General Science

所在平台: Udemy

课程主页: https://www.udemy.com/course/general-science/

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**课程名称:** 通识科学 **课程概述:** 本课程将带领学习者深入了解我们赖以生存的家园——地球。地球是太阳系中一颗独一无二的行星,我们目前所知唯一拥有生命的星球。尽管在太阳系中,地球并非最大的行星,但它是唯一一颗表面存在液态水的行星。地球的体积与近邻金星相近,是距离太阳最近的四颗岩石行星中最大的一颗。 课程将追溯地球的起源,探讨其在大约45亿年前,作为太阳形成过程中遗留下来的尘埃和气体云凝聚而成的过程。我们将了解地球早期内部的演化,包括放射性元素衰变释放的热量如何逐渐导致其内部熔化,铁元素下沉形成地核,以及早期地表发生的剧烈地质活动,如火山爆发和熔岩流。 课程还将解释地球如何逐渐冷却,形成坚实的岩石层(地壳),以及火山活动和地壳裂缝如何释放出内部的水蒸气,最终在凹陷的地表汇聚形成海洋,塑造了我们今天所见的地球面貌。

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Our home planet is the third planet from the Sun, and the only place we know of so far that's inhabited by living things.While Earth is only the fifth largest planet in the solar system, it is the only world in our solar system with liquid water on the surface. Just slightly larger than nearby Venus, Earth is the biggest of the four planets closest to the Sun, all of which are made of rock and metal. The name Earth is at least 1,000 years old. All of the planets, except for Earth, were named after Greek and Roman gods and goddesses. However, the name Earth is a Germanic word, which simply means "the ground."Earth, along with the other planets, is believed to have been born 4.5 billion years ago as a solidified cloud of dust and gases left over from the creation of the Sun. For perhaps 500 million years, the interior of Earth stayed solid and relatively cool, perhaps 2,000F. The main ingredients, according to the best available evidence, were iron and silicates, with small amounts of other elements, some of them radioactive. As millions of years passed, energy released by radioactive decay?mostly of uranium, thorium, and potassium?gradually heated Earth, melting some of its constituents. The iron melted before the silicates, and, being heavier, sank toward the center. This forced up the silicates that it found there. After many years, the iron reached the center, almost 4,000 mi deep, and began to accumulate. No eyes were around at that time to view the turmoil that must have taken place on the face of Earth?gigantic heaves and bubblings on the surface, exploding volcanoes, and flowing lava covering everything in sight. Finally, the iron in the center accumulated as the core. Around it, a thin but fairly stable crust of solid rock formed as Earth cooled. Depressions in the crust were natural basins in which water, rising from the interior of the planet through volcanoes and fissures, collected to form the oceans. Slowly, Earth acquired its present appearance.

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