How Do You Calculate the Force Earth Exerts Tangentially?

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To calculate the force Earth exerts regarding its tangential motion, one must first determine the orbital velocity vector, which is perpendicular to the radius vector from the Sun. The gravitational force acting on Earth can be expressed using the equation GMm/r^2, which equals the centripetal force mv^2/r. By calculating the orbital velocity from this relationship, one can identify the force needed to counteract Earth's motion. To bring Earth to a halt, the work required can be calculated using the work-energy principle. Understanding these dynamics is crucial for any analysis involving forces in orbital mechanics.
kepler
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Hi,

If at a particular time, I have the r distance from the Sun to Earth, the value of the velocity of Earth, and the angle between the velocity vector and the r vector, how can I calculate the force that Earth has regarding the tangent? Suppose I wanted to go againts the movement of the Earth. Which force should I go against and how do I calculate it?

Kind regards,

Kepler
 
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In a direction tangential to its orbit , Earth has an obital velocity vector prependicular to the vector 'r' . This velocity vector can be calculated easily.

Considering the system to be considering only of Sun and Earth , therefore , Sun's gravitational pull provides the necessary centripedal force :

<br /> <br /> \frac {GMm}{r^2} = \frac {mv^2}{r}<br />

Calculate the velocity from here . This the velocity you have to counteract by going against the motion of earth. To bring Earth to rest , you can calculate the work needed by the work-energy principle.

BJ
 
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