Title: Stars
1Stars Temperature
- Hotter objects emit shorter wavelengths
- Cooler objects emit longer wavelengths
- Ex. Sun is a medium hot (5800 K or about 5500
C) star and emits X-rays - Cooler stars emit infrared
- Determining surface temperature by maximum
emitted wavelength (Wiens Law) - NOTE 0 degrees Celsius 273 Kelvin
- -273 degrees Celsius 0 Kelvin
2Stars Color
- 25,000 K star looks blue
- 6,000 K star looks yellow (like our sun)
- 3,000 K star looks red
- Chemical composition of burning gas
- Determined by passing light through a prism to
generate a spectrum - Light passed through nebula may have absorption
lines - Ex. Sun is 74 Hydrogen, 25 Helium, 1 Other
- Spectral Class combination of temperature and
chemical composition - Signified by a letter O, B, A, F, G, K, M
(hottest to coolest) - Our sun is G2
3Stars Finding Distance by Brightness
- Why do you think stars would be different
brightness levels? - Apparent Brightness combination of energy
emitted and distance from Earth, brightness
decreased by square of distance. - Intrinsic Brightness known as LUMINOSITY,
measured in watts. - If you know the apparent and intrinsic
brightness, you can figure distance.
4Star Evolution
- Group 1 Star Formation Birth (11-1)
- Group 2 Star Energy Helium Fusion
- Group 3 Stellar Structure and Energy Transport
(11-3) - Group 4 Why is there a Main Sequence?
(p.262-267) - Group 5 Post-Main-Sequence Evolution (12-2)
- Group 6 Evidence of Evolution Star Clusters
(12-3)
5Stars Motion Determined by Light
- Doppler Effect Motion of a lights source
affects its observed wavelength of light - Approaching observer, waves compressed, shortened
wavelengths (BLUESHIFT) - Moving away from observer, waves spread out,
lengthened wavelengths (REDSHIFT) - Perpendicular motion to observer does not shift
the wavelength
6Remember that old commercial?
- Draw a person or an ear to represent the
observer. - Animations of Doppler Effect
7EW We are going to be reviewing today for the
final next Monday. Write down what the big
bang theory and evidence for it are.
8Tuesday, June 3rd, 2014
- LT I will be able to discuss the big bang
theory, evidence for it and star life cycles.
- Agenda
- -Review for final next week
- -can use note card on final
- Tomorrow
- -Climate Change
9- Origins
- began with a large explosion called the big bang
theory - only energy before this, no matter
- first hydrogen and helium were formed
- larger elements were formed later by stars
10The Big Bang Theory
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12Big Bang Theory
- Expansion indicates a denser, hotter past
uniform, hot gas that cools as it expands - NOT an explosion from a point, but a simultaneous
expansion from all places - 13.7 billion years ago
13Big Bang
- EVIDENCE
- 1. Cosmic microwave background radiation
noise, same in all directions - 1965 Arno Penzias and Robert Wilson
- 2. Expansion measured by Hubble constant
- Distant galaxies are redshifted (based on
electromagnetic spectrum) - This is the doppler effect being applied to light
- 1929 Edwin Hubble
- 3. most elements in universe are H and He (light
elements) - Created during first moments of Big Bang
- when stars reach the end of their life cycle,
they distribute C, O, and Fe into the universe - if the universe was older, there would be more C,
O, and Fe
14Expanding Universe
- All distant galaxies are redshifted. What does
this mean about their distance from us? - Hubble Law further away a galaxy is, the faster
it is speeding away - If we can determine how fast the universe is
expanding (aka Hubble constant), we can determine
the AGE OF THE UNIVERSE!
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16- Continuation of Expanding Universe
- is expanding, therefore must have been smaller
at one point - evident by galaxies red shift
- most look red because they are moving away from
us - if they were moving towards us, they would look
bluer (blue shift)
17Observers looking at an object that is moving
away from them see light that has a longer
wavelength than it had when it was emitted (a
redshift), while observers looking at an
approaching source see light that is shifted to
shorter wavelength (a blueshift).
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19Cosmic background radiation
- scientists found noise in our galaxy that was
the cosmic microwave background radiation
predicted by the Big Bang theory - The radiation can only be detected with a radio
telescope which makes it show as a faint glow. - Thermal radiation thought to be left over by Big
Bang - Happened 300,000 years after The Big Bang (so
still about 13.7 billion years ago!)
20What is a radio telescope?
- Radio waves are a form of electromagnetic
radiation, just like visible light! - How they work?
- -waves bounce off a radio telescope, with this
information computers can make images of the sky!
21Can make images like this of our Universe!
22New Evidence!
- Theory of inflation
- -first proposed in 1980s but recently found
evidence for it! - -Found evidence that the universe was expanding
exponentially seconds after the Big Bang
23Life Cycle of Stars
- Our sun is an average star in our solar system!
- life cycle varies depending on the size
- For most stars, 90 of life cycle is spent fusing
hydrogen that turns into helium - all begin life inside a huge cloud of gas (mostly
hydrogen) and dust called a nebula
24When an average star ends its life cycle!
- hydrogen fusion stops
- Fusing of helium begins to create heavier
elements (like oxygen, iron) - no more energy exploding outward
- gravity pulls matter inwards
- First makes a large red giant
- outer layers often expand and drift away creating
a planetary nebula - VERY high density, bright, and is called a white
dwarf
25Life cycle of Larger Stars
- for larger stars
- elements up to iron are fused together
- eventually may turn into a supernova
- quickly collapses because run out of energy and
gravity is now the strongest force - core collapses and then rebounds outward with a
shock wave that makes a bright explosion
(supernova) - at this point, the heavier elements are finally
created - if the leftover core is very, very dense, it may
form a very small neutron star or a black hole
with VERY powerful gravity
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27Cosmology
- How did the cosmos begin, and what will happen to
it? - Study of the history and future of the universe
- Universe everything that exists in space and
time