'Metallic hydrogen' diaporamas de présentation

Course

Astronomy 101 The Solar System Tuesday, Thursday 2:30-3:45 pm Hasbrouck 20 Tom Burbine tomburbine@astro.umass.edu. Course. Course Website: http://blogs.umass.edu/astron101-tburbine/ Textbook: Pathways to Astronomy (2nd Edition) by Stephen Schneider and Thomas Arny .

1.19k views • 104 slides

Course

Astronomy 101 The Solar System Tuesday, Thursday 2:30-3:45 pm Hasbrouck 20 Tom Burbine tomburbine@astro.umass.edu. Course. Course Website: http://blogs.umass.edu/astron101-tburbine/ Textbook: Pathways to Astronomy (2nd Edition) by Stephen Schneider and Thomas Arny .

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Chapter 8 Jovian Planet Systems

Chapter 8 Jovian Planet Systems. 8.1 A Different Kind of Planet. Our goals for learning: What are jovian planets made of? What are jovian planets like on the inside? What is the weather like on jovian planets?. What are jovian planets made of?. Jovian Planet Composition. Jupiter and Saturn

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Homework #4

Homework #4. Due on Thursday August 4 after class (2005) Chapter 11, p 300, Discussion 14 What is the cause of Io's volcanic activity? Chapter 11, p 300, Discussion 19 What might be the consequences of the discovery of life on Europa?

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EART 160: Planetary Science

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Planetary Magnetic Fields

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The formation of stars and planets

The formation of stars and planets . Day 5, Topic 1: The Solar System and Extrasolar Planets Lecture by: C.P. Dullemond. The Solar System. The Solar System. The Solar System. Inner rocky planets: Mercury, Venus, Earth, Mars Asteroid belt

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ESS 298: OUTER SOLAR SYSTEM

ESS 298: OUTER SOLAR SYSTEM. Francis Nimmo. Io against Jupiter, Hubble image, July 1997. Giant Planets. Interiors Composition and phase diagrams Gravimetry / interior structure Heating and energy budget Magnetic fields Formation Rings Atmospheres Structure Dynamics

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EART160 Planetary Sciences

EART160 Planetary Sciences. Exam results. Mean score = 81.1% 3 people had scores above 100%. Should take advantage of the extra credit. Last week. Surface temperature depends on solar distance, albedo, atmosphere (greenhouse effect)

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EART160 Planetary Sciences

EART160 Planetary Sciences. Francis Nimmo. Last week. Surface temperature depends on solar distance, albedo, atmosphere (greenhouse effect) Scale height and lapse rate are controlled by bulk properties of atmosphere (and gravity)

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EART160 Planetary Sciences

EART160 Planetary Sciences. Francis Nimmo. Last week. Surface temperature depends on solar distance, albedo, atmosphere (greenhouse effect) Scale height and lapse rate are controlled by bulk properties of atmosphere (and gravity)

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Where are we?

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Ch 7--The Outer Planets

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Saturn

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The Gas Giants

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How do we know that Earth is geologically active?

How do we know that Earth is geologically active?. Volcanoes Seismology Measuring the temperature inside All of the above 1 and 2. How does the cooling of planets and potatoes vary with size?. Larger makes it harder for heat from inside to escape

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Chapter 3 The Solar System

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Saturn

Saturn. Vote Saturn, Vote Spectacularly. Saturn Overview:. Size: 2 nd largest planet, 74,600 miles in diameter, almost ten times the size of Earth. Name: Derived from the Roman god of agriculture Gravity : 100 lbs. on Earth is 116 lbs. on Saturn Discovery: Discovered by Galileo in 1610

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Jupiter

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Novel xenon-hydrogen compound forms under pressure

Novel xenon-hydrogen compound forms under pressure Russell J. Hemley (Carnegie Institution of Washington) DMR 0508988.

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