A piece of ejecta is thrown up, what is the velocity

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The discussion revolves around calculating the velocity of ejecta thrown from a celestial body, specifically using energy conservation principles. Participants clarify the use of gravitational potential energy equations, emphasizing the importance of correctly measuring distances from the center of mass. The initial velocity and gravitational acceleration values are debated, leading to a derived final velocity of approximately 1447.98 m/s. Concerns are raised about the implications of such a high impact speed on the surface. Overall, the calculations highlight the complexities involved in determining the velocity of ejecta in a gravitational field.
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Homework Statement


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Homework Equations


energy conservation

The Attempt at a Solution


I used this equation:

1/2 mg R^2/ r1 + 1/2 mv1^2 = 1/2 mg R^2/ r2 + 1/2 mv2^2
For r1, it is 1738 km (radius) + 1000 km (above surface) ?
But for r2 , it is on the surface, so would it be 0??
 
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nysnacc said:
1/2 mg R^2/ r1
That does not look quite right to me. Are you sure you have quoted it correctly?
Also you need to think about the sign.
 
Sorry.
mg R^2/ r1 + 1/2 mv1^2 = mg R^2/ r2 + 1/2 mv2^2
For r1, it is 1738 km (radius) + 1000 km (above surface) ?
But for r2 , it is on the surface, so would it be 0??
 
nysnacc said:
Sorry.
mg R^2/ r1 + 1/2 mv1^2 = mg R^2/ r2 + 1/2 mv2^2
For r1, it is 1738 km (radius) + 1000 km (above surface) ?
But for r2 , it is on the surface, so would it be 0??
I edited my first reply while you were responding...
 
So it would be - before mg? based on the definition?

But my concern is mainly what happened with the potiential energe when it hits the surface, because the radius above surface will be 0, making the expression 1/0
 
nysnacc said:
So it would be - before mg? based on the definition?

But my concern is mainly what happened with the potiential energe when it hits the surface, because the radius above surface will be 0, making the expression 1/0
The equations you quote all take radii as being measured from the centre of mass of the moon.
 
Big R is the radius of the moon
while r is the distance above the surface?
 
nysnacc said:
Big R is the radius of the moon
while r is the distance above the surface?
You are given the distance above the surface, but the equations you quote require r to be measured from the mass centre of the gravitational body.
 
V = 1447.98 m/s ??
 
  • #10
nysnacc said:
V = 1447.98 m/s ??
Seems too much. Please post all your working.
 
  • #11
-mg R2/ r1 +1/2 m v12 = -mg R2/r2 +1/2 m v22

r1 is radius + distance above > R , r2 = R

so
-g R2/ r1 +1/2 v12 = -g R +1/2 v22

With v1 = 200 m/s, g = 1.62 m/s2

-2g R2/ r1 + 2g R +v12 = v22

-2g {R2/ r1 - R} + v12 = v22

-2(1.62) (17380002/2738000 - 1738000) + (200)2 = v22

So then v2 is sqrt of the left hand side, = 1447.98 m/s
 
  • #12
nysnacc said:
-mg R2/ r1 +1/2 m v12 = -mg R2/r2 +1/2 m v22

r1 is radius + distance above > R , r2 = R

so
-g R2/ r1 +1/2 v12 = -g R +1/2 v22

With v1 = 200 m/s, g = 1.62 m/s2

-2g R2/ r1 + 2g R +v12 = v22

-2g {R2/ r1 - R} + v12 = v22

-2(1.62) (17380002/2738000 - 1738000) + (200)2 = v22

So then v2 is sqrt of the left hand side, = 1447.98 m/s
Fair enough... my rough estimate must have had a mistake somewhere. The 200m/s turns out to be insignificant.
 
  • #13
But does it make sense to crash the surface at such speed?
 
  • #14
nysnacc said:
But does it make sense to crash the surface at such speed?
Quick lower bound: up to 1738km from surface, g is at least 1.6/22=0.4m/s2. Using v2=2as=800,000m2/s2, v is at least 900m/s.
 

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