a history of the universe astronomy 315 professor lee carkner lecture 2
TRANSCRIPT
A History of the Universe
Astronomy 315Professor Lee
CarknerLecture 2
Practice Observing
Write your name (clearly!) at the top of each exercise!
Label all constellations and bright stars
Always face due N or S Always fill in completely Object,
Location, Date and Time and Notes
Our Place in the Universe Before we look at the history of the
universe, we will look at our place in it
We now realize that we occupy no unique or special place in the universe
After Nicolaus Copernicus who theorized that the sun, and not the Earth, was the center of the solar system
So where are we?
The Solar System
Where Do We Fit In? We can think about our position in the universe in
terms of scale Planet is in a planetary system around a star (Solar
System) Galaxy is in a cluster (Local Group)
Supercluster is in a (the?) universe Each “step up” is a huge increase in size
Scale Models
We want to make a scale model to try to understand astronomical distances
Need to find the scale
example: miles per inch or light years per cm
Once you have the scale you can find the model size for any real object
(model size) = (real size) / scale
The Big Bang
The best model for the beginning of the universe is the hot big bang model
Key points: The early universe was very hot Th
Why do we believe this? The universe looks like it is expanding from a
hotter, denser state
About the Big Bang We can see the expansion of the universe
and the glow of the early hot universe
The universe has a beginning but no center or edge
The universe is not really like any macroscopic object we are familiar with
The First Three Minutes What was the early universe like?
What do we know?
Universe consists of photons and subatomic particles (like quarks)
Universe went through an early period of very rapid expansion called inflation
Cooled to the point where atoms could form after about 1 million years
Formation of Structure After about 1 billion years the universe is a
big ball of atoms and photons
Why?
This is why we have matter organized into stars, galaxies and clusters of galaxies, instead of a big uniform cloud of stuff
The Early Stars The first stars were made out of hydrogen
and helium, the two simplest elements
Nuclear reactions inside the stars produced heavier elements
Most of the universe (80%) is still hydrogen, however
Stellar Products The next generation of stars had small
amounts of these heavier elements in them
When any star dies it leaves behind a burned out core
Collectively known as compact objects
Composition of the Universe
Galaxies made up of: “Normal” stars (maybe with planets) Gas (hydrogen) and dust (heavier
elements)
The Future What effects the future of the universe? Mass
If universe has enough mass, gravity might stop expansion
Dark energy
If there is enough dark energy it might rip universe apart
The Fate of the Universe Possible ends for the universe Big Crunch
Gravity pulls universe back into a point source
Big Rip Dark energy rips universe apart
Big Chill Universe expands forever
Next Time
Read Chapter 1.1-1.5 Meet in Planetarium on Friday!