The exploration of Mars has been an important part of the space exploration programs of the Soviet Union, the United States, Europe, and Japan. Dozens of robotic spacecraft, including orbiters, landers, and rovers, have been launched toward Mars since the 1960s. These missions were aimed at gathering data about current conditions and answering questions about the history of Mars as well as a preparation for a possible human mission to Mars. The questions raised by the scientific community are expected to not only give a better appreciation of the red planet but also yield further insight into the past, and possible future, of Earth.
The exploration of Mars has come at a considerable financial cost with roughly two-thirds of all spacecraft destined for Mars failing before completing their missions, with some failing before they even begin. Such a high failure rate can be attributed to the complexity and large number of variables involved in an interplanetary journey, and has led researchers to jokingly speak of The Great Galactic Ghoul [1] which subsists on a diet of Mars probes. This phenomenon is also informally known as the Mars Curse.[2] As of January 2010, there are two functioning pieces of equipment on the surface of Mars beaming signals back to Earth: the Spirit rover and the Opportunity rover.
In October 2009, an agreement was signed between United states' space agency, NASA, and Europe's space agency, ESA in order to increase cooperation and expand collective capabilities, resources and expertise to continue the exploration of Mars; this agreement is named the Mars Joint Exploration Initiative (MEJI).[3][4]
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Mars has long been the subject of human fascination. Early telescopic observations revealed color changes on the surface which were originally attributed to seasonal vegetation as well as apparent linear features which were ascribed to intelligent design. These early and erroneous interpretations led to widespread public interest in Mars. Further telescopic observations found Mars' two moons - Phobos and Deimos, the polar ice caps and the feature now known as Olympus Mons, the solar system's tallest mountain.[5] These 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 far thinner atmosphere, it has a cold and desert-like surface. It is notable, however, that although the planet has only one quarter of the surface area of the Earth, it has about the same land area, since only one quarter of the surface area of the Earth is land.
In order to understand the history of the robotic exploration of Mars it is important to note that minimum-energy launch windows occur at intervals of approximately 2.135 years, i.e. 780 days (the planet's synodic period with respect to Earth). This is a consequence of the Hohmann transfer orbit for minimum-energy interplanetary transfer. The slight inclination and eccentricity of Mars' orbit relative to Earth's orbit means that the minimum energy launch date differs from that implied by the synodic period slightly. Launch window width is subject to vehicle constraints but are typically on the order of one month wide. The windows for recent/future years were/will be centred on the following dates:
Minimum energy inbound (Mars to Earth) launch windows also occur at similar intervals.
In addition to these minimum-energy trajectories, which occur when the planets are aligned so that the Earth to Mars transfer trajectory goes halfway around the Sun, an alternate trajectory which has been proposed goes first inward toward Venus orbit, and then outward, resulting in a longer trajectory which goes about 360 degrees around the Sun ("opposition-class trajectory").
The Marsnik program was the first Soviet unmanned spacecraft interplanetary exploration program, which consisted of two flyby probes launched towards Mars in October 1960, Marsnik 1 and 2 dubbed Mars 1960A and Mars 1960B (also known as Korabl 4 and Korabl 5 respectively). After launch, the third stage pumps on both Marsnik launchers were unable to develop enough thrust 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 fly-by mission, launched on October 24, 1962 and Mars 1962B a lander mission, launched in late December of the same year 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 the Mars trajectory.
Mars 1 (1962 Beta Nu 1) an automatic interplanetary station launched to Mars on November 1, 1962 was the first probe of the Soviet Mars probe program. 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. Sixty-one radio transmissions were held, initially at two day intervals and later at 5 days in 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 the spacecraft's antenna orientation system.
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.
The USSR intended to have the first artificial satellite of Mars beating the planned American Mariner 8 and Mariner 9 martian orbiters. But on May 5, 1971 Cosmos 419 (Mars 1971C), a heavy probe of the Soviet Mars program M-71, failed on launch. This spacecraft was designed as an orbiter only, while the second and third probes of project M-71, Mars 2 and Mars 3, were multi-aimed combinations of orbiter and lander.
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, and it failed to reach Mars. Three weeks later, on November 28, 1964, Mariner 4 was launched successfully on a 7½-month voyage to the red planet.
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 lunar-type impact craters.
NASA continued the Mariner program with another pair of Mars flyby probes, Mariner 6 and 7, at the next launch window. These probes 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, it and two Soviet orbiters (Mars 2 and Mars 3, see Mars probe program below) 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 evidence that liquid water might at one time have flowed on the planetary surface.
The Viking Orbiters caused a revolution in our ideas about water on Mars. Huge river valleys were found in many areas. They showed that floods of water broke through dams, carved deep valleys, eroded grooves into bedrock, and traveled thousands of kilometers. Areas of branched streams, in the southern hemisphere, suggested that rain once fell.[6][7][8]
The images below, some of the best from the Viking Orbiters, are mosaics of many small, high resolution images. Click on the images for more detail. Some of the pictures are labeled with place names.
Streamlined Islands seen by Viking showed that large floods occurred on Mars. Image is located in Lunae Palus quadrangle. |
Tear-drop shaped islands caused by flood waters from Maja Valles, as seen by Viking Orbiter. Image is located in Oxia Palus quadrangle. The islands are formed in the ejecta of Lod Crater, Bok Crater, and Gold Crater. |
Scour Patterns, located in Lunae Palus quadrangle, were produced by flowing water from Maja Vallis, which lies just to the left of this mosaic. Detail of flow around Dromore Crater is shown on the next image. |
Great amounts of water were required to carry out the erosion shown in this Viking image. Image is located in Lunae Palus quadrangle. The erosion shaped the ejecta around Dromore Crater. |
Waters from Vedra Vallis, Maumee Vallis, and Maja Vallis went from Lunae Planum on the left, to Chryse Planitia on the right. Image is located in Lunae Palus quadrangle and was taken by Viking Orbiter. |
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. |
The ejecta from Arandas Crater acts like mud. It moves around small craters (indicated by arrows), instead of just falling down on them. Craters like this suggest that large amounts of frozen water were melted when the impact crater was produced. Image is located in Mare Acidalium quadrangle and was taken by Viking Orbiter. |
This view of the flank of Alba Patera shows several chnnels/troughs. Some channels are associated with lava flows; others are probably caused by running water. A large trough or graben turns into a line of collapse pits. Image is located in Arcadia quadrangle and was taken by Viking Orbiter. |
Branched channels in Thaumasia quadrangle, as seen by Viking Orbiter. Networks of channels like this are strong evidence for rain on Mars in the past. |
The branched channels seen by Viking from orbit strongly suggested that it rained on Mars in the past. Image is located in Margaritifer Sinus quadrangle. |
Ravi Vallis, as seen by Viking Orbiter. Ravi Vallis was probably formed when catastrophic floods came out of the ground to the right (chaotic terrain). Image located in Margaritifer Sinus quadrangle. |
The following is a map of landings on Mars.
The Soviet Union intended to beat the USA by sending landers first in the Mars probe program M-69 in 1969, but both probes of the new heavy 5-ton design, Mars 1969A and Mars 1969B, failed at launch.
The first probes to impact and land on Mars were the Soviet Union's Mars 2 and Mars 3, as part of the Mars probe program M-71 in 1971. Each carried a lander. The Mars 2 lander crashed; Mars 3 was the first successful lander but stopped transmitting data and images from the surface after 22 seconds of operation.
Mars 6 and Mars 7 landers on the next Soviet Mars probe program M-73 failed their missions; the first impacted on the surface while the second missed the planet.
The first landers to successfully accomplish their missions were the American Viking 1 and Viking 2.
The high failure rate of missions launched from Earth attempting to explore Mars has become informally known as the "Mars Curse". The "Galactic Ghoul" is a fictional space monster that consumes Mars probes, a term coined in 1997 by Time Magazine journalist Donald Neff.[9][10][11]
Of 38 launches from Earth in an attempt to reach the planet, only 19 succeeded, a success rate of 50%. Twelve of the missions included attempts to land on the surface, but only seven transmitted data after landing.
The majority of the failed missions occurred in the early years of space exploration and were part of the Soviet and later Russian Mars probe program that suffered several technical difficulties, other than the largely successful Venera program for the exploration of Venus.
Modern missions have an improved success rate; however, the challenge, complexity and length of the missions make it inevitable that failures will occur.[12]
The U.S. NASA Mars exploration program has had a somewhat better record of success in Mars exploration, achieving success in 13 out of 20 missions launched (a 65% success rate), and succeeding in six out of seven (an 86% success rate) of the launches of Mars landers.
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Many people have long advocated a manned mission to Mars as the next logical step for a manned space program after lunar exploration. Aside from the prestige such a mission would bring, advocates argue that humans would easily be able to outperform robotic explorers, justifying the expenses. Critics contend, however, that robots can perform better than humans at a fraction of the expense. A list of hypothetical or proposed manned Mars missions proposals is located at manned mission to Mars.
Mission (1960–1969) | Launch | Arrival at Mars | Termination | Objective | Result |
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Marsnik 1 (Mars 1960A) | 10 October 1960 | 10 October 1960 | Flyby | Launch failure | |
Marsnik 2 (Mars 1960B) | 14 October 1960 | 14 October 1960 | Flyby | Launch failure | |
Sputnik 22 (Mars 1962A) | 24 October 1962 | 24 October 1962 | Flyby | Broke up shortly after launch | |
Mars 1 | 1 November 1962 | 21 March 1963 | Flyby | Some data collected, but lost contact before reaching Mars | |
Sputnik 24 (Mars 1962B) | 4 November 1962 | 19 January 1963 | Lander | Failed to leave Earth's orbit | |
Mariner 3 | 5 November 1964 | 5 November 1964 | Flyby | Failure during launch ruined trajectory. | |
Mariner 4 | 28 November 1964 | 14 July 1965 | 21 December 1967 | Flyby | Success (first successful flyby) |
Zond 2 | 30 November 1964 | May 1965 | Flyby | Lost contact | |
Mariner 6 | 25 February 1969 | 31 July 1969 | August 1969 | Flyby | Success |
Mariner 7 | 27 March 1969 | 5 August 1969 | August 1969 | Flyby | Success |
Mars 1969A | 27 March 1969 | 27 March 1969 | Orbiter | Launch failure | |
Mars 1969B | 2 April 1969 | 2 April 1969 | Orbiter | Launch failure | |
Mission (1970–1989) | Launch | Arrival at Mars | Termination | Objective | Result |
Mariner 8 | 8 May 1971 | 8 May 1971 | Orbiter | Launch failure | |
Cosmos 419 (Mars 1971C) | 10 May 1971 | 12 May 1971 | Orbiter | Launch failure | |
Mariner 9 | 30 May 1971 | 13 November 1971 | 27 October 1972 | Orbiter | Success (first successful orbit) |
Mars 2 | 19 May 1971 | 27 November 1971 | 22 August 1972 | Orbiter | Success |
27 November 1971 | Lander / rover[13] | Crashed on surface of Mars | |||
Mars 3 | 28 May 1971 | 2 December 1971 | 22 August 1972 | Orbiter | Success |
2 December 1971 | Lander / rover[13] | Partial Success. First successful landing; landed softly, but ceased transmission within 15 seconds. | |||
Mars 4 | 21 July 1973 | 10 February 1974 | 10 February 1974 | Orbiter | Did not enter orbit, but made a close flyby |
Mars 5 | 25 July 1973 | 2 February 1974 | 21 February 1974 | Orbiter | Partial success. Entered orbit, and returned data, but failed within 9 days |
Mars 6 | 5 August 1973 | 12 March 1974 | 12 March 1974 | Lander | Partial success. Data returned during descent, but not after landing on Mars |
Mars 7 | 9 August 1973 | 9 March 1974 | 9 March 1974 | Lander | Landing probe separated prematurely; entered heliocentric orbit. |
Viking 1 | 20 August 1975 | 20 July 1976 | 17 August 1980 | Orbiter | Success |
13 November 1982 | Lander | Success | |||
Viking 2 | 9 September 1975 | 3 September 1976 | 25 July 1978 | Orbiter | Success |
11 April 1980 | Lander | Success | |||
Phobos 1 | 7 July 1988 | 2 September 1988 | Orbiter | Contact lost while on route to Mars | |
lander | Not deployed | ||||
Phobos 2 | 12 July 1988 | 29 January 1989 | 27 March 1989 | Orbiter | Partial success: entered orbit and returned some data. Contact lost just before deployment of landers |
Landers | Not deployed | ||||
Mission (1990–1999) | Launch | Arrival at Mars | Termination | Objective | Result |
Mars Observer | 25 September 1992 | 24 August 1993 | 21 August 1993 | Orbiter | Lost contact just before arrival |
Mars Global Surveyor | 7 November 1996 | 11 September 1997 | 5 November 2006 | Orbiter | Success |
Mars 96 | 16 November 1996 | 17 November 1996 | Orbiter / landers | Launch failure | |
Mars Pathfinder | 4 December 1996 | 4 July 1997 | 27 September 1997 | Lander / rover | Success |
Nozomi (Planet-B) | 3 July 1998 | 9 December 2003 | Orbiter | Complications while on route; Never entered orbit | |
Mars Climate Orbiter | 11 December 1998 | 23 September 1999 | 23 September 1999 | Orbiter | Crashed on surface due to metric-imperial mix-up |
Mars Polar Lander | 3 January 1999 | 3 December 1999 | 3 December 1999 | Lander | Crash landed on surface due to improper hardware testing |
Deep Space 2 (DS2) | Hard landers | ||||
Mission (2000–present) | Launch | Arrival at Mars | Termination | Objective | Result |
2001 Mars Odyssey | 7 April 2001 | 24 October 2001 | Currently operational | Orbiter | Success |
Mars Express | 2 June 2003 | 25 December 2003 | Currently operational | Orbiter | Success |
Beagle 2 | 6 February 2004 | Lander | Lost contact in December 2003 after separation from Mars Express. Fate unknown. | ||
MER-A Spirit | 10 June 2003 | 4 January 2004 | Currently operational, stuck | Rover | Success |
MER-B Opportunity | 7 July 2003 | 25 January 2004 | Currently operational | Rover | Success |
Rosetta | 2 March 2004 | February 25, 2007 | Currently operational | Gravity assist enroute to comet 67P/Churyumov-Gerasimenko | Success |
Mars Reconnaissance Orbiter | 12 August 2005 | 10 March 2006 | Currently operational | Orbiter | Success |
Phoenix | 4 August 2007 | 25 May 2008 | 10 November 2008 | Lander | Success |
Dawn | 27 September 2007 | Feb. 17, 2009 | Currently operational | Gravity assist to Vesta | (Successful launch; successful to date) |
Future missions | Launch schedule | Estimated arrival at Mars | — | Objective | Notes |
Phobos-Grunt | 2012[14] | Orbiter, lander, sample return | Will attempt to bring samples of Phobos’ soil back to Earth in 2014 (or 2012).[15][16] | ||
Yinghuo-1 | Orbiter | Will travel with the Russian Phobos-Grunt mission | |||
MSL Curiosity | 15 September 2011 | 2012 | Rover | Powered by radioisotopes, it will perform chemical and physical analysis on martian soil and atmosphere. | |
MetNet | 2011–2019 | Multi-lander network | Simultaneous meteorological measurements at multiple locations.[17] | ||
Northern Light | 2012 | Lander / rover | Solar powered, it will perform chemical and physical analysis on Martian soil and atmosphere.[18] | ||
MAVEN | 2013 | Orbiter | Part of the Mars Scout Program | ||
Mars mission | Between 2013-2015[19] | Orbiter | The ISRO has begun the conceptual phase for an orbiter mission to Mars.[20][21] | ||
ARES (martian rocketplane) | Possibly by 2016 | aircraft | Search for life on Mars, water, atmospherics, magnetics | ||
and ExoMars | 2016 | Orbiter, static lander | TGM orbiter will deliver the ExoMars static lander. | ||
2018 | Two rovers | ExoMars rover and MAX-C rover. | |||
and Mars sample return mission | Possibly by 2020 | Orbiter, lander, rover, sample return | Being considered but not yet funded or scheduled. |
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