Calculating Period of Rotation for Mars-Bound Weight at 3.8 m/s2

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To simulate a Mars-bound weight of 3.8 m/s² for astronauts in a spacecraft with a diameter of 2.8 km, the period of rotation must be calculated. The gravitational force equation and centripetal acceleration are equated to derive the velocity needed for the desired acceleration. Substituting this velocity into the formula for the period of rotation leads to the final equation for T. The solution indicates that the required period of rotation is approximately 1.2 * 10² seconds. Understanding the relationship between mass, acceleration, and rotation is crucial for achieving the desired simulation of Martian gravity.
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Homework Statement


As a spacecraft of diameter 2.8km approaches Mars, the astronauts want to experience what their Mars-bound weight will be. What should the period of rotation be to simulate an acceleration due to gravity of magnitude 3.8 m/s2 ?

Mass of Mars = 6.37*1023
Radius of Mars = 3.40*106

Homework Equations


(1) Fg = (GMm)/r2

(2) ac = (mv2)/r

(3) T = (2∏r)/v

The Attempt at a Solution



Fg = ac
(GMm)/r2 = (mv2)/r

Solving for v
v = √((GM)/r)

Sub v into eqn. (3)
T = (2∏r)*(√(r)/√(GM))
T = (2∏r(3/2))/√(GM)

And that's as far as i got cause I'm not sure what to do with the given information... The answer is 1.2*102s.
 
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You don't need to do anything with G or those mass figures. They already gave you the acceleration required. So the force produced will be F=ma=m*(3.8m/s^2). Equate that to mv^2/r.
 
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