Q88878785
high proper-motion star in the constellation Corona Australis
Press Enter · cited answer in seconds
0 sources
Q88878785
Summary
Q88878785 is a high proper-motion star[1].
Key Facts
- Q88878785's instance of is recorded as high proper-motion star[2].
- Q88878785's constellation is recorded as Corona Australis[3].
- Q88878785's spectral class is recorded as G3V[4].
- Q88878785's catalog code is recorded as CCDM J19021-3917AB[5].
- Q88878785's catalog code is recorded as CD-39 13077[6].
- Q88878785's catalog code is recorded as CPC 18 9853[7].
- Q88878785's catalog code is recorded as CPD-39 8263[8].
- Q88878785's catalog code is recorded as GSC 07917-02535[9].
- Q88878785's catalog code is recorded as HD 176460[10].
- Q88878785's catalog code is recorded as HIC 93465[11].
- Q88878785's catalog code is recorded as HIP 93465[12].
- Q88878785's catalog code is recorded as IDS 18552-3926 AB[13].
- Q88878785's catalog code is recorded as PPM 298461[14].
- Q88878785's catalog code is recorded as SAO 210838[15].
- Q88878785's catalog code is recorded as TYC 7917-2535-1[16].
- Q88878785's catalog code is recorded as 2MASS J19020609-3917254[17].
- Q88878785's catalog code is recorded as WDS J19021-3917AB[18].
- Q88878785's catalog code is recorded as uvby98 100176460[19].
- Q88878785's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.319'}[20].
- Q88878785's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.033'}[21].
- Q88878785's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.958'}[22].
- Q88878785's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.54'}[23].
- Q88878785's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.18'}[24].
- Q88878785's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.52'}[25].
- Q88878785's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-5.20'}[26].
Body
Definition and Type
Q88878785's instance of is recorded as high proper-motion star[2].