PPT-The Formation, Evolution,

and Future of Binary Stars Max Moe University of Arizona Einstein Fellows Symposium Oct 12 2017 Formation of Very Close Binaries 80 of solartype binaries with P inner lt 7 days have tertiary companions. 149 1998 D Lazzaro et al eds ORBITAL RESONANCES AND CHAOS IN THE SOLAR SYSTEM Renu Malhotra Lunar and Planetary Institute 3600 Bay Area Blvd Houston TX 77058 USA Email renulpijscnasagov Abstract Long term solar system dynamics is a tale of orbital r Thorsten Naab . MPA, . Garching. . What regulates galaxy formation? . Leiden, April, 22. nd. How do massive galaxies get their gas and stars?. Gas accretion involves dissipation – energy can be radiated away . Galaxies. T.Naab. , P. Johansson, R. . Cen. , K. . Nagamine. , R. . Joung. . and J.P.O.. PPPL:, 19 Dec . 2012. ApJ.L.,. 658,710 . (2007) ApJ.,697, . 38 . (2009). ApJ.L.,699,L178 (. 2009. ). ApJ.,725,2312 . . CDM Cosmology. Oleg . Gnedin. (University of Michigan. ). What we knew before HST: globular clusters are old, dense, compact – a distinct type of stellar spheroids. Kormendy. (1985). Over 20 years the Hubble Space Telescope has revealed young massive star clusters in interacting and gas-rich galaxies.. e. arly type galaxies. and their dark matter haloes. Gian. Luigi . Granato. . INAF – Trieste. Cinthia. . Ragone. -Figueroa. Mario . Abadi. IATE-Cordoba. Plan:. Generalities on the problem. Why puffing-up cannot explain what we see so far. Christopher W. Ashcraft M.S., M.Ed.. Big Bang vs. Creation. Origin of Stars. Solar System: Evidence of Design. Age of the Cosmos. Are we being told all the evidence or just selected information to support a particular idea?. Prof. Gerhardt R Meurer. Galaxy evolution in a nutshell. Galaxy Evolution. 2. Time machines. The farther we peer. The farther back in time we see. Reveal cosmic history. Hubble: to < 1 . Gyr. after big bang. Embryonic Mouth Formation. Non-molting vs. Molting. Review. Animal Evolution. What’s this?. Deuterostomia. Protostomia. Embryo Formation. Deuterostomia. Protostomia. Embryo Formation. Non-organs vs. Organs. Boshongo. people of central Africa, in the beginning, there was only darkness, water, and the great god . Bumba. . One day . Bumba. , in pain from a stomach ache, vomited up the sun. The sun dried up some of the water, leaving land. Still in pain, . The INITIAL patterns of evolution L eonid E. Grinin Laboratory for monitoring of socio-political destabilization risks, HSE THE ORIGINS OF THE WORLD’S FUNDUMENTALS AND THE BASIC SIMILARITIES OF THE MATTER Formation of the Moon Before visit to the Observatory Overview Introduction to the Formation of the Moon Video about the Evolution of the Moon Classroom demonstrations on distances to the Moon Classroom activity – Craters on the Moon Warm Up: Set up your notes in your notebook. Page: 55. Title: Cladograms. Date: 1/18. EQ: How can I model divergent evolution. Standard. : B8B Categorize organisms using a hierarchical classification system based on similarities and differences shared among groups. Michelle Kirchoff. Southwest Research Institute. Center for Lunar Origin and Evolution. Southwest Research Institute in Boulder. http://. www.boulder.swri.edu. /. Center for Lunar Origin and Evolution (CLOE). Where we are and . where we are going.. D.J. Pisano . (WVU). djpisano@mail.wvu.edu. The Big Questions . How does the gas content of galaxies evolve over cosmic time and in different environments?. How does gas flow into and out of galaxies?.