Q88795980
high proper-motion star in the constellation Sagittarius
Press Enter · cited answer in seconds
0 sources
Q88795980
Summary
Q88795980 is a high proper-motion star[1].
Key Facts
- Q88795980's instance of is recorded as high proper-motion star[2].
- Q88795980's constellation is recorded as Sagittarius[3].
- Q88795980's spectral class is recorded as G3V[4].
- Q88795980's catalog code is recorded as CD-32 15143[5].
- Q88795980's catalog code is recorded as CPC 17 10579[6].
- Q88795980's catalog code is recorded as CPD-32 5910[7].
- Q88795980's catalog code is recorded as GSC 07428-00081[8].
- Q88795980's catalog code is recorded as HD 182137[9].
- Q88795980's catalog code is recorded as HIC 95420[10].
- Q88795980's catalog code is recorded as HIP 95420[11].
- Q88795980's catalog code is recorded as PPM 298952[12].
- Q88795980's catalog code is recorded as SAO 211240[13].
- Q88795980's catalog code is recorded as TYC 7428-81-1[14].
- Q88795980's catalog code is recorded as 2MASS J19243560-3155294[15].
- Q88795980's catalog code is recorded as WISEA J192435.64-315531.2[16].
- Q88795980's catalog code is recorded as Gaia DR2 6745797444672234368[17].
- Q88795980's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.301'}[18].
- Q88795980's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.980'}[19].
- Q88795980's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.994'}[20].
- Q88795980's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.66'}[21].
- Q88795980's apparent magnitude is recorded as {'unit': '1', 'amount': '+10.31'}[22].
- Q88795980's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.4068'}[23].
- Q88795980's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+12.6337'}[24].
- Q88795980's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-19.93'}[25].
- Q88795980's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+79.1534'}[26].