PPT-Chemical constraints on Theories of Planet Formation

Vincent Geers Institute for Astronomy ETH Zurich Star amp Planet Formation group A Banzatti S Bruderer F Lahuis I Pascucci Th Henning P Ábrahám A Juhász. Chemical Butyl Acetate Chemical Butylated Hydroxytoluene Chemical Coal ar Chemical Cocamide DEALauramide DEA Chemical Diazolidinyl Urea Chemical Ethyl Acetate Chemical Formaldehyde Chemical P The lack of transparency introduced by poorly anchored math ematical models the psychological persuasiveness of stories and the way the profession neglects relevant issues are suggested as explanations for how what we perhaps should see as displays Topic:. Orbital dynamics and. the restricted 3-body problem. Lecture by: C.P. Dullemond. Objects of the Solar System. Kuiper Belt. (30-50 AU). 10 AU. 1 AU. Earth. Mars. 1 AU. 1.38-. 1.67 AU. e. = 0.1. Topic:. Collapsing clouds. and the. formation of disks. Lecture by: C.P. Dullemond. Formation of a star from a . spherical molecular cloud core. Hydrostatic pre-stellar Cloud Core. Equation of hydrostatic equilibrium:. Planet-Host Stars. 2013. 2. 22. . Wonseok. Kang . Kyung . Hee. University. Sang-. Gak. Lee. . Seoul National University. Why? : Abundances of Planet Host Stars. 2. Workshop on Stars, Planets, and Life 2013. Topic:. Formation of. rocky planets from. planetesimals. Lecture by: C.P. Dullemond. Standard model of rocky planet formation. Start with a sea of planetesimals (~1...100 km). Mutual gravitational stirring, increasing „dynamic temperature“ of the planetesimal swarm.. Location in Solar System. Landscape and Climate. Is it like Earth in any way? Explain. Interesting Facts. Why is it the best planet to colonize?. Structures needed. A note to teachers. Activity Description. This presentation can be used to help consolidate the material learnt in the Planet Mission workshop. There is also an additional activity for pupils to create a postcard from their favourite planet.. by Transit Observations. Norio Narita. National Astronomical Observatory of Japan. Outline. Introduction of transit photometry. Further studies for transiting planets. Future studies in this field. Building Leadership and Entrepreneurial Capacity for a Sustainable Hawaii. Linda M. Lewandowski, DEL-MEM Candidate. Advisor: Michael Orbach, Ph.D.. Research Question and Objectives. Research question: What is the design of the partnership and program model needed to accomplish the Planet Pioneer mission?. Size. Appearance. Having moons. Having rings. Period of rotation (how long a day is). How Can We classify Planets?. Look at your chart of information.. Approximate Diameter= How Big or small it is.. Period of Rotation = How long fast the planet spins on its axis. . Insights from recent surveys. Gaspard . Duchêne. (UC Berkeley, Obs. Grenoble). © NASA/JPL/Caltech. Planets in multiple systems?. © . LucasFilm. Ltd.. They must exist!. Planets in multiple systems!. Dewayne E Perry. ARiSE. , ECE, UT Austin. perry@ece.utexas.edu. Theories D & E. I begin with two simple theories:. A theory about design – D. A theory about empirical evaluation – E. And a theory about how to model theories. RF is formed of large number of neurons . present through the entire brainstem, it . extends upward to the level of the thalamus . and downward to be continuous with the . interneurons. of the spinal cord..