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Published byDennis Hoover Modified over 9 years ago
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Astrophysics and Cosmology Some of the biggest ideas of the last 100 years Of the Stars, the Universe and Everything!!! (the answer is 42... )
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Star Life Cycle: Birth Stars are born out of a cloud of dust Dust Collapses together due to gravity When sufficient heat and pressure, nuclear fusion starts – Atoms combine – Releasing lots of Energy – Star shines
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Star Life Cycle: Life Our sun is a typical star Typical lifetime is 10 billion years for sun- sized star Combines Hydrogen into Helium Hotter stars burn brighter, Blue Colder stars burn Red
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Star Life Cycle: Death the form star-death takes depends on star’s size
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Star Life Cycle: Supernova Heavy stars can collapse in a Supernova Two types of Supernova – Small star eats bigger star (Ia) – Massive star collapse (IIa)
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Some History Supernovae observed by Chinese and Arab astronomers (1006 ACE, possibly others) Tycho observed a supernova in 1572 – Convinced him that stars change – A nail in the coffin of Aristotelian “spheres” Most recent in Milky Way observed by Kepler in 1604 Nova means “new” Supernovae are “new” stars – they appear suddenly – Are brightest in sky for a month – Visible during daytime – Visible at night for a year or two – Leave behind a Nebula
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Supernova Part of Cycle Shockwave drives nebular gas together Creating more dense clumps of gas Igniting new stars Supernovae produce and spread heavy elements – So we are “star stuff”
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Star Life Cycle: Black Hole Large enough star collapses So dense, that light’s path is bent by gravity as it travels – Gravity so strong – Light can’t escape: Black Hole
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Black Holes – Very Weird Center – Singularity Edge: “Event Horizon” – Anything falling in is gone forever Time slows to a stop inside Inside event horizon, forces rip matter apart “Rip” in Space-Time Gravity can swallow other stars or planets – Making Black Hole bigger
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Cosmology: The Big Bang
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Edwin Hubble (of Hubble telescope) big name Saw galaxies moving away from each other – Tracing backwards, then... All matter in the universe starts off at one point -- “singularity” Expands outward rapidly – “Inflation” Matter at first “hot soup” of particles
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The Process Expands, cools into atoms Atoms clump up into gas Gas clumps up into stars and galaxies Process currently theorized to take place over 13.75 billion years
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Cosmology: Evidence – Universe Expanding
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Arno Penzias and Robert Wilson 1965: Cosmic Microwave Background Had Antenna to measure microwaves Looking for point sources (Stars!) Found constant buzz through all of sky Thought there was a problem – Cleaned out bird poo – Buzz still there Evidence for: the Big Bang
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What does it mean? Radiation released when matter first formed Went in all directions Universe expanded This light is only getting to us now – 13.75 billion years later! – From the edge of the Universe Uneven parts are clumps – That later became galaxies
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Dark Matter The Galaxies are rotating faster than predicted – What force causes the galaxies to rotate? – What does it mean if they rotate fast? – And what does that imply? Dark Matter – Acts like matter in terms of gravitational pull – Unlike normal matter (stars, dust), emits no radiation – Hence “Dark”, we can’t see it It’s a “Conceptual Placeholder”
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Dark Matter is a “Conceptual Placeholder” If we stick with Newton’s Theory of Gravity, we need it Might be made of new particles Or just lots of planets we can’t see – According to Newton/Einstein theory, 83% of matter in the Universe is Dark Matter Or maybe the Theory’s just insufficient as it is... We don’t really know
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