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Download Astronomy – The Milky Way Galaxy
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Astronomy – The Milky Way Galaxy The ______________ _________ Galaxy • Contains more than ______ billion stars • Is one of the two largest among 40 galaxies in the ___________ ____________. • Our Solar System is located a little more than _______________ from the galactic center to the edge of the galactic disk. • Only one of roughly ______ billion ______________ in the Observable Universe. Galaxies • Definition: a system that contains ______________ or ________ stars. • _____________ _____________: groups of galaxies with more than a few dozen members • __________________: galaxies and galaxy clusters ___________ packed together. • Classified using a diagram called “Hubble’s Tuning Fork” Our Cosmic Address 1. 2. 3. 4. 5. 6. Milky Way Galaxy Structure • Known to look like ___________ pancake with a ___________ in the center. • Named a _______________ Galaxy because of its _________ __________. • Approximately ________________ light years away from the nuclear bulge. Parts of the Milky Way Galaxy • _______________ ______________: sphere of stars and other material at the heart of our galaxy. – about 4000 parsecs across (about a fifth of the total spread of the spiral arms of the galaxy.) – The very _____________ of our galaxy is a super-massive __________ _______. • • ___-___ million times as massive as the sun. • Appears to be powering a bright source of radio emission known as Sagittarius A*. Disk: _______, ____________ region of stars, dust and gas called ______________ ___________ around the Nuclear Bulge. – Can obstruct view for observations towards the Nuclear bulge. – Approximately 1,000 light years in thickness and 100,000 light years across • ____________ ________: well defined ________ in the disk because of brilliantly _________ stars. • ____________: ________________ in shape and contains little gas, dust, or star formation. • ______________ _____________: a large _____________ spherical star cluster, typically of _______ stars in the outer regions of a galaxy. Formation of Galaxies 1. A Protogalactic cloud contains _____________ and ______________. 2. Halo stars begin to form as the protogalactic cloud starts to _______________. 3. Conservation of angular momentum ensures the remaining gas ___________ into a disk. 4. Billions of years later, the star-gas-star cycle supports ongoing _________ ______________ within the disk. The lack of gas in the halo _______________ star formation outside the disk. Facts about Galaxies and the Universe • Galaxies move ____________. • Expansion began about _________ billion years ago (the ______ __________) – This is called cosmological _______________. – Proven by observing a faint glow of __________________ that is a remnant of _________ from the Big Bang. – Early Universe = __________ and ____________ – Today’s Universe = __________ and ________ ___________ because of _________________. • If you look at a galaxy that is 7 billion light years away you are seeing that galaxy as it appeared 7 billion years ago. • The number of stars in the observable universe is equal to the number of grains of dry sand on all beaches on Earth. • Large Magellanic Cloud and Small Magellanic Cloud orbit the Milky Way at 150,000 light years and 200,000 light years. Nearby Galaxies (Our Neighbors!) • __________________ Galaxy is comparable in size, though slightly larger. • Small galaxies (Sagittarius and _________ ____________ Dwarf Galaxies) are ____________ with us right now! – These small collisions cause ____________ in our galaxy and create new ________ at points of _______________. ____________ _____________ (1889-1953) • Studied ________ and ______________ outside the Milky Way galaxy. • Designed a period-luminosity relation that proved that Andromeda is much too far _______ to be part of Milky Way. • Known for __________ _________ • The more ____________ the galaxy, the ___________ its moving away = __________________ ___________________ • Galaxies are moving _________ in our _______________ universe.