This artist illustration depicts four orbiters as part of the International-Mars Ice Mapper (I-MIM) mission concept. Low and to the left, an orbiter passes above the Martian surface, detecting buried water ice through a radar instrument and large reflector antenna. Circling Mars at a higher altitude are three telecommunications orbiters with one shown relaying data back to Earth.
Mars Exploration Ice Mapper
|Mission type||Mars orbiter|
|Operator||NASA / JAXA / CSA / ASI|
|Mission duration||2 years (planned)|
|Start of mission|
|Launch site||Cape Canaveral|
|Reference system||Areocentric orbit|
|Periareon altitude||250–320 km (160–200 mi)|
|Apoareon altitude||250–320 km (160–200 mi)|
The International-Mars Ice Mapper (I-MIM) mission is a proposed Mars orbiter being developed by NASA in collaboration with the Japan Aerospace Exploration Agency (JAXA), the Canadian Space Agency (CSA), and the Italian Space Agency (ASI). As the mission concept evolves, there may be opportunities for other space agency and commercial partners to join the mission. The goal of the orbiter is the quantification of extent and volume of water ice in non-polar regions of Mars. The results are intended to support future Mars missions, especially with respect to the search for habitable environments and accessible In situ resource utilization (ISRU) resources. The International-Mars Ice Mapper is an "exploration precursor mission", comparing it to the Lunar Reconnaissance Orbiter (LRO) mission. The planned launch date of the mission is 2026.
The mission is to search for ice deposits under the surface of Mars, precursor for human missions there. By identifying locations where water ice may exist within 5-10 meters of the surface and thus could be accessed by crewed expeditions. The mission plans to scan specific locations on the Martian surface below 2 km (1.2 mi) elevation (to enable entry, descent and landing). The target areas for radar scans are between 25° and 40° northern latitude and 25° and 40° southern latitude. The upper limit of 40° was chosen to have favorable conditions for solar arrays. The lower bound of 25° is intended to maximize the proximity of locating ground ice (since availability of ground ice generally decreases toward the equator due to increased insolation).
The ice-mapping mission could help the agency identify potential science objectives for initial human missions to Mars, which are expected to be designed for about 30 days of exploration on the surface. For example, identifying and characterizing accessible water ice could lead to human-tended science, such as ice coring to support the search for life. Mars Ice Mapper also could provide a map of water-ice resources for later human missions with longer surface expeditions, as well as help meet exploration engineering constraints, such as avoidance of rock and terrain hazards. Mapping shallow water ice could also support supplemental high-value science objectives related to Martian climatology and geology.
Beyond promoting scientific observations while the orbiter completes its reconnaissance work, the agency partners will explore mission-enabling rideshare opportunities as part of their next phase of study. All science data from the mission would be made available to the international science community for both planetary science and Mars reconnaissance. This approach is similar to what NASA is doing at the Moon under the Artemis program – sending astronauts to lunar South Pole, where ice is trapped in the permanently shadowed regions of the pole.
Access to water ice would also be central to scientific investigations on the surface of Mars that are led by future human explorers. Such explorers may one day core, sample, and analyze the ice to better understand the record of climatic and geologic change on Mars and its astrobiological potential, which could be revealed through signs of preserved ancient microbial life or even the possibility of living organisms, if Mars ever harbored life. Ice is also a critical natural resource that could eventually supply hydrogen and oxygen for fuel. These elements could also provide resources for backup life support, civil engineering, mining, manufacturing, and, eventually, agriculture on Mars. Transporting water from Earth to deep space is extremely costly, so a local resource is essential to sustainable surface exploration.
"In addition to supporting plans for future human missions to Mars, learning more about subsurface ice will bring significant opportunities for scientific discovery", said Eric Ianson, NASA Planetary Science Division Deputy Director and Mars Exploration Program Director. "Mapping near-surface water ice would reveal an as-yet hidden part of the Martian hydrosphere and the layering above it, which can help uncover the history of environmental change on Mars and lead to our ability to answer fundamental questions about whether Mars was ever home to microbial life or still might be today".
The Red Planet is providing great research return for robotic exploration and the search for ancient life in our Solar System. This latest news comes ahead of the agency's Perseverance rover landing on Mars, which is scheduled to take place on 18 February 2021, following a seven-month journey in space. NASA and the European Space Agency (ESA) also recently announced they are moving forward with the Mars sample-return mission.
The CSA would provide the radar instrument, JAXA the spacecraft bus and ASI the communications subsystem for the spacecraft. NASA would be responsible for overall mission management and for providing the launch of the spacecraft. The mission will cost US$185 million.
The NASA included an illustration of Mars Ice Mapper communicating with three spacecraft in Mars orbit, acting as communications relays back to Earth. The NASA have previously discussed developing a communications satellite network at Mars, perhaps through public-private partnerships, to support Mars Ice Mapper.
The radar has the following technical specification: