The planet Venus orbits the Sun in periodic motion (as yearly motion) and simultaneously spins about its axis (as diurnal motion). Venus has a (yearly) period of orbit of 225 days and a (diurnal) period of rotation of 243 days. So for Venus inhabitants, a day would last longer than a year! Determine the frequency of orbit and the frequency of rotation (in Hertz) on Venus. For yearly motion → 5.1 x 108 Hz, For diurnal motion → 4.8 x 108 Hz, O For yearly motion → 1.7 x 108 Hz, For diurnal motion 1.8 x 108 Hz, For yearly motion → 2.5 x 106 Hz, For diurnal motion → 1.8 x 107HZ, For yearly motion → 4.3 x 107 Hz, For diurnal motion → 48.0 x 107 Hz,

The planet Venus orbits the Sun in periodic motion (as yearly motion) and simultaneously spins about its axis (as diurnal motion). Venus has a (yearly) period of orbit of 225 days and a (diurnal) period of rotation of 243 days. So for Venus inhabitants, a day would last longer than a year! Determine the frequency of orbit and the frequency of rotation (in Hertz) on Venus. For yearly motion → 5.1 x 108 Hz, For diurnal motion → 4.8 x 108 Hz, O For yearly motion → 1.7 x 108 Hz, For diurnal motion 1.8 x 108 Hz, For yearly motion → 2.5 x 106 Hz, For diurnal motion → 1.8 x 107HZ, For yearly motion → 4.3 x 107 Hz, For diurnal motion → 48.0 x 107 Hz,

College Physics

11th Edition

ISBN:9781305952300

Author:Raymond A. Serway, Chris Vuille

Publisher:Raymond A. Serway, Chris Vuille

Chapter1: Units, Trigonometry. And Vectors

Section: Chapter Questions

Problem 1CQ: Estimate the order of magnitude of the length, in meters, of each of the following; (a) a mouse, (b)...

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Concept explainers

Proper Length

The theory of special relativity explains the connection between space and time to objects that move in a straight line at a constant speed. The objects move at the speed of light. When an object approaches light speed, its mass is endless and cannot move faster than light. The most crucial postulate of Einstein's special relativity is that the laws of nature do not change in each frame of reference.

Question

The planet Venus orbits the Sun in periodic motion (as yearly motion) and simultaneously spins
about its axis (as diurnal motion). Venus has a (yearly) period of orbit of 225 days and a (diurnal)
period of rotation of 243 days. So for Venus inhabitants, a day would last longer than a year!
Determine the frequency of orbit and the frequency of rotation (in Hertz) on Venus.
O For yearly motion 5.1 x 108 Hz,
For diurnal motion
— 4.8 х 108 Hz,
O For yearly motion
+ 1.7 x 108 Hz,
For diurnal motion 1.8 x 10-8 Hz,
O For yearly motion → 2.5 x 106 Hz,
For diurnal motion
+ 1.8 х 107Hz,
O For yearly motion
→ 4.3 x 107 Hz,
For diurnal motion
→ 48.0 x 10-7 Hz,

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