Terrestrial planet
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[[Image:Terrestrial planet size comparisons.jpg|thumb|400px|The inner planets, [[Mercury (planet)|Mercury]], [[Venus]], [[Earth]], and [[Mars]], their sizes to scale.]]
A '''terrestrial planet''', '''telluric planet''' or '''rocky planet''' is a [[planet]] that is primarily composed of [[silicate]] [[Rock (geology)|rock]]s. They are also the closest planets to the Sun. The terms are derived from [[Latin]] words for [[Earth]] (''[[Terra]]'' and ''[[Tellus]]''), so an alternative definition would be that these are planets which are, in some notable fashion, "Earth-like". Terrestrial planets are substantially different from [[gas giant]]s, which might not have solid surfaces and are composed mostly of some combination of [[hydrogen]], [[helium]], and [[water]] existing in various [[phase (matter)|physical state]]s.
==Structure==
Terrestrial planets all have roughly the same structure: a central metallic core, mostly [[iron]], with a surrounding silicate [[Mantle (geology)|mantle]]. The [[Moon]] is similar, but lacks an iron core. Terrestrial planets have [[canyon]]s, [[Impact crater|craters]], [[mountain]]s, and [[volcano]]es. Terrestrial planets possess [[secondary atmosphere]]s — atmospheres generated through internal vulcanism or comet impacts, as opposed to the gas giants, which possess [[primary atmosphere]]s — atmospheres captured directly from the original [[solar nebula]].
Theoretically, there are two types of terrestrial or rocky planets, one dominated by silicon compounds and another dominated by carbon compounds, like [[carbonaceous chondrite]] asteroids. These are the silicate planets and [[carbon planet]]s (or "diamond planets") respectively.
==Solar terrestrial planets==
Earth's [[solar system]] has four terrestrial planets: [[Mercury (planet)|Mercury]], [[Venus (planet)|Venus]], [[Earth]] and [[Mars (planet)|Mars]], and one terrestrial [[dwarf planet]], [[Ceres (dwarf planet)|Ceres]]. Objects like [[Pluto (planet)|Pluto]] are similar to terrestrial planets in the fact that they do have a solid surface, but are composed of more icy materials (see [[Ice dwarf]]). During the formation of the solar system, there were probably many more ([[planetesimals]]), but they have all merged with or been destroyed by the four remaining worlds in the [[solar nebula]]. Only one terrestrial planet, Earth, is known to have an active [[hydrosphere]].
In addition, Earth's moon and Jupiter's satellites [[Io (moon)|Io]] and [[Europa (moon)|Europa]] can also be regarded as terrestrial worlds, though since they orbit planets they cannot be considered planets themselves. Io and Europa have mainly rocky compositions despite forming beyond the [[Frost line (astrophysics)|snow line]]. This may be because the region of the circum-Jovian disc in which they formed was kept too warm by radiation from the proto-Jupiter to contain large quantities of icy material.
==Density Trends==
The uncompressed density of the solar terrestrial planets, [[Ceres (dwarf planet)|Ceres]] and the two largest [[asteroid|asteroids]] generally trends towards lower densities as the distance from the [[sun]] increases.
{|class="wikitable"
|-
!Object
!mean density
!uncompressed density
!semi-major axis
|-
|[[Mercury (planet)|Mercury]]
|5.4 g/cm³
|5.3 g/cm³
|0.39 AU
|-
|[[Venus]]
|5.2 g/cm³
|4.4 g/cm³
|0.72 AU
|-
|[[Earth]]
|5.5 g/cm³
|4.4 g/cm³
|1.0 AU
|-
|[[Moon]]
|3.3 g/cm³
|3.3 g/cm³
|1.0 AU
|-
|[[Mars]]
|3.9 g/cm³
|3.8 g/cm³
|1.5 AU
|-
|[[4 Vesta|Vesta]]
|3.4 g/cm³
|3.4 g/cm³
|2.3 AU
|-
|[[2 Pallas|Pallas]]
|2.8 g/cm³
|2.8 g/cm³
|2.8 AU
|-
|[[Ceres (dwarf planet)|Ceres]]
|2.1 g/cm³
|2.1 g/cm³
|2.8 AU
|}
The main exception to this rule is the density of the [[moon]], which owes its smaller density to its unusual [[Moon#Origin_and_geologic_evolution|origin]]. It remains to be seen whether extrasolar terrestrial planets will also follow this trend.
==Extrasolar terrestrial planets==
{{seealso|Super-earth|Pulsar planet}}
[[Image:Earthlike planet-browse.jpg|thumb|left|[[Space Interferometry Mission|SIM PlanetQuest]] will be able to detect Earth-sized planets, such as in this artist's rendering.]]
The majority of planets found outside our [[solar system]] to date have been [[gas giants]], presumably because gas giants are larger and therefore easier to see or infer from observation. However, a number of extrasolar planets are known or suspected to be terrestrial.
[[Aleksander Wolszczan]] detected the first extrasolar terrestrial [[planets]]. The three planets orbit the [[pulsar]] [[PSR B1257+12]] with masses of 0.02, 4.3, and 3.9 times that of Earth's. They were discovered by accident: their transit caused interruptions in the pulsar's radio emissions (had they not been orbiting around a pulsar, they would not have been found).
When [[51 Pegasi b]], the first extrasolar planet found around a [[Stellar nucleosynthesis|fusing]] star, was discovered, many astronomers assumed it must be a gigantic terrestrial, as it was assumed no gas giant could exist as close to its star (0.052 AU) as 51 Pegasi b did. However, subsequent diameter measurements of a similar extrasolar planet ([[HD 209458 b]]), which transited its star showed that these objects were indeed gas giants.
In [[June 2005]], the first planet around a fusing star that is almost certainly terrestrial was found orbiting around the [[red dwarf]] [[star]] [[Gliese 876]], 15 light years away. That planet has a mass of 5 to 7 times that of earth and an orbital period of just two Earth days.
On [[10 August]], [[2005]], [[Probing Lensing Anomalies Network|Probing Lensing Anomalies NETwork]]/[[Robotic Telescope Network]] (PLANET/RoboNet) and [[Optical Gravitational Lensing Experiment]] (OGLE) observed the signature of a cold planet designated [[OGLE-2005-BLG-390Lb]], about 5.5 times the mass of Earth, orbiting a star about 21,000 [[light year]]s away in the constellation Scorpius. The newly discovered planet orbits its parent star at a distance similar to that of our solar system's [[asteroid belt]]. The planet revealed its existence through a technique known as [[gravitational microlensing]], currently unique in its capability to detect cool planets with masses down to that of Earth.
[[Image:Carbon Planet.JPG|thumb|left|180px|Re-creation of [[carbon planet]]]]
In [[April 2007]], a team of 11 European scientists announced the discovery of a planet outside our solar system that is potentially habitable, with Earth-like temperatures. The planet was discovered by the [[European Southern Observatory]]'s telescope in [[La Silla]], Chile, which has a special instrument that splits light to find wobbles in different wave lengths. Those wobbles can reveal the existence of other worlds. What they revealed is a planet circling the red dwarf star, [[Gliese 581]]. The discovery of the new planet, named [[Gliese 581 c]], is sure to fuel studies of planets circling similar dim stars. About 80 percent of the stars near Earth are red dwarfs. The new planet is about five times heavier than Earth, classifying it as a [[super-earth]]. Its discoverers aren't certain if it is rocky, like Earth, or if it is a frozen ice ball with liquid water on the surface. If it is rocky like Earth, which is what the prevailing theory proposes, it has a diameter about 1 1/2 times bigger than our planet. If it is an iceball, it would be even bigger.
A number of telescopes capable of directly imaging extrasolar terrestrial planets are on the drawing board. These include the [[Terrestrial Planet Finder]], [[Space Interferometry Mission]], [[Darwin (ESA)|Darwin]], [[New Worlds Mission]], [[kepler mission|the kepler mission]], and [[Overwhelmingly Large Telescope]].
===Most Earthlike exoplanets===
{| class="wikitable"
|-
! Title
! Planet
! Star
! Notes
|-
| Closest planet to 1 ''M''<sub>Earth</sub>
| [[PSR_B1257%2B12C|PSR 1257+12 C]]
| [[PSR 1257+12]]
| 3.9 M<sub>Earth</sub>
|-
| rowspan=3| Closest planet to 1 AU orbital
| [[HD 142#HD 142 b|HD 142 b]] (gas giant)
| [[HD 142]]
| 0.980 AU
|-
| [[HD 28185 b]] (gas giant)
| [[HD 28185]]
| 1.031 AU
|-
| [[HD 128311#HD 128311 b|HD 128311 b]] (gas giant)
| [[HD 128311]]
| 1.02 AU
|-
| rowspan=2| Closest planet to 365-day orbit
| HD 142 b (gas giant)
| HD 142
| 337 d
|-
| [[HD 92788|HD 92788 b]] (gas giant)
| [[HD 92788]]
| 378 d
|-
| rowspan=2| Closest to 300 [[Kelvin|K]]
| [[Mu Arae e]]
| [[Mu Arae]]
| 308 K
|-
| [[Gliese 581 c]]
| [[Gliese 581]]
| 290 K; A first Earth-like planet in [[habitable zone]], possibility of liquid water.
|}
==See also==
* [[Jovian planet]]/[[Gas giant]] planet
* [[Chthonian planet]]
* [[Dwarf planet]]
* [[Gliese 581 c]]
* [[Planetarium]]
* [[Planetary habitability]]
* [[Polytrope]]
==References==
* [http://www.eso.org/outreach/press-rel/pr-2007/pr-22-07.html Astronomers Find First Earth-like Planet in Habitable Zone] ESO - European Organisation for Astronomical Research in the Southern Hemisphere, 27 April 2007
* [http://www.nature.com/news/2006/060123/full/060123-5.html Found: one Earth-like planet] Astronomers use gravity lensing to spot homely planets. By Mark Peplow, News @ Nature.com, 25 January 2006.
* [http://www.nature.com/nature/journal/v439/n7075/abs/nature04441.html Beaulieu J.P., et al. (2006)] ''Nature,'' '''439,''' 437-440.
* [http://www.nsf.gov/news/news_summ.jsp?cntn_id=105759 National Science Foundation press release] "Closer to Home."
* [http://www.nsf.gov/news/newsmedia/planet06/index.jsp A New Path to New Earths] National Science Foundation webcast.
* [http://www.nsf.gov/discoveries/disc_summ.jsp?cntn_id=100670 Ogling Distant Stars] National Science Foundation grant report.
* [http://www.astro.psu.edu/users/alex/pulsar_planets_text.html Wolszczan's Pulsar Planets].
* [http://planet.iap.fr PLANET Homepage].
* [http://www.astro.livjm.ac.uk/RoboNet RoboNet Homepage].
* [http://ogle.astrouw.edu.pl OGLE Homepage].
* [http://www.phys.canterbury.ac.nz/moa/ MOA Homepage].
==External links==
* SPACE.com: [http://www.space.com/scienceastronomy/060816_planet_qanda.html Q&A: The IAU's Proposed Planet Definition] 16 August 2006 2:00 am ET
* BBC News: [http://news.bbc.co.uk/1/hi/sci/tech/4798205.stm Q&A New planets proposal] Wednesday, 16 August 2006, 13:36 GMT 14:36 UK
{{Solar System}}
[[Category:Types of planet]]
[[Category:Terrestrial planets| ]]
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[[bg:Земеподобна планета]]
[[ca:Planeta tel·lúric]]
[[cs:Terestrická planeta]]
[[de:Erdähnlicher Planet]]
[[et:Maa-tüüpi planeedid]]
[[es:Planeta terrestre]]
[[eo:Tersimila planedo]]
[[fr:Planète tellurique]]
[[ko:지구형 행성]]
[[hr:Terestrički planet]]
[[it:Pianeta terrestre]]
[[he:כוכב לכת ארצי]]
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[[ja:地球型惑星]]
[[nn:Terrestrisk planet]]
[[pl:Planeta skalista]]
[[pt:Planeta telúrico]]
[[ru:Планеты земной группы]]
[[sk:Terestriálna planéta]]
[[sl:Zemeljski planet]]
[[sr:Терестричка планета]]
[[fi:Maankaltainen planeetta]]
[[sv:Stenplanet]]
[[vi:Hành tinh kiểu Trái Đất]]
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