Calculating Comet Halley's Speed Across Neptune's Orbit

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SUMMARY

To calculate Comet Halley's speed when it crossed Neptune's orbit in 2006, the conservation of energy principle is applied. At its perihelion in February 1986, the comet was 8.79x107 km from the Sun and traveling at 54.6 km/s. The necessary distance from the Sun when the comet crossed Neptune's orbit can be determined using the mean distance of Neptune from the Sun. This approach allows for the cancellation of the comet's mass and focuses on the Sun's mass for the calculations.

PREREQUISITES
  • Understanding of conservation of energy in physics
  • Familiarity with gravitational potential energy equations
  • Knowledge of orbital mechanics and distances in the solar system
  • Basic algebra for solving equations
NEXT STEPS
  • Research the conservation of mechanical energy in celestial mechanics
  • Learn how to calculate gravitational potential energy using the formula U = -GMm/r
  • Investigate the mean distance of Neptune from the Sun and its implications for orbital calculations
  • Explore the concept of perihelion and its significance in comet trajectories
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Astronomy students, physics enthusiasts, and anyone interested in celestial mechanics and the dynamics of cometary orbits.

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Homework Statement


At its perihelion in February 1986, Comet Halley was 8.79x10^7 km form the Sun and was moving at 54.6 km/s. What was its speed when it crossed Neptune's orbit in 2006?


Homework Equations


K0+U0=K+U


The Attempt at a Solution


I know I need to do this using conservation of energy. I have v-initial and r-initial, and presumably I can look up r-final. The mass of the comet will cancel, and big M will be the mass of the sun(also can look up). I am just confused about the r's, though. I was wondering why it is necessary to know the dates or that it was at its perihelion. How do I find the distance it was from the sun when it crossed Neptune's orbit?
 
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I figured it out. You actually just have to use the mean distance of Neptune from the Sun, and then you have all of the necessary information to use conservation of energy.
 

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