PPT-Planet Formation

Topic Orbital dynamics and the restricted 3body problem Lecture by CP Dullemond Objects of the Solar System Kuiper Belt 3050 AU 10 AU 1 AU Earth Mars 1 AU 138 167 AU e 01. Topic:. Formation of. gas giant planets. Lecture by: C.P. Dullemond. Two main theories. Gravitational instability of the gas disk. Core accretion scenario. Giant Planet Formation by. Gravitational Instability. 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:. 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.. Lecture by C.P. Dullemond. Institute for Theoretical Astrophysics. Heidelberg University. Image . Credit. : NASA. The Big Questions. After C. Mordasini. > 10 billion galaxies in the Universe. 100 billion stars in each. 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. Growth of Protoplanets. Starter. Hubble images. https://www.youtube.com/watch?v=1lPXy-WKn7k&list=PLiuUQ9asub3Ta8mqP5LNiOhOygRzue8kN. https. ://. www.youtube.com/watch?v=PuY0GfGLFMU&list=PLiuUQ9asub3Ta8mqP5LNiOhOygRzue8kN. 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?. and a fly’s-eye ‘. evryscope. ’. at Antarctica. Philip . Yock. , Auckland, New Zealand. 20th Microlensing Workshop . Institut. . d'Astrophysique. de Paris. 13-15 January 2016 . Twenty years ago. 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. . 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. | . 2000 – 2003. Décrivez. les . spécialités. de . cette. formation : . vos. . diplômes. , les options de la formation, . etc. …. FORMATION. | . 2000 – 2003. Décrivez. les . spécialités. 1Planet is an Earth data and analytics company producing 25 terabytes of data per day from approximately 200satellites the largest Earth imaging satellite fleet everPlanets proprietarydata powersa hig 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..