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URL - StealthSkater
URL - StealthSkater

... humans are not up to the task, creatures from other planets may try. So why are we not overrun by visitors from the Future? This is the argument used by the famous English physicist Stephen Hawking in what he called his "Chronology Protection Conjecture". Like many other scientists, Hawking is troub ...
Lec11_2D
Lec11_2D

... Between any two stars are gravitational balance points, where the attraction of one star equals the attraction of the other. The point directly between the stars is called the Lagrange point. The balance points in general map out the star’s Roche Lobe. If a star’s surface extends further than its Ro ...
General relativistic cosmology
General relativistic cosmology

PHYS 2410 General Astronomy Homework 8
PHYS 2410 General Astronomy Homework 8

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... We introduce here a relativistically consistent software called RMI (Relativistic Motion Integrator). We compare it with the GINS software [2] as an example of the classical approach consisting in the Newtonian formalism plus relativistic corrections. GINS is a software routinely used to evaluate th ...
ppt
ppt

... Those problems are especially relevant when modeling tiny geophysical effects through orbitography, like for example the waxing-waning mechanism of the Martian polar caps, with temporal frequencies in the same band as relativistic effects. In the more appropriate frame of General Relativity, we stud ...
Document
Document

... Momentum => Rotation rate: few to many times per second!!! Huge Magnetic field: 1012 x Earth's! What type of object can these conditions produce? ...
- Europhysics News
- Europhysics News

... He would probably be first struck by the density of stars around him: one million times larger than in the sun’s neighbourhood. He would also be amazed by the beauty of mixed blue and red luminous ribbons that wrap as some spiral arms around what appears as a dense cluster of particularly bright sta ...
Compact Objects in the Solar System
Compact Objects in the Solar System

... http://lh3.ggpht.com/_4ruQ7t4zrFA/SdG3vEI963I/AAAAAAAAB70/Yb5XCaaVlTQ/earth-orbiting-black-hole.jpg ...
Astronomy news
Astronomy news

MasteringPhysics: Assignmen
MasteringPhysics: Assignmen

... The Schwarzschild radius of an object is the distance within which nothing, not even light, can escape its gravitational attraction. The sphere surrounding a black hole whose radius is the Schwarzschild radius is also called the event horizon. Part E Would a black hole of this size fit inside the ea ...
Black Holes
Black Holes

... Spacetime is not a static background where Newtonian physics happens; spacetime is a dynamic fabric with definite, physical properties. ...
ppt
ppt

... error prone. Those problems are especially relevant when modeling tiny geophysical effects through orbitography, like for example the waxing-waning mechanism of the Martian polar caps, with temporal frequencies in the same band as relativistic effects. In the more appropriate frame of General Relati ...
Blackholes - Indiana University Astronomy
Blackholes - Indiana University Astronomy

... • Event Horizon – The boundary that marks the “point of no return” between a black hole and the outside universe. Events that occur within the event horizon can have no influence on our observable universe. • Schwarzschild Radius – A measure of the size of the event horizon of a black hole. ...
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File

AP Physics - Froehlich`s Physics
AP Physics - Froehlich`s Physics

Monday, April 17, 2017 Exam 4, Skywatch 4, Friday, April 21
Monday, April 17, 2017 Exam 4, Skywatch 4, Friday, April 21

Angular Momentum of Dark Matter Black Holes
Angular Momentum of Dark Matter Black Holes

Short theoretical questions – solutions
Short theoretical questions – solutions

... Taking into account other kind of orbits (without peri and apogeum) one has to make the angle  free (unfixed). The assessment is that 2 point for each element ...
Massive Star (10 to 15 times the size of our Sun) Nuclear Fusion
Massive Star (10 to 15 times the size of our Sun) Nuclear Fusion

Black Holes: Myths, Legends and Truths
Black Holes: Myths, Legends and Truths

Math Notes - UNC Physics and Astronomy
Math Notes - UNC Physics and Astronomy

...  G = Newton’s gravitational constant  c = speed of light  Recall the escape speed equation from Lesson 2:  vesc = (2GM / R)1/2  Solving for R yields:  R = 2GM / vesc2  Setting vesc = c yields the Schwazschild radius of the object:  Rs = 2GM / c2  If an object of mass M is compressed to the ...
Lesson 1.4 Equations and Inequalities
Lesson 1.4 Equations and Inequalities

... placing an inequality symbol, such as “<“ or “>” between two expressions. < is less than < is less than or equal to > is greater than or equal to > is greater than ...
PowerPoint Presentation - Super Massive Black Holes
PowerPoint Presentation - Super Massive Black Holes

... Brief Review of case for Super-Massive Black Holes in these observed AGN ...
Selected Physical and Astronomical Constants Conversion Factors
Selected Physical and Astronomical Constants Conversion Factors

... comfortable? Do I see the stars overhead as I fall into a black hole? If so, do these stars change position or color as I fall? How fast do I fall? Does my speed reach or exceed the speed of light? Once inside, can I receive messages and packages from my friends on the outside? Is it true that, once ...
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Kerr metric

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