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Chapter 1
Here and Now
Michael Seeds
Dana Backman
The longest journey
begins with a single step.
- Lao Tse
• You are about to go on a
voyage to the limits of the
known universe.
• You will travel outward, away from your
home on Earth, past the moon and the sun
and the other planets of our solar system,
past the stars you see in the night sky, and
beyond billions more stars that can be
seen only with the aid of telescopes.
• You will visit the most distant
galaxies—great globes and whirlpools
of stars.
• Then, you will continue on, carried only
by experience and imagination,
seeking to understand the structure of
the universe.
• Astronomy is more than the study
of planets, stars, and galaxies.
• It is the study of the whole
universe in which you live.
• Humanity is confined to a small planet
circling an average star.
• The study of astronomy can take you
beyond these boundaries and help you not
only see where you are in the universe, but
understand what you are.
• Your imagination is the key
to discovery.• It will be your scientific space-and-time machine
transporting you across the universe and into the
past and future.
• Go back in time to watch the formation of
the sun and Earth, the birth of the first
stars, and ultimately the creation of the
universe.
• Then, rush into the future to see what will
happen when the sun dies and Earth
withers.
• Although you will discover a beginning to
the universe, you will not find an edge or
an end in space.
• No matter how far you voyage, you will not
run into a wall, but you will discover
evidence that the universe may be infinite.
• That is, it may extend in all directions without
limit.
• Astronomy will introduce you to sizes,
distances, and times far beyond your
usual experience on Earth.
• Your task in the chapter is to grasp the
meaning of these unfamiliar sizes,
distances, and times.
• The solution lies in a single word—scale.
• In this chapter, you will compare
objects of different sizes in order to
comprehend the scale of the
universe.
• You should begin with something
familiar—like the size of yourself and
your surroundings. • The figure shows a region
about 16 meters (52 feet)
across occupied by a
human being, a sidewalk,
and a few trees—all objects
with sizes you can relate to.
• Each picture in the following
sequence shows you a frame or field
of view within the universe that is 100
times wider than the preceding
picture.
• In this figure, your field of view has
increased in size by a factor of 100, and
you can see an area 1.6 kilometers
(1 mile) in diameter.• The arrow points to the
scene shown in the previous
figure.
• Now, you can see an entire college
campus and the surrounding streets
and houses.• This is still the world you
know and can relate to
the scale of your body.
• This figure has a span of 160
kilometers (100 miles).
• This is an infrared photo—in which
healthy green leaves and crops show
up as red.• Your eyes are sensitive to
only a narrow range of
colors.
• As you explore the universe,
you will need to learn to use
a wide range of ‘colors’—from X rays to radio
waves—revealing sights
invisible to your unaided
eyes.
• The college campus is now invisible.
• The patches of gray are towns and cities,
including Wilmington, Delaware, visible in
the lower right corner.
• At this scale, you can see the natural
features of Earth’s surface.• The Allegheny Mountains of southern Pennsylvania
cross the picture at the upper left.
• The Susquehanna River
flows southeast into
Chesapeake Bay.
• What look like white bumps
are actually puffs of clouds.
• Mountains and valleys are only
temporary features on Earth that
are slowly but constantly
changing.• As you explore the universe, you will come to
see that it is also always evolving.
• At the next step in your journey, you
will see the entire planet Earth—about
13,000 km (8000 miles) in diameter.• The picture shows most of
the daylight side.
• The blurriness at the
extreme right is the sunset
line.
• The rotation of Earth on its axis each
24 hours carries you eastward.• As you cross the sunset line into darkness, you say the
sun has set.
• At the scale of this figure, the
atmosphere on which your life depends
is thinner than a strand of thread.
• Enlarge your field of view again by a
factor of 100, and you see a region
1,600,000 km (1 million miles) wide.• Earth is the small blue dot in the center.
• The moon—with a diameter
of only about one-fourth
that of Earth—is an even
smaller dot along its orbit.
• If you had a high-mileage car, it may
have made the equivalent of a trip to
the moon—which has an average
distance from Earth of 380,000
kilometers (240,000 miles).• These numbers are so large that it is
inconvenient to write them out.
•Astronomy is the science
of big numbers.• You will use numbers much larger than these to
describe the universe.
• Rather than writing out these
numbers, it is more convenient to
write them in scientific notation. • This is nothing more than a simple way to write
numbers without writing lots of zeros.
• For example, you would write 380,000 as
3.8 x 105.
• When you once again enlarge your field of
view by a factor of 100, Earth, its moon,
and the moon’s orbit all lie in the small red
box at lower left.
• This figure has a
diameter of
1.6 x 108 kilometers.
• Now, you can see the sun and two
other planets that are part of our solar
system.• Our solar system consists of
the sun, its family of planets,
and some smaller bodies
such as moons, asteroids,
and comets.
• Like Earth, Venus and Mercury are
planets—small, nonluminous bodies
that shine by reflecting light.• Venus is about the size of
Earth and Mercury is
a bit larger than
Earth’s moon.
• In this figure, they
are both too small to
be seen as anything
but tiny dots.
• The sun is a star—a self-luminous ball
of hot gas that generates its own
energy. • The sun is 110 times larger
in diameter than Earth, but
it too is nothing more than
a dot in the diagram.
• Another way astronomers
deal with large numbers is
to define new units.
• The average distance from
Earth to the sun is called the astronomical
unit (AU)—a distance of 1.5 x 108 kilometers
(93 million miles).• For example, you can say,
the average distance from
Venus to the sun is about
0.7 AU.
• Your first field of view was only about
16 meters (52 feet) in width.
• After just six steps, each enlarging by
a factor of 100, you now see the entire
solar system.
• Your view now is 1 trillion (1012)
times wider than in the first figure.• The details of the previous figure are lost in the red
square at the center of this figure.
• You see only the brighter,
more widely separated
objects as you back away.
• The sun, Mercury, Venus, and Earth lie so
close together that you cannot separate
them at this scale.
• Mars, the next outward planet, lies only
1.5 AU from the sun.
• In contrast, Jupiter, Saturn, Uranus,
and Neptune are so far from the sun
that they are easy to find in the figure.• Light from the sun reaches
Earth in only 8 minutes,
but it takes over 4 hours to
reach Neptune.
• Pluto orbits mostly outside
Neptune’s orbit, but it is no
longer considered a major
planet.
• When you again enlarge your field of
view by a factor of 100, the solar
system becomes invisibly small.• The sun is only a point of light,
and all the planets and their
orbits are now crowded
into the small red square
at the center.
• The planets are too small
and reflect too little light
to be visible so near the
brilliance of the sun.
• Nor are any stars visible except for
the sun.• The sun is a fairly typical star, a bit larger than average,
and is located in a fairly normal neighborhood in the
universe.
• Although there are many
billions of stars like the sun,
none is close enough to be
visible in the figure.
• The stars are separated by average
distances about 30 times larger than
this view, which has a diameter of
11,000 AU.
• It is difficult to grasp the isolation
of the stars.• If the sun were represented by a golf ball in New York
City, the nearest star would be another golf ball in
Chicago.
• Now, your field of view has expanded
to a diameter a bit over 1 million AU. • The sun is at the center,
and you see a few
of the nearest stars.
• These stars are so distant
that it is not reasonable
to give their distances in
AU.
• Astronomers have defined a
new larger unit of distance—
the light-year. • One light-year (ly) is the distance that light travels
in one year—roughly 1013 km or 63,000 AU.
• The diameter of your field of view
in the figure is 17 ly.• The nearest star to the sun,
Proxima Centauri, is 4.2 ly
from Earth.
• In other words, light from
Proxima Centauri takes
4.2 years to reach Earth.
• Although stars are roughly the same
size as the sun, they are so far away
that you cannot see them as anything
but points of light.• Even with the largest telescopes on Earth, you still
see only points of light when you look at stars.
• Any planets that might circle those stars are much too
small and faint to be visible.
• In the figure, the sizes of the dots
represent not the sizes of the stars
but their brightness. • This is the custom in
astronomical diagrams,
and it is also how
starlight is recorded.
• Bright stars make larger
spots in a photo or
electronic picture than
faint stars.
• When you expand your field of view by
another factor of 100, the sun and its
neighboring stars vanish into the
background of thousands of other stars. • The field of view is
1,700 ly in diameter.
• No one has ever journeyed thousands
of light-years to look back and
photograph the sun’s neighborhood.• So, this is a representative
picture of a part of the sky
that can be used as a
reasonable simulation.
• The sun is faint enough that
it would not be easily located
in a photo at this scale.
• Some things that are invisible in
this figure are actually critically
important.• You do not see the thin
gas that fills the spaces
between the stars.
• Although those clouds of gas are
thinner than the best vacuum
produced in laboratories on Earth, it
is those clouds that give birth to new
stars.• The sun formed from such a cloud about 5 billion
years ago.
• If you expand your field of view by
a factor of 100, you see our
galaxy. • A galaxy is a great cloud of
stars, gas, and dust bound
together by the combined
gravity of all the matter.
• In the night sky, you see our galaxy
from the inside as a great, cloudy
wheel of stars ringing the sky as the
Milky Way.
• Our galaxy is known
as the Milky Way
Galaxy.
• Of course, no one has
photographed our galaxy.• This figure shows a galaxy similar to our own.
• Our sun would be invisible in such
a picture.• If you could see it, you would find it about two-thirds
of the way from the center to the edge.
• Our galaxy, like many others, has
graceful spiral arms winding outward
through the disk.• You will learn that stars are born in great clouds of
gas and dust as they pass
through these arms.
• The visible disk of our galaxy is
roughly 80,000 ly in diameter.
• Only a century ago, astronomers
thought it was the entire universe—
an island universe of stars in an
otherwise empty vastness.
• Now, Milky Way is known to be not
unique.• It is a typical galaxy in many respects, although larger
than most.
• In fact, ours is only one of many billions of galaxies
scattered throughout the universe.
• As you expand your field of view by
another factor of 100, our galaxy
appears as a tiny luminous speck
surrounded by other specks.• The figure includes a
region 17 million ly in
diameter.
• Each dot represents a
galaxy.
• Our galaxy is part of a cluster of a
few dozen galaxies.• You will find that galaxies
are commonly grouped
together in clusters.
• Some of these galaxies
have beautiful spiral
patterns like our own
galaxy, but others do not.
• The figure represents a view with a
diameter of 1.7 billion light years by
combining observations with theoretical
calculations.
• Clusters of galaxies are connected
in a vast network.• Clusters are grouped into superclusters—clusters of
clusters.
• The superclusters are linked
to form long filaments and
walls outlining voids that
seem nearly empty of
galaxies.
• These appear to be the
largest structures in the
universe.
• Were you to expand your view
frame one more time, you would
probably see a uniform fog of
filaments and voids.• When you puzzle over the origin of these
structures, you are at the frontier of human
knowledge.
• The sequence of figures ends here—
it has reached the limits of the largest
telescopes on Earth.• Our view with the largest
telescopes does not extend
as far as the region that
would be covered by a
figure 100 times larger than
the figure.
• A problem in studying
astronomy is keeping a proper
sense of scale.
• Remember that each of the billions of
galaxies contains billions of stars.
• Many of those stars probably have families
of planets like our solar system.
• On some of those billions of planets,
liquid-water oceans and protective
atmospheres may have sheltered the
spark of life.
• It is possible that some other planets are
inhabited by intelligent creatures who
share your curiosity, wonder at the scale
of the cosmos, and are looking back at
you when you gaze into the heavens.