Q66650237

Summary

Q66650237 is a high proper-motion star^[1].

Key Facts

• Q66650237's instance of is recorded as high proper-motion star^[2].
• Q66650237's spectral class is recorded as F3IV/V^[3].
• Q66650237's catalog code is recorded as HD 177345^[4].
• Q66650237's catalog code is recorded as CPC 21 4446^[5].
• Q66650237's catalog code is recorded as GSC 09079-00046^[6].
• Q66650237's catalog code is recorded as HIC 94063^[7].
• Q66650237's catalog code is recorded as HIP 94063^[8].
• Q66650237's catalog code is recorded as 2MASS J19085716-6532007^[9].
• Q66650237's catalog code is recorded as PPM 363790^[10].
• Q66650237's catalog code is recorded as SAO 254471^[11].
• Q66650237's catalog code is recorded as uvby98 100177345^[12].
• Q66650237's catalog code is recorded as Gaia DR1 6435179770526465792^[13].
• Q66650237's catalog code is recorded as TYC 9079-46-1^[14].
• Q66650237's catalog code is recorded as Gaia DR2 6435179774825284096^[15].
• Q66650237's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.93'}^[16].
• Q66650237's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.54'}^[17].
• Q66650237's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.4428'}^[18].
• Q66650237's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.796'}^[19].
• Q66650237's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.687'}^[20].
• Q66650237's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.601'}^[21].
• Q66650237's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+9.6177'}^[22].
• Q66650237's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-23.53'}^[23].
• Q66650237's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+103.9750'}^[24].
• Q66650237's SIMBAD ID is recorded as HD 177345^[25].
• Q66650237's right ascension is recorded as {'unit': 'http://www.wikidata.org/entity/Q28390', 'amount': '+287.23813549046550'}^[26].