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Ch. 14 OUTLINEShorter than book
• 14.1 The Milky Way Revealed
• 14.2 Galactic Recycling (closely related to Ch. 13)
• 14.3 The History of the Milky Way
• 14.4 The Mysterious Galactic Center
14.1 The Milky Way Revealed
• Our Goals for Learning (not exactly like book)
• What does our galaxy look like?
• Where do stars form in our galaxy?
Dusty gas clouds obscure our view because they absorb visible light
This is the interstellar medium that makes new star systems
All-Sky View at visible wavelengths plotted in galactic coordinates
What if we could see through most of that dust?
Remember Extinction and Reddening: interstellar dust will make stars look fainter and redder. Dust will affect more the shorter (bluer) wavelengths and less the longer (redder) wavelengths. By looking at infrared wavelengths we can see through most of the dust.
We see our galaxy edge-on
Primary features: disk, bulge, halo, globular clusters
The Shape of our Galaxy: a flattened disk
How do we know what our galaxy would look like if viewed from the top? Infrared and Radio observations penetrate dark interstellar clouds
Stellar Populations• Turns out that there are two types of stars in
the Galaxy– Population I: Relatively young. Similar to the
Sun. Tend to be in the galactic disk. Richer in heavy elements
– Population II: Few heavy elements, very old (12-14 billion years), tend to be in the center of the galaxy or in globular clusters
Two types of star clusters• Open clusters:
young, contain up to several thousand stars and are found in the disk of the galaxy (Population I).
• Globular clusters: old, contain hundreds of thousands of stars, all closely packed together. They are found mainly in the halo of the galaxy (Population II).
14.2 Galactic Recycling
• Our Goals for Learning• How does our galaxy recycle gas into stars?
• Where do stars tend to form in our galaxy?
Question 4What happens after an interstellar cloud of gas
and dust is compressed and collapses:
A. It will heat and contract
B. If it gets hot enough (10 million K) it can produce energy through hydrogen fusion
C. It can produce main sequence stars
Question 4What happens after an interstellar cloud of gas
and dust is compressed and collapses:
A. It will heat and contract
B. If it gets hot enough (10 million K) it can produce energy through hydrogen fusion
C. It can produce main sequence stars
D. All of the above
Cycle of Birth and Deaths of Stars• Interstellar cloud of gas and dust is
compressed and collapses to form stars
• After leaving the main sequence red giants eject their outer layers back to the interstellar medium
• Supernovas explode and eject their outer layers back to the interstellar medium
• Supernova explosions and other events can compress an interstellar cloud of gas and dust that collapses to form stars ………..
Disk: emission nebulae, blue stars star formation
Halo: No emission nebulae, no blue stars no star formation
Much of star formation in disk happens in spiral arms
The Whirlpool Galaxy
Emission NebulaeBlue StarsGas Clouds
Spiral arms are waves of star formation
14.3 The History of the Milky Way
• Our Goals for Learning
• What clues to our galaxy’s history do halo stars hold?
• How did our galaxy form?
Halo Stars: 0.02-0.2% heavy elements (O, Fe, …), only old stars
Disk Stars: 2% heavy elements, stars of all ages
Halo Stars: 0.02-0.2% heavy elements (O, Fe, …), only old stars
Disk Stars: 2% heavy elements, stars of all ages
Halo stars formed first, then stopped
Halo Stars: 0.02-0.2% heavy elements (O, Fe, …), only old stars
Disk Stars: 2% heavy elements, stars of all ages
Halo stars formed first, then stopped
Disk stars formed later, kept forming
What have we learned?• What clues to our galaxy’s history do halo
stars hold?• The halo generally contains only old, low-mass
stars with a much smaller proportion of heavy elements than stars in the disk. Thus, halo stars must have formed early in the galaxy’s history, before the gas settled into a disk.
What have we learned?• How did our galaxy form?
• The galaxy probably began as a huge blob of gas called a protogalactic cloud. Gravity caused the cloud to shrink in size, and conservation of angular momentum caused the gas to form the spinning disk of our galaxy. Stars in the halo formed before the gas finished collapsing into the disk.
14.4 The Mysterious Galactic Center
• Our Goals for Learning• What lies in the center of our galaxy?
Stars appear to be orbiting something massive but invisible … a black hole!
Orbits of stars indicate a mass of about 4 million MSun