Meteor K-12 Experiments
Meteoroid vs Asteroid vs Meteorite vs Meteor
Meteoroid: A small rocky or metallic object in orbit around the Sun (or another star). A meteoroid which strikes the Earth (or other large body) is called a meteorite.
Asteroid: A rocky or metallic object, smaller than a planet but bigger than a meteoroid, that orbits the Sun or another star; also known as a minor planet.
Meteorite: A solid portion of a meteoroid that survives its fall to Earth, or to some other body.
Meteor: The light phenomenon, known popularly as a shooting star or falling star, that results from the entry into Earth’s atmosphere of a solid particle, or meteoroid, from space.
- The Worlds of David Darling
Meteor
A meteor is the visible path of a meteoroid that enters the Earth's (or another body's) atmosphere, commonly called a shooting star or falling star.
For bodies with a size scale larger than the atmospheric mean free path
(10 cm to several meters) the visibility is due to the heat produced by
the ram pressure (not friction, as is commonly assumed) of atmospheric entry.
Since the majority of meteors are from small sand-grain size meteoroid
bodies, most visible signatures are caused by dexcitation following the
individual collisions between vaporized meteor atoms and atmospheric
constituents.
A very bright meteor may be called a fireball or bolide.
The International Meteor Organisation defines fireballs as being
meteors of magnitude -3 or brighter. The meteor section of the British
Astronomical Association on the other hand has a much stricter
definition, requiring the meteor to be magnitude -5 or brighter.
If a meteoroid survives its transit of the atmosphere to come to rest on the surface, the resulting object is called a meteorite. A meteor striking the Earth or other object may produce an impact crater.
Molten terrestrial material "splashed" from such a crater can cool and solidify into an object known as a tektite.
Meteor dust particles left by falling meteoroids can persist in the
atmosphere for up to several months. These particles might affect
climate, both by scattering electromagnetic radiation and by catalyzing
chemical reactions in the upper atmosphere.
Ionization trails
During the entry of a meteoroid into the upper atmosphere, an ionization trail is created, where the molecules in the upper atmosphere are ionized by the passage of the meteor. Such ionization trails can last up to 45 minutes at a time. Small, sand-grain
sized meteoroids are entering the atmosphere constantly, essentially
every few seconds in a given region, and thus ionization trails can be
found in the upper atmosphere more or less continuously. When radio
waves are bounced off these trails, it is called meteor scatter
communication.
Meteor scatter has been used for experimental secure military
battlefield communications systems. The basic idea of such a system is
that such an ion trail will act as a mirror for radio waves, which can
be bounced off the trail. Security arises from the fact that as a
mirror, only receivers in the correct position will hear the transmitter,
much as with a real mirror, what is seen in reflection depends upon
one's position with respect to the mirror. Because the sporadic nature
of meteor entry, such systems are limited to low data rates, typically
459600 baud.
Amateur radio operators sometimes use meteor scatter communication on VHF bands. Snowpack information from the Sierra Nevada mountains in California is transmitted from remote sites via meteor scatter. Meteor radars can measure atmospheric density and winds by measuring the decay rate and Doppler shift of a meteor trail.
Large meteoroids can leave behind very large ionization trails, which then interact with the Earth's magnetic field. As the trail dissipates, megawatts of electromagnetic energy can be released, with a peak in the power spectrum at audio frequencies.
Curiously, although the waves are electromagnetic, they can be heard:
they are powerful enough to make grasses, plants, eyeglass frames,
frizzy hair and other materials vibrate. See for example, Listening to Leonids (NASA, 2001) for details and references on the auditory phenomenon.
See also
This article is licensed under the GNU Free Documentation License. It uses material from Wikipedia Encyclopedia article "Meteor"
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