Relay-Version: version B 2.10 5/3/83; site utzoo.UUCP Posting-Version: version B 2.10.3 4.3bsd-beta 6/6/85; site ucbvax.BERKELEY.EDU Path: utzoo!watmath!clyde!burl!ulysses!mhuxr!mhuxt!houxm!ihnp4!qantel!lll-crg!ucdavis!ucbvax!space From: KFL@MIT-MC.ARPA ("Keith F. Lynch") Newsgroups: net.space Subject: Slingshot effect Message-ID: <[MIT-MC.ARPA].726285.851121.KFL> Date: Thu, 21-Nov-85 00:20:37 EST Article-I.D.: <[MIT-MC.ARPA].726285.851121.KFL> Posted: Thu Nov 21 00:20:37 1985 Date-Received: Sun, 24-Nov-85 06:12:58 EST Sender: daemon@ucbvax.BERKELEY.EDU Organization: The ARPA Internet Lines: 111 Date: 19 Nov 85 20:00:07 GMT From: decwrl!dec-rhea!dec-tle!crimmin@ucbvax.berkeley.edu (DTN 1-2015) Subject: slingshot effect Is the trajectory a hyperbola while the probe is en route to Jupiter, or only after it misses? The trajectory isn't really a simple curve, since it is influenced by both the Sun and Jupiter. At first, you can regard it as being an ellipse about the Sun. If Jupiter didn't get in the way, it would continue to orbit the Sun in an elliptical orbit with perihelion near Earth's orbit and a aphelion near Jupiter's orbit. Eventually, it would get close enough to either Jupiter or Earth that its orbit would be perturbed (or it would crash into one of those planets, or perhaps into an asteroid - not into Mars though, it passes above or below Mars' orbit). But of course the elliptical orbit is so designed that Jupiter will be at the apogee when the probe is there, so it never completes even one full elliptical orbit of the Sun. This, by the way, is called a Hohmann minimum energy orbit - the least energy way to get from here to Jupiter. The probe does not quite hit Jupiter, but it does pass so close that Jupiter's effect on the probe greatly overwhelms the Sun's effect. If we now switch to a frame of reference in which Jupiter is stationary (we were in a frame of reference in which the Sun was stationary), we see the probe coming almost directly towards Jupiter in nearly a straight line. As the probe gets closer it speeds up and curves towards Jupiter. It swings past, the path straightens out in a new direction, and it slows down. Once more it is in a nearly straight line, going almost directly away from Jupiter, and is going at the same speed it came in at. Note that since it 'fell' to Jupiter from a great altitude, it had more than Jupiter-escape-velocity at every distance from Jupiter, so it could not possibly have become a satellite of Jupiter. No matter how it was aimed, unless it hit Jupiter it had to leave the vicinity of Jupiter as fast as it came in. In the vicinity of Jupiter and in the reference frame in which Jupiter is stationary, the path of the probe was a hyperbola with Jupiter at one focus. Switching back to a Sun centered reference frame we see that the velocity is not the same as it was. After passing by Jupiter the probe is now going much faster. Once it becomes distant enough from Jupiter that the Sun's gravity is the only significant force on the probe, the path of the probe is a hyperbola with the Sun at one focus. If nothing gets in the way, the probe will continue out of the solar system and into interstellar space to wander among the stars for countless eons. The chances of it ever running into a star or a planet in another solar system are vanishingly small, even though it will be roaming entirely within our galaxy - it doesn't have galactic escape velocity. It is an interesting exercise to imagine how one would go about detecting a Voyager/Pioneer type probe in interstellar space, even assuming there are several in each cubic light year (launched by other civilizations). Watching from Jupiter, the probe approaches and departs at the same velocity. Right. Does the probe perceive a faster velocity in relation to Jupiter? to the Sun? After leaving the vicinity of Jupiter, the probe is going faster relative to the Sun than relative to Jupiter. A few years later, when Jupiter is on the other side of the Sun, the probe is going faster relative to Jupiter than to the Sun, not that that is especially relevant. What is the meaning of *zero* the orbital speed of the planet relative to the Sun? I meant that if the probe was in the vicinity of Jupiter and was at rest relative to the Sun, Jupiter could accelerate the probe to twice Jupiter's orbital velocity, relative to the Sun. That alone is faster than solar escape velocity. The Voyager and Pioneer probes were not at rest relative to the Sun, however their velocity relative to the Sun in the vicinity of Jupiter WAS less than Jupiter's, i.e. Jupiter overtook the probes. It's kind of confusing. One could, in principly, go anywhere simply by aiming your rocket in the right direction. But we don't have anywhere near enough energy to do it that way. So it is done in the most energy efficient way possible, hence the various Hohmann orbits and slingshot effects. Is this correct? From the Sun, the probe appears to accelerate to a speed twice that of Jupiter in its orbit of the Sun. But from Jupiter, the probe appears to come and go at a constant velocity. Right. Not really twice Jupiter's speed, that is the theoretical maximum. Anyway, you don't really want to go that fast if you want to get to Saturn and to pass both Jupiter and Saturn as SLOWLY as possible, to have lots of time for observations. Also (in the Jupiter frame), the probe does come and go at the SAME velocity, but it isn't really a CONSTANT velocity. It increases to a maximum at the closest point to Jupiter and then decreases back to the original value. I think there is an out-of-ecliptic-plane probe being planned, that will pass underneath Jupiter so as to rise up out of the plane which all the planets travel around the Sun. This will give us the first clear view of the Sun's north and south poles. It is ironic that a probe meant to study the Sun has to go past Jupiter first, since Jupiter is four times further than the Sun, and in the opposite direction. But it is the most energy efficient way to get a probe out of the ecliptic plane. It would be done in the same way if the probe was to drop straight into the Sun. In space it is just as hard to lose velocity as to gain it, and any probe to the Sun has to lose the Earth's orbital velocity about the Sun or it will just continue to orbit the Sun in the vicinity of Earth. Hope this answers your question. ...Keith