2. Earth is rotating about the Sun in our solar system. The distance between the Earth and Sun is 1.5 x 10"m. Consider the impact of an asteroid of mass 8.9 x1015 kg and a speed of 90,000 km/h with respect to the Earth's surface. The asteroid strikes the Earth at the equator as shown in Figure. Consider the mass and radius of the Earth are ME = 5.97 x 1024 kg and RE = 6.38 x10° m, respectively. Assume that the axial and orbital axis of rotations are parallel to each other. Earth North Pole

College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
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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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(d) How much energy is needed to stop the Earth’s rotation about its axis after the collision?  

(e) What would be the moment of inertia of the Earth if the axis of rotation is parallelly shifted so that it touches the equator?  

2. Earth is rotating about the Sun in our solar system. The distance between the Earth and Sun
is 1.5 x 10'm. Consider the impact of an asteroid of mass 8.9 x1015 kg and a speed of 90,000
km/h with respect to the Earth's surface. The asteroid strikes the Earth at the equator as shown
in Figure. Consider the mass and radius of the Earth are ME = 5.97 x 1024 kg and RE = 6.38
x10° m, respectively. Assume that the axial and orbital axis of rotations are parallel to each
other.
Earth
North Pole
Transcribed Image Text:2. Earth is rotating about the Sun in our solar system. The distance between the Earth and Sun is 1.5 x 10'm. Consider the impact of an asteroid of mass 8.9 x1015 kg and a speed of 90,000 km/h with respect to the Earth's surface. The asteroid strikes the Earth at the equator as shown in Figure. Consider the mass and radius of the Earth are ME = 5.97 x 1024 kg and RE = 6.38 x10° m, respectively. Assume that the axial and orbital axis of rotations are parallel to each other. Earth North Pole
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