If the earth rotates around the sun at the speed of 108,000 km an hour, why does the air in earth's atmosphere not disperse and become lost to the vast vacuum that is space?
The Earth and its atmosphere are in orbit together around the sun, so there is no differential force pulling the atmosphere away.
An orbit is considered to be free fall toward a larger mass, where the transverse velocity of the smaller mass is enough to keep the two from colliding. Newton showed that the acceleration of the smaller body was only dependent on the mass of the larger.
In other words, the Earth and its atmosphere are both accelerating toward the sun at the same rate. Since there is no difference in acceleration caused by the sun, the Earth's gravity is enough to dominate the atmosphere. The sun's solar wind, however, would be able to strip away the Earth's atmosphere if we did not have a strong magnetosphere to protect us. Astronomers believe that this is what happened to Mars's atmosphere.
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Because gravity opposes the outward centrifugal force brought about by Earth's rotation, Earth's gravity holds onto its atmosphere and keeps it from dispersing into space.
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When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
When evaluating a one-sided limit, you need to be careful when a quantity is approaching zero since its sign is different depending on which way it is approaching zero from. Let us look at some examples.
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