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Transcript
Chapter 1
Our Place in the Universe
Syllabus
• 4 tests: June 18, June 30, July 10, July 21
• Comprehensive Final - check schedule
• Website link on blackboard
1.1 Our Modern View of the Universe
Our goals for learning:
• What is our place in the universe?
• How did we come to be?
• How can we know what the universe was like in the
past?
• Can we see the entire universe?
What happens if you miss a
class?
•
•
•
•
Points will be deducted from your grade
Extra points will not be added to your grade
I will email you a warning
I will miss you
What is my name?
•
•
•
•
•
•
Dr. Allain
Dr. Rhett
Dr. Williams
Dr. Blanchard
Mrs. Moore
Mr. Rhett
Success Tips
• Read the text (it is surprisingly good)
• (read before class)
• Do the online activities - I will give you a
code
• Do the homework in the text
• Discuss with me and others
• Participate in class
• Don’t have the goal of copying everything
Survey Questions
Learning Stuff
•
•
•
•
School is like a gym
I am the trainer
You must do the work
If you are not sore and sweaty, its not a
good workout
My Goals
• Critical Thinking
• Key Ideas in Science:
–
–
–
–
Energy
Light
Matter
Forces
• Historical Perspectives on Science
• The nature of science
What is Farthest from us?
•
•
•
•
The moon
The sun
Jupiter
A star
What is our place in the universe?
Our “Cosmic Address”
Star
A large, glowing ball of gas that generates heat
and light through nuclear fusion
Planet
Mars
Neptune
A moderately large object that orbits a star; it
shines by reflected light. Planets may be rocky,
icy, or gaseous in composition.
Moon (or satellite)
An object that orbits
a planet.
Ganymede (orbits Jupiter)
Asteroid
A relatively small
and rocky object
that orbits a star.
Ida
Comet
A relatively
small and icy
object that
orbits a star.
Solar (Star) System
A star and all
the material
that orbits it,
including its
planets and
moons
Nebula
An interstellar cloud
of gas and/or dust
Galaxy
A great island of stars in space, all held
together by gravity and orbiting a
common center
M31, The Great Galaxy
in Andromeda
Universe
The sum total of all matter and energy;
that is, everything within and between
all galaxies
How did we come to be?
How can we know what the universe was
like in the past?
• Light travels at a finite speed (300,000 km/s).
Destination
Light travel time
Moon
1 second
Sun
8 minutes
Sirius
8 years
Andromeda Galaxy
2.5 million years
• 1 Light year = distance light travels in one year
•At great distances, we see objects as they were
when the universe was much younger.
Can we see the entire universe?
1.2 The Scale of the Universe
Our goals for learning:
•
•
•
•
•
How big is Earth compared to our solar system?
How far away are the stars?
How big is the Milky Way Galaxy?
How big is the universe?
How do our lifetimes compare to the age of the
universe?
The scale of the solar system
• On a 1-to-10 billion
scale:
— Sun is the size
of a large
grapefruit (14
cm)
— Earth is the size
of a tip of a ball
point pen, 15
meters away.
Relative Distance of the Nearest Star
How far away are the stars?
On our 1-to-10 billion scale, it’s just a few minutes
walk to Pluto.
How far would you have to walk to reach Alpha
Centauri?
A.
B.
C.
D.
1 mile
10 miles
100 miles
the distance across the United States
(2500 miles)
How big is the Milky Way Galaxy?
The Milky
Way has
about 100
billion stars.
On the same
ten billion-toone scale…
The Size of the Milky Way
Thought Question
Suppose you tried to count the more than 100 billion
stars in our galaxy, at a rate of one per second…
How long would it take you?
A. A few weeks
B. A few months
C. A few years
D. A few thousand years
•
•
•
•
•
Which of the following is the
correct ordering from largest to
smallest?
Solar System, Milky
Way,
Local Supercluster, Local
Group
Milky Way, Solar System,
Local Group, Local
Supercluster
Local Group, Local
Supercluster, Solar System,
Milky Way
Local Supercluster, Local
Group, Milky Way, Solar
System
Local Supercluster, Milky
Way, Solar System, Local
Group
• Now let’s step through the Universe in powers of 10:
Zooming Out or Zooming In 26 Orders of Magnitude
How do our lifetimes compare to the age
of the Universe?
• The Cosmic Calendar: A scale on which we
compress the history of the universe into 1 year.
How is Earth moving in our solar system?
• Contrary to our perception, we are not “sitting still.”
• We are moving with the Earth in several ways, and at
surprisingly fast speeds.
Earth rotates around its
axis once every day.
Earth orbits the Sun (revolves) once every year…
• at an average distance of 1 AU ≈ 150 million km.
• with Earth’s axis tilted by 23.5º (pointing to Polaris).
• and rotates in the same direction it orbits, counterclockwise as viewed from above the North Pole.
Our Sun moves randomly relative to the other stars
in the local Solar neighborhood…
• at typical relative speeds of more than 70,000 km/hr.
• but stars are so far away that we cannot easily notice
their motion.
… And it orbits the galaxy every 230 million years.
•
How do galaxies move within the universe?
Galaxies are carried along with the expansion of the universe.
But how did Hubble figure out that the universe is expanding?
Hubble discovered that…
• all galaxies outside our Local Group are
moving away from us.
• the more distant the galaxy, the faster it is
racing away.
Conclusion: We live in an expanding universe.
What happens to the raisins in the
Interactive Figure?
•
•
•
•
•
They move apart and get bigger.
They move apart and stay the same size.
They do not move, but they get bigger.
They get closer together and get smaller.
They get closer together and get bigger.
Raisin Cake