Meteor: the visible streak of light (popularly called a shooting star or a falling star). The column of light is usually less than 1 meter in diameter but tens of kilometers long.
Meteoroid: the solid object that creates the streak. They range in size from large fragments of asteroids or comets to extremely small micrometeoroids. Most visible meteors are created by meteoroids the size of a grain of sand.
Meteorite: the surviving object if it reaches the ground.

Fireball: a meteor brighter than the evening or morning star, Venus (technically, brighter than magnitude -4).
Bolide: a fireball that explodes in a bright flash often with visible fragmentation. Also the generic name for a large crater-forming projectile (comet, asteroid or UFO).
Meteor Trail: the trail of ionized dust and gas that remains along the path of a meteor.

Meteor Stream: a group of meteoroids in a given orbit as they travel around the sun. These meteoroids are usually the by-product of comets, so it is possible for the parent comet to be traveling in the same orbit--if it still exists.
Meteor Shower: the occurrence of meteors as Earth's orbit intersects a meteor stream. The meteors in a shower appear to emanate from a point in the sky known as the radiant. A meteor shower is named after the constellation in which its radiant is located.
Meteor Storm: an intense meteor shower that exceeds 1000 meteors per hour which occurs when Earth encounters a dense group of meteoroids within a meteor stream.
Minor Meteor Showers: meteor showers that produce less than 10 meteors per hour at the time of maximum activity.
Sporadic Meteor: a meteor that occurs randomly, instead of being associated with a meteor shower. There are about 5 per hour in the night sky (peak viewing time is in the autumn before morning twilight).


Most meteors occur in the upper mesosphere and lower thermosphere (from about 50 to 75 miles or 80 to 120 km altitude). This is a general guideline only, since very fast meteors may first become visible above this height, and slow, bright meteors may penetrate below this range. Meteors were once thought to be a purely atmospheric phenomena. It was not until the mid-1800's that the extra-terrestrial origin of meteors was widely recognized.

When a meteoroid plunges into the atmosphere at a velocity of between 25,000 mph and 160,000 mph (11 and 72 km/sec), the air does not have time to flow around the meteoroid. The result is that friction produces enough heat to ablate (vaporize) the meteoroid and to ionize air molecules, producing a highly charged plasma. The ions quickly recombine and energy is released as light. The whole process usually takes a few tenths of a second and so a meteor appears as a moving streak of light. (The light streak is not just the glowing hot meteoroid itself.)

The wide range in meteoroid speeds is caused partly by the fact that the Earth itself is traveling at about 67,000 mph (30 km/sec) as it revolves around the sun. On the evening side, or trailing edge of the Earth, meteoroids must catch up to the earth's atmosphere to cause a meteor, and tend to be slow. On the morning side, or leading edge of the earth, meteoroids can collide head-on with the atmosphere and tend to be fast.

Internet Resources

The American Meteor Society has a good FAQ page
Gary Kronk's Meteor site
Windows to the Universe meteors page
IPS Radio & Space Services
Anomalous meteor phenomena (UFO's, perhaps?)
Long Duration Exposure Facility - meteoroid impacts on exposed hardware in low earth orbit

Pictures of meteorite types in Ellie Crystal's Meteors-Meteorites page
The Meteorite Market for more details and pictures; also offers meteorites for sale
The Peekskill meteorite and videos of the meteor
Antarctic Meteorites
Impact Craters (whence landed some really big meteorites)
The Tunguska event of 1908
Chelyabinsk meteor

The asteroid impact theory of dinosaur extinction
A volcano theory of dinosaur extinction

The Meteor of 1860 inspired poet Walt Whitman as well as the title of a book about the 1860 Presidential election.

Major Annual Meteor Showers

Date of Peak DisplayName of Shower
Jan 3-4 Quadrantids
Apr 21-22 April Lyrids
May 4-5 Eta Aquarids
Jul 28-29 Delta Aquarids
Aug 12-13 Perseids
Oct 21-22 Orionids
Nov 3-13 Taurids
Nov 16-17 Leonids
Dec 13-14 Geminids *
Dec 21-22 Ursids
* The Geminids are known to be of asteroidal (3200 Phaethon) origin rather than of cometary origin.