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Living World Open Night, Friday, April 1, 2016 Astronomy Open
Living World Open Night, Friday, April 1, 2016 Astronomy Open

... Imagine a world where all segments of society demanded environmentally benign products! Imagine if all consumers, all retailers and all manufacturers insisted on buying and selling only non-toxic materials! The unfortunate reality is that, even if this situation were to occur, our knowledge of mater ...
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Sound Waves - Ellsworth High School

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... within the incidence of the Sun. According to (Oort, 1950) exist cloud around the Sun of comet nuclei, called the Oort cloud. This cloud is not available observations. But if it exists, the comet nucleus moving near the outskirts of the solar system. At the outskirts of the solar system must take in ...
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Purdue University PHYS221 EXAM II Solutions are

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... • Radio waves sent to Viking, Mars lander (1979) • Radio waves sent to Cassini, Saturn orbiting spacecraft, on other side of Sun (2003) • Gravity Probe B, in Earth orbit (2011) ...
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... – Only stars more massive than the Sun have had enough time to live their lives. These stars aren’t all that common, so it doesn’t seem like there’s enough of them – Again, the dead stars would need to be distributed in space differently than the living stars, hard to imagine how this could be! ...
Stellar Remnants
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Lecture Eleven (Powerpoint format)

...  Einstein’s Theory of General Relativity predicts that spacetime itself will form ripples which propagate at the speed of light.  Where are these gravitational waves? Because gravity is a weak force in comparison to electromagnetism, we have not yet directly detected any gravitational waves.  Phy ...
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... 31. What kind of waves can be used to treat some cancerous tumors? Gamma Rays 32.When you increase the frequency of a sound wave… a. the period will also increase. c. pitch will decrease. b. the period will decrease . d. loudness will increase. 33.Mechanical waves can NOT transport… a. energy b. mat ...
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... Conservation of angular momentum: before collapsing, the star’s core probably rotates once every few hours. Collapse by a factor of x decreases the rotation period by a factor of x2. The core collapses by roughly a factor of 1000, so it spins about 10002 = 106 times more often. Final rotation period ...
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Research Powerpoint - Department of Astronomy

... Prof. Suvi Gezari searches for transients associated with the tidal disruption of stars by dormant supermassive black holes lurking in the nuclei of distant galaxies. Shown here is an event discovered by GALEX and Pan-STARRS1, and the computer simulation of the fate of the star being ripped apart b ...
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Introduction to Astrophysics Tutorial 4: Supernovae

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First observation of gravitational waves

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