What is a 'Gravitational Slingshot'?

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SUMMARY

A gravitational slingshot, or gravity assist, is a maneuver used by space probes to gain speed by passing close to a planet, exchanging momentum with it. The probe can achieve significant velocity increases, with maximum changes in speed noted as 3.01 km/s for Mercury and up to 42.73 km/s for Jupiter, depending on the proximity of the flyby. While the probe retains the speed gained from the slingshot, its trajectory will continue to be influenced by the gravitational forces of other celestial bodies. This complex maneuver requires precise planning and execution to optimize the benefits of the gravitational interaction.

PREREQUISITES
  • Understanding of basic physics concepts, particularly momentum and gravity.
  • Familiarity with orbital mechanics and space probe trajectories.
  • Knowledge of planetary characteristics, including mass and gravitational pull.
  • Basic mathematical skills to comprehend velocity calculations and formulas.
NEXT STEPS
  • Research "Gravity Assist" techniques and their applications in interplanetary missions.
  • Study the mathematical formulas related to gravitational slingshots and momentum exchange.
  • Explore case studies of missions utilizing gravitational slingshots, such as the Cassini mission.
  • Learn about the limitations and constraints of gravitational slingshot maneuvers in mission planning.
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Aerospace engineers, astrophysicists, students of physics, and anyone interested in the mechanics of space exploration and orbital dynamics will benefit from this discussion on gravitational slingshots.

xilc
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I was wondering, since I've heard it said so many times. They space probes use gravitational slingshots. Okay, I get it, a probe goes around a planet or something, and when it goes around the other side, its faster right? Well...how exactly does it work?
1: How does a Gravitational Slingshot work?
2: How much faster does the slingshot make the object?
3: Does the object go on at the speed the slingshot gives it forever? (In space, i thought you never slow down since there is no friction.)
4: Is there some mathematical formula for this? If so, what is it? thanks!
5: anything else you can tell me about it helpful? ANYTHING about gravitational slingshots really will help!
 
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1. As a probe swings past a planet, they exchange some of their momentum. If the trajectory is planned well, the probe comes away with a little more momentum and the planet coems away with a little less. Slingshot 100 million probes past Jupiter, and it'll start falling sunward.

It can work in reverse too. You can slow probes the same way. You might want to do this if going to an inner planet and you want to slow to go into orbit (it will have too much velocity from falling sunward).

2. http://en.wikipedia.org/wiki/File:Cassini's_speed_related_to_Sun.png

3. Well, it gives it a kick. What happens to it after that is up to the gravity of any other objects it's around (the sun will work on it as long as it is in or near the solar system).

4. It's a pretty complex maneuver.

5. http://en.wikipedia.org/wiki/Gravity_assist
 
Last edited:
2. According to [1] the maximum change in speed for an unpowered planetary flyby is

3.01 km/s Mercury
7.33 km/s Venus
7.91 km/s Earh
3.55 km/s Mars
42.73 km/s Jupiter
25.62 km/s Saturn
15.18 km/s Uranus
16.75 km/s Neptune
1.10 km/s Pluto (still counted as a planet back in 1998 :)

Since change in speed very much depends on how close a probe passes the planet, the maximum values above comes from assuming the probe just grazes the planet surface during flyby (any closer and the probe will impact on the surface). Since probes in practice obviously has to stay out of any planetary atmosphere that might be present, the actual maximum change obtainable in a practical mission may be somewhat lower. There may also be other constraints that "lowers" the maximum on a particular mission, such as geometrically constraints requiring the probe to originate from one planet, flyby a second and then head off to a third.

[1] Multiple Gravity Assist Interplanetary Trajectories, Labunsky, Papkov, and Sukhanov. Gordon and Breach Science Publishers, 1998.
 

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