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SOLAR SYSTEM
Jiri W a g n e r , Jr., wag@volny.cz

METEOROIDS, METEORS, METEORITES

A meteor is a bright streak of light in the sky (a "shooting star" or a "falling star") produced by the entry of a small meteoroid into the Earth's atmosphere. If you have a dark clear sky you will probably see a few per hour on an average night; during one of the annual meteor showers you may see as many as 100/hour. Very bright meteors are known as fireballs.

Meteorites are bits of the solar system that have fallen to the Earth. Most come from asteroids, including few are believed to have come specifically from 4 Vesta; a few probably come from comets. A small number of meteorites have been shown to be of Lunar (15 finds) or Martian (13) origin.

Though meteorites may appear to be just boring rocks, they are extremely important in that we can analyze them carefully in our labs. Aside from the few kilos of moon rocks brought back by the Apollo and Luna missions, meteorites are our only material evidence of the universe beyond the Earth.

 

Meteorite Types
Iron	primarily iron and nickel; similar to type M asteroids
Stony Iron	mixtures of iron and stony material like type S asteroids
Chondrite	by far the largest number of meteorites fall into this class; similar in composition to the mantles and crusts of the terrestrial planets
Carbonaceous Chondrite	very similar in composition to the Sun less volatiles; similar to type C asteroids
Achondrite	similar to terrestrial basalts; the meteorites believed to have originated on the Moon and Mars are achondrites

A "fall" means the meteorite was witnessed by someone as it fell from the sky. A "find" means the meteorite was not witnessed and the meteorite was found after the fact. About 33% of the meteorites are witnessed falls. The following table is from a book by Vagn F. Buchwald. Included are all known meteorites (4660 in all, weighing a total of 494625 kg) in the period 1740-1990 (excluding meteorites found in Antarctica).

 

Meteorite Statistics
Type	Fall %	Find %	Fall Weight	Find Weight
Stony	95.0	79.8	15200	8300
Stony-Iron	1.0	1.6	525	8600
Iron	4.0	18.6	27000	435000

A very large number of meteoroids enter the Earth's atmosphere each day amounting to several hundred tons of material. But they are almost all very small, just a few milligrams each. Only the largest ones ever reach the surface to become meteorites. The largest found meteorite (Hoba, in Namibia) weighs 60 tons.

The average meteoroid enters the atmosphere at between 10 and 70 km/sec. But all but the very largest are quickly decelerated to a few hundred km/hour by atmospheric friction and hit the Earth's surface with very little fanfare. However meteoroids larger than a few hundred tons are slowed very little; only these large (and fortunately rare) ones make craters.

A good example of what happens when a small asteroid hits the Earth is Barringer Crater (a.k.a. Meteor Crater) near Winslow, Arizona. It was formed about 50,000 years ago by an iron meteor about 30-50 meters in diameter. The crater is 1200 meters in diameter and 200 meters deep. About 120 impact craters have been identified on the Earth, so far (see below).

A more recent impact occured in 1908 in a remote uninhabited region of western Siberia known as Tunguska. The impactor was about 60 meters in diameter and probably consisting of many loosely bound pieces. In contrast to the Barringer Crater event, the Tunguska object completely disintegrated before hitting the ground and so no crater was formed. Nevertheless, all the trees were flattened in an area 50 kilometers across. The sound of the explosion was heard half-way around the world in London.

 

There are probably at least 1000 asteroids larger than 1 km in diameter that cross the orbit of Earth. One of these hits the Earth about once in 300,000 years on average. Larger ones are less numerous and impacts are less frequent, but they do sometimes happen and with disasterous consequences.

 

 

The impact of a comet or asteroid about the size of Hephaistos or Shoemaker-Levy 9 comet hitting the Earth was probably responsible for the extinction of the dinosaurs 65 million years ago. It left a 180 km crater now buried below the jungle near Chicxulub in the Yucatan Peninsula (right).

Calculations based on the observed number of asteroids suggest that we should expect about 3 craters 10 km or more across to be formed on the Earth every million years. This is in good agreement with the geologic record. It is more difficult to compute the frequency of larger impacts like Chicxulub but once per 100 million years seems like a reasonable guess.

 

Here are educated guesses about the consequences of impacts of various sizes:

Impactor Diameter (meters)	Yield (megatons)	Interval (years)	Consequences
< 50	< 10	< 1	meteors in upper atmosphere most don't reach surface
75	10 - 100	1000	irons make craters like Meteor Crater; stones produce airbursts like Tunguska; land impacts destroy area size of city
160	100 - 1000	5000	irons,stones hit ground; comets produce airbursts; land impacts destroy area size of large urban area (New York, Tokyo)
350	1000 - 10,000	15,000	land impacts destroy area size of small state; ocean impact produces mild tsunamis
700	10,000 - 100,000	63,000	land impacts destroy area size of moderate state (Virginia) ocean impact makes big tsunamis
1700	100,000 - 1,000,000	250,000	land impact raises dust with global implication; destroys area size of large state (California, France)

(from 'The Impact Hazard', by Morrison, Chapman and Slovic, published in Hazards due to Comets and Asteroids)

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Source: The Nine Planets

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