'Hot jupiters' diaporamas de présentation

Chapter 13 Other Planetary Systems

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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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?.

628 views • 45 slides

What do we know about extrasolar planets?

What do we know about extrasolar planets?. Neill Reid STScI. The big questions. Over 145 extrasolar planets in more than 125 stellar systems have been discovered since 1995 -this includes several multiplanet systems ?What are the properties of those planetary systems?

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EART164: PLANETARY ATMOSPHERES

EART164: PLANETARY ATMOSPHERES. Francis Nimmo. Last Week - Dynamics. u l ~( e l) 1/3. Reynolds number, turbulent vs. laminar flow Velocity fluctuations, Kolmogorov cascade Brunt-Vaisala frequency, gravity waves Rossby waves, Kelvin waves, baroclinic instability

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EART164: PLANETARY ATMOSPHERES

EART164: PLANETARY ATMOSPHERES. Francis Nimmo. Last Week - Dynamics. u l ~( e l) 1/3. Reynolds number, turbulent vs. laminar flow Velocity fluctuations, Kolmogorov cascade Brunt-Vaisala frequency, gravity waves Rossby waves, Kelvin waves, baroclinic instability

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Important Stuff (Section 3)

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Lecture II: Gas Giant Planets

Lecture II: Gas Giant Planets. The Mass-Radius diagram - interiors Equations of State and Phase transitions Phase separation Hot Jupiters. The Giant Planets. HD 209458b: a Hot Jupiter. HD 168443b: highly eccentric one. More diversity than expected ?.

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Goal: To understand how we find Exo-Solar planets

Goal: To understand how we find Exo-Solar planets. Objectives: To learn what Hot Jupiters are and how we find them To learn about the transit method To learn about microlensing. What are hot Jupiters? http://www.theregister.co.uk/2008/12/10/nasa_co2_gas_giant/. Gas giants

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Atmospheric Circulation of hot Jupiters Adam Showman LPL

Atmospheric Circulation of hot Jupiters Adam Showman LPL Collaborators: J. Fortney, N. Lewis, L. Polvani, D. Perez-Becker, Y. Lian, M. Marley, H. Knutson. Spitzer light curves for HD 189733b . Knutson et al. (2007, 2009). 24 m m. 8 m m.

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Florian Rodler

What do we know about the exo-planets? & How to detect direct signals from exo-planets?. Florian Rodler. Introduction 201 confirmed planetary candidates + 14 confirmed planets found around solar-like stars and pulsars (in 175 planetary systems). -12. Introduction

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Florian Rodler

What do we know about the exo-planets? & How to detect direct signals from exo-planets?. Florian Rodler. Introduction 201 confirmed planetary candidates + 14 confirmed planets found around solar-like stars and pulsars (in 175 planetary systems). -12. Introduction

241 views • 23 slides

Origin & Evolution of Planetary Systems: Theories versus Observations

Origin & Evolution of Planetary Systems: Theories versus Observations. D.N.C. Lin University of California, Santa Cruz, KIAA, Peking University, with. S. Ida, J.L. Zhou, K. Kretke, C. Baruteau, K. Schlaufman

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Other planetary systems

269 views • 16 slides

Magnetospheric protection of ``Hot Jupiters'': The key role of magnetodisks in scaling

Magnetospheric protection of ``Hot Jupiters'': The key role of magnetodisks in scaling of a planetary magnetospheric obstacle. M. L. Khodachenko 1 , I. I. Alexeev 2 , E. Belenkaya 2 , H. Lammer 1 (1) Space Research Institute, Austrian Academy of Sciences, Graz, Austria,

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OmegaTranS: are we ready?

199 views • 12 slides

Concept of Thermal Bulges

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Hot Jupiter in a Tube

Hot Jupiter in a Tube. 0.5 m. Mirror. Mirror. Detector. HR mirror. HR mirror. Source. Sulfur discharge. Numerical solution of laser rate equations for quantum cascade laser with weak intracavity absorption line shows feasibility of detecting molecular absorption at level of 10 -6 Torr.

121 views • 1 slides