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Darcy Pattison - Eclipse: How the 1919 Solar Eclipse Proved Einsteins Theory of Relativity

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Darcy Pattison Eclipse: How the 1919 Solar Eclipse Proved Einsteins Theory of Relativity
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Eclipse: How the 1919 Solar Eclipse Proved Einsteins Theory of Relativity: summary, description and annotation

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In 1915, British astronomer Arthur Stanley Eddington was fascinated with Einsteins new theory of general relativity. The theory talks about how forces push and pull objects in space. Einstein said that the suns gravity could pull and bend light.
To test this, astronomers decided to photograph a solar eclipse. The eclipse would allow them to photograph the stars before and during the solar eclipse. If the stars position moved, then it was evidence that that light had bent. Eddington and his team traveled from England to the island of Principe, just off the African coast, to photograph the eclipse.
In simple language, this nonfiction illustrated picture book explains how the push (acceleration) and pull (gravity) of space affects light. Back matter includes information on Einstein, Eddington, and the original photograph of the 1919 solar eclipse.

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cover ECLIPSE How the 1919 Solar Eclipse Proved Einsteins Theory of General Rela - photo 1
ECLIPSE How the 1919 Solar Eclipse Proved Einsteins Theory of General Rela - photo 2
ECLIPSE: How the 1919 Solar Eclipse Proved Einsteins Theory of General Rela vity
Wri en by Darcy Pa son
Illustrated by Peter Willis
Text copyright 2019 by Darcy Pa son.
Illustra ons copyright 2019 by Mims House.
All rights reserved.
Publishers Cataloging-in-Publica on Data
Names: Pa son, Darcy, author. | Willis, Peter, illustrator.
Title: Eclipse : how the 1919 solar eclipse proved Einsteins theory of general rela vity / wri en by Darcy
Pa son and illustrated by Peter Willis.
Series: Moments in Science
Descrip on: Li le Rock, AR: Mims House, 2019.
Summary: Bri sh astronomer Arthur Stanley Eddington photographed the 1919 solar eclipse to prove
Einsteins theory of general rela vity by demonstra ng that the suns gravity could pull and bend light.
Iden ers: ISBN 9781629441252 (hardcover) | 9781629441269 (paperback) | 9781629441276 (ebook)
Subjects: LCSH General rela vity (Physics)--Juvenile literature. | Rela vity (Physics)--Juvenile literature. |
Gravity--Juvenile literature. | Gravita on--Juvenile literature. | Solar eclipses--1919--Juvenile literature. |
Eddington, Arthur Stanley, Sir, 1882-1944--Juvenile literature. | Einstein, Albert, 1879-1955--Juvenile liter-
ature. | Astrophysics--History--20th century--Juvenile literature. | Physics--History--20th century--Juvenile
literature. | Astronomy--History--20th century--Juvenile literature. | BISAC JUVENILE NONFICTION /
Science & Nature / Physics | JUVENILE NONFICTION / Science & Nature / History of Science
Classi ca on: LCC QC173.585 .P38 2019 | DDC 530.11--dc23
SOURCES:
Dyson, F. W., A.S. Eddington, and C. Davidson. A Determination of the Deflection of Light by the Suns Gravitational Field, from
Observations Made at the Total Eclipse of May 29, 1919. Philosophical Transactions of the Royal Society of London. Series A, Con-
taining Papers of a Mathematical or Physical Character, Vol. 220 (1920), pp. 291-333. http://www.jstor.org/stable/91137
Kennefick, Daniel. Not Only Because of Theory: Dyson, Eddington and the Competing Myths of the 1919 Eclipse Expedition.-
Paper presented at the 7th Conference on the History of General Relativity, Tenerife, Spain, 2005. https://arxiv.org/ftp/arxiv/
papers/0709/0709.0685.pdf.
Kennefick, Daniel. Personal letter and emails to author, April 2019.
Its a scientific fact During a rainstorm you cant see the sun the - photo 3
Its a scientific fact . During
a rainstorm , you cant see
the sun , the moon , or
the stars . Or a solar eclipse .
WHAT IS AN ECLIPSE During an eclipse the moons shadow makes part of the - photo 4
WHAT IS AN ECLIPSE During an eclipse the moons shadow makes part of the - photo 5
WHAT IS AN ECLIPSE ?
During an eclipse , the moons shadow
makes part of the earth dark . As the
moon travels across the suns path ,
the sun looks like a shrinking crescent .
Finally , the sun is totally black with only
a corona , or glowing light , around the
edge . When the sun is totally blocked
by the moon , its called the totality .
Totality only lasts a couple of minutes .
As the moon keeps moving , the sun is
a growing crescent un l the moon has
completely passed . To see an eclipse ,
you must travel to the places where the
moons shadow falls . And hope the skies
are clear .
British astronomer or star scientist Stanley Eddington needed to see - photo 6
British astronomer or star scientist Stanley Eddington needed to see - photo 7
British astronomer , or star
scientist , Stanley Eddington
needed to see the May ,
1919 solar eclipse . He planned
to photograph distant stars
during the eclipse and change
science forever .
SIR ARTHUR STANLEY
EDDINGTON ( 1882 1944 ),
known as Stanley , was a Brish
astrophysicist , a scienst who studies
the stars and physics . A Quaker ,
he was a conscienous objector
to World War I . He was excused
from military service because of his
astronomy work . Stanley was the
head of the Cambridge Observatory .
He joined Frank Dyson , the director
of the Greenwich Observatory , to
plan an expedion to Prncipe Island
to photograph the 1919 solar eclipse .
Stanley was also known for his work
on what makes up the insides of
stars , the luminosity of stars , and
other theories .
His plans to photograph the 1919 solar eclipse started four years earlier - photo 8
His plans to photograph the 1919 solar eclipse started four years earlier - photo 9
His plans to photograph
the 1919 solar eclipse
started four years
earlier . German scientist
Albert Einstein was
studying how forces
objects in space . On
November , 1915 ,
Einstein explained to other
scientists his new theory
of general relativity .
and
and
WHAT IS A THEORY?
A theory is an explana on of
something in science . When
a theory is rst developed , it
might later be proved to be a
scien c fact , or not . A theory
needs observa ons , experiments ,
and other evidence to prove it .
Developing and tes ng theories is
what science is all about .
Earth Path of starlight Real location of star A pparent location of star - photo 10
Earth
Path of starlight
Real location
of star
A
pparent
location
of star
Gravity is a force that p u l l s an object toward another object At the - photo 11
Gravity is a force that p
u l l s an object toward
another object .
At the time , scientists
thought that light traveled
in a straight line . But
Einstein said something
startling . He said that the
suns huge gravity pulled
and bent light . To prove
his new theory , he needed
observations from an
astronomer like
Stanley Eddington .
u l l s
EXAMPLE OF GRAVITY
Earth has a strong gravity . If you
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