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[ BOOK ATOM: AN ODYSSEY FROM THE BIG BANG TO LIFE ON EARTH...AND BEYOND by LAWRENCE M. KRAUSS OVERVIEW ]

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The story of matter and the history of the cosmos from the perspective of a single oxygen atom, told with the insight and wit of one of the most dynamic physicists and writers working today.

Through this astonishing work, he manages to stoke wonder at the powers and unlikely events that conspired to create our solar system, our ecosystem, and us.

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Book ID Asin: B000FA5SO8
Book Title: Atom: An Odyssey from the Big Bang to Life on Earth...and Beyond
Book Author: Lawrence M. Krauss
Book Format and Price:
Book Format Name: Kindle
Book Format Price: $9.99
Book Format Name: Hardcover
Book Format Price: $12.99-$35.14
Book Format Name: Paperback
Book Format Price: $8.00-$18.99
Book Price: unknown
Book Category: Kindle Store, Kindle eBooks, Science & Math and unknown
Book Rating: 112 ratings

Atom: An Odyssey from the Big Bang to Life on Earth...and Beyond by Lawrence M. Krauss Book Review

Name: Rama Rao
Rating: 5.0 out of 5 stars
Title: Stars are the cosmic incubators for all natural elements
Date: Reviewed in the United States 🇺🇸 on August 22, 2007
Review: This book requires basic knowledge of physics and chemistry. Chapters 1 - 7 introduce cosmology; Chapters 8 - 9 describes evolution of stars, and physical and chemical process for the production of chemical elements; Chapters 10 - 13 addresses the evolution of life on hospitable planets such as earth. Chapters 8, 9 and 11 provide significant amount of information, while some chapters are too descriptive and boring.

When the universe was at its infancy, it consisted of clouds of hydrogen and helium molecules that started to collapse over millions of years (mass accretion) under gravity. Progressively the temperature increased due to compression and the molecules started to dissociate into atoms and finally to ions at high pressure and temperatures. At 15 million degrees, about one in a 100 million protons gain sufficient energy to collide and fuse with each other to produce deuterium nuclei, further nuclear reactions generated helium-3 nucleus. Collision of two helium-3 nuclei results in helium-4 and two protons, generating intense radiation (energy) and pressure (centrifugal force) to counter the gravitational (centripetal) force. Thus thermonuclear reactions produce heat and light of a star over billions of years of its existence which affects geological process and biological evolution in orbiting planets. If a star is massive, gravitational collapse continues and the temperature at inner core rises to 100 million degrees when two helium-4 nuclei fuse to form berylluim-8 nuclei; at higher core temperatures collision of helium-4 with beryllium-8 results in carbon-12. After millions of years of burning helium, the inner core continues to fall as the compression continues to raise core temperature and this promotes carbon-12 and helium-4 nuclear fusion producing oxygen-16 nucleus. When helium nuclei are completely exhausted; the star would have produced significant quantities of carbon and oxygen nuclei. This result in two shells; an inner core of carbon and oxygen followed by an outer shell of burning helium, which is surrounded by a shell of burning hydrogen. When helium is exhausted, the inner core is compressed further raising temperature, then two carbon nuclei fuse to produce a plethora of nuclei from oxygen to sodium and magnesium. When carbon burning is completely exhausted, the core compresses further raising temperature and pressure to promote fusion of oxygen nuclei to produce silicon, neon, and then sulfur. As the temperatures rises to one billion degrees, fusion of silicon nuclei results in iron-56 nucleus; beyond this point no further elements are generated, since heavier nuclei bind less tightly. At this stage when the temperature is 5 billion degrees, the density reaches 10,000 tons per cubic centimeter. The core starts to lose energy in the form escaping neutrinos, and fusion of protons and electrons results in increasing amounts of neutrons. As the core energy decreases, the gravitational force of matter dominates. At a density of 100 million tons per cubic centimeter, the core predominantly contains neutrons and at this point laws of quantum mechanics precludes neutrons squeezed any further thus forming a neutron star. Eventually the star collapses in a gigantic explosion called supernova. At this point the temperature is very high and during this hot expanding neutron-rich environment capture of neutrons by various elements quickly produces all natural elements up to uranium. These are expelled into the interstellar medium to great distances in spacetime, eventually cooling the debris. During cooling process; the nuclei capture electrons to become atoms and elements such as iron, silicon, aluminum and carbon will condense into microscopic solid grains at appropriate temperatures. Low molecular weight compounds such as carbon monoxide, iron oxides, silicates and water are formed at right temperatures and pressure. Photochemical reactions in presence of iron and aluminum produce carbon dioxide, methanol, ethanol, formaldehyde, and glycine (amino acid) etc. Carbon, hydrogen, oxygen and nitrogen continue to form more complex organic and biomolecules, the source material for life. Oxygen remains adhered to grains of aluminum oxide. As the stellar dust and gas collapse inward toward a central plane of rotating material which will fragment to form planetismals (planetary nebula) around a star. Much of water was provided by comets (from Oort clouds outside the solar system) hitting earth over millions of years. The planet turned from state of high levels of carbon dioxide and nitrogen to a more tolerable levels, and habitable temperatures which lead to the raise in oxygen concentration. It is a concerted effort of sun and the Jupiter; geological process followed by biological evolution created the blue planet. This book contains an exhaustive amount of scientific material that could serve as a reference material, and it is highly recommended.

Name: John H. Evans
Rating: 5.0 out of 5 stars
Title: One of the best science books ever
Date: Reviewed in the United States 🇺🇸 on October 25, 2014
Review: First, “Atom” is one of the two best science books I’ve ever read. (*) Krauss is both an excellent writer and an outstanding story-teller. The majority of this book is compelling, at least to a science geek like me. Carl Sagan famously said, “We are all star-stuff.” Krauss uses the fictional life of an oxygen atom to explain to the reader HOW we all came to be made from star-stuff – how we came to be here – and speculations about the future and fate of the Universe.

Second, this is definitely a geek-book and will be of interest only to those who desire to know the details how our world came be.

This book was published in 2001 before the days of Kindle, so the Kindle version leaves something to be desired. I’d recommend a hard copy.

(*) my favorite science book ever …. “Unweaving the Rainbow: Science, Delusion and the Appetite for Wonder” Paperback – April 5, 2000 by Richard Dawkins

Atom: An Odyssey from the Big Bang to Life on Earth...and Beyond [Kindle Edition] By Lawrence M. Krauss. Review by John H Evans – October 24, 2014

Name: J.R. Mc
Rating: 4.0 out of 5 stars
Title: Following Matter Through Time
Date: Reviewed in the United States 🇺🇸 on May 8, 2015
Review: Okay, so I couldn't give it a 4.5 star rating which is where I would actually put it. Krauss is a skillful writer. In this book, it did seem to go slowly at times; but, overall, this is a fascinating concept. Following the creation of the constituents of an oxygen atom, the primordial atoms from the big bang, through it being a part of a supernova and star dust, star and planet systems and being a part of living cells and on to the ultimate destiny at the end of the universe as we know or can know it, all of this kept me wanting to read instead of mowing the lawn or other interesting jobs around the house and property. It's like what I always wished I could do, follow a toy boat from the local rivulet into creeks, rivers and eventually the Mississippi River and the Gulf of Mexico, only more interesting.

Name: James Draw
Rating: 4.0 out of 5 stars
Title: lots of interesting information
Date: Reviewed in the United States 🇺🇸 on March 27, 2013
Review: The author describes the big bang; then when an oxygen atom is formed, he follows it through the remaining history of the universe. A few parts were a little too detailed and slow, but for the most part, the narrative went smoothly and kept my attention.

Name: phoenixrising
Rating: 5.0 out of 5 stars
Title: Fascinating story, not unlike a cosmology class!
Date: Reviewed in the United States 🇺🇸 on April 18, 2017
Review: This is a wonderful story about the life of an oxygen atom, told from the perspective of the atom. If you enjoy Sagan, or Tyson, you will find this story most intriguing!

Name: Tim Samuel
Rating: 5.0 out of 5 stars
Title: Best science book I've read for a very long time
Date: Reviewed in the United States 🇺🇸 on January 23, 2014
Review: Begins with an excellent explanation of the early universe and gets better. The description of how the Earth formed, the contribution of comets, the effect of impacts by large meteorites, the role of iron in safeguarding life in its early stages, etc. makes this the best, most informative book on "creation" I have ever read. Highly recommended.

Name: Wayne Wilmot
Rating: 5.0 out of 5 stars
Title: Finally we know where we came from.
Date: Reviewed in the United States 🇺🇸 on March 14, 2014
Review: This is an excellent review of where the earth's makeup originated. This true story was made possible by scientific advances in the last century. Mankind has gotten beyond myth to finally begin to understand how we came to be on this little lonely planet. Gripping reading if you want to replace myth with fact.

Name: Poetic naturalist
Rating: 5.0 out of 5 stars
Title: Now, that's an historical thread
Date: Reviewed in the United States 🇺🇸 on June 17, 2014
Review: What a brilliant concept! From nucleosynthesis to cosmology to galaxy and star formation to chemistry to geology. It's a thread that reaches back to the very beginning and touches so much interesting science along the way and, of course, Krauss is a great story teller, as always.