PPT-Studying the dynamics of the Milky Way: Where are we, and

Author : jane-oiler | Published Date : 2017-11-03

Paul McMillan Collaborators James Binney Tilmann Piffl Jason Sanders Two fundamental problems We can only observe positions amp velocities not acceleration

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Studying the dynamics of the Milky Way: Where are we, and: Transcript


Paul McMillan Collaborators James Binney Tilmann Piffl Jason Sanders Two fundamental problems We can only observe positions amp velocities not acceleration Were inside the Milky Way moving with it. Lec21: The Milky Way The Milky Way GalaxyLecture 21APOD Lec21: The Milky WayAtomic, molecular, and ionized gas Lec. 21: The Milky Way21 -2 Lec21: The Milky Way Recap. Canvas homework: due on Wednesday. Lab this week: Galaxy Morphology. Campus Observatory. Milky Way galaxy. Stars: . brightnesses. , masses, sizes, compositions, evolution. Interstellar matter: gas, dust. Mini-University 2013. Our Milky Way . in Space and Time. Our Journey…. Where in the Galaxy Are We?. The Local Neighborhood. Top Milky Way Destinations!. The Dark Heart of the Galaxy. Formation of the Milky Way. William Herschel’s map of the Milky Way based on star counts. In the early 1800’s William Herschel, the man who discovered the planet Uranus, tried to understand the shape of the Milky Way by counting stars. He counted how many stars there were in each of dozens of different directions and then plotted the count versus direction. . Nicholas Cross. , Rob Blake, Ross Collins, Mark Holliman, Mike Read, . Eckhard. . Sutorius. , Nigel . Hambly. , . Andy Lawrence, Bob Mann, Keith Noddle. Wide Field Astronomy Unit, Institute for Astronomy, University of Edinburgh, UK. The Milky Way: Our Home Galaxy. What are the different. components of the Milky Way?. How do we see those components?. What does a map of each component look like from our point of view?. Stars in the Milky Way. Spiral Structure. . The Astronomical Context. By the 1920’s, we knew that the once-mysterious spiral nebulae were flattened galaxies. . Our Milky . Way is . also. flattened. . Two obvious . questions arose:. Our Place Within It. . . The Visible Milky Way. The Milky Way as Seen From Texas. (from Canada, we can. ’. t see the Southern Cross). The Obvious Questions. How big is the Milky Way, and where are we located? At the . bye:. Angelina Battle. The legend of The Milky Way. This is what old people told me when I was a child. Long ago, when the world was new, there were not many stars in the sky. In those days people depended on corn for their food. They would grind it and keep it in bins behind their homes. Bread made from cornmeal, often kept them from starving during the long winter months. . Vital Statistics. It’s our home!. Contains more than 200 billion stars, and a mass of ~10. 12. suns. It’s almost as old as the Universe itself!. 13.7 billion years old. Structure. The core and spiral arms are of different . Contains more than 100 billion stars. Is one of the two largest among 40 galaxies in the Local Group. Our Solar System is located a little more than half way from the galactic center to the edge of the galactic disk.. Chapter 2. Lesson 1. Studying Geography. Physical maps show land and water features.. Studying Geography. Political maps show the names and borders of countries.. Studying Geography. Special purpose maps show patterns such as climate, natural resources, or population.. Here’s the mystery story we’ll unfold…. Fuzzy blobs in the sky – new solar systems, or “galaxies”?. Observational tests. Herschel’s map of the “universe” . (what we today know as just our Galaxy). László Dobos, Tamás Budavári, Carrie Filion,. Rosie. Wyse, Alex Szalay. Dept. . of . Physics. & . Astronomy. , The . Johns. Hopkins University. Subaru . Prime. . Focus. . Spectrograph. Manua.

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