Q66612841

Summary

Q66612841 is an infrared source^[1].

Key Facts

• Q66612841's instance of is recorded as infrared source^[2].
• Q66612841's instance of is recorded as high proper-motion star^[3].
• Q66612841's spectral class is recorded as F5V^[4].
• Q66612841's catalog code is recorded as HD 203555^[5].
• Q66612841's catalog code is recorded as CPC 0 19364^[6].
• Q66612841's catalog code is recorded as GSC 07983-00639^[7].
• Q66612841's catalog code is recorded as HIC 105656^[8].
• Q66612841's catalog code is recorded as HIP 105656^[9].
• Q66612841's catalog code is recorded as 2MASS J21240364-4001484^[10].
• Q66612841's catalog code is recorded as PPM 327157^[11].
• Q66612841's catalog code is recorded as SAO 230662^[12].
• Q66612841's catalog code is recorded as TD1 28010^[13].
• Q66612841's catalog code is recorded as uvby98 100203555^[14].
• Q66612841's catalog code is recorded as Gaia DR1 6582251957686814720^[15].
• Q66612841's catalog code is recorded as TYC 7983-639-1^[16].
• Q66612841's catalog code is recorded as Gaia DR2 6582251961983723392^[17].
• Q66612841's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.76'}^[18].
• Q66612841's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.35'}^[19].
• Q66612841's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.2392'}^[20].
• Q66612841's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.524'}^[21].
• Q66612841's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.374'}^[22].
• Q66612841's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.299'}^[23].
• Q66612841's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+13.7906'}^[24].
• Q66612841's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-21.00'}^[25].
• Q66612841's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+72.5132'}^[26].

Body

Definition and Type

Recorded instance of include infrared source^[2] and high proper-motion star^[3].