PPT-Planet Formation

Topic Resonances Lecture by CP Dullemond Literature Murray amp Dermott Solar System Dynamics What is a resonance A resonance is when two characteristic frequencies of a system match up. Paul DiGiacomo and Kerry Sawyer (NOAA). CEOS . SIT Technical Workshop. EUMETSAT, Darmstadt, Germany. 17. th. – 18. th. . September. 2015. Committee on Earth Observation Satellites. “Oceans and Society: Blue Planet” . 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). Vincent . Geers. Institute for Astronomy, ETH Zurich. Star & Planet Formation group. A. . Banzatti. , S. . Bruderer. , F. . Lahuis. , I. . Pascucci. , Th. Henning, . P. . Ábrahám. , A. . Juhász. 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. a. nd stellar multiplicity. Insights from recent surveys. Gaspard . Duchêne. (UC Berkeley, Obs. Grenoble). © NASA/JPL/Caltech. Planets in multiple systems?. © . LucasFilm. Ltd.. They must exist!. 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?. Zorcon. Welcome to the year 2094!. Planet . Zorcon. Gather in groups of 5.. Each person needs a job:. Project Director (leads the group). Surveyor (travels & collects resources). Data Collector (tallies & records the data). 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. Lightcurve. 0. Choose your . lightcurve. (a . GLPlanet. ). Assumptions:. a Gould & Loeb planetary (. GLPlanet. ) caustic crossing . perturbation. No parallax. No blending. Goal: Estimate 7 Parameters of a 2L1S Model. 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!. Certificate in Pastoral Ministry Course: Adult Faith Formation. 1. Prayer . We are Disciples. Who is it that discipled you into faith? This person is/these persons are at the heart of why you are faith-filled today.. 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