The Milky Way - PowerPoint PPT Presentation

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The Milky Way

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The Milky Way – PowerPoint PPT presentation

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Title: The Milky Way


1
The Milky Way
  • Our home galaxy, full of stars, gas and
    mysterious dark matter
  • We decompose it into a disk and a halo and a few
    other parts

2
Almost a View of our Milky Way
NGC 4526, a spiral galaxy like the MW but about
30 Mpc away it has a similar size, luminosity
and structure
3
Edge-on View and View of MW
4
Key Parts of the Milky Way
  • HALO Contains most globular clusters, and most
    Pop II stars roughly 30 kpc (105 lt-yr) in
    diameter.
  • THICK DISK roughly 5 kpc thick, and 30 kpc in
    diameter contains Pop I stars (but low density).
  • THIN DISK 500 pc thick contains MOST stars
    includes spiral arms and great majority of
    luminosity.
  • DUST DISK only 50 pc thick new stars are born in
    the molecular clouds found within this very thin
    disk.
  • SPIRAL ARMS are wrapped within the dust/thin
    disk contain almost all hot, luminous (O and B)
    stars.

5
Overall Structure of the Milky Way
6
Inner Parts
  • GALACTIC BULGE roughly 2 kpc in radius
    around center highest concentration of stars,
    including many globular clusters.
  • GALACTIC CENTER in the direction of the
    constellation Sagittarius, some 8 kpc from the
    Solar System (SS).
  • Multiwavelength Milky Way

7
MAPPING the MILKY WAY
  • Dust, mainly in molecular clouds, shrouds the
    Disk we see few stars beyond 2 kpc from SS in
    the thin disk, where the number of stars is much
    greater
  • Originally astronomers thought the Milky Way WAS
    the Whole Universe SS central to it (because
    of visible light extinction by dust)
  • Location of Globular Clusters in halo implied
    center towards Sagittarius and SS actually
    towards one side in early 20th century.
  • Atomic Hydrogen gas sends 21 cm radio waves that
    allow us to map the far side of the galaxy, and
    the outer reaches where there are few stars

8
Our Nearest Big Neighbor, M31, the Andromeda
Galaxy
Andromeda, about 30 kpc across down to nucleus
only 15pc
9
A Limited Conception of the MW
Herschels map of the Galaxy from star
counts More in the MW plane, but thought the Sun
near the center and got the size too small
didnt understand dust
10
Distribution of Globular Clusters
11
How do stars orbit in our galaxy?
12
Stars in the disk all orbit in the same direction
with a little up-and-down motion
13
Orbits of stars in the bulge and halo have random
orientations
14
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15
Thought Question
  • Why do orbits of bulge stars bob up and down?
  • A. Theyre stuck to interstellar medium
  • B. Gravity of disk stars pulls toward disk
  • C. Halo stars knock them back into disk

16
Thought Question
  • Why do orbits of bulge stars bob up and down?
  • A. Theyre stuck to interstellar medium
  • B. Gravity of disk stars pulls toward disk
  • C. Halo stars knock them back into disk
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