Q88994676
star in the constellation Scorpius
Press Enter · cited answer in seconds
0 sources
Q88994676
Summary
Q88994676 is a star[1].
Key Facts
- Q88994676's instance of is recorded as star[2].
- Q88994676's constellation is recorded as Scorpius[3].
- Q88994676's spectral class is recorded as K2III[4].
- Q88994676's catalog code is recorded as CD-28 11690[5].
- Q88994676's catalog code is recorded as CPD-28 5228[6].
- Q88994676's catalog code is recorded as GSC 06791-01348[7].
- Q88994676's catalog code is recorded as HD 142406[8].
- Q88994676's catalog code is recorded as HIC 77988[9].
- Q88994676's catalog code is recorded as HIP 77988[10].
- Q88994676's catalog code is recorded as PPM 264866[11].
- Q88994676's catalog code is recorded as SAO 183930[12].
- Q88994676's catalog code is recorded as SRS 13239[13].
- Q88994676's catalog code is recorded as TYC 6791-1348-1[14].
- Q88994676's catalog code is recorded as YZ 119 9986[15].
- Q88994676's catalog code is recorded as 2MASS J15553193-2911252[16].
- Q88994676's catalog code is recorded as Gaia DR2 6041103468722632192[17].
- Q88994676's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.957'}[18].
- Q88994676's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.435'}[19].
- Q88994676's apparent magnitude is recorded as {'unit': '1', 'amount': '+5.227'}[20].
- Q88994676's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.03'}[21].
- Q88994676's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.33'}[22].
- Q88994676's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.6914'}[23].
- Q88994676's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+4.1411'}[24].
- Q88994676's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-1.86'}[25].
- Q88994676's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+241.4817'}[26].
Body
Definition and Type
Q88994676's instance of is recorded as star[2].