PDF-Main nebular Low-T material Fraction of nebular mass H, He Gas H2, He

Author : giovanna-bartolotta | Published Date : 2016-06-30

Jupiter Almost nebula composition due to gas capture 20 Mnebula 100 20 Mjupiter 5 Mjupiter is minimum mass required oSaturn Cooler than Jupiter with slightly

Presentation Embed Code

Download Presentation

Download Presentation The PPT/PDF document "Main nebular Low-T material Fraction of ..." is the property of its rightful owner. Permission is granted to download and print the materials on this website for personal, non-commercial use only, and to display it on your personal computer provided you do not modify the materials and that you retain all copyright notices contained in the materials. By downloading content from our website, you accept the terms of this agreement.

Main nebular Low-T material Fraction of nebular mass H, He Gas H2, He: Transcript


Jupiter Almost nebula composition due to gas capture 20 Mnebula 100 20 Mjupiter 5 Mjupiter is minimum mass required oSaturn Cooler than Jupiter with slightly different composition . – Dept. Physics and Astronomy University of . Hawai`i. Hilo. Daniel . Berke. . – James Clerk Maxwell Telescope . Forest Bremer . - Dept. Physics and Astronomy University of . The Physics and Chemistry of Nebular EvolutionF. J. Ciesla and S. B. CharnleyNASA Ames Research Center Primitive materials in the solar system, found in both chondritic meteorites and comets, recorddi • Based on solar photosphere and chondrite compositions, we can come up with a best - guess at the nebular composition (here relative to 10 6 Si atoms): Data from Lodders and Fegley, Planet Wang, C.-C., and D. J. . Kirshbaum. , . 2015. : Thermally forced convection over a mountainous tropical island. . J. . Atmos. Sci.. , 72, 2484–2506.. Outline. Observations. Control simulations. Sensitivity tests. Session 4 – The Nebular Theory. In the past few sessions we looked at the Big Bang theory and how it tries to explain the universe as a whole. Today we will look on a smaller scale of our solar system, and how the Big Bang theory explains (or doesn’t explain) the formation of the solar system. 25.5. Any theory about the origin of the solar system must explain. why all of the planets’ orbits lie more or less in a plane . Why all of the planets orbit the sun in the same direction. . It must also explain the differences in size and composition between the terrestrial planets and the gas giants.. © 2015 Pearson Education, Inc.. 6.1 A Brief Tour of the Solar System. Our goals for learning:. What does the solar system look like?. © 2015 Pearson Education, Inc.. What does the solar system look like?. © 2015 Pearson Education, Inc.. 6.1 A Brief Tour of the Solar System. Our goals for learning:. What does the solar system look like?. © 2015 Pearson Education, Inc.. What does the solar system look like?. Wang, C.-C., and D. J. . Kirshbaum. , . 2015. : Thermally forced convection over a mountainous tropical island. . J. . Atmos. Sci.. , 72, 2484–2506.. Outline. Observations. Control simulations. Sensitivity tests. WWBAT: Describe the telescopes and define the Nebular Theory. Homework: study for the . quiz tomorrow. Nebular Theory. Gravity. Definition: attractive force bringing items towards itself. Bigger objects have more gravity. . Naturalism . is the doctrine that scientific procedures and laws are applicable to all phenomena.. Evolutionary Theory. . has roots in ancient Greece, as well as Eastern Sources. In fact, evolution is part of the larger question of cosmogony, the study of the origin of the cosmos.. Learn planetary characteristics such as number of moons, size, composition, type of atmosphere, gravity, temperature and surface features.. Understand the movement of planetary bodies.. Understand which planetary characteristics are more important than others when it relates to our understanding of other worlds. . 14 billion years ago. Creation of all matter. Hydrogen and Helium the first. More complex elements evolved through time. The Expanding . Universe. The Doppler effect is used to document the expanding universe. In drug discovery workflow and for compound library generation small molecules must be purified before structures activitiesandpharmacoSample applicationystem softwarecontrols sampleinjection separati

Download Document

Here is the link to download the presentation.
"Main nebular Low-T material Fraction of nebular mass H, He Gas H2, He"The content belongs to its owner. You may download and print it for personal use, without modification, and keep all copyright notices. By downloading, you agree to these terms.

Related Documents