{"id":2031,"date":"2026-10-15T15:10:58","date_gmt":"2026-10-15T15:10:58","guid":{"rendered":"https:\/\/redzine.co.uk\/index.php\/2026\/10\/15\/how-did-mars-get-its-moons-japans-mmx-space-mission-aims-to-solve-the-puzzle\/"},"modified":"2026-10-15T15:10:58","modified_gmt":"2026-10-15T15:10:58","slug":"how-did-mars-get-its-moons-japans-mmx-space-mission-aims-to-solve-the-puzzle","status":"publish","type":"post","link":"https:\/\/redzine.co.uk\/index.php\/2026\/10\/15\/how-did-mars-get-its-moons-japans-mmx-space-mission-aims-to-solve-the-puzzle\/","title":{"rendered":"How did Mars get its moons? Japan\u2019s MMX space mission aims to solve the puzzle"},"content":{"rendered":"<figure><img decoding=\"async\" src=\"https:\/\/images.theconversation.com\/files\/766274\/original\/file-20261014-73-bf9ypn.jpg?ixlib=rb-4.1.1&amp;rect=58%2C0%2C1798%2C1198&amp;q=45&amp;auto=format&amp;w=1050&amp;h=700&amp;fit=crop\" \/><figcaption><span class=\"caption\">Phobos is dominated by Stickney crater, a 9km (5.6 mile) bowl visible on the right.<\/span> <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/science.nasa.gov\/mars\/moons\/phobos\/\">NASA\/JPL-Caltech\/University of Arizona<\/a><\/span><\/figcaption><\/figure>\n<p>The Earth got its Moon when a small planet collided with our planet more than four billion years ago. This impact hurled molten rock into space, which eventually coalesced to form the satellite we can see every night from across our planet.<\/p>\n<p>But what of our neighbour, Mars? The <a href=\"https:\/\/theconversation.com\/topics\/mars-178\">red planet<\/a> has two small, irregularly shaped moons called Phobos and Deimos. There are several theories on how these natural satellites formed, but no clear front-runner. Soon, a Japanese-led space mission called Martian Moons Exploration (MMX) will begin its hunt for the answer. <\/p>\n<p>On Monday October 19, MMX is due to lift off on an H3 rocket from Tanegashima Space Center in southern Japan. The mission will aim to land on Phobos and collect a sample of soil. The spacecraft will then send this precious payload to Earth, for study in laboratories.<\/p>\n<figure class=\"align-right zoomable\">\n            <a aria-label=\"Zoomable image\" href=\"https:\/\/images.theconversation.com\/files\/766413\/original\/file-20261015-50-reup31.jpg?ixlib=rb-4.1.1&amp;q=45&amp;auto=format&amp;w=1000&amp;fit=clip\"><img decoding=\"async\" alt=\"Asaph Hall\" src=\"https:\/\/images.theconversation.com\/files\/766413\/original\/file-20261015-50-reup31.jpg?ixlib=rb-4.1.1&amp;q=45&amp;auto=format&amp;w=237&amp;fit=clip\"><\/a><figcaption>\n              <span class=\"caption\">American astronomer Asaph Hall discovered Phobos and Deimos in 1887.<\/span><br \/>\n              <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/www.history.navy.mil\/content\/history\/nhhc\/our-collections\/photography\/numerical-list-of-images\/nhhc-series\/nh-series\/NH-49000\/nh-49228-commander-asaph-hall--usn-.html\">Naval History and Heritage Command<\/a><\/span><br \/>\n            <\/figcaption><\/figure>\n<p>Of the two Martian moons, Phobos is the largest and orbits closer to the planet. It has a mean diameter of 22.2km and a mass of 10,637 million million kg. Deimos has a mean diameter of 12.5km and a mass of 1,480 million million kg. <\/p>\n<p>The moons were discovered during a six-day window in 1877 <a href=\"https:\/\/www.universetoday.com\/articles\/finding-phobos-discovery-of-a-martian-moon\">by the American astronomer Asaph Hall<\/a>, who was working at the US Naval Observatory in Washington DC. <\/p>\n<p>Two main hypotheses dominate discussions of how Mars got these moons. The <a href=\"https:\/\/link.springer.com\/article\/10.1007\/s00159-011-0044-6\">giant impact theory proposes<\/a> that a celestial object a third of Mars\u2019 size hit the planet early in its history, ejecting material into space. <\/p>\n<p><a href=\"https:\/\/www.sciencedirect.com\/science\/article\/abs\/pii\/S0019103515000639\">The general mechanism<\/a> is similar to how scientists think Earth\u2019s natural satellite formed. But in the Martian impact theory, a single \u201cgiant\u201d moon was created by the ejected material, along with a host of smaller satellites.<\/p>\n<p>Over time, each one broke up and fell to Mars\u2019 surface. Simulations by Pascal Rosenblatt, from the Laboratoire de Plan\u00e9tologie et G\u00e9odynamique (LPG) in Nantes, France, and his colleagues <a href=\"https:\/\/www.nature.com\/articles\/ngeo2742\">show that<\/a> Phobos and Deimos would have been the sole moons to survive.<\/p>\n<h2>Gravitational capture<\/h2>\n<p>The <a href=\"https:\/\/www.science.org\/doi\/10.1126\/science.168.3933.828\">other main idea<\/a> is known as the captured asteroid theory, which <a href=\"https:\/\/academic.oup.com\/gji\/article\/15\/1-2\/205\/595919\">goes back to the 1960s<\/a>. This suggests that Phobos and Deimos were originally asteroids that wandered so close to Mars they were captured by the planet\u2019s gravity. <\/p>\n<p>According to this idea, the moons may have originated from within or just beyond the asteroid belt that lies between Mars and Jupiter. The moons might even have been what\u2019s known as a binary \u2013 two asteroids that orbit each other.<\/p>\n<p>The moons are characterised by their low density, which implies they have porous interiors.<\/p>\n<figure class=\"align-center zoomable\">\n            <a aria-label=\"Zoomable image\" href=\"https:\/\/images.theconversation.com\/files\/766480\/original\/file-20261015-50-czyqdj.jpg?ixlib=rb-4.1.1&amp;q=45&amp;auto=format&amp;w=1000&amp;fit=clip\"><img decoding=\"async\" alt=\"Deimos\" src=\"https:\/\/images.theconversation.com\/files\/766480\/original\/file-20261015-50-czyqdj.jpg?ixlib=rb-4.1.1&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\"><\/a><figcaption>\n              <span class=\"caption\">Deimos, the smaller of Mars\u2019 moons, orbits further from the planet than Phobos.<\/span><br \/>\n              <span class=\"attribution\"><a class=\"source\" href=\"https:\/\/science.nasa.gov\/mars\/moons\/deimos\/\">Nasa\/JPL-Caltech\/University of Arizona<\/a><\/span><br \/>\n            <\/figcaption><\/figure>\n<p>The captured asteroid hypothesis, however, requires an extremely dense Martian atmosphere to explain how the asteroids were trapped by tidal forces. Mars today has a thin atmosphere mainly composed of carbon dioxide. Also, asteroids captured by planets tend to have highly eccentric orbits. The orbits of Phobos and Deimos around Mars are, by contrast, almost circular.<\/p>\n<p>Scientists have also proposed other theories for the origins of these moons, but they command lower levels of support among the scientific community. One visualises the origin of these moons as debris from the destruction of a single \u201cproto-moon\u201d. <\/p>\n<p>Another lesser known idea proposes that Mars undergoes <a href=\"https:\/\/www.nature.com\/articles\/ngeo2916\">billion-year cycles<\/a> where rings of rocky material orbiting Mars coalesce over time into moons. <\/p>\n<p>Once the moons are formed, they are eventually ripped apart by gravitational (tidal) forces to form new rings. Under this scenario, we just happen to live in an era where the debris is in the form of moons and not as rings.<\/p>\n<h2>Solving the mystery<\/h2>\n<p>Amid this ongoing uncertainty surrounding the moons\u2019 origins, <a href=\"https:\/\/www.mmx.jaxa.jp\/en\/\">MMX aims to collect<\/a> more than 10g of material from Phobos \u2013 marking the world\u2019s first sample return mission from the Moon. <\/p>\n<p>If the samples contain a large amount of material from Mars itself, along with material from the asteroid that collided with the red planet, then it would favour the giant impact theory. If the composition of Phobos is similar to that of meteorites from known categories of asteroid, it would favour the asteroid capture theory.<\/p>\n<p>MMX\u2019s round trip to Mars will take five years in total. It will arrive at the red planet in late 2027, and return to Earth in 2031. <\/p>\n<p>The spacecraft consists of three modules, one to get to Mars, one to land on Phobos and another to return the sample to Earth. It houses 11 scientific instruments, including a gamma-ray and neutron spectrometer for measuring the chemical composition of Phobos, two cameras and a near-infrared instrument for characterising minerals. MMX will also deploy a 25kg rover called Idefix on Phobos\u2019 surface.<\/p>\n<p>For decades, the origin of Mars\u2019s unusual moons has been subject to intense debate. Now, with the launch of this landmark space mission, scientists could be on the verge of a breakthrough.<\/p>\n<p><img loading=\"lazy\" decoding=\"async\" src=\"https:\/\/counter.theconversation.com\/content\/294426\/count.gif\" alt=\"The Conversation\" width=\"1\" height=\"1\" \/><\/p>\n<p class=\"fine-print\"><em><span>Lana Williams does not work for, consult, own shares in or receive funding from any company or organisation that would benefit from this article, and has disclosed no relevant affiliations beyond their academic appointment.<\/span><\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Phobos is dominated by Stickney crater, a 9km (5.6 mile) bowl visible on the right. NASA\/JPL-Caltech\/University of Arizona The Earth got its Moon when a small planet collided with our planet more than four billion years ago. This impact hurled molten rock into space, which eventually coalesced to form the satellite we can see every [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[1],"tags":[],"class_list":["post-2031","post","type-post","status-publish","format-standard","hentry","category-uncategorized"],"_links":{"self":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/posts\/2031","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/comments?post=2031"}],"version-history":[{"count":0,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/posts\/2031\/revisions"}],"wp:attachment":[{"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/media?parent=2031"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/categories?post=2031"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/redzine.co.uk\/index.php\/wp-json\/wp\/v2\/tags?post=2031"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}