A Brief History of Time: From the Big Bang to Black HolesStephen Hawking has earned a reputation as the most brilliant theoretical physicist since Einstein. In this landmark volume, Professor Hawking shares his blazing intellect with nonscientists everywhere, guiding us expertly to confront the supreme questions of the nature of time and the universe. Was there a beginning of time? Will there be an end? Is the universe infinite or does it have boundaries? From Galileo and Newton to modern astrophysics, from the breathtakingly cast to the extraordinarily tiny, Professor Hawking leads us on an exhilarating journey to distant galaxies, black holes, alternate dimensions--as close as man has ever ventured to the mind of God. From the vantage point of the wheelchair from which he has spent more than twenty years trapped by Lou Gehrig's disease, Stephen Hawking has transformed our view of the universe. Cogently explained, passionately revealed, "A Brief History of Time is the story of the ultimate quest for knowledge: the ongoing search for the tantalizing secrets at the heart of time and space. |
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Página 85
After the war the problem of gravitational collapse was largely forgotten as most scientists be- came caught up in what happens on the scale of the atom and its nucleus . In the 1960s , however , interest in the large - scale problems ...
After the war the problem of gravitational collapse was largely forgotten as most scientists be- came caught up in what happens on the scale of the atom and its nucleus . In the 1960s , however , interest in the large - scale problems ...
Página 88
Gravity gets weaker the farther you are from the star , so the gravitational force on our intrepid astronaut's feet would ... However , within just a few hours , as the region continued to collapse , the difference in the gravitational ...
Gravity gets weaker the farther you are from the star , so the gravitational force on our intrepid astronaut's feet would ... However , within just a few hours , as the region continued to collapse , the difference in the gravitational ...
Página 91
Accord- ing to this view , any nonrotating star , however complicated its shape and internal structure , would end up after gravitational collapse as a perfectly spherical black hole , whose size would depend only on its mass .
Accord- ing to this view , any nonrotating star , however complicated its shape and internal structure , would end up after gravitational collapse as a perfectly spherical black hole , whose size would depend only on its mass .
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LibraryThing Review
Crítica de los usuarios - jcvogan1 - LibraryThingFirst hundred pages are excellent, but then it gets to the then current day and becomes more a standard academic ‘this is what I think’ book. Leer comentario completo
LibraryThing Review
Crítica de los usuarios - benkaboo - LibraryThingSummary: Deep dive summary of the world of physics over the last 500 odd years. Things I liked: Objective: Trying to break heavy duty science into the language and ideas that regular folk can ... Leer comentario completo
Otras ediciones - Ver todas
A Brief History of Time: From the Big Bang to Black Holes Stephen Hawking,Carl Sagan Vista de fragmentos - 1988 |
Términos y frases comunes
able according appear arrow atoms attraction beginning believed big bang black hole body boundary called caused collapse complete contracting density describe developed dimensions direction disorder distance early earth effect Einstein electrons emitted energy event event horizon example exist expanding explain fact fall field FIGURE force galaxies gravitational collapse gravity happen histories idea increase infinite initial known later laws less light limit look mass matter means measure million million million moving neutron Newton objects observe orbits particles past paths phase planets position possible predictions principle probably quantum mechanics quarks question radiation rays reason regions relativity result rotating seems showed single singularity space space-time speed stars started string suggested surface temperature theory thought uncertainty unified theory universe waves weak zero