Universal Gravitation and Local G

AI Thread Summary
To find a person's weight on another planet, use the formula F = G(m1*m2)/r^2, where F is weight, G is the gravitational constant, m1 is the mass of the planet, m2 is the person's mass, and r is the radius of the planet. If a person weighs 1000 N on Earth, their weight on a planet with twice Earth's mass and the same radius can be calculated by recognizing that weight is directly proportional to the planet's mass. Doubling the mass of the planet while keeping the radius constant will also double the weight experienced by the person. Therefore, Max would weigh 2000 N on the new planet. Understanding this relationship allows for the calculation of weight on different celestial bodies.
physicalx
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K, so I don't quite understand how I find a persons weight on a different planet using the said person's weight, the mass of the other planet, and the radius of the planet?

So, for example:

Max weighs 1000 N on Earth. What would his weight be on a planet with twice the mass of Earth, but with the same radius?

How would I go about answering this and similar questions? Thanks for your help!
x
 
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physicalx said:
K, so I don't quite understand how I find a persons weight on a different planet using the said person's weight, the mass of the other planet, and the radius of the planet?

So, for example:

Max weighs 1000 N on Earth. What would his weight be on a planet with twice the mass of Earth, but with the same radius?

How would I go about answering this and similar questions? Thanks for your help!
x


Weight is a force, F:

F = G \frac{m_1 m_2}{r^2}

If you have a constant, known m1 and a constant r (like Earth) the equation can be simplified down to:

F = m_2 g

where:

g = \frac{G m_1}{r^2} (basically all the other values in the equation besides m2. m1 was the mass of Earth, so m2 is the so-called "test mass" (you or me, or a ball, for instance).

So look at the first equation. What happens to F when we double m?
 
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