* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Download 10 relativity, black holes_
Astrobiology wikipedia , lookup
Dyson sphere wikipedia , lookup
International Ultraviolet Explorer wikipedia , lookup
History of Solar System formation and evolution hypotheses wikipedia , lookup
Perseus (constellation) wikipedia , lookup
Rare Earth hypothesis wikipedia , lookup
Extraterrestrial life wikipedia , lookup
Cygnus (constellation) wikipedia , lookup
Astronomical unit wikipedia , lookup
Formation and evolution of the Solar System wikipedia , lookup
Planetary habitability wikipedia , lookup
Dialogue Concerning the Two Chief World Systems wikipedia , lookup
Astronomical spectroscopy wikipedia , lookup
Aquarius (constellation) wikipedia , lookup
Stellar kinematics wikipedia , lookup
Star formation wikipedia , lookup
Corvus (constellation) wikipedia , lookup
Kerr metric wikipedia , lookup
Hawking radiation wikipedia , lookup
Agenda Types of star deaths Relativity Black holes Evidence for both Start registering your clickers. There’s a link from webct. H runs out: star becomes a red giant Exterior expanding H fusing He core contracting Mass alone determines death Small mass: White dwarf Med. Mass: Neutron star or pulsar Large mass: Black hole Determined by S. Chandreskhar What type of death will our Sun die? What will happen to us? Diameter (times present value) Sun’s fate Orbits of: Mars Earth Venus Mercury 100 10 Helium shell flashes Contraction Leaves Main sequence Now 1 0 5 First Red giant peak White dwarf 10 12.1 12.2 12.3 12.3650 12.3655 Age (billions of years) Diameter (times present value) Sun’s fate Orbits of: Mars Earth Venus Mercury 100 10 Helium shell flashes Contraction Leaves Main sequence Now 1 0 5 First Red giant peak White dwarf 10 12.1 12.2 12.3 12.3650 12.3655 Age (billions of years) Diameter (times present value) Sun’s fate Orbits of: Mars Earth Venus Mercury 100 10 Helium shell flashes Contraction Leaves Main sequence Now 1 0 5 First Red giant peak White dwarf 10 12.1 12.2 12.3 12.3650 12.3655 Age (billions of years) Death of a low mass star Red giant shrinks, becomes very hot Expands to become a red giant again Outer layers ejected into space. Death of a low mass star Planetary nebulae are formed Eventually becomes a white dwarf On the HR diagrams, white dwarf stars are A. B. C. D. On the upper right On the upper left On the lower right On the lower left The Hertzsprung-Russell (HR) Diagram Absolute magnitude -10 Main Sequence Stars -5 Red Giant Stars 0 5 Sun White Dwarf Stars 10 15 O B A F Spectral Class Hot, not too bright G K M Higher mass stars Fusion of heavier elements Contraction (increasing temperature) Cycle continues until core is made of Fe (iron) Death of higher mass stars Explodes in a type II supernova Then becomes a neutron star or a black hole Supernova 1987A (Type II) Gas from the explosion hitting cool ring of gas 1994 2003 NASA Neutron stars Fe core collapses Electrons enter nuclei, neutrons and neutrinos formed Carries energy outward, causing an explosion Neutron star or black hole? If very massive it becomes a black hole Otherwise it the remaining core is called a neutron star If this spins, we call it a pulsar Jocelyn Bell Burnell discovered pulsars! What’s a theory? Start with an hypothesis Must fit evidence Testable Falsifiable Einstein’s theory of Relativity Fits evidence? Testable? Falsifiable? Relativity in a nutshell Matter tells space-time how to curve Space-time tells matter how to move Evidence – time dilation Sun Earth Viking Lander sent a signal to Earth Space was stretched, so time was too! Viking Lander Evidence – GPS Many of us own GPS receivers. Uses time signals from satellites orbiting Earth. Does not work unless corrected for relativity! wikipedia; DoD Evidence: Wobble of Mercury Shown by Einstein Cornell Evidence: gravitational lensing Demo: bending light Evidence: gravitational lensing Evidence: gravitational lensing Demo: Lensing in water When a star stops fusing If it has more than 25 X M sun No outward force can resist gravity It will become a black hole Nothing on the surface can escape (including light) What forces act between a black hole and a nearby object? Gravity is the only force acting!!!! Depends on: Mass of objects Distance between them If the sun turned into a black hole, what would happen to the Earth? Can you get sucked into a black hole? Escape velocity How fast does the shuttle have to go in order to leave Earth’s surface? 7 miles every second! (25,000 mph) The moon? 5320 mph The Sun? 1.38 million mph Escape velocity Depends on the gravity between you and the object you want to escape! For a black hole, the escape velocity (inside the event horizon) is greater than the speed of light! Do Black Holes Really Suck? event horizon Normal Weird Singularity The center of a black hole is a sphere (so is the event horizon) Field trip to a black hole!! event horizon Normal Weird Singularity Volunteers? At the event horizon Time slows waaaaayyy down Someone jumping in would die a nasty death Someone watching would see the person freeze in time Finding black holes How can we see something that emits no light? Look for binary systems Make sure candidate is not a neutron star! Finding black holes Matter near the black hole is traveling close to the speed of light When it rubs together, it gives off x rays we can see NASA/CXC Summary Relativity tells us space and time can be stretched Escape velocity, event horizon Black holes can be found, but not directly seen