{"id":73153,"date":"2026-07-31T05:30:00","date_gmt":"2026-07-31T05:30:00","guid":{"rendered":"https:\/\/gameblog.fr\/en\/?p=73153"},"modified":"2026-07-31T05:30:00","modified_gmt":"2026-07-31T05:30:00","slug":"bepicolombo-spacecraft-completes-its-cruise-stage-and-is-about-to-enter-mercurys-orbit","status":"publish","type":"post","link":"https:\/\/gameblog.fr\/en\/trends\/73153-bepicolombo-spacecraft-completes-its-cruise-stage-and-is-about-to-enter-mercurys-orbit\/","title":{"rendered":"BepiColombo spacecraft completes its cruise stage and is about to enter Mercury\u2019s orbit !"},"content":{"rendered":"<p>The BepiColombo mission is a joint effort by the European Space Agency (ESA) and the Japan Aerospace Exploration Agency (JAXA) to study Mercury. Named after the Italian mathematician Giuseppe Bepi Colombo, the mission aims to increase understanding of one of the solar system\u2019s least accessible planets.<\/p>\n<h2>Mission Setup and Partners<\/h2>\n<p>Launched on October 20, 2018, BepiColombo carries two main orbiters : the Mercury Planetary Orbiter (MPO) built by ESA and the Mercury Magnetospheric Orbiter (Mio) provided by JAXA. The spacecraft travel protected by the MOSIF shield (a heat-resistant protective shield) as they head toward Mercury.<\/p>\n<p>A wide group of countries contributed to the mission, including France, Germany, Italy, United Kingdom, Belgium, Spain, and Switzerland, explain <a href=\"https:\/\/sciencepost.fr\/la-sonde-bepicolombo-vient-de-terminer-sa-phase-de-croisiere-et-va-bientot-atteindre-lorbite-de-mercure\/\" rel=\"noopener noreferrer\" target=\"_blank\">Sciencepost<\/a>. French agencies like CNES and CNRS, plus several universities, also play a major role.<\/p>\n<p>The mission hit a key phase on July 10, 2026, when it switched into a controlled free-fall toward Mercury after traveling over 9 billion kilometers. That unpowered descent leads to orbit insertion in November 2026, followed by the separation of the two orbiters. Mio will take a high elliptical orbit at roughly 12,000 kilometers from Mercury\u2019s surface, while MPO will settle into a closer, circular orbit at about 1,500 kilometers. Scientific operations are scheduled to begin in April 2027.<\/p>\n<h2>What BepiColombo Wants To Learn<\/h2>\n<p>The mission has ambitious scientific aims. Mio will study Mercury\u2019s magnetic field and how the magnetosphere interacts with the solar wind. MPO will focus on surface mapping and geological work, probing Mercury\u2019s internal structure to shed light on its origin and evolution.<\/p>\n<p>Together, the instruments will study Mercury to improve understanding of rocky planets and provide data relevant to studies of exoplanets.<\/p>\n<p>Mercury has some unusual traits: it\u2019s the closest planet to the Sun and has a core that makes up about 85% of its radius. Despite the heat, there is water ice in some polar craters where sunlight never reaches.<\/p>\n<h2>Navigation Challenges and Engineering Solutions<\/h2>\n<p>Getting a spacecraft to Mercury is difficult. One major challenge is Mercury\u2019s gravity. To manage that, BepiColombo used gravity assists, two flybys of Venus and six of Mercury, to shape its path before the final approach. The energy needed to brake and slow down near Mercury is large ; the spacecraft must lose enough speed to be captured into orbit, so navigation and engineering have to be precise.<\/p>\n<p>Another major hurdle is the extreme temperature swing. Mercury\u2019s temperatures vary from -170\u00b0C to +430\u00b0C because of its thin exosphere and close solar exposure. The spacecraft must tolerate those swings, requiring advanced thermal engineering.<\/p>\n<p>BepiColombo builds on data from missions such as Mariner 10 and NASA\u2019s MESSENGER, which revealed Mercury\u2019s large metallic core and ice-filled craters. This mission aims to provide a deeper picture of Mercury\u2019s role in planetary formation.<\/p>\n<p>As BepiColombo collects data, it may change hypotheses about the solar system\u2019s history, including Mercury\u2019s thin mantle, past giant collisions, and conditions near the young Sun. Scientists will use the results to refine models of planetary formation and evolution.<\/p>\n","protected":false},"excerpt":{"rendered":"","protected":false},"author":2,"featured_media":73152,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_acf_changed":false,"footnotes":""},"categories":[116],"tags":[],"class_list":["post-73153","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-trends","generate-columns","tablet-grid-50","mobile-grid-100","grid-parent","grid-33"],"acf":[],"_links":{"self":[{"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/posts\/73153","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/comments?post=73153"}],"version-history":[{"count":1,"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/posts\/73153\/revisions"}],"predecessor-version":[{"id":73155,"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/posts\/73153\/revisions\/73155"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/media\/73152"}],"wp:attachment":[{"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/media?parent=73153"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/categories?post=73153"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/gameblog.fr\/en\/wp-json\/wp\/v2\/tags?post=73153"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}