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Myth: Asteroid fields would be dangerous to fly through.

The reality is that the asteroids in asteroid fields are incredibly far apart and most of the objects in these fields are very tiny. There’s generally hundreds of thousands of miles between the objects and most of these objects are no bigger than a tennis ball and are called meteoroids, with the cutoff for being called an asteroid at around 164 feet (50 meters) on a side.

In fact, if you added up the mass of all the asteroids in our solar system’s asteroid belt, it’s a mere 4% of the mass of our moon with about 1/3 of that total mass coming from just one asteroid, Ceres, and about 1/2 of the total mass from just four asteroids, Ceres, Vesta, Pallas, and Hygiea.

It’s Gonna Be a Bumpy Ride?

So that’s our asteroid belt. What about others? Could there be an asteroid belt out there that would be dangerous to fly through? It’s a big universe, so it’s entirely possible that there exists such fields at any given moment in time somewhere in the universe, but it would be very unlikely that you’d encounter it, even if you could travel anywhere you wanted. The reason being that even if the asteroid belt is initially packed with debris that’s colliding everywhere (basically what is depicted by Hollywood), this would quickly (on a galactic time scale) sort itself out with most of the mass being ejected from the belt, due to these collisions. Eventually, the system would stabilize itself, becoming as sparse as our own asteroid belt is. So you’d need to find a system that was just forming and even then you’d likely see vast distances between the objects in such a system.

It’s estimated that our asteroid belt once contained about 1000 times the mass it currently contains. However, within about one million years of its formation, it was down to the stabilized amount we see today. Once this system was stabilized with almost no collisions, the asteroids simply travel in their respective orbits within the field itself, neither increasing nor decreasing in mass significantly since that initial stabilization period.

So how many collisions actually occur in our solar system’s asteroid belt? Of the asteroids above about 6 miles wide, it’s expected they’ll encounter about one collision of some sort every 10 million years. While that’s certainly a lot of collisions on a galactic time scale, it would have made Han Solo’s daring flight through the Hoth system’s asteroid field a bit less dramatic if depicted accurately…

For reference, NASA estimates the odds of one of their probes traveling through the asteroid field actually hitting an asteroid to be about one in a billion.

Bonus Science Stuff:

To date, 12 probes have traveled through the asteroid field: Pioneer 10; Pioneer 11; Voyagers 1 and 2; Ulysses; Galileo; NEAR, Hayabusa, Cassini; Stardust; New Horizons; and Roesseta. None has encountered a problem due to asteroids or debris and several of them didn’t spot any asteroids whatsoever while they passed through. It should also be noted that of some of those that did spot asteroids did so because they were specifically aimed such as part of their mission.

NASA recently launched a new probe aimed at being the first to encounter two asteroids in our asteroid field. This Dawn spacecraft is set to look at Vesta and Ceres and study them in detail. If it happens to still be functional afterward, they plan on pointing it at other asteroids to study them as well.

The largest known asteroid in our solar system’s asteroid field is Ceres, which is around 650 miles in diameter and is now sometimes classified as a dwarf planet. The runner-up is Pallas, which is about 360 miles in diameter.

Ceres was discovered by Giuseppe Piazzi in 1801. Once it was realized that it was neither a comet nor a planet, Sir William Herschel named it an asteroid, a word he made up. The word itself means “star-rock” or “star-planet” (aster-oid). Sir William Herschel was also the astronomer who discovered Uranus.

To date about 280,000+ asteroids have been found in our solar system with that number continuing to rise rapidly. Of those 280,000 only about 200 are bigger than about 60 miles in diameter (about 100km). It’s estimated that there are around 1-2 million asteroids in our solar system.

The vast majority of asteroids seem to be made of mostly carbon (75%, called C-type); the vast majority of the rest seem to be made of iron and nickel (M-type) with some are composed of silicates (S-type).

[Reposted (with editing) from Misconception Junction]