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{{Infobox planet
'''2M1207b''' adalah sebuah [[planet ekstrasurya]] yang meng[[orbit]] [[2M1207]], sebuah [[bintang]] [[katai coklat]] di [[rasi]] [[Hydra]] dan berjarak sekitar 200 [[tahun cahaya]] dari Bumi. Tercatat sebagai planet ekstrasurya pertama yang teramati secara langsung melalui pencitraan [[inframerah]], planet ini ditemukan pada awal [[2005]] menggunakan ''[[Very Large Telescope]]'' di [[Observatorium Paranal]] [[Chili]] oleh sebuah tim dari ''[[European Southern Observatory]]'' yang dipimpin oleh [[Gael Chauvin]]. Dipercaya planet ini memiliki massa sekitar 5 kali massa [[Yupiter]] dan mengorbit bintang induk pada jarak sekitar 2 kali jarak [[Neptunus]] – [[Matahari]].
| name = 2M1207b
| symbol =
| image = Exoplanet Comparison 2M1207 b.png
| image_size =
| image_alt =
| caption = Perbandingan ukuran 2M1207b dengan Jupiter.
| background =
| bgcolour =
| label_width =
<!-- DISCOVERY -->
| discoverer = [[Gael Chauvin|Chauvin]] et al.
| discovery_site = [[Observatorium Paranal]], [[Chile]]
| discovered = April 2004
| discovery_method = Pencitraan
| discovery_ref =
<!-- DESIGNATIONS -->
| exosolar planets =
| minorplanet =
| extrasolarplanet =
| mpc_name =
| pronounced =
| named_after =
| alt_names =
| mp_category =
| adjectives =
<!-- ORBITAL -->
| orbit_ref =
| orbit_diagram =
| epoch =
| uncertainty =
| observation_arc =
| earliest_precovery_date =
| apsis = astron
| aphelion =
| perihelion =
| semimajor = {{convert|24|-|231|AU|km|abbr=on}}<ref name="Blunt2017"/>
| mean_orbit_radius =
| eccentricity = {{val|0.02|-|0.98}}<ref name="Blunt2017"/>
| period = {{val|633|-|20046}}<ref name="Blunt2017"/> [[year|y]]
| synodic_period =
| avg_speed =
| mean_anomaly =
| mean_motion =
| inclination = {{val|13|-|150}}<ref name="Blunt2017"/>
| angular_dist =
| asc_node = {{val|7|-|174}}<ref name="Blunt2017"/>
| long_periastron =
| time_periastron = {{val|2107.69|-|12883.36}}<ref name="Blunt2017"/>
| arg_peri = {{val|4|-|176}}<ref name="Blunt2017"/>
| semi-amplitude =
| satellite_of =
| satellites =
| star =
| allsatellites =
| tisserand =
<!-- PHYS CHARS -->
| physical_ref =
| dimensions =
| mean_diameter =
| mean_radius = 1.5<ref name=encyc /> {{Jupiter radius|link=y}}
| equatorial_radius =
| polar_radius =
| flattening =
| circumference =
| surface_area =
| volume =
| mass = {{val|4|6|-1}}<ref name=encyc /> {{Jupiter mass|link=y}}
| density =
| surface_grav =
| moment_of_inertia_factor =
| escape_velocity =
| rotation =
| sidereal_day =
| rot_velocity =
| axial_tilt =
| right_asc_north_pole =
| declination =
| pole_ecliptic_lat =
| pole_ecliptic_lon =
| albedo =
| single_temperature = 1600 ± 100 K<ref name=mohanty />
| spectral_type =
| magnitude =
| abs_magnitude =
| angular_size =
| family =
<!-- ATMOSPHERE -->
| atmosphere_ref =
| atmosphere =
| scale_height =
| surface_pressure =
| atmosphere_composition =
<!-- NOTES -->
| note =
}}
 
'''2M1207b''' adalah [[Planet#Benda bermassa planet|objek bermassa planet]] yang mengorbit sebuah katai coklat [[2M1207]], di konstelasi [[Centaurus]], sekitar 170 tahun cahaya dari Bumi. Objek ini adalah salah satu kandidat exoplanet pertama yang dapat diamati secara langsung (dengan pencitraan [[inframerah]]). Planet ini ditemukan pada bulan April 2004 oleh [[Very Large Telescope]] (VLT) di [[Observatorium Paranal]] di Chili oleh tim dari [[European Southern Observatory]] yang dipimpin oleh [[Gaël Chauvin]]. Planet ini diduga memiliki massa antara 3 sampai 10 kali massa Jupiter dan mungkin mengorbit 2M1207 pada jarak yang setara dengan Pluto ke Matahari.
{{astronomi-stub}}
 
== Referensi ==
{{reflist|refs=
<ref name="Blunt2017">{{cite journal | title=Orbits for the Impatient: A Bayesian Rejection-sampling Method for Quickly Fitting the Orbits of Long-period Exoplanets | last1=Blunt | first1=Sarah | last2=Nielsen | first2=Eric L. | last3=De Rosa | first3=Robert J. | last4=Konopacky | first4=Quinn M. | last5=Ryan | first5=Dominic | last6=Wang | first6=Jason J. | last7=Pueyo | first7=Laurent | last8=Rameau | first8=Julien | last9=Marois | first9=Christian | last10=Marchis | first10=Franck | last11=MacIntosh | first11=Bruce | last12=Graham | first12=James R. | last13=Duchêne | first13=Gaspard | last14=Schneider | first14=Adam C. | display-authors=1 | journal=The Astronomical Journal | volume=153 | issue=5 | at=229 | year=2017 | arxiv=1703.10653 | bibcode=2017AJ....153..229B | doi=10.3847/1538-3881/aa6930 }}</ref>
 
<ref name=encyc>[http://exoplanet.eu/star.php?st=2M1207 Star: 2M1207] {{webarchive|url=https://web.archive.org/web/20111006004013/http://exoplanet.eu/star.php?st=2M1207 |date=2011-10-06 }}, ''Extrasolar Planets Encyclopaedia''. Accessed on line June 15, 2008.</ref>
 
<ref name=mohanty>The Planetary Mass Companion 2MASS 1207-3932B: Temperature, Mass, and Evidence for an Edge-on Disk, Subhanjoy Mohanty, Ray Jayawardhana, Nuria Huelamo, and Eric Mamajek, ''Astrophysical Journal'' '''657''', #2 (March 2007), pp. 1064–1091. {{Bibcode|2007ApJ...657.1064M}} {{doi|10.1086/510877}}.</ref>
}}
{{Sky|12|07|33.47|-|39|32|54.0|172}}
 
{{DEFAULTSORT:2m1207b}}
[[Kategori:Eksoplanet]]
[[Kategori:Planet luar surya]]
[[Kategori:Rasi bintang Hydra]]
 
 
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