View source for Gliese 436

{{Short description|Star in the constellation Leo}}
{{Starbox begin
| name = Gliese 436 / Noquisi
}}
{{Starbox observe
| epoch = J2000
| constell = [[Leo (constellation)|Leo]]<ref name="Roman1987"/>
| ra = {{RA|11|42|11.09334}}<ref name="GaiaDR3"/>
| dec = {{DEC|+26|42|23.6508}}<ref name="GaiaDR3"/>
| appmag_v = 10.67<ref name="Butler2004"/>
}}
{{Starbox character
| class = M2.5&nbsp;V<ref name="Butler2004"/>
| appmag_1_passband = B
| appmag_1 = ~12.20<ref name=aj128_1_463/>
| appmag_2_passband = V
| appmag_2 = ~10.68<ref name=aj128_1_463/>
| appmag_3_passband = J
| appmag_3 = {{nowrap|6.900 ± 0.024}}<ref name=2MASS/>
| appmag_4_passband = H
| appmag_4 = {{nowrap|6.319 ± 0.023}}<ref name=2MASS/>
| appmag_5_passband = K
| appmag_5 = {{nowrap|6.073 ± 0.016}}<ref name=2MASS/>
| b-v = +1.52<ref name="Butler2004"/>
| u-b = +1.23<ref name="Simbad"/>
| variable =
}}
{{Starbox astrometry
| radial_v = {{val|+8.87|0.16}}<ref name="GaiaDR3"/>
| prop_mo_ra = {{val|895.088|(26)}}
| prop_mo_dec = {{val|-813.550|(25)}}
| pm_footnote = <ref name="GaiaDR3"/>
| parallax = 102.3014
| p_error = 0.0302
| parallax_footnote = <ref name="GaiaDR3"/>
| absmag_v = 10.63<ref name="Butler2004"/>
}}
{{Starbox detail
|source=<ref name="Pineda2021"/>
| mass = 0.425{{±|0.009}}
| radius = 0.432{{±|0.011}}
| luminosity = 0.02463{{±|0.00029}}
| temperature = {{val|3477|46|44|fmt=commas}}
| metal_fe = -0.46{{±|0.31|0.24}}<ref name="Wang2021"/>
| gravity = 4.833{{±|0.013}}<ref name="Wang2021"/>
| rotational_velocity = 1.0<ref name=apj704_2_975/>
| rotation = {{Val|39.9|0.8|u=d}}<ref name=mnras452_3_2745/>
| age_gyr = 7.41–11.05<ref name=saffe/>
}}
{{Starbox catalog
| names = {{odlist | name = Noquisi | 2MASS = J11421096+2642251 | GJ = 436 | HIP = 57087 | LTT = 13213 | LHS = 310 | Ross = 905 }}<ref name="Simbad"/>
}}
{{Starbox reference
| Simbad = LHS+310
| EPE = GJ+436
}}
{{Starbox end}}
'''Gliese 436''' is a [[red dwarf]] located {{Convert|31.9|ly|pc|abbr=off|lk=on}} away in the [[zodiac]] [[constellation]] of [[Leo (constellation)|Leo]]. It has an [[apparent visual magnitude]] of 10.67,<ref name="Butler2004"/> which is much too faint to be seen with the naked eye. However, it can be viewed with even a modest telescope of {{Convert|2.4|in|cm|abbr=on|sigfig=1}} [[aperture]].<ref name=sherrod_koed2003/> In 2004, the existence of an [[extrasolar planet]], [[Gliese 436 b]], was verified as orbiting the star. This planet was later discovered to transit its host star.
[[File:Gliese-436-b.jpg|thumb|Gliese 436]]
==Nomenclature==
The designation ''Gliese 436'' comes from the [[Gliese Catalogue of Nearby Stars]]. This was the 436th star listed in the first edition of the catalogue.
In August 2022, this planetary system was included among 20 systems to be named by the third [[NameExoWorlds]] project.<ref>{{cite web |url=https://www.nameexoworlds.iau.org/2022exoworlds |title=List of ExoWorlds 2022 |date=8 August 2022 |website=nameexoworlds.iau.org |publisher=[[International Astronomical Union|IAU]] |access-date=27 August 2022 |archive-date=8 March 2023 |archive-url=https://web.archive.org/web/20230308103542/https://www.nameexoworlds.iau.org/2022exoworlds |url-status=live }}</ref> The approved names, proposed by a team from the [[United States]], were announced in June 2023. Gliese 436 is named '''Noquisi''' and its planet is named '''Awohali''', after the [[Cherokee]] words for "star" and "eagle".<ref name="NEW2022"/>
==Properties==
Gliese 436 is a [[stellar classification|M2.5V star]],<ref name="Butler2004"/> which means it is a [[red dwarf]]. Stellar models give both an estimated mass and size of about 43% that of the [[Sun]]. The same model predicts that the [[stellar atmosphere|outer atmosphere]] has an [[effective temperature]] of 3,480&nbsp;K,<ref name="Pineda2021"/> giving it the orange-red hue of an [[M-type star]].<ref name=csiro/> Small stars such as this generate energy at a low rate, giving it only 2.5% of the Sun's luminosity.<ref name="Pineda2021"/>
Gliese 436 is older than the Sun by several billion years and it has an abundance of [[metallicity|heavy elements]] (with masses greater than helium-4) less than half%<ref name=apj653/> that of the Sun. The projected rotation velocity is 1.0&nbsp;km/s, and the [[chromosphere]] has a low level of [[Stellar magnetic field|magnetic activity]].<ref name="Butler2004"/> Gliese 436 is a member of the "[[old-disk star|old-disk population]]" with velocity components in the [[galactic coordinate system]] of ''U''=+44, ''V''=−20 and ''W''=+20&nbsp;km/s.<ref name="Butler2004"/>
==Planetary system==
The star is orbited by one known planet, designated [[Gliese 436 b]]. The planet has an orbital period of 2.6 Earth days and [[Methods of detecting extrasolar planets#Transit method|transits]] the star as viewed from Earth. It has a mass of 22.2 [[Earth mass]]es and is roughly 55,000&nbsp;km in diameter, giving it a mass and radius similar to the [[Gas giant|ice giant]] planets [[Uranus]] and [[Neptune]] in the Solar System. In general, Doppler spectroscopy measurements do not measure the true mass of the planet, but instead measure the product <var>m</var> [[sine|sin]] <var>i</var>, where <var>m</var> is the true mass and <var>i</var> is the inclination of the orbit (the angle between the line-of-sight and the [[normal vector|normal]] to the planet's orbital plane), a quantity that is generally unknown. However, for Gliese 436 b, the transits enable the determination of the inclination, as they show that the planet's orbital plane is very nearly in the line of sight (i.e. that the inclination is close to 90 [[degree (angle)|degrees]]). Hence the mass quoted is the actual mass. The planet is thought to be largely composed of hot [[Volatile (astrogeology)|ices]] with an outer envelope of [[hydrogen]] and [[helium]], and is termed a "hot Neptune".<ref>{{cite journal | bibcode = 2007A&A...472L..13G | author = Gillon, M. | display-authors = etal | title = Detection of transits of the nearby hot Neptune GJ 436 b | journal = Astronomy and Astrophysics | volume = 472 | issue = 2 | pages = L13–L16 | date = 2007 | doi = 10.1051/0004-6361:20077799|arxiv = 0705.2219 | s2cid = 13552824 }}</ref>
{{OrbitboxPlanet begin
| table_ref = <ref name="Trifonov2018"/>
}}
{{OrbitboxPlanet
| exoplanet = [[Gliese 436 b|b / Awohali]]
| mass_earth = {{val|21.36|0.20|0.21}}
| semimajor = {{val|0.028|0.01}}
| period = {{val|2.64388|0.00006}}
| eccentricity = {{val|0.152|0.009|0.008}}
| inclination = {{val|85.80|0.25|0.21}}
| radius_earth = 4.33 ± 0.18
}}
{{Orbitbox end}}
GJ 436 b's orbit is likely misaligned with its star's rotation.<ref>{{cite journal| title=A ''Spitzer'' Transmission Spectrum for the Exoplanet GJ 436b |date=2011| last1=Knutson | first1=Heather A.| doi=10.1088/0004-637X/735/1/27| journal=Astrophysical Journal| volume=735, 27 |issue=1|arxiv=1104.2901 |bibcode = 2011ApJ...735...27K | pages=27|s2cid=18669291}}</ref> In addition the planet's orbit is [[orbital eccentricity|eccentric]]. Because [[tidal force]]s would tend to circularise the orbit of the planet on short timescales, this suggested that Gliese 436 b is being perturbed by an additional planet orbiting the star.<ref name="deming">{{cite journal|author=Deming, D. |display-authors=etal |title=Spitzer Transit and Secondary Eclipse Photometry of GJ 436b|date=2007|journal=[[The Astrophysical Journal]]|volume=667|issue=2|pages=L199–L202|doi=10.1086/522496|bibcode=2007ApJ...667L.199D|arxiv = 0707.2778 |s2cid=13349666 }}</ref>
===Claims of additional planets===<!-- this section is linked from redirect "[[Gliese 436 c]]"-->
In 2008, a second planet, designated "Gliese 436 c" was claimed to have been discovered, with an orbital period of 5.2 days and an orbital semimajor axis of 0.045 AU.<ref>{{cite journal | author = Ribas, I. | author2 = Font-Ribera, S. | author3 = Beaulieu, J. P. | name-list-style = amp | title = A ~5 M<sub>⊙</sub> Super-Earth Orbiting GJ 436?: The Power of Near-Grazing Transits | date = 2008 | journal = [[The Astrophysical Journal]] | volume = 677 | issue = 1 | pages = L59–L62 | doi = 10.1086/587961 | bibcode = 2008ApJ...677L..59R |arxiv = 0801.3230 | s2cid = 14132568 }}</ref> The planet was thought to have a mass of roughly 5 [[Earth mass]]es and have a radius about 1.5 times larger than the Earth's.<ref name="reuters"/> Due to its size, the planet was thought to be a rocky, [[terrestrial planet]].<ref>{{cite web | url=http://www.space.com/scienceastronomy/080409-smallest-exoplanet.html | title=New Super-Earth is Smallest Yet | work=Space.com | date=9 April 2008 | access-date=2008-04-10 | archive-date=2010-10-30 | archive-url=https://web.archive.org/web/20101030081226/http://www.space.com/scienceastronomy/080409-smallest-exoplanet.html | url-status=live }}</ref> It was announced by Spanish scientists in April 2008 by analyzing its influence on the orbit of Gliese 436 b.<ref name="reuters">{{cite news |title=Smallest planet outside solar system found |website=[[Reuters]] |date=9 April 2008 |archive-url=https://web.archive.org/web/20230607031428/https://www.reuters.com/article/scienceNews/idUSL0956988620080409 |archive-date=2023-06-07 |url-status=live |url=https://www.reuters.com/article/scienceNews/idUSL0956988620080409}}</ref> Further analysis showed that the transit length of the inner planet is not changing, a situation which rules out most possible configurations for this system. Also, if it did orbit at these parameters, the system would be the only "unstable" orbit on UA's Extrasolar Planet Interactions chart.<ref>[http://www.lpl.arizona.edu/~rory/research/xsp/dynamics/ Extrasolar Planet Interactions] {{Webarchive|url=https://web.archive.org/web/20160505160348/http://www.lpl.arizona.edu/~rory/research/xsp/dynamics/ |date=2016-05-05 }}</ref> The existence of this "Gliese 436 c" was thus regarded as unlikely,<ref>{{cite journal | author = Alonso, R. | display-authors = etal | title = Limits to the planet candidate GJ 436c | date = 2008 | journal = [[Astronomy and Astrophysics]] | volume = 487 | issue = 1 | pages = L5–L8 | doi = 10.1051/0004-6361:200810007 | bibcode = 2008A&A...487L...5A|arxiv = 0804.3030 | s2cid = 119194288 }}</ref> and the discovery was eventually retracted at the Transiting Planets conference in Boston, 2008.<ref>{{cite encyclopedia | url = http://voparis-exoplanet-new.obspm.fr/catalog/gj_436_b/ | title = Planet GJ 436 b | encyclopedia = The Extrasolar Planets Encyclopaedia | author = Schneider, J. | access-date = 2013-02-23 | url-status = dead | archive-url = https://web.archive.org/web/20141223004957/http://voparis-exoplanet-new.obspm.fr/catalog/gj_436_b/ | archive-date = 2014-12-23 }}</ref>
Despite the retraction, studies concluded that the possibility that there is an additional planet orbiting Gliese 436 remained plausible.<ref>{{cite journal|author=Bean, J. L.|author2=Seifahrt, A.|name-list-style=amp|title=Observational Consequences of the Recently Proposed Super-Earth Orbiting GJ436|date=2008|journal=[[Astronomy and Astrophysics]]|volume=487|issue=2|pages=L25–L28|doi=10.1051/0004-6361:200810278|bibcode=2008A&A...487L..25B|arxiv = 0806.3270 |s2cid=14811323}}</ref> With the aid of an unnoticed transit automatically recorded at NMSU on January 11, 2005, and observations by amateur astronomers, it has been suggested that there is a trend of increasing inclination of the orbit of Gliese 436 b, though this trend remains unconfirmed. This trend is compatible with a perturbation by a planet of less than 12 Earth masses on an orbit within about 0.08 AU of the star.<ref name=coughlin>{{cite journal|author=Coughlin, J. L. |display-authors=etal|title=New Observations and a Possible Detection of Parameter Variations in the Transits of Gliese 436b|date=2008|journal=[[The Astrophysical Journal]]|volume=689|issue=2|pages=L149–L152|doi=10.1086/595822|bibcode=2008ApJ...689L.149C|arxiv = 0809.1664 |s2cid=14893633}}</ref>
In July 2012, NASA announced that astronomers at the [[University of Central Florida]], using the [[Spitzer Space Telescope]], strongly believed they had observed a second planet.<ref name="SMH">{{cite web
|url          = http://www.smh.com.au/technology/sci-tech/alien-exoplanet-smaller-than-earth-discovered-20120719-22bc4.html
|title        = Alien exoplanet smaller than Earth discovered
|agency       = Reuters
|date         = July 2012
|publisher    = Sydney Morning Herald
|access-date  = 2012-07-19
|archive-date = 2014-04-11
|archive-url  = https://web.archive.org/web/20140411104522/http://www.smh.com.au/technology/sci-tech/alien-exoplanet-smaller-than-earth-discovered-20120719-22bc4.html
|url-status   = live
}}</ref> This candidate planet was given the preliminary designation UCF-1.01, after the University of Central Florida.<ref>{{cite web |url=https://www.orlandosentinel.com/2012/07/18/planet-ucf-101-is-introduced-to-the-world-of-astronomy/ |title=Planet UCF 1.01 is introduced to the world of astronomy |date=July 18, 2012 |access-date=July 20, 2012 |last=Powers |first=Scott |work=[[Orlando Sentinel]] |archive-date=September 7, 2015 |archive-url=https://web.archive.org/web/20150907182920/http://articles.orlandosentinel.com/2012-07-18/news/os-ucf-planet-discovey-20120718_1_earth-size-planets-red-dwarf-star-nasa-spitzer-space-telescope |url-status=live }}</ref> It was measured to have a radius of around two thirds that of Earth and, assuming an Earth-like density of 5.5 g/cm<sup>3</sup>, was estimated to have a mass of 0.3 times that of Earth and a surface gravity of around two thirds that of Earth. It was thought to orbit at 0.0185 AU from the star, every 1.3659 days. The astronomers also believed they had found some evidence for an additional planet candidate, UCF-1.02, which is of a similar size, though with only one detected transit its orbital period is unknown.<ref name="Stevenson2012"/> Follow up observations with the [[Hubble Space Telescope]] as well as a reanalysis of the Spitzer Space Telescope data were unable to confirm these planets.<ref name="Stevenson2014"/><ref name="Lanotte2014"/>
==See also==
* [[List of stars in Leo]]
==References==
{{reflist|refs=
<ref name="GaiaDR3">{{Cite Gaia DR3|4017860992519744384}}</ref>
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<ref name=apj653>{{cite journal | last1=Bean | first1=Jacob L. | last2=Benedict | first2=G. Fritz | last3=Endl | first3=Michael | title=Metallicities of M Dwarf Planet Hosts from Spectral Synthesis | journal=The Astrophysical Journal | date=2006 | volume=653 | issue=1 | pages=L65–L68 | bibcode=2006ApJ...653L..65B | doi=10.1086/510527 | type=abstract | arxiv=astro-ph/0611060 | s2cid=16002711 }}—for the [[metallicity]], note that <math>\begin{smallmatrix}10^{-0.32} = 0.48\end{smallmatrix}</math> or 48%</ref>
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<ref name=mnras452_3_2745>{{citation
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}}</ref>
<ref name="Lanotte2014">{{cite journal | title=A global analysis of Spitzer and new HARPS data confirms the loneliness and metal-richness of GJ 436 b | url=https://www.aanda.org/articles/aa/full_html/2014/12/aa24373-14/aa24373-14.html | last1=Lanotte | first1=A. A. | last2=Gillon | first2=M. | last3=Demory | first3=B.-O. | last4=Fortney | first4=J. J. | last5=Astudillo | first5=N. | last6=Bonfils | first6=X. | last7=Magain | first7=P. | last8=Delfosse | first8=X. | last9=Forveille | first9=T. | last10=Lovis | first10=C. | last11=Mayor | first11=M. | last12=Neves | first12=V. | last13=Pepe | first13=F. | last14=Queloz | first14=D. | last15=Santos | first15=N. | last16=Udry | first16=S. | display-authors=1 | journal=Astronomy and Astrophysics | volume=572 | at=A73 | year=2014 | arxiv=1409.4038 | bibcode=2014A&A...572A..73L | doi=10.1051/0004-6361/201424373 | s2cid=55405647 | access-date=2018-03-18 | archive-date=2022-10-06 | archive-url=https://web.archive.org/web/20221006045915/https://www.aanda.org/articles/aa/full_html/2014/12/aa24373-14/aa24373-14.html | url-status=live }}</ref>
<ref name="Roman1987">{{cite journal | title=Identification of a Constellation From a Position | last1=Roman | first1=Nancy G. | journal=Publications of the Astronomical Society of the Pacific | volume=99 | issue=617 | pages=695–699 | year=1987 | bibcode=1987PASP...99..695R | doi=10.1086/132034 | doi-access=free }} [http://vizier.u-strasbg.fr/vizier/VizieR/constellations.htx Vizier query form ] {{Webarchive|url=https://web.archive.org/web/20190717180728/http://vizier.u-strasbg.fr/vizier/VizieR/constellations.htx |date=2019-07-17 }}</ref>
<ref name="Simbad">{{cite simbad | title=Gliese 436 | access-date=2018-10-06}}</ref>
<ref name="Stevenson2012">{{cite journal | title=Two nearby sub-Earth-sized exoplanet candidates in the GJ 436 system | last1=Stevenson | first1=Kevin B. | last2=Harrington | first2=Joseph | last3=Lust | first3=Nate B. | last4=Lewis | first4=Nikole K. | last5=Montagnier | first5=Guillaume | last6=Moses | first6=Julianne I. | last7=Visscher | first7=Channon | last8=Blecic| first8=Jasmina | last9=Hardy | first9=Ryan A. | last10=Cubillos| first10=Patricio| last11=Campo | first11=Christopher J. | display-authors=1 | journal=The Astrophysical Journal | volume=755 | issue=1 | at=9 | year=2012 | arxiv=1207.4245 | bibcode=2012ApJ...755....9S | doi=10.1088/0004-637X/755/1/9 | s2cid=118678765 }}</ref>
<ref name="Stevenson2014">{{cite journal | title=A Hubble Space Telescope Search for a Sub-Earth-sized Exoplanet in the GJ 436 System | last1=Stevenson | first1=Kevin B. | last2=Bean | first2=Jacob L. | last3=Fabrycky | first3=Daniel | last4=Kreidberg | first4=Laura | display-authors=1 | journal=The Astrophysical Journal | volume=796 | issue=1 | at=32 | year=2014 | arxiv=1410.0002 | bibcode=2014ApJ...796...32S | doi=10.1088/0004-637X/796/1/32 | s2cid=118412895 }}</ref>
<ref name="Trifonov2018">{{cite journal |doi=10.1051/0004-6361/201731442 |title=The CARMENES search for exoplanets around M dwarfs. First visual-channel radial-velocity measurements and orbital parameter updates of seven M-dwarf planetary systems |last1=Trifonov |first1=Trifon |last2=Kürster |first2=Martin |last3=Zechmeister |first3=Mathias |last4=Tal-Or |first4=Lev |last5=Caballero |first5=José A. |last6=Quirrenbach |first6=Andreas |last7=Amado |first7=Pedro J. |last8=Ribas |first8=Ignasi |last9=Reiners |first9=Ansgar |last10=Reffert |first10=Sabine |last11=Dreizler |first11=Stefan |last12=Hatzes |first12=Artie P. |last13=Kaminski |first13=Adrian |last14=Launhardt |first14=Ralf |last15=Henning |first15=Thomas K. |last16=Montes |first16=David |last17=Béjar |first17=Victor J. S. |last18=Mundt |first18=Reinhard |last19=Pavlov |first19=Aleksei |last20=Schmitt |first20=Jürgen H. M. M. |last21=Seifert |first21=Walter |last22=Morales |first22=Juan Carlos |last23=Nowak |first23=Grzegorz |last24=Jeffers |first24=Sandra V. |last25=Rodríguez-López |first25=Cristina |last26=del Burgo |first26=Carlos |last27=Anglada-Escudé |first27=Guillem |last28=López-Santiago |first28=Javier |last29=Mathar |first29=Richard J. |last30=Ammler-von Eiff |first30=Matthias <!-- over 100 more -->|display-authors=9 |journal=Astronomy and Astrophysics |volume=609 |at=A117 |year=2018 |arxiv=1710.01595 |bibcode=2018A&A...609A.117T |s2cid=119340839 }}</ref>
<ref name="Wang2021">{{cite journal | last1=Wang | first1=Xian-Yu | last2=Wang | first2=Yong-Hao | last3=Wang | first3=Songhu | last4=Wu | first4=Zhen-Yu | last5=Rice | first5=Malena | last6=Zhou | first6=Xu | last7=Hinse | first7=Tobias C. | last8=Liu | first8=Hui-Gen | last9=Ma | first9=Bo | last10=Peng | first10=Xiyan | last11=Zhang | first11=Hui | last12=Yu | first12=Cong | last13=Zhou | first13=Ji-Lin | last14=Laughlin | first14=Gregory | display-authors=1 | title=Transiting Exoplanet Monitoring Project (TEMP). VI. The Homogeneous Refinement of System Parameters for 39 Transiting Hot Jupiters with 127 New Light Curves | journal=The Astrophysical Journal Supplement Series | date=1 July 2021 | volume=255 | issue=1 | at=15 | arxiv=2105.14851 | bibcode=2021ApJS..255...15W | doi=10.3847/1538-4365/ac0835 | s2cid=235253975 | doi-access=free }}</ref>
<ref name="Pineda2021">{{cite journal
| title=The M-dwarf Ultraviolet Spectroscopic Sample. I. Determining Stellar Parameters for Field Stars
| last1=Pineda | first1=J. Sebastian | last2=Youngblood | first2=Allison
| last3=France | first3=Kevin | display-authors=1
| journal=The Astrophysical Journal
| volume=918 | issue=1 | id=40 | pages=23 | date=September 2021
| doi=10.3847/1538-4357/ac0aea | arxiv=2106.07656
| bibcode=2021ApJ...918...40P | s2cid=235435757 | doi-access=free }}</ref>
<ref name="NEW2022">{{cite web |url=https://www.nameexoworlds.iau.org/2022approved-names |title=2022 Approved Names |website=nameexoworlds.iau.org |publisher=[[International Astronomical Union|IAU]] |access-date=7 June 2023 |archive-date=1 May 2024 |archive-url=https://web.archive.org/web/20240501010333/https://nameexoworlds.iau.org/2022approved-names |url-status=live }}</ref>
}}
==External links==
*{{cite web
| url=http://solstation.com/stars2/gl436.htm
| title=Gliese 436 / AC+27 28217
| publisher=Sol Company
| access-date=2007-11-28
| archive-date=2015-09-13
| archive-url=https://web.archive.org/web/20150913055200/http://solstation.com/stars2/gl436.htm
| url-status=dead
}}
* {{cite web
| url=http://media4.obspm.fr/exoplanets/base/etoile.php?nom=GJ+436
| title=GJ 436
| publisher=l'Observatoire de Paris
| access-date=2009-05-20
| archive-url=https://web.archive.org/web/20120401193040/http://media4.obspm.fr/exoplanets/base/etoile.php?nom=GJ+436
| archive-date=2012-04-01
| url-status=dead
}}
* {{cite web
| url=http://news.NationalGeographic.com/news/2012/07/120719-new-planet-ucf-spitzer-science-space-stevenson
| archive-url=https://web.archive.org/web/20120720194534/http://news.nationalgeographic.com/news/2012/07/120719-new-planet-ucf-spitzer-science-space-stevenson/
| url-status=dead
| archive-date=July 20, 2012
| title=New Planet Found: Molten "Mars" Is "Right Around the Corner"
| publisher=National Geographic
| access-date=2012-07-20}}
{{Sky|11|42|11.0941|+|26|42|23.652|33.4}}
{{Stars of Leo}}
{{DEFAULTSORT:Gliese 436}}
[[Category:Leo (constellation)]]
[[Category:M-type main-sequence stars]]
[[Category:Hipparcos objects|057087]]
[[Category:Gliese and GJ objects|0436]]
[[Category:Ross objects|905]]
[[Category:Planetary transit variables]]
[[Category:Planetary systems with one confirmed planet]]
[[Category:2MASS objects|J11421096+2642251]]
[[Category:Stars with proper names|Noquisi]]
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