MadSci Network: Physics |
Simulations of giant impacts on planetary surfaces are very interesting indeed! And, impacts of two large planetary bodies have definitely occurred in the history of our solar system. Let me tell you about one particular impact of this sort that is well-agreed upon by the majority of scientists to have happened as our solar system formed – and this example is much closer to home for us here on Earth. The prevailing theory for how our Moon (yes, the Moon that you see at night, the same Moon that orbits Earth) was created is called the “Giant Impact Hypothesis”. This theory states that early in Earth’s history, roughly 4.3 Billion years ago, Earth was struck by an object about half of the Earth’s size. This object collided with Earth and released an enormous amount of energy which vaporized much of the smaller object as well as a large amount of the upper layers of the Earth itself. Other material from both planetary bodies was broken up and ejected into space. But, Earth was large enough that some of this material remained in orbit around Earth and recondensed into our Moon. Needless to say, the entire details of this theory are very complicated, but there are a number of very good websites that contain further discussion: 1. The Planetary Science Institute has a page devoted to the “Origin of the Moon” (link below) which contains a number of artists renditions of what this event would have looked like, as well as the logic and evidence behind this theory. This page was put together by following the two scientists who initially proposed the “Giant Impact Hypothesis” in 1975. 2. NOVA did a program on the Origin of the Moon and they have an animation you can view on their online site (link below). The people at NOVA called it “The Big Whack”, but impact cratering scientists call it the “Giant Impact Hypothesis”. You will be able to find much more information on it by searching for the correctly used scientific term rather than a phrase that sounded good on television. 3. Space.com has a nice series of images from different times throughout the impact itself. Although it is not an animation, you can get more detailed information about what the impact looked like in viewing these time slices. Go to the Space.com “Making of the Moon” page (link below), scroll a third of the way down and click on the image on the right side of the page. As you can see, the idea of large objects hitting one another in space is something that interests many scientists. Hopefully I’ve given you an idea of what that type of impact might look like. However, let me now specifically address your question regarding Jupiter. While I’m unaware of any specific work done on this question, there is some basic information about impacts and their results that I can give you and apply to a giant impact on Jupiter. Any impact of one object (let’s call it “Big”) with another that is roughly half the size of the first object (let’s call it “Medium”) will produce a tremendous amount of energy, especially when “Big” is the size of a planet, be it the Earth or Jupiter. This absolutely enormous amount of energy will generate a lot of heat and break up a lot of the material that both “Big” and “Medium” are made up of. What happens to that material when it gets broken up mainly depends on how “Medium” hit “Big”. If “Medium” hits “Big” head-on, then the most likely scenario is that both objects would cease to exist as they did before. This is to say that the amount of energy would act like a huge explosion and blow both “Big” and “Medium” apart. If, however, “Medium” hit “Big” at an angle, say it just grazed the top of “Big”, then enough of “Big” might remain to gravitationally attract some of the other material that was broken up, which would then either crash back into “Big” or maybe recondense to form a smaller object in orbit around “Big”. (This is basically the situation that happened when the Moon was formed and you can see in many of the animations how “Medium” hit “Big” almost sideways, instead of straight on.) Now, there is one big difference between the Moon-forming Giant Impact and the type of impact that you are asking about with Jupiter. Jupiter is a Gas Giant planet – it does not have a solid surface like we are used to here on Earth. Rather, it is almost entirely an atmosphere that simply gets more and more dense as you move into the planet (much like how when you walk into a foggy area, the fog gets denser and denser). Atmospheres can affect what happens during an impact but mainly only in very small impacts. As we saw in 1994 when Comet Shoemaker-Levy 9 hit Jupiter (link below), there is still an enormous amount of energy generated in Jupiter’s atmosphere by even a small body during an impact. So, it is my best guess that if a solid body half the size of Jupiter hit Jupiter, there would be enough energy generated that the smaller body would be completely disrupted or ripped apart and vaporized. The planet Jupiter would lose a lot of material from its atmosphere and probably be very different from the planet we know today once (and if) it recovered from this giant impact. If the smaller body hit Jupiter head-on and at a fast enough velocity, then it is possible that Jupiter itself would be destroyed and its material spread throughout the solar system. Luckily, the only planetary body in our solar system that is half the size of Jupiter or larger is Saturn and Saturn’s orbit will never intersect with Jupiter’s, so that is good news for Jupiter! Planetary Science Institute’s “Origin of the Moon” page http://www.psi.edu/projec ts/moon/moon.html NOVA online has movie of “The Big Whack” http://www.pbs. org/wgbh/nova/tothemoon/origins2.html Space.com “The Making of the Moon” http://www.space.com/scienceastronomy/solarsystem/moon_making_01081 5-1.html Lunar and Planetary Laboratory’s “Collision with Jupiter” page http://seds.lpl.arizona.edu /sl9/sl9.html
Try the links in the MadSci Library for more information on Physics.