Q66492911
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Q66492911
Summary
Q66492911 is a high proper-motion star[1].
Key Facts
- Q66492911's instance of is recorded as high proper-motion star[2].
- Q66492911's spectral class is recorded as K2[3].
- Q66492911's catalog code is recorded as HD 192168[4].
- Q66492911's catalog code is recorded as GSC 01081-01635[5].
- Q66492911's catalog code is recorded as HIC 99623[6].
- Q66492911's catalog code is recorded as HIP 99623[7].
- Q66492911's catalog code is recorded as IRAS 20106+1141[8].
- Q66492911's catalog code is recorded as 2MASS J20130313+1151029[9].
- Q66492911's catalog code is recorded as PPM 137892[10].
- Q66492911's catalog code is recorded as SAO 105843[11].
- Q66492911's catalog code is recorded as YZ 11 7784[12].
- Q66492911's catalog code is recorded as AG+11 2445[13].
- Q66492911's catalog code is recorded as BD+11 4180[14].
- Q66492911's catalog code is recorded as TYC 1081-1635-1[15].
- Q66492911's catalog code is recorded as Gaia DR2 1802747243295833216[16].
- Q66492911's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.72'}[17].
- Q66492911's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.51'}[18].
- Q66492911's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.1595'}[19].
- Q66492911's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.795'}[20].
- Q66492911's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.982'}[21].
- Q66492911's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.929'}[22].
- Q66492911's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+7.1893'}[23].
- Q66492911's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+10.85'}[24].
- Q66492911's metallicity is recorded as {'unit': '1', 'amount': '+0.00'}[25].
- Q66492911's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+139.0956'}[26].
Body
Definition and Type
Q66492911's instance of is recorded as high proper-motion star[2].