Q66654237
Press Enter · cited answer in seconds
0 sources
Q66654237
Summary
Q66654237 is a star[1].
Key Facts
- Q66654237's instance of is recorded as star[2].
- Q66654237's instance of is recorded as infrared source[3].
- Q66654237's spectral class is recorded as F6V[4].
- Q66654237's catalog code is recorded as HD 44642[5].
- Q66654237's catalog code is recorded as GSC 06518-01251[6].
- Q66654237's catalog code is recorded as HIC 30223[7].
- Q66654237's catalog code is recorded as HIP 30223[8].
- Q66654237's catalog code is recorded as 2MASS J06213119-2909023[9].
- Q66654237's catalog code is recorded as PPM 250259[10].
- Q66654237's catalog code is recorded as SAO 171623[11].
- Q66654237's catalog code is recorded as TD1 6924[12].
- Q66654237's catalog code is recorded as uvby98 100044642[13].
- Q66654237's catalog code is recorded as YZ 119 2913[14].
- Q66654237's catalog code is recorded as TYC 6518-1251-1[15].
- Q66654237's catalog code is recorded as Gaia DR1 2898166140893152128[16].
- Q66654237's catalog code is recorded as Gaia DR2 2898166145191649792[17].
- Q66654237's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.21'}[18].
- Q66654237's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.71'}[19].
- Q66654237's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.5795'}[20].
- Q66654237's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.725'}[21].
- Q66654237's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.480'}[22].
- Q66654237's apparent magnitude is recorded as {'unit': '1', 'amount': '+6.406'}[23].
- Q66654237's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+15.0998'}[24].
- Q66654237's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '+66.01'}[25].
- Q66654237's distance from Earth is recorded as {'unit': 'http://www.wikidata.org/entity/Q12129', 'amount': '+66.2260'}[26].
Body
Definition and Type
Recorded instance of include star[2] and infrared source[3].