2 Lecture 10: Cosmochemistry: origin of nuclei, solar system, and earth What is the bulk composition of the solar system? Where/when/how did the atoms.
Origins of Regular and Irregular Satellites ASTR5830 March 19, 2013 12:30-1:45 pm.
Mass Distribution and Planet Formation in the Solar Nebula Steve Desch School of Earth and Space Exploration Arizona State University Planet Formation.
Opacities and Chemical Equilibria for Brown Dwarf and Extra-Solar Giant Planet Models Christopher M. Sharp June 9, 2004.
Signatures of Exoplanets HD209458b: a Hot Jupiter Orbiting a Bright Star Sara Seager Carnegie Institution of Washington Image credit: NASA/JPL-Caltech/R.
A new concept in stellar astrophysics based on internal rotation: Effective mass and its place in the A- and B-star puzzle Mutlu Yıldız Ege University,
Geophysics of Icy Saturnian Satellites Torrence V. Johnson Jet Propulsion Laboratory, Caltech.
Geoffrey A. Blake GPS Division Astronomy Colloqium, 26October2005, Caltech VV Ser Spιtzer+Keck Spectroscopy & the Building Blocks of Planetary Systems.
Planet Formation During the Migration Episode of a Giant Planet Áron Süli Eötvös University Department of Astronomy 5th Austrian-Hungarian Workshop, Wien.
Improving our understanding of Stellar Evolution with PLATO 2.0 Santi Cassisi INAF - Astronomical Observatory of Teramo, Italy.
Why do we need to continue to measure solar neutrinos ? Why a need for low energy measurements.
Chapter two The physics of stellar interiors