What force acts on the earth perpendicular to the force of the sun which causes the tangential accelerations characteristic of an ellipse?
There is no such force.
The elliptical orbit that we observe is actually a projection of the four-dimensional geodesic onto our familiar three-dimensional space. According to Einstein's General Theory of Relativity, the mass of the Sun bends the fabric of four-dimensional spacetime, and the Earth is actually traveling along a geodesic—an extension of a straight line in four dimensions—instead of gravitational force or centripetal force.
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The centripetal force is the force that acts on Earth perpendicular to the force of the Sun, resulting in the tangential accelerations that define an ellipse.
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The force acting on the Earth perpendicular to the force of the Sun, which causes the tangential accelerations characteristic of an ellipse, is known as the centripetal force.
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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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