Q80127880
star in the constellation Lepus
Press Enter · cited answer in seconds
0 sources
Q80127880
Summary
Q80127880 is a star[1].
Key Facts
- Q80127880's instance of is recorded as star[2].
- Q80127880's constellation is recorded as Lepus[3].
- Q80127880's spectral class is recorded as F8V[4].
- Q80127880 is part of AB Doradus Moving Group[5].
- Q80127880's catalog code is recorded as 2MASS J05062769-1549303[6].
- Q80127880's catalog code is recorded as BD-16 1042[7].
- Q80127880's catalog code is recorded as GSC 05901-01109[8].
- Q80127880's catalog code is recorded as HD 32981[9].
- Q80127880's catalog code is recorded as PPM 215289[10].
- Q80127880's catalog code is recorded as SAO 150148[11].
- Q80127880's catalog code is recorded as TYC 5901-1109-1[12].
- Q80127880's catalog code is recorded as YZ 105 1444[13].
- Q80127880's catalog code is recorded as 1RXS J050627.8-154923[14].
- Q80127880's catalog code is recorded as ASAS J050628-1549.5[15].
- Q80127880's catalog code is recorded as RAVE J050627.7-154930[16].
- Q80127880's catalog code is recorded as Gaia DR1 2986060653741078784[17].
- Q80127880's catalog code is recorded as Gaia DR2 2986060653741078784[18].
- Q80127880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.029'}[19].
- Q80127880's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.813'}[20].
- Q80127880's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.743'}[21].
- Q80127880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.46'}[22].
- Q80127880's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.12'}[23].
- Q80127880's apparent magnitude is recorded as {'unit': '1', 'amount': '+9.75'}[24].
- Q80127880's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.9194'}[25].
- Q80127880's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+11.7544'}[26].
Body
Definition and Type
Q80127880's instance of is recorded as star[2].
Use and Application
Q80127880 is part of AB Doradus Moving Group[5].