Mars sample-return mission
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A Mars sample-return mission (MSR) would be a spaceflight mission to collect rock and dust samples on Mars and then return them to Earth. Sample-return would be a very powerful type of exploration, because analysis is freed from the time, budget, and space constraints of spacecraft sensors. Any of Earth's laboratories could study a sample.
According to Louis Friedman, Executive Director of The Planetary Society, a Mars sample-return mission is often described by the planetary science community as one of the most important robotic space missions, due to its high expected scientific return on investment.
Over time, several concept missions has been studied, but none of them got beyond the study phase. The three latest concepts for a MSR mission are a NASA-ESA proposal, a Russian proposal (Mars-Grunt), and a Chinese proposal.
Scientific value[edit | edit source | hide | hide all]
The return of Mars samples would be beneficial to science by allowing more extensive analysis to be undertaken of the samples than could be done by instruments painstakingly transferred to Mars. Also, the presence of the samples on Earth would allow scientific equipment to be used on stored samples, even years and decades after the sample-return mission.
In 2006, MEPAG identified 55 important future science investigations related to the exploration of Mars. In 2008, they concluded that about half of the investigations "could be addressed to one degree or another by MSR", making MSR "the single mission that would make the most progress towards the entire list" of investigations. Moreover, it was found that a significant fraction of the investigations cannot be meaningfully advanced without returned samples.
One source of Mars samples is what are thought to be Martian meteorites, which are rocks ejected from Mars that made their way to Earth. Of over 61,000 meteorites that have been found on Earth, 132 were identified as Martian as of 3 March 2014[update]. These meteorites are thought to be from Mars because they have elemental and isotopic compositions that are similar to rocks and atmosphere gases analyzed by spacecraft on Mars.
In 1996 the possibility of life on Mars was questioned again when apparent microfossils might have been found in a Mars meteorite (see ALH84001). This led to a renewed interest in a Mars sample-return, and several different architectures were considered. NASA administrator Goldin laid out three options for MSR: "paced", "accelerated", and "aggressive". It was thought that MSR could be done for less than 100 million USD per year, with something similar to then-current Mars exploration budgets.
History[edit | edit source | hide]
For at least three decades, Western scientists have advocated the return of geological samples from Mars. One concept was studied with the Sample Collection for Investigation of Mars (SCIM) proposal, which involved sending a spacecraft in a grazing pass through Mars upper atmosphere to collect dust and air samples without landing or orbiting.
The Soviet Union considered a Mars sample-return mission, Mars 5NM, in 1975 but it was cancelled due to the repeated failures of the N1 rocket that would have been used to launch it. A double sample-return mission, Mars 5M (Mars-79) planned for 1979, was cancelled due to complexity and technical problems.
One mission concept (provisionally named simply Mars Sample-Return) was originally considered by NASA's Mars Exploration Program to return samples by 2008, but was cancelled following a review of the program. A NASA-ESA concept mission was aborted in 2012.
The United States' Mars Exploration Program, formed after Mars Observer's failure in September 1992, supported a Mars sample-return. One example of a mission architecture was the Groundbreaking Mars Sample-Return by MacPhereson in the early 2000s.
In early 2011, the National Research Council's Planetary Science Decadal Survey, which laid out mission planning priorities for the period 2013–2022 at the request of NASA and the NSF, declared a MSR campaign its highest priority Flagship Mission for that period. In particular, it endorsed the proposed Mars Astrobiology Explorer-Cacher (MAX-C) mission in a "descoped" (less ambitious) form, although this mission plan was officially cancelled in April 2011.
The key mission requirement for the planned Mars 2020 rover is that it must help prepare NASA for its MSR campaign,. which is needed before any crewed mission takes place. Such effort would require three additional vehicles: an orbiter, a fetch rover, and a Mars ascent vehicle (MAV).
NASA–ESA concept[edit | edit source | hide]
In mid-2006, the international Mars Architecture for the Return of Samples (iMARS) Working Group was chartered by the International Mars Exploration Working Group (IMEWG) to outline the scientific and engineering requirements of an internationally sponsored and executed Mars sample-return mission in the 2018–2023 time frame.
In October 2009, NASA and ESA established the Mars Exploration Joint Initiative to proceed with the ExoMars mission, whose ultimate aim is "the return of samples from Mars in the 2020s". A first step in this was one particular proposal, a joint project between NASA and ESA called ExoMars, would launch in 2018 with unspecified missions to return the sample itself expected in the 2020–2022 time frame. The cancellation of the caching rover MAX-C and later NASA withdrawal from ExoMars, pushed back a sample-return mission to an undetermined date.
Due to budget limitations the MAX-C mission, which was the first NASA-ESA mission leading to a MSR, was canceled in 2011 and the overall plan in 2012. The pull-out was described as "traumatic" for the science community. However, in April 2018, a letter of intent was signed by NASA and ESA that may provide a basis for a Mars sample-return mission.
NASA proposals[edit | edit source | hide]
In September 2012, NASA announced its intention to further study several strategies of bringing a sample of Mars to Earth – including a multiple launch scenario, a single-launch scenario and a multiple-rover scenario – for a mission beginning as early as 2018. Dozens of samples would be collected and cached by the Mars 2020 rover, and would be left on the surface of Mars for possible later retrieval. A "fetch rover" would retrieve the sample caches and deliver them to a Mars ascent vehicle (MAV). In July 2018 NASA contracted Airbus to produce a "fetch rover" concept. The MAV would launch from Mars and enter a 500 km orbit and rendezvous with a new Mars orbiter. The sample container would be transferred to an Earth entry vehicle (EEV) which would bring it to Earth, enter the atmosphere under a parachute and hard-land for retrieval and analyses in specially designed safe laboratories.
Two-launches architecture[edit | edit source | hide]
In this scenario, the sample-return mission would span two launches at an interval of about four years. The first launch would be for the orbiter, the second for the lander. The lander would include the Mars Ascent Vehicle (MAV).
Three-launches architecture[edit | edit source | hide]
This concept is to have the sample-return mission split into a total of three launches. In this scenario, the sample-collection rover (e.g. Mars 2020 rover) would be launched separately to land on Mars first, and carry out analyses and sample collection over a lifetime of at least 500 Sols (Martian days).
Some years later, a Mars orbiter would be launched, followed by the lander including the Mars Ascent Vehicle (MAV). The lander would bring a small and simple "fetch rover", whose sole function would be to retrieve the sample containers from the caches left on the surface or directly from the Mars 2020 rover, and return them to the lander where it would be loaded onto the MAV for delivery to the orbiter and then be sent to Earth.
This design would ease the schedule of the whole mission, giving controllers time and flexibility to carry out the required operations. Furthermore, the program could rely on the successful landing system developed for the Mars Science Laboratory, avoiding the costs and risks associated with developing and testing yet another landing system from scratch.
SCIM[edit | edit source | hide]
SCIM (Sample Collection for Investigation of Mars) was a low-cost low-risk Mars sample-return mission design, proposed in the Mars Scout Program. SCIM would return dust and air samples without landing or orbiting, by dipping through the atmosphere as it collects Mars material. It uses heritage from the successful Stardust and Genesis sample-return missions.
Additional plans[edit | edit source | hide]
Russia[edit | edit source | hide]
A Russian Mars sample-return mission concept is Mars-Grunt. It is meant to use Fobos-Grunt design heritage. Plans as of 2011 envisioned a two-stage architecture with an orbiter and a lander (but no roving capability), with samples gathered from the immediate surroundings of the lander by a robotic arm.
China[edit | edit source | hide]
China has plans for a Mars sample-return mission by 2030. The mission plan combines elements of remote sensing of the surface, soft landing, using a rover to gather samples, then sample-return.
France[edit | edit source | hide]
France has worked towards a sample-return for many years. This included the preparation of laboratories for returned samples, and numerous proposals. They worked on the development of a Mars sample-return orbiter, which would capture and return the samples as part of a joint mission with either the United States, or other European countries.
Japan[edit | edit source | hide]
On 9 June 2015, the Japanese Aerospace Exploration Agency (JAXA) unveiled a plan named Martian Moons Exploration (MMX) to retrieve samples from one of the moons of Mars. This mission will build on the expertise to be gained from the Hayabusa 2 and SLIM missions. Of the two moons, Phobos's orbit is closer to Mars and its surface may have adhered particles blasted from the red planet; thus the Phobos samples collected by MMX may contain material originating from Mars itself. Japan has also shown interest on participating in an international Mars sample-return mission.
Potential for back contamination[edit | edit source | hide]
Since it is currently unknown whether life forms exist on Mars, the mission could potentially transfer viable organisms resulting in back contamination—the introduction of extraterrestrial organisms into Earth's biosphere. The scientific consensus is that the potential for large-scale effects, either through pathogenesis or ecological disruption, is extremely small. Nevertheless, returned samples from Mars will be treated as potentially biohazardous until scientists can determine that the returned samples are safe. The goal is to reduce the probability of release of a Mars particle to less than one in a million. In addition, the proposed NASA Mars Sample-return mission will not be approved by NASA until the National Environmental Policy Act (NEPA) process has been completed. The NEPA process would require a public review of all potential impacts that could result from MSR, including worst case back contamination scenarios. It is likely that a formal Environmental Impact Statement (EIS) would have to be prepared. Furthermore, under the terms of Article VII of the Outer Space Treaty and probably various other legal frameworks, were a release of organisms to occur, the releasing nation or nations would be liable for any resultant damages.
Part of the sample-return mission would be to prevent contact between the Martian environment and the exterior of the sample container. In order to eliminate the risk of parachute failure, the current plan is to use the thermal protection system to cushion the capsule upon impact (at terminal velocity). The sample container will be designed to withstand the force of the impact. To receive the returned samples, NASA proposed a specially designed Biosafety Level 4 containment facility, the Mars Sample-Return Receiving facility (MSRRF). Not knowing what properties (e.g., size) any Martian organisms might exhibit is a complication in design of such a facility.
Precisely because Mars is an environment of great potential biological interest, it is possible that on Mars there are pathogens, organisms which, if transported to the terrestrial environment, might do enormous biological damage - a Martian plague, the twist in the plot of H. G. Wells' War of the Worlds, but in reverse. This is an extremely grave point. On the one hand, we can argue that Martian organisms cannot cause any serious problems to terrestrial organisms, because there has been no biological contact for 4.5 billion years between Martian and terrestrial organisms. On the other hand, we can argue equally well that terrestrial organisms have evolved no defenses against potential Martian pathogens, precisely because there has been no such contact for 4.5 billion years. The chance of such an infection may be very small, but the hazards, if it occurs, are certainly very high.
The NRC and ESF studies came to the conclusion that though the potential for large-scale negative effects appears to be very low, it is not demonstrably zero . These findings on risks of environmental disruption are accepted by most participants in this debate (with the notable exception of Robert Zubrin). As a result, it is agreed by most researchers that a full and open public debate of the back contamination issues is needed at an international level. This is also a legal requirement.
The view of NASA, and ESA, is that these risks can be contained and that a sample return can be carried out safely provided the correct precautions are taken. For details see Mars Sample Receiving Facility and sample containment
The International Committee Against Mars Sample Return are of the view that, given that equipment can fail and there can be accidents, such a sample return is hard to guarantee safe to the level that would be needed when the fate of the environment of Earth itself could be at stake. They recommend searching for life in situ first, and have as their main goal, that samples are certified safe in situ or in space first before they are returned to Earth.
Having planetary/cometary samples certified as "biosphere safe" in space or in-situ before they are transferred to the Earth’s surface is our main goal and intention.
NASA Sample-Return Robot Challenge[edit | edit source | hide]
The Sample-Return Robot Challenge, as part of NASA's Centennial Challenges program, offered a total $1.5 million to teams that can build fully autonomous robots that can find, retrieve, and return up to 10 different sample types within a large outdoor environment (80,000 m2). The challenge started in 2012 and ended in 2016. Over 50 teams competed during the 5-year history of the NASA Challenge. A robot named Cataglyphis, developed by Team Mountaineers from West Virginia University completed the final challenge in 2016.
See also[edit | edit source | hide]
- ExoMars, Aurora multi-mission flagship
- Fobos-Grunt, Russian-Chinese sample-return mission to Phobos (moon of Mars) (crashed)
- InSight, Mars sample-return mission (launched 2018)
- Mars 2020 rover, plans may include a sample-cacher
- Mars Astrobiology Explorer-Cacher (MAX-C) (cancelled in 2012)
- Mars meteorite
References[edit | edit source | hide]
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"Assessment of Planetary Protection Requirements for Mars Sample Return Missions", National Research Council, 2009, chapter 5, "The Potential for Large-Scale Effects".
"Thus, a key question posed to the committe is whether a putative martian organism or organisms, inadvertently released from containment, could produce large-scale negative pathogenic effects in humans or have a destructive impact on Earth's ecological system or environments." (page 45)
They divide it into 3 categories
- Large-scale negative pathogenic effects in humans;
- Destructive impacts on Earth's ecological systems or environments; and
- Toxic and other effects attributable to microbes, their cellular structures, or extracellular products.
They conclude that the last one is unlikely. But for the other two
The committee found that the potential for large-scale negative effects on Earth's inhabitants or environment by a returned martian life form appears to be low, but is not demonstrably zero.(page 48)
- Robert Zubrin "Contamination From Mars: No Threat", The Planetary Report July/Aug. 2000, P.4–5
- transcription of a tele-conference interview with ROBERT ZUBRIN conducted on March 30, 2001 by the class members of STS497 I, "Space Colonization"; Instructor: Dr. Chris Churchill
- "5: "The Potential for Large-Scale Effects"". Mars Sample Return backward contamination - strategic advice (PDF) (Report). European Science Foundation. 2012.
RECOMMENDATION 10: Considering the global nature of the issue, consequences resulting from an unintended release could be borne by a larger set of countries than those involved in the programme. It is recommended that mechanisms dedicated to ethical and social issues of the risks and benefits raised by an MSR are set up at the international level and are open to representatives of all countries.line feed character in
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- Mars Sample Return backward contamination – Strategic advice and requirements see 7.2: Responsibility and liability of States
- M. S. Race Planetary Protection, Legal Ambiguity, and the Decision Making Process for Mars Sample Return Adv. Space Res. vol 18 no 1/2 pp (1/2)345-(1/2)350 1996
- ICAMSR - Charter
- Harbaugh, Jennifer (2015-07-15). "NASA's Centennial Challenges: Sample-Return Robot Challenge". Retrieved 2016-09-16.
[edit | edit source | hide]
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