Calculating Centripetal Acceleration of Space Telescope in Orbit

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To calculate the centripetal acceleration of a space telescope in orbit, the formula used is Ac = GM[e]/R^2, where G is the gravitational constant, M[e] is the mass of the Earth, and R is the distance from the Earth's center to the telescope. The mass of the telescope cancels out, simplifying the calculation. The user is obtaining an unexpectedly large value for acceleration, while the expected answer is 4.0 m/s^2. A key point of confusion is the need to convert the radius from kilometers to meters for accurate results. Ensuring proper unit conversion is crucial for obtaining the correct centripetal acceleration.
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I've done a bunch of these before, but don't know why I'm not getting the right answer this time around:

A space telescope of mass m[t]=10,000 kg is in a stable circular orbit above the Earth at an altitude h=3630 km. The radius and mass of the Earth are R[e]=6370 and M[e]=6x10^24 kg. Newtons gravitational constant is 6.672x10^-11.

What is the acceleration of the space telescope as it orbits the earth?

_____________

So this is simple enough-we're looking for the centripetal acceleration. So m[t]*Ac=GM[e]m[t]/R^2[earth center to satellite]. The m[t]'s cancel out, so we have centripetal acceleration =GM[e]/R^2, and I'm getting a really large number, even though the answer is supposed to be 4.0 m/s^2. What do you see I'm doing wrong?
 
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R[e] is in km, did you convert it meters?
 

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