Island Universes. Up to 1920 s, many thought that Milky Way encompassed entire universe.
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1 Island Universes Up to 1920 s, many thought that Milky Way encompassed entire universe. Observed three types of nebulas (clouds): - diffuse, spiral, elliptical - many were faint, indistinct - originally listed in Messier catalog - assumed to be within the Milky Way - some thought to be forming solar Systems Edwin Hubble - using largest telescope in world inch (2.5 m) telescope on Mount Wilson near Los Angeles - could see individual stars in some nebulas - including Cepheid variable stars - pulsating giant stars -period related to luminosity - can determine distances
2 - many nebulas were - entire galaxies far outside the boundaries of the Milky Way - distances more than 1 million ly! Milky Way is one of many island universes Diffuse nebulas clouds of gas & dust Spiral, Elliptical nebulas distant galaxies with billions of stars
3 The Local Group A cluster of galaxies including : -The Milky Way Galaxy -The Andromeda Galaxy -over 50 smaller galaxies -roughly 3 million light years across
4 M31, Andromeda Galaxy M33, Triangulum Galaxy Small/Large Magellanic Clouds
5 The Local (Virgo) Supercluster An enormous region of space containing: -The Local Group -The Virgo Cluster -up to 100 other galaxy clusters -up to 100 million light years in size
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8 Hubble Deep Field Survey
9 Hubble Deep Field with Redshifts z = 1.0 r = 7.8 billion ly z = 4.0; r = 12.0 billion ly
10 Hubble Ultra Deep Field: 1,000,000 second exposure (11 ½ days) Most distant object ever observed!! z = 11.9; r = 13.3 billion ly
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12 Cosmology and the Evolution of the Universe Edwin Hubble, 1929: -almost all galaxies have a redshift -moving away from us -greater distance greater redshift
13 Implications of the Hubble Law: - Universe is changing (getting bigger!) - it is not static, unchanging - Universe had a beginning!! - could not have been expanding forever HUBBLE LAW: v = H o r v = velocity (speed); r = distance
14 Rate of expansion: H o = Hubble constant (slope of line) The Hubble Constant tells us: - Size of observable universe largest redshift = largest distance - Age of universe how long ago everything was together - Fate of universe what will happen in future Most accurate measurements (2014): H o = 70.4 to 74.3 km/s per Mpc Age = to billion years The Big Bang Model Universe began from a single point - that was extremely dense and hot Cosmic Singularity
15 - "Explosion" of matter and energy (and space and time!) -today, still expanding - properties of universe change with time - had different conditions in the past - will have diff. conditions in future - ultimate fate is unknown The Early Universe: Initially was very HOT! - Hot enough for Hydrogen fusion everywhere in space! - explains why 25% of universe is Helium Basic Principles of Big Bang Model 1. Universe cools as it expands: Time Temperature 0.01 s 100 billion Kelvin 180 s 1 billion Kelvin 400,000 yrs 3000 Kelvin
16 2. High energy radiation (photons) create matter E = m c 2 Gamma Rays electron positron 3. Energy of radiation (photons) depends on temperature of universe - As universe expands and cools - radiation loses energy - universe is a blackbody PREDICTION: According to Big Bang Model: What is temperature of universe TODAY? Prediction: 3 Kelvin (1964, Peebles and Dicke, Princeton Univ.)
17 1964, A. Penzias and R. Wilson (Bell Labs) -built antenna for satellite communications -detected "noise" in all directions -background noise corresponds to temperature of 3 Kelvin! Energy leftover from the BIG BANG!!! Cosmic Microwave Background (CMB)
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19 1989, satellite COBE - accurate measurements of Cosmic Microwave Background - Temperature of Universe: T = / K
20 Expansion of the Universe: - the space between objects is expanding - objects are not moving through space.
21 Cosmological Principle: - there is no center, no edge - every location appears to be at center - same at every location (large scales) Homogeneous - same appearance in every direction Isotropic
22 Clusters, Superclusters, Voids - origins should be seen in the CMB , temp fluctuations of K - seeds of large scale structure Surprising Discovery in 1998: - rate of expansion is increasing! - previously thought that gravity would slow expansion over time - what can overcome affects of gravity? - repulsive, anti-gravity force - Dark Energy
23 Fate of the Universe: Three Possible Fates: - based on overall density of universe - need to know total mass - need to know overall size (H o )
24 Closed Universe: - expansion will eventually stop - gravity will cause universe to collapse - Universe will end in "Big Crunch" - maybe start again (?) Overall geometric shape of universe is spherical
25 Flat universe: - expands forever, always slowing down - not enough gravity to start collapse - Universe will end in Cold Death - all forms of energy becomes evenly distributed in space. - everywhere in universe is same temperature -close to absolute zero Overall shape of universe is flat. - Flat universe is predicted by current theories.
26 Open Universe: - expands forever, possibly going faster and faster - dark energy overwhelms gravity - Universe will end in Big Rip - dark energy overwhelms all other forces. - expansion will accelerate so much, all matter will get ripped apart Overall shape of universe is hyperbolic.
27 TIME seconds seconds seconds seconds 400,000 yrs 1 2 billion years 9 10 billion years Today (14 billion years) EVENT The Planck Time: Nothing is known during this time.? Inflation: Universe goes through period of enormous expansion, grows by factor of 10 43!! Production of Matter: quarks and electrons created from extremely hot photons Nucleosynthesis Era: 2 H and 4 He created by fusion reactions throughout the universe Era of Recombination: Electrons combine with nuclei to form atoms; (T = 3000 K), space is now transparent Formation of Galaxies: Young galaxies seen as quasars Formation of Solar System: Sun and planets form within the Galaxy (4.6 billion years ago) Universe still expanding; Average temperature T = K Radiation Dominated Universe (Primordial Fireball) Matter Dominated Universe (Transparent)
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Cosmology and the Evolution of the Edwin Hubble, 1929: -almost all galaxies have a redshift -moving away from us -exceptions in Local Group -with distance measurements - found a relationship greater distance
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