Physics: Gravitational Force Circular Motion

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SUMMARY

The discussion focuses on gravitational force and circular motion, addressing three specific problems related to gravitational acceleration, the gravitational balance point between the Earth and the Moon, and the orbital radius of the asteroid Ceres. For problem A, the acceleration due to gravity at 1500 km altitude is calculated using the formula a = (GM)/r², where G is the gravitational constant. In problem B, the gravitational forces from the Earth and Moon are equated to find the balance point. Problem C involves calculating Ceres' orbital radius using the formula r = (GMT²)/(4π²), with G being 6.67 × 10⁻¹¹ and the Sun's mass as 1.99 × 10³⁰ kg.

PREREQUISITES
  • Understanding of Newton's law of universal gravitation
  • Familiarity with circular motion equations
  • Knowledge of gravitational constant (G = 6.67 × 10⁻¹¹)
  • Basic algebra and calculus for solving equations
NEXT STEPS
  • Calculate gravitational acceleration at various altitudes using the formula a = (GM)/r²
  • Explore the concept of Lagrange points in celestial mechanics
  • Learn about orbital mechanics and Kepler's laws of planetary motion
  • Investigate the mass distribution in the asteroid belt and its implications for gravitational interactions
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Students and educators in physics, astrophysics enthusiasts, and anyone interested in gravitational forces and orbital mechanics.

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Homework Statement



A.) What is the acceleration due to gravity at an altitude of 1500 km above the Earth's surface. Neglect the effect of the Earth's rotation. The Earth's radius is 6378100 m and its mass is 5.98 * 10^{24}kg.

B.) The moon has a mass of 7.35 * 10^{22} kg and is located 3.84 * 10^{8} m from the Earth (center to center). At some point between the Earth and the Moon, the gravitational force due to the Earth on any object cancels the gravitational force due to the Moon. Where is that position, relative to the center of the Earth?

C.) The asteroid belt consists of so many particles, we haven't counted them all yet. However, more than half of the mass of the belt is contained in the four largest asteroids. The largest - Ceres - takes 4.6 years on average to circle the Sun. What is the orbital radius of Ceres in meters.

1 year = 365 days, 1 day=24 hours, 1 hour=3600 seconds

Homework Equations



F=(GMm)/r^{2}
F=ma
a=v^{2}/r
v=(2\pir)/T
G=6.67 * 10^{-11}
Sun's Mass = 1.99 * 10^{30}

The Attempt at a Solution



A.) (GMm)/r^{2}=(mv^{2})/r
the m's cancel out and you are left with a (which was equal to v^{2}/r) = (Gm)/r^{2}
so a = \underline{(6.67*10^{-11})(5.98 * 10^{24} } (1500+6378100)

B.) I really don't understand what this question is asking. I think that it means that there is a place between the moon and the Earth that an object has no gravity. Would that mean that
(GM_{earth}m)/r^{2}_{x} = (GM_{moon}m)/r^{2}_{x} then everything just cancels out.

C.) (GMm)/r^{2}=(mv^{2})/r the m's cancel out. Then you replace v^2 with \underline{4\pi^{2}r}/T^{2}. And then you move the r to the other side. So

r=\sqrt[3]{GMT^{2}}/ \sqrt[3]{4\pi^{2}}


Thanks for any help.
 
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Sorry, for my attempt

A.) a=(GM)/r^2

C.) r=the cube root of [(GMT^2)/4pi^2)]
 
for C.) v=(2 pi r)/T so v^2 = (4 pi^2 r^2)/T^2
 

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