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Why Almost No Shooting Star Ever Reaches the Ground
¶1 Every clear night, small streaks of light flash across the sky. Observers call all of them shooting stars, but none of these streaks are actually stars. Each one is a small chunk of rock or metal, called a meteoroid, burning as it plunges into the atmosphere. What decides the outcome is not how bright the streak looks or how fast it moves. It comes down almost entirely to size, and that one factor splits meteoroids into two very different outcomes. Some burn away completely, and these are called meteors. A rare few reach the surface intact, and these are called meteorites.
¶2 Most meteoroids burn away completely because they are tiny, no larger than a grain of sand or a pebble. Even so, they travel at enormous speed, often more than twenty kilometers per second. Friction with the air heats a meteoroid's outer surface far faster than heat can spread through its interior. That outer layer boils off almost instantly, a process called ablation. A fresh layer is exposed to the same intense heat a moment later. For an object this small, the entire mass ablates within seconds, well above seventy kilometers in altitude, long before gravity could pull it any closer. The Perseid meteor shower, visible every August, is made almost entirely of dust and gravel shed by a passing comet. Even though dozens of Perseid streaks can appear in a single hour, essentially none of that debris ever reaches the ground. Every particle finishes ablating high in the atmosphere.
¶3 Meteorites survive for the opposite reason: they enter the atmosphere already too large, or too tough, for ablation to strip away their whole mass. Unlike the sand-sized grains that produce meteor showers, an object heavier than a car cannot fully vaporize before it slows down. [A] In February 1947, an iron mass weighing many tons entered the atmosphere over the Sikhote-Alin Mountains of eastern Russia. [B] It burned brighter than the sun and stayed visible even in daylight. [C] It broke apart under aerodynamic stress a few kilometers above the ground, scattering more than one hundred fragments across a strewn field. [D] The heaviest single piece recovered weighed over seventeen hundred kilograms, and craters more than twenty meters wide still mark where the largest fragments struck.
¶4 Size decides most outcomes, but composition tilts the odds further. Iron meteoroids are denser and structurally tougher than stony ones, so an iron object of a given size ablates more slowly and is less likely to shatter under the pressure of entry. A stony meteoroid the same weight as the Sikhote-Alin fragments would be far more likely to crumble into pieces too small to survive. That difference is part of why most meteorites recovered on the ground are iron, or stone mixed with iron. Iron itself, however, makes up only a small share of the rock and metal that enters the atmosphere overall.
¶5 Researchers now use networks of all-sky cameras to record fireballs and calculate a falling object's size, speed, and path within minutes of its entry. Knowing whether an object is large enough, and tough enough, to survive ablation lets them predict a strewn field before anyone searches for fragments on the ground. Astronomers had long noticed a pattern that this reasoning explains: meteor showers, built from comet dust, almost never leave meteorites behind. Isolated meteoroids heavy enough to become meteorites, in turn, rarely arrive as predictable showers.
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11 questions — every TOEFL Reading question type, in test order.
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Highlighted: "Iron meteoroids are denser and structurally tougher than stony ones, so an iron object of a given size ablates more slowly and is less likely to shatter under the pressure of entry."
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Witnesses hundreds of kilometers away reported seeing the light and hearing a delayed roar minutes later.
Where would the sentence best fit?
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Meteors Meteorites