Download Untitled - Dommelroute

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Impact event wikipedia , lookup

Extraterrestrial life wikipedia , lookup

Spitzer Space Telescope wikipedia , lookup

Definition of planet wikipedia , lookup

Aquarius (constellation) wikipedia , lookup

Astronomical unit wikipedia , lookup

Tropical year wikipedia , lookup

IAU definition of planet wikipedia , lookup

Advanced Composition Explorer wikipedia , lookup

Nebular hypothesis wikipedia , lookup

Orrery wikipedia , lookup

Sample-return mission wikipedia , lookup

History of Solar System formation and evolution hypotheses wikipedia , lookup

Panspermia wikipedia , lookup

Beta Pictoris wikipedia , lookup

Timeline of astronomy wikipedia , lookup

Astronomical spectroscopy wikipedia , lookup

Cosmic dust wikipedia , lookup

Comparative planetary science wikipedia , lookup

Oort cloud wikipedia , lookup

Star formation wikipedia , lookup

Solar System wikipedia , lookup

Formation and evolution of the Solar System wikipedia , lookup

Directed panspermia wikipedia , lookup

Transcript
THIS PAGE
LEFT BLANK
INTENTIONALLY
This book is dedicated to Calli and Cori Neal.
Seven Wonders of Asteroids, Comets, and Meteors
Copyright © 2011 by Ron Miller
2
All rights reserved. International copyright secured. No part of this book may be reproduced, stored in a retrieval
system, or transmitted in any form or by any means—electronic, mechanical, photocopying, recording, or otherwise—
without the prior written permission of Lerner Publishing Group, Inc., except for the inclusion of brief quotations in
an acknowledged review.
Twenty-First Century Books
A division of Lerner Publishing Group, Inc.
241 First Avenue North
Minneapolis, MN 55401 U.S.A.
Website address: www.lernerbooks.com
Library of Congress Cataloging-in-Publication Data
Miller, Ron, 1947–
Seven wonders of asteroids, comets, and meteors / By Ron Miller.
p. cm. — (Seven wonders)
Includes bibliographical references and index.
ISBN 978–0–7613–5451–2 (lib. bdg. : alk. paper)
1. Asteroids—Juvenile literature. 2. Comets—Juvenile literature. 3. Meteors—Juvenile literature. I. Title.
QB651.M553 2011
523.5—dc22
2010015559
Manufactured in the United States of America
1 – DP – 12/31/10
eISBN: 978-0-7613-7279-0
Contents
Introduction —— 4
CERES —— 7
GANYMED AND OTHER
EARTHGRAZERS —— 17
HALLEY’S COMET —— 23
BOREALIS BASIN —— 35
THE PERSEID METEOR SHOWER —— 45
THE KUIPER BELT —— 55
PLUTO
AND
CHARON —— 65
Ceres
Timeline —— 72
Choose an Eighth Wonder —— 73
Glossary and Pronunciation Guide —— 74
Source Notes —— 75
Selected Bibliography —— 76
Further Reading and Websites —— 76
Index —— 78
3
INTRODUCTION
P
EOPLE LOVE TO MAKE LISTS OF THE BIGGEST
AND THE BEST. ALMOST TWENTY-FIVE HUNDRED YEARS AGO, A
WRITER NAMED
HERODOTUS
GREEK
MADE A LIST OF THE MOST AWESOME
THINGS EVER BUILT BY PEOPLE.
THE
LIST INCLUDED BUILDINGS,
STATUES, AND OTHER OBJECTS THAT WERE LARGE, WONDROUS, AND
IMPRESSIVE.
WRITERS
LATER,
OTHER WRITERS ADDED NEW ITEMS TO THE LIST.
EVENTUALLY AGREED ON A FINAL LIST. IT WAS CALLED THE
SEVEN WONDERS
OF THE
ANCIENT WORLD.
The list became so famous that people began imitating it. They made
other lists of wonders. They listed the Seven Wonders of the Modern
World and the Seven Wonders of the Middle Ages. People even made lists
of undersea wonders and the wonders of science and technology.
But Earth doesn’t contain all the wonders that have been discovered.
Our planet shares the solar system with many other worlds. They all have
wonderful things to see.
THE BUILDING BLOCKS
OF THE SOLAR SYSTEM
After a house is built, a big pile of material is always left over. The same
thing happened after the formation of the solar system. The Sun and the
planets were formed from a huge cloud of dust and gas. This dust and
gas came together to form tiny clumps of rock, metal, and ice. These tiny
clumps gathered into bigger clumps. After millions of years, these clumps
were large enough to become the Sun and the planets.
4
The asteroid belt in the solar system is made up of the orbiting pieces of rock, ice, and metal left over
after the planets and the Sun formed. This illustration shows a view of the Sun from an asteroid.
Not all the matter in the original dust cloud was used up. Chunks of rock,
metal, and ice were left over. These are what we call asteroids and comets and
meteors. They are important wonders because they are remnants of the very
earliest beginnings of our solar system.
5
Other asteroids have even more unusual shapes. For instance, 4179
Toutatis and 1620 Geographos are shaped like rounded-off boxcars. On
the other hand, 216 Kleopatra looks like a dog bone, and 4769 Castalia
resembles a hamburger bun.
An even more interesting asteroid is 624 Hektor. It is shaped like two
beach balls just touching each other. It is probably the result of two asteroids
colliding. But the collision was a gentle one. Instead of hitting so hard they
shattered, the two asteroids stuck together. Visiting Hektor would be a weird
experience. If you were to hike to the contact region, you would see a
mountain of rock 93 miles (150 km) high hanging directly over your head!
Astronomers have discovered asteroids with many unusual shapes. The asteroid 216 Kleopatra
resembles a dog bone.
Seven Wonders of Asteroids, Comets, and Meteors
Originally there was only an enormous cloud of dust and gas. This cloud was
large enough that the pull of the gravity on its particles started shrinking the cloud.
As it shrank, the particles grew closer together. This increased the gravitational
pull, which made the particles pull together even faster. The dust and the gas were
densest in the center of the cloud. As this material became compressed, it heated
up. Eventually it was hot enough to create a new star, the Sun.
Within the cloud surrounding the new sun, tiny particles of dust collided
and stuck together, forming clumps of material. As these clumps—called
planetesimals—grew in size, they attracted more particles. Most of these early
collisions were relatively gentle, so the planetesimals didn’t knock themselves
into pieces. Soon grains of dust grew to the size of rocks. Then the rocks
grew into boulders and then into asteroids miles across. The whole process
of growing from the size of a large pinhead to a mountain may have taken
one hundred thousand years or so. Then the process began to slow down.
The original dust and gas had been used up, and the cloud thinned. Several
stars—such as Beta Pictoris—have been observed with large, thin disks of dust
surrounding them. These may be solar systems at this stage of development.
14
This composite image
of the star Beta
Pictoris shows a large
disk of dust around
the star. It may
be that this star is
another solar system
more than ifty light
years from Earth.
A light year is the
distance light travels
in a year—5.9 trillion
miles (9.5 trillion
km).