07/27/2017

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The Time Misconception number 3. In order to be successful and all have time, you must learn to do things quickly and efficiently. With this approach, we fill the day before the rejection by various chores and tasks, trying to get done as soon as possible more and fill in any spare time with something useful. In this part of the processes are crumpled up and poorly executed - a report drawn up in haste, which would still have to adapt, lunch on the run, not bringing any benefit or pleasure, a quick visit to the client, not leading to improved relations. However, many important matters remain outstanding at all - sports, time with family, self-development. If you learn to perceive your day as the limited space that can accommodate only a certain number of cases and events that you consciously choose precisely the problem that you are really important in this the period of your life. Misconception number 4. Need to compile a list of important things not only for the day, but weekly and monthly. Discard the compilation of lists of cases and replace it with a list of main areas in which you work this period of life. Firstly, in terms of reality - you must be flexible enough to respond to the diverse contingencies that continually arise in life. And it means that your the list will still be constantly changing and updated. Secondly, we are all very unrealistic estimate the time required for a particular case and do not take into account the time to buildup, preparation or completion of the case that some data up to 20 percent of the time.
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Black And White Holes The notion of a black hole is inextricably linked with the birth of stars. All particles of a newborn star (protostar), of which it is formed, are attracted to its center of gravity forces, meeting no resistance. Therefore, the star begins to shrink. As the contraction of the protostar, the temperature increases, and occurs in the nucleus of a thermonuclear reaction. As the temperature in the inner layers of the star increases the internal pressure which tends to loosen it. When Contraction occurs balance (gravity) and decompresses the forces (centrifugal forces and internal pressure), protostar becomes a star, and can exist in a stable condition billions of Earth years. When burn out all the hydrogen and helium in turn, old age comes the star. And then - death. Large and small stars are dying in different ways. Small stars, which include our Sun, do not die so spectacularly as massive. When gravitational forces are directed into our solar balanced by the forces of repulsion that exist between individual particles, the compression stop, and the sun gradually cooled down and turned into a white dwarf. Otherwise, things with big stars. Continue to learn more with: Chase Koch, Wichita KS. There are two possibilities. If after a certain compression star still retained a certain amount of matter that could explode, it explodes, releasing its outer layers into space. However, if the mass of the large star is much greater than twice the mass of our Sun, its ability to explode sooner or later run out. It will continue to shrink to a critical radius and critical density.

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