Climate over the long term (Ch. 3 - 6 highlights) Long-term climate changes Plate tectonics What maintains Earth’s habitability? Faint Young Sun paradox.
AST101 Why Does the Sun Shine?. Is the Sun on Fire? Fire (oxidation) produces light and heat, just like the Sun. Source: chemical potential energy Suppose.
Atmosphere Temperature Precipitation Humidity Wind Radiation CO 2 Nitrogen Climate Feedbacks Sensible heat, Latent heat Albedo Net radiation Momentum CO.
1 Nuclear reactions in the Sun A first look at the SunA first look at the Sun A deeper look: helioseismologyA deeper look: helioseismology Neutrino: the.
Earth Systems Science Chapter 1 I. CHANGES it is the nature of dynamic systems to change, often even in the absence of external “forcings”. Some important.
Stellar Interiors Physical Astronomy Professor Lee Carkner Lecture 10.
Andrej Čadež Colaborators Uroš Kostić Massimo Calvani Andreja Gomboc Tidal energy release before plunging into a black hole Andrej Čadež Uroš Kostić Massimo.
Centimeter and Millimeter Observations of Very Young Binary and Multiple Systems -Orbital Motions and Mass Determination -Truncated Protoplanetary Disks.
The understanding of the origin of life was largely speculative until the 1920s, when Oparin and Haldane, working independently, proposed a theoretical.
Session 5 – Refuting Evolution Pt.1 In this session we will turn our focus away from addressing the evidence used to support evolution, and instead look.
GNO and the pp - Neutrino Challenge T.Kirsten/GNO Till A. Kirsten Max-Planck-Institut für Kernphysik, Heidelberg for the GNO Collaboration NDM03 Nara/Japan.
Solar Structure
