Chapter 11 The Interstellar Medium Chapter 11 The

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Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium Goals • Explain what the interstellar medium is •

Chapter 11: The Interstellar Medium Goals • Explain what the interstellar medium is • Describe emission nebula • Describe “dark” nebula • Describe the star formation process • Describe the formation of star clusters

Chapter 11: The Interstellar Medium Region in the Constellation Orion named the Orion Nebula

Chapter 11: The Interstellar Medium Region in the Constellation Orion named the Orion Nebula which is the closest star formation region to us. Jets and disks appear to be part of the star birth process

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium Astronomers can determine what the interstellar material is made

Chapter 11: The Interstellar Medium Astronomers can determine what the interstellar material is made of, its temperature, and velocity by observing the absorption lines produced when starlight passes through the clouds of material. Blue light is also scattered more easily than red so the red light makes it through better, thus objects appear reddened.

Chapter 11: The Interstellar Medium The interstellar medium is the region between the stars.

Chapter 11: The Interstellar Medium The interstellar medium is the region between the stars. It is composed of gas and dust that ultimately are the raw materials from which stars and planetary systems are made. This wide angle photograph of our milky way galaxy shows dark dust lanes cutting through the plane of our galaxy.

Chapter 11: The Interstellar Medium The clouds and dust of the interstellar medium tend

Chapter 11: The Interstellar Medium The clouds and dust of the interstellar medium tend to be cold and thin by our standards. Average temperature is 100 K with an average density of one atom per cm 3. On average there is one dust particle for every trillion atoms.

Chapter 11: The Interstellar Medium Emission Nebula

Chapter 11: The Interstellar Medium Emission Nebula

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium Dark Nebula

Chapter 11: The Interstellar Medium Dark Nebula

Chapter 11: The Interstellar Medium 21 centimeter radiation is produced when the spins of

Chapter 11: The Interstellar Medium 21 centimeter radiation is produced when the spins of the electron and proton flip in a Hydrogen atom. Radio astronomers can thus map out the distribution of Hydrogen throughout the galaxy

Chapter 11: The Interstellar Medium Star formation take about 10 million years

Chapter 11: The Interstellar Medium Star formation take about 10 million years

Chapter 11: The Interstellar Medium The emission part of the star formation region is

Chapter 11: The Interstellar Medium The emission part of the star formation region is only a small part of the giant cloud.

Chapter 11: The Interstellar Medium The Orion Nebula

Chapter 11: The Interstellar Medium The Orion Nebula

Chapter 11: The Interstellar Medium More Orion Individual stars forming in density fingers

Chapter 11: The Interstellar Medium More Orion Individual stars forming in density fingers

Chapter 11: The Interstellar Medium We think clusters of stars are formed when large

Chapter 11: The Interstellar Medium We think clusters of stars are formed when large clouds fragment into smaller and smaller pieces until multiple star from.

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium

Chapter 11: The Interstellar Medium Brown dwarfs

Chapter 11: The Interstellar Medium Brown dwarfs

Chapter 11: The Interstellar Medium Young Cluster Old Cluster

Chapter 11: The Interstellar Medium Young Cluster Old Cluster