Q86652067
high proper-motion star in the constellation Capricornus
Press Enter · cited answer in seconds
0 sources
Q86652067
Summary
Q86652067 is a high proper-motion star[1].
Key Facts
- Q86652067's instance of is recorded as high proper-motion star[2].
- Q86652067's constellation is recorded as Capricornus[3].
- Q86652067's spectral class is recorded as G2V[4].
- Q86652067's catalog code is recorded as BD-19 5932[5].
- Q86652067's catalog code is recorded as CPD-19 7912[6].
- Q86652067's catalog code is recorded as GSC 06352-00344[7].
- Q86652067's catalog code is recorded as HD 198395[8].
- Q86652067's catalog code is recorded as LTT 8249[9].
- Q86652067's catalog code is recorded as NLTT 49976[10].
- Q86652067's catalog code is recorded as PPM 722262[11].
- Q86652067's catalog code is recorded as TYC 6352-344-1[12].
- Q86652067's catalog code is recorded as 2MASS J20503537-1858519[13].
- Q86652067's catalog code is recorded as RAVE J205035.4-185852[14].
- Q86652067's catalog code is recorded as USNO-B1.0 0710-00809579[15].
- Q86652067's catalog code is recorded as DENIS J205035.3-185852[16].
- Q86652067's catalog code is recorded as Gaia DR1 6858457593641053824[17].
- Q86652067's catalog code is recorded as Gaia DR2 6858457597937161088[18].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.619'}[19].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.284'}[20].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.268'}[21].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.115'}[22].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.5'}[23].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.358'}[24].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.741'}[25].
- Q86652067's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.203'}[26].
Body
Definition and Type
Q86652067's instance of is recorded as high proper-motion star[2].