(Please include diagram or drawing) Two clay meteors, each with a mass m, collide in outer space and stick together. This collision occurs at a distance D from the center of the Earth. Following the collision, the combined meteors move towards the Earth. Before the collision: Meteor 1 has a velocity v1. Meteor 2 has a velocity v2. The velocities V1 and v2 are at right angles to each other.           a) Calculate the fraction of kinetic energy lost during the collision of the two meteors. b)  Determine the velocity of the stuck-together meteors just before they crash into the Earth assuming you know the mass and radius of earth. Air resistance can be neglected.

The Solar System
9th Edition
ISBN:9781305804562
Author:Seeds
Publisher:Seeds
Chapter10: Origin Of The Solar System And Extrasolar Planets
Section: Chapter Questions
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(Please include diagram or drawing) Two clay meteors, each with a mass m, collide in outer space and stick together.

This collision occurs at a distance D from the center of the Earth. Following the collision, the combined meteors move towards the Earth. Before the collision:

Meteor 1 has a velocity v1. Meteor 2 has a velocity v2. The velocities V1 and v2 are at right angles to each other.          

a) Calculate the fraction of kinetic energy lost during the collision of the two meteors.

b)  Determine the velocity of the stuck-together meteors just before they crash into the Earth assuming you know the mass and radius of earth. Air resistance can be neglected.

V₂
M
* Earth not included
Transcribed Image Text:V₂ M * Earth not included
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