V Leonis
variable star in the constellation Leo
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V Leonis
Summary
V Leonis is a Mira variable[1].
Key Facts
- V Leonis's instance of is recorded as Mira variable[2].
- V Leonis's instance of is recorded as astrophysical maser[3].
- V Leonis's constellation is recorded as Leo[4].
- V Leonis's spectral class is recorded as M5-6e[5].
- V Leonis's catalog code is recorded as DO 14055[6].
- V Leonis's catalog code is recorded as GCRV 6373[7].
- V Leonis's catalog code is recorded as HD 86608[8].
- V Leonis's catalog code is recorded as HIC 49026[9].
- V Leonis's catalog code is recorded as HIP 49026[10].
- V Leonis's catalog code is recorded as IRAS 09572+2130[11].
- V Leonis's catalog code is recorded as 2MASS J10000193+2115444[12].
- V Leonis's catalog code is recorded as BD+21 2140[13].
- V Leonis's catalog code is recorded as TYC 1418-712-1[14].
- V Leonis's catalog code is recorded as WEB 9095[15].
- V Leonis's catalog code is recorded as Gaia DR2 629454777516193152[16].
- V Leonis's catalog code is recorded as V Leo[17].
- V Leonis's type of variable star is recorded as Mira variable[18].
- V Leonis's apparent magnitude is recorded as {'unit': '1', 'amount': '+11.57'}[19].
- V Leonis's apparent magnitude is recorded as {'unit': '1', 'amount': '+8.40'}[20].
- V Leonis's apparent magnitude is recorded as {'unit': '1', 'amount': '+7.6569'}[21].
- V Leonis's apparent magnitude is recorded as {'unit': '1', 'amount': '+4.65'}[22].
- V Leonis's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.79'}[23].
- V Leonis's apparent magnitude is recorded as {'unit': '1', 'amount': '+3.28'}[24].
- V Leonis's parallax is recorded as {'unit': 'http://www.wikidata.org/entity/Q21500224', 'amount': '+0.6521'}[25].
- V Leonis's radial velocity is recorded as {'unit': 'http://www.wikidata.org/entity/Q3674704', 'amount': '-23.00'}[26].
Body
Designation and Status
Recorded instance of include Mira variable[2] and astrophysical maser[3].
History and Context
Catalog codes include DO 14055[6], GCRV 6373[7], HD 86608[8], HIC 49026[9], HIP 49026[10], and IRAS 09572+2130[11].