Radially falling towards the Earth

In summary, the conversation discusses the time it takes for an object to reach Earth from infinity and the equations involved. It is determined that the trajectory from Earth to infinity is given by a general solution and that the object will fall from any finite distance in a finite time.
  • #1
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Heey everyone,

I was wondering how long it takes for a small mass to reach the Earth from infinity . The trajectory is completely radial, so it's a relatively simple equation.

$$r''(t ) =\frac{ - GM} {r(t)^2}. $$

But what if we multiplied both sides by ##2r'(t) ##. Then it follows,

$$2r'(t) r''(t ) =\frac{ - 2GM} {r(t)^2}r'(t).$$ $$ \implies \frac{d} {dt} (r'(t) ^2) =\frac{ - 2GM} {r(t)^2}r'(t).$$

Integrate with respect to t from t=t to t=##\infty##. and $$r'(\infty) =0 $$ and ##r(\infty) =\infty##.

$$ r'(\infty) ^2 - r'(t) ^2 =\frac{2GM} {r(\infty)} -\frac{2GM} {r(t)} $$, leaving with $$r(t)r'(t) ^2 =2 GM$$
Which has general solution:
$$r(t) =(3/2) ^{(2/3)} (C+\sqrt{2GM}t)^{(2/3)} $$.
Letting ##r(0)=R## we can determine C, that is ##C=2/3R^{(3/2)}##.

So our trajectory from Earth to infinity is given by:
$$r(t) =(3/2)^{(2/3)} [(2/3)R^{(3/2)}+\sqrt{2GM}t] ^{(2 /3)}$$
Differentiating gives:
$$r'(t) =(3/2)^{(2/3)}\frac{2 \sqrt{2GM}}{3(\sqrt{2GM}t+2R^{(3/2) } /3)^{(1/3)}} $$ $$ r'(0)= \sqrt{\frac{2GM}{R}}$$. Which validates the escape velocity.

I approached the problem by shooting the mass from the Earth to infinity and now I have come to the conclusion that it takes infinite amount of time.. Oops.

I suppose dropping it from any given height will give:
$$r'(t) ^2 =\frac{2GM}{r(t)}-\frac{2GM}{b} $$ where b is the height we are dropping it from.

Then $$b\pi/2 -\sqrt{2GM/b}t=b\tan^{-1}(\sqrt{\frac{r(t)}{b-r(t)}})-\sqrt{r(t)(b-r(t))}$$.

Then for ##t=t_{final} ## we must have ##r(t_{final}) =R##. Then the time can be determined how long the fall would take from b to R.

Thanks
 
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  • #2
An object falls from any finite distance in a finite time. Mathematically, as the distance tends to infinity, so does the time.
 

Related to Radially falling towards the Earth

1. What is "radially falling towards the Earth"?

Radially falling towards the Earth is a term used to describe the motion of an object as it falls towards the center of the Earth in a straight line, due to the force of gravity.

2. How is "radially falling towards the Earth" different from normal falling?

Normal falling occurs when an object falls towards the Earth in a curved path due to a combination of gravity and air resistance. In contrast, radially falling towards the Earth is a straight downward path towards the center of the Earth, with minimal air resistance.

3. What factors affect the speed of "radially falling towards the Earth"?

The speed of an object radially falling towards the Earth is affected by its mass and the strength of the Earth's gravitational pull. Objects with a larger mass will fall faster, while objects with a smaller mass will fall slower. Additionally, the strength of the Earth's gravity can vary slightly depending on the altitude and location of the object.

4. Can an object "radially falling towards the Earth" ever reach a constant speed?

Yes, an object falling towards the Earth will eventually reach a constant speed, known as terminal velocity. This occurs when the force of air resistance on the falling object is equal to the force of gravity pulling it towards the Earth.

5. What is the formula for calculating the speed of "radially falling towards the Earth"?

The formula for calculating the speed of an object radially falling towards the Earth is V = √(2GM/R), where V is the velocity, G is the gravitational constant, M is the mass of the Earth, and R is the distance from the center of the Earth to the object.

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