PDF-Planet

brPage 1br YHF57347XQH57347EURVVH57347HW57347VRXV57347XQ5734757536OHW57347G57527HDX57347IUDLFKH5735957347QHWWRH57347VRLJQHX HUPH57347OH57347ERFD. 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:. 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 milky way. (seen from Bryce Canyon, UT). The Solar System. ?. “A . system. is a set of . interacting. or interdependent. components . forming an integrated whole” (Wikipedia). The Solar System. 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:. 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. 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.. 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. Made by. :. . Syrtsova. Aleksandra. Protagonist . . of the film is . Matthew . McConaughey. .. Mackenzie Foy and Jessica . Chastain played . Cooper’s daughter. .. Cooper . flys. . in space.. He got into . 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). 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. 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?.