Astronomy:Human mission to Mars

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Short description: Proposed concepts
Concept for a Mars base, with ice home, pressurized rover, and Mars suits, 2016

The idea of sending humans to Mars has been the subject of aerospace engineering and scientific studies since the late 1940s as part of the broader exploration of Mars. Some have also considered exploring the Martian moons of Phobos and Deimos.[1] Long-term proposals have included sending settlers and terraforming the planet. Proposals for human missions to Mars came from e.g. NASA, Russia, Boeing, and SpaceX. As of 2022, only robotic landers and rovers have been on Mars. The farthest humans have been beyond Earth is the Moon.

Conceptual proposals for missions that would involve human explorers started in the early 1950s, with planned missions typically being stated as taking place between 10 and 30 years from the time they are drafted.[2] The list of crewed Mars mission plans shows the various mission proposals that have been put forth by multiple organizations and space agencies in this field of space exploration. The plans for these crews have varied, from scientific expeditions, in which a small group (between two and eight astronauts) would visit Mars for a period of a few weeks or more, to a continuous presence (e.g. through research stations, colonization, or other continuous habitation). By 2020, virtual visits to Mars, using haptic technologies, had also been proposed.[3]

Meanwhile, the unmanned exploration of Mars has been a goal of national space programs for decades, and was first achieved in 1965 with the Mariner 4 flyby. Human missions to Mars have been part of science fiction since the 1880s, and more broadly, in fiction, Mars is a frequent target of exploration and settlement in books, graphic novels, and films. The concept of a Martian as something living on Mars is part of the fiction.

Travel to Mars

The minimum distance between the orbits of Mars and Earth from 2014 to 2061, measured in astronomical units

The energy needed for transfer between planetary orbits, or delta-v, is lowest at intervals fixed by the synodic period. For EarthMars trips, the period is every 26 months (2 years, 2 months), so missions are typically planned to coincide with one of these launch periods. Due to the eccentricity of Mars's orbit, the energy needed in the low-energy periods varies on roughly a 15-year cycle[4] with the easiest periods needing only half the energy of the peaks.[5] In the 20th century, a minimum existed in the 1969 and 1971 launch periods and another low in 1986 and 1988, then the cycle repeated.[4] The next low-energy launch period occurs in 2033.[6]

Several types of mission plans have been proposed, including opposition class and conjunction class,[5] or the Crocco flyby.[7] The lowest energy transfer to Mars is a Hohmann transfer orbit, which would involve a roughly 9-month travel time from Earth to Mars, about 500 days (16 mo) at Mars to wait for the transfer window to Earth, and a travel time of about 9 months to return to Earth.[8][9] This would be a 34-month trip.

Shorter Mars mission plans have round-trip flight times of 400 to 450 days,[10] or under 15 months, but would require significantly higher energy. A fast Mars mission of 245 days (8.0 months) round trip could be possible with on-orbit staging.[11] In 2014, ballistic capture was proposed, which may reduce fuel cost and provide more flexible launch windows compared to the Hohmann.[12]

Three views of Mars, Hubble Space Telescope, 1997

In the Crocco grand tour, a crewed spacecraft would get a flyby of Mars and Venus in under a year in space.[13] Some flyby mission architectures can also be extended to include a style of Mars landing with a flyby excursion lander spacecraft.[14] Proposed by R. Titus in 1966, it involved a short-stay lander-ascent vehicle that would separate from a "parent" Earth-Mars transfer craft prior to its flyby of Mars. The Ascent-Descent lander would arrive sooner and either go into orbit around Mars or land, and, depending on the design, offer perhaps 10–30 days before it needed to launch itself back to the main transfer vehicle.[14] (See also Mars flyby.)

In the 1980s, it was suggested that aerobraking at Mars could reduce the mass required for a human Mars mission lifting off from Earth by as much as half.[15] As a result, Mars missions have designed interplanetary spacecraft and landers capable of aerobraking.[15]

Landing on Mars

Inserts depict observation and analysis to find a safe landing site

A number of unmanned spacecraft have landed on the surface of Mars, while some, such as the Schiaparelli EDM (2016), have failed what is considered a difficult landing. The Beagle2 failed in 2003. Among the successes:

Orbital capture

When an expedition reaches Mars, braking is required to enter orbit. Two options are available - rockets or aerocapture. Aerocapture at Mars for human missions was studied in the 20th century.[16] In a review of 93 Mars studies, 24 used aerocapture for Mars or Earth return.[16] One of the considerations for using aerocapture on crewed missions is a limit on the maximum force experienced by the astronauts. The current scientific consensus is that 5 g, or five times Earth gravity, is the maximum allowable deceleration.[16]

Survey work

Conducting a safe landing requires knowledge of the properties of the atmosphere, first observed by Mariner 4, and a survey of the planet to identify suitable landing sites. Major global surveys were conducted by Mariner 9 and Viking 1 and two orbiters, which supported the Viking landers. Later orbiters, such as Mars Global Surveyor, 2001 Mars Odyssey, Mars Express, and Mars Reconnaissance Orbiter, have mapped Mars in higher resolution with improved instruments. These later surveys have identified the probable locations of water, a critical resource.[17]


The largest limiting factor for sending humans to Mars is funding. In 2010, the estimated cost was roughly US$500 billion, though the actual costs are likely to be more.[18] Starting in the late 1950s, the early phase of space exploration was conducted as much to make a political statement as to make observations of the solar system. However, this proved to be both wasteful and unsustainable, and the current climate is one of international cooperation, with large projects such as the International Space Station and the proposed Lunar Gateway being built and launched by multiple countries.

Critics argue that the immediate benefits of establishing a human presence on Mars are outweighed by the immense cost, and that funds could be better redirected towards other programs, such as robotic exploration. Proponents of human space exploration contend that the symbolism of establishing a presence in space may garner public interest to join the cause and spark global cooperation. There are also claims that a long-term investment in space travel is necessary for humanity's survival.[18]

One factor reducing the funding needed to place a human presence on Mars may be space tourism. As the space tourism market grows and technological developments are made, the cost of sending humans to other planets will likely decrease accordingly. A similar concept can be examined in the history of personal computers; when computers were used only for scientific research, with minor use in big industry, they were big, rare, heavy, and costly. When the potential market increased and they started to become common in many homes (in Western and developed countries) for the purpose of entertainment such as computer games, and booking travel/leisure tickets, the computing power of home devices skyrocketed and prices plummeted.[19]


Main page: Medicine:Space medicine
Comparison of radiation doses – includes the amount detected on the trip from Earth to Mars by the RAD inside the MSL (2011–2013).[20][21][22] Vertical axis is in logarithmic scale, so the dose over a Mars year is about 15 times the DOE limit, not less than twice, as a quick glance might suggest. The actual dose would depend on factors such as spacecraft design and natural events such as solar flares.

Several key physical challenges exist for human missions to Mars:[23]

Artistic vision of spacecraft providing artificial gravity by spinning. (see also Centrifugal force)
  • Psychological effects of isolation from Earth and, by extension, the lack of community due to lack of a real-time connection with Earth (Compare Hermit)
  • Social effects of several humans living under cramped conditions for more than one Earth year, and possibly two or three years, depending on spacecraft and mission design
  • Lack of medical facilities
  • Potential failure of propulsion or life-support equipment

Some of these issues were estimated statistically in the HUMEX study.[36] Ehlmann and others have reviewed political and economic concerns, as well as technological and biological feasibility aspects.[37] While fuel for roundtrip travel could be a challenge, methane and oxygen can be produced using Martian H2O (preferably as water ice instead of liquid water) and atmospheric CO2 with mature technology.[38]

Planetary protection

Robotic spacecraft to Mars are currently required to be sterilized. The allowable limit is 300,000 spores on the exterior of general craft, with stricter requirements for spacecraft bound for "special regions" containing water.[39][40] Otherwise there is a risk of contaminating not only the life-detection experiments but possibly the planet itself.[41]

Sterilizing human missions to this level is impossible, as humans are host to typically a hundred trillion (1014) microorganisms of thousands of species of the human microbiota, and these cannot be removed. Containment seems the only option, but it is a major challenge in the event of a hard landing (i.e. crash).[42] There have been several planetary workshops on this issue, but with no final guidelines for a way forward yet.[43] Human explorers would also be vulnerable to back contamination to Earth if they become carriers of microorganisms.[44]

Mission proposals

Main page: Astronomy:List of crewed Mars mission plans

Over the past seven decades, a wide variety of mission architectures have been proposed or studied for human spaceflights to Mars. These have included chemical, nuclear, and electric propulsion, as well as a wide variety of landing, living, and return methodologies.

Artist's rendering of the planned Orion/DSH/Cryogenic Propulsion Module assembly.

A number of nations and organizations have long-term intentions to send humans to Mars.

  • The United States has several robotic missions currently exploring Mars, with a sample-return planned for the future. The Orion Multi-Purpose Crew Vehicle (MPCV) is intended to serve as the launch/splashdown crew delivery vehicle, with a Deep Space Habitat module providing additional living-space for the 16-month-long journey. The first crewed Mars Mission, which would include sending astronauts to Mars, orbiting Mars, and a return to Earth, is proposed for the 2030s.[2][45][46][47] Technology development for US government missions to Mars is underway, but there is no well-funded approach to bring the conceptual project to completion with human landings on Mars by the mid-2030s, the stated objective.[48] NASA is under presidential orders to land humans on Mars by 2033 although later years like 2035 or even late 2030s seem as a more realistic approach. NASA-funded engineers are studying a way to build potential human habitats there by producing bricks from pressurized Martian soil.[49]
  • The ESA has a long-term goal to send humans, but has not yet built a crewed spacecraft. It has sent robotic probes such as ExoMars in 2016 and plans to send the next probe in 2022.
  • Russia plans to send humans in the 2040–2045 timeframe.[50]

Technological innovations and hurdles

Depiction of plants growing in a Mars base. NASA plans to grow plants for space food.[51]
NASA has stated that robots will prepare an underground base for a human surface mission.[52]

Significant technological hurdles need to be overcome for human spaceflight to Mars.

Entry into the thin and shallow Martian atmosphere will pose significant difficulties with re-entry; compared to Earth with much denser atmosphere, any spacecraft will descend very rapidly to the surface and must be slowed down.[53] A heat shield has to be utilized.[54] NASA is carrying out research on retropropulsive deceleration technologies to develop new approaches to Mars atmospheric entry. A key problem with propulsive techniques is handling the fluid flow problems and attitude control of the descent vehicle during the supersonic retropropulsion phase of the entry and deceleration.[55]

A return mission to Mars will need to land a rocket to carry crew off the surface. Launch requirements mean that this rocket would be significantly smaller than an Earth-to-orbit rocket. Mars-to-orbit launch can also be achieved in single stage. Despite this, landing an ascent rocket on Mars will be difficult. Re-entry for a large rocket will be difficult.

In 2014, NASA proposed the Mars Ecopoiesis Test Bed.[56]

Intravenous fluid

One of the medical supplies that might be needed is a considerable mass of intravenous fluid, which is mainly water, but contains other substances so it can be added directly to the human blood stream. If it could be created on the spot from existing water, this would reduce mass requirements. A prototype for this capability was tested on the International Space Station in 2010.[57]

Advanced resistive exercise device

A person who is inactive for an extended period of time loses strength and muscle and bone mass. Spaceflight conditions are known to cause loss of bone mineral density in astronauts, increasing bone fracture risk. Last mathematical models predict 33% of astronauts will be at risk for osteoporosis during a human mission to Mars.[30] A resistive exercise device similar to ARED would be needed in the spaceship.

Breathing gases

While humans can breathe pure oxygen, usually additional gases such as nitrogen are included in the breathing mix. One possibility is to take in situ nitrogen and argon from the atmosphere of Mars, but they are hard to separate from each other.[58] As a result, a Mars habitat may use 40% argon, 40% nitrogen, and 20% oxygen.[58]

An idea for keeping carbon dioxide out of the breathing air is to use reusable amine-bead carbon dioxide scrubbers.[59] While one carbon dioxide scrubber filters the astronaut's air, the other is vented to the Mars atmosphere.[59]

Related missions

Some missions may be considered a "Mission to Mars" in their own right, or they may only be one step in a more in-depth program. An example of this is missions to Mars's moons, or flyby missions.

Missions to Deimos or Phobos

Many Mars mission concepts propose precursor missions to the moons of Mars, for example a sample return mission to the Mars moon Phobos[60] – not quite Mars, but perhaps a convenient stepping stone to an eventual Martian surface mission. Lockheed Martin, as part of their "Stepping stones to Mars" project, called the "Red Rocks Project", proposed to explore Mars robotically from Deimos.[61][62][63]

Use of fuel produced from water resources on Phobos or Deimos has also been proposed.

Mars sample return missions

Artist concept of SCIM gathering a sample of the Martian atmosphere
Sample return mission concept

An uncrewed Mars sample return mission (MSR) has sometimes been considered as a precursor to crewed missions to Mars's surface.[64] In 2008, the ESA called a sample return "essential" and said it could bridge the gap between robotic and human missions to Mars.[64] An example of a Mars sample return mission is Sample Collection for Investigation of Mars.[65] Mars sample return was the highest priority Flagship Mission proposed for NASA by the Planetary Decadal Survey 2013–2022: The Future of Planetary Science.[66] However, such missions have been hampered by complexity and expense, with one ESA proposal involving no less than five different uncrewed spacecraft.[67]

Sample return plans raise the concern, however remote, that an infectious agent could be brought to Earth.[67] Regardless, a basic set of guidelines for extraterrestrial sample return has been laid out depending on the source of sample (e.g. asteroid, Moon, Mars surface, etc.)[68]

At the dawn of the 21st century, NASA crafted four potential pathways to Mars human missions,[69] of which three included a Mars sample return as a prerequisite to human landing.[69]

Currently, the rover Perseverance is equipped with a device that will allow it to pick up and seal samples of rock from Mars, to be returned at a later date by another mission. Perseverance as part of the Mars 2020 mission was launched on top of an Atlas V rocket on 30 July 2020 at (11:50 UTC).[70] Confirmation that the rover had landed on Mars was received on 18 February 2021 at 20:55 UTC.[71]

Crewed orbital missions

Starting in 2004, NASA scientists have proposed to explore Mars via telepresence from human astronauts in orbit.[72][73]

A similar idea was the proposed "Human Exploration using Real-time Robotic Operations" mission.[74][75]

See also


  1. JAXA (2021-09-20). "Japan Space Agency: Why We're Exploring the Moons of Mars" (in en-US). 
  2. 2.0 2.1 Wall, Mike (27 August 2019). "Astronauts Will Face Many Hazards on a Journey to Mars - NASA is trying to bring the various risks down before launching astronauts to Mars in the 2030s.". 
  3. Von Drehle, David (15 December 2020). "Humans don't have to set foot on Mars to visit it". The Washington Post. 
  4. 4.0 4.1 David S. F. Portree, Humans to Mars: Fifty Years of Mission Planning, 1950–2000, NASA Monographs in Aerospace History Series, Number 21, February 2001. Available as NASA SP-2001-4521.
  5. 5.0 5.1 Page 18–19 in Chapter 3 of David S. F. Portree's Humans to Mars: Fifty Years of Mission Planning, 1950–2000, NASA Monographs in Aerospace History Series, Number 21, February 2001. Available as NASA SP-2001-4521
  6. Wooster, Paul D. (2007). "Mission design options for human Mars missions". International Journal of Mars Science and Exploration 3: 12. doi:10.1555/mars.2007.0002. Bibcode2007IJMSE...3...12W. 
  7. Page 15–16 in Chapter 3 of David S. F. Portree's Humans to Mars: Fifty Years of Mission Planning, 1950–2000, NASA Monographs in Aerospace History Series, Number 21, February 2001. Available as NASA SP-2001-4521
  8. "Hohmann transfer orbit diagram" (in en). 
  9. "Homann Transfers". 
  10. Wernher von Braun, "Popular Science". Bonnier Corporation. March 1964. 
  11. "Folta, et al. - FAST MARS TRANSFERS THROUGH ON-ORBIT STAGING. (2012)". 
  12. Matt Williams – Universe Today. "Making A Trip To Mars Cheaper & Easier: The Case For Ballistic Capture". io9. 
  13. "Crocco". 
  14. 14.0 14.1 "To Mars by Flyby-Landing Excursion Mode (FLEM) (1966)". Wired. 
  15. 15.0 15.1 "Photo-s88_35629". 
  16. 16.0 16.1 16.2 Vaughan, Diane; James, Bonnie F.; Murk, Michelle M. (26 April 2005). A Comparative Study of Aerocapture Missions with a Mars Destination. Retrieved 16 March 2019. 
  17. Anderson, Gina (2015-09-28). "NASA Confirms Evidence That Liquid Water Flows on Today's Mars". 
  18. 18.0 18.1 Taylor, Fredric (2010). The Scientific Exploration of Mars. Cambridge: Cambridge University Press. pp. 306. ISBN 978-0-521-82956-4. 
  19. Sheetz, Michael (September 26, 2020). "How SpaceX, Virgin Galactic, Blue Origin and others compete in the growing space tourism market". 
  20. 20.0 20.1 Kerr, Richard (31 May 2013). "Radiation Will Make Astronauts' Trip to Mars Even Riskier". Science 340 (6136): 1031. doi:10.1126/science.340.6136.1031. PMID 23723213. Bibcode2013Sci...340.1031K. 
  21. 21.0 21.1 Zeitlin, C. (31 May 2013). "Measurements of Energetic Particle Radiation in Transit to Mars on the Mars Science Laboratory". Science 340 (6136): 1080–1084. doi:10.1126/science.1235989. PMID 23723233. Bibcode2013Sci...340.1080Z. 
  22. 22.0 22.1 Chang, Kenneth (30 May 2013). "Data Point to Radiation Risk for Travelers to Mars". The New York Times. 
  23. Regis, Ed (September 21, 2015). "Let's Not Move To Mars". New York Times. 
  24. Scharf, Calib A. (20 January 2020). "Death on Mars - The martian radiation environment is a problem for human explorers that cannot be overstated". Scientific American. 
  25. Saganti, Premkumar B.; Cucinotta, Francis A.; Wilson, John W.; Cleghorn, Timothy F.; Zeitlin, Cary J. (October 2006). "Model calculations of the particle spectrum of the galactic cosmic ray (GCR) environment: Assessment with ACE/CRIS and MARIE measurements". Radiation Measurements 41 (9–10): 1152–1157. doi:10.1016/j.radmeas.2005.12.008. Bibcode2006RadM...41.1152S. 
  26. Shiga, David (2009-09-16). "Too much radiation for astronauts to make it to Mars". New Scientist (2726). 
  27. Fong, MD, Kevin (12 February 2014). "The Strange, Deadly Effects Mars Would Have on Your Body". Wired. Retrieved 12 February 2014. 
  28. Gelling, Cristy (29 June 2013). "Atom & cosmos: Mars trip would mean big radiation dose: Curiosity instrument confirms expectation of major exposures: Atom & cosmos: Mars trip would mean big radiation dose: Curiosity instrument confirms expectation of major exposures". Science News 183 (13): 8. doi:10.1002/scin.5591831304. 
  29. Scott, Jim (30 September 2017). "Large solar storm sparks global aurora and doubles radiation levels on the martian surface". 
  30. 30.0 30.1 Axpe, Eneko; Chan, Doreen; Abegaz, Metadel F.; Schreurs, Ann-Sofie; Alwood, Joshua S.; Globus, Ruth K.; Appel, Eric A. (2020). "A human mission to Mars: Predicting the bone mineral density loss of astronauts". PLOS ONE 15 (1): e0226434. doi:10.1371/journal.pone.0226434. PMID 31967993. Bibcode2020PLoSO..1526434A. 
  31. Mader, Thomas H.; Gibson, C. Robert; Pass, Anastas F.; Kramer, Larry A.; Lee, Andrew G.; Fogarty, Jennifer; Tarver, William J.; Dervay, Joseph P. et al. (October 2011). "Optic Disc Edema, Globe Flattening, Choroidal Folds, and Hyperopic Shifts Observed in Astronauts after Long-duration Space Flight". Ophthalmology 118 (10): 2058–2069. doi:10.1016/j.ophtha.2011.06.021. PMID 21849212. 
  32. Puiu, Tibi (November 9, 2011). "Astronauts' vision severely affected during long space missions". 
  33. "Breaking News Videos, Story Video and Show Clips –". CNN. 
  34. Strickland, Ashley (15 November 2019). "Astronauts experienced reverse blood flow and blood clots on the space station, study says". CNN News. 
  35. Marshall-Goebel, Karina (13 November 2019). "Assessment of Jugular Venous Blood Flow Stasis and Thrombosis During Spaceflight". JAMA Network Open 2 (11): e1915011. doi:10.1001/jamanetworkopen.2019.15011. PMID 31722025. 
  36. Horneck, Gerda (2006). "General human health issues for Moon and Mars missions: Results from the HUMEX study". Advances in Space Research 37 (1): 100–108. doi:10.1016/j.asr.2005.06.077. Bibcode2006AdSpR..37..100H. 
  37. Ehlmann, Bethany L. (2005). "Humans to Mars: A feasibility and cost–benefit analysis". Acta Astronautica 56 (9–12): 851–858. doi:10.1016/j.actaastro.2005.01.010. PMID 15835029. Bibcode2005AcAau..56..851E. 
  38. Rapp, D.; Andringa, J.; Easter, R.; Smith, J.H.; Wilson, T.J.; Clark, D.L.; Payne, K. (2005). "Preliminary system analysis of in situ resource utilization for Mars human exploration". 2005 IEEE Aerospace Conference. pp. 319–338. doi:10.1109/AERO.2005.1559325. ISBN 0-7803-8870-4. 
  39. Queens University Belfast scientist helps NASA Mars project "No one has yet proved that there is deep groundwater on Mars, but it is plausible as there is certainly surface ice and atmospheric water vapour, so we wouldn't want to contaminate it and make it unusable by the introduction of micro-organisms."
  40. COSPAR PLANETARY PROTECTION POLICY (20 October 2002; As Amended to 24 March 2011)
  41. An Astrobiology Strategy for the Exploration of Mars. 2007. doi:10.17226/11937. ISBN 978-0-309-10851-5. Retrieved 12 June 2015. 
  42. When Biospheres Collide – a history of NASA's Planetary Protection Programs, Michael Meltzer, May 31, 2012, see Chapter 7, Return to Mars – final section: "Should we do away with human missions to sensitive targets"
  43. Johnson, James E. "Planetary Protection Knowledge Gaps for Human Extraterrestrial Missions: Goals and Scope." (2015)
  44. Safe on Mars page 37 "Martian biological contamination may occur if astronauts breathe contaminated dust or if they contact material that is introduced into their habitat. If an astronaut becomes contaminated or infected, he or she conceivably could transmit Martian biological entities or even disease to fellow astronauts, or introduce such entities into the biosphere upon returning to Earth. A contaminated vehicle or item of equipment returned to Earth could also be a source of contamination."
  45. "Nasa's Orion spacecraft prepares for launch in first step towards manned Mars mission". The Associated Press. 
  46. "Twitter feed of NASA". Twitter. 
  47. "NASA's Orion Flight Test and the Journey to Mars". NASA website. 
  48. Berger, Eric (2016-10-12). "Why Obama's "giant leap to Mars" is more of a bunny hop right now". Ars Technica. 
  49. Johnston, Ian. "'Incredibly brave' Mars colonists could live in red-brick houses, say engineers", The Independent (April 27, 2017).
  50. "Error: no |title= specified when using {{Cite web}}" (in ru). 
  51. Rainey, Kristine (7 August 2015). "Crew Members Sample Leafy Greens Grown on Space Station". 
  52. "NASA Chief: We're Closer to Sending Humans on Mars Than Ever Before". 
  53. Coates, Andrew. "Decades of attempts show how hard it is to land on Mars – here's how we plan to succeed in 2021".,surface%2C%20and%20must%20be%20slowed.. 
  54. "Spinning heat shield for future spacecraft". 
  55. Morring, Frank, Jr. (2014-10-16). "NASA, SpaceX Share Data On Supersonic Retropropulsion : Data-sharing deal will help SpaceX land Falcon 9 on Earth and NASA put humans on Mars". Aviation Week. Retrieved 2014-10-18. "the requirements for returning a first stage here on the Earth propulsively, and then ... the requirements for landing heavy payloads on Mars, there's a region where the two overlap—are right on top of each other ... If you start with a launch vehicle, and you want to bring it down in a controlled manner, you're going to end up operating that propulsion system in the supersonic regime at the right altitudes to give you Mars-relevant conditions." 
  56. Hall, Loura (2017-03-24). "Mars Ecopoiesis Test Bed" (in en). NASA. 
  57. "A Solution for Medical Needs and Cramped Quarters in Space IVGEN Undergoes Lifetime Testing in Preparation For Future Missions". NASA. 7 June 2013. 
  58. 58.0 58.1 "The Caves of Mars – Martian Air Breathing Mice". 
  59. 59.0 59.1 "Suiting Up for the Red Planet". 30 September 2015. 
  60. Natasha, Bosanac; Ana, Diaz; Victor, Dang; Frans, Ebersohn; Stefanie, Gonzalez; Jay, Qi; Nicholas, Sweet; Norris, Tie et al. (1 March 2014). Manned sample return mission to Phobos: A technology demonstration for human exploration of Mars. pp. 1–20. ISBN 9781479955824. 
  61. Geoffrey A. Landis, "Footsteps to Mars: an Incremental Approach to Mars Exploration," Journal of the British Interplanetary Society, Vol. 48, pp. 367-342 (1995); presented at Case for Mars V, Boulder CO, 26–29 May 1993; appears in From Imagination to Reality: Mars Exploration Studies, R. Zubrin, ed., AAS Science and Technology Series Volume 91 pp. 339-350 (1997). (text available as Footsteps to Mars pdf file)
  62. Larry Page Deep Space Exploration – Stepping Stones builds up to "Red Rocks : Explore Mars from Deimos"
  63. "One Possible Small Step Toward Mars Landing: A Martian Moon". 20 April 2011. 
  64. 64.0 64.1 esa. "Mars Sample Return: bridging robotic and human exploration". 
  65. Jones, S.M. (2008). "Ground Truth From Mars (2008) – Mars Sample Return at 6 Kilometers per Second: Practical, Low Cost, Low Risk, and Ready". USRA. 
  66. "Science Strategy – NASA Solar System Exploration". 
  67. 67.0 67.1 "Mars Sample Return". 
  68. "Archived copy". 
  69. 69.0 69.1 "Next On Mars". 
  70. "Launch Windows" (in en). 
  71. "Touchdown! NASA's Mars Perseverance Rover Safely Lands on Red Planet" (in en). 
  72. Landis, G.A. (2008). "Teleoperation from Mars Orbit: A Proposal for Human Exploration". Acta Astronautica 62 (1): 59–65. doi:10.1016/j.actaastro.2006.12.049. Bibcode2008AcAau..62...59L. ; presented as paper IAC-04-IAA., 55th International Astronautical Federation Congress, Vancouver BC, Oct. 4-8 2004.
  73. M. L. Lupisella, "Human Mars Mission Contamination Issues", Science and the Human Exploration of Mars, January 11–12, 2001, NASA Goddard Space Flight Center, Greenbelt, MD. LPI Contribution No. 1089. (accessed 11/15/2012)
  74. George R. Schmidt, Geoffrey A. Landis, and Steven R. Oleson NASA Glenn Research Center, Cleveland, Ohio, 44135 HERRO Missions to Mars and Venus using Telerobotic Surface Exploration from Orbit 48th AIAA Aerospace Sciences Meeting Including the New Horizons Forum and Aerospace Exposition 4–7 January 2010, Orlando, Florida
  75. HERRO TeleRobotic Exploration of Mars, Geoffrey Landis, Mars Society 2010 4 part YouTube Video

Further reading

External links