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Mars
Mars
is the fourth planet from the Sun
Sun
and the second-smallest planet in the Solar System
Solar System
after Mercury. In English, Mars
Mars
carries a name of the Roman god of war, and is often referred to as the "Red Planet"[14][15] because the reddish iron oxide prevalent on its surface gives it a reddish appearance that is distinctive among the astronomical bodies visible to the naked eye.[16] Mars
Mars
is a terrestrial planet with a thin atmosphere, having surface features reminiscent both of the impact craters of the Moon
Moon
and the valleys, deserts, and polar ice caps of Earth. The rotational period and seasonal cycles of Mars
Mars
are likewise similar to those of Earth, as is the tilt that produces the seasons. Mars
Mars
is the site of Olympus Mons, the largest volcano and second-highest known mountain in the Solar System, and of Valles Marineris, one of the largest canyons in the Solar System. The smooth Borealis basin
Borealis basin
in the northern hemisphere covers 40% of the planet and may be a giant impact feature.[17][18] Mars
Mars
has two moons, Phobos and Deimos, which are small and irregularly shaped. These may be captured asteroids,[19][20] similar to 5261 Eureka, a Mars
Mars
trojan. There are ongoing investigations assessing the past habitability potential of Mars, as well as the possibility of extant life. Future astrobiology missions are planned, including the Mars 2020
Mars 2020
and ExoMars rovers.[21][22][23][24] Liquid water cannot exist on the surface of Mars
Mars
due to low atmospheric pressure, which is less than 1% of the Earth's,[25] except at the lowest elevations for short periods.[26][27] The two polar ice caps appear to be made largely of water.[28][29] The volume of water ice in the south polar ice cap, if melted, would be sufficient to cover the entire planetary surface to a depth of 11 meters (36 ft).[30] In November 2016, NASA
NASA
reported finding a large amount of underground ice in the Utopia Planitia region of Mars. The volume of water detected has been estimated to be equivalent to the volume of water in Lake Superior.[31][32][33] Mars
Mars
can easily be seen from Earth
Earth
with the naked eye, as can its reddish coloring. Its apparent magnitude reaches −2.91,[8] which is surpassed only by Jupiter, Venus, the Moon, and the Sun. Optical ground-based telescopes are typically limited to resolving features about 300 kilometers (190 mi) across when Earth
Earth
and Mars
Mars
are closest because of Earth's atmosphere.[34]

Contents

1 Physical characteristics

1.1 Internal structure 1.2 Surface geology 1.3 Soil 1.4 Hydrology

1.4.1 Polar caps

1.5 Geography and naming of surface features

1.5.1 Map of quadrangles 1.5.2 Impact topography 1.5.3 Volcanoes 1.5.4 Tectonic sites 1.5.5 Holes

1.6 Atmosphere

1.6.1 Aurora

1.7 Climate

2 Orbit and rotation 3 Habitability and search for life

3.1 Search for life

4 Moons 5 Exploration

5.1 Future

6 Astronomy
Astronomy
on Mars 7 Viewing

7.1 Closest approaches

7.1.1 Relative 7.1.2 Absolute, around the present time

8 Historical observations

8.1 Ancient and medieval observations 8.2 Martian
Martian
"canals" 8.3 Spacecraft
Spacecraft
visitation

9 In culture

9.1 Intelligent "Martians" 9.2 2018 rediscovery

10 See also 11 Notes 12 References 13 External links

Physical characteristics Mars
Mars
is approximately half the diameter of Earth
Earth
with a surface area only slightly less than the total area of Earth's dry land.[8] Mars
Mars
is less dense than Earth, having about 15% of Earth's volume and 11% of Earth's mass, resulting in about 38% of Earth's surface gravity. The red-orange appearance of the Martian
Martian
surface is caused by iron(III) oxide, or rust.[35] It can look like butterscotch;[36] other common surface colors include golden, brown, tan, and greenish, depending on the minerals present.[36]

Comparison: Earth
Earth
and Mars

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Animation (00:40) showing major features of Mars

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Video (01:28) showing how three NASA
NASA
orbiters mapped the gravity field of Mars

Internal structure Like Earth, Mars
Mars
has differentiated into a dense metallic core overlaid by less dense materials.[37] Current models of its interior imply a core with a radius of about 1,794 ± 65 kilometers (1,115 ± 40 mi), consisting primarily of iron and nickel with about 16–17% sulfur.[38] This iron(II) sulfide core is thought to be twice as rich in lighter elements as Earth's.[39] The core is surrounded by a silicate mantle that formed many of the tectonic and volcanic features on the planet, but it appears to be dormant. Besides silicon and oxygen, the most abundant elements in the Martian
Martian
crust are iron, magnesium, aluminum, calcium, and potassium. The average thickness of the planet's crust is about 50 km (31 mi), with a maximum thickness of 125 km (78 mi).[39] Earth's crust averages 40 km (25 mi). Surface geology Main article: Geology of Mars Mars
Mars
is a terrestrial planet that consists of minerals containing silicon and oxygen, metals, and other elements that typically make up rock. The surface of Mars
Mars
is primarily composed of tholeiitic basalt,[40] although parts are more silica-rich than typical basalt and may be similar to andesitic rocks on Earth
Earth
or silica glass. Regions of low albedo suggest concentrations of plagioclase feldspar, with northern low albedo regions displaying higher than normal concentrations of sheet silicates and high-silicon glass. Parts of the southern highlands include detectable amounts of high-calcium pyroxenes. Localized concentrations of hematite and olivine have been found.[41] Much of the surface is deeply covered by finely grained iron(III) oxide dust.[42][43]

Geologic map of Mars
Mars
(USGS, 2014)[44]

Although Mars
Mars
has no evidence of a structured global magnetic field,[45] observations show that parts of the planet's crust have been magnetized, suggesting that alternating polarity reversals of its dipole field have occurred in the past. This paleomagnetism of magnetically susceptible minerals is similar to the alternating bands found on Earth's ocean floors. One theory, published in 1999 and re-examined in October 2005 (with the help of the Mars
Mars
Global Surveyor), is that these bands suggest plate tectonic activity on Mars four billion years ago, before the planetary dynamo ceased to function and the planet's magnetic field faded.[46] It is thought that, during the Solar System's formation, Mars
Mars
was created as the result of a stochastic process of run-away accretion of material from the protoplanetary disk that orbited the Sun. Mars
Mars
has many distinctive chemical features caused by its position in the Solar System. Elements with comparatively low boiling points, such as chlorine, phosphorus, and sulphur, are much more common on Mars
Mars
than Earth; these elements were probably pushed outward by the young Sun's energetic solar wind.[47] After the formation of the planets, all were subjected to the so-called "Late Heavy Bombardment". About 60% of the surface of Mars shows a record of impacts from that era,[48][49][50] whereas much of the remaining surface is probably underlain by immense impact basins caused by those events. There is evidence of an enormous impact basin in the northern hemisphere of Mars, spanning 10,600 by 8,500 km (6,600 by 5,300 mi), or roughly four times the size of the Moon's South Pole – Aitken basin, the largest impact basin yet discovered.[17][18] This theory suggests that Mars
Mars
was struck by a Pluto-sized body about four billion years ago. The event, thought to be the cause of the Martian
Martian
hemispheric dichotomy, created the smooth Borealis basin
Borealis basin
that covers 40% of the planet.[51][52]

Artist's impression of how Mars
Mars
may have looked four billion years ago[53]

The geological history of Mars
Mars
can be split into many periods, but the following are the three primary periods:[54][55]

Noachian
Noachian
period (named after Noachis Terra): Formation of the oldest extant surfaces of Mars, 4.5 to 3.5 billion years ago. Noachian
Noachian
age surfaces are scarred by many large impact craters. The Tharsis
Tharsis
bulge, a volcanic upland, is thought to have formed during this period, with extensive flooding by liquid water late in the period. Hesperian
Hesperian
period (named after Hesperia Planum): 3.5 to between 3.3 and 2.9 billion years ago. The Hesperian
Hesperian
period is marked by the formation of extensive lava plains. Amazonian period (named after Amazonis Planitia): between 3.3 and 2.9 billion years ago to the present. Amazonian regions have few meteorite impact craters, but are otherwise quite varied. Olympus Mons
Olympus Mons
formed during this period, with lava flows elsewhere on Mars.

Geological activity is still taking place on Mars. The Athabasca Valles is home to sheet-like lava flows created about 200 Mya. Water flows in the grabens called the Cerberus Fossae
Cerberus Fossae
occurred less than 20 Mya, indicating equally recent volcanic intrusions.[56] On February 19, 2008, images from the Mars Reconnaissance Orbiter
Mars Reconnaissance Orbiter
showed evidence of an avalanche from a 700-metre-high (2,300 ft) cliff.[57] Soil Main article: Martian
Martian
soil

Exposure of silica-rich dust uncovered by the Spirit rover

The Phoenix lander returned data showing Martian
Martian
soil to be slightly alkaline and containing elements such as magnesium, sodium, potassium and chlorine. These nutrients are found in soils on Earth, and they are necessary for growth of plants.[58] Experiments performed by the lander showed that the Martian
Martian
soil has a basic pH of 7.7, and contains 0.6% of the salt perchlorate.[59][60][61][62] Streaks are common across Mars
Mars
and new ones appear frequently on steep slopes of craters, troughs, and valleys. The streaks are dark at first and get lighter with age. The streaks can start in a tiny area, then spread out for hundreds of metres. They have been seen to follow the edges of boulders and other obstacles in their path. The commonly accepted theories include that they are dark underlying layers of soil revealed after avalanches of bright dust or dust devils.[63] Several other explanations have been put forward, including those that involve water or even the growth of organisms.[64][65] Hydrology Main article: Water on Mars Liquid water cannot exist on the surface of Mars
Mars
due to low atmospheric pressure, which is less than 1% that of Earth's,[25] except at the lowest elevations for short periods.[26][27] The two polar ice caps appear to be made largely of water.[28][29] The volume of water ice in the south polar ice cap, if melted, would be sufficient to cover the entire planetary surface to a depth of 11 meters (36 ft).[30] A permafrost mantle stretches from the pole to latitudes of about 60°.[28] Large quantities of water ice are thought to be trapped within the thick cryosphere of Mars. Radar data from Mars Express
Mars Express
and the Mars Reconnaissance Orbiter
Mars Reconnaissance Orbiter
show large quantities of water ice at both poles (July 2005)[66][67] and at middle latitudes (November 2008).[68] The Phoenix lander directly sampled water ice in shallow Martian
Martian
soil on July 31, 2008.[69]

Photomicrograph by Opportunity showing a gray hematite concretion, nicknamed "blueberries", indicative of the past existence of liquid water

Landforms visible on Mars
Mars
strongly suggest that liquid water has existed on the planet's surface. Huge linear swathes of scoured ground, known as outflow channels, cut across the surface in about 25 places. These are thought to be a record of erosion caused by the catastrophic release of water from subsurface aquifers, though some of these structures have been hypothesized to result from the action of glaciers or lava.[70][71] One of the larger examples, Ma'adim Vallis is 700 km (430 mi) long, much greater than the Grand Canyon, with a width of 20 km (12 mi) and a depth of 2 km (1.2 mi) in places. It is thought to have been carved by flowing water early in Mars's history.[72] The youngest of these channels are thought to have formed as recently as only a few million years ago.[73] Elsewhere, particularly on the oldest areas of the Martian surface, finer-scale, dendritic networks of valleys are spread across significant proportions of the landscape. Features of these valleys and their distribution strongly imply that they were carved by runoff resulting from precipitation in early Mars
Mars
history. Subsurface water flow and groundwater sapping may play important subsidiary roles in some networks, but precipitation was probably the root cause of the incision in almost all cases.[74] Along crater and canyon walls, there are thousands of features that appear similar to terrestrial gullies. The gullies tend to be in the highlands of the southern hemisphere and to face the Equator; all are poleward of 30° latitude. A number of authors have suggested that their formation process involves liquid water, probably from melting ice,[75][76] although others have argued for formation mechanisms involving carbon dioxide frost or the movement of dry dust.[77][78] No partially degraded gullies have formed by weathering and no superimposed impact craters have been observed, indicating that these are young features, possibly still active.[76] Other geological features, such as deltas and alluvial fans preserved in craters, are further evidence for warmer, wetter conditions at an interval or intervals in earlier Mars
Mars
history.[79] Such conditions necessarily require the widespread presence of crater lakes across a large proportion of the surface, for which there is independent mineralogical, sedimentological and geomorphological evidence.[80]

Composition of "Yellowknife Bay" rocks. Rock veins are higher in calcium and sulfur than "portage" soil (Curiosity, APXS, 2013).

Further evidence that liquid water once existed on the surface of Mars comes from the detection of specific minerals such as hematite and goethite, both of which sometimes form in the presence of water.[81] In 2004, Opportunity detected the mineral jarosite. This forms only in the presence of acidic water, which demonstrates that water once existed on Mars.[82] More recent evidence for liquid water comes from the finding of the mineral gypsum on the surface by NASA's Mars
Mars
rover Opportunity in December 2011.[83][84] It is believed that the amount of water in the upper mantle of Mars, represented by hydroxyl ions contained within the minerals of Mars's geology, is equal to or greater than that of Earth
Earth
at 50–300 parts per million of water, which is enough to cover the entire planet to a depth of 200–1,000 m (660–3,280 ft).[85] In 2005, radar data revealed the presence of large quantities of water ice at the poles[66] and at mid-latitudes.[68][86] The Mars
Mars
rover Spirit sampled chemical compounds containing water molecules in March 2007. The Phoenix lander directly sampled water ice in shallow Martian soil on July 31, 2008.[69] On March 18, 2013, NASA
NASA
reported evidence from instruments on the Curiosity rover of mineral hydration, likely hydrated calcium sulfate, in several rock samples including the broken fragments of "Tintina" rock and "Sutton Inlier" rock as well as in veins and nodules in other rocks like "Knorr" rock and "Wernicke" rock.[87][88][89] Analysis using the rover's DAN instrument provided evidence of subsurface water, amounting to as much as 4% water content, down to a depth of 60 cm (24 in), during the rover's traverse from the Bradbury Landing site to the Yellowknife Bay area in the Glenelg terrain.[87] In September 2015, NASA
NASA
announced that they had found conclusive evidence of hydrated brine flows on recurring slope lineae, based on spectrometer readings of the darkened areas of slopes.[90][91][92] These observations provided confirmation of earlier hypotheses based on timing of formation and their rate of growth, that these dark streaks resulted from water flowing in the very shallow subsurface.[93] The streaks contain hydrated salts, perchlorates, which have water molecules in their crystal structure.[94] The streaks flow downhill in Martian
Martian
summer, when the temperature is above −23 degrees Celsius, and freeze at lower temperatures.[95] On September 28, 2015, NASA
NASA
announced the presence of briny flowing salt water on the Martian
Martian
surface.[96] Researchers believe that much of the low northern plains of the planet were covered with an ocean hundreds of meters deep, though this remains controversial.[97] In March 2015, scientists stated that such an ocean might have been the size of Earth's Arctic Ocean. This finding was derived from the ratio of water to deuterium in the modern Martian
Martian
atmosphere compared to that ratio on Earth. The amount of Martian
Martian
deuterium is eight times the amount that exists on Earth, suggesting that ancient Mars
Mars
had significantly higher levels of water. Results from the Curiosity rover had previously found a high ratio of deuterium in Gale Crater, though not significantly high enough to suggest the former presence of an ocean. Other scientists caution that these results have not been confirmed, and point out that Martian climate models have not yet shown that the planet was warm enough in the past to support bodies of liquid water.[98] Polar caps Main article: Martian
Martian
polar ice caps

North polar early summer ice cap (1999)

South polar midsummer ice cap (2000)

Mars
Mars
has two permanent polar ice caps. During a pole's winter, it lies in continuous darkness, chilling the surface and causing the deposition of 25–30% of the atmosphere into slabs of CO2 ice (dry ice).[99] When the poles are again exposed to sunlight, the frozen CO2 sublimes. These seasonal actions transport large amounts of dust and water vapor, giving rise to Earth-like frost and large cirrus clouds. Clouds of water-ice were photographed by the Opportunity rover
Opportunity rover
in 2004.[100] The caps at both poles consist primarily (70%) of water ice. Frozen carbon dioxide accumulates as a comparatively thin layer about one metre thick on the north cap in the northern winter only, whereas the south cap has a permanent dry ice cover about eight metres thick. This permanent dry ice cover at the south pole is peppered by flat floored, shallow, roughly circular pits, which repeat imaging shows are expanding by meters per year; this suggests that the permanent CO2 cover over the south pole water ice is degrading over time.[101] The northern polar cap has a diameter of about 1,000 km (620 mi) during the northern Mars
Mars
summer,[102] and contains about 1.6 million cubic kilometres (380,000 cu mi) of ice, which, if spread evenly on the cap, would be 2 km (1.2 mi) thick.[103] (This compares to a volume of 2.85 million cubic kilometres (680,000 cu mi) for the Greenland ice sheet.) The southern polar cap has a diameter of 350 km (220 mi) and a thickness of 3 km (1.9 mi).[104] The total volume of ice in the south polar cap plus the adjacent layered deposits has been estimated at 1.6 million cubic km.[105] Both polar caps show spiral troughs, which recent analysis of SHARAD
SHARAD
ice penetrating radar has shown are a result of katabatic winds that spiral due to the Coriolis Effect.[106][107] The seasonal frosting of areas near the southern ice cap results in the formation of transparent 1-metre-thick slabs of dry ice above the ground. With the arrival of spring, sunlight warms the subsurface and pressure from subliming CO2 builds up under a slab, elevating and ultimately rupturing it. This leads to geyser-like eruptions of CO2 gas mixed with dark basaltic sand or dust. This process is rapid, observed happening in the space of a few days, weeks or months, a rate of change rather unusual in geology – especially for Mars. The gas rushing underneath a slab to the site of a geyser carves a spiderweb-like pattern of radial channels under the ice, the process being the inverted equivalent of an erosion network formed by water draining through a single plughole.[108][109][110][111] Geography and naming of surface features Main article: Geography of Mars For more on how geographic references are determined, see Geodetic datum. See also: Category:Surface features of Mars

A MOLA-based topographic map showing highlands (red and orange) dominating the southern hemisphere of Mars, lowlands (blue) the northern. Volcanic plateaus delimit regions of the northern plains, whereas the highlands are punctuated by several large impact basins.

These new impact craters on Mars
Mars
occurred sometime between 2008 and 2014, as detected from orbit

Although better remembered for mapping the Moon, Johann Heinrich Mädler and Wilhelm Beer
Wilhelm Beer
were the first "areographers". They began by establishing that most of Mars's surface features were permanent and by more precisely determining the planet's rotation period. In 1840, Mädler combined ten years of observations and drew the first map of Mars. Rather than giving names to the various markings, Beer and Mädler simply designated them with letters; Meridian Bay (Sinus Meridiani) was thus feature "a".[112] Today, features on Mars
Mars
are named from a variety of sources. Albedo features are named for classical mythology. Craters larger than 60 km are named for deceased scientists and writers and others who have contributed to the study of Mars. Craters smaller than 60 km are named for towns and villages of the world with populations of less than 100,000. Large valleys are named for the word "Mars" or "star" in various languages; small valleys are named for rivers.[113] Large albedo features retain many of the older names, but are often updated to reflect new knowledge of the nature of the features. For example, Nix Olympica (the snows of Olympus) has become Olympus Mons (Mount Olympus).[114] The surface of Mars
Mars
as seen from Earth
Earth
is divided into two kinds of areas, with differing albedo. The paler plains covered with dust and sand rich in reddish iron oxides were once thought of as Martian
Martian
"continents" and given names like Arabia Terra (land of Arabia) or Amazonis Planitia
Amazonis Planitia
(Amazonian plain). The dark features were thought to be seas, hence their names Mare Erythraeum, Mare Sirenum and Aurorae Sinus. The largest dark feature seen from Earth
Earth
is Syrtis Major Planum.[115] The permanent northern polar ice cap is named Planum Boreum, whereas the southern cap is called Planum Australe. Mars's equator is defined by its rotation, but the location of its Prime Meridian
Prime Meridian
was specified, as was Earth's (at Greenwich), by choice of an arbitrary point; Mädler and Beer selected a line for their first maps of Mars
Mars
in 1830. After the spacecraft Mariner 9
Mariner 9
provided extensive imagery of Mars
Mars
in 1972, a small crater (later called Airy-0), located in the Sinus Meridiani
Sinus Meridiani
("Middle Bay" or "Meridian Bay"), was chosen for the definition of 0.0° longitude to coincide with the original selection.[116] Because Mars
Mars
has no oceans and hence no "sea level", a zero-elevation surface had to be selected as a reference level; this is called the areoid[117] of Mars, analogous to the terrestrial geoid. Zero altitude was defined by the height at which there is 610.5 Pa (6.105 mbar) of atmospheric pressure.[118] This pressure corresponds to the triple point of water, and it is about 0.6% of the sea level surface pressure on Earth
Earth
(0.006 atm).[119] In practice, today this surface is defined directly from satellite gravity measurements. Map of quadrangles For mapping purposes, the United States Geological Survey
United States Geological Survey
divides the surface of Mars
Mars
into thirty "quadrangles", each named for a prominent physiographic feature within that quadrangle.[120][121] The quadrangles can be seen and explored via the interactive image map below.

0°N 180°W / 0°N 180°W / 0; -180 0°N 0°W / 0°N -0°E / 0; -0 90°N 0°W / 90°N -0°E / 90; -0 MC-01 Mare Boreum MC-02 Diacria MC-03 Arcadia MC-04 Mare Acidalium MC-05 Ismenius Lacus MC-06 Casius MC-07 Cebrenia MC-08 Amazonis MC-09 Tharsis MC-10 Lunae Palus MC-11 Oxia Palus MC-12 Arabia MC-13 Syrtis Major MC-14 Amenthes MC-15 Elysium MC-16 Memnonia MC-17 Phoenicis MC-18 Coprates MC-19 Margaritifer MC-20 Sabaeus MC-21 Iapygia MC-22 Tyrrhenum MC-23 Aeolis MC-24 Phaethontis MC-25 Thaumasia MC-26 Argyre MC-27 Noachis MC-28 Hellas MC-29 Eridania MC-30 Mare Australe

The thirty cartographic quadrangles of Mars, defined by the United States Geological Survey.[120][122] The quadrangles are numbered with the prefix "MC" for " Mars
Mars
Chart."[123] Click on a quadrangle name link and you will be taken to the corresponding article. North is at the top; 0°N 180°W / 0°N 180°W / 0; -180 is at the far left on the equator. The map images were taken by the Mars
Mars
Global Surveyor. [view · talk]

Impact topography

Bonneville crater and Spirit rover's lander

The dichotomy of Martian
Martian
topography is striking: northern plains flattened by lava flows contrast with the southern highlands, pitted and cratered by ancient impacts. Research in 2008 has presented evidence regarding a theory proposed in 1980 postulating that, four billion years ago, the northern hemisphere of Mars
Mars
was struck by an object one-tenth to two-thirds the size of Earth's Moon. If validated, this would make the northern hemisphere of Mars
Mars
the site of an impact crater 10,600 by 8,500 km (6,600 by 5,300 mi) in size, or roughly the area of Europe, Asia, and Australia combined, surpassing the South Pole–Aitken basin
South Pole–Aitken basin
as the largest impact crater in the Solar System.[17][18]

Fresh asteroid impact on Mars
Mars
at 3°20′N 219°23′E / 3.34°N 219.38°E / 3.34; 219.38. These before and after images of the same site were taken on the Martian
Martian
afternoons of March 27 and 28, 2012 respectively (MRO)[124]

Mars
Mars
is scarred by a number of impact craters: a total of 43,000 craters with a diameter of 5 km (3.1 mi) or greater have been found.[125] The largest confirmed of these is the Hellas impact basin, a light albedo feature clearly visible from Earth.[126] Due to the smaller mass of Mars, the probability of an object colliding with the planet is about half that of Earth. Mars
Mars
is located closer to the asteroid belt, so it has an increased chance of being struck by materials from that source. Mars
Mars
is more likely to be struck by short-period comets, i.e., those that lie within the orbit of Jupiter.[127] In spite of this, there are far fewer craters on Mars compared with the Moon, because the atmosphere of Mars
Mars
provides protection against small meteors and surface modifying processes have erased some craters. Martian
Martian
craters can have a morphology that suggests the ground became wet after the meteor impacted.[128] Volcanoes

Viking 1
Viking 1
image of Olympus Mons. The volcano and related terrain are approximately 550 km (340 mi) across.

Main article: Volcanology of Mars The shield volcano Olympus Mons
Olympus Mons
(Mount Olympus) is an extinct volcano in the vast upland region Tharsis, which contains several other large volcanoes. Olympus Mons
Olympus Mons
is roughly three times the height of Mount Everest, which in comparison stands at just over 8.8 km (5.5 mi).[129] It is either the tallest or second-tallest mountain in the Solar System, depending on how it is measured, with various sources giving figures ranging from about 21 to 27 km (13 to 17 mi) high.[130][131] Tectonic sites

Valles Marineris
Valles Marineris
(2001 Mars
Mars
Odyssey)

The large canyon, Valles Marineris
Valles Marineris
(Latin for "Mariner Valleys", also known as Agathadaemon in the old canal maps), has a length of 4,000 km (2,500 mi) and a depth of up to 7 km (4.3 mi). The length of Valles Marineris
Valles Marineris
is equivalent to the length of Europe and extends across one-fifth the circumference of Mars. By comparison, the Grand Canyon
Grand Canyon
on Earth
Earth
is only 446 km (277 mi) long and nearly 2 km (1.2 mi) deep. Valles Marineris was formed due to the swelling of the Tharsis
Tharsis
area, which caused the crust in the area of Valles Marineris
Valles Marineris
to collapse. In 2012, it was proposed that Valles Marineris
Valles Marineris
is not just a graben, but a plate boundary where 150 km (93 mi) of transverse motion has occurred, making Mars
Mars
a planet with possibly a two-tectonic plate arrangement.[132][133] Holes Images from the Thermal Emission Imaging System
Thermal Emission Imaging System
(THEMIS) aboard NASA's Mars
Mars
Odyssey orbiter have revealed seven possible cave entrances on the flanks of the volcano Arsia Mons.[134] The caves, named after loved ones of their discoverers, are collectively known as the "seven sisters".[135] Cave
Cave
entrances measure from 100 to 252 m (328 to 827 ft) wide and they are estimated to be at least 73 to 96 m (240 to 315 ft) deep. Because light does not reach the floor of most of the caves, it is possible that they extend much deeper than these lower estimates and widen below the surface. "Dena" is the only exception; its floor is visible and was measured to be 130 m (430 ft) deep. The interiors of these caverns may be protected from micrometeoroids, UV radiation, solar flares and high energy particles that bombard the planet's surface.[136] Atmosphere Main article: Atmosphere
Atmosphere
of Mars

The tenuous atmosphere of Mars
Mars
visible on the horizon

Mars
Mars
lost its magnetosphere 4 billion years ago,[137] possibly because of numerous asteroid strikes,[138] so the solar wind interacts directly with the Martian
Martian
ionosphere, lowering the atmospheric density by stripping away atoms from the outer layer. Both Mars
Mars
Global Surveyor and Mars Express
Mars Express
have detected ionised atmospheric particles trailing off into space behind Mars,[137][139] and this atmospheric loss is being studied by the MAVEN orbiter. Compared to Earth, the atmosphere of Mars
Mars
is quite rarefied. Atmospheric pressure
Atmospheric pressure
on the surface today ranges from a low of 30 Pa (0.030 kPa) on Olympus Mons
Olympus Mons
to over 1,155 Pa (1.155 kPa) in Hellas Planitia, with a mean pressure at the surface level of 600 Pa (0.60 kPa).[140] The highest atmospheric density on Mars
Mars
is equal to that found 35 km (22 mi)[141] above Earth's surface. The resulting mean surface pressure is only 0.6% of that of Earth
Earth
(101.3 kPa). The scale height of the atmosphere is about 10.8 km (6.7 mi),[142] which is higher than Earth's, 6 km (3.7 mi), because the surface gravity of Mars
Mars
is only about 38% of Earth's, an effect offset by both the lower temperature and 50% higher average molecular weight of the atmosphere of Mars. The atmosphere of Mars
Mars
consists of about 96% carbon dioxide, 1.93% argon and 1.89% nitrogen along with traces of oxygen and water.[8][143] The atmosphere is quite dusty, containing particulates about 1.5 µm in diameter which give the Martian
Martian
sky a tawny color when seen from the surface.[144] It may take on a pink hue due to iron oxide particles suspended in it.[15]

Potential sources and sinks of methane (CH 4) on Mars

Methane
Methane
has been detected in the Martian
Martian
atmosphere with a concentration of about 30 ppb;[145][146] it occurs in extended plumes, and the profiles imply that the methane was released from discrete regions. In northern midsummer, the principal plume contained 19,000 metric tons of methane, with an estimated source strength of 0.6 kilograms per second.[147][148] The profiles suggest that there may be two local source regions, the first centered near 30°N 260°W / 30°N 260°W / 30; -260 and the second near 0°N 310°W / 0°N 310°W / 0; -310.[147] It is estimated that Mars
Mars
must produce 270 tonnes per year of methane.[147][149] Methane
Methane
can exist in the Martian
Martian
atmosphere for only a limited period before it is destroyed—estimates of its lifetime range from 0.6–4 years.[147][150] Its presence despite this short lifetime indicates that an active source of the gas must be present. Volcanic activity, cometary impacts, and the presence of methanogenic microbial life forms are among possible sources. Methane
Methane
could be produced by a non-biological process called serpentinization[c] involving water, carbon dioxide, and the mineral olivine, which is known to be common on Mars.[151]

Escaping atmosphere on Mars
Mars
(carbon, oxygen, and hydrogen) by MAVEN in UV[152]

The Curiosity rover, which landed on Mars
Mars
in August 2012, is able to make measurements that distinguish between different isotopologues of methane,[153] but even if the mission is to determine that microscopic Martian
Martian
life is the source of the methane, the life forms likely reside far below the surface, outside of the rover's reach.[154] The first measurements with the Tunable Laser Spectrometer (TLS) indicated that there is less than 5 ppb of methane at the landing site at the point of the measurement.[155][156][157][158] On September 19, 2013, NASA
NASA
scientists, from further measurements by Curiosity, reported no detection of atmospheric methane with a measured value of 6999180000000000000♠0.18±0.67 ppbv corresponding to an upper limit of only 1.3 ppbv (95% confidence limit) and, as a result, conclude that the probability of current methanogenic microbial activity on Mars
Mars
is reduced.[159][160][161] The Mars Orbiter Mission
Mars Orbiter Mission
by India
India
is searching for methane in the atmosphere,[162] while the ExoMars
ExoMars
Trace Gas Orbiter, launched in 2016, would further study the methane as well as its decomposition products, such as formaldehyde and methanol.[163] On December 16, 2014, NASA
NASA
reported the Curiosity rover detected a "tenfold spike", likely localized, in the amount of methane in the Martian
Martian
atmosphere. Sample measurements taken "a dozen times over 20 months" showed increases in late 2013 and early 2014, averaging "7 parts of methane per billion in the atmosphere." Before and after that, readings averaged around one-tenth that level.[164][165] Ammonia was tentatively detected on Mars
Mars
by the Mars
Mars
Express satellite, but with its relatively short lifetime, it is not clear what produced it.[166] Ammonia is not stable in the Martian
Martian
atmosphere and breaks down after a few hours. One possible source is volcanic activity.[166] In September 2017, NASA
NASA
reported radiation levels on the surface of the planet Mars
Mars
were temporarily doubled, and were associated with an aurora 25 times brighter than any observed earlier, due to a massive, and unexpected, solar storm in the middle of the month.[167] Aurora In 1994, the European Space Agency's Mars Express
Mars Express
found an ultraviolet glow coming from "magnetic umbrellas" in the southern hemisphere. Mars does not have a global magnetic field which guides charged particles entering the atmosphere. Mars
Mars
has multiple umbrella-shaped magnetic fields mainly in the southern hemisphere, which are remnants of a global field that decayed billions of years ago. In late December 2014, NASA's MAVEN spacecraft detected evidence of widespread auroras in Mars's northern hemisphere and descended to approximately 20–30 degrees North latitude of Mars's equator. The particles causing the aurora penetrated into the Martian
Martian
atmosphere, creating auroras below 100 km above the surface, Earth's auroras range from 100 km to 500 km above the surface. Magnetic fields in the solar wind drape over Mars, into the atmosphere, and the charged particles follow the solar wind magnetic field lines into the atmosphere, causing auroras to occur outside the magnetic umbrellas.[168] On March 18, 2015, NASA
NASA
reported the detection of an aurora that is not fully understood and an unexplained dust cloud in the atmosphere of Mars.[169] Climate Main article: Climate of Mars

Dust storm
Dust storm
on Mars

November 18, 2012

November 25, 2012

Opportunity and Curiosity rovers are noted.

Of all the planets in the Solar System, the seasons of Mars
Mars
are the most Earth-like, due to the similar tilts of the two planets' rotational axes. The lengths of the Martian
Martian
seasons are about twice those of Earth's because Mars's greater distance from the Sun
Sun
leads to the Martian
Martian
year being about two Earth
Earth
years long. Martian
Martian
surface temperatures vary from lows of about −143 °C (−225 °F) at the winter polar caps[11] to highs of up to 35 °C (95 °F) in equatorial summer.[12] The wide range in temperatures is due to the thin atmosphere which cannot store much solar heat, the low atmospheric pressure, and the low thermal inertia of Martian soil.[170] The planet is 1.52 times as far from the Sun
Sun
as Earth, resulting in just 43% of the amount of sunlight.[171] If Mars
Mars
had an Earth-like orbit, its seasons would be similar to Earth's because its axial tilt is similar to Earth's. The comparatively large eccentricity of the Martian
Martian
orbit has a significant effect. Mars
Mars
is near perihelion when it is summer in the southern hemisphere and winter in the north, and near aphelion when it is winter in the southern hemisphere and summer in the north. As a result, the seasons in the southern hemisphere are more extreme and the seasons in the northern are milder than would otherwise be the case. The summer temperatures in the south can be warmer than the equivalent summer temperatures in the north by up to 30 °C (54 °F).[172] Mars
Mars
has the largest dust storms in the Solar System, reaching speeds of over 160 km/h (100 mph). These can vary from a storm over a small area, to gigantic storms that cover the entire planet. They tend to occur when Mars
Mars
is closest to the Sun, and have been shown to increase the global temperature.[173] Orbit and rotation Main article: Orbit of Mars

Mars
Mars
is about 230 million kilometres (143,000,000 mi) from the Sun; its orbital period is 687 (Earth) days, depicted in red. Earth's orbit is in blue.

Mars's average distance from the Sun
Sun
is roughly 230 million kilometres (143,000,000 mi), and its orbital period is 687 (Earth) days. The solar day (or sol) on Mars
Mars
is only slightly longer than an Earth
Earth
day: 24 hours, 39 minutes, and 35.244 seconds.[174] A Martian
Martian
year is equal to 1.8809 Earth
Earth
years, or 1 year, 320 days, and 18.2 hours.[8] The axial tilt of Mars
Mars
is 25.19 degrees relative to its orbital plane, which is similar to the axial tilt of Earth.[8] As a result, Mars
Mars
has seasons like Earth, though on Mars, they are nearly twice as long because its orbital period is that much longer. In the present day epoch, the orientation of the north pole of Mars
Mars
is close to the star Deneb.[13] Mars
Mars
passed an aphelion in March 2010[175] and its perihelion in March 2011.[176] The next aphelion came in February 2012[176] and the next perihelion came in January 2013.[176] Mars
Mars
has a relatively pronounced orbital eccentricity of about 0.09; of the seven other planets in the Solar System, only Mercury has a larger orbital eccentricity. It is known that in the past, Mars
Mars
has had a much more circular orbit. At one point, 1.35 million Earth
Earth
years ago, Mars
Mars
had an eccentricity of roughly 0.002, much less than that of Earth
Earth
today.[177] Mars's cycle of eccentricity is 96,000 Earth
Earth
years compared to Earth's cycle of 100,000 years.[178] Mars
Mars
has a much longer cycle of eccentricity, with a period of 2.2 million Earth years, and this overshadows the 96,000-year cycle in the eccentricity graphs. For the last 35,000 years, the orbit of Mars
Mars
has been getting slightly more eccentric because of the gravitational effects of the other planets. The closest distance between Earth
Earth
and Mars
Mars
will continue to mildly decrease for the next 25,000 years.[179] Habitability and search for life Main article: Colonization of Mars Search for life Main articles: Life on Mars
Life on Mars
and Viking lander biological experiments

Viking 1
Viking 1
lander's sampling arm scooped up soil samples for tests (Chryse Planitia)

The current understanding of planetary habitability—the ability of a world to develop environmental conditions favorable to the emergence of life—favors planets that have liquid water on their surface. Most often this requires the orbit of a planet to lie within the habitable zone, which for the Sun
Sun
extends from just beyond Venus
Venus
to about the semi-major axis of Mars.[180] During perihelion, Mars
Mars
dips inside this region, but Mars's thin (low-pressure) atmosphere prevents liquid water from existing over large regions for extended periods. The past flow of liquid water demonstrates the planet's potential for habitability. Recent evidence has suggested that any water on the Martian
Martian
surface may have been too salty and acidic to support regular terrestrial life.[181]

Detection of impact glass deposits (green spots) at Alga crater, a possible site for preserved ancient life[182]

This image from Gale crater in 2018 prompted speculation that some shapes were worm-like fossils, but they were geological formations probably formed under water.[183]

The lack of a magnetosphere and the extremely thin atmosphere of Mars are a challenge: the planet has little heat transfer across its surface, poor insulation against bombardment of the solar wind and insufficient atmospheric pressure to retain water in a liquid form (water instead sublimes to a gaseous state). Mars
Mars
is nearly, or perhaps totally, geologically dead; the end of volcanic activity has apparently stopped the recycling of chemicals and minerals between the surface and interior of the planet.[184] In situ investigations have been performed on Mars
Mars
by the Viking landers, Spirit and Opportunity rovers, Phoenix lander, and Curiosity rover. Evidence suggests that the planet was once significantly more habitable than it is today, but whether living organisms ever existed there remains unknown. The Viking probes
Viking probes
of the mid-1970s carried experiments designed to detect microorganisms in Martian
Martian
soil at their respective landing sites and had positive results, including a temporary increase of CO 2 production on exposure to water and nutrients. This sign of life was later disputed by scientists, resulting in a continuing debate, with NASA
NASA
scientist Gilbert Levin asserting that Viking may have found life. A re-analysis of the Viking data, in light of modern knowledge of extremophile forms of life, has suggested that the Viking tests were not sophisticated enough to detect these forms of life. The tests could even have killed a (hypothetical) life form.[185] Tests conducted by the Phoenix Mars lander
Mars lander
have shown that the soil has a alkaline pH and it contains magnesium, sodium, potassium and chloride.[186] The soil nutrients may be able to support life, but life would still have to be shielded from the intense ultraviolet light.[187] A recent analysis of martian meteorite EETA79001 found 0.6 ppm ClO− 4, 1.4 ppm ClO− 3, and 16 ppm NO− 3, most likely of Martian
Martian
origin. The ClO− 3 suggests the presence of other highly oxidizing oxychlorines, such as ClO− 2 or ClO, produced both by UV oxidation of Cl and X-ray radiolysis of ClO− 4. Thus, only highly refractory and/or well-protected (sub-surface) organics or life forms are likely to survive.[188] A 2014 analysis of the Phoenix WCL showed that the Ca(ClO 4) 2 in the Phoenix soil has not interacted with liquid water of any form, perhaps for as long as 600 Myr. If it had, the highly soluble Ca(ClO 4) 2 in contact with liquid water would have formed only CaSO 4. This suggests a severely arid environment, with minimal or no liquid water interaction.[189] Scientists have proposed that carbonate globules found in meteorite ALH84001, which is thought to have originated from Mars, could be fossilized microbes extant on Mars
Mars
when the meteorite was blasted from the Martian
Martian
surface by a meteor strike some 15 million years ago. This proposal has been met with skepticism, and an exclusively inorganic origin for the shapes has been proposed.[190] Small quantities of methane and formaldehyde detected by Mars
Mars
orbiters are both claimed to be possible evidence for life, as these chemical compounds would quickly break down in the Martian atmosphere.[191][192] Alternatively, these compounds may instead be replenished by volcanic or other geological means, such as serpentinization.[151] Impact glass, formed by the impact of meteors, which on Earth
Earth
can preserve signs of life, has been found on the surface of the impact craters on Mars.[193][194] Likewise, the glass in impact craters on Mars
Mars
could have preserved signs of life if life existed at the site.[195][196][197] In May 2017, evidence of the earliest known life on land on Earth
Earth
may have been found in 3.48-billion-year-old geyserite and other related mineral deposits (often found around hot springs and geysers) uncovered in the Pilbara Craton
Pilbara Craton
of Western Australia. These findings may be helpful in deciding where best to search for early signs of life on the planet Mars.[198][199] In early 2018, media reports speculated that certain rock features at a site called Jura looked like a type of fossil, but project scientists say the formations likely resulted from a geological process at the bottom of an ancient drying lakebed, and are related to mineral veins in the area similar to gypsum crystals.[183] Moons Main articles: Moons of Mars, Phobos (moon), and Deimos (moon)

Enhanced-color HiRISE
HiRISE
image of Phobos, showing a series of mostly parallel grooves and crater chains, with Stickney crater at right

Enhanced-color HiRISE
HiRISE
image of Deimos (not to scale), showing its smooth blanket of regolith

Mars
Mars
has two relatively small (compared to Earth's) natural moons, Phobos (about 22 km (14 mi) in diameter) and Deimos (about 12 km (7.5 mi) in diameter), which orbit close to the planet. Asteroid
Asteroid
capture is a long-favored theory, but their origin remains uncertain.[200] Both satellites were discovered in 1877 by Asaph Hall; they are named after the characters Phobos (panic/fear) and Deimos (terror/dread), who, in Greek mythology, accompanied their father Ares, god of war, into battle. Mars
Mars
was the Roman counterpart of Ares.[201][202] In modern Greek, though, the planet retains its ancient name Ares
Ares
(Aris: Άρης).[203] From the surface of Mars, the motions of Phobos and Deimos appear different from that of the Moon. Phobos rises in the west, sets in the east, and rises again in just 11 hours. Deimos, being only just outside synchronous orbit – where the orbital period would match the planet's period of rotation – rises as expected in the east but slowly. Despite the 30-hour orbit of Deimos, 2.7 days elapse between its rise and set for an equatorial observer, as it slowly falls behind the rotation of Mars.[204]

Orbits of Phobos and Deimos (to scale)

Because the orbit of Phobos is below synchronous altitude, the tidal forces from the planet Mars
Mars
are gradually lowering its orbit. In about 50 million years, it could either crash into Mars's surface or break up into a ring structure around the planet.[204] The origin of the two moons is not well understood. Their low albedo and carbonaceous chondrite composition have been regarded as similar to asteroids, supporting the capture theory. The unstable orbit of Phobos would seem to point towards a relatively recent capture. But both have circular orbits, near the equator, which is unusual for captured objects and the required capture dynamics are complex. Accretion early in the history of Mars
Mars
is plausible, but would not account for a composition resembling asteroids rather than Mars itself, if that is confirmed. A third possibility is the involvement of a third body or a type of impact disruption.[205] More-recent lines of evidence for Phobos having a highly porous interior,[206] and suggesting a composition containing mainly phyllosilicates and other minerals known from Mars,[207] point toward an origin of Phobos from material ejected by an impact on Mars
Mars
that reaccreted in Martian
Martian
orbit,[208] similar to the prevailing theory for the origin of Earth's moon. Although the VNIR
VNIR
spectra of the moons of Mars
Mars
resemble those of outer-belt asteroids, the thermal infrared spectra of Phobos are reported to be inconsistent with chondrites of any class.[207] Mars
Mars
may have moons smaller than 50 to 100 metres (160 to 330 ft) in diameter, and a dust ring is predicted to exist between Phobos and Deimos.[20] Exploration Main article: Exploration of Mars

Panorama of Gusev crater, where Spirit rover
Spirit rover
examined volcanic basalts

Mars Science Laboratory
Mars Science Laboratory
under parachute during its atmospheric entry at Mars

Dozens of crewless spacecraft, including orbiters, landers, and rovers, have been sent to Mars
Mars
by the Soviet Union, the United States, Europe, and India
India
to study the planet's surface, climate, and geology. As of 2018[update], Mars
Mars
is host to eight functioning spacecraft: six in orbit—2001 Mars
Mars
Odyssey, Mars
Mars
Express, Mars
Mars
Reconnaissance Orbiter, MAVEN, Mars Orbiter Mission
Mars Orbiter Mission
and ExoMars
ExoMars
Trace Gas Orbiter—and two on the surface— Mars Exploration Rover
Mars Exploration Rover
Opportunity and the Mars Science Laboratory
Mars Science Laboratory
Curiosity. Observations by the Mars Reconnaissance Orbiter have revealed possible flowing water during the warmest months on Mars.[209] In 2013, NASA's Curiosity rover discovered that Mars's soil contains between 1.5% and 3% water by mass (albeit attached to other compounds and thus not freely accessible).[210] The public can request images of Mars
Mars
via the Mars Reconnaissance Orbiter's HiWish program. The Mars
Mars
Science Laboratory, named Curiosity, launched on November 26, 2011, and reached Mars
Mars
on August 6, 2012 UTC. It is larger and more advanced than the Mars
Mars
Exploration Rovers, with a movement rate up to 90 m (300 ft) per hour.[211] Experiments include a laser chemical sampler that can deduce the make-up of rocks at a distance of 7 m (23 ft).[212] On February 10, 2013, the Curiosity rover obtained the first deep rock samples ever taken from another planetary body, using its on-board drill.[213] On September 24, 2014, Mars Orbiter Mission
Mars Orbiter Mission
(MOM), launched by the Indian Space Research Organisation, reached Mars
Mars
orbit. ISRO
ISRO
launched MOM on November 5, 2013, with the aim of analyzing the Martian atmosphere and topography. The Mars Orbiter Mission
Mars Orbiter Mission
used a Hohmann transfer orbit to escape Earth's gravitational influence and catapult into a nine-month-long voyage to Mars. The mission is the first successful Asian interplanetary mission.[214] The European Space Agency, in collaboration with Roscosmos, launched the ExoMars Trace Gas Orbiter
ExoMars Trace Gas Orbiter
and Schiaparelli lander on March 14, 2016.[215] While the Trace Gas Orbiter successfully entered Mars
Mars
orbit on October 19, 2016, Schiaparelli crashed during its landing attempt.[216] Future Main article: Exploration of Mars
Exploration of Mars
§ Timeline of Mars
Mars
exploration

Concept for a Bimodal Nuclear Thermal Transfer Vehicle in low Earth orbit

Planned for May 2018 is the launch of NASA's InSight
InSight
lander, along with the twin MarCO CubeSats that will fly by Mars
Mars
and provide a telemetry relay for the landing. The mission is expected to arrive at Mars
Mars
in November 2018.[217] NASA
NASA
plans to launch its Mars
Mars
2020 astrobiology rover in July or August 2020.[218] The European Space Agency
European Space Agency
will launch the ExoMars rover
ExoMars rover
and surface platform in July 2020.[219] The United Arab Emirates' Mars Hope
Mars Hope
orbiter is planned for launch in 2020, reaching Mars
Mars
orbit in 2021. The probe will make a global study of the Martian
Martian
atmosphere.[220] Several plans for a human mission to Mars
Mars
have been proposed throughout the 20th century and into the 21st century, but no active plan has an arrival date sooner than the 2020s. SpaceX
SpaceX
founder Elon Musk presented a plan in September 2016 to, optimistically, launch space tourists to Mars
Mars
in 2024 at an estimated development cost of US$10 billion.[221] In October 2016, President Barack Obama
Barack Obama
renewed U.S. policy to pursue the goal of sending humans to Mars
Mars
in the 2030s, and to continue using the International Space Station
International Space Station
as a technology incubator in that pursuit.[222][223] The NASA
NASA
Authorization Act of 2017 directed NASA
NASA
to get humans near or on the surface of Mars
Mars
by the early 2030s.[224] Astronomy
Astronomy
on Mars Main article: Astronomy
Astronomy
on Mars See also: Solar eclipses on Mars With the presence of various orbiters, landers, and rovers, it is possible to practice astronomy from Mars. Although Mars's moon Phobos appears about one-third the angular diameter of the full moon on Earth, Deimos appears more or less star-like, looking only slightly brighter than Venus
Venus
does from Earth.[225] Various phenomena seen from Earth
Earth
have also been observed from Mars, such as meteors and auroras.[226] The apparent sizes of the moons Phobos and Deimos are sufficiently smaller than that of the Sun; thus, their partial "eclipses" of the Sun
Sun
are best considered transits (see transit of Deimos and Phobos from Mars).[227][228] Transits of Mercury and Venus
Venus
have been observed from Mars. A transit of Earth
Earth
will be seen from Mars
Mars
on November 10, 2084.[229] On October 19, 2014, Comet
Comet
Siding Spring passed extremely close to Mars, so close that the coma may have enveloped Mars.[230][231][232][233][234][235]

Earth
Earth
and the Moon
Moon
(MRO HiRISE, November 2016)[236]

Phobos transits the Sun
Sun
(Opportunity, March 10, 2004)

Tracking sunspots from Mars

Viewing

Animation of the apparent retrograde motion of Mars
Mars
in 2003 as seen from Earth

Because the orbit of Mars
Mars
is eccentric, its apparent magnitude at opposition from the Sun
Sun
can range from −3.0 to −1.4. The minimum brightness is magnitude +1.6 when the planet is in conjunction with the Sun.[10] Mars
Mars
usually appears distinctly yellow, orange, or red; the actual color of Mars
Mars
is closer to butterscotch, and the redness seen is just dust in the planet's atmosphere. NASA's Spirit rover
Spirit rover
has taken pictures of a greenish-brown, mud-colored landscape with blue-grey rocks and patches of light red sand.[237] When farthest away from Earth, it is more than seven times farther away than when it is closest. When least favorably positioned, it can be lost in the Sun's glare for months at a time. At its most favorable times—at 15- or 17-year intervals, and always between late July and late September—a lot of surface detail can be seen with a telescope. Especially noticeable, even at low magnification, are the polar ice caps.[238] As Mars
Mars
approaches opposition, it begins a period of retrograde motion, which means it will appear to move backwards in a looping motion with respect to the background stars. The duration of this retrograde motion lasts for about 72 days, and Mars
Mars
reaches its peak luminosity in the middle of this motion.[239] Closest approaches Relative The point at which Mars's geocentric longitude is 180° different from the Sun's is known as opposition, which is near the time of closest approach to Earth. The time of opposition can occur as much as 8.5 days away from the closest approach. The distance at close approach varies between about 54[240] and about 103 million km due to the planets' elliptical orbits, which causes comparable variation in angular size.[241] The last Mars
Mars
opposition occurred on May 22, 2016 at a distance of about 76 million km.[242] The next Mars opposition occurs on July 27, 2018 at a distance of about 58 million km.[242] The average time between the successive oppositions of Mars, its synodic period, is 780 days; but the number of days between the dates of successive oppositions can range from 764 to 812.[243] As Mars
Mars
approaches opposition it begins a period of retrograde motion, which makes it appear to move backwards in a looping motion relative to the background stars. The duration of this retrograde motion is about 72 days. Absolute, around the present time

Mars
Mars
oppositions from 2003–2018, viewed from above the ecliptic with Earth
Earth
centered

Mars
Mars
made its closest approach to Earth
Earth
and maximum apparent brightness in nearly 60,000 years, 55,758,006 km (0.37271925 AU; 34,646,419 mi), magnitude −2.88, on August 27, 2003 at 9:51:13 UT. This occurred when Mars
Mars
was one day from opposition and about three days from its perihelion, making it particularly easy to see from Earth. The last time it came so close is estimated to have been on September 12, 57,617 BC, the next time being in 2287.[244] This record approach was only slightly closer than other recent close approaches. For instance, the minimum distance on August 22, 1924 was 7010557775660904950♠0.37285 AU, and the minimum distance on August 24, 2208 will be 7010557685902182530♠0.37279 AU.[178] Historical observations Main article: History of Mars
Mars
observation The history of observations of Mars
Mars
is marked by the oppositions of Mars, when the planet is closest to Earth
Earth
and hence is most easily visible, which occur every couple of years. Even more notable are the perihelic oppositions of Mars, which occur every 15 or 17 years and are distinguished because Mars
Mars
is close to perihelion, making it even closer to Earth. Ancient and medieval observations The ancient Sumerians believed that Mars
Mars
was Nergal, the god of war and plague.[245] During Sumerian times, Nergal
Nergal
was a minor deity of little significance,[245] but, during later times, his main cult center was the city of Nineveh.[245] In Mesopotamian texts, Mars
Mars
is referred to as the "star of judgement of the fate of the dead".[246] The existence of Mars
Mars
as a wandering object in the night sky was recorded by the ancient Egyptian astronomers and, by 1534 BCE, they were familiar with the retrograde motion of the planet.[247] By the period of the Neo-Babylonian Empire, the Babylonian astronomers
Babylonian astronomers
were making regular records of the positions of the planets and systematic observations of their behavior. For Mars, they knew that the planet made 37 synodic periods, or 42 circuits of the zodiac, every 79 years. They invented arithmetic methods for making minor corrections to the predicted positions of the planets.[248][249] In the fourth century BCE, Aristotle
Aristotle
noted that Mars
Mars
disappeared behind the Moon
Moon
during an occultation, indicating that the planet was farther away.[250] Ptolemy, a Greek living in Alexandria,[251] attempted to address the problem of the orbital motion of Mars. Ptolemy's model and his collective work on astronomy was presented in the multi-volume collection Almagest, which became the authoritative treatise on Western astronomy for the next fourteen centuries.[252] Literature from ancient China confirms that Mars
Mars
was known by Chinese astronomers by no later than the fourth century BCE.[253] In the fifth century CE, the Indian astronomical text Surya Siddhanta
Surya Siddhanta
estimated the diameter of Mars.[254] In the East Asian
East Asian
cultures, Mars
Mars
is traditionally referred to as the "fire star" (Chinese: 火星), based on the Five elements.[255][256][257] During the seventeenth century, Tycho Brahe
Tycho Brahe
measured the diurnal parallax of Mars
Mars
that Johannes Kepler
Johannes Kepler
used to make a preliminary calculation of the relative distance to the planet.[258] When the telescope became available, the diurnal parallax of Mars
Mars
was again measured in an effort to determine the Sun- Earth
Earth
distance. This was first performed by Giovanni Domenico Cassini
Giovanni Domenico Cassini
in 1672. The early parallax measurements were hampered by the quality of the instruments.[259] The only occultation of Mars
Mars
by Venus
Venus
observed was that of October 13, 1590, seen by Michael Maestlin
Michael Maestlin
at Heidelberg.[260] In 1610, Mars
Mars
was viewed by Galileo Galilei, who was first to see it via telescope.[261] The first person to draw a map of Mars
Mars
that displayed any terrain features was the Dutch astronomer Christiaan Huygens.[262] Martian
Martian
"canals"

Map of Mars
Mars
by Giovanni Schiaparelli

Mars
Mars
sketched as observed by Lowell before 1914 (south on top)

Map of Mars
Mars
from the Hubble Space Telescope
Telescope
as seen near the 1999 opposition (north on top)

Main article: Martian
Martian
canal By the 19th century, the resolution of telescopes reached a level sufficient for surface features to be identified. A perihelic opposition of Mars
Mars
occurred on September 5, 1877. In that year, the Italian astronomer Giovanni Schiaparelli
Giovanni Schiaparelli
used a 22 cm (8.7 in) telescope in Milan
Milan
to help produce the first detailed map of Mars. These maps notably contained features he called canali, which were later shown to be an optical illusion. These canali were supposedly long, straight lines on the surface of Mars, to which he gave names of famous rivers on Earth. His term, which means "channels" or "grooves", was popularly mistranslated in English as "canals".[263][264] Influenced by the observations, the orientalist Percival Lowell founded an observatory which had 30 and 45 cm (12 and 18 in) telescopes. The observatory was used for the exploration of Mars during the last good opportunity in 1894 and the following less favorable oppositions. He published several books on Mars
Mars
and life on the planet, which had a great influence on the public.[265][266] The canali were independently found by other astronomers, like Henri Joseph Perrotin and Louis Thollon in Nice, using one of the largest telescopes of that time.[267][268] The seasonal changes (consisting of the diminishing of the polar caps and the dark areas formed during Martian
Martian
summer) in combination with the canals led to speculation about life on Mars, and it was a long-held belief that Mars
Mars
contained vast seas and vegetation. The telescope never reached the resolution required to give proof to any speculations. As bigger telescopes were used, fewer long, straight canali were observed. During an observation in 1909 by Flammarion with an 84 cm (33 in) telescope, irregular patterns were observed, but no canali were seen.[269] Even in the 1960s articles were published on Martian
Martian
biology, putting aside explanations other than life for the seasonal changes on Mars. Detailed scenarios for the metabolism and chemical cycles for a functional ecosystem have been published.[270] Spacecraft
Spacecraft
visitation Main article: Exploration of Mars Once spacecraft visited the planet during NASA's Mariner missions in the 1960s and 70s, these concepts were radically broken. The results of the Viking life-detection experiments aided an intermission in which the hypothesis of a hostile, dead planet was generally accepted.[271] Mariner 9
Mariner 9
and Viking allowed better maps of Mars
Mars
to be made using the data from these missions, and another major leap forward was the Mars Global Surveyor mission, launched in 1996 and operated until late 2006, that allowed complete, extremely detailed maps of the Martian topography, magnetic field and surface minerals to be obtained.[272] These maps are available online; for example, at Google Mars. Mars Reconnaissance Orbiter and Mars Express
Mars Express
continued exploring with new instruments, and supporting lander missions. NASA
NASA
provides two online tools: Mars
Mars
Trek, which provides visualizations of the planet using data from 50 years of exploration, and Experience Curiosity, which simulates traveling on Mars
Mars
in 3-D with Curiosity.[273]

In culture Main articles: Mars in culture
Mars in culture
and Mars
Mars
in fiction

Mars
Mars
is named after the Roman god of war. In different cultures, Mars represents masculinity and youth. Its symbol, a circle with an arrow pointing out to the upper right, is used as a symbol for the male gender. The many failures in Mars
Mars
exploration probes resulted in a satirical counter-culture blaming the failures on an Earth- Mars
Mars
"Bermuda Triangle", a " Mars
Mars
Curse", or a "Great Galactic Ghoul" that feeds on Martian
Martian
spacecraft.[274] Intelligent "Martians" Main article: Mars
Mars
in fiction The fashionable idea that Mars
Mars
was populated by intelligent Martians exploded in the late 19th century. Schiaparelli's "canali" observations combined with Percival Lowell's books on the subject put forward the standard notion of a planet that was a drying, cooling, dying world with ancient civilizations constructing irrigation works.[275]

An 1893 soap ad playing on the popular idea that Mars
Mars
was populated

Many other observations and proclamations by notable personalities added to what has been termed " Mars
Mars
Fever".[276] In 1899, while investigating atmospheric radio noise using his receivers in his Colorado Springs lab, inventor Nikola Tesla
Nikola Tesla
observed repetitive signals that he later surmised might have been radio communications coming from another planet, possibly Mars. In a 1901 interview Tesla said:

It was some time afterward when the thought flashed upon my mind that the disturbances I had observed might be due to an intelligent control. Although I could not decipher their meaning, it was impossible for me to think of them as having been entirely accidental. The feeling is constantly growing on me that I had been the first to hear the greeting of one planet to another.[277]

Tesla's theories gained support from Lord Kelvin
Kelvin
who, while visiting the United States in 1902, was reported to have said that he thought Tesla had picked up Martian
Martian
signals being sent to the United States.[278] Kelvin
Kelvin
"emphatically" denied this report shortly before leaving: "What I really said was that the inhabitants of Mars, if there are any, were doubtless able to see New York, particularly the glare of the electricity."[279] In a New York Times
New York Times
article in 1901, Edward Charles Pickering, director of the Harvard College Observatory, said that they had received a telegram from Lowell Observatory
Lowell Observatory
in Arizona
Arizona
that seemed to confirm that Mars
Mars
was trying to communicate with Earth.[280]

Early in December 1900, we received from Lowell Observatory
Lowell Observatory
in Arizona a telegram that a shaft of light had been seen to project from Mars (the Lowell observatory makes a specialty of Mars) lasting seventy minutes. I wired these facts to Europe and sent out neostyle copies through this country. The observer there is a careful, reliable man and there is no reason to doubt that the light existed. It was given as from a well-known geographical point on Mars. That was all. Now the story has gone the world over. In Europe it is stated that I have been in communication with Mars, and all sorts of exaggerations have spring up. Whatever the light was, we have no means of knowing. Whether it had intelligence or not, no one can say. It is absolutely inexplicable.[280]

Pickering later proposed creating a set of mirrors in Texas, intended to signal Martians.[281] In recent decades, the high-resolution mapping of the surface of Mars, culminating in Mars
Mars
Global Surveyor, revealed no artifacts of habitation by "intelligent" life, but pseudoscientific speculation about intelligent life on Mars
Mars
continues from commentators such as Richard C. Hoagland. Reminiscent of the canali controversy, these speculations are based on small scale features perceived in the spacecraft images, such as "pyramids" and the "Face on Mars". Planetary astronomer Carl Sagan
Carl Sagan
wrote:

Mars
Mars
has become a kind of mythic arena onto which we have projected our Earthly hopes and fears.[264]

Martian
Martian
tripod illustration from the 1906 French edition of The War of the Worlds by H. G. Wells

The depiction of Mars in fiction
Mars in fiction
has been stimulated by its dramatic red color and by nineteenth century scientific speculations that its surface conditions might support not just life but intelligent life.[282] Thus originated a large number of science fiction scenarios, among which is H. G. Wells' The War of the Worlds, published in 1898, in which Martians seek to escape their dying planet by invading Earth. Influential works included Ray Bradbury's The Martian
Martian
Chronicles, in which human explorers accidentally destroy a Martian
Martian
civilization, Edgar Rice Burroughs' Barsoom
Barsoom
series, C. S. Lewis' novel Out of the Silent Planet
Planet
(1938),[283] and a number of Robert A. Heinlein
Robert A. Heinlein
stories before the mid-sixties.[284] Jonathan Swift
Jonathan Swift
made reference to the moons of Mars, about 150 years before their actual discovery by Asaph Hall, detailing reasonably accurate descriptions of their orbits, in the 19th chapter of his novel Gulliver's Travels.[285] A comic figure of an intelligent Martian, Marvin the Martian, appeared in Haredevil Hare
Haredevil Hare
(1948) as a character in the Looney Tunes
Looney Tunes
animated cartoons of Warner Brothers, and has continued as part of popular culture to the present.[286] After the Mariner and Viking spacecraft had returned pictures of Mars as it really is, an apparently lifeless and canal-less world, these ideas about Mars
Mars
had to be abandoned, and a vogue for accurate, realist depictions of human colonies on Mars
Mars
developed, the best known of which may be Kim Stanley Robinson's Mars
Mars
trilogy. Pseudo-scientific speculations about the Face on Mars
Face on Mars
and other enigmatic landmarks spotted by space probes have meant that ancient civilizations continue to be a popular theme in science fiction, especially in film.[287] 2018 rediscovery In March 2018, cosmologist Peter Dunsby reported the existence of a very bright optical transient to The Astronomer's Telegram, a messaging service used by astronomers to announce new discoveries.[288] The object was quickly identified as the planet Mars, and an erratum issued.[289][290] The incident caught the attention of the Internet, and The Astronomer's Telegram issued Professor Dunsby a certificate via Twitter for his "discovery", which Professor Dunsby accepted in good humour, saying "The world needs to smile more, so that's something good that has come out of this episode."[291][292] See also

Book: Mars Book: Solar System

Outline of Mars List of missions to Mars

Mars
Mars
portal Solar System
Solar System
portal

Notes

^ This image was taken by the Rosetta spacecraft's Optical, Spectroscopic, and Infrared Remote Imaging System (OSIRIS), at a distance of ≈240,000 kilometres (150,000 mi) during its February 2007 encounter. The view is centered on the Aeolis quadrangle, with Gale crater, the landing site of the Curiosity rover, prominently visible just left of center. The darker, more heavily cratered terrain in the south, Terra Cimmeria, is composed of older terrain than the much smoother and brighter Elysium Planitia
Elysium Planitia
to the north. Geologically recent processes, such as the possible existence of a global ocean in Mars's past, could have helped lower-elevated areas, such as Elysium Planitia, retain a more youthful look. ^ a b c Best-fit ellipsoid ^ There are many serpentinization reactions. Olivine
Olivine
is a solid solution between forsterite and fayalite whose general formula is (Fe,Mg) 2SiO 4. The reaction producing methane from olivine can be written as: Forsterite
Forsterite
+ Fayalite
Fayalite
+ Water + Carbonic acid → Serpentine + Magnetite + Methane, or (in balanced form): 18Mg 2SiO 4 + 6Fe 2SiO 4 + 26H 2O + CO 2 → 12Mg 3Si 2O 5(OH) 4 + 4Fe 3O 4 + CH 4.

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and Earth: The Top 10 Close Passes Since 3000 B.C." Space.com. Archived from the original on May 20, 2009. Retrieved June 13, 2006.  ^ a b c Rabkin, Eric S. (2005). Mars: A Tour of the Human Imagination. Westport, Connecticut: Praeger. pp. 9–11. ISBN 0-275-98719-1.  ^ Thompson, Henry O. (1970). Mekal: The God of Beth-Shan. Leiden, Germany: E. J. Brill. p. 125.  ^ Novakovic, B. (2008). "Senenmut: An Ancient Egyptian Astronomer". Publications of the Astronomical Observatory of Belgrade. 85: 19–23. arXiv:0801.1331 . Bibcode:2008POBeo..85...19N.  ^ North, John David (2008). Cosmos: an illustrated history of astronomy and cosmology. University of Chicago Press. pp. 48–52. ISBN 0-226-59441-6.  ^ Swerdlow, Noel M. (1998). "Periodicity and Variability of Synodic Phenomenon". The Babylonian theory of the planets. Princeton University Press. pp. 34–72. ISBN 0-691-01196-6.  ^ Poor, Charles Lane (1908). The solar system: a study of recent observations. Science series. 17. G. P. Putnam's sons. p. 193.  ^ Harland, David Michael (2007). "Cassini at Saturn: Huygens results". p. 1. ISBN 0-387-26129-X ^ Hummel, Charles E. (1986). The Galileo connection: resolving conflicts between science & the Bible. InterVarsity Press. pp. 35–38. ISBN 0-87784-500-X. ^ Needham, Joseph; Ronan, Colin A. (1985). The Shorter Science and Civilisation in China: An Abridgement of Joseph Needham's Original Text. The shorter science and civilisation in China. 2 (3rd ed.). Cambridge University Press. p. 187. ISBN 0-521-31536-0.  ^ Thompson, Richard (1997). "Planetary Diameters in the Surya-Siddhanta" (PDF). Journal of Scientific Exploration. 11 (2): 193–200 [193–6]. Archived from the original (PDF) on January 7, 2010. Retrieved March 13, 2010.  ^ de Groot, Jan Jakob Maria (1912). "Fung Shui". Religion in China – Universism: A Key to the Study of Taoism and Confucianism. American Lectures on the History of Religions, volume 10. G. P. Putnam's Sons. p. 300. OCLC 491180.  ^ Crump, Thomas (1992). The Japanese Numbers Game: The Use and Understanding of Numbers in Modern Japan. Nissan Institute/Routledge Japanese Studies Series. Routledge. pp. 39–40. ISBN 0-415-05609-8.  ^ Hulbert, Homer Bezaleel (1909) [1906]. The Passing of Korea. Doubleday, Page & Company. p. 426. OCLC 26986808.  ^ Taton, Reni (2003). Reni Taton, Curtis Wilson and Michael Hoskin, eds. Planetary Astronomy
Astronomy
from the Renaissance to the Rise of Astrophysics, Part A, Tycho Brahe
Tycho Brahe
to Newton. Cambridge University Press. p. 109. ISBN 0-521-54205-7. CS1 maint: Uses editors parameter (link) ^ Hirshfeld, Alan (2001). Parallax: the race to measure the cosmos. Macmillan. pp. 60–61. ISBN 0-7167-3711-6.  ^ Breyer, Stephen (1979). "Mutual Occultation
Occultation
of Planets". Sky and Telescope. 57 (3): 220. Bibcode:1979S&T....57..220A.  ^ Peters, W. T. (1984). "The Appearance of Venus
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in 1610". Journal of the History of Astronomy. 15 (3): 211–214. Bibcode:1984JHA....15..211P.  ^ Sheehan, William (1996). "2: Pioneers". The Planet
Planet
Mars: A History of Observation and Discovery. uapress.arizona.edu. Tucson: University of Arizona. Retrieved January 16, 2010.  ^ Snyder, Dave (May 2001). "An Observational History of Mars". Retrieved February 26, 2007.  ^ a b Sagan, Carl (1980). Cosmos. New York City: Random House. p. 107. ISBN 0-394-50294-9.  ^ Basalla, George (2006). "Percival Lowell: Champion of Canals". Civilized Life in the Universe: Scientists on Intelligent Extraterrestrials. Oxford University Press US. pp. 67–88. ISBN 0-19-517181-0.  ^ Dunlap, David W. (October 1, 2015). "Life on Mars? You Read It Here First". The New York Times. Retrieved October 1, 2015.  ^ Maria, K.; Lane, D. (2005). "Geographers of Mars". Isis. 96 (4): 477–506. doi:10.1086/498590. PMID 16536152.  ^ Perrotin, M. (1886). "Observations des canaux de Mars". Bulletin Astronomique, Serie I (in French). 3: 324–329. Bibcode:1886BuAsI...3..324P.  ^ Zahnle, K. (2001). "Decline and fall of the Martian
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empire". Nature. 412 (6843): 209–213. doi:10.1038/35084148. PMID 11449281.  ^ Salisbury, F. B. (1962). " Martian
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Mars
to a New Generation". Retrieved August 5, 2015.  ^ Dinerman, Taylor (September 27, 2004). "Is the Great Galactic Ghoul losing his appetite?". The space review. Retrieved March 27, 2007.  ^ "Percivel Lowell's Canals". Archived from the original on February 19, 2007. Retrieved March 1, 2007.  ^ Fergus, Charles (2004). " Mars
Mars
Fever". Research/Penn State. 24 (2). Archived from the original on August 31, 2003. Retrieved August 2, 2007.  ^ Tesla, Nikola (February 9, 1901). "Talking with the Planets". Collier's. Vol. 26 no. 19. pp. 4–5.  ^ Cheney, Margaret (1981). Tesla: Man Out of Time. Englewood Cliffs, New Jersey: Prentice-Hall. p. 162. ISBN 978-0-13-906859-1. OCLC 7672251.  ^ "Departure of Lord Kelvin". The New York Times. May 11, 1902. p. 29.  ^ a b Pickering, Edward Charles (January 16, 1901). "The Light Flash From Mars" (PDF). The New York Times. Archived from the original (PDF) on June 5, 2007. Retrieved May 20, 2007.  ^ Fradin, Dennis Brindell (1999). Is There Life on Mars?. McElderry Books. p. 62. ISBN 0-689-82048-8.  ^ Lightman, Bernard V. (1997). Victorian Science in Context. University of Chicago Press. pp. 268–273. ISBN 0-226-48111-5.  ^ Schwartz, Sanford (2009). C. S. Lewis
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External links

Find more aboutMarsat's sister projects

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at Curlie (based on DMOZ) Mars Exploration Program
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Images

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images by NASA's Mars
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Videos

Rotating color globe of Mars
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by the United States Geological Survey NASA's Curiosity Finds Ancient Streambed – First Evidence of Water on Mars
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on YouTube
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by The Science Channel (2012, 4:31) Flight Into Mariner Valley by Arizona
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and Tharsis
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(see album for more)

Cartographic resources

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nomenclature and quadrangle maps with feature names by the United States Geological Survey Geological map of Mars
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Regions

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Physical Features

Canyons Catenae Chaos terrain Craters Fossae Gullies Mensae Labyrinthi Mountains

by height

Observed rocks Outflow channels Plains Valley network Valleys Gravity

Geology

Brain terrain Canals (list) Carbonates Chaos terrain Color Composition Concentric crater fill Dark slope streak Dichotomy Fretted terrain Geysers Glaciers Groundwater Gullies Lakes Lava tubes Lobate debris apron Meteorites

on Earth on Mars

North Polar Basin Ocean hypothesis Ore resources Polar caps Recurring slope lineae
Recurring slope lineae
(RSL) Ring mold craters Rootless cones Seasonal flows Soil Spherules Surface "Swiss cheese" feature Terrain softening Tharsis
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bulge Volcanology Water Yardangs

History

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Astronomy

Moons

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Deimos

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Transits

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5261 Eureka 1998 VF31 1999 UJ7 2007 NS2

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close approach, 19 Oct 2014)

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Proposed

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Simulations

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Related

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scientist Mythology Phobos and Deimos in fiction

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Geography and geology of Mars

Cartography

Regions

Arabia Terra Cerberus Hemisphere Cydonia Eridania Lake Iani Chaos Olympia Undae Planum Australe Planum Boreum Quadrangles Sinus Meridiani Tempe Terra Terra Cimmeria Terra Sabaea Tharsis Undae Ultimi Scopuli Vastitas Borealis

Quadrangles

Aeolis Amazonis Amenthes Arabia Arcadia Argyre Casius Cebrenia Coprates Diacria Elysium Eridania Hellas Iapygia Ismenius Lacus Lunae Palus Mare Acidalium Mare Australe (South Pole) Mare Boreum (North Pole) Mare Tyrrhenum Margaritifer Sinus Memnonia Noachis Oxia Palus Phaethontis Phoenicis Lacus Sinus Sabaeus Syrtis Major Tharsis Thaumasia

Geology

Overview

Brain terrain Canals (list) Carbonates Chaos terrain Color Composition Concentric crater fill Dark slope streak Dichotomy Fretted terrain Geysers Glaciers Groundwater Gullies Lakes Lava tubes Lobate debris apron North Polar Basin Ocean hypothesis Ore resources Polar caps Recurring slope lineae
Recurring slope lineae
(RSL) Ring mold craters Rootless cones Seasonal flows Soil Spherules Surface "Swiss cheese" feature Terrain softening Tharsis
Tharsis
bulge Water Yardangs

History

Amazonian Hesperian Noachian Observation history Classical albedo features

Rocks observed

Curiosity

Bathurst Inlet Coronation Goulburn Hottah Jake Matijevic Link Rocknest Rocknest 3 Tintina

Opportunity

Bounce El Capitan Last Chance

Sojourner

Barnacle Bill Yogi

Spirit

Adirondack Home Plate Mimi Pot of Gold

Viking

Big Joe

Other

Face Monolith

Meteorites found on Mars

Block Island Heat Shield Mackinac Island Meridiani Planum Oileán Ruaidh Shelter Island

Martian
Martian
meteorites found on Earth

Balsaltic Breccia Chassignites Nakhlites Shergottites Other List

Topography

Mountains and volcanoes

Acidalia Colles Alba Mons Albor Tholus Anseris Mons Apollinaris Mons Arsia Mons Ascraeus Mons Astapus Colles Ausonia Montes Biblis Tholus Centauri Montes Ceraunius Tholus Charitum Montes Columbia Hills Echus Montes Elysium Elysium Mons Erebus Montes Galaxius Mons Hadriacus Mons Hellas Montes Hecates Tholus Jovis Tholus Libya Montes Mount Sharp Nereidum Montes Olympus Mons Orcus Patera Pavonis Mons Peneus Patera Phlegra Montes Pityusa Patera Syrtis Major Planum Tartarus Montes Tharsis Tharsis
Tharsis
Montes Tharsis
Tharsis
Tholus Tholus Tyrrhenus Mons Ulysses Tholus Uranius group Uranius Mons Uranius Tholus Volcanology By height

Plains and plateaus

Acidalia Planitia Aeolis Palus Amazonis Planitia Arcadia Planitia Argyre Planitia Chryse Planitia Daedalia Planum Elysium Planitia Eridania Planitia Hellas Planitia Hesperia Planum Icaria Planum Isidis Planitia Lunae Planum Meridiani Planum Oxia Planum Planum Australe Planum Boreum Syria Planum Syrtis Major Planum Utopia Planitia

Canyons and valleys

Aram Chaos Arsia Chasmata Aromatum Chaos Atlantis Chaos Aureum Chaos Candor Chasma Chasma Boreale Coprates Chasma Echus Chasma Eos Chaos Eos Chasma Galaxias Chaos Ganges Chasma Gorgonum Chaos Hebes Chasma Hydaspis Chaos Hydraotes Chaos Iani Chaos Ister Chaos Ius Chasma Juventae Chasma Melas Chasma Ophir Chasma Tithonium Chasma Apsus Ares Arnus Asopus Athabasca Auqakuh Bahram Buvinda Dao Enipeus Frento Harmakhis Hebrus Hrad Huo Hsing Hypanis Iberus Indus Ituxi Kasei Labou Ladon Lethe Licus Ma'adam Mad Maja Mamers Mangala Marineris Marte Mawrth Minio Naktong Nanedi Niger Nirgal Padus Paraná Patapsco Peace Rahway Ravi Reull Sabis Samara Scamander Shalbatana Simud Stura Tader Tinia Tiu Tyras Uzboi Verde Warrego Olympus Rupes Gullies Outflow channels Valley networks

Fossae, mensae and labyrinthi

Amenthes Fossae Ceraunius Fossae Cerberus Fossae Coloe Fossae Cyane Fossae Elysium Fossae Galaxias Fossae Hephaestus Fossae Icaria Fossae Labeatis Fossae Mangala Fossa Mareotis Fossae Medusae Fossae Memnonia Fossae Nili Fossae Olympica Fossae Oti Fossae Sirenum Fossae Tantalus Fossae Tithonium Fossae Tractus Fossae Aeolis Mensae Capri Mensa Cydonia Mensae Deuteronilus Mensae Ganges Mensa Nilosyrtis Mensae Protonilus Mensae Sacra Mensa Angustus Labyrinthus Noctis Labyrinthus

Catenae and craters

Artynia Catena Tithoniae Catenae Tractus Catena Adams Agassiz Airy Airy-0 Aniak Antoniadi Arandas Argo Arkhangelsky Arrhenius Asimov Bacolor Bakhuysen Baldet Baltisk Bamberg Barabashov Barnard Beagle Becquerel Beer Belz Bernard Bianchini Boeddicker Bok Bond Bonestell Bonneville Brashear Briault Burroughs Burton Campbell Canso Cassini Caxias Cerulli Chafe Chapais Chincoteague Clark Coblentz Columbus Copernicus Corby Crewe Crivitz Crommelin Cruls Curie Da Vinci Danielson Darwin Davies Dawes Dejnev Denning Dilly Dinorwic Douglass Dromore Du Martheray Eagle Eberswalde Eddie Ejriksson Emma Dean Endeavour Endurance Erebus Escalante Eudoxus Fenagh Fesenkov Firsoff Flammarion Flaugergues Focas Fontana Fournier Fram Galdakao Gale Galle Garni Gasa Gilbert Gill Gledhill Gold Graff Green Grindavik Gusev Hadley Haldane Hale Halley Hartwig Heaviside Heimdal Heinlein Helmholtz Henry Herschel Hipparchus Holden Holmes Hooke Huggins Hussey Hutton Huxley Huygens Iazu Ibragimov Inuvik Janssen Jarry-Desloges Jeans Jezero Jezža Joly Jones Kaiser Keeler Kepler Kinkora Kipini Knobel Koga Korolev Kufra Kuiper Kunowsky Lambert Lamont Lampland Lassell Lau Le Verrier Li Fan Liais Lipik Liu Hsin Llanesco Lockyer Lod Lohse Lomonosov Lowell Lyell Lyot Mädler Magelhaens Maggini Main Mandora Maraldi Mariner Marth Martz Masursky Maunder McLaughlin McMurdo Mellish Mendel Mie Milankovic Millochau Mitchel Miyamoto Mohawk Mojave Molesworth Montevallo Moreux Müller Nansen Nereus Newton Nhill Nicholson Niesten Nipigon Onon Orson Welles Oudemans Palana Pangboche Pasteur Penticton Perepelkin Peridier Persbo Pettit Phillips Pickering Playfair Pollack Poona Porter Porth Priestley Proctor Ptolemaeus Púnsk Quenisset Rabe Radau Rahe Rayleigh Redi Renaudot Reuyl Reynolds Richardson Ritchey Robert Sharp Roddenberry Ross Rossby Rudaux Russell Rutherford Sagan Saheki Santa Maria Schaeberle Schiaparelli Schmidt Secchi Semeykin Sharonov Sibu Sinton Sitka Sklodowska Slipher Smith South Spallanzani Srīpur Steno Stokes Stoney Suess Suzhi Tarsus Taytay Teisserenc de Bort Terby Thila Thira Tikhonravov Tikhov Timbuktu Tombaugh Tooting Trouvelot Troy Trud Trumpler Tugaske Tycho Brahe Tyndall Udzha Vernal Very Victoria Vinogradov Vinogradsky Virrat Vishniac Vogel Von Kármán Wallace Wegener Weinbaum Wells Williams Winslow Wirtz Wislicenus Wright Yuty Zumba Zunil

v t e

Spacecraft
Spacecraft
missions to Mars

Current

Orbiters

ExoMars
ExoMars
Trace Gas Orbiter Mangalyaan Mars
Mars
Express Mars
Mars
Reconnaissance Orbiter MAVEN 2001 Mars
Mars
Odyssey

Rovers

Curiosity

timeline

Opportunity

observations

Past

Flybys

Dawn Mariner 4 Mariner 6 Mariner 7 Mars
Mars
1† Mars
Mars
6 Mars
Mars
7 Nozomi† Rosetta Zond 2†

Orbiters

Mariner 9 Mars
Mars
2 Mars
Mars
3 Mars
Mars
4† Mars
Mars
5† Mars
Mars
Climate Orbiter† Mars
Mars
Global Surveyor Mars
Mars
Observer† Phobos program

Phobos 1† Phobos 2†

Viking program

Viking 1 Viking 2

Landers

Beagle 2† ExoMars
ExoMars
Schiaparelli† Mars
Mars
2† Mars
Mars
3† Mars
Mars
6† Mars
Mars
7† Mars
Mars
Pathfinder Mars
Mars
Polar Lander† / Deep Space 2† Phoenix Viking 1 Viking 2

Rovers

Prop-M† Sojourner Spirit

observations

Special

Zond 3
Zond 3
(crossed Mars
Mars
orbit)

Failed launch

Fobos-Grunt
Fobos-Grunt
/ Yinghuo-1 Kosmos 419 1M No.1 1M No.2 2MV-4 No.1 2MV-3 No.1 Mariner 3 2M No.521 2M No.522 Mariner 8 Mars
Mars
96

Planned

InSight
InSight
(2018)

Mars
Mars
Cube One

Hope Mars Mission
Hope Mars Mission
(2020) ExoMars
ExoMars
(2020)

rover surface platform

Mars 2020
Mars 2020
(2020)

NASA
NASA
Mars
Mars
Helicopter Scout

Mars
Mars
Global Remote Sensing Orbiter and Small Rover (2020) Mars Terahertz Microsatellite
Mars Terahertz Microsatellite
(2020) Mars Orbiter Mission
Mars Orbiter Mission
2 (2021 or 2022) Psyche (2023, flyby only) MMX (2024)

Proposed

BOLD Icebreaker Life Inspiration Mars Mars
Mars
2022 Mars
Mars
Geyser
Geyser
Hopper Mars-Grunt Mars
Mars
Micro Orbiter‎ Mars
Mars
One Mars
Mars
sample return mission MELOS
MELOS
rover MetNet Northern Light PADME Phootprint SCIM Sky-Sailor

Cancelled / concepts

ARES Astrobiology
Astrobiology
Field Laboratory Beagle 3 Mars 4NM
Mars 4NM
& 5NM Mars 5M
Mars 5M
(Mars-79) Mars-Aster Mars
Mars
Astrobiology
Astrobiology
Explorer-Cacher Mars
Mars
Surveyor Lander Mars
Mars
Telecommunications Orbiter NetLander Red Dragon Vesta Voyager

Related

Colonization of Mars Exploration of Mars List of artificial objects on Mars List of Mars
Mars
orbiters Mars
Mars
race Terraforming of Mars

† indicates failure en route or before intended mission data returned.

v t e

Human missions to Mars

List of human Mars
Mars
mission plans

21st-century proposals

Aurora
Aurora
programme Austere Human Missions to Mars Chinese mission to Mars Constellation program Inspiration Mars Mars
Mars
Base Camp Mars
Mars
One Mars
Mars
Piloted Orbital Station Mars
Mars
to Stay SpaceX
SpaceX
Mars
Mars
transportation infrastructure Vision for Space Exploration

20th-century proposals

The Mars
Mars
Project Martian
Martian
Piloted Complex TMK Ride Report Space Exploration Initiative Mars
Mars
Direct The Case for Mars Mars
Mars
Design Reference Mission

3.0

Mars
Mars
analogs (list)

MARS-500 Mars
Mars
Analogue Research Station Program

FMARS MDRS Euro-MARS MARS-Oz

Arctic Mars
Mars
Analog Svalbard Expedition Concordia Station HI-SEAS NEEMO

Advocacy

Caves of Mars
Mars
Project ICAMSR Mars
Mars
Institute Mars
Mars
Society

Hardware concepts

Mars
Mars
habitat Crewed Mars
Mars
rover Mars
Mars
suit Mars
Mars
Excursion Module Mars
Mars
cycler Mars
Mars
lander Mars
Mars
rover

Miscellaneous

Colonization of Mars Exploration of Mars Fiction

Films Novels

Mars
Mars
orbit rendezvous Terraforming of Mars Mars
Mars
atmospheric entry Mars
Mars
flyby

v t e

The Solar System

The Sun Mercury Venus Earth Mars Ceres Jupiter Saturn Uranus Neptune Pluto Haumea Makemake Eris

Planets

Terrestrial planets

Mercury Venus Earth Mars

Giant planets

Jupiter Saturn Uranus Neptune

Dwarf planets

Ceres Pluto Haumea Makemake Eris

Rings

Jovian Saturnian (Rhean) Charikloan Chironean Uranian Neptunian Haumean

Moons

Terrestrial

Moon other near- Earth
Earth
objects

Martian

Phobos Deimos

Jovian

Ganymede Callisto Io Europa all 69

Saturnian

Titan Rhea Iapetus Dione Tethys Enceladus Mimas Hyperion Phoebe all 62

Uranian

Titania Oberon Umbriel Ariel Miranda all 27

Neptunian

Triton Proteus Nereid all 14

Plutonian

Charon Nix Hydra Kerberos Styx

Haumean

Hiʻiaka Namaka

Makemakean

S/2015 (136472) 1

Eridian

Dysnomia

Lists

Solar System
Solar System
objects

By size By discovery date

Minor planets Gravitationally rounded objects Possible dwarf planets Natural satellites Comets

Small Solar System bodies

Meteoroids Minor planets

moons

Comets Damocloids Mercury-crossers Venus-crossers Venus
Venus
trojans Near- Earth
Earth
objects Earth-crossers Earth
Earth
trojans Mars-crossers Mars
Mars
trojans Asteroid
Asteroid
belt Asteroids

first discovered: Ceres Pallas Juno Vesta

Families Notable asteroids Kirkwood gap Main-belt comets Jupiter
Jupiter
trojans Jupiter-crossers Centaurs Saturn-crossers Uranus
Uranus
trojans Uranus-crossers Neptune
Neptune
trojans Cis-Neptunian objects Trans-Neptunian objects Neptune-crossers Plutoids Kuiper belt

Plutinos Cubewanos

Scattered disc Detached objects Sednoids Hills cloud Oort cloud

Hypothetical objects

Vulcan Vulcanoids Phaeton Planet
Planet
V Theia Fifth giant Planets beyond Neptune Tyche Nemesis Planet
Planet
Nine

Exploration (outline)

Discovery

Astronomy Timeline

Spaceflight Robotic spacecraft Human spaceflight List of crewed spacecraft Colonization List of probes Timeline

Mercury Venus Moon Mars Ceres Asteroids

Mining

Comets Jupiter Saturn Uranus Neptune Pluto Deep space

Outline of the Solar System Portals Solar System Astronomy Earth
Earth
sciences Mars Jupiter Uranus Cosmology

Solar System → Local Interstellar Cloud → Local Bubble → Gould Belt → Orion Arm → Milky Way → Milky Way
Milky Way
subgroup → Local Group → Virgo Supercluster → Laniakea Supercluster → Observable universe → Universe Each arrow (→) may be read as "within" or "part of".

Authority control

WorldCat Identities VIAF: 316741886 LCCN: sh85081548 GND: 4037687-4 SUDOC: 029043387 BNF: cb120752119 (d

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