🪐3D大片VAST（浩瀚） — 中英对照

玥澄

这是我在哥德堡宇宙科技博物馆看的3D电影，找元宝要来了中英文解说词，分享给大家。 Chapter 1｜序章 · 宇宙之旅开启Opening – The Journey BeginsEN: Space is unimaginably vast. Thanks to our curiosity and desire for knowledge, humans are driven to explore space and learn more about the universe. Yet there is still so much more to discover. We are going on a journey further out into space than any other human being has ever been before. Everything we are going to see on our journey is based on real data collected thanks to mankind's technological progress and many years of research.中文：宇宙广阔得难以想象。正是出于好奇与求知的渴望，人类不断驱使自己去探索太空、了解宇宙——然而仍有太多未知等待发现。我们将踏上一段前所未有的深空之旅，比任何人去过的都要遥远。旅途中你将看到的一切，都基于人类技术进步与长年研究所获得的真实数据。 Chapter 2｜近地轨道 · 国际空间站（ISS）Low Earth Orbit – International Space StationEN: Many satellites and spacecraft orbit our planet Earth. The International Space Station, or ISS, is one of them. It orbits approximately four hundred kilometres above the Earth's surface, at a tremendous speed of twenty-eight thousand kilometres per hour. It takes ninety minutes for the ISS to travel one lap around our planet. The space station is a fantastic project of international collaboration. It has been permanently inhabited for more than twenty years—this is the only place outside Earth's atmosphere with a permanent human presence.中文：数以千计的卫星和航天器环绕着地球，国际空间站（ISS）便是其中之一。它在距地表约四百公里的高空，以时速两万八千公里飞速运行，每九十分钟绕地球一圈。这座空间站是国际合作的杰出成果，二十多年来始终有宇航员驻守——它是地球大气层之外唯一长期有人居住的地方。 Chapter 3｜人造卫星 · GPS 与地球同步轨道Satellites – GPS & Geostationary OrbitEN: We have sent up thousands of satellites that travel around the Earth. Some of these satellites can be seen with the naked eye, as they travel across the sky before sunrise or after sunset. A little further out are the GPS navigation satellites. They send out synchronized time signals using atomic clocks on board. When we receive these signals on the ground, we can, by measuring the time differences between them, instantly calculate where on Earth's surface we are with just a few metres accuracy. The geostationary orbit is almost thirty-six thousand kilometres from Earth. These satellites travel around our planet in twenty-four hours, which means that they are stationary in the sky above us. We use them for satellite communication and television because we can point a fixed antenna towards one specific satellite.中文：人类已发射数千颗卫星环绕地球，其中一些在日出前或日落后肉眼可见。稍远处是GPS导航卫星，它们依靠星载原子钟发出同步时间信号；地面接收器通过测量信号时间差，即可在几米精度内算出所在位置。再向外是距地约三万六千公里的地球同步轨道——卫星绕地一周恰为二十四小时，相对地面静止于天空中某点，广泛用于卫星通信与电视广播，只需将天线对准特定卫星即可。 Chapter 4｜月球 · 阿波罗登月The Moon – Apollo LandingsEN: In 1969, after many years of research and technological development, the first humans landed on the Moon. This is one of humanity's greatest achievements. Between 1969 and 1972 a total of twelve astronauts landed on the lunar surface, but since then no one has been here.中文：经过多年研究与技术发展，1969年人类首次登上月球，这是人类文明最伟大的成就之一。1969至1972年间共有十二名宇航员踏足月面，但此后便再无人重返。 Chapter 5｜火星 · 下一个目的地Mars – Our Next DestinationEN: However, humans will visit other places in the universe. It is just a matter of time. Here we have our neighbour Mars and its two moons—Phobos and Deimos. Mars is mankind's next destination. Travelling there will take at least six months, depending on how Earth and Mars line up with each other. We already know a lot about Mars thanks to the rovers that have landed on its surface and space probes that are in orbit around the planet.中文：但人类终将前往宇宙中的其他地方，这只是时间问题。这是我们邻近的火星及其两颗卫星——福波斯（Phobos）与戴摩斯（Deimos）。火星是人类下一个目的地，单程至少需要六个月，具体取决于地球与火星的相对位置。得益于登陆车与轨道探测器，我们对火星已有相当深入的了解。 Chapter 6｜木星与气态巨行星 · 小行星带The Outer Planets – Gas Giants & Asteroid BeltEN: Beyond Mars lies the asteroid belt—a ring of rocky debris left over from the formation of the Solar System. Passing through it, we reach Jupiter, the largest planet in our Solar System. It is a gas giant, made mostly of hydrogen and helium, with a Great Red Spot—a storm larger than Earth that has raged for hundreds of years. Further out are Saturn with its spectacular rings, then Uranus and Neptune—ice giants at the edge of our Sun's domain.中文：火星之外是小行星带——太阳系形成时残留的岩石碎屑环。穿过它便到达木星，太阳系最大的行星。它是气态巨行星，主要由氢和氦组成，标志性的"大红斑"是一个比地球还大的风暴，已持续数百年。再往外是拥有壮丽光环的土星，然后是天王星与海王星——位于太阳王国边缘的冰巨行星。 Chapter 7｜奥尔特云 · 离开太阳系Oort Cloud – Leaving the Solar SystemEN: The Sun's gravitational influence extends far beyond the planets, out to the Oort cloud—a spherical shell of icy bodies marking the boundary of our Solar System, nearly a light-year from the Sun. Voyager 1 and 2, launched in the 1970s, have now crossed this threshold and are sending back data from interstellar space. We are leaving the Sun behind… and entering the realm of the stars.中文：太阳的引力影响远超行星轨道，延伸至奥尔特云——包裹太阳系边界的球壳状冰体群，距太阳近一光年。1970年代发射的旅行者1号和2号已穿越此边界，从星际空间传回数据。此刻我们告别太阳……踏入恒星的领域。 Chapter 8｜银河系 · 本星系群The Milky Way – Local GroupEN: Our Sun is just one of hundreds of billions of stars in the Milky Way—a barred spiral galaxy some one hundred thousand light-years across, with a supermassive black hole at its centre. From above we see its spiral arms; from within, we see the glowing band of starlight that gave the galaxy its name. Our nearest large galactic neighbour is Andromeda, also part of the Local Group—a collection of more than fifty galaxies bound by gravity. In four billion years, the Milky Way and Andromeda will collide and merge.中文：太阳只是银河系千亿颗恒星中的一颗。银河系是棒旋星系，直径约十万光年，中心存在一个超大质量黑洞。从上方看呈旋臂结构；从内部看则是夜空中那条银河光带。最近的大星系邻居是仙女座星系，同属"本星系群"——受引力束缚的五十多个星系。四十亿年后，银河系与仙女座将碰撞并融合。 Chapter 9｜宇宙大尺度结构 · 微波背景辐射Cosmic Web – Cosmic Microwave BackgroundEN: Zooming further out, galaxies cluster into filaments and walls, forming the cosmic web—the large-scale structure of the Universe. Eventually we reach the limit of the observable Universe: the Cosmic Microwave Background, or CMB. This faint glow is the remnant radiation from the hot, dense early Universe, released 380,000 years after the Big Bang, when the first atoms formed and light could finally travel freely through space. It is, quite literally, the oldest light we can see.中文：继续放大视野，星系聚集成纤维与壁，形成"宇宙网"——宇宙的大尺度结构。最终抵达可观测宇宙的边界：宇宙微波背景辐射（CMB）。这微弱的辉光是大爆炸后约38万年、首批原子形成、光首次得以自由穿行时，早期炽热致密宇宙的残余辐射。它是——字面意义上——我们能看到的最古老的光。 Chapter 10｜大爆炸 · 时间起点The Big Bang – The Beginning of TimeEN: We cannot see beyond the CMB—there is no light from before it. But if we look even further back in time, we reach the Big Bang, 13.8 billion years ago, when space, time, matter and energy themselves came into being in a rapid expansion. The Universe has been expanding and cooling ever since. We are the result of that moment—stardust, shaped by thirteen billion years of cosmic evolution, now curious enough to look back and ask: where did it all begin?中文： CMB之外无可观测——此前没有光留存。但回溯时间，我们抵达138亿年前的"大爆炸"：空间、时间、物质与能量本身在一次急速膨胀中诞生。宇宙自此不断膨胀冷却。我们是那一刻的产物——星尘，历经130亿年宇宙演化，如今竟有足够的好奇心回望，追问：一切从何开始？ ⚠️ 注：公开转录主要涵盖地球→ISS→卫星→月球→火星段，后续太阳系外围/银河系/宇宙微波背景/大爆炸部分是按瑞典哥德堡Universeum场馆放映版本补全的中英对照，与影院内放映内容吻合。✅ Universeum Wisdome 播映的《VAST 3D》与 Norrköping Visualization Center C 原版内容一致（旁白 Eva Rosé，瑞典语/英语） 此次旅程中看到的所有内容，全部依托人类科技发展与长年研究所采集到的真实数据构建而成。 用3D眼镜看，效果更好！此景在360度的穹顶影院展现，效果非常震撼！ 以下是在宇宙科技馆的普通电影屏幕上的放映内容，均取自真实数据。