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Chapter 26.4

Chapter 26.4. Groups of Stars. Groups of Stars: Constellations Stars that seem to form a picture. These stars are may or may not be close to one another. Constellations. Circumpolar – “Circle” North and South Pole Can be seen all year

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Chapter 26.4

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  1. Chapter 26.4 Groups of Stars

  2. Groups of Stars: Constellations Stars that seem to form a picture. These stars are may or may not be close to one another.

  3. Constellations Circumpolar – • “Circle” North and South Pole • Can be seen all year Ex: Ursa Major (Big Bear with the Big Dipper), Draco (Dragon) Polaris = North Star

  4. Constellations Zodiac – “Birthday” Constellations “Move” on the ecliptic line – and can only be seen during certain months. The month of your birthday, you cannot see your zodiac constellation because it is BEHIND the sun.

  5. Binary Stars – Two stars orbit around a shared center of mass Alcor and Mizar in the Dipper appear as double stars Over 65% of stars may have companion stars. “Star System” 2 or more stars orbit around a center of mass.

  6. Other groups of stars Open Clusters – PleiadesA cluster of 100s - 1000s of stars – in this case young blue stars Closed (Globular) ClustersOlder stars densely packed.

  7. Galaxies = Groups of millions - trillions stars that are held together by gravity. Milky Way Stats 100 000 LY across 2 000 LY thick 5 Spiral Arms Our sun is 2/3 the way out on the Orion spiral arm. Moves around center at a speed of 500,000 mi/hr (It takes 200 million yrs to complete one rotation) Try this simulation: http://amazing-space.stsci.edu/resources/explorations/galaxies-galore/build/index.html http://www.telescope.org/btl/data/01904.gif

  8. A. Central Bulge – Most stars are located here. Old stars are concentrated here. Possible location for BLACK HOLES B. Disk – Flattened pancake of young stars C. Arms – Lanes that radiate from center – Young blue stars D. Halo – surrounds bulge & arms. Contains old stars, globular clusters, & possibly dark matter. Types of Galaxies Spiral C D Spirals have a good deal of dust & gas B A B A http://www.telescope.org/btl/data/01904.gif

  9. Types of Galaxies Spiral-Barred – Types of Galaxies - Ellipitical Elliptical Galaxies are shaped like ovals or footballs. They are dense and the stars in them are VERY OLD. Stars “swarm” around like bees inside. The giant elliptical galaxy M87 (AAO)

  10. Types of Galaxies – Irregular • No real shape • Common in distant (early) universe • Younger stars, gas, & dust • Sometimes a result of galaxy collisions Test your knowledge of galaxy types here!: http://amazing-space.stsci.edu/resources/explorations/galaxies-galore/hunt/index.html

  11. Quasars Very distant objects that release energy in outputs = to that of hundreds of GALAXIES combined Quasars may be powered by SUPERMASSIVE black holes that “accrete” galaxies.

  12. Galaxy Collisions Simulations: http://www.cita.utoronto.ca/~dubinski/tflops/ The Milky Way is predicted to collide with our larger neighbor Andromeda in about 5 billion years. (It is approaching us at 670,000 mi/hr). Eventually they may merge to form an elliptical galaxy. Because stars are so far apart – it may have no affect … then again – we could get ejected out of our “place” on the Orion arm due to collision.

  13. Deep Space Hubble Telescope takes a picture of deep space. Each “star” is actually an entire galaxy made up of billions of stars. Many of these galaxies are over 13 billion LY away. It took light 13 billion years for the light to travel to us.

  14. Groupings of Galaxies The Milky Way orbits in a circle with a group of neighboring galaxies called our LOCAL GROUP. These GROUP of GALAXIES orbits with other GROUPS of GALAXIES in a SUPERCLUSTER Our Official Address: Planet Earth Sol Solar System Orion Arm, Milky Way Galaxy Local Group Virgo Supercluster Observable Universe This is Andromeda – one of the spiral galaxies in our Local Group (2.2 million LY)

  15. Magnitude = Star Brightness Some stars seem brighter than others. Brightness (Magnitude) depends on.. a. Closeness (closer brighter) b. Size (bigger = brighter) c. Temperature (hotter = brighter) Magnitude Scale -1 0 1 2 3 4 Very Bright Bright Dim Absolute Magnitude = How bright something REALLY is Apparent Magnitude = How bright it SEEMS (maybe its close)

  16. Magnitude Questionshttp://www.enchantedlearning.com/subjects/astronomy/stars/bright.shtml Star A has a magnitude of 2 Star B has a magnitude of 1 1. Which is brighter? 2. Bernard’s Star is one of the closest stars to us. It has a magnitude of 8. What conclusions can you make about Proxima Centauri based on this?

  17. Parallax http://instruct1.cit.cornell.edu/courses/astro101/java/parallax/parallax.html Black Hole Song/Visual http://www.rdrop.com/users/green/school/form.htm

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