cornell notes
DESCRIPTION
Cornell Notes. TITLE. This column gets filled out LATER! Can be key questions about notes used as study questions for test Can also be questions about things you did not understand. Notes will go here from my PowerPoints Bulleted or outlined information works best - PowerPoint PPT PresentationTRANSCRIPT
![Page 1: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/1.jpg)
Cornell Notes...TITLE
•This column gets filled out LATER!•Can be key questions about notes-used as study questions for test•Can also be questions about things you did not understand
•Notes will go here-from my PowerPoints•Bulleted or outlined information works best-Try not to use long sentences-Avoid paragraphs•Use abbreviations YOU understand
![Page 2: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/2.jpg)
A helpful guide...
FOR THESE NOTES ONLY...
I’m going to include some helpful hints on how I organize my notes.
They will be in small boxes off to the side, in bright blue font.
Don’t write those things down.
![Page 3: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/3.jpg)
Formation of the Universe
Formation of the Universe
Credit: NASA / WMAP Science Team
![Page 4: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/4.jpg)
Cosmology• The study of the universe
• Its current nature
• Its origin and evolution
Key vocabulary is bolded and
underlined. These are very
important!
Big ideas or topics are at
the top. These should be your sub-
headings, with your
bullets following
below
![Page 5: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/5.jpg)
The Universe• Universe is expanding
• Which means it had to have a beginning.
![Page 6: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/6.jpg)
How the Universe Began
• Theories of how the universe began:
• Steady State Theory
• Big Bang Theory
• Inflationary Model
Usually when I give you lists like this, we will discuss each of them in class. You probably do NOT
need to write anything but the title
down.
![Page 7: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/7.jpg)
Steady State Theory
• Proposes that the universe looks the same on large scales, and has always looked that way
• Universe does not change with time
• BUT! If the universe is expanding, how can this be true?
• New matter is created and added to the universe as it expands The italicized
question does NOT need to be written
down. It’s just something to think
about.
![Page 8: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/8.jpg)
Big Bang Theory
• NOT an explosion into space
• IS an expansion of space with matter along for the ride
![Page 9: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/9.jpg)
The Big Bang Model
• Consists of a competition between:
• Outward momentum of expansion
• Inward force of gravity
• This is how the universe acts to slow the expansion
![Page 10: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/10.jpg)
B.B.T. - Outcomes of Expansion• Three outcomes for the universe:
• Open Universe
• Expansion never stops
• Closed Universe
• Expansion will stop and turn into contraction
• Flat Universe:
• Expansion will slow to a halt in an infinite amount of time, but never contract
If there is information
written under each bullet in a list, then this is info
you should probably have in
your notes.
![Page 11: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/11.jpg)
Inflationary Model
• Version of the Big Bang Model
• Universe began as a fluctuation in a vacuum
• Expanded very rapidly for a fraction of a second
• Settled into a more orderly expansion
![Page 12: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/12.jpg)
Research of Theories
• Many observational tests can be done to provide support for all theories
• Today, evidence weighs in favor of the Big Bang Theory
![Page 13: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/13.jpg)
B.B.T. - Present Day
• Appears that the rate of expansion slowed for awhile, but is now gathering speed
• What is causing this?
• Some scientists suggest it is caused by an unknown force
• Stronger than gravity
• Pushing galaxies apart
![Page 14: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/14.jpg)
Looking Back
• A trip through space and time to put the B.B.T. in perspective.
• Journey to the Big Bang
Credit: NASA / WMAP Science Team
![Page 15: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/15.jpg)
Formation of Our Galaxy
Formation of Our Galaxy
Hubble image: NASA and ESA
![Page 16: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/16.jpg)
Stars and Planets• Formed from interstellar clouds
• Clouds of dust and gas
• Mostly hydrogen and helium gas
• Many interstellar clouds are observed along the Milky Way
• Have low density
• This means their materials are very spread out
• BUT they can condense because of gravity
• Eventually becomes stars and possibly planets
• Hypothesis on how our solar system was created!
![Page 17: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/17.jpg)
Collapse of the Cloud
• Very slow at first
• Speeds up and starts rotating as it collapses
• Becomes a rotating disk (solar nebula)
• Center of the disk (densest part) eventually becomes the Sun
• As the disk cooled, different elements were able to form in solid and liquid states
![Page 18: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/18.jpg)
Growth of Objects
• As condensing slowed, small particles started to accumulate
• These began to merge together to make larger ones
• Eventually became hundreds of kilometers in diameter
• Called planetesimals
![Page 19: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/19.jpg)
Planetesimals• Continued to grow and merge with others
• Merges were violent
• Sometimes planetesimals were destroyed
• Overall result was a small number of large bodies (planets)
![Page 20: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/20.jpg)
The Planets• Jupiter formed first
• Continued to grow
• Saturn was next
• Then the other gas planets
• None of the planets could get as big as Jupiter because it already had so much of the galaxy’s material
![Page 21: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/21.jpg)
Asteroid Belt• Actually just planetesimals that never merged
• Stayed between Mars and Jupiter
• Jupiter’s gravitational force prevented them from merging.
• Asteroid - rocky remnant of the early system
• A few kilometers to 1000 kilometers in diameter
![Page 22: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/22.jpg)
Meteoroid, Meteor,
Meteorite• Meteoroid - any interplanetary object that falls and enters Earth’s atmosphere
• Meteor - a meteoroid that burns and produced a streak of light.
• Meteorite - a meteoroid that does not burn up completely and part of it hits the ground.
![Page 23: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/23.jpg)
Comets• Small bodies with highly eccentric orbits around
the Sun
• Made of ice and rock
• 1-10 km in diameter
• Two major clusters of comets:
• Kuiper Belt - close to Pluto (30-50 Astronomical Units (AU))
• 1 AU = 149,600,000 km
• Oort Cloud - 100,000 AU from the Sun
![Page 24: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/24.jpg)
Comets (continued)
• When we see comets, it’s because they are within 3 AU of the Sun
• Start of evaporate, forming a head and tail
• Hale Bopp - last seen in 1997 - will be seen again in 4397
• Periodic Comets - those that repeatedly orbit into the inner solar system
• Halley’s Comet - last seen in 1985-86 - will be seen again in 2061 - has a 76 year period
![Page 25: Cornell Notes](https://reader036.vdocuments.us/reader036/viewer/2022062301/5681511c550346895dbf3b3f/html5/thumbnails/25.jpg)
Meteor Shower• When Earth intersects a cometary orbit