PPT-The basics of terrestrial planet formation

Author : trish-goza | Published Date : 2016-02-28

The origin of water 1798 engraving Pass Lecture 3 Formation of the Terrestrial Planets and Origin of Earths water Earth forms here Ice forms here Sources of water

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The basics of terrestrial planet formation: Transcript

The origin of water 1798 engraving Pass Lecture 3 Formation of the Terrestrial Planets and Origin of Earths water Earth forms here Ice forms here Sources of water for the Earth Standard Mean Ocean Water DH150 . 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. spinels. would also corroborate evidence for mantle or . ultramafic. material in KT boundary . ejecta. as proposed by:. . DePaolo. , . Kyte. , Marshall, O’Neil & . Smit. ; EPSL Vol. 64, Sept. 1983. . Topic:. Collapsing clouds. and the. formation of disks. Lecture by: C.P. Dullemond. Formation of a star from a . spherical molecular cloud core. Hydrostatic pre-stellar Cloud Core. Equation of hydrostatic equilibrium:. 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. 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!. 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. Resolution ~ 10x JVLA . Frequency range: 1. . – 50, 70 – 115 GHz. https://. science.nrao.edu. /futures/. ngvla. T. he Very Large Array: 2 min history. 1972 – Approved by Congress. 1980 – Full science operations. | . 2000 – 2003. Décrivez. les . spécialités. de . cette. formation : . vos. . diplômes. , les options de la formation, . etc. …. FORMATION. | . 2000 – 2003. Décrivez. les . spécialités. spinels. would also corroborate evidence for mantle or . ultramafic. material in KT boundary . ejecta. as proposed by:. . DePaolo. , . Kyte. , Marshall, O’Neil & . Smit. ; EPSL Vol. 64, Sept. 1983. .

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