Meteorites


 

Impact
by Douglas Preston
Amazon Price: CDN$ 19.44
Customer Review: I enjoyed the science fiction aspect of this book (or was it sci fi?) It was an interesting story that a person can pick up and read on and off during the summer. If you're into Mars and alien artif...

The Day of the Triffids
by John Wyndham
Amazon Price: CDN$ 12.05
Customer Review: This is a wonderfully told apocalyptic tale, as relevant today as it was in nineteen hundred and fifty one, when it was first published. Well-written, with believable characters and dialogue, it is ri...

The Ice Limit
by Douglas Preston, Lincoln Child
Amazon Price: CDN$ 9.50
Customer Review: This book is very similar to his other books yet different. To completely understand this you will have to read it. I found the book very entertaining...I know I use the word entertaining a lot, but t...

The Fallen Sky
by Christopher Cokinos
Amazon Price: CDN$ 28.00

Lunar Meteoroid Impacts and How to Observe Them
by Brian Cudnik
Amazon Price: CDN$ 23.16

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.

A meteorite is a meteor that survives an impact with the Earth's surface. While it's still out in space it is called a meteoroid. When it enters the atmosphere, impact pressure causes the meteoroid to heat up and emit light, thus forming a metwor or fireball. The term bolide refers to either an extraterrestrial body that collides with the Earth, or to an exceptionally bright, fireball-like meteor regardless of whether it ultimately impacts the surface or not.

More generally, a meteorite on the surface of any celestial body is a natural object that has come from elsewhere in space. Meteorites have been found on the Moon and Mars.

Meteorites that are recovered after being observed as they came through the atmosphere or impacted the Earth are called falls. All other meteorites are known as finds. As of mid-2006, there are approximately 1, 050 witnessed falls having specimens in the world's collections. In contrast, there are over 31, 000 well-documented meteorite finds.

Meteorites are always named for the place where they were found, usually a nearby town or geographic feature. One notable exception is Barringer Crater (commonly referred to as Meteor Crater) in Arizona which is named after the man who posited that it was formed in an impact with an extraterrestrial object. In cases where many meteorites were found in one place, the name may be followed by a number or letter (e.g., Allan Hills 84001 or Dimmitt (b)). Some meteorites have informal nicknames: the Sylacauga meteorite is sometimes called the "Hodges meteorite" after Ann Hodges, the woman who was struck by it; the Canyon Diablo meteorite, which formed Meteor Crater has dozens of these aliases. However, the single, official name designated by the Meteoritical Society is used by scientists, catalogers, and most collectors.

Meteorites have traditionally been divided into three broad categories: stony meteorites are rocks, mainly composed of silicate minerals; iron meteorites are largely composed of metallic iron-nickel; and, stony-iron meteorites contain large amounts of both metallic and rocky material. Modern classification schemes divide meteorites into groups according to their structure, chemical and isotopic composition and mineralogy.

Most meteoroids disintegrate when entering Earth's atmosphere. However, an estimated 500 meteorites ranging in size from marbles to basketballs or larger do reach the surface each year; only 5 or 6 of these are typically recovered and made known to scientists. Few meteorites are large enough to create large impact craters. Instead, they typically arrive at the surface at their terminal velocity and, at most, create a small pit. Even so, falling meteorites have reportedly caused damage to property, livestock and people.

One of the primary goals of studying meteorites is to determine the history and origin of their parent bodies. Several metoerites recovered from Antarctica since 1981 have conclusively been shown to have originated from the moon based on compositional matches of lunar rocks obtained by the Apollo missions of 1969-1972. Sources of other specific metorites remain unproven, although another set of eight meteorites are suspected to have come from Mars. These meteorites contain trapped atmospheric gases which match the composition of the Martian atmosphere as measured by the Viking landers in 1976. All other groups are presumed to have originated on asteroids or comets; the majority of meteorites are believed to be fragments of asteroids.

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