Chapter 1 Here and Now - mymission.lamission.edu CH 1.pdf · beyond these boundaries and help you...

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.