Physics centripetal acceleration/ mass

In summary, using the given information of a moon's orbit with a period of 1.8 days and a radius of 420,000,000 meters, the mass of the planet can be found by equating the centripetal force to the gravitational force, and solving for the mass in terms of the period and radius. By substituting the given values, the mass of the planet is approximately 10^15 kg, which is close to the mass of Jupiter's satellite Io. It is important to remember to square the velocity when using the equation for centripetal acceleration.
  • #1
astru025
163
0

Homework Statement



A moon orbits a planet of unknown mass with a period of 1.8 days. If the radius of the moon's orbit is 420,000,000 meters, find the mass of the planet.

Homework Equations



For the speed of the moon I got: v=2 x pie x r / v
2 x pie x 420000000 / v = 1.8 days or 155520 seconds since speed is m/s.
v= 16968.5 m/s.

For the centripetal acceleration of the moon I got this: a= v^2/ r
16968.5 ^2 / 420000000 = .69 s

Now for the mass of the planet I am not quite sure how to figure out. If I know the speed and centripetal acceleration for the moon how do I use this to get the mass of the planet orbiting the moon??

The Attempt at a Solution


My attempt but was un successful:
v^2= G (Me/r)
16968.5 m/s^2= 6.67E-11 ( Me/420000000)
1.03E10
 
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  • #2
Looks pretty good! The first bit confuses me because you use v for velocity and also for period (usually T), but I agree with your velocity number. I also agree with the a = .69, but the units are m/s², not seconds. I don't quite see how you are getting the mass in the last part. It appears you forgot to square the velocity.

Astru, I would like to offer you a hot tip. Whenever you see the word "orbit" in a problem, immediately write down "centripetal force equals gravitational force" or Fc = Fg. Then replace the Fg with your big G formula and Fc with either the formula with v in it or the one with T in it. In this case, you are given the period, so use the one with the T and don't bother to calculate the velocity. (If you only have Fc = mv²/R, then replace the v with 2πR/T to get Fc = 4π²mR/T²)
You'll soon have an equation where you can cancel the mass of the moon and solve for the mass of the planet in terms of period and radius - only one calc instead of three so less chance for error! For me, the mass works out to roughly 10 to the 15th kg.
 
  • #3
You forgot to square the speed, haven't you?

The parameters are pretty close to those of Jupiter's satellite Io. So I expect you'll get a mass close to Jupiter's mass. Order of magnitude 10^27 kg.
 
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FAQ: Physics centripetal acceleration/ mass

What is centripetal acceleration?

Centripetal acceleration is the acceleration experienced by an object moving in a circular path. It is directed towards the center of the circle and its magnitude is equal to (v^2)/r, where v is the velocity and r is the radius of the circle.

How is centripetal acceleration related to mass?

Centripetal acceleration is not directly related to mass. It is dependent on the speed and radius of the circular motion, as well as the force causing the object to move in a circular path. However, the force required to maintain the centripetal acceleration does depend on the mass of the object, as given by the equation F = mv^2/r.

Can centripetal acceleration change the mass of an object?

No, centripetal acceleration does not change the mass of an object. It only affects the object's motion by causing it to accelerate towards the center of the circle. The mass of an object remains constant unless acted upon by an external force.

How does centripetal acceleration affect the motion of objects?

Centripetal acceleration causes objects to move in a circular path. Without this acceleration, objects would move in a straight line at a constant speed. It also changes the direction of an object's velocity, as it is always directed towards the center of the circle.

What are some real-life examples of centripetal acceleration?

Some common examples of centripetal acceleration include the motion of a car around a curved road, the rotation of a Ferris wheel or merry-go-round, and the orbit of planets around the sun. It is also seen in the movement of objects in a centrifuge and the spinning of a ball on a string.

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