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Exploration of Mars

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Not to be confused with Human mission to Mars or Colonization of Mars.
Self-portrait of Perseverance rover and Ingenuity helicopter (to the left) located at Wright Brothers Field, the Ingenuity helicopter drop site (7 April 2021)
Active Mars missions, 1997 to presentα
Year Number of missions
1997
2
1998
1
1999
1
2000
1
2001
2
2002
2
2003
3
2004
5
2005
5
2006
6
2007
5
2008
6
2009
5
2010
5
2011
4
2012
5
2013
5
2014
7
2015
7
2016
8
2017
8
2018
9
2019
8
2020
8
2021
11
2022
11
2023
10

The planet Mars has been explored remotely by spacecraft. Probes sent from Earth, beginning in the late 20th century, have yielded a large increase in knowledge about the Martian system, focused primarily on understanding its geology and habitability potential.[1][2] Engineering interplanetary journeys is complicated and the exploration of Mars has experienced a high failure rate, especially the early attempts. Roughly sixty percent of all spacecraft destined for Mars failed before completing their missions, with some failing before their observations could begin. Some missions have been met with unexpected success, such as the twin Mars Exploration Rovers, Spirit and Opportunity, which operated for years beyond their specification.[3]

Current status

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There are two functional rovers on the surface of Mars, the Curiosity and Perseverance rovers, both operated by the American space agency NASA. Perseverance was accompanied by the Ingenuity helicopter, which scouted sites for Perseverance to study before the helicopter's mission ended in 2024.[4] The Zhurong rover, part of the Tianwen-1 mission by the China National Space Administration (CNSA)[5][6] was active until 20 May 2022 when it went into hibernation due to approaching sandstorms and Martian winter; the rover was expected to awaken from hibernation in December 2022, but as of April 2023 it has not moved and is presumed to be permanently inactive.[7]

There are seven orbiters surveying the planet: Mars Odyssey, Mars Express, Mars Reconnaissance Orbiter, MAVEN, the Trace Gas Orbiter, the Hope Mars Mission, and the Tianwen-1 orbiter, which have contributed massive amounts of information about Mars. Thus there are nine total vehicles currently exploring Mars: 2 rovers and 7 orbiters.

Various Mars sample return missions are being planned like NASA-ESA Mars Sample Return that will pick up the samples currently being collected by the Perseverance rover.[8]

In April 2024, NASA selected several companies to begin studies on providing commercial services to further enable robotic science on Mars.[9]

Martian system

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Main articles: Mars, Martian surface, Atmosphere of Mars, and Moons of Mars

Mars has long been the subject of human interest. Early telescopic observations revealed color changes on the surface that were attributed to seasonal vegetation and apparent linear features were ascribed to intelligent design. Further telescopic observations found two moons, Phobos and Deimos, polar ice caps and the feature now known as Olympus Mons, the Solar System's tallest mountain. The discoveries piqued further interest in the study and exploration of the red planet. Mars is a rocky planet, like Earth, that formed around the same time, yet with only half the diameter of Earth, and a thin atmosphere; it has a cold and desert-like surface.[10]

One way the surface of Mars has been categorized, is by thirty "quadrangles", with each quadrangle named for a prominent physiographic feature within that quadrangle.[11][12]

Mars Quad Map
0°N 180°W / 0°N 180°W / 0; -180
Mars Quad Map
The image above contains clickable linksClickable image of the 30 cartographic quadrangles of Mars, defined by the USGS.[11][13] Quadrangle numbers (beginning with MC for "Mars Chart")[14] and names link to the corresponding articles. 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 Global Surveyor.
(
)

Launch windows

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Spacecraft launches and Mars distance from Earth in millions of kilometers

The minimum-energy launch windows for a Martian expedition occur at intervals of approximately two years and two months (specifically 780 days, the planet's synodic period with respect to Earth).[15] In addition, the lowest available transfer energy varies on a roughly 16-year cycle.[15] For example, a minimum occurred in the 1969 and 1971 launch windows, rising to a peak in the late 1970s, and hitting another low in 1986 and 1988.[15]

Launch opportunities[16][17][18]
Year Window Spacecraft (launched or planned)
2013 Nov MAVEN, Mars Orbiter Mission
2016 Mar ExoMars TGO
2018 May InSight
2020 Jul–Sep (1) Mars Hope orbiter
(2) Tianwen-1 orbiter, deployable and remote camera, lander and Zhurong rover
(3) Mars 2020 Perseverance rover and Ingenuity helicopter
2022 Aug–Nov none
2024 Oct–Nov none
2026 Nov–Dec (1) Martian Moons eXploration (MMX)[19]

(2) Impulse/Relativity Mars lander[20]

2028/

2029

Dec–Jan (1) Rosalind Franklin
(2) Mars Orbiter Mission 2

Past missions

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Main article: List of missions to Mars
Launches to Mars
Decade
1960s
13
1970s
11
1980s
2
1990s
8
2000s
8
2010s
6
2020s
3

Starting in 1960, the Soviet space program launched a series of probes to Mars including the first intended (but unsuccessful) flybys and hard (impact) landing (Mars 1962B),[21] and the first successful soft landing (Mars 3). The first successful flyby of Mars was on 14–15 July 1965, by NASA's Mariner 4.[22] On November 14, 1971, Mariner 9 became the first space probe to orbit another planet when it entered into orbit around Mars.[23] The amount of data returned by probes increased substantially as technology improved.[21]

The first to contact the surface were two Soviet probes: Mars 2 lander on November 27 and Mars 3 lander on December 2, 1971—Mars 2 failed during descent and Mars 3 failed about twenty seconds after the first Martian soft landing.[24] Mars 6 failed during descent but did return some corrupted atmospheric data in 1974.[25] The 1975 NASA launches of the Viking program consisted of two orbiters, each with a lander that successfully soft landed in 1976. Viking 1 remained operational for six years, Viking 2 for three years. The Viking landers relayed the first color panoramas of Mars.[26]

The Soviet probes Phobos 1 and 2 were sent to Mars in 1988 to study Mars and its two moons, with a focus on Phobos. Phobos 1 lost contact on the way to Mars. Phobos 2, while successfully photographing Mars and Phobos, failed before it was set to release two landers to the surface of Phobos.[27]

Missions that ended prematurely after Phobos 1 and 2 (1988) include (see Probe difficulties section for more details):

Following the 1993 failure of the Mars Observer orbiter, the NASA Mars Global Surveyor achieved Mars orbit in 1997. This mission was a complete success, having finished its primary mapping mission in early 2001. Contact was lost with the probe in November 2006 during its third extended program, spending exactly 10 operational years in space. The NASA Mars Pathfinder, carrying a robotic exploration vehicle Sojourner, landed in the Ares Vallis on Mars in the summer of 1997, returning many images.[28]

Map of Mars
Interactive image map of the global topography of Mars, overlaid with the position of Martian rovers and landers. Coloring of the base map indicates relative elevations of Martian surface.
Clickable image: Clicking on the labels will open a new article.
(   Active •   Inactive •   Planned)
Bradbury Landing
Deep Space 2
Mars Polar Lander
Perseverance
Schiaparelli EDM
Spirit
Viking 1
Mars landing sites (16 December 2020)

NASA's Mars Odyssey orbiter entered Mars orbit in 2001.[29] Odyssey's Gamma Ray Spectrometer detected significant amounts of hydrogen in the upper metre or so of regolith on Mars. This hydrogen is thought to be contained in large deposits of water ice.[30]

The Mars Express mission of the European Space Agency (ESA) reached Mars in 2003. It carried the Beagle 2 lander, which was not heard from after being released and was declared lost in February 2004. Beagle 2 was located in January 2015 by the HiRise camera on NASA's Mars Reconnaissance Orbiter (MRO) having landed safely but failed to fully deploy its solar panels and antenna.[31][32] In early 2004, the Mars Express Planetary Fourier Spectrometer team announced the orbiter had detected methane in the Martian atmosphere, a potential biosignature. ESA announced in June 2006 the discovery of aurorae on Mars by the Mars Express.[33]

Martian sunset, Spirit rover, 2005
North polar view, Phoenix lander, 2008

In January 2004, the NASA twin Mars Exploration Rovers named Spirit (MER-A) and Opportunity (MER-B) landed on the surface of Mars. Both have met and exceeded all their science objectives. Among the most significant scientific returns has been conclusive evidence that liquid water existed at some time in the past at both landing sites. Martian dust devils and windstorms have occasionally cleaned both rovers' solar panels, and thus increased their lifespan.[34] Spirit rover (MER-A) was active until 2010, when it stopped sending data because it got stuck in a sand dune and was unable to reorient itself to recharge its batteries.[8]

Rosetta came within 250 km of Mars during its 2007 flyby.[35] Dawn flew by Mars in February 2009 for a gravity assist on its way to investigate Vesta and Ceres.[36]

Phoenix landed on the north polar region of Mars on May 25, 2008.[37] Its robotic arm dug into the Martian soil and the presence of water ice was confirmed on June 20, 2008.[38][39] The mission concluded on November 10, 2008, after contact was lost.[40] In 2008, the price of transporting material from the surface of Earth to the surface of Mars was approximately US$309,000 per kilogram.[41]

The Indian Space Research Organisation (ISRO) launched their Mars Orbiter Mission (MOM) on November 5, 2013, and it was inserted into Mars orbit on September 24, 2014. India's ISRO is the fourth space agency to reach Mars, after the Soviet space program, NASA and ESA.[42] India successfully placed a spacecraft into Mars orbit, and became the first country to do so in its maiden attempt.[43]

Overview of missions

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The following entails a brief overview of previous missions to Mars, oriented towards orbiters and flybys; see also Mars landing and Mars rover.

Early Soviet missions

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Main articles: Mars 1M, Mars 1, and Mars program
1960s
[edit]
Mars 1M spacecraft

Between 1960 and 1969, the Soviet Union launched nine probes intended to reach Mars. They all failed: three at launch; three failed to reach near-Earth orbit; one during the burn to put the spacecraft into trans-Mars trajectory; and two during the interplanetary orbit.

The Mars 1M programs (sometimes dubbed Marsnik in Western media) was the first Soviet uncrewed spacecraft interplanetary exploration program, which consisted of two flyby probes launched towards Mars in October 1960, Mars 1960A and Mars 1960B (also known as Korabl 4 and Korabl 5 respectively). After launch, the third stage pumps on both launchers were unable to develop enough pressure to commence ignition, so Earth parking orbit was not achieved. The spacecraft reached an altitude of 120 km before reentry.

Mars 1962A was a Mars flyby mission, launched on October 24, 1962, and Mars 1962B an intended first Mars lander mission, launched in late December of the same year (1962). Both failed from either breaking up as they were going into Earth orbit or having the upper stage explode in orbit during the burn to put the spacecraft into trans-Mars trajectory.[8]

The first success
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Selected Soviet Mars probes
Spacecraft Orbiter or flyby outcome Lander outcome
Mars 1 Failure Failure
Mars 2 Success Failure
Mars 3 Partial success Partial success
Mars 4 Failure —
Mars 5 Partial success —
Mars 6 Success Failure
Mars 7 Success Failure
Phobos 1 Failure Not deployed
Phobos 2 Partial success Not deployed

Mars 1 (1962 Beta Nu 1), an automatic interplanetary spacecraft launched to Mars on November 1, 1962, was the first probe of the Soviet Mars probe program to achieve interplanetary orbit. Mars 1 was intended to fly by the planet at a distance of about 11,000 km and take images of the surface as well as send back data on cosmic radiation, micrometeoroid impacts and Mars' magnetic field, radiation environment, atmospheric structure, and possible organic compounds.[44][45] Sixty-one radio transmissions were held, initially at 2-day intervals and later at 5-day intervals, from which a large amount of interplanetary data was collected. On 21 March 1963, when the spacecraft was at a distance of 106,760,000 km from Earth, on its way to Mars, communications ceased due to failure of its antenna orientation system.[44][45]

In 1964, both Soviet probe launches, of Zond 1964A on June 4, and Zond 2 on November 30, (part of the Zond program), resulted in failures. Zond 1964A had a failure at launch, while communication was lost with Zond 2 en route to Mars after a mid-course maneuver, in early May 1965.[8]

In 1969, and as part of the Mars probe program, the Soviet Union prepared two identical 5-ton orbiters called M-69, dubbed by NASA as Mars 1969A and Mars 1969B. Both probes were lost in launch-related complications with the newly developed Proton rocket.[46]

1970s
[edit]

The USSR intended to have the first artificial satellite of Mars beating the planned American Mariner 8 and Mariner 9 Mars orbiters. In May 1971, one day after Mariner 8 malfunctioned at launch and failed to reach orbit, Cosmos 419 (Mars 1971C), a heavy probe of the Soviet Mars program M-71, also failed to launch. This spacecraft was designed as an orbiter only, while the next two probes of project M-71, Mars 2 and Mars 3, were multipurpose combinations of an orbiter and a lander with small skis-walking rovers, PrOP-M, that would be the first planet rovers outside the Moon. They were successfully launched in mid-May 1971 and reached Mars about seven months later. On November 27, 1971, the lander of Mars 2 crash-landed due to an on-board computer malfunction and became the first man-made object to reach the surface of Mars. On 2 December 1971, the Mars 3 lander became the first spacecraft to achieve a soft landing, but its transmission was interrupted after 14.5 seconds.[47]

The Mars 2 and 3 orbiters sent back a relatively large volume of data covering the period from December 1971 to March 1972, although transmissions continued through to August. By 22 August 1972, after sending back data and a total of 60 pictures, Mars 2 and 3 concluded their missions. The images and data enabled creation of surface relief maps, and gave information on the Martian gravity and magnetic fields.[48]

In 1973, the Soviet Union sent four more probes to Mars: the Mars 4 and Mars 5 orbiters and the Mars 6 and Mars 7 flyby/lander combinations. All missions except Mars 7 sent back data, with Mars 5 being most successful. Mars 5 transmitted just 60 images before a loss of pressurization in the transmitter housing ended the mission. Mars 6 lander transmitted data during descent, but failed upon impact. Mars 4 flew by the planet at a range of 2200 km returning one swath of pictures and radio occultation data, which constituted the first detection of the nightside ionosphere on Mars.[49] Mars 7 probe separated prematurely from the carrying vehicle due to a problem in the operation of one of the onboard systems (attitude control or retro-rockets) and missed the planet by 1,300 kilometres (8.7×10−6 au).[citation needed]

Mariner program

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Main articles: Mariner program, Mariner 4, Mariner 6 and 7, and Mariner 9
The first close-up images taken of Mars in 1965 from Mariner 4 show an area about 330 km across by 1200 km from limb to bottom of frame.

In 1964, NASA's Jet Propulsion Laboratory made two attempts at reaching Mars. Mariner 3 and Mariner 4 were identical spacecraft designed to carry out the first flybys of Mars. Mariner 3 was launched on November 5, 1964, but the shroud encasing the spacecraft atop its rocket failed to open properly, dooming the mission. Three weeks later, on November 28, 1964, Mariner 4 was launched successfully on a 71⁄2-month voyage to Mars.[citation needed]

Mariner 4 flew past Mars on July 14, 1965, providing the first close-up photographs of another planet. The pictures, gradually played back to Earth from a small tape recorder on the probe, showed impact craters. It provided radically more accurate data about the planet; a surface atmospheric pressure of about 1% of Earth's and daytime temperatures of −100 °C (−148 °F) were estimated. No magnetic field[50][51] or Martian radiation belts[52] were detected. The new data meant redesigns for then planned Martian landers, and showed life would have a more difficult time surviving there than previously anticipated.[53][54][55][56]

Mariner Crater, as seen by Mariner 4. The location is Phaethontis quadrangle.

NASA continued the Mariner program with another pair of Mars flyby probes, Mariner 6 and 7. They were sent at the next launch window, and reached the planet in 1969. During the following launch window the Mariner program again suffered the loss of one of a pair of probes. Mariner 9 successfully entered orbit about Mars, the first spacecraft ever to do so, after the launch time failure of its sister ship, Mariner 8. When Mariner 9 reached Mars in 1971, it and two Soviet orbiters (Mars 2 and Mars 3) found that a planet-wide dust storm was in progress. The mission controllers used the time spent waiting for the storm to clear to have the probe rendezvous with, and photograph, Phobos. When the storm cleared sufficiently for Mars' surface to be photographed by Mariner 9, the pictures returned represented a substantial advance over previous missions. These pictures were the first to offer more detailed evidence that liquid water might at one time have flowed on the planetary surface. They also finally discerned the true nature of many Martian albedo features. For example, Nix Olympica was one of only a few features that could be seen during the planetary duststorm, revealing it to be the highest mountain (volcano, to be exact) on any planet in the entire Solar System, and leading to its reclassification as Olympus Mons.[citation needed]

Viking program

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Main articles: Viking program, Viking 1, Viking 2, and Viking spacecraft biological experiments

The Viking program launched Viking 1 and Viking 2 spacecraft to Mars in 1975; The program consisted of two orbiters and two landers – these were the second and third spacecraft to successfully land on Mars. In 1976, Viking 1 and Viking 2 touched down on the Martian surface. These landers were significantly larger than the Soviet Mars 3 lander (Viking 1 was 3,527 kilograms compared to the 358 kg Mars 3 lander).[57] They were able to take the first photographs from the surface of Mars.[58][59]

Viking 1 operated on the surface of Mars for around six years (On Nov 11, 1982 the Lander stopped operating after getting a faulty command) and Viking 2 for over three years (mission ended in early 1980). Both landers were equipped with a robotic sampler arm which successfully scooped up soil samples and tested them with instruments such as a Gas chromatography–mass spectrometer. The landers measured temperatures ranging from negative 86 degrees Celsius before dawn to negative 33 degrees Celsius in the afternoon. Both landers had issues obtaining accurate results from their seismometers.[59][60][61][62]

Photographs from the landers and orbiters surpassed expectations in quality and quantity. The total exceeded 4,500 from the landers and 52,000 from the orbiters.

Surface of Mars taken by Viking 1, large rock to the right was nicknamed 'Big Joe' by NASA scientists[63][64]

The Viking landers recorded atmospheric pressures ranging from below 7 millibars (0.0068 bars) to over 10 millibars (0.0108 bars) over the Martian year, leading to the conclusion that atmospheric pressure varies by 30 percent during the Martian year because carbon dioxide condenses and sublimes at the polar caps. Martian winds generally blow more slowly than expected, scientists had expected them to reach speeds of several hundred miles an hour from observing global dust storms, but neither lander recorded gusts over 120 kilometers (74 miles) an hour, and average velocities were considerably lower. Nevertheless, the orbiters observed more than a dozen small dust storms. The Viking landers detected nitrogen in the atmosphere for the first time, and that it was a significant component of the Martian atmosphere. There was speculation from the atmospheric analysis that the atmosphere of Mars used to be much denser.[65][66]

Taken by the Viking 1 lander shortly after it touched down on Mars, this image is the first photograph ever taken from the surface of Mars. It was taken on July 20, 1976.[59]
Viking 1 lander site (1st color, July 21, 1976)
Viking 2 lander site (1st color, September 5, 1976)
Viking 2 lander site (September 25, 1977)
(False color image) Frost at Viking 2 site (May 18, 1979)
Martian sunset over Chryse Planitia at Viking 1 site (August 20, 1976)

The primary scientific objectives of the lander mission were to search for biosignatures and observe meteorologic, seismic and magnetic properties of Mars. The results of the biological experiments on board the Viking landers remain inconclusive, with a reanalysis of the Viking data published in 2012 suggesting signs of microbial life on Mars.[67][68]

Flood erosion at Dromore crater
Tear-drop shaped islands at Oxia Palus
Streamlined islands in Lunae Palus
Scour patterns located in Lunae Palus

The Viking orbiters revealed that large floods of water carved deep valleys, eroded grooves into bedrock, and traveled thousands of kilometers. Areas of branched streams, in the southern hemisphere, suggest that rain once fell.[69][70][71]

Mars Pathfinder, Sojourner rover

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Sojourner takes Alpha Proton X-ray Spectrometer measurements of the Yogi Rock.
Main articles: Mars Pathfinder, Sojourner (rover), and Mars landing

Mars Pathfinder was a U.S. spacecraft that landed a base station with a roving probe on Mars on July 4, 1997. It consisted of a lander and a small 10.6-kilogram (23 lb) wheeled robotic rover named Sojourner, which was the first rover to operate on the surface of Mars.[72][73] In addition to scientific objectives, the Mars Pathfinder mission was also a "proof-of-concept" for various technologies, such as an airbag landing system and automated obstacle avoidance, both later exploited by the Mars Exploration Rovers.[72]

Mars Global Surveyor

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Main article: Mars Global Surveyor
This image from Mars Global Surveyor spans a region about 1500 meters across. Gullies, similar to those formed on Earth, are visible from Newton Basin in Sirenum Terra.
Gullies, similar to those formed on Earth, are visible on this image from Mars Global Surveyor.

After the 1992 failure of NASA's Mars Observer orbiter, NASA retooled and launched Mars Global Surveyor (MGS). Mars Global Surveyor launched on November 7, 1996, and entered orbit on September 12, 1997. After a year and a half trimming its orbit from a looping ellipse to a circular track around the planet, the spacecraft began its primary mapping mission in March 1999. It observed the planet from a low-altitude, nearly polar orbit over the course of one complete Martian year, the equivalent of nearly two Earth years. Mars Global Surveyor completed its primary mission on January 31, 2001, and completed several extended mission phases until communication was lost in 2007.[74]

The mission studied the entire Martian surface, atmosphere, and interior, and returned more data about the red planet than all previous Mars missions combined. The data has been archived and remains available publicly.[75]

This color-coded elevation map was produced from data collected by Mars Global Surveyor. It shows an area around Northern Kasei Valles, showing relationships among Kasei Valles, Bahram Vallis, Vedra Vallis, Maumee Vallis, and Maja Valles. Map location is in Lunae Palus quadrangle and includes parts of Lunae Planum and Chryse Planitia.
A color-coded elevation map produced from data collected by Mars Global Surveyor indicating the result of floods on Mars

Among key scientific findings, Global Surveyor took pictures of gullies and debris flow features that suggest there may be current sources of liquid water, similar to an aquifer, at or near the surface of the planet. Similar channels on Earth are formed by flowing water, but on Mars the temperature is normally too cold and the atmosphere too thin to sustain liquid water. Nevertheless, many scientists hypothesize that liquid groundwater can sometimes surface on Mars, erode gullies and channels, and pool at the bottom before freezing and evaporating.[76]

Magnetometer readings showed that the planet's magnetic field is not globally generated in the planet's core, but is localized in particular areas of the crust. New temperature data and closeup images of the Martian moon Phobos showed that its surface is composed of powdery material at least 1 metre (3 feet) thick, caused by millions of years of meteoroid impacts. Data from the spacecraft's laser altimeter gave scientists their first 3-D views of Mars' north polar ice cap in January 1999.[77]

Faulty software uploaded to the vehicle in June 2006 caused the spacecraft to orient its solar panels incorrectly several months later, resulting in battery overheating and subsequent failure.[78] On November 5, 2006, MGS lost contact with Earth.[79] NASA ended efforts to restore communication on January 28, 2007.[80]

Mars Odyssey and Mars Express

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Main articles: 2001 Mars Odyssey and Mars Express
Animation of 2001 Mars Odyssey's trajectory around Mars from 24 October 2001 to 24 October 2002
   2001 Mars Odyssey ·   Mars
Animation of Mars Express's trajectory around Mars from 25 December 2003 to 1 January 2010
   Mars Express ·   Mars

In 2001, NASA's Mars Odyssey orbiter arrived at Mars. Its mission is to use spectrometers and imagers to hunt for evidence of past or present water and volcanic activity on Mars. In 2002, it was announced that the probe's gamma-ray spectrometer and neutron spectrometer had detected large amounts of hydrogen, indicating that there are vast deposits of water ice in the upper three meters of Mars' soil within 60° latitude of the south pole.[citation needed]

On June 2, 2003, the European Space Agency's Mars Express set off from Baikonur Cosmodrome to Mars. The Mars Express craft consists of the Mars Express Orbiter and the stationary lander Beagle 2. The lander carried a digging device and the smallest mass spectrometer created to date, as well as a range of other devices, on a robotic arm in order to accurately analyze soil beneath the dusty surface to look for biosignatures and biomolecules.[citation needed]

The orbiter entered Mars orbit on December 25, 2003, and Beagle 2 entered Mars' atmosphere the same day. However, attempts to contact the lander failed. Communications attempts continued throughout January, but Beagle 2 was declared lost in mid-February, and a joint inquiry was launched by the UK and ESA. The Mars Express Orbiter confirmed the presence of water ice and carbon dioxide ice at the planet's south pole, while NASA had previously confirmed their presence at the north pole of Mars.[citation needed]

The lander's fate remained a mystery until it was located intact on the surface of Mars in a series of images from the Mars Reconnaissance Orbiter.[81][82] The images suggest that two of the spacecraft's four solar panels failed to deploy, blocking the spacecraft's communications antenna. Beagle 2 is the first British and first European probe to achieve a soft landing on Mars.[citation needed]

MER, Opportunity rover, Spirit rover, Phoenix lander

[edit]
Main articles: Mars Exploration Rover, Opportunity rover, Spirit rover, and Phoenix lander
See also: Mars landing
Polar surface as seen by the Phoenix lander

NASA's Mars Exploration Rover Mission (MER), started in 2003, was a robotic space mission involving two rovers, Spirit (MER-A) and Opportunity, (MER-B) that explored the Martian surface geology. The mission's scientific objective was to search for and characterize a wide range of rocks and soils that hold clues to past water activity on Mars. The mission was part of NASA's Mars Exploration Program, which includes three previous successful landers: the two Viking program landers in 1976; and Mars Pathfinder probe in 1997.[citation needed]

Rosetta and Dawn swingbys

[edit]
Main articles: Rosetta (spacecraft) and Dawn Mission

The ESA Rosetta space probe mission to the comet 67P/Churyumov-Gerasimenko flew within 250 km of Mars on February 25, 2007, in a gravitational slingshot designed to slow and redirect the spacecraft.[83]

The NASA Dawn spacecraft used the gravity of Mars in 2009 to change direction and velocity on its way to Vesta, and tested out Dawn's cameras and other instruments on Mars.[84]

Fobos-Grunt

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Main article: Fobos-Grunt

On November 8, 2011, Russia's Roscosmos launched an ambitious mission called Fobos-Grunt. It consisted of a lander aimed to retrieve a sample back to Earth from Mars' moon Phobos, and place the Chinese Yinghuo-1 probe in Mars' orbit. The Fobos-Grunt mission suffered a complete control and communications failure shortly after launch and was left stranded in low Earth orbit, later falling back to Earth.[85] The Yinghuo-1 satellite and Fobos-Grunt underwent destructive re-entry on January 15, 2012, finally disintegrating over the Pacific Ocean.[86][87][88]

Mars Orbiter Mission

[edit]

The Mars Orbiter Mission, also called Mangalyaan, was launched on 5 November 2013 by the Indian Space Research Organisation (ISRO).[89] It was successfully inserted into Martian orbit on 24 September 2014. The mission is a technology demonstrator, and as secondary objective, it will also study the Martian atmosphere. This is India's first mission to Mars, and with it, ISRO became the fourth space agency to successfully reach Mars after the Soviet Union, NASA (USA) and ESA (Europe). It was completed in a record low budget of $71 million,[90][91] making it the least-expensive Mars mission to date.[92] The mission concluded on September 27, 2022, after contact was lost.

InSight and MarCO

[edit]
Main article: InSight

In August 2012, NASA selected InSight, a $425 million lander mission with a heat flow probe and seismometer, to determine the deep interior structure of Mars.[93][94][95] InSight landed successfully on Mars on 26 November 2018.[96] Valuable data on the atmosphere,[97] surface[98] and the planet's interior[99] were gathered by Insight. Insight's mission was declared as ended on 21 December 2022.

Two flyby CubeSats called MarCO were launched with InSight on 5 May 2018[100] to provide real-time telemetry during the entry and landing of InSight. The CubeSats separated from the Atlas V booster 1.5 hours after launch and traveled their own trajectories to Mars.[101][102][103]

Current missions

[edit]
NASA missions to Mars (28 September 2021)(Perseverance rover; Ingenuity Mars helicopter; InSight lander; Odyssey orbiter; MAVEN orbiter; Curiosity rover; Mars Reconnaissance Orbiter)

On 10 March 2006, NASA's Mars Reconnaissance Orbiter (MRO) probe arrived in orbit to conduct a two-year science survey. The orbiter began mapping the Martian terrain and weather to find suitable landing sites for upcoming lander missions. The MRO captured the first image of a series of active avalanches near the planet's north pole in 2008.[104]

The Mars Science Laboratory mission was launched on November 26, 2011, and delivered the Curiosity rover on the surface of Mars on August 6, 2012 UTC. It is larger and more advanced than the Mars Exploration Rovers, with a velocity of up to 90 meters per hour (295 feet per hour).[105] Experiments include a laser chemical sampler that can deduce the composition of rocks at a distance of 7 meters.[106]

MAVEN orbiter was launched on 18 November 2013, and on 22 September 2014, it was injected into an areocentric elliptic orbit 6,200 km (3,900 mi) by 150 km (93 mi) above the planet's surface to study its atmosphere. Mission goals include determining how the planet's atmosphere and water, presumed to have once been substantial, were lost over time.[107]

The ExoMars Trace Gas Orbiter arrived at Mars in 2016 and deployed the Schiaparelli EDM lander, a test lander. Schiaparelli crashed on surface, but it transmitted key data during its parachute descent, so the test was declared a partial success.[108]

Overview of missions

[edit]

Mars Reconnaissance Orbiter

[edit]
Main article: Mars Reconnaissance Orbiter
Slope streaks as seen by HiRISE[109]

The Mars Reconnaissance Orbiter (MRO) is a multipurpose spacecraft designed to conduct reconnaissance and exploration of Mars from orbit. The US$720 million spacecraft was built by Lockheed Martin under the supervision of the Jet Propulsion Laboratory, launched August 12, 2005, and entered Mars orbit on March 10, 2006.[110]

The MRO contains a host of scientific instruments such as the HiRISE camera, CTX camera, CRISM, and SHARAD. The HiRISE camera is used to analyze Martian landforms, whereas CRISM and SHARAD can detect water, ice, and minerals on and below the surface. Additionally, MRO is paving the way for upcoming generations of spacecraft through daily monitoring of Martian weather and surface conditions, searching for future landing sites, and testing a new telecommunications system that enable it to send and receive information at an unprecedented bitrate, compared to previous Mars spacecraft. Data transfer to and from the spacecraft occurs faster than all previous interplanetary missions combined and allows it to serve as an important relay satellite for other missions.[citation needed]

Curiosity rover

[edit]
Main articles: Mars Science Laboratory, Curiosity rover, and Timeline of Mars Science Laboratory
A self-portrait of the Curiosity rover, which landed on Mars in 2012

The NASA Mars Science Laboratory mission with its rover named Curiosity, was launched on November 26, 2011,[111][112] and landed on Mars on August 6, 2012, on Aeolis Palus in Gale Crater. The rover carries instruments designed to look for past or present conditions relevant to the past or present habitability of Mars.[113][114][115][116]

MAVEN

[edit]

NASA's MAVEN is an orbiter mission to study the upper atmosphere of Mars.[117] It also serves as a communications relay satellite for robotic landers and rovers on the surface of Mars. MAVEN was launched 18 November 2013 and reached Mars on 22 September 2014.[citation needed]

Trace Gas Orbiter and EDM

[edit]
Main articles: Trace Gas Orbiter and Schiaparelli EDM lander

The ExoMars Trace Gas Orbiter is an atmospheric research orbiter built in collaboration between ESA and Roscosmos. It was injected into Mars orbit on 19 October 2016 to gain a better understanding of methane (CH
4) and other trace gases present in the Martian atmosphere that could be evidence for possible biological or geological activity. The Schiaparelli EDM lander was destroyed when trying to land on the surface of Mars.[118]

Hope

[edit]

The United Arab Emirates launched the Hope Mars Mission, in July 2020 on the Japanese H-IIA booster.[119] It was successfully placed into orbit on 9 February 2021. It is studying the Martian atmosphere and weather.

Tianwen-1 and Zhurong rover

[edit]
Martian surface captured by Zhurong rover

Tianwen-1 was a Chinese mission launched on 23 July 2020 which included an orbiter, a lander, and a 240-kilogram (530 lb) rover along with a package of deployable and remote cameras.[120] Tianwen-1 entered orbit on 10 February 2021 and the Zhurong rover successfully landed on 14 May 2021 and deployed on 22 May 2021.[6] Zhurong had been in operation for 347 Martian days and traveled 1,921 meters across Mars before entering hibernation state in May 22.[121] The rover has never been awaken since then, but the orbiter continued to work.[122]

Mars 2020, Perseverance rover, Ingenuity helicopter

[edit]
Mapping Perseverance's samples collected to date

The Mars 2020 mission by NASA was launched on 30 July 2020 on a United Launch Alliance Atlas V rocket from Cape Canaveral. It is based on the Mars Science Laboratory design. The scientific payload is focused on astrobiology.[123] It includes the Perseverance rover and the retired Ingenuity helicopter. Unlike older rovers that relied on solar power, Perseverance is nuclear powered, to survive longer than its predecessors in this harsh, dusty environment. The car-size rover weighs about 1 ton, with a robotic arm that reaches about 7 feet (2.1 m), zoom cameras, a chemical analyzer and a rock drill.[124][125]

After traveling 293 million miles (471 million km) to reach Mars over the course of more than six months, Perseverance successfully landed on February 18, 2021. Its initial mission is set for at least one Martian year, or 687 Earth days. It will search for signs of ancient life and explore the red planet's surface.[126][127]

As of October 19, 2021, Perseverance had captured the first sounds from Mars. Recordings consisted of five hours of Martian wind gusts, rover wheels crunching over gravel, and motors whirring as the spacecraft moves its arm. The sounds give researchers clues about the atmosphere, such as how far sound travels on the planet.[citation needed]

Europa Clipper, Hera and Psyche

[edit]

The NASA Europa Clipper to Jupiter and Europa, NASA Psyche space probe mission to the metal-rich asteroid 16 Psyche and ESA Hera to Didymos will undertake flybys of Mars on March 1, 2025,[128] March 2025, and May 2026 respectively, in a gravitational slingshot designed to slow and redirect the spacecraft.[129]

Future missions

[edit]
See also: Mars sample return mission

Proposals

[edit]

Other future mission concepts include polar probes, Martian aircraft and a network of small meteorological stations.[138] Longterm areas of study may include Martian lava tubes, resource utilization, and electronic charge carriers in rocks.[142][143]

Human mission proposals

[edit]
Concept for NASA Design Reference Mission Architecture 5.0 (2009)
Main article: Human mission to Mars

The human exploration of Mars has been an aspiration since the earliest days of modern rocketry; Robert H. Goddard credits the idea of reaching Mars as his own inspiration to study the physics and engineering of space flight.[144] Proposals for human exploration of Mars have been made throughout the history of space exploration. Currently there are multiple active plans and programs to put humans on Mars within the next ten to thirty years, both governmental and private, some of which are listed below.

NASA

[edit]

Human exploration by the United States was identified as a long-term goal in the Vision for Space Exploration announced in 2004 by then US President George W. Bush.[145] The planned Orion spacecraft would be used to send a human expedition to Earth's moon by 2020 as a stepping stone to a Mars expedition. On September 28, 2007, NASA administrator Michael D. Griffin stated that NASA aims to put a person on Mars by 2037.[146]

On December 2, 2014, NASA's Advanced Human Exploration Systems and Operations Mission Director Jason Crusan and Deputy Associate Administrator for Programs James Reuthner announced tentative support for the Boeing "Affordable Mars Mission Design" including radiation shielding, centrifugal artificial gravity, in-transit consumable resupply, and a lander which can return.[147][148] Reuthner suggested that if adequate funding was forthcoming, the proposed mission would be expected in the early 2030s.[149]

Journey to Mars – Science, Exploration, Technology

On October 8, 2015, NASA published its official plan for human exploration and colonization of Mars. They called it "Journey to Mars". The plan operates through three distinct phases leading to fully sustained colonization.[150]

  • The first stage, already underway, is the "Earth Reliant" phase. This phase continues using the International Space Station until 2024; validating deep space technologies and studying the effects of long-duration space missions on the human body.
  • The second stage, "Proving Ground," moves away from Earth reliance and ventures into cislunar space for most of its tasks. This is when NASA plans to capture an asteroid, test deep space habitation facilities, and validate the capabilities required for human exploration of Mars.
  • The last stage, the "Earth Independent" phase, includes long-term missions on the lunar surface which leverage surface habitats that only require routine maintenance, and the harvesting of Martian resources for fuel, water, and building materials. NASA is still aiming for human missions to Mars in the 2030s, though Earth independence could take decades longer.[151]

On August 28, 2015, NASA funded a year-long simulation to study the effects of a year-long Mars mission on six scientists. The scientists lived in a biodome on a Mauna Loa mountain in Hawaii with limited connection to the outside world and were only allowed outside if they were wearing spacesuits.[152][153]

NASA's human Mars exploration plans have evolved through the NASA Mars Design Reference Missions, a series of design studies for human exploration of Mars.

In 2017, the focus of NASA shifted to a return to the Moon by 2024 with the Artemis program, a flight to Mars could follow after this project.

SpaceX

[edit]

The long-term goal of the private corporation SpaceX is the establishment of routine flights to Mars to enable colonization.[154][155][156] To this end, the company is developing Starship, a spacecraft capable of crew transportation to Mars and other celestial bodies, along with its booster Super Heavy. In 2016 SpaceX announced plans to send two uncrewed Starships to Mars by 2022, followed by two more uncrewed flights and two crewed flights in 2024.[155] SpaceX is currently targeting the first uncrewed launches NET 2026, with the first crewed flights happening NET 2028.[157]

Starship is planned to have a payload of at least 100 tonnes[158] and is designed to use a combination of aerobraking and propulsive descent, using fuel produced from a Mars (in situ resource utilization) facility.[155] As of 2024, the Starship development program has seen multiple integrated test flights and is progressing towards full reusability. SpaceX’s plans involve the mass manufacturing of Starship and initially sustained by resupply from Earth, and in situ resource utilization on Mars, until the Mars colony reaches full self sustainability. Any future human mission to Mars will likely take place within the optimal Mars launch window, which occurs every 26 months.[159][160]

Zubrin

[edit]

Mars Direct, a low-cost human mission proposed by Robert Zubrin, founder of the Mars Society, would use heavy-lift Saturn V class rockets, such as the Ares V, to skip orbital construction, LEO rendezvous, and lunar fuel depots. A modified proposal, called "Mars to Stay", involves not returning the first immigrant explorers immediately, if ever (see Colonization of Mars).[145][146][161][162]

Probe difficulties

[edit]
Deep Space 2 technology
Mars Spacecraft 1988–1999
Spacecraft Outcome
Phobos 1 Failure
Phobos 2 Partial success
Mars Observer Failure
Mars 96 Failure
Mars Pathfinder Success
Mars Global Surveyor Success
Mars Climate Orbiter Failure
Mars Polar Lander Failure
Deep Space 2 Failure
Nozomi Failure

The challenge, complexity and length of Mars missions have led to many mission failures.[163] The high failure rate of missions attempting to explore Mars is informally called the "Mars Curse" or "Martian Curse".[164] The phrase "Galactic Ghoul"[165] or "Great Galactic Ghoul" refers to a fictitious space monster that subsists on a diet of Mars probes, and is sometimes facetiously used to "explain" the recurring difficulties.[166][167][168][169]

Two Soviet probes were sent to Mars in 1988 as part of the Phobos program. Phobos 1 operated normally until an expected communications session on 2 September 1988 failed to occur. The problem was traced to a software error, which deactivated Phobos 1's attitude thrusters, causing the spacecraft's solar arrays to no longer point at the Sun, depleting Phobos 1's batteries. Phobos 2 operated normally throughout its cruise and Mars orbital insertion phases on January 29, 1989, gathering data on the Sun, interplanetary medium, Mars, and Phobos. Shortly before the final phase of the mission – during which the spacecraft was to approach within 50 m of Phobos' surface and release two landers, one a mobile 'hopper', the other a stationary platform – contact with Phobos 2 was lost. The mission ended when the spacecraft signal failed to be successfully reacquired on March 27, 1989. The cause of the failure was determined to be a malfunction of the on-board computer.[citation needed]

Just a few years later in 1992, Mars Observer, launched by NASA, failed as it approached Mars. Mars 96, an orbiter launched on November 16, 1996, by Russia failed, when the planned second burn of the Block D-2 fourth stage did not occur.[170]

Following the success of Global Surveyor and Pathfinder, another spate of failures occurred in 1998 and 1999, with the Japanese Nozomi orbiter and NASA's Mars Climate Orbiter, Mars Polar Lander, and Deep Space 2 penetrators all suffering various fatal errors. The Mars Climate Orbiter was noted for mixing up U.S. customary units with metric units, causing the orbiter to burn up while entering Mars' atmosphere.[171]

The European Space Agency has also attempted to land two probes on the Martian surface; Beagle 2, a British-built lander that failed to deploy its solar arrays properly after touchdown in December 2003, and Schiaparelli, which was flown along the ExoMars Trace Gas Orbiter. Contact with the Schiaparelli EDM lander was lost 50 seconds before touchdown.[172] It was later confirmed that the lander struck the surface at a high velocity, possibly exploding.[173]

See also

[edit]
Mars
General

Notes

[edit]
^α The diagram includes missions that are active on the surface, such as operational rovers and landers, as well as probes in Mars orbit. The diagram does not include missions that are en route to Mars, or probes that performed a fly-by of Mars and moved on.

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Bibliography

[edit]
  • Mars – A Warmer, Wetter Planet by Jeffrey S. Kargel (published July 2004; ISBN 978-1-85233-568-7)
  • The Compact NASA Atlas of the Solar System by Ronald Greeley and Raymond Batson (published January 2002; ISBN 0-521-80633-X)
  • Mars: The NASA Mission Reports / edited by Robert Godwin (2000) ISBN 1-896522-62-9
[edit]
Wikimedia Commons has media related to Mars exploration.
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