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DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

DICTIONARY OF GEOPHYSICS, ASTROPHYSICS, and ASTRONOMY

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helium (for which the early tracers were metals<br />

like Ca,Fe, <strong>and</strong> Na). The solar value is about<br />

1.7%, or Z = 0.017. Observed values range<br />

from 10 −4 of solar metallicity (for the oldest<br />

stars in the halos of our own <strong>and</strong> other galaxies)<br />

to perhaps 2 to 3 times solar (for stars in<br />

the centers of large elliptical galaxies <strong>and</strong> the<br />

ionized gas near the centers of quasars). Frequently<br />

metallicity is given as the log 10 of the<br />

ratio of iron/hydrogen of the star divided by<br />

iron/hydrogen in the sun. This is abbreviated<br />

[Fe/H]. See elliptical galaxies, halo, quasar.<br />

metamorphism If sedimentary rocks are<br />

buried in a sedimentary basin, the temperature<br />

can become sufficiently high so that chemical<br />

reactions can occur. These reactions can transform<br />

a sedimentary rock into a metamorphic<br />

rock.<br />

meteor Any phenomenon in the air (a cloud<br />

is a humid meteor), but especially the glowing<br />

track of a meteoroid as it travels through the air.<br />

Such meteors also are often called shooting<br />

stars or falling stars. Most of the debris creating<br />

meteors is extremely small (dust to s<strong>and</strong>-sized)<br />

<strong>and</strong> burns up during the atmospheric passage.<br />

If the material survives the passage through the<br />

atmosphere <strong>and</strong> l<strong>and</strong>s on the surface, it is called<br />

a meteorite. A meteor shower occurs when large<br />

numbers of meteors are seen radiating from the<br />

same area of the sky.<br />

meteorite Meteoroids that survive to impact<br />

onto a body’s surface. Meteorites are classified<br />

as stones, meteorites that are composed primarily<br />

of silicates <strong>and</strong> are similar to terrestrial rocks;<br />

stony-ironmeteoriteswhichhaveapproximately<br />

equal amounts of iron <strong>and</strong> silicates; iron meteorites,<br />

composed almost entirely of nickel-iron;<br />

<strong>and</strong> further subdivided according to compositional<br />

details. Stony-irons are the least common.<br />

Most meteorites show thermal processing, <strong>and</strong><br />

arebelievedtobefragmentsoflargerparentbodies,<br />

probably asteroids, although Martian meteorites<br />

<strong>and</strong> lunar meteorites have also been identified.<br />

Meteorites are also often characterized<br />

as falls (seen to fall <strong>and</strong> recovered shortly thereafter)<br />

<strong>and</strong> finds, which are found long after they<br />

havel<strong>and</strong>ed. Stonymeteoritesarethemostcommon<br />

types of falls <strong>and</strong> are thus believed to rep-<br />

© 2001 by CRC Press LLC<br />

meteor shower<br />

resent the majority of meteoritic material. Irons<br />

are the most common types of finds simply because<br />

they do not erode as quickly, nor are they<br />

easily confused with terrestrial rocks. See meteorite<br />

parent body, SNC meteorites, <strong>and</strong> under<br />

the different classes of meteorites.<br />

meteorite parent body Different classes of<br />

meteorites have been differentiated to various<br />

degrees, <strong>and</strong> have been subjected to elevated<br />

temperatures <strong>and</strong> pressures. These processes<br />

presumably occurred while the meteorite was<br />

still part of a parent body. The breakup of such<br />

parent bodies resulted in the various meteortite<br />

classes observed. Particular asteroid classes<br />

have been identified with parent bodies of various<br />

meteorite types based on spectral similarities.<br />

meteoroid A metallic or rocky small body<br />

orbiting the sun in space; small particles that<br />

may derive from comets; larger (1 cm or larger)<br />

particles that probably derive from the asteroid<br />

belt. Meteoroids seen passing through an atmosphere<br />

are called meteors, <strong>and</strong> if they survive to<br />

l<strong>and</strong> on the surface, they are called meteorites.<br />

Small meteoroids are also often called interplanetary<br />

dust particles (IDPs). Sunlight reflecting<br />

off this material gives rise to the zodiacal light<br />

<strong>and</strong> the gegenschein.<br />

meteor shower A large number of meteors<br />

radiating from the same area of the sky. Meteor<br />

showers are caused when the Earth passes<br />

through an area of space with an enhanced<br />

amount of small debris. Most meteor showers<br />

are associated with cometary debris left behind<br />

in the comet’s orbit. Meteors in a meteor<br />

shower appear to radiate from the same area of<br />

the sky since the material causing the shower is<br />

located in a relatively small region of space. The<br />

constellation encompassing the area of the sky<br />

from which the meteors appear to radiate provides<br />

the name of the meteor shower (e.g., the<br />

Perseids appear to radiate from the constellation<br />

Perseus, the Leonids come from the constellation<br />

Leo, etc.). Debris large enough to survive<br />

passage through the atmosphere <strong>and</strong> l<strong>and</strong> on the<br />

surface as a meteorite is very rare during meteor<br />

showers.<br />

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