Download PDF by David A. Weintraub: How Old Is the Universe?

By David A. Weintraub

ISBN-10: 0691147310

ISBN-13: 9780691147314

Astronomers have decided that our universe is 13.7 billion years previous. How precisely did they arrive to this designated end? How previous Is the Universe? tells the marvelous tale of ways astronomers solved probably the most compelling mysteries in technological know-how and, alongside the best way, introduces readers to basic options and state-of-the-art advances in smooth astronomy.

The age of our universe poses a deceptively uncomplicated query, and its resolution incorporates profound implications for technological know-how, faith, and philosophy. David Weintraub strains the centuries-old quest through astronomers to fathom the secrets and techniques of the night sky. Describing the achievements of the visionaries whose discoveries jointly unveiled a primary secret, he exhibits what number self reliant traces of inquiry and masses painstakingly accumulated facts, while equipped jointly like items in a cosmic puzzle, resulted in the long-sought solution. Astronomers don't think the universe is 13.7 billion years old--they comprehend it. you are going to too after examining this publication. through concentrating on some of the most the most important questions on the universe and demanding readers to appreciate the reply, Weintraub familiarizes readers with the guidelines and phenomena on the middle of contemporary astronomy, together with pink giants and white dwarfs, cepheid variable stars and supernovae, clusters of galaxies, gravitational lensing, darkish topic, darkish power and the accelerating universe--and even more. delivering a different historic method of astronomy, How outdated Is the Universe? sheds mild at the internal workings of clinical inquiry and divulges how astronomers grapple with deep questions about the actual nature of our universe.

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They reasoned that if the core temperature of the Sun were much hotter than 10 million K, the intense pressure from the super hot gas deep inside the Sun would cause the outer layers of the Sun to expand, increasing its size much above its present diameter. Clearly, if stars generate energy through nuclear fusion but do so at temperatures of millions of degrees rather than billions of degrees, then our simple picture of the fusion process is so far inadequate. We need to furnish two additional and crucial links.

In general, interstellar clouds are in a precarious balance between expansion and collapse. Their internal heat generates expansive pressure while gravity from the particles of matter in the cloud works to pull the particles closer together. When an interstellar cloud cools off, its thermal pressure weakens and the cloud loses the ability to resist the compressive force of gravity. The balance tips in favor of gravity and the cloud collapses in on itself. The rotational motion of the collapsing cloud, however, prevents all of the material in the cloud from falling all the way to the center; instead, while the cloud shrinks it also flattens, forming a disk of gas and dust that revolves around the newborn star at its center.

Over time, they collided with other small objects. Through these sticky collisions, the CAIs were incorporated into bigger objects that grew from dust-grains into pebbles, rocks, and boulders. These larger objects continued to orbit the Sun. Those that remain we call asteroids. Every year, some asteroids collide or exert enough gravitational at- chapter 3 • 26 traction on each other to change each others’ orbits so that a few of them, or fragments of a few of them, end up in orbits that intersect the orbit of the Earth.

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How Old Is the Universe? by David A. Weintraub


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