BLACK HOLES National College Iasi. What is a black hole?  A black hole is a region of space from which nothing, not even light, can escape.  It is the.

Slides:



Advertisements
Similar presentations
General Relativity Physics Honours 2009 Prof. Geraint F. Lewis Rm 560, A29 Lecture Notes 4.
Advertisements

Gravitation Newton’s Law of Gravitation Superposition Gravitation Near the Surface of Earth Gravitation Inside the Earth Gravitational Potential Energy.
Black Holes. Dark stars a star that has an escape velocity greater than the speed of light.
Copyright © 2010 Pearson Education, Inc. Chapter 13 Black Holes.
1. black hole - region of space where the pull of gravity is so great that even light cannot escape. Possible end of a very massive star.
Chapter 11 – Gravity Lecture 2
Scott Johnson, John Rossman, Charles Harnden, Rob Schweitzer, Scott Schlef Department of Physics, Bridgewater State College // Bridgewater MA, Mentor:
How do we transform between accelerated frames? Consider Newton’s first and second laws: m i is the measure of the inertia of an object – its resistance.
1. White Dwarf If initial star mass < 8 M Sun or so. (and remember: Maximum WD mass is 1.4 M Sun, radius is about that of the Earth) 2. Neutron Star If.
Black Holes Old ideas for black holes Theory of black holes Real-life black holes Stellar mass Supermassive Speculative stuff (if time)
Black Holes Dennis O’Malley. How is a Black Hole Created? A giant star (more than 25x the size of the sun) runs out of fuel –The outward pressure of the.
Lecture 18 Black Holes (cont) ASTR 340 Fall 2006 Dennis Papadopoulos.
Chapter 13 Gravitation.
Chapter 12 Gravitation. Theories of Gravity Newton’s Einstein’s.
Levels of organization: Stellar Systems Stellar Clusters Galaxies Galaxy Clusters Galaxy Superclusters The Universe Everyone should know where they live:
Black Holes By Irina Plaks. What is a black hole? A black hole is a region in spacetime where the gravitational field is so strong that nothing, not even.
Announcements Exam 4 is Monday May 4. Tentatively will cover Chapters 9, 10, 11 & 12 Sample questions will be posted soon Observing Night tomorrow night.
BY: Nathan Schmidt Period: 5 Astronomy. A brief history of black holes About 2 centuries ago John Michel was the first person to suggest that it was possible.
Black Holes & Relativity
Black Holes Physics James Chambers. What is a Black hole? The theory of general relativity predicts that a sufficiently compact mass will deform.
Black Hole (BH)  Introduction to BH  Motivation to study BH  Formation of BH  Cool slides  Size of BH  Properties of BH  Evidence for BH.
Chapter 13 Black Holes. What do you think? Are black holes just holes in space? What is at the surface of a black hole? What power or force enables black.
Copyright © 2010 Pearson Education, Inc. Neutron Stars and Black Holes Unit 9.
A black hole is a region of space with such a strong gravitational field that not even light can escape.
Black Holes Escape velocity Event horizon Black hole parameters Falling into a black hole.
Bending Time Physics 201 Lecture 11. In relativity, perception is not reality Gravity affects the way we perceive distant events For example, although.
Copyright © 2012 Pearson Education Inc. Orbital motion, final review Physics 7C lecture 18 Thursday December 5, 8:00 AM – 9:20 AM Engineering Hall 1200.
Teaching Black Holes Donald Marolf, UCSB July 20, 2006.
Black Holes Formation Spacetime Curved spacetime Event horizon Seeing black holes Demo: 1L Gravity Well - Black Hole.
Lecture 27: Black Holes. Stellar Corpses: white dwarfs white dwarfs  collapsed cores of low-mass stars  supported by electron degeneracy  white dwarf.
Lecture 6: Schwarzschild’s Solution. Karl Schwarzschild Read about Einstein’s work on general relativity while serving in the German army on the Russian.
Black hole For large enough masses, as far as we know, nothing is stiff enough to stop the collapse. It continues down to a singularity: a defect in space.
Space Warps. Light is believed to travel the shortest distance between two points But…… the path of light is curved in the presence of a gravitational.
By Katy O’Donohue. Black Holes Black Holes are a region of space from which nothing can escape, including light. Light is made up of massless particles.
Historical SN and their properties Total energy released ~10 54 erg in a few hours.
Black Hole Vacuum Cleaner of the Universe. Formation of Black Hole nuclear fusionnuclear fusion - tends to blow the star's hydrogen outward from the star's.
Black Holes Chapter 14. Review What is the life cycle of a low mass star (
Star Life Cycle Review. Transports energy from the radiative zone to the surface of the sun. Sunspot Corona Photosphere Convective zone.
Physics 311 General Relativity Lecture 18: Black holes. The Universe.
Black Holes Pierre Cieniewicz. What are they? A Black Hole (BH) is a place in space from which nothing can escape The reason for this is gravity Some.
Copyright © 2010 Pearson Education, Inc. Chapter 13 Neutron Stars and Black Holes Lecture Outline.
It was discovered in the early 1990’s that the pulse period of a millisecond pulsar 500 parsecs from earth varies in a regular way.
Neutron Stars & Black Holes (Chapter 11) APOD. Student Learning Objective Indentify properties of Neutron Stars & Black Holes NASA.
BLACK HOLES Project by Grigorescu Mihai Cristea Flavius.
BLACK HOLES
Announcements Grades for third exam are now available on WebCT Observing this week and next week counts on the third exam. Please print out the observing.
Einstein’s relativity Y&feature=relatedhttp:// Y&feature=related Did Newton's.
Universe Tenth Edition
General Relativity and Grade-9 Astronomy. 0) Gravity causes time to slow down. Everyday Einstein: The GPS and Relativity OAPT Conference May 12 – 14 McMaster.
A black hole: The ultimate space-time warp Ch. 5.4 A black hole is an accumulation of mass so dense that nothing can escape its gravitational force, not.
Copyright © 2010 Pearson Education, Inc. Clicker Questions Chapter 13 Neutron Stars and Black Holes.
Astronomy: A Beginner’s Guide to the Universe Seventh Edition © 2013 Pearson Education, Inc. Neutron Stars and Black Holes Chapter 13 Clickers.
Black Holes A stellar mass black hole accreting material from a companion star 1.
Chapter 14: Chapter 14: Black Holes: Matters of Gravity.
 Sun-like star  WHITE DWARF  Huge Star  NEUTRON STAR  Massive Star  BLACK HOLE.
18 October 2001Astronomy 102, Fall Today in Astronomy 102: “real” black holes, as formed in the collapse of massive, dead stars  Formation of a.
Neutron Stars & Black Holes (Chapter 11) APOD. Student Learning Objective Indentify properties of Neutron Stars & Black Holes NASA.
© 2017 Pearson Education, Inc.
Supernovas Neutron Stars and Black Holes
A neutron star over the Sandias?
Exam Monday Covers reading and related notes from chapters
Black Holes By Katy O’Donohue.
It was discovered in the early 1990’s that the pulse period of a millisecond pulsar 500 parsecs from earth varies in a regular way.
The Rotating Black Hole
Black Holes.
Chapter 22 Black Holes Chapter 22 opener. Neutron stars and black holes are among the more exotic members of the vast population of stars throughout the.
Active Figure 13.1  The gravitational force between two particles is attractive. The unit vector r12 is directed from particle 1 toward particle 2. Note.
Parts, existence of, origin,
Black Holes Chapter 14.
Black Holes Escape velocity Event horizon Black hole parameters
Presentation transcript:

BLACK HOLES National College Iasi

What is a black hole?  A black hole is a region of space from which nothing, not even light, can escape.  It is the result of the deformation of spacetime caused by a very compact mass. National College Iasi More about the black holes

Why it’s call ‘black’?  It is called "black" because it absorbs all the light that hits it, reflecting nothing, just like a perfect black body in thermodynamics. thermodynamics National College Iasi

Simulation  Lensing by a black hole. Animated simulation of gravitational lensing caused by a Schwarzschild black hole going past a background galaxy.Schwarzschild National College Iasi

Event horizon Far away from the black hole a particle can move in any direction. It is only restricted by the speed of light. Closer to the black hole spacetime starts to deform. There are more paths going towards the black hole than paths moving away. Inside of the event horizon all paths bring the particle closer to the center of the black hole. It is no longer possible for the particle to escape. National College Iasi

Singularity  At the center of a black hole as described by general relativity lies a gravitational singularity, a region where the spacetime curvature becomes infinite.  For a non-rotating black hole this region takes the shape of a single point and for a rotating black hole it is smeared out to form a ring singularity lying in the plane of rotation. National College Iasi

Accretion of matter

Photon sphere  The photon sphere is a spherical boundary of zero thickness such that photons moving along tangents to the sphere will be trapped in a circular orbit. National College Iasi

Ergosphere The ergosphere is an oblate spheroid region outside of the event horizon, where objects cannot remain stationary. National College Iasi

The Youngest Black Hole Near Earth

As you can see in the image attached to this article there is a supernova within the M100 galaxy that astronomers from NASA think it can contain the youngest black hole, near in our neighborhood. The image shows Chandra’s X- rays which are gold colored, while the data collected from the ESO Telescope shows them in red and blue, and the data from Spitzer shows them in red. The location of this awesome supernova is labeled as SN1979C. National College Iasi

Authors  Carp Roxana Paula  Condurache Andreea Geanina National College Iasi