PART I—THE CELESTIAL SPHERE.

[Illustration:

=The Lunar “Crater” Copernicus=

Photographed from Nasmyth and Carpenter's plaster-of-paris model of

the moon.

In this model the topography of the moon is faithfully represented as

seen with powerful telescopes.

]

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Astronomy in a

Nutshell

The Chief Facts and Principles

Explained in Popular Language

for the General Reader

and for Schools

By

Garrett P. Serviss

_=With 47 Illustrations=_

G. P. Putnam's Sons

New York and London

+The Knickerbocker Press+

1912

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COPYRIGHT, 1912

BY

GARRETT P. SERVISS

+The Knickerbocker Press, New York+

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PREFACE

How many thousands of educated people, trained in the best schools, or

even graduates of the great universities, have made the confession: “I

never got a grip on astronomy in my student days. They didn't make it

either plain or interesting to me; and now I am sorry for it.”

The purpose of the writer of this book is to supply the need of such

persons, either in school, or at home, after school-days are ended. He

does not address himself to special students of the subject—although

they, too, may find the book useful at the beginning—but to that vast,

intelligent public for whom astronomy is, more or less, a “mystical

midland,” from which, occasionally, fascinating news comes to their

ears. The ordinary text-book is too overladen with technical details,

and too summary in its treatment of the general subject, to catch and

hold the attention of those who have no special preliminary interest in

astronomy. The aim here is to tell all that really needs to be told, and

no more, and to put it as perspicuously, compactly, and interestingly,

as possible. For that reason the book is called a “nutshell.”

* * * * *

The author has been sparing in the use of diagrams, because he believes

that, in many cases, they have been over-pressed. There is a tendency to

try to represent everything to the eye. This is well to a certain

extent, but there is danger that by pursuing this method too far the

power of mental comprehension will be weakened. After all, it is only by

an intelligent use of the imagination that progress can be made in such

a science as astronomy. The reader is urged to make a serious effort to

understand what is said in the text, and to picture it in his mind's

eye, before referring to the diagrams. After he has thus presented the

subject to his imagination, he may refer to the illustrations, and

correct with their aid any misapprehension. For this reason the cuts,

with their descriptions, have been made independent of the regular text,

although they are placed in their proper connections throughout the

book.

G. P. S.

April, 1912.

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CONTENTS

PART I—THE CELESTIAL SPHERE.

PAGES

Definition of Astronomy—Fundamental Law of the 3-64

Stars—Relations of the Earth to the

Universe—Ordinary Appearance of the Sky—The

Horizon, the Zenith, and the Meridian—Locating

the Stars—Altitude and Azimuth—Circular or

Angular Measure—Altitude Circles and Vertical

Circles—The Apparent Motion of the Heavens—The

North Star and Phenomena Connected with

it—Revolution of the Stars round the

Pole—Locating the Stars on the Celestial

Sphere—Astronomical Equivalents of Latitude and

Longitude—Parallels of Declination and Hour

Circles—“The Greenwich of the Sky”—Effects

Produced by Changing the Observer's Place on the

Earth—The Parallel Sphere, the Right Sphere, and

the Oblique Sphere—The Astronomical Clock—The

Ecliptic—Apparent Annual Revolution of the Sun

round the Earth—Inclination of the Ecliptic to

the Equator: its Cause and its Effects—The

Equinoxes—Importance of the Vernal Equinox—The

Equinoctial Colure—The Solstices—Poles of the

Ecliptic—Celestial Latitude and Longitude—The

Zodiac—The Precession of the Equinoxes: its

Cause and Effects—Revolution of the Celestial

Poles—Past and Future Pole Stars

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