03 Oct 2000ASTR103, GMU, Dr. Correll1 Ch 8--Asteroids, Meteors, Comets.

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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.