The Great BrownDuck wrote:
So, an object large enough to create an earth sized crater smashes into Jupiter, going completely unnoticed until after the impact and it's just "neat"? I realize Jupiter is some 400 million miles from Earth and about 11 times its diameter, but shouldn't we be able to detect something this big before it happens? NASA wasn't even remotely aware of the impact until someone who just happened to be spying Jupiter gave them a heads up. Sounds like our NEO search funding needs a boost.
There are no craters on gas giant planets. The largest fragment from Shoemaker-Levy 9, the fragmented comet that impacted Jupiter back in 1994, was only 2km(1.2mi) across. It left a blemish on Jupiter's atmosphere about 12000km in diameter, about twice that of Earth's. It was traveling close to 60km a second when it impacted.
Because Jupiter has no solid surface (discounting a possible solid core), the only thing an impactor has to impact against is gas. The friction caused by entering the atmosphere caused a fireball that reached nearly 24000K, and was itself thousands of kilometers in diameter. As it plunged into the atmosphere, the fragment's surface vaporized, leaving behind huge amounts of itself at various levels of the atmosphere, not to mention stirring up the juicy lower levels of the atmosphere as well.
Factor in the extreme speed of winds and atmospheric circulation in Jupiter, and it's not hard to see how such a (relatively) small impactor can create such a large impact feature that lasts for months.
If the same cometary fragment were to plummet though Earth's thin atmosphere and strike continental rock, it would create a transient crater about 20km across and 7km deep, with a final complex crater about 31km across and only 1km deep.
Basically, the entire impact energy is expended in one single kaboom when striking a rocky world, but on a gas giant the impact energy is spread out of a much larger area and depth.
As far as our instruments not detecting it, I'm fine with it. This rock or comet was only about 500m across, traveling at 60km/s, and was 5-6AU away from us. Had it been closer, it would have been brighter and much easier to spot.
As for Earth-crossing cometary orbits... Most comets have a highly elliptical orbit that takes them from the outer reaches of the solar system (35+AU) to very close to the sun (.1-.5AU). Luckily, most comets have their orbit highly inclined to the ecliptic, which means that when viewed from above the orbit may look like it would cross Earth's, but when viewed from the side it's easy to see that it comes nowhere close to us. Not to say we've never been impacted by a comet, but the chances of an impact similar impact to the one in the op occuring on Earth is about once every 7,200,000 years.
Edited, Jul 22nd 2009 11:38am by Tzemesce