'Extrasolar planets' presentation slideshows

Chapter 13 Other Planetary Systems: The New Science of Distant Worlds

Chapter 13 Other Planetary Systems: The New Science of Distant Worlds. 13.1 Detecting Extrasolar Planets. Our goals for learning: Why is it so difficult to detect planets around other stars? How do we detect planets around other stars?.

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Planets and ExoPlanets

Planets and ExoPlanets. Earth, as viewed by the Voyager spacecraft. What does the solar system look like?. There are eight major planets with nearly circular orbits. Pluto and Eris are smaller than the major planets and have more elliptical orbits.

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Detecting Extrasolar Planets

Detecting Extrasolar Planets. Radial Velocity Measurements. First Proposed in 1952. Radial Velocity Variations. https://upload.wikimedia.org/wikipedia/commons/5/59/Orbit3.gif. Radial Velocity Variations. Radial Velocity Variations.

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The Stars

The Stars. The Sun is a Star. Surface of the Sun. Solar Prominence. Solar Corona. The Stars in the Sky. Vary in Brightness Distance Size Vary in Color Color = Temperature. Star Names. Proper star names mostly Arabic Greek Letters, Numbers Catalog Identifiers

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Chapter 15 The Formation of Planetary Systems

Chapter 15 The Formation of Planetary Systems. Units of Chapter 15. 15.1 Modeling Planet Formation 15.2 Formation of the Solar System 15.3 Terrestrial and Jovian Planets 15.4 Interplanetary Debris 15.5 Solar System Regularities and Irregularities The Angular Momentum Problem

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Search for Extraterrestrial Intelligence

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The formation of stars and planets

The formation of stars and planets. Image credit: Michael Sherick. Lecture by C.P. Dullemond Max-Planck-Institute for Astronomy Heidelberg. Sorry about:. Topic of Star- and Planet Formation is too vast to cover completely, and in sufficient depth, in 15 hours.

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The formation of stars and planets

The formation of stars and planets. Image credit: Michael Sherick. Lecture by C.P. Dullemond Max-Planck-Institute for Astronomy Heidelberg. Sorry about:. Topic of Star- and Planet Formation is too vast to cover completely, and in sufficient depth, in 15 hours.

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The Origin of the Solar System

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The Origin of the Solar System

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August 2006

TELESCOPES and DETECTORS. LSST - A Plan for Photo-z Calibrations. August 2006 Bogdan Popescu. OVERVIEW 1.

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Announcements

Announcements. Homework 7 due today Pick up Homework 8 Next test will be next week. Our Solar System and Others. 16 October 2006. Today:. Solar system patterns Age of the solar system (and a crash course in nuclear physics) Formation of the solar system Planets around other stars.

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GEOL 208 Lecture 1b

CON U

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The Formation of the Solar System

The Formation of the Solar System. Model Requirements. Each planet is relatively isolated in space. The orbits of the planets are nearly circular. The orbits of the planets all lie in nearly the same plane.

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A planet-building universe

A planet-building universe. dissemination. production. The top ten elements:. Note that the most common elements in your body all occur in the top ten, formed by a variety of mechanisms (most obvious absentees are calcium and phosphorus). A planet-building universe.

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Binary stars and clusters

Binary stars and clusters. Chapter 11. Review. Properties of stars apparent brightness (apparent magnitude) measure energy/area/second luminosity (absolute magnitude) calculate distance, use inverse-square law distance to the star parallax temperature

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Chapter 21, Section 4 Star Systems and Galaxies

Chapter 21, Section 4 Star Systems and Galaxies. Based on Prentice Hall Textbook by Rusty Sturken May, 2009. Background imag http://mayda.com/astro/Img/M31_LRGB-03C-1k.jpg e from http://mayda.com/astro/Img/M31_LRGB-03C-1k.jpg. Star Systems.

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Origins 3D03 Introduction

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