PPT-Planet

Building Part 1 Solar Nebulas Chemical Composition Chemical Composition Everything astronomers know about the solar system indicates that it began as an interstellar gas cloud Cloud would have been mostly hydrogen with some helium small amounts of the heavier elements. 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. The . Pluto. Files. By Neil Degrasse Tyson. February 18, 1930. Pluto was discovered by Clyde W. Tombaugh, an amateur astronomer from Illinois at Arizona’s Lowell Observatory.. He considered naming the planet Percival, after Percival Lowell.. 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. 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. 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. . 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. 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 LAST UPDATED JANUARY 2018SUPPORTPLANETCOM PLANETCOM Mercury At a Glance.. Mercury is the closest planet to the Sun and due to its proximity it is not easily seen except during twilight. For every two orbits of the Sun, Mercury completes three rotations about its axis and up until 1965 it was thought that the same side of Mercury constantly faced the Sun. Thirteen times a century Mercury can be observed from the Earth passing across the face of the Sun in an event called a transit, the next will occur on the 9th May 2016..