'Earth moon system' diaporamas de présentation

CHAPTER 20

CHAPTER 20. A Family of Planets. Chapter 20.

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Astronomy

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Intro Geophysics GRAVITY AND THE FIGURE OF THE EARTH

Intro Geophysics GRAVITY AND THE FIGURE OF THE EARTH. Newton's Law of Universal Gravitation. Consider two point masses, m 1 and m 2 , separated by a distance r. Let r 1 be a unit vector pointing from m 1 to m 2 , then we can write the force F on mass m 2 due to mass m 1 as:.

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Astronomy 251 Life on Other Worlds Mondays 4-6, MP102 Prof. Ray Jayawardhana MP 1408 416 946 7291 rayjay@astro.ut

Astronomy 251 Life on Other Worlds Mondays 4-6, MP102 Prof. Ray Jayawardhana MP 1408 416 946 7291 rayjay@astro.utoronto.ca Office hours: Tuesdays 11-12 or by appt. Course website and syllabus: http://www.astro.utoronto.ca/~rayjay/ast251 Astronomy 251 Life on Other Worlds TAs:

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Earth Science, 10e

Earth Science, 10e. Edward J. Tarbuck & Frederick K. Lutgens. Origin of Modern Astronomy Chapter 20. Earth Science, 10e Stan Hatfield and Ken Pinzke Southwestern Illinois College. Early history of astronomy. Ancient Greeks Used philosophical arguments to explain natural phenomena

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Survey of Astronomy

Introduction. Welcome. This is Phys 1040 and Astro 1040. Survey of Astronomy. Astro1010-lee.com. Please pick up one each of the papers on the table up front. twlee2016@gmail.com. Introduction. Survey of Astronomy. Astro1010-lee.com. twlee2016@gmail.com. Introduction. My e-mail.

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Pearson Prentice Hall Physical Science: Concepts in Action

Pearson Prentice Hall Physical Science: Concepts in Action. Chapter 25 The Solar System. 25.1 Exploring the Solar System. Objectives: 1. Compare and contrast the geocentric and heliocentric models of the solar system

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Origin of modern astronomy

Earth Science Ch. 22. Origin of modern astronomy. 22.1 Early Astronomy. Ancient Greek Contributions Aristotle Concluded the Earth is round because it always casts a curved shadow on the moon Eratosthenes

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The Earth and moon viewed from Mercury

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Ch. 28-Minor Bodies of Solar System

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Ge/Ay133

When and how did the cores of terrestrial planets form?. Ge/Ay133. Two end member hypotheses for core formation:. Estimated core sizes of the terrestrial planets. Two end member hypotheses for core formation:. Q: Why is heterogeneous accretion unlikely?.

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Planet Earth

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Our Barren Moon

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22.2 Earth Moon-Sun System

22.2 Earth Moon-Sun System. Vocabulary: Phases of the moon,Lunar vs. solar eclipse, precession, apogee, perigee rotation, revolution, aphelion, perihelion. Phases of the Moon. New moon, 1 st quarter, Half moon, 3 rd quarter, Full moon,. Earth- Moon System.

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Earth and Moon

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Earth and Moon

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Chapter 5

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The Earth-Moon System

The Earth-Moon System. Moon Mass 7.3483 x 10 22 kg Equatorial Radius 1737.4 km Earth Mass 5.97219 x 10 24 kg Mean Radius 6371.00 km. Orbital Parameters. Average distance from Earth 384,400 km (0.00257 A.U.) Perigee 363,300 km Eccentricity 0.05490

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