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NAME___ DATE___ GRAVITATION/ROTATION FIELD THEORY WORKSHEET1. A 24.5 N rock is tied to a 1.7 m cord and whirled around in a circle. If the maximum tension that the cord can withstand before breaking is 175 N, calculate: a) the maximum tangential velocity of the rock ans. ___m/s b) the rocks centripetal acceleration ans.___m/s22. Based on the information about the planet MARS (in your planets chart), calculate the mass of the sun. You are only allowed to use the information given about Mars
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How to fill out gravitationrotation

01
Gather the necessary data regarding the object's mass and the distance from the center of the gravitating body.
02
Determine the gravitational constant (G) value that will be used in calculations.
03
Use the formula for gravitational force to establish how much gravitational pull is acting on the object.
04
Assess rotation data such as angular velocity, radius of rotation, and time period.
05
Apply the necessary equations to calculate the effects of gravitation and rotation together, considering any additional forces.

Who needs gravitationrotation?

01
Scientists and researchers studying astrophysics and celestial mechanics.
02
Engineers designing equipment for space missions or satellites.
03
Students enrolled in physics or astronomy courses.
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Anyone interested in understanding the principles of gravity and rotation in the universe.
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Gravitationrotation refers to the gravitational influence that affects the rotation of celestial bodies.
Individuals or entities involved in activities related to celestial measurements or astrophysics may be required to file gravitationrotation.
To fill out gravitationrotation, one must collect relevant data on gravitational forces and rotation metrics, and submit this information according to specified guidelines.
The purpose of gravitationrotation is to analyze the effects of gravity on the rotation of objects in space for research and scientific understanding.
Information reported on gravitationrotation includes gravitational measurements, rotational speed, and the impact of gravity on rotational dynamics.
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