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Cosmology - Facts and speculation

机译:宇宙学-事实与推测

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Among scientists (specially physicists), there has been a discussion for a long time about how much of a science is cosmology. The difficulty earlier (before 1920s) was the absence of any observations and the stronghold of mythology. Even broad observed features were highly ambiguous. Only in the twentieth century was it realized that what were thought of as nebulae were really distant galaxies. In 1927, Hubble observed faraway galaxies and their velocities and formulated Hubble's law which says, 'The farther a galaxy is, the faster it is running away from us'. This gave rise to the model of the expanding universe now known as the 'Big Bang'. Almost forty years later, in 1965, the cosmic microwave background radiation (CMBR) was discovered accidentally. The non-uniformity or anisotropy of CMBR was discovered only in 1992. It is only in the last two
机译:在科学家(特别是物理学家)中,关于科学的多少是宇宙学已有很长时间的讨论。较早(1920年代之前)的困难是缺乏任何观察和神话据点。甚至观察到的广泛特征也非常模棱两可。直到二十世纪才意识到,被认为是星云的确实是遥远的星系。 1927年,哈勃观察到遥远的星系及其速度,并制定了哈勃定律,该定律说:“星系越远,它逃离我们的速度就越快”。这产生了现在称为“大爆炸”的宇宙膨胀模型。大约四十年后的1965年,偶然发现了宇宙微波背景辐射(CMBR)。 CMBR的非均匀性或各向异性仅在1992年被发现。仅在最近两个

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