'Galileo' presentation slideshows

Radio Wave Propagation

Radio Wave Propagation. Carl Luetzelschwab K9LA k9la@arrl.net. A Little About K9LA. Novice WN9AVT in October 1961 WA9AVT in May 1962, selected K9LA in 1977 Enjoy propagation, DXing , contesting, and antennas WorldRadio Propagation columnist since Jan 1997

2.2k views • 125 slides

Chapter 19

Chapter 19. Vibrations and Waves . There are two ways to transmit information and energy in our universe:. Particle Motion and Wave Motion . Vibration -. Wiggle in time. Light and Sound Both are vibrations of different kinds. Wave -. Wiggle in space . 1. VIBRATION OF A PENDULUM.

916 views • 52 slides

CHAPTER OBJECTIVES

CHAPTER OBJECTIVES. Review important principles of statics Use the principles to determine internal resultant loadings in a body Introduce concepts of normal and shear stress. Discuss applications of analysis and design of members subjected to an axial load or direct shear. CHAPTER OUTLINE.

605 views • 45 slides

Jupiter

Jupiter. Jupiter. Distance 800 million km (500 million miles) Diameter: 143,000 x 133,000 km (88,000 x 80,000 miles) or 11 x 10 Earths Rotates in 10 hours Polar Flattening: 1/16 (Earth = 1/298) Circles Sun in 12 years Mass: 318 Earths Volume: 1321 Earths Density: 1.326 gm/cc

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The Galileo Affair

The Galileo Affair. An Italian soap opera in two acts. From the Encyclopedia of Catholicism.

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The Solar System

The Solar System. Observing the Solar System. Guide For Reading. How do the heliocentric and geocentric description of the solar system differ? What did Kepler discover about the orbits of the planets? What two factors keep the planets in their orbits?. Wandering Stars.

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Jupiter

550 views • 26 slides

The Motion of the Planets

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The Motion of the Planets

542 views • 25 slides

The Link between Nutrition, Physical Activity and Academic Achievement

The Link between Nutrition, Physical Activity and Academic Achievement. Sigrid Quendler Vienna University, Austria, Europe for ILSI Center for Health Promotion, Atlanta, 2002. Background.

491 views • 23 slides

PHYSICS 231 INTRODUCTORY PHYSICS I pa.msu/courses/phy231

PHYSICS 231 INTRODUCTORY PHYSICS I www.pa.msu.edu/courses/phy231. Scott Pratt prattsc@msu.edu (517) 355-9200, ext. 2016 Office Hours: Monday, 9-10:30 AM in 1248 BPS. Course Information. http://www.pa.msu.edu/courses/phy231. Succeeding in Physics 231. Do your homework (yourself)!

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Galileo: Early Years

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Problem Based Learning in the Middle School

Problem Based Learning in the Middle School. 1. Orchestrated immersion 2. Relaxed alertness 3. Active processing. The three instructional techniques associated with brain-based learning:. Goals for PBL in the Middle School. Raise test scores Meet QCC objectives

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Ch 15: Milky Way Galaxy

649 views • 15 slides

The Outer Planets

The Outer Planets. The Inner Planets to Scale. 3,031 mi 7,521 mi 7,926 mi 4,222 mi. 5.4 g/cm3 5.2 g/cm3 5.5 g/cm3 3.9 g/cm^3. The Outer Planets to Scale. 88,700 mi 75,000 mi 31,700 mi 30,200 mi. 1.3 g/cm3 0.7 g/cm3 1.3 g/cm3 1.6 g/cm3.

398 views • 13 slides

1609 : A HISTORIC YEAR FOR ASTRONOMY

1609 : A HISTORIC YEAR FOR ASTRONOMY. Changing times.

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Chapter 2

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A Brief Introduction to Gravity

356 views • 11 slides

Parametric Equations

256 views • 7 slides

The Scientific Revolution

The Scientific Revolution. How did science begin to change the way people thought?. Copernicus. Galileo. Newton. I. Copernicus: Heliocentric Theory. A. Prior to 1500s true or false was determined by referring to an ancient thinker or the Bible

198 views • 5 slides