The Cosmic Perspective Chapter 12 Lecture 27

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26 Terms

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Jupiter nudges the asteroids through the influence of

Orbital Reasonance

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Can an asteroid be pure metal?

Yes, it must have been the core of a shattered asteroid

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Did a large terrestrial planet ever form in the region of the asteroid belt?

No, because Jupiter prevented one from accreting

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What does Pluto most resemble?

a comet

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How big an object causes a typical shooting star?

a grain of sand or a small pebble

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Which have the most elliptical and tilted orbits?

Oort cloud comets

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Which are thought to have formed farthest from the Sun?

Kuiper belt comets

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About how often does a 1-kilometer object strike the Earth?

every million years

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What would happen if a 1-kilometer object struck the Earth?

It would cause widespread devastation and climate change.

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Measuring Asteroid Properties

Size

Shape

Mass

Density

Composition

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Size

few to hundreds of km radius

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Shape

potatoes to spheres

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Mass

how to measure

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Density

Low like Rubble Piles

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Composition

Spectra of Rocky vs Metallic vs Carbon Rich

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What causes these 'gaps' in the asteroid belt?

Orbital resonances

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orbital Resonances & the asteroid belt

resonances with Jupiter stir up asteroid belt:

makes orbits elliptical,

causes collisions, clears gaps

•Prevented a terrestrial planet from forming there

•Most original mass accreted onto other planets

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Rules for Resonances

similar in mass = a bit elliptical

Massive = Hardly ever changes, other orbit can get VERY elliptical

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Types of Metorites

Primitive

Processed

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Primitive Meteorites

Raw materials from solar nebula

Most Stony with some metals

Some dark carbon rich some with water

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Primitive Meteorites characteristics

Stony with metallic flakes

Carbon rich with H2O

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Where do PRIMITIVE METEORITES come prom

Inner and outer regions of asteroid belt

The remains of the birth of solar system

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Processed Meteorites characteristics

Iron rich like earth's core

Stony like earth's mantle or crust

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Processed Meteorites

Significantly changed since solar system formation

Some metallic like terrestrial planet cores

From a differentiated body

Others are rocky, mantle-like, some basalts

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Where do PROCESSED METEORITES come from

Once part of a larger object

From core of shattered Asteroid

From Mantle, crust, or surface of astroid

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History of an Iron Meteorite

1) Iron formed in stars/stellar explosions

2)The solar nebula formed

3)Rock and metal condensed

4)Particles accreted into a small terrestrial world (but rock & metal were mixed together)

5)Differentiation separated rock & metal

6)A collision shattered the object

7)Orbital resonances nudged the fragments onto collision courses with Earth

8)An iron meteorite fell to Earth*