R Leonis

From Wikipedia, the free encyclopedia
Jump to navigation Jump to search

Template:Short description

R Leonis
Template:Location mark
Location of R Leonis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Leo
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 4.4 - 11.3[2]
Characteristics
Spectral type M6e-M8IIIe-M9.5e[2]
Apparent magnitude (J) −0.7[3]
B−V Template:Engvar 1.26
Variable type Mira variable
Astrometry
Proper motion (μ) RA: 6.132[1] mas/yr
Dec.: −53.097[1] mas/yr
Parallax (π)14.0566±0.8378 mas[1]
Distance372 ly
(114[4] pc)
Details
Mass0.7[5] Template:Solar mass
Radius320Template:Snd350[6] Template:Solar radius
Luminosity3,537[4] Template:Solar luminosity
Temperature2,930Template:Snd3,080[6] K
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBADdata

Script error: No such module "Check for unknown parameters".

R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo.

File:RLeoLightCurve.png
The light curve of R Leonis from AAVSO V band data[7]

The apparent magnitude of R Leonis varies between 4.31 and 11.65 with a period of 312 days. At maximum it can be seen with the naked eye, while at minimum a telescope of at least 7 cm is needed. The star's effective temperature is estimated to be 2,930Template:Snd3,080Script error: No such module "String".kelvins and radius spans Script error: No such module "convert".,[6] roughly Mars's orbital zone.

Possible planet

File:R Leonis evaporating planet.png
Artistic rendering of R Leonis's putative evaporating planetary companion

In 2009 Wiesemeyer et al.[5] proposed that quasi-periodic fluctuations observed for the star R Leonis may be due to the presence of an evaporating substellar companion, probably an extrasolar planet. They have inferred a putative mass for the orbiting body of twice the mass of Jupiter, orbital period of 5.2 years and likely orbital separation of 2.7 astronomical units. If confirmed such a planetary object could likely be an evaporating planet, with a long comet-like trail as hinted by intense SiO maser emissions.

Template:OrbitboxPlanet begin Template:OrbitboxPlanet hypothetical

|}Script error: No such module "Check for unknown parameters".

References

<templatestyles src="Reflist/styles.css" />

  1. a b c d e Template:Cite Gaia DR2
  2. a b Script error: No such module "citation/CS1".
  3. Template:Cite simbad
  4. a b Script error: No such module "Citation/CS1".
  5. a b Script error: No such module "Citation/CS1".
  6. a b c Script error: No such module "Citation/CS1".
  7. Script error: No such module "citation/CS1".

Script error: No such module "Check for unknown parameters".

External links

Template:Stars of Leo