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Satellites for Internet Communication

机译:互联网通讯卫星

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摘要

Orbiting satellites were first considered centuries ago in a famous problem solved by Sir Isaac Newton himself. He first posed the artificial Earth-orbiting satellite scenario in Mathematical Principals of Natural Philosophy published in 1687. He imagined that a cannon could shoot a projectile to circumnavigate the globe and envisioned that at a sufficiently high radial velocity, the projectile would have a higher radial velocity than falling velocity and hence would always miss the Earth, staying on a circular path about the Earth. At low orbit the projectile's velocity must be greater than that of the rotating Earth's radial velocity. But as the projectile goes into a higher orbit, the velocity necessary to stay in orbit decreases, until at 22,300 miles above the Earth's surface, the velocity of the projectile matches exactly that of Earth. In this orbit we have geo-sta-tionary orbit, that is, the satellite remains above a fixed point on the Earth.
机译:艾萨克·牛顿爵士本人解决了一个著名的问题,几个世纪前就首先考虑了轨道卫星。他首先在1687年发表的《自然哲学的数学原理》中提出了人造地球轨道卫星情景。他设想大炮可以射击弹丸以绕地球旋转,并设想在足够高的径向速度下,弹丸的径向半径会更高。速度比下降速度高,因此总是会错过地球,停留在围绕地球的圆形路径上。在低轨道,弹丸的速度必须大于旋转地球的径向速度。但是,随着射弹进入更高的轨道,停留在轨道上所需的速度会降低,直到到达地球表面上方22,300英里时,射弹的速度才与地球的速度完全匹配。在这个轨道上,我们有地球静止轨道,也就是说,卫星保持在地球固定点上方。

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