Asteroid on a collision course with Earth
NEOs, as their name suggests, are objects that in their travels around the Sun can occasionally come close to the Earth or even, sometimes, ram straight into it. There are three main types: asteroids, meteoroids, and comets. According to the definition used by NEO scientists, near-Earth asteroids (NEAs) range from 50 metres to a few tens of kilometres across and have orbits that never take them more than 1.3 astronomical units from the Sun. (An astronomical unit is the mean distance of the Earth from the Sun – about 150 million kilometres.) Asteroids are made of rock but often not just a single chunk of rock. Many of the smaller ones seem to be “rubble-pile” objects, composed of rocky debris held together loosely by gravity. A surprisingly high fraction of near-Earth asteroids are binaries (two objects close together, orbiting around each other, some actually in contact) Near-Earth meteoroids are, in NEO terminology, anything smaller than 50 metres across.
Near-Earth comets are a slightly different kettle of fish. Comets are made of more volatile stuff than asteroids; in other words, as well as chunks of rock they contain lots of materials, like water ice and frozen methane, that vaporise if the comet gets into a path that brings it close to the warming rays of the Sun. That’s why comets grow tails when they enter the inner parts of the Solar System, and also why comets that repeatedly come close to the Sun eventually burn out so that all that’s left behind is a dark porous rocky husk.
With the growing realization that NEOs have caused “extinction-level” events in Earth’s history, and that even much smaller ones can have devastating local and regional consequences, scientists, politicians, and the public at large have become concerned with what to do about this danger. The Earth will be hit again, many times, in the future by everything from city-buster Tunguska-type missiles to extinction-class behemoths, unless we do something about the threat.
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