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Angels Kicking All The Options Around For Outfield - RealGM Wiretap
The Los Angeles Angels have been linked to big-name outfielders this offseason and even with Jason Heyward off the board Thomas Jaguaribe Bedinelli Jersey , Yoenis Cespedes, Chris Davis and Justin Upton remain available.


Billy Eppler said he is still "having conversations" with agents for the sluggers, "and we're kicking all the options around."


Eppler also made comments about looking for well-rounded players for the Angels' offense, which may indicate that Alex Gordon is a target.

Four Umpires Get First World Series Assignment - RealGM Wiretap

A handful of Major League umpires will work in the World Series for the first time next week.


The seven-man crew includes a rare four newcomers, according to a source.


Hunter Wendelstedt, Eric Cooper, Jim Reynolds and Jerry Meals will be the first-time umpires in the Fall Classic.


Jeff Kellogg will be the crew chief and call his fifth World Series when Kansas City hosts San Francisco in Game 1 on Tuesday night. Ted Barrett and Jeff Nelson will work the Fall Classic for the third time.

Rangers Wont Receive Compensation If Napoli Signs Elsewhere - RealGM Wiretap

The Rangers did not issue a one-year Stefan Frei Jersey , $13.3 million qualifying offer to Mike Napoli by Friday's deadline, meaning they won't receive compensation if he signs elsewhere as a free agent.


Texas has interest in re-signing Napoli, but they didn't want to risk having to pay him $13.3 million if he accepted the offer.


Napoli made $9.4 million in 2012. A salary of $13.3 million would have made him the third-highest-paid catcher in baseball behind Joe Mauer ($23 million annually) and Yadier Molina ($15 million annually).

锘? Black holes are among the strangest objects in the Universe. Hard to find, hard to explain, hard to understand and hard to imagine they defy the known laws of physics at their centre and provide mind boggling results at their edges. A black hole is impossible to see but there has been enough evidence to certify their existence. They are an important part of the solar life cycle and perhaps an even more important factor in galaxy formation.

In 1785 a man named Peirre Simon Laplace concluded that if enough mass were packed into a sufficiently small space that the gravity would be so intense that not even light would be able to escape. The idea is based on escape velocities being proportional to the mass of an object. For example, the energy needed to escape the gravitational pull of Earth is 19,700 mph greater than what is needed to break free of the Moon.

Laplace theorised that when gravity reaches a massively high value that the escape velocity would be faster than the speed of light Roman Torres Jersey , trapping light particles and rendering the object invisible. During the early 20th century physicists such as Oppenheimer, Volkoff, Snyder and notably Karl Schwarzschild would refine the theory and provide mathematical formulae to back it up.

The only known way for a black hole to form is from the death of a massive star, this is the only way that such a huge mass can be packed into such a small volume. During the main phase of their life stars are trying to explode through nuclear fusion but at the same time are held together by their own gravity. These two forces balance the volume of the star and will define its size.

When the star runs out of fuel for nuclear fusion then there is no outward force and so gravity causes it collapse in on itself. The collapse heats up the core to a massive degree and will cause a supernova explosion. After the supernova all that is left of the star is a highly compressed core, continually collapsing under its own gravity. The gravity becomes so strong that light cannot escape and so a black hole is formed.

Black holes effect spacetime in strangely different ways to other bodies. They cannot be seen by visible light, but have a number of interesting properties. The defining feature of black holes is the event horizon, a real point of no return. The event horizon is the point at which the gravity becomes so intense the the escape velocity reaches light speed. The horizon surrounds the singularity at the centre of the black hole and effectively forms the mouth of the black hole. From the outside Osvaldo Alonso Jersey , nothing inside the event horizon can be seen.

Outside the event horizon objects can orbit the black hole like they would any other large body of mass. The escape velocity will increase the closer you get to the horizon, but at a large enough distance the orbit will be no different to orbiting a star or planet

Crossing the event horizon will prove fatal to anyone that tried. In theory if one were able to cross an event horizon in a spacecraft it would seem initially unremarkable. Far away objects would appear distorted due to gravitational lensing but you would still be able to see out of the black hole into space. As your craft flies further from the horizon it would experience tidal forces so strong that eventually it would torn apart, right down to the atomic level. The time frame for this happening varies depending on the size of the singularity at the centre but is typically just a few seconds.

What can be confusing is thinking about what a distant observer would see as your doomed craft flew into the black hole. As the approach to the event horizon is made the light will take longer and longer to leave the craft because of the intense gravitational pull. This would make it seem as if the c