Calculating Comet Halley's Speed at Perihelion

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The discussion revolves around calculating the speed of Comet Halley at perihelion using its orbital parameters. Participants clarify that the closest approach distance is indeed the perihelion distance, and they explore methods to derive the comet's velocity at this point. The conversation highlights the importance of using Kepler's laws and conservation of angular momentum to find the necessary values. Ultimately, the correct speed at perihelion is determined to be 54,200 m/s, along with the aphelion speed and the ratio of perihelion to aphelion distances. The accuracy of calculations is emphasized, noting that the order of solving the equations affects the results.
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Use the following data to calculate the speed vp of comet Halley at perihelion. Comet Halley orbits the Sun with a period of 76 years and in 1986 had a distance of closest approach of 8.90×1010 m and an aphelion distance of 5.30×1012 m.

I'm stumped so far on this one. I'm assuming the closest approach distance is useless info thrown in there. I know I could use keplers law of periods to find what the perihelion distance is, and I know that angular momentum is constant, so I could find the velocity at aphelion if I knew vp, but I can't figure out how to get vp. :confused:
 
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Total energy (gravitational potential + kinetic) is also conserved, since only gravity is acting on the comet.
 
so how would you find vp?
 
I'll toss you a bone here. The closest approach distance is the perhelion.
 
oh ok, but still, even if i know both distances, i don't see how i would solve for vp
 
Felix83 said:
oh ok, but still, even if i know both distances, i don't see how i would solve for vp

There are a number of ways to get this answer, here's one:

Use the the two distances given to find the semi-major axis of the orbit (the average orbital distance.)

With this and the given period of the orbit you can get the orbital velocity at that distance.

This in turn gives you the angular momentum of the comet.

Find the velocity at the perhelion distance which gives you the same angular momentum.
 
Using conservation of angular momentum relative to the Sun, find the ratio of the comet's perihelion distance Rp to its aphelion distance Ra from the values of vp and va.

since distance of closest approach - perihelion distance and the aphelion distance are given, you would just divide the two to get the ratio. so it would be either 0.0168 or 59.5. however, the computer says both of these are wrong...?
 
ok using the formula v= (GM(2/ra - 1/a))^.5 i can find va if i calculate a, since i already know ra.

I used kepler's law of periods to calculate a=2.68*10^12m

I plugged that back into the formula along with ra to calculate
va=752m/s , which the computer says is wrong

do you guys get the same numbers when you calculate this?
 
  • #10
ok, there are 3 parts to the problem:
1) vp=?
2) va=?
3) rp/ra=?

once you have vp, I could easily find the other 2. i was surfing around the internet and happened to find that vp=54200m/s, which i plugged in and it was correct. then i calculated that va=963m/s and that rp/ra=0.0178 which were both also correct.

then I decided to try v= (GM(2/r - 1/a))^.5 for vp, and sure enough i got 54200m/s. the reason va, and rp/ra were wrong before is that i tried to calculate them before vp, and the rounding changes the answers slightly, so you have to calculate the 3 parts in a specific order.
 
  • #11
anyone have a proof of the forumula v= (GM(2/r - 1/a))^.5 ?
 
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