THE CHARACTERISATION OF TITAN’S ATMOSPHERIC PHYSICAL PROPERTIES BY THE HUYGENS ATMOSPHERIC STRUCTURE INSTRUMENT (HASI) M. FULCHIGNONI1,3 , F. FERRI2,7 , F. ANGRILLI2 ,…

Slide 11 of 30© Boardworks Ltd 2009 Slide 2 2 of 30© Boardworks Ltd 2007 Slide 3 3 of 30© Boardworks Ltd 2009 Detecting elements and compounds Mass spectrometry is a highly…

Surprising Science Surprising (or Mind-Blowing) Science By Kevin W. Rusch Factoid #1: Quark Pairs and Hadrons Quarks are elementary particles and a fundamental constituent…

Slide 1 O. Mousis (UTINAM, Université de Franche-Comté, France) L. N. Fletcher (Oxford U., UK), N. André (IRAP, France), M. Blanc (IRAP, France), A. Coustenis (LESIA,…

Slide 1 Dark Life and DUSEL Dark Life – what is it and why is it important? Why DUSEL? Slide 2 Deep Subsurface (> 1 km) Biomass – extremely low - diminishes with depth…

Slide 1 Australian Petroleum Production and Exploration Association Adelaide, 16 April 2007 The Future Environment for Energy Business Jesse H. Ausubel Program for the Human…

Slide 1 Announcements Tests will be graded by Wednesday Due to server problems, you may turn in Homework 6 as late as Wednesday. Pick up Homework 7 (due Monday) First project…

Slide 1 EXPReS: towards e-EVN Arpad Szomoru Joint Institute for VLBI in Europe 4th EVN-NREN Workshop, Schiphol, 12 Oct 2005. Slide 2 2006 200320042005 Telescope last mile…

Slide 1 15 February 2005AST 2010: Chapter 101 The Giant Planets Slide 2 15 February 2005AST 2010: Chapter 102 Jupiter Saturn Uranus Neptune The Jovian Worlds Slide 3 15 February…

Slide 1 The Outer Solar System Slide 2 The “Gas Giants” The outer planets have no solid surface, and are much bigger. The primary gases are hydrogen and helium (like…