PPT-How is our body like a planet?

We are all very lucky to be here on EARTH We are all very lucky to be here on EARTHour HYDROSPHERE We are all very lucky to be here on EARTHour HYDROSPHERE Water never enters or leaves our . 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.. Tidal deformation. Rotational deformation. Tidal torques. Orbit decay and spin down rates. Tidal circularization. Hot . Jupiters. Tidal and rotational deformations. Give information on the interior of a body, so are of particular interest. A note to teachers. Activity Description. This presentation can be used to help consolidate the material learnt in the Planet Mission workshop. There is also an additional activity for pupils to create a postcard from their favourite planet.. 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. 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?. HEADLINE. Body. text,. body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text, body text. 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. 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). Resource Specialist (instructs as to which resources to collect). 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. Train the Trainer: Schedule. Introductions: What’s it all about?. The need for sustainable cooking for our planet. Meat vs Insects. Neophobia and novel proteins. Insects in the kitchen. What’s it all about?. 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..