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

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SUMMARY

The discussion focuses on calculating the period of rotation required for a spacecraft to simulate a Mars-bound weight of 3.8 m/s². Using the gravitational force equation Fg = (GMm)/r² and centripetal acceleration ac = (mv²)/r, the solution derives the velocity v as v = √((GM)/r). Substituting this into the period equation T = (2∏r)/v leads to T = (2∏r(3/2))/√(GM). The final calculated period of rotation is 1.2 × 10² seconds.

PREREQUISITES
  • Understanding of gravitational force equations, specifically Fg = (GMm)/r²
  • Knowledge of centripetal acceleration and its formula ac = (mv²)/r
  • Familiarity with the concept of orbital mechanics and period of rotation
  • Basic algebra skills for manipulating equations and solving for variables
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  • Learn about the effects of centrifugal force in space travel
  • Study the principles of orbital mechanics and their applications in spacecraft navigation
  • Explore advanced calculations involving the gravitational constant G and its role in astrophysics
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Aerospace engineers, physics students, and anyone involved in spacecraft design and orbital mechanics will benefit from this discussion.

HKfish
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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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