How Do You Calculate Acceleration and Distance of a Free-Falling Object?

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The acceleration of a free-falling object remains constant at 10 m/s², meaning its velocity increases linearly: 10 m/s after one second, 20 m/s after two seconds, and 30 m/s after three seconds. The distance traveled in the third second is not 10,000 m; rather, it is calculated using the formula for distance under constant acceleration. To determine gravitational acceleration at 100 km above Earth, the formula g = (G*m1*m2) / r² is used, where r is the distance from Earth's center. An alternative method involves using g at sea level adjusted for altitude with the relation g at h = g at sea level * (r Earth / (r Earth + altitude))². Understanding these principles is crucial for accurately calculating the motion of free-falling objects.
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my question leads to something bigger but to start g force on Earth is 9.8m/s2 for simlicity let's say 10.

1-is it rite to say if you drop an object in the 1st sec its acceleration is 10m/s2 in the 2nd sec it's 100m/s then in the 3rd sec it's 10000 m/s
2-if the above is correct what is the distance traveled i.e in the 3rd sec has the object traveled a total of 10000m.
3-how do you calculate g 100km above the earth.
 
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jsm6252 said:
1-is it rite to say if you drop an object in the 1st sec its acceleration is 10m/s2 in the 2nd sec it's 100m/s then in the 3rd sec it's 10000 m/s

No. After one second, its velocity is 10 m/s, after two seconds its velocity is 20 m/s, after three seconds its velocity is 30 m/s, etc. Its acceleration remains constant at 10 m/s^2.
 
To calculate g at 100km you need to use the equation:

g = (G*m1*m2) / r2

Where G is the gravitational constant, m1 is the mass of the earth, m2 is the mass of the body currently at 100km, r2 is the distance from the centre of the Earth (Earth's radius plus altitude of 100km).
 
thank you
 
A quicker way to calculate g at a given altitude h is to use the relation:

g at h = g at sea level * (r Earth / (r Earth + altitude))^2

where r Earth = average radius of the earth.

The quantity G * m1 * m2 / r^2 is the gravitational force acting between two masses m1 and m2 which are a distance r apart.
 
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