The Interstellar Medium

• Interstellar medium = gas and dust between

stars

– Temp ~0 − 300 K (Ave. 100 K)

– Low density ~106 atoms/m3

– gas

• individual atoms

• 90% H, 9% He, + trace elements

– dust

• clumps of atoms and molecules (like chalk dust)

• composition not well known (silicates, iron, carbon,

ices)

1

Extinction

• Light from a star going through the

interstellar medium is scattered by the dust.

• Wavelength of light scattered ~ size of dust

particles

• Dust scatters blue light more efficiently

– “reddening”

– Need to use spectral classification to identify

temperature of stars since color can be affected

by extinction.

2

3

Nebulae

• Nebula = cloud of interstellar gas and dust.

– Looks like fuzzy patch in the sky.

– Composition roughly the same as the

interstellar medium.

4

Emission Nebula

• Glowing clouds of hot, interstellar gas

• Each has very hot O or B type star inside.

• High energy photons ionize the gas

• When electrons recombine they emit light.

• Nebula appear red because on of the main

recombination lines of H is in the red

5

Hydrogen

Lines

6

Reflection Nebula

• Light enters nebula and blue light is

scattered.

• Nebula appears blue.

See only blue scattered light

Blue light is

scattered

Star appears

reddened, but

cloud is blue

7

Trifid Nebula

8

http://antwrp.gsfc.nasa.gov/apod/image/0505/m20_jacobsen_full.jpg

Spider and the Fly

9

Dark Dust Clouds

• Cool (10-20 K) dense clouds made mainly

of gas with some dust.

• Dust obscures visible light.

• Can measure several parsecs across.

10

Dark dust cloud and

reddening

11

12

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