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03 Oct 2000 ASTR103, GMU, Dr. Correll 1
Ch 8--Asteroids, Meteors, CometsCh 8--Asteroids, Meteors, Comets
03 Oct 2000 ASTR103, GMU, Dr. Correll 2
What do you think?What do you think?
• Are the asteroids a planet that was somehow destroyed?
• How far apart are the asteroids on average?• Why do comets have tails?• In which direction does a comet tail point?• What is a shooting star?
03 Oct 2000 ASTR103, GMU, Dr. Correll 3
Early Solar SystemEarly Solar System
• From studying cratering on the Moon and the planets– First half-billion
year had many collisions between planetesimals
– More recently the collisions are much less frequent, but do occur!
03 Oct 2000 ASTR103, GMU, Dr. Correll 4
AsteroidsAsteroids
• Asteroids:– remnant planetesimals
• also known as “minor planets”
– mainly concentrated in the asteroid belt between Mars and Jupiter--about 10 million miles average separation
– Mostly stony or metallic in composition
03 Oct 2000 ASTR103, GMU, Dr. Correll 5
AsteroidsAsteroids
• 1801--Piazza discovers Ceres--the first asteroid
03 Oct 2000 ASTR103, GMU, Dr. Correll 6
Asteroids--OriginsAsteroids--Origins
• A destroyed planet?– Probably not
• Jupiter’s gravity creates “resonances” which create bands of stable orbits and gaps of unstable orbits– Kirkwood gaps
discovered 1867
03 Oct 2000 ASTR103, GMU, Dr. Correll 7
Asteroids outside the beltAsteroids outside the belt
• Gravitational perturbations eject comets from the belt into elliptical orbits– Some approach the inner planets– “Apollo” asteroids cross the Earth’s orbit
• Near-Earth Objects (NEOs)
• Near-Earth Asteroids (NEAs)
• Potentially Hazardous Objects (PHOs)
03 Oct 2000 ASTR103, GMU, Dr. Correll 8
CometsComets
• Comets--best thought of as “dirty snowballs” orbiting the Sun which evaporate due to solar heating
03 Oct 2000 ASTR103, GMU, Dr. Correll 9
Comets OriginsComets Origins
• Primordial gas, dust, and ice frozen in clumps at the outer limits of the solar system– Kuiper belt--out to 500
AU– Oort Cloud--50,000
AU
• Occasionally perturbed into elliptical orbits approaching the Sun
03 Oct 2000 ASTR103, GMU, Dr. Correll 10
Parts of a CometParts of a Comet
• Coma--spherical cloud of vaporized gas around the frozen nucleus
• Tails--trail of debris– dust tail--dust
particles blown away by solar radiation
– ion tail--ions carried away by solar wind
03 Oct 2000 ASTR103, GMU, Dr. Correll 11
Parts of a CometParts of a Comet
• Tails always point away from the Sun!
03 Oct 2000 ASTR103, GMU, Dr. Correll 12
Comets DemiseComets Demise
• Comets eventually– breakup into smaller fragments (Comet West below)– evaporate– collide with the sun– collide with other planets
03 Oct 2000 ASTR103, GMU, Dr. Correll 13
Comets DemiseComets Demise
03 Oct 2000 ASTR103, GMU, Dr. Correll 14
Comets DemiseComets Demise
03 Oct 2000 ASTR103, GMU, Dr. Correll 15
Meteoroids, Meteors, MeteoritesMeteoroids, Meteors, Meteorites
• Meteoroids--small rocky or metallic particles throughout the solar system
• Meteors--upon entering Earth’s atmosphere, friction causes heat and disintegration--shooting stars
• Meteorites--remnants surviving on the ground
16ASTR103, GMU, Dr. Correll 03 Oct 2000UWO Meteor Group
Earth’sEarth’sLocationLocation
everyeveryNov 17Nov 17
Meteor Showers/Storms--Earth occasionally passes through cometary debris streams leading meteor showers!
Leonid Meteor Shower (Comet Temple-Tuttle stream)
03 Oct 2000 ASTR103, GMU, Dr. Correll 17
MeteoritesMeteorites
• Meteorites--remnants surviving on the ground– Mostly remnants of asteroids
(to have survived entry into Earth’s atmosphere)
• Stony meteorites
• Iron meteorites
– Show melting and wearing patterns from processing in asteroids
– Carbonaceous Chondrites show no melting
• may be primordial components of solar system
• contain organic material!
03 Oct 2000 ASTR103, GMU, Dr. Correll 18
Dino Killers?Dino Killers?
• Evidence for large impact 65 Million years ago
• Alvarez theory of K-T boundary
• Impact crater evidence found off north shore Yucatan at Chixulub
03 Oct 2000 ASTR103, GMU, Dr. Correll 19
More Recent EventsMore Recent Events
• Peekskill 1993– ~1m size
• Tunguska 1908– ~ 1/2 km size– 2200 sq km area
• Meteor Crater– 30,000 BCE– 1.2 km crater– 30 m meteor
03 Oct 2000 ASTR103, GMU, Dr. Correll 20
Planetary Defense?Planetary Defense?
Easy to study; expensive to carry out!
03 Oct 2000 ASTR103, GMU, Dr. Correll 21
What do you think?What do you think?
• Are the asteroids a planet that was somehow destroyed?– No, the gravitational pull of Jupiter prevented the planetesimal in the
asteroid belt to coalesce into planet
• How far apart are the asteroids on average?– The distance between asteroids averages about 10 million miles
• Why do comets have tails?– Gas and dust evaporated from the comet nucleus are blow away by
the solar wind and solar radiation pressure, respectively
• In which direction does a comet tail point?– Gas tails point directly away from the Sun; Dust tails point indirectly
away from the sun in arcs
• What is a shooting star?– A piece of space debris plunging white hot into the Earth’s
atmosphere--a meteor, not a star
03 Oct 2000 ASTR103, GMU, Dr. Correll 22
Questions for ThoughtQuestions for Thought
• Explain the origins of comets and describe the various features seen when near the Sun.