PPT-Minor Planet Astrometry

With CCD Images CLEA Summer Workshop June 20 2010 Glenn A Snyder Project CLEA Outline I Introduction II Mathematics of Astrometry III Methodology IV Reference Catalogs V Minor Planet Orbits. 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:. 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:. 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.. 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. New Science Enabled by Microarcsecond Astrometry. Workshop held 2009 July 21–23. Socorro, New Mexico. Jon . Romney -- NRAO, Socorro. for the Sensitivity Upgrade team:. Walter . Brisken. , Adam . 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. Methods of Searching for Alien Planets. Pulsar Timing. Astrometry. Radial Velocity. Transits. Lensing. Imaging. Planets cause stars to wobble. There are 3 ways to detect the wobbling of stars caused by planets: pulsar timing, astrometry, and radial velocity.. 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. 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). PLANETS JUPITERXABIGRAYun and is the largest in the solar systemIt is named after the Roman God JupiterJupiter is primarily composed of hydrogenwith a quarter of its mass being heliumThe lengthof a ye LAST UPDATED JANUARY 2018SUPPORTPLANETCOM PLANETCOM