The relationship between distance from the Sun and the period of rotation is described by Kepler's Third Law, which states that the square of a planet's orbital period is proportional to the cube of its average distance from the Sun. As for eccentricity, there isn't a direct relationship with distance; eccentricity measures the shape of an orbit, which can vary among planets at similar distances from the Sun. However, generally, planets further from the Sun tend to have more circular orbits, resulting in lower eccentricities.
eccentricity = distance between foci ________________ length of major axis
Due to the vast distance between the earth and polaris, the earths axis of rotation essentially lines up with polaris at all times, so when the stars are visible, and viewed from the north pole, the earths rotation causes the stars to appear to rotate around polaris.
Measure the distance between the two points (start and end) then multiply by the scale of the map. For example - suppose the distance from town A to town B is 12cm and the scale is 1:25000 - then the actual distance between the two towns is 3km !
What is the relationship between Amelia Earhart and G.P. Putnam
The SCALE of the map indicates the relationship between lengths measured on a map and the actual distances. It can indicate the ratio of distances (e.g. 1:10000) or the equivalent actual distance for an inch or centimeter as measured on the map, often providing a measurement bar for various distances.
As the distance between foci increases the eccentricity increases, or the reverse relationship.
eccentricity = distance between foci ________________ length of major axis
the eccentricity will increase.
When the distance between the foci of an ellipse increases, the eccentricity of the ellipse also increases. Eccentricity is a measure of how much an ellipse deviates from being circular, calculated as the ratio of the distance between the foci to the length of the major axis. As the foci move further apart, the ellipse becomes more elongated, leading to a higher eccentricity value. Therefore, an increase in the distance between the foci results in a more eccentric ellipse.
The eccentricity of that ellipse is 0.4 .
There is no real relationship, a planets spin depends on collisions it may have had in the past, rather than on its distance from the sun (which governs its orbital rotation time around the sun).
tangential speed is directly proportional to rotational speed at nay fixed distance from the axis of rotation
-- the eccentricity or -- the distance between the foci or -- the ratio of the major and minor axes
The relationship between torque, force, and distance is expressed by the equation torque equals force times distance. This means that the torque applied to an object is directly proportional to both the force applied and the distance from the point of rotation. In other words, the greater the force applied and the longer the distance from the point of rotation, the greater the torque produced.
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