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去年 8 月,火星耶泽罗陨石坑边缘,毅力号火星车的相机捕捉到一个略带阴影的天体掠过太阳盘面——火星卫星火卫一正在发生凌日。这颗以希腊恐惧之神命名的卫星,在一分钟内横穿太阳,却因体积太小而无法让火星天空真正变暗。这颗直径仅二十余公里的小卫星,其起源至今仍是太阳系最大的未解之谜之一。而 10 月 20 日,日本宇宙航空研究开发机构(JAXA)的火星卫星探测任务(MMX)搭乘 H3 火箭从种子岛航天中心升空,将首次尝试登陆火卫一表面并采样返回地球。
“土豆”卫星:太阳系起源的关键线索
火卫一与另一颗卫星火卫二均以古希腊神话中的恐惧与 terror 之神命名,它们的宇宙起源至今没有定论。目前存在两种主流假说:其一是这两颗卫星原本是火星与木星之间小行星带的成员,被火星引力捕获;其二是远古时期一个大型天体撞击火星,将碎片抛入轨道,火卫一和火卫二由此凝聚而成。部分模型显示,它们可能是一个卫星群中仅存的幸存者。
从科学角度看,火卫一是一个典型的“碎石堆”——由岩石和尘埃松散聚合而成。由于其质量太小,无法在自身引力下形成球体,呈现出土豆般的不规则形状,长约 27 公里,表面重力仅为地球的 1/1800。这意味着一个成年人在火卫一上的体重,相当于地球上的一颗网球。火卫一表面最引人注目的地貌是直径约 9 公里的 Stickney 大陨石坑,几乎占据了其整个表面视野。分析火卫一的物质成分,有望区分上述两种起源假说,进而揭示火星乃至内太阳系早期的演化历史。
【关键数据】
- 发射时间: 2026 年 10 月 20 日,H3 火箭,种子岛航天中心
- 到达火星: 2027 年(后续进入火卫一环绕轨道)
- 火卫一尺寸: 长约 27 公里,重力为地球的 1/1800
- 采样规模: 约 10 克火卫一表面样本
- 样本返回: 2031 年下半年抵达地球

微重力着陆:“就像把气球放到地面”
在重力近乎为零的松散天体上着陆,是 MMX 任务面临的最棘手工程难题。JAXA 的 MMX 项目经理川胜康弘打了一个形象的比方:“我常说,在火卫一上着陆就像试图降落一只气球——让气球平稳落地并保持不倾斜、不弹跳,非常困难。”微重力环境下,探测器的任何微小推力都可能使其反弹甚至逃逸,因此着陆策略必须极度精细。此外,工程师还需要设计环绕一颗“绕大行星运行的小卫星”的特殊轨道,应对火星周期性遮挡地火通信链路的窗口限制,并解决巡视器如何在松散表面行走、如何钻取样本等技术问题。
MMX 采用了三模块设计:推进模块负责深空巡航和火星轨道切入制动;探测模块搭载巡视器、采样装置及科学载荷;返回模块则携带再入舱,完成样本的地球之旅。任务搭载了包括 NASA 在内的多个航天机构的科学载荷,法德航天机构(CNES 与 DLR)与 JAXA 联合研制了名为“Idefix”的小型巡视器。法国国家科学研究中心研究主任、Idefix 联合首席科学家 Patrick Michel直言:“这是我所见过的最复杂的任务。”采样完成后,探测模块与返回模块将一同从火卫一表面起飞,随后探测模块被抛弃,返回模块独自踏上归途。
深空博弈:采样返回的技术竞赛
从飞行剖面看,MMX 进入地球低轨道后,推进模块点火开启近一年的深空巡航;抵达火星时,飞船需要进行一次长时间的精确制动点火,才能被火星引力捕获,否则将飞掠火星被甩入太阳系深处。意大利都灵理工大学航天动力学专家 Nicola Baresi 参与的轨道设计团队,需要解决火卫一引力场不规则、火星潮汐摄动叠加等复杂问题。若一切按计划推进,MMX 将于 2031 年下半年把约 10 克火卫一样本送回地球,这将是人类首次从火星卫星系统取回样本,其科学价值可能不亚于从火星本体采样——火卫一表面可能保存着火星被撞击溅射出的古老物质。
从全球深空探测格局看,MMX 是 JAXA 继隼鸟号、隼鸟2号小行星采样返回之后的又一次技术跃升,也是 H3 火箭承担的关键任务之一。对于持续加码月球与火星采样返回的中国航天以及推进火星样本返回的 NASA 而言,MMX 的微重力着陆与取样技术路线同样具有参考意义。未来五年,这颗“土豆卫星”能否吐露太阳系早期的秘密,答案将随 2031 年那个高速再入地球大气层的小小返回舱一同揭晓。
出处:How Do You Land on a Moon With Almost No Gravity?
英文原文Last August, looking up from the edge of an ancient river delta on Mars, the Perseverance rover ’s electronic eye spied an oblong shadow crossing the distant, glowing Sun. Phobos , the Martian moon named for the Greek god of fear and panic, was transiting the solar disk. Too small to darken the pale, dust-tinged sky, but orbiting close enough to eclipse a significant fraction of the Sun, Phobos passed in less than a minute. NASA’s Perseverance rover captured Phobos passing in front of the Sun from the surface of Mars. ASU/MSSS/SSI/JPL-Caltech/NASA The tiny moon, with its murky origins, is an enigma, and one whose makeup and history could tell us much about Mars and the wider solar system. And now the international Martian Moons eXploration (MMX) mission, which successfully launched on 20 October , seeks to explore that mystery with an unprecedented series of landings on the unknown surface of Phobos. This mission brings unusual challenges—for example, designing an orbit to study a microgravity moon orbiting a much larger planet. Engineers also had to figure out how to assess and land on this low-gravity pile of loosely assembled dirt and rock, how a rover might rove across it, and how the spacecraft might take samples and return them to Earth. “I often say that landing on Phobos is like trying to land a balloon,” says Yasuhiro Kawakatsu , project manager of MMX at the Japan Aerospace Exploration Agency (JAXA). “It’s very difficult to drop a balloon to the ground and prevent it from tilting or bouncing.” Why Phobos Is Such a Strange Moon Phobos is one of two small Martian moons; the other is Deimos , named after the Greek god of dread and terror. Their cosmic origins are unknown, though there are two prevailing theories. One holds that the moons were once asteroids from the belt between Mars and Jupiter, captured by the smaller planet’s gravity. In the other theory, Phobos and Deimos formed when a large celestial body slammed into Mars, sending debris into orbit. Some models suggest the pair are the last survivors from a cluster of satellites. The enormous Stickney crater, roughly 9 kilometers across, dominates this view of Phobos taken by NASA’s Mars Reconnaissance Orbiter. University of Arizona/JPL-Caltech/NASA Scientifically speaking, Phobos is considered a rubble pile, a loosely consolidated aggregate of rock and dust. Far too small to become spherical under its own mass, it’s shaped like a lumpy potato, roughly 27 kilometers in length, with only 1/1,800 th of Earth’s gravity. On Phobos, a typical adult would weigh about as much as a tennis ball does on Earth. More than 10 years in the making, MMX launched on Japan’s flagship H3 rocket from Tanegashima spaceport on 20 October local time. It will arrive at Mars in 2027 carrying scientific payloads from several space agencies, including NASA, and a new rover called Idefix developed by the French and German space agencies (CNES and DLR) in collaboration with JAXA. Engineers assembled MMX’s modules at Japan’s Tanegashima Space Center before the spacecraft’s October 2026 launch. JAXA MMX consists of three modules: a propulsion module to power its journey to Mars and apply the brakes to enter orbit around the red planet; an exploration module carrying the rover, sampling gear, and other scientific instruments; and a return module, attached to the exploration module, that harbors the capsule destined for a high-speed reentry into Earth’s atmosphere. After collecting samples on Phobos, the exploration and return modules will lift off together. The exploration module will then be jettisoned while the return module sets a course back home. If all goes according to plan, MMX will deliver a 10-gram sample to Earth in the second half of 2031. But the mission will face a series of daunting challenges to reach that end point, including navigating complex orbits around Phobos and landing on its surface while Mars periodically blocks communications with Earth. The MMX’s modular design includes the propulsion module [left] and the exploration and return modules [right]. Kyodo News/Getty Images “It’s the most complex mission I have ever seen,” says Patrick Michel , director of research at CNRS (the French National Center for Scientific Research) and co-principal investigator on Idefix. How MMX Will Orbit Phobos An H3 rocket carried MMX into space on 20 October 2026, beginning the mission’s five-year journey to Phobos and back. The Asahi Shimbun/Getty Images Once MMX reached low Earth orbit, its propulsion module’s engine fired, kicking off a nearly year-long deep-space cruise to Mars. On arrival, the spacecraft will need to fire its engines in an extended, carefully timed burn to slow down enough to be captured by Mars gravity. The propulsion module will then be jettisoned, leaving the exploration and return modules to orbit Mars. “If something doesn’t go according to plan, MMX will fly by Mars and get catapulted into the solar system,” says Nicola Baresi , an astrodynamic