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characteristics of stars
characteristics of stars

... close even though they are separated by large distance. Most of the stars outside the bulge are arranged in long ____________, called _________ which curve around the bulge. The entire Milky Way rotates around this bulge. The Milky Way Galaxy is called a ____________galaxy because of its circular, s ...
HNRS 227 Lecture #2 Chapters 2 and 3
HNRS 227 Lecture #2 Chapters 2 and 3

... Young star clusters give insight into star formation and evolution  Newborn stars may form an open or galactic cluster  Stars are held together in such a cluster by gravity  Occasionally a star moving more rapidly than average will escape, or leave the cluster  A stellar association is a group ...
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... Just before Ellie is dropped out of the machine, she sees a group of shiny lights shooting across the sky. What do you think this could be? _________________________________________________________________________ ...
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Summary for week #2

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Name: ____________________________ Date: _____________ Per. _________ Stars Study Guide (Ch. 21)

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STARS - AN INTRODUCTION

... Stars are balls of burning gas. Different types of gases make the star burn. They give off light and heat. The Sun is a medium sized star. It is bigger than all eight planets combined! However, there are stars a lot bigger than the Sun! The largest stars are called ...
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Astronomy - SchoolNotes

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Figures I through VII in Section 1 on the following sheet

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Astronomy 114 Problem Set # 7 Due: 30 Apr 2007 SOLUTIONS 1
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... measurements and observations. ____ 3. Factor in an experiment that can be manipulated by the experimenter. ____ 4. Factor in an experiment that can change if other factors are changed. ____ 5. After careful observation and applying background knowledge, ______ are formed by the observer. ____ 6. St ...
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Future of an expanding universe

Observations suggest that the expansion of the universe will continue forever. If so, the universe will cool as it expands, eventually becoming too cold to sustain life. For this reason, this future scenario is popularly called the Big Freeze.If dark energy—represented by the cosmological constant, a constant energy density filling space homogeneously, or scalar fields, such as quintessence or moduli, dynamic quantities whose energy density can vary in time and space—accelerates the expansion of the universe, then the space between clusters of galaxies will grow at an increasing rate. Redshift will stretch ancient, incoming photons (even gamma rays) to undetectably long wavelengths and low energies. Stars are expected to form normally for 1012 to 1014 (1–100 trillion) years, but eventually the supply of gas needed for star formation will be exhausted. And as existing stars run out of fuel and cease to shine, the universe will slowly and inexorably grow darker, one star at a time. According to theories that predict proton decay, the stellar remnants left behind will disappear, leaving behind only black holes, which themselves eventually disappear as they emit Hawking radiation. Ultimately, if the universe reaches a state in which the temperature approaches a uniform value, no further work will be possible, resulting in a final heat death of the universe.
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