Q89041722

Summary

Q89041722 is a high proper-motion star^[1].

Key Facts

• Q89041722's instance of is recorded as high proper-motion star^[2].
• Q89041722's constellation is recorded as Sagittarius^[3].
• Q89041722's spectral class is recorded as F7V^[4].
• Q89041722's catalog code is recorded as CD-26 14200^[5].
• Q89041722's catalog code is recorded as CPD-26 6769^[6].
• Q89041722's catalog code is recorded as GSC 06880-01192^[7].
• Q89041722's catalog code is recorded as HD 182817^[8].
• Q89041722's catalog code is recorded as PPM 269805^[9].
• Q89041722's catalog code is recorded as SAO 188143^[10].
• Q89041722's catalog code is recorded as TYC 6880-1192-1^[11].
• Q89041722's catalog code is recorded as YZ 116 13541^[12].
• Q89041722's catalog code is recorded as 2MASS J19272953-2612266^[13].
• Q89041722's catalog code is recorded as Gaia DR1 6766392289592267136^[14].
• Q89041722's catalog code is recorded as Gaia DR2 6766392293891632896^[15].
• Q89041722's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.62'}^[16].
• Q89041722's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.08'}^[17].
• Q89041722's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.987'}^[18].
• Q89041722's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.712'}^[19].
• Q89041722's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.608'}^[20].
• Q89041722's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9312'}^[21].
• Q89041722's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+11.4556'}^[22].
• Q89041722's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-21.48'}^[23].
• Q89041722's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+87.2936'}^[24].
• Q89041722's SIMBAD ID is recorded as HD 182817^[25].
• Q89041722's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+291.87305413090150'}^[26].