What is *Cosmos* by Carl Sagan about?

*Cosmos* by Carl Sagan explores humanity’s place in the universe, tracing 15 billion years of cosmic evolution from the Big Bang to modern scientific discovery. It interweaves astronomy, biology, and history, highlighting key figures like Johannes Kepler and Isaac Newton, while advocating for scientific curiosity and the pursuit of extraterrestrial life. The book emphasizes Earth’s fragility and the unifying power of science.

Who should read *Cosmos* by Carl Sagan?

Science enthusiasts, astronomy lovers, and readers curious about humanity’s cosmic journey will find *Cosmos* compelling. Its accessible prose makes it ideal for both casual readers and students seeking to understand complex topics like planetary exploration, evolution, and the history of scientific thought. Sagan’s engaging style appeals to anyone intrigued by the universe’s mysteries.

Is *Cosmos* by Carl Sagan worth reading?

Yes. *Cosmos* remains a landmark work in popular science, praised for making complex ideas accessible. It spent 70 weeks on the *New York Times* bestseller list and has inspired generations with its blend of poetic narrative and rigorous science. Its themes of cosmic connectedness and scientific optimism remain deeply relevant.

What are the main themes in *Cosmos*?

Key themes include the vastness of the universe, the evolution of life, the history of scientific inquiry, and humanity’s potential for space exploration. Sagan also emphasizes science as a tool for overcoming biases and addressing global challenges like nuclear warfare, urging readers to embrace curiosity and critical thinking.

How does *Cosmos* explore the history of science?

The book highlights pivotal moments, such as the Ionian Awakening in ancient Greece, the Renaissance contributions of Kepler and Newton, and 20th-century space missions. Sagan connects these milestones to show how scientific progress has reshaped humanity’s understanding of the cosmos, celebrating both triumphs and setbacks.

What famous scientists are discussed in *Cosmos*?

Sagan profiles astronomers like Tycho Brahe and Johannes Kepler, physicists like Isaac Newton, and ancient scholars like Hypatia and Democritus. These figures illustrate the collaborative, international nature of scientific discovery and its enduring impact on society.

How does Carl Sagan discuss extraterrestrial life in *Cosmos*?

Sagan speculates on life beyond Earth using principles of chemistry and biology, arguing that the universe’s vastness makes alien life probable. He examines the challenges of interstellar communication and urges humility, noting that humanity’s existence is a tiny fraction of cosmic time.

What is the significance of the Library of Alexandria in *Cosmos*?

The library symbolizes the fragility of human knowledge, as its destruction set back scientific progress for centuries. Sagan uses it to warn against anti-intellectualism and underscore the importance of preserving and expanding collective knowledge.

COSMOS

カール・セーガン

4.4(156250 Reviews)

『COSMOS』の概要

ニューヨーク・タイムズのベストセラーリストに70週間にわたってランクインした、カール・セーガンの画期的な名著とともに宇宙へと飛び込みましょう。ヒューゴー賞を受賞した本作は、数え切れないほどの科学者たちのキャリアにインスピレーションを与え、世界中で500万部を売り上げました。科学をたまらなく身近なものにしたこの一冊には、どのような天体の謎が待ち受けているのでしょうか？

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1冊の本。さまざまな聴き方。

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第1章

Unveiling the Cosmic Tapestry

In a universe teeming with billions of galaxies, Carl Sagan's "Cosmos" stands as a singular beacon that illuminates our place in the vastness of space. Unlike most science books that merely inform, Cosmos transforms raw information into profound knowledge and wonder. Since its publication in 1980, this masterpiece has sold over 5 million copies and been translated into 40 languages, making it one of the most influential science books ever written. The U.S. Library of Congress designated it among the 88 "books that shaped America" - a testament to its cultural significance. What makes this work extraordinary is how it weaves astronomy, biology, history, anthropology, and philosophy into a coherent narrative that speaks to our deepest questions about existence. When Neil deGrasse Tyson revived the Cosmos television series in 2014, he acknowledged standing on the shoulders of Sagan, whose ability to make complex scientific concepts accessible to everyone transformed public understanding of science. At its core, Cosmos isn't merely about stars and planets-it's about us, our origins, and our responsibility to preserve the pale blue dot we call home.

第2章

The Shores of the Cosmic Ocean

The Cosmos encompasses everything that exists, ever existed, or will exist-a concept so vast it defies ordinary comprehension. Our contemplations of it stir profound emotional responses-a tingling spine, a catch in the voice-as we approach the greatest mysteries of existence. The vastness of cosmic space and time makes human concerns seem trivial, yet paradoxically reveals our remarkable potential through curiosity and courage. Our understanding emerges from balancing skepticism with imagination-the latter carrying us to unexplored realms while the former distinguishes fact from fancy. Earth's surface represents merely the shore of a cosmic ocean we've barely begun to explore, having only dampened our toes. Something within us recognizes this ocean as our origin and longs to return. The immensity of space requires measurement in light-years rather than familiar earthly units. In this vastness, planets are precious rarities-the odds of randomly finding ourselves near one are less than one in a billion trillion trillion. From an intergalactic vantage point, we'd see countless galaxies as wispy tendrils of light, each containing billions of stars and potentially billions of planets. Given these overwhelming numbers, it seems far more likely that life exists elsewhere than that Earth alone is inhabited. Our journey through space reveals the Local Group of galaxies, past the Andromeda galaxy, into our own Milky Way with its 400 billion stars of all types and ages. Each star system exists in isolation, separated by light-years, possibly surrounded by planets in various stages of evolution. Some may harbor intelligent life that, like us, gradually discovers its place in the Cosmos. This cosmic perspective was first glimpsed by ancient minds like Eratosthenes, who measured Earth's circumference with remarkable accuracy 2,200 years ago. Using just sticks, eyes, feet, and curiosity, he became the first person to accurately measure a planet's size. With shadows in Alexandria falling at a 7-degree angle while those in Syene cast none, he calculated Earth's circumference as 40,000 kilometers-an achievement that inspired subsequent voyages of exploration and forever changed humanity's understanding of our place in the universe.

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『COSMOS』の一語一語が音声に合わせてリアルタイムでハイライトされ、自然に読み進められます。

第3章

One Voice in the Cosmic Fugue

The possibility of life elsewhere in the universe raises profound questions about our own origins. Would extraterrestrial life be carbon-based like Earth life? Would it resemble terrestrial organisms or be stunningly different? The abundance of organic molecules detected in interstellar clouds suggests that life's building blocks are widespread throughout the cosmos, hinting that given enough time, life's emergence might be a cosmic inevitability-though its evolution into intelligence may be rare. Evolution's power becomes evident in examples like Japan's Heike crab, whose shells bear markings resembling samurai faces. After the naval battle of 1185 where Emperor Antoku and the Heike clan perished, fishermen began throwing back crabs with face-like patterns, believing them to embody drowned samurai spirits. This practice created evolutionary pressure-crabs with more samurai-like shell patterns survived to reproduce while others were eaten. This demonstrates artificial selection, where humans unconsciously shaped another species' evolution by selecting which individuals would survive based on appearance. Humans have deliberately shaped plants and animals for thousands of years through selective breeding. Ten thousand years ago, there were no dairy cows with distended udders, specialized dog breeds, or large ears of corn. By controlling which individuals reproduce, we've transformed wild ancestors into domesticated varieties that serve our needs. The dramatic changes achieved in just thousands of years-sheep wool increasing from one kilogram of rough hair to twenty kilograms of fine down, or milk production rising hundredfold-demonstrate evolution's power when selection pressures are applied. If humans can create new varieties through artificial selection, nature must do the same through natural selection-Darwin and Wallace's great discovery. In nature's prolific abundance, more creatures are born than can survive, and the environment selects those variants better suited for survival. Mutations provide the raw material, and environmental pressures select which ones persist. The process works through death and time-countless deaths of imperfectly adapted organisms and immense spans of time for favorable mutations to accumulate. Earth condensed from interstellar matter 4.6 billion years ago, with life emerging around 4 billion years ago in the primitive oceans. The first life wasn't even a cell, but humble molecules that, by accident, learned to make crude copies of themselves. DNA evolved as the master molecule of life, with mutations-random changes in nucleotides-driving evolution. Four billion years ago, Earth was a molecular Eden without predators, where self-reproducing molecules competed and evolved. Specialized molecules eventually joined to form the first cells. Sex, invented two billion years ago, dramatically accelerated evolution by allowing organisms to exchange whole sections of genetic code rather than relying solely on random mutations. Green plants fundamentally altered Earth's atmosphere by generating oxygen-a poison to early life forms that created an evolutionary crisis. Today, 99 percent of our atmosphere is biologically produced; the sky itself is made by life. For three billion years, microscopic blue-green algae dominated Earth, until the Cambrian explosion 600 million years ago unleashed a proliferation of complex life forms.

第4章

The Harmony of Worlds

The universe exists in a perfect balance for science to flourish-neither completely static nor randomly chaotic, but governed by discernible patterns and natural laws. Humans have always excelled at understanding these patterns, which allowed our ancestors to hunt, build fires, and eventually develop science. The night sky offered our earliest laboratory, where we projected our cultural preoccupations onto star patterns, creating constellations that reflected our interests and concerns. Ancient peoples built sophisticated devices to track celestial movements across cultures and continents. The Anasazi constructed a ceremonial kiva in Chaco Canyon with a window precisely positioned to capture the sunrise on June 21, the year's longest day. Similar astronomical alignments appear at Angkor Wat, Stonehenge, Abu Simbel, and Chichen Itza. In the American Southwest, three upright slabs were positioned to create a "sun dagger" that bisects a carved spiral on the summer solstice and flanks it with two light beams on winter solstice. Astronomy emerged from practical necessity-tracking animal migrations, knowing when fruits ripened, planting and harvesting at appropriate times, and coordinating tribal gatherings. The celestial cycles-the reappearing crescent moon, the sun rising after eclipse or nightfall-also provided metaphors for immortality and surviving death. As measurement precision improved, record-keeping became essential, spurring the development of mathematics and writing. While astronomy developed as an empirical science, astrology emerged as a curious assault of mysticism into science. Modern astrology traces back to Ptolemy, who codified Babylonian traditions. Today, astrology remains far more popular than astronomy-more astrologers than astronomers exist, horoscopes appear in nearly every newspaper. Yet astrology fails basic tests: twins born minutes apart often have radically different fates, and astrologers cannot predict character or future events when given only birth details. Ptolemy, working in Alexandria's Library in the second century, developed a geocentric model of the universe where Earth stood immobile at center while celestial bodies revolved around it. To explain the planets' peculiar retrograde motions, he devised an ingenious system of spheres with smaller off-center wheels (epicycles). This model predicted planetary positions with reasonable accuracy for its time but hindered astronomical progress for a millennium until Copernicus proposed his revolutionary sun-centered system in 1543. Kepler's laws revealed the clockwork of the solar system. His first two laws showed planets move in ellipses and sweep out equal areas in equal times, while his third "harmonic law" established that the squares of planetary periods are proportional to the cubes of their distances from the Sun. Beyond merely describing planetary motion, Kepler sought underlying causes, suggesting magnetism as the force that made planets speed up near the Sun and slow when distant-a stunning anticipation of universal gravitation. Newton discovered the law of inertia and the nature of gravitational force, showing that the same universal force that pulls an apple earthward keeps the Moon in orbit. This inverse square law-where force declines as the square of distance increases-explains planetary motion and allowed Newton to derive all of Kepler's laws mathematically. From these principles, he proudly wrote in the Principia, "I now demonstrate the frame of the System of the World."

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第5章

Heaven and Hell

The Earth appears placid, with changes occurring slowly enough that we may never personally witness major natural disasters. This breeds complacency, despite clear evidence of catastrophic events preserved on other planetary landscapes. Such devastating events, unthinkable in human timescales, become inevitable over millions of years. The Tunguska Event of June 30, 1908, when a massive fireball crossed the Siberian sky and exploded, leveling 2,000 square kilometers of forest, offers a sobering reminder of cosmic dangers. This event was likely caused by an icy cometary fragment about 100 meters across-the size of a football field-weighing a million tons and moving at 30 kilometers per second. Such an impact today might be mistaken for a nuclear explosion, potentially triggering nuclear war, as it would simulate all effects of a one-megaton nuclear burst except for gamma radiation and radioactive fallout. Throughout history, comets evoked fear and superstition, challenging the notion of an unchanging cosmos. They were seen as harbingers of disaster-Babylonians thought them celestial beards, Greeks flowing hair, Arabs flaming swords. Some religious figures like Andreas Celichius claimed comets were "the thick smoke of human sins" kindled by divine anger. Comets may have contributed significantly to planetary atmospheres-Mars' current water could be explained by a recent cometary impact. Newton speculated that Earth's oceans originated from comets and that cometary "spirit" sustains life. Far beyond the planets exists a vast spherical cloud containing a trillion cometary nuclei. Occasionally, gravitational disturbances send these kilometer-sized "snowballs" into highly elliptical orbits toward the inner solar system, where solar heating creates their characteristic tails. Between Mars and Jupiter lie countless asteroids-tiny terrestrial planets, the largest being a few hundred kilometers across. Many have irregular shapes and tumble through space. This asteroid belt functions as a great grinding mill, with frequent collisions producing smaller and smaller fragments. Some of these pieces occasionally strike Earth as meteorites. Venus has nearly identical mass, size and density to Earth, making it our sister planet. But what lies beneath its featureless clouds? The first real clues came through spectroscopy, which revealed Venus's atmosphere contains enormous quantities of carbon dioxide but, surprisingly, no detectable water vapor. The breakthrough came from radio astronomy in 1956, when Venus was discovered emitting radio waves indicating extremely high temperatures. Venus is a planet-wide catastrophe. Surface temperatures reach around 480C (900F)-hotter than most household ovens-with crushing atmospheric pressure 90 times Earth's, equivalent to being 1 kilometer deep in Earth's oceans. The atmosphere is 96% carbon dioxide with traces of nitrogen, water vapor, and other gases. Venus's distinctive yellowish clouds consist primarily of concentrated sulfuric acid with small amounts of hydrochloric and hydrofluoric acids. Venus's extreme heat results from a massive greenhouse effect. Sunlight passes through its semi-transparent clouds and reaches the surface. The heated surface tries to radiate this energy back to space as infrared radiation, but the carbon dioxide and water vapor in Venus's atmosphere trap this heat almost completely. Earth also has a greenhouse effect that keeps our oceans liquid and makes life possible. While Venus has its 90 atmospheres of CO2 in gaseous form, Earth has an equivalent amount locked in limestone and other carbonates.

第6章

Blues for a Red Planet

Mars has captivated human imagination like no other planet, becoming a mythic arena onto which we project our earthly hopes and fears. Its apparent Earth-like features-polar ice caps, white clouds, dust storms, seasonal surface changes, and 24-hour day-have made it tempting to imagine as an inhabited world. Yet our psychological predispositions shouldn't mislead us; only evidence matters, and the definitive evidence about life on Mars isn't yet in. H.G. Wells' 1897 classic "The War of the Worlds" captured humanity's haunting fear and fascination with potential life beyond Earth, particularly on Mars. Three years earlier, Percival Lowell established an observatory dedicated to studying Mars, building on Giovanni Schiaparelli's 1877 observation of "canali" (channels) on Mars-mistranslated as "canals," implying intelligent design. This sparked Mars mania across Europe and America. In 1907, Alfred Russel Wallace, co-discoverer of evolution by natural selection, delivered a devastating critique of Lowell's theories. Wallace demonstrated that Lowell had miscalculated Martian temperatures, which were actually below freezing almost everywhere. He argued that Mars had much thinner air than Lowell calculated, should be covered with craters like the Moon, and that any attempt to transport water across such a desert planet would be "the work of madmen." Despite Wallace's critique and other astronomers' inability to confirm the canals, Lowell's vision gained popular acceptance. It resonated with the nineteenth century's engineering marvels-the Suez Canal, Corinth Canal, Panama Canal, and American irrigation projects. If humans could build such structures, why not more advanced Martians battling planetary desiccation? The Viking mission faced numerous constraints in selecting landing sites. Sites needed to be low elevation (for atmospheric braking), with minimal winds, moderate latitudes for communication, and surfaces neither too rough nor too soft. After traveling 100 million kilometers, both landers touched down safely-a triumph of engineering with an element of luck. The first images showed a surprisingly Earth-like landscape with rocks, sand drifts and distant hills reminiscent of the American Southwest. Though Viking found no visible life, Mars' history parallels Earth's when our planet had CO2-rich atmosphere and harsh UV radiation. Since microbes thrived on Earth for three billion years before large organisms colonized land, Viking was designed to search for microscopic life. The Viking landers carried experiments that yielded initially promising results. Two of the three biology experiments appeared positive-one showed something in Martian soil breaking down Earth nutrients as if microbes were metabolizing it, and another showed soil combining with Earth gases as if photosynthetic organisms were creating organic matter. However, scientists now believe these results may be misleading. Very little effort had been made to calibrate the experiments with plausible inorganic Martian materials. Recent experiments show that montmorillonite clays (identified on Mars by Mariner 9 and Viking) can reproduce key features of the "successful" Viking experiments. The clays have complex active surfaces that adsorb and release gases and catalyze chemical reactions.

聴きながら、すべての言葉を目で追えます

『COSMOS』の一語一語が音声に合わせてリアルタイムでハイライトされ、自然に読み進められます。

第7章

Travelers' Tales

The Voyager missions represent our first true interplanetary voyages, carrying instruments to distant worlds just as Dutch sailing vessels once carried explorers to new continents. These journeys, whether across oceans or space, share similar motivations: curiosity, national pride, commercial interests, and the thirst for discovery. The Voyager 2 spacecraft, launched in August 1977, represents humanity's first true interstellar vessel. Weighing nearly a ton and powered by nuclear energy, it carries sophisticated instruments including cameras, spectrometers, and sensors. By July 1979, it had reached Jupiter, navigating through dangerous radiation belts and debris rings. Its trajectory would use Jupiter's gravity to propel it toward Saturn, then Uranus and Neptune, before leaving our solar system entirely to wander among the stars. The revolutionary Dutch Republic of the seventeenth century exemplifies the spirit of exploration that now drives our ventures into space. Having declared independence from Spain, Holland embraced the European Enlightenment and built its economy on global maritime trade. The Dutch East India Company sent ships worldwide, combining commercial exploitation with scientific curiosity. The connection between Holland's exploratory power and its intellectual achievements was profound. Technological advances in shipbuilding fostered innovation in all fields. The challenges of navigation demanded better scientific understanding, while encounters with exotic lands shook established beliefs. Huygens' contributions to astronomy were revolutionary. He was the first to measure another planet's size, discover Venus' cloud cover, draw Mars' surface features, determine the Martian day length, and recognize Saturn's ring system. He also discovered Titan, Saturn's largest moon. Beyond astronomy, Huygens invented the pendulum clock to solve the longitude problem in navigation, created the spiral balance spring for watches, and made fundamental contributions to mechanics and probability theory. The Voyager spacecraft are spiritual descendants of both the Dutch sailing expeditions and Huygens' scientific vision-caravels bound for the stars. Like ancient explorers who returned with tales of exotic lands, Voyagers send back modern "travelers' tales" of worlds previously unimagined: shattered crystal spheres, cobwebbed globes, potato-shaped moons, and underground oceans. Of all Voyager's discoveries, the findings on Io proved most remarkable. Before the mission, scientists knew only that Io was extremely red and exhibited strange changes in its infrared properties. Voyager revealed a bizarre multicolored surface unlike any other in the solar system, mysteriously devoid of impact craters despite being near the asteroid belt. Linda Morabito of the Navigation Team accidentally discovered the first active volcano beyond Earth while enhancing an image. Voyager ultimately revealed nine large active volcanoes and hundreds of extinct ones.

第8章

The Backbone of Night

I grew up in Bensonhurst, Brooklyn, intimately knowing my immediate neighborhood but viewing the territory beyond 86th Street as alien and mysterious. As a child, I wondered about the stars-those twinkling lights whose nature adults couldn't explain. When I received my first library card, I discovered an astonishing truth: stars were suns, just incredibly distant ones. This revelation expanded my cosmos immeasurably. I reasoned that if our sun had planets, other stars must too, possibly harboring life. This childhood wonder sparked my astronomical ambitions during humanity's first era of planetary exploration. Our ancestors gazed at the night sky, creating stories about star patterns. Some believed stars were distant campfires of other tribes, others imagined them as holes in a great skin revealing flame beyond. They noticed wandering stars (planets) and pondered their nature. The !Kung Bushmen called the Milky Way "the backbone of night," believing it held up the darkness. These early metaphors eventually evolved into elaborate mythologies with gods controlling nature's unpredictable forces. Around 2,500 years ago, a revolutionary intellectual awakening occurred in Ionia. Suddenly, people proposed that everything was made of atoms, that humans evolved from simpler forms, that diseases weren't caused by demons, and that Earth orbited the Sun. This revolution transformed Chaos into Cosmos-revealing an ordered universe with natural laws. Ionia's unique position at cultural crossroads, its merchant-driven economy, widespread literacy, and political diversity created perfect conditions for free inquiry without enforced conformity. Thales and Anaximander pioneered scientific thinking in Miletus. Anaximander conducted experiments measuring seasons with shadows, created the first Greek sundial and celestial globe, and proposed Earth remained unsupported at the universe's center. He conceived of spontaneous life originating in mud and evolving through transmutation, believing in infinite inhabited worlds cycling through dissolution and regeneration-all without invoking divine intervention. Empedocles performed the first recorded experiment on air using a clepsydra (water thief), proving that invisible air could exert pressure and occupy space. His contemporary Democritus of Abdera developed atomic theory, arguing that everything consists of indivisible atoms moving through void-a purely mechanistic view of reality without divine intervention. As Ionian science flourished, religious opposition grew. Anaxagoras was imprisoned for impiety after teaching that the Moon reflected the Sun's light, that the Sun was a "fiery stone" larger than the Peloponnesus, and that the Moon had mountains. Though released through Pericles' intervention, this marked the turning of the tide against scientific inquiry in Greece. The brilliant Ionian experimental method was largely abandoned for two thousand years due to anti-empirical attitudes. Plato urged astronomers to think about the heavens but not observe them. The slave economy played a crucial role in science's decline-experimentation required manual labor, which slaveholders disdained, yet only they had leisure for intellectual pursuits.

『COSMOS』をもっと深く楽しむ

毎日の新しい気づきを10万件以上のレッスンから
言葉をハイライトして音声と同期
ライブラリを保存して、どの端末からでも利用

第9章

Travels in Space and Time

Space and time are interwoven-we cannot look into space without looking back in time. Light travels incredibly fast, but cosmic distances are vast. When we observe Beta Andromedae, we see it as it was 75 years ago. The Andromeda Galaxy appears to us as it was 2 million years ago, before humans existed. The most distant quasars show us the universe 8-10 billion years ago, before Earth formed. This finite speed of light creates a fundamental constraint in Einstein's special theory of relativity: nothing can travel faster than light. This isn't merely an engineering challenge like breaking the sound barrier, but a fundamental law of nature. Einstein's revolutionary insight came from simple questions about simultaneity-how events might appear different to observers moving at different speeds. His conclusion: there are no privileged reference frames in the universe, and light's speed remains constant regardless of the observer's motion. Time dilation-the slowing of time at speeds approaching light-offers a theoretical pathway to the stars. A traveler moving near light speed would hardly age while decades passed for friends back home. While light-speed travel remains impossible, engineers have designed potential starships like Project Orion, which would use nuclear explosions for propulsion, and Project Daedalus, which assumes future nuclear fusion technology. With continuous 1g acceleration, a spacecraft could approach light speed, allowing travelers to reach Barnard's Star in 8 years ship-time, the galactic center in 21 years, or even circumnavigate the universe in 56 years-though billions of years would pass on Earth. While we can travel into the future through relativistic effects, traveling to the past raises paradoxes. If you prevented your parents from meeting, you would never exist to make the journey. Some physicists propose that alternative histories could exist side by side-different timelines where every imaginable history plays out. History consists of deeply interwoven threads where small events at critical junctures might profoundly change outcomes. What if the scientific tradition of the ancient Ionian Greeks had survived and flourished? If science and experimental methods had been pursued 2,000 years before the Industrial Revolution, we might have saved ten or twenty centuries. Leonardo's contributions might have been made a thousand years ago, Einstein's five hundred. In such an alternate Earth, we might already be venturing to the stars, with great fleets of interstellar transports under construction, perhaps marked with Greek symbols. Evidence suggests planetary systems are abundant throughout the galaxy. In our vicinity, Jupiter, Saturn and Uranus each has a satellite system resembling our solar system in miniature. Though we cannot yet directly see planets around other stars, we can detect their gravitational influence. With perhaps a hundred billion planetary systems in the galaxy, we'll find worlds of breathtaking diversity-some with multiple suns or moons, particle rings spanning horizons, or views of gaseous nebulae.

第10章

The Lives of the Stars

To make an apple pie requires ingredients made of molecules, which are made of atoms-most of which were created inside stars. Only hydrogen formed in the Big Bang; everything else was cooked in stellar furnaces. Matter is mostly empty space-atoms are clouds of electrons surrounding tiny nuclei. Yet these empty structures hold firm through electrical forces, preventing my elbow from passing through the table. Atoms are incredibly small-one hundred million would span your fingertip, with nuclei a hundred thousand times smaller still. The emptiness of matter is profound; what prevents objects from passing through each other is the electrical repulsion between electron clouds. Cutting an atom transmutes elements, as medieval alchemists dreamed of doing. Modern physics has reduced the sensible world to astonishing simplicity: protons, neutrons and electrons arranged in various patterns make essentially everything. The universe is 99 percent hydrogen and helium, the two simplest elements. All other elements evolved from these primordial gases under extreme conditions. Creating heavier elements requires overcoming electrical repulsion by bringing nuclear particles close together, which happens only at temperatures of tens of millions of degrees-conditions found only inside stars. Stars and their planets form through gravitational collapse of interstellar gas clouds. Nuclear fusion ignites when compressed hydrogen atoms begin combining into helium, releasing energy as photons that take a million years to reach the surface. The Sun converts 400 million tons of hydrogen into helium every second in a controlled thermonuclear reaction that has sustained it for five billion years. When the Sun exhausts its central hydrogen in 5-6 billion years, fusion will migrate outward while the core contracts and heats until helium begins fusing into carbon and oxygen. The Sun will expand into a red giant, engulfing Mercury, Venus and likely Earth. Its atmosphere will eventually pulse and spew outward, creating a planetary nebula-a beautiful shell of glowing gas illuminated by the exposed hot stellar core. Finally, the Sun will become a white dwarf, cooling slowly over billions of years to a dark, dead black dwarf. Atoms synthesized in stellar interiors return to space through red giant winds, planetary nebulae, and supernova explosions. Stars forge elements sequentially-hydrogen fuses to helium, helium to carbon, carbon to oxygen, and in massive stars, all the way to iron. The nitrogen in our DNA, calcium in our teeth, iron in our blood, and carbon in our apple pies were all cooked in ancient stars. Some rarer elements form during supernova explosions themselves. Life and stars are intimately connected: our atoms were forged in stars; a nearby supernova likely triggered the solar system's formation; solar energy sparked the complex molecules leading to life; almost all life runs on sunlight; and cosmic rays from distant supernovae cause mutations that drive evolution. We are, in the most literal sense, made of starstuff. A star's mass determines its ultimate fate. While our Sun will become a red giant and white dwarf, more massive stars face dramatic ends. When stars several times the Sun's mass exhaust their nuclear fuel after just millions of years, they generate iron cores that collapse catastrophically. The implosion forces electrons into protons, creating neutron stars-essentially giant atomic nuclei about 30 kilometers across. For even more massive stars, typically five times the Sun's mass or greater, gravity overwhelms all resistance, creating black holes-regions where space-time is so severely warped that nothing, not even light, escapes.

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『COSMOS』の一語一語が音声に合わせてリアルタイムでハイライトされ、自然に読み進められます。

第11章

Who Speaks for Earth?

We have only recently discovered the Cosmos-for most of human existence, we believed Earth was the entire universe. Now we understand we inhabit a fragile world adrift in cosmic immensity. National boundaries are not evident when we view the Earth from space, and fanatical ethnic or religious chauvinisms seem absurd when we see our planet as a fragile blue crescent against the bastion of stars. The human species now undertakes a venture as important as colonizing land-breaking Earth's shackles both metaphorically and physically. Yet our energies focus on war. By the late twentieth century, nuclear weapons had proliferated worldwide, with a single thermonuclear bomb containing the destructive force of the entire Second World War. The 15,000 targeted warheads represented over 10,000 megatons-a World War II every second for an afternoon. Nuclear deterrence depends on psychological manipulation-occasional postures of irrationality make nuclear threats credible. The danger is that pretended irrationality becomes real. This global balance of terror holds Earth's citizens hostage, with each superpower testing the other's limits through military provocations. Almost half the world's scientists work on military matters, rewarded with high salaries and honors while protected by secrecy from responsibility for their actions. Our cerebral cortex, devoted to reason, gives us the capacity to cooperate and care for one another. Altruism is built into us. We've brilliantly deciphered Nature's patterns, yet our global civilization teeters on failure in its most important task: preserving life on Earth. Shouldn't we vigorously explore fundamental redesigns of our economic, political, social and religious institutions? Laboratory experiments reveal that mammals raised without physical affection develop abnormal characteristics. James Prescott's cross-cultural analysis of 400 preindustrial societies shows cultures lavishing physical affection on infants tend toward nonviolence. Where infants receive physical affection and adolescent sexuality isn't repressed, the likelihood of a violent society drops to just 2 percent. Recent centuries have seen remarkable progress-the near-elimination of slavery, growing equality for women, and increasing revulsion against war. Science-that characteristically human endeavor-gives us a true picture of our place in a Cosmos of exploding stars, forming galaxies, and possible extraterrestrial civilizations. It works through two simple rules: no sacred truths, and discard what contradicts facts. Alexandria once housed humanity's greatest scientific civilization, where discoveries in mathematics, physics, astronomy, and medicine laid foundations we still build upon. Yet those brilliant minds never challenged their society's assumptions about slavery or shared knowledge with the masses. Hypatia-mathematician, astronomer, physicist, and philosopher-moved freely through male domains in Roman Alexandria despite being a woman in a time when women were treated as property. As Christianity consolidated power, she stood at the epicenter of social upheaval, maintaining her friendship with the Roman governor and representing science and learning. Archbishop Cyril's parishioners murdered her brutally in 415 CE, flaying her with abalone shells before burning her remains and obliterating her works. Our achievements rest on 40,000 generations of human predecessors, most nameless and forgotten. From the Big Bang's explosive birth through hydrogen atoms condensing into stars, from nuclear fusion creating heavy elements to planetary formation, from simple molecules in primordial oceans evolving into self-replicating organisms to the development of plants, animals, and finally humans-this is our cosmic heritage. In fifteen billion years, hydrogen atoms have transformed into beings who can send spacecraft to other worlds. Human history shows a slowly expanding circle of loyalty-from family to tribe to nation. Now we must extend it to the entire planet. We are a rare and endangered species; in a hundred billion galaxies, there are no other humans. Our space exploration uses the same technologies as warfare, but redirects them toward life rather than death. We are the Cosmos grown to self-awareness, and our obligation to survive extends beyond ourselves to the ancient universe from which we spring.

★★★★★

『COSMOS』を最後まで読み終えました

100万人以上の学習者に愛用されています

“23日間、毎日使い続けています。今では日課の一部です。”

jayallen

『COSMOS』の主要テーマ

cosmic perspective
scientific skepticism
evolutionary biology
extraterrestrial life
human origins

『COSMOS』の名言

We are made of starstuff.
Somewhere, something incredible is waiting to be known.
The nitrogen in our DNA, the calcium in our teeth, the iron in our blood, the carbon in our apple pies were made in the interiors of collapsing stars. We are made of starstuff.
For small creatures such as we the vastness is bearable only through love.

『COSMOS』の登場人物

Carl SaganAuthor and astronomer who explores the universe
EratosthenesAncient scholar who measured Earth's circumference
Alfred Russel WallaceCo-discoverer of the theory of evolution
Neil deGrasse TysonAstrophysicist who revived the Cosmos series

著者について

科学の金字塔的著作『コスモス』の著者であるカール・セーガンは、先駆的な天体物理学者であり、ピューリッツァー賞を受賞した作家、そして天文学に対する一般社会の関わり方を再構築した象徴的なサイエンス・コミュニケーターでした。コーネル大学の教授であり、NASAのバイキング計画やボイジャー計画の主要な貢献者でもあったセーガンは、惑星科学における専門知識と、宇宙における人類の地位に関する哲学的な考察を織り交ぜました。

『コスモス』は、宇宙の進化、地球外生命体、そして科学的探究の歴史といったテーマを掘り下げており、科学的知識を民主化するというセーガンの生涯にわたる使命を反映しています。その他の著名な著作には、科学的懐疑主義の宣言書である『悪霊にさいなまれる世界：暗黒の世を照らす科学の灯』や、メジャー映画化されたSF小説『コンタクト』などがあります。

セーガンは1980年のPBSシリーズ『コスモス』のホストを務め、この番組は世界中で5億人以上の視聴者に届けられ、現在も科学教育の基準であり続けています。彼はまた、星間宇宙へと打ち上げられた地球文化のタイムカプセルである「ボイジャーのゴールデンレコード」を主導しました。

20以上の言語に翻訳された『コスモス』は、世界中で数百万部を売り上げ、2014年のテレビ版リブートにもインスピレーションを与えました。セーガンの遺産は、NASAの殊勲公務員賞や、彼を称えて命名された小惑星2709セーガンなど、数多くの栄誉を通じて称えられています。

COSMOSの要約をダウンロード

COSMOSの要約をPDFまたはEPUBで無料でダウンロード。印刷やオフラインでいつでもお読みいただけます。

他のユーザーのお気に入り

Cosmosapiens

John Hands

[cosmos-by-carl-sagan:c0000] Cosmos p1-1

[cosmos-by-carl-sagan:c0001] Cosmos p1-1

[cosmos-by-carl-sagan:c0002] Cosmos p1-1

[cosmos-by-carl-sagan:c0003] Cosmos p1-1

24 sources

Cosmos: Our Place in the Stardust

Origin Story

David Christian

Until the End of Time

Brian Greene

Welcome to the Universe

Neil deGrasse Tyson & Michael A. Strauss & J. Richard Gott

Starry Messenger

Neil deGrasse Tyson

Genesis

Guido Tonelli

The Demon-Haunted World

Carl Sagan

この本に関するよくある質問

学習プラン

The Cosmic Mirror: Science Meets Spirit

This plan is essential for seekers and thinkers looking to reconcile modern physics with ancient metaphysical truths. It is designed for those who want to move beyond reductionist science toward a deeper, unified understanding of the mind and the cosmos.

1 h 30 m•3 セクション

学習プラン

The Cosmic Blueprint: Logic and Proof

This plan offers a profound cross-cultural journey into the evolution of human logic and its connection to the universe. It is ideal for philosophy students, history buffs, and science enthusiasts seeking to understand the metaphysical foundations of mathematics.

2 h•4 セクション

学習プラン

Faith Among the Stars

This plan is essential for explorers and thinkers seeking to reconcile the harsh realities of deep-space physics with profound spiritual questions. It is ideal for those who want to find divine purpose while navigating the technical and existential challenges of the universe.

1 h 36 m•3 セクション

学習プラン

Astronomy

Astronomy connects us to the vastness beyond Earth, offering profound insights about our place in the cosmos. This learning plan benefits curious minds seeking to understand celestial mechanics, cosmic evolution, and the frontiers of space exploration without requiring advanced physics or mathematics.

4 h 15 m•4 セクション

学習プラン

Secrets of a Strange Earth

This plan is designed for curious minds who want to look beyond conventional knowledge to understand the anomalies of our universe and species. It is perfect for lifelong learners and trivia enthusiasts seeking to bridge the gap between science, history, and psychology.

1 h 36 m•4 セクション

学習プラン

i want to learn about the universe

This learning plan provides a structured journey from our local solar system to the furthest reaches of theoretical physics. It is ideal for curious minds and aspiring astronomers who want to bridge the gap between basic space facts and complex cosmological theories.

4 h 32 m•4 セクション

学習プラン

Read high-concept sci-fi exploring extremes

High-concept science fiction pushes the boundaries of imagination, challenging readers to confront radical ideas about humanity's future and the nature of reality itself. This learning plan is ideal for readers seeking to move beyond conventional sci-fi narratives into more intellectually demanding works that explore consciousness, technological transcendence, and the outer limits of speculative thought.

5 h 22 m•4 セクション

学習プラン

The Physics of Interstellar Survival

This plan bridges the gap between theoretical physics and practical engineering for the future of humanity. It is essential for aspiring aerospace engineers, science enthusiasts, and anyone fascinated by the technical realities of becoming a multi-planetary species.

1 h 12 m•3 セクション

コロンビア大学卒業生がサンフランシスコで開発

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BeFreedがウェブ上でどのように話題になっているかをもっと見る

コロンビア大学卒業生がサンフランシスコで開発

LOVED BY

1,000,000+ curious minds.

4.7

avg rating

1M+ learners

"Instead of endless scrolling, I just hit play on BeFreed. It saves me so much time."

@Moemenn

"I never knew where to start with nonfiction—BeFreed’s book lists turned into podcasts gave me a clear path."

@Chloe, Solo founder, LA

117

"Perfect balance between learning and entertainment. Finished ‘Thinking, Fast and Slow’ on my commute this week."

@Raaaaaachelw

"Crazy how much I learned while walking the dog. BeFreed = small habits → big gains."

@Matt, YC alum

108

"Reading used to feel like a chore. Now it’s just part of my lifestyle."

@Erin, Investment Banking Associate , NYC

254

"Feels effortless compared to reading. I’ve finished 6 books this month already."

@djmikemoore

"BeFreed turned my guilty doomscrolling into something that feels productive and inspiring."

@Pitiful

4.5K

"BeFreed turned my commute into learning time. 20-min podcasts are perfect for finishing books I never had time for."

@SofiaP

"BeFreed replaced my podcast queue. Imagine Spotify for books — that’s it. 🙌"

@Jaded_Falcon

201

"It is great for me to learn something from the book without reading it."

@OojasSalunke

"The themed book list podcasts help me connect ideas across authors—like a guided audio journey."

@Leo, Law Student, UPenn

483

"Makes me feel smarter every time before going to work"

@Cashflowbubu

"Instead of endless scrolling, I just hit play on BeFreed. It saves me so much time."

@Moemenn

"I never knew where to start with nonfiction—BeFreed’s book lists turned into podcasts gave me a clear path."

@Chloe, Solo founder, LA

117

"Perfect balance between learning and entertainment. Finished ‘Thinking, Fast and Slow’ on my commute this week."

@Raaaaaachelw

"Crazy how much I learned while walking the dog. BeFreed = small habits → big gains."

@Matt, YC alum

108

"Reading used to feel like a chore. Now it’s just part of my lifestyle."

@Erin, Investment Banking Associate , NYC

254

"Feels effortless compared to reading. I’ve finished 6 books this month already."

@djmikemoore

"BeFreed turned my guilty doomscrolling into something that feels productive and inspiring."

@Pitiful

4.5K

"BeFreed turned my commute into learning time. 20-min podcasts are perfect for finishing books I never had time for."

@SofiaP

"BeFreed replaced my podcast queue. Imagine Spotify for books — that’s it. 🙌"

@Jaded_Falcon

201

"It is great for me to learn something from the book without reading it."

@OojasSalunke

"The themed book list podcasts help me connect ideas across authors—like a guided audio journey."

@Leo, Law Student, UPenn

483

"Makes me feel smarter every time before going to work"

@Cashflowbubu

"Instead of endless scrolling, I just hit play on BeFreed. It saves me so much time."

@Moemenn

"I never knew where to start with nonfiction—BeFreed’s book lists turned into podcasts gave me a clear path."

@Chloe, Solo founder, LA

117

"Perfect balance between learning and entertainment. Finished ‘Thinking, Fast and Slow’ on my commute this week."

@Raaaaaachelw

"Crazy how much I learned while walking the dog. BeFreed = small habits → big gains."

@Matt, YC alum

108

"Reading used to feel like a chore. Now it’s just part of my lifestyle."

@Erin, Investment Banking Associate , NYC

254

"Feels effortless compared to reading. I’ve finished 6 books this month already."

@djmikemoore

"BeFreed turned my guilty doomscrolling into something that feels productive and inspiring."

@Pitiful

4.5K

"BeFreed turned my commute into learning time. 20-min podcasts are perfect for finishing books I never had time for."

@SofiaP

"BeFreed replaced my podcast queue. Imagine Spotify for books — that’s it. 🙌"

@Jaded_Falcon

201

"It is great for me to learn something from the book without reading it."

@OojasSalunke

"The themed book list podcasts help me connect ideas across authors—like a guided audio journey."

@Leo, Law Student, UPenn

483

"Makes me feel smarter every time before going to work"

@Cashflowbubu

BeFreedがウェブ上でどのように話題になっているかをもっと見る

今すぐ学習の旅を始めよう

第11章

COSMOS

概要『COSMOS』の概要

1冊の本。さまざまな聴き方。

Unveiling the Cosmic Tapestry

The Shores of the Cosmic Ocean

聴きながら、すべての言葉を目で追えます

One Voice in the Cosmic Fugue

The Harmony of Worlds

『COSMOS』をもっと深く楽しむ

Heaven and Hell

Blues for a Red Planet

聴きながら、すべての言葉を目で追えます

Travelers' Tales

The Backbone of Night

『COSMOS』をもっと深く楽しむ

Travels in Space and Time

The Lives of the Stars

聴きながら、すべての言葉を目で追えます

Who Speaks for Earth?

『COSMOS』を最後まで読み終えました

『COSMOS』の主要テーマ

『COSMOS』の名言

『COSMOS』の登場人物

著者について

COSMOSの要約をダウンロード

他のユーザーのお気に入り

この本に関するよくある質問

What is Cosmos by Carl Sagan about?

Who should read Cosmos by Carl Sagan?

Is Cosmos by Carl Sagan worth reading?

What are the main themes in Cosmos?

もっと見る

1,000,000+ curious minds.

1,000,000+ curious minds.

1冊の本。さまざまな聴き方。

Unveiling the Cosmic Tapestry

The Shores of the Cosmic Ocean

聴きながら、すべての言葉を目で追えます

One Voice in the Cosmic Fugue

The Harmony of Worlds

『COSMOS』をもっと深く楽しむ

Heaven and Hell

Blues for a Red Planet

聴きながら、すべての言葉を目で追えます

Travelers' Tales

The Backbone of Night

『COSMOS』をもっと深く楽しむ

Travels in Space and Time

The Lives of the Stars

聴きながら、すべての言葉を目で追えます

Who Speaks for Earth?

『COSMOS』を最後まで読み終えました

他のユーザーのお気に入り

もっと見る

『COSMOS』の概要