'Complete revolution' diaporamas de présentation

Chapter 5 Trigonometric Functions

Chapter 5 Trigonometric Functions. Section 5.1 Angles and Arcs. Definition of an Angle. An angle is formed by rotating a given ray about its endpoint to some terminal position. The original ray is the initial side of the angle, and the second ray is the terminal side of the angle.

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SBBS 112: GENERAL PHYSICS

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Lesson 1 Reading Guide - KC

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The Solar System

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EARTH, MOON & SUN

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Earth Science 22.2B Motions Earth-Moon System

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Power Consumption

Power Consumption. How do we measure the electricity we use? This presentation came from Virginia Tech and has not been edited by the Georgia Curriculum Office. Performance objective.

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Warm-Up 8/15

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Earth in Space

Earth in Space. Chapter 1 Section 1. Focus Questions. What causes day and night? What causes the cycle of seasons on Earth?. Days and Years. The ancient Egyptians were among the first people to study the stars Ancient astronomers also studies the movements of the sun and the moon

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TCAP Stuffs

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Uniform Circular Motion

Uniform Circular Motion. Circular Coordinates. r -radial. r. ? -tangential. ?. Conditions. Uniform Circular motion occurs when an object is moving in a circular path at a constant speed. | v|=v. ? the instantaneous velocity v is always TANGENT to the path and a constant LENGTH. r.

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Radian and Degree Measure

Radian and Degree Measure. 4-1. Angles. Thinking about angles differently: Rotating a ray to create an angle Initial side - where we start Terminal side - where we stop. Angles. Standard Position- the initial side is on the positive side of the x axis with the vertex on the origin

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Exploration of the Universe

Exploration of the Universe

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Unit 1: Introduction to Trigonometry

Unit 1: Introduction to Trigonometry. LG 1-1: Angle Measures (Test 8/15) LG 1-2: THE Unit Circle (Test 8/21) LG 1-3: Evaluating Trig Functions (Test 8/23) LG 1-4: Arc Length (Test 8/28). Consider a circle, centered at the origin with 2 rays extending from the center. .

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Da Moon

Da Moon. Moon Motion. The moon orbits the Earth roughly once a month It revolves counterclockwise It takes 27.3 days to make one complete revolution. Does the Moon rotate? Yes How long does it take for the Moon to make one complete rotation? 27.3 days

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Galaxies

Galaxies. What is a Galaxy?. A galaxy is a massive, gravitationally bound system that consists of stars and stellar remnants and an interstellar medium of gas and dust . Gravitationally bound- held together by gravity Stellar remnants - Leftover material from dead stars

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Radian and Degree Measure

Radian and Degree Measure. Objectives: Describe Angles Use Radian and Degree measures. Trigonometry: the measurement of triangles the relationships among the sides and angles of triangles.

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Sidereal and Synodic Months

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