the milky way Flashcards

1
Q

Thomas Wright’s Milky Way (1750)

A

The Milky Way is “an optical effect due to our immersion in
what locally approximates to a flat layer of stars.”
First to suggest that faint nebulae were galaxies similar to
the Milky Way, but much further away.

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2
Q

Harlow Shapley (1921)

A

Noticed Globular Clusters are:
1. Uniformly above & below the MW.
2. Concentrated toward Sagittarius
Observations:
Used RR Lyrae variables to
map the cluster
distribution in space.

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3
Q

Why was Herschel’s strategy for mapping our Galaxy
flawed?

A

He relied on visual wavelengths, which are obscured by
dust.

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4
Q

Schematic of the Milky Way

A

Disk is 100,000 light years (30 kpc) in diameter
* Sun ~8 kpc from the center (Sagittarius)
* Galactic Center and disk obscured by dust

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5
Q

Imagine that you could travel at the speed of light.
Starting from Earth, how long would it take you to travel
to the center of the Milky Way Galaxy?

A

26,000 years

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6
Q

The image below represents the Milky Way Galaxy.
What is the approximate diameter of the white dot?

A

10,000 light years

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7
Q

Thin disk

A

400 light years thick
* youngest stars (1-10 Byr)
* gas & dust
* Sun is 70 ly above the mid-plane

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8
Q

Thick disk

A

2000 light years thick
* older stars (11 Byr)
* 5% the mass of the thin disk

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9
Q

Bulge

A

Inner region of the Galaxy (within 10,000 ly of the center)
* contains the central bar
* old stars
* little gas and dust
* visible through the disk at infrared wavelengths

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10
Q

halo

A

Spherical distribution of very old (13 Byr),
faint stars, centered on bulge
* sparsely populated
* extends well beyond (150,000 ly) the
visible light from the disk
* globular clusters
* dark matter

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11
Q

spiral arms

A

Pattern of hot stars, star clusters,
gas & dust in the disk
tracers:
* O&B Stars
* emission nebulae (HII regions)
* gas and dust Clouds

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12
Q

Spiral Arms in the Milky Way

A

Two major, several smaller arms
* Sun sits in a minor arm called
the ‘Orion Spur’ (10,000 ly long)

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13
Q

Rotation Speeds
Inner Parts

A

Rise from Zero to few hundred km/sec

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14
Q

rotation speed outer parts

A

Nearly constant at a few hundred km/sec

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15
Q

Density Waves

A

Pass through disk like water waves pass over the
ocean.
* Stars move through the spiral arms.
* Gas clouds try to move through, but some
form stars (collision)

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16
Q

For an orbit

A

the speed depends only
on the mass inside the orbit:

17
Q

What is the extra mass if not stars?

A

dark matter

18
Q

What observations suggest the mass of the Galaxy goes
much farther out than its visible disk

A

the rotation curve of the outermost portions of the disk