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The Traveling Exhibit Science Background Part B: Star & Planet Formation prepared by Dr. Cherilynn Morrow for the Space Science Institute Boulder, CO.
The Traveling Exhibit Science Background Part B: Star & Planet Formation prepared by Dr. Cherilynn Morrow for the Space Science Institute Boulder, CO.
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The Formation and Structure of Stars Chapter 9. The Big Picture Stars exist because of gravity. Gravity causes interstellar material to collapse to form.
The Formation and Structure of Stars Chapter 9. The Big Picture Stars exist because of gravity. Gravity causes interstellar material to collapse to form.
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Bhert
Bhert
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The Interstellar Medium Chapter 10. You have begun your study of the sun and other stars, but now it is time to study the thin gas and dust that drifts.
The Interstellar Medium Chapter 10. You have begun your study of the sun and other stars, but now it is time to study the thin gas and dust that drifts.
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The Life History of Stars – Young Stars The Importance of Mass The entire history of a star depends on its mass and almost nothing else The more mass.
The Life History of Stars – Young Stars The Importance of Mass The entire history of a star depends on its mass and almost nothing else The more mass.
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The Formation and Structure of Stars Chapter 9. The space between the stars is not completely empty, but filled with very dilute gas and dust, producing.
The Formation and Structure of Stars Chapter 9. The space between the stars is not completely empty, but filled with very dilute gas and dust, producing.
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On your notes write out your address… Now what country… What continent… What planet… What galaxy? After today’s lesson, you should be able to answer all.
On your notes write out your address… Now what country… What continent… What planet… What galaxy? After today’s lesson, you should be able to answer all.
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The Interstellar Medium. I. Visible-Wavelength Observations A. Nebulae B. Extinction and Reddening C. Interstellar Absorption Lines II. Long- and Short-Wavelength.
The Interstellar Medium. I. Visible-Wavelength Observations A. Nebulae B. Extinction and Reddening C. Interstellar Absorption Lines II. Long- and Short-Wavelength.
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Nebulae. “Nebula” comes from the Latin word for cloud. “Nebulae” is the plural. It is loosely applied to anything that looks fuzzy or extended in a telescope.
Nebulae. “Nebula” comes from the Latin word for cloud. “Nebulae” is the plural. It is loosely applied to anything that looks fuzzy or extended in a telescope.
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The Interstellar Medium
The Interstellar Medium
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The Life History of Stars – Young Stars
The Life History of Stars – Young Stars
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The Origin of the Elements and the Evolution of the Composition of the Cosmos
The Origin of the Elements and the Evolution of the Composition of the Cosmos
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