'Rapid rotation' diaporamas de présentation

Second-Order Conditioning

Second-Order Conditioning. Pair CS 1 with US Pair CS 2 with CS 1 CS 2 produces CR CS 1 serves as US for CS 2. Blair & Shimp (1992). Unpleasant experience paired with music Brand paired with music. Design. Pre-conditioning phase Subjects listen to theme music

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Part 4: Our Solar System, Life in the Universe

Part 4: Our Solar System, Life in the Universe. Monday, April 7 Reading: Chapter 15 (12 th Edition of the textbook) Solar System: Introduction and Formation; Other Solar Systems Wednesday, April 9 Reading: Chapter 18 (planets)

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Issues Relating to Observables of Rapidly Rotating Stars

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History of Space Exploration

History of Space Exploration. People to remember:. Galileo Robert Goddard Neil A rmstrong. G alileo. Studied the planets with a telescope in the 1600s His studies led him to believe a theory of Copernicus, that the planets orbit the sun. Robert Goddard Father of Modern Rocketry.

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The Jovian Planets (Gas Giants)

The Jovian Planets (Gas Giants). Saturn. Jupiter. Uranus. Neptune. (roughly to scale). Discoveries. Jupiter and Saturn known to ancient astronomers. Uranus discovered in 1781 by Sir William Herschel (England).

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How Do I Connect With What is Beneath My Feet and Within My Reach?

How Do I Connect With What is Beneath My Feet and Within My Reach?. Draw a Picture Map of the Earth Forming Events. Small dot containing all mass and energy appears Big bang Universe unfolds Formation of Stars and Galaxies

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Science Summary Omer Blaes (UCSB)

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Neutron Stars

0. Neutron Stars . 0. Gradual compression of a stellar iron core. Radial Structure of a Neutron Star. - Heavy Nuclei ( 56 Fe). - Heavy Nuclei ( 118 Kr); free neutrons; relativistic, degenerate e -. - Superfluid neutrons. 0. Properties of Neutron Stars. Typical size: R ~ 10 km.

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THE SKY

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A Pulsational Mechanism for Producing Keplerian Disks around Rapidly Rotating Stars

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THE SKY

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