Q88403757
star in the constellation Pavo
Press Enter · cited answer in seconds
0 sources
Q88403757
Summary
Q88403757 is a star[1].
Key Facts
- Q88403757's instance of is recorded as star[2].
- Q88403757's constellation is recorded as Pavo[3].
- Q88403757's spectral class is recorded as K4/5III[4].
- Q88403757's catalog code is recorded as CD-72 1551[5].
- Q88403757's catalog code is recorded as CPC 21.1 3805[6].
- Q88403757's catalog code is recorded as CPD-72 2419[7].
- Q88403757's catalog code is recorded as GSC 09314-00316[8].
- Q88403757's catalog code is recorded as HD 184974[9].
- Q88403757's catalog code is recorded as HIC 97027[10].
- Q88403757's catalog code is recorded as HIP 97027[11].
- Q88403757's catalog code is recorded as IRAS 19374-7159[12].
- Q88403757's catalog code is recorded as PPM 374326[13].
- Q88403757's catalog code is recorded as SRS 20124[14].
- Q88403757's catalog code is recorded as TYC 9314-316-1[15].
- Q88403757's catalog code is recorded as 2MASS J19430844-7152238[16].
- Q88403757's catalog code is recorded as Gaia DR2 6416435197515244288[17].
- Q88403757's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.255'}[18].
- Q88403757's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.507'}[19].
- Q88403757's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.242'}[20].
- Q88403757's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.21'}[21].
- Q88403757's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.85'}[22].
- Q88403757's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.5497'}[23].
- Q88403757's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+1.5909'}[24].
- Q88403757's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+19.05'}[25].
- Q88403757's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+628.5750'}[26].
Body
Definition and Type
Q88403757's instance of is recorded as star[2].