10].
- Q85616936's catalog code is recorded as HIP 62598[11].
- Q85616936's catalog code is recorded as PPM 8266[12].
- Q85616936's catalog code is recorded as SAO 7673[13].
- Q85616936's catalog code is recorded as TYC 4407-90-1[14].
- Q85616936's catalog code is recorded as 2MASS J12493727+7412581[15].
- Q85616936's catalog code is recorded as Gaia DR1 1691535692293335680[16].
- Q85616936's catalog code is recorded as Gaia DR2 1691535692293335680[17].
- Q85616936's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.98'}[18].
- Q85616936's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.837'}[19].
- Q85616936's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.554'}[20].
- Q85616936's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.499'}[21].
- Q85616936's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.66'}[22].
- Q85616936's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.8603'}[23].
- Q85616936's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.2631'}[24].
- Q85616936's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-10.94'}[25].
- Q85616936's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+75.3972'}[26].
Body
Definition and Type
Q85616936's instance of is recorded as star[2].