R Leonis
{{Short description|Variable star in the constellation Leo}}
{{Starbox begin
| name = R Leonis
}}
{{Starbox image
| image=
{{Location mark
|image=Leo constellation map.svg|alt=|float=center|width=280
|label=|position=right
|mark=Red circle.svg|mark_width=8|mark_link=R Leo
|x=908|y=612
}}
|caption=Location of R Leonis (circled)
}}
{{Starbox observe
| epoch = J2000.0
| constell = Leo
| appmag_v = 4.4 - 11.3{{cite web
|title=GCVS Query=R Leo
|publisher=General Catalogue of Variable Stars @ Sternberg Astronomical Institute, Moscow, Russia
|url=http://www.sai.msu.su/gcvs/cgi-bin/search.cgi?search=R+Leo
|accessdate=2012-08-22}}
}}
{{Starbox character
| appmag_1_passband = J
| appmag_1 = −0.7{{cite simbad |title=V* R Leo |access-date=2012-08-21}}
| r-i =
| v-r =
| b-v = 1.26
| u-b =
| variable = Mira variable
}}
{{Starbox astrometry
| parallax = 14.0566
| p_error = 0.8378
| parallax_footnote = {{cite Gaia DR2|612958873284128128}}
| dist_ly = 372
}}
{{Starbox detail
| radius = 320{{snd}}350{{Cite journal | arxiv=astro-ph/0411133 | author=Fedele | display-authors=etal | title=The K -Band Intensity Profile of R Leonis Probed by VLTI/VINCI | journal=Astronomy and Astrophysics | volume=431 | issue=3 | pages=1019–1026 | date=2005 | bibcode=2005A&A...431.1019F|doi = 10.1051/0004-6361:20042013 | s2cid=15500217 }}
| temperature = 2,930{{snd}}3,080
}}
{{Starbox catalog
| names = {{odlist | V=R Leo | AAVSO=0942+11 | HIP=48036 | HD=84748 | HR=3882 | BD=+12°2096 | SAO=98769 }}
}}
{{Starbox reference
|Simbad=R+Leo
}}
{{Starbox end}}
R Leonis is a red giant Mira-type variable star located approximately 370 light years away in the constellation Leo.
File:RLeoLightCurve.png of R Leonis from AAVSO V band data]]
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 2,930{{snd}}3,080{{nbsp}}kelvins and radius spans {{convert|320|solar radius|km au|abbr=off|lk=on}}, roughly Mars's orbital zone.
Possible planet
Image:R Leonis evaporating planet.png
In 2009 Wiesemeyer et al.{{Cite journal | arxiv=0809.0359 | author=Wiesemeyer | display-authors=etal | title=Precessing planetary magnetospheres in SiO stars?. First detection of quasi-periodic polarization fluctuations in R Leonis and V Camelopardalis| journal=Astronomy and Astrophysics | volume=498 | issue=3 | pages=801–810 | date=2009 | bibcode=2009A&A...498..801W|doi = 10.1051/0004-6361/200811242 | s2cid=14531031 }} 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.
{{OrbitboxPlanet begin}}
{{OrbitboxPlanet hypothetical
| exoplanet = b
| mass = ≥2
| period = 1898
| semimajor = ≥2.7
| eccentricity = 0
}}
{{Orbitbox end}}
References
External links
- [http://www.aavso.org/vstar/vsots/0401.shtml AAVSO Variable Star of the Month. April, 2001: R Leonis] {{Webarchive|url=https://web.archive.org/web/20031106073859/http://www.aavso.org/vstar/vsots/0401.shtml |date=2003-11-06 }}
{{Stars of Leo}}
{{DEFAULTSORT:R Leonis}}
Category:Hypothetical planetary systems