Thursday, May 02, 2013

Chapter 14 Notes Jessica Brandon


Chapter 14 Our Galaxy

14.1 The Milky Way Revealed
The Milky Way galaxy appears in our sky as a faint band of light
Dusty gas clouds obscure our view because they absorb visible light.
This is the interstellar medium that makes new star systems.
We see our galaxy edge-on Primary features: disk, bulge, halo, globular clusters.
If we could view the Milky Way from above the disk, we would see its spiral arms.
Stars in the disk all orbit in the same direction with a little up-and-down motion.
Orbits of stars in the bulge and halo have random orientations.
Sun’s orbital motion (radius and velocity) tells us mass within Sun’s orbit:1.0 x 1011 MSun
14.2 Galactic Recycling
Star-gas-star cycle Recycles gas from old stars into new star systems.
High-mass stars have strong stellar winds that blow bubbles of hot gas
Lower mass stars return gas to interstellar space through stellar winds and planetary nebulae.
X-rays from hot gas in supernova remnants reveal newly made heavy elements.
Supernova remnant cools and begins to emit visible light as it expands New elements made by supernova mix into interstellar medium.
Multiple supernovae create huge hot bubbles that can blow out of disk
Gas clouds cooling in the halo can rain back down on disk.
Atomic hydrogen gas forms as hot gas cools, allowing electrons to join with protons
Molecular clouds form next, after gas cools enough to allow to atoms to combine into molecules
Radiation from newly formed stars is eroding these star forming clouds.
We observe star-gas-star cycle operating in Milky Way’s disk using many different wavelengths of light.
Infrared light reveals stars whose visible light is blocked by gas clouds
Radio waves from carbon monoxide (CO) show locations of molecular clouds.
Long-wavelength infrared emission shows where young stars are heating dust grains
Gamma rays show where cosmic rays from supernovae collide with atomic nuclei in gas clouds
Ionization nebulae are found around short-lived high-mass stars, signifying active star formation
14.3 The History of the Milky Way
Halo stars formed first as gravity caused cloud to contract.
Remaining gas settled into spinning disk
Stars continuously form in disk as galaxy grows older.
Detailed studies: Halo stars formed in clumps that later merged
14.4 The Mysterious Galactic Center
Stars appear to be orbiting something massive but invisible … a black hole? Orbits of stars indicate a mass of about 4 million MSun.

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