PPT-Cool planet mass function

and a flyseye evryscope at Antarctica Philip Yock Auckland New Zealand 20th Microlensing Workshop Institut dAstrophysique de Paris 1315 January 2016 Twenty years ago. All of you know that it is advisable not to put hot things in a refrigerator for you somehow shock it and it will not last long In 1963 when I was in form 3 in Magamba Secondary School Tanzania I used to make icecream The boys at the school do this Cool is a small language that can be implemented in a one semester course Still Cool retains many of the features of modern programming languages including objects static typing and automatic memory management Cool 2015 is a new language diering fro Topic:. Planet migration. Lecture by: C.P. Dullemond. Planet migration: different kinds. Type I migration (small mass planets). Type II migration (high mass planets). Type III migration (rare type II variant). Topic:. Resonances. Lecture by: C.P. Dullemond. Literature: Murray & Dermott „Solar System Dynamics“. What is a resonance?. A resonance is when two characteristic frequencies of a system match up. 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.. Graham . Woan. University of Glasgow. 2. Astronomy and Space Physics in Scotland. Exoplanets. Galaxy dynamics. Cosmology. Solar physics. Scottish Universities . Physics Alliance. Gravitational waves. 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?. , . Ilaria. . Pascucci. , Daniel . Apai. University of Arizona. An Increase in Planet Formation Efficiency around Low-Mass Stars. EOS (PI: Daniel . Apai. ). a. NASA . NexSS. program. Planet Formation Efficiency. What is the Theory of Plate Tectonics?. “It is a theory that describes the formation, movements, and interactions of earth’s plates.”. Video: Planet Earth, The Living Machine. How can the Grand Canyon reveal the history of the Earth?. Daisuke Suzuki. ISAS / JAXA. the MOA collaboration. August . 8. , 2017 . 2017 Sagan Summer Workshop. Microlensing in the Era of WFIRST . a. snow. . = 2.7 (. M. /. M. Sun. ) AU. http://. exoplanet.eu. S. un. Outside the Asteroid belt . 8. th. largest planet in solar system. How long to orbit the sun:164.79 years.. Solar system. Its extreme weather.. neptune. is known for. Sergei . popov. Sizes and masses. 1312.3323. Radius vs. mass. 1604.07558. Results of modeling.. Old (relaxed) planets.. Colors correspond to . different fractions . of light elements.. Light elements contribution. Juliette Becker, Fred Adams, Tali Khain, Stephanie Hamilton, David Gerdes. Contact me. : Juliette Becker, jcbecker@umich.edu (425-876-9946). Planet Nine. Sheppard & Trujillo (2016). Batygin & Brown (2016). Introduction. Finding Planets. Pulsar Timing. Astrometry. Polarimetry. Direct Imaging. Transit Method. Radial Velocity. Selecting Planets. Recap. What else do we want to know?. Proposed Plan. Outline.