Mile Tyson Quotes

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From out there on the moon, international politics look so petty. You want to grab a politician by the scruff of the neck and drag him a quarter of a million miles out and say, “Look at that!” —EDGAR MITCHELL, APOLLO 14 ASTRONAUT, 1974
Neil deGrasse Tyson (Space Chronicles: Facing the Ultimate Frontier)
Take America’s Global Positioning System, GPS—two dozen satellites in orbit at about 12,500 miles above Earth, more than fifty times higher than ordinary low-Earth-orbit satellites
Neil deGrasse Tyson (Accessory to War: The Unspoken Alliance Between Astrophysics and the Military (Astrophysics for People in a Hurry Series))
This general flattening of objects that rotate is why Earth’s pole-to-pole diameter is smaller than its diameter at the equator. Not by much: three-tenths of one percent—about twenty-six miles.
Neil deGrasse Tyson (Astrophysics for People in a Hurry)
Here in our solar system, a hundred-meter-wide asteroid sails into Earth every millennium or so at speeds upward of fifty thousand miles an hour, generating a destructive impact equal to 2,500 atomic bombs.
Neil deGrasse Tyson (Accessory to War: The Unspoken Alliance Between Astrophysics and the Military (Astrophysics for People in a Hurry Series))
discovery of enormous masses of organisms at depths a mile or more beneath the basalts of Washington State, living mainly on geothermal heat, suggests that we may someday find the Europan oceans alive with organisms unlike any on Earth. But one pressing question remains: Would we call the creatures Europans or Europeans? Mars
Neil deGrasse Tyson (Origins: Fourteen Billion Years of Cosmic Evolution)
By day, contrary to common wisdom, you probably won’t see the Great Pyramids at Giza, and you certainly won’t see the Great Wall of China. Their obscurity is partly the result of having been made from the soil and stone of the surrounding landscape. And although the Great Wall is thousands of miles long, it’s only about twenty feet wide—much narrower than the U.S. interstate highways you can barely see from a transcontinental jet. From orbit, with the unaided eye, you would have seen smoke plumes rising from the oil-field fires in Kuwait at the end of the first Persian Gulf War in 1991 and smoke from the burning World Trade Center towers in New York City on September 11, 2001. You will also notice the green–brown boundaries between swaths of irrigated and arid land. Beyond that shortlist, there’s not much else made by humans that’s identifiable from hundreds of miles up in the sky. You can see plenty of natural scenery, though, including hurricanes in the Gulf of Mexico, ice floes in the North Atlantic, and volcanic eruptions wherever they occur.
Neil deGrasse Tyson (Astrophysics for People in a Hurry)
At the altitude of about 23,000 miles the satellite takes 23 hours and 56 minutes to orbit Earth. Earth takes 23 hours and 56 minutes to rotate.
Neil deGrasse Tyson (Merlin's Tour of the Universe: A Skywatcher's Guide to Everything from Mars and Quasars to Comets, Planets, Blue Moons, and Werewolves)
The actual recipe for the asteroid belt? Take a mere 2.5 percent of the Moon’s mass (itself, just 1/81 the mass of Earth), crush it into thousands of assorted pieces, but make sure that three-quarters of the mass is contained in just four asteroids. Then spread them all across a 100-million-mile-wide belt that tracks along a 1.5-billion-mile path around the Sun.
Neil deGrasse Tyson (Death by Black Hole)
You develop an instant global consciousness, a people orientation, an intense dissatisfaction with the state of the world, and a compulsion to do something about it. From out there on the Moon, international politics look so petty. You want to grab a politician by the scruff of the neck and drag him a quarter of a million miles out and say, “Look at that, you son of a bitch.” —Edgar D. Mitchell, Apollo 14 astronaut
Neil deGrasse Tyson (Starry Messenger: Cosmic Perspectives on Civilization)
Along with osmium and platinum, iridium is one of the three heaviest (densest) elements on the Table—two cubic feet of it weighs as much as a Buick, which makes iridium one of the world’s best paperweights, able to defy all known office fans. Iridium is also the world’s most famous smoking gun. A thin layer of it can be found worldwide at the famous Cretaceous-Paleogene (K-Pg) boundary† in geological strata, dating from sixty-five million years ago. Not so coincidentally, that’s when every land species larger than a carry-on suitcase went extinct, including the legendary dinosaurs. Iridium is rare on Earth’s surface but relatively common in six-mile metallic asteroids, which, upon colliding with Earth, vaporize on impact, scattering their atoms across Earth’s surface. So, whatever might have been your favorite theory for offing the dinosaurs, a killer asteroid the size of Mount Everest from outer space should be at the top of your list.
Neil deGrasse Tyson (Astrophysics for People in a Hurry (Astrophysics for People in a Hurry Series))
Just as I was crossing Madison Avenue, I somehow found myself flat out in the middle of the street. I had not tripped or missed a step. And yet there I was, down on the gravel with my heart galloping away. I quickly gathered myself and stumbled to my feet, shaken by what might have been if a car had sped through there. Oh no, Miles Davis, I’m not going with you, I thought as I stood. I wanted you in life, not in death. You chose to leave this place, but I’m not going anywhere. I believed then, as I do now, that Miles aimed to take me with him. And yet three decades later, I am, by God’s mercy, still right here.
Cicely Tyson (Just As I Am)
We use the effect of centrifugal forces on matter to offer insight into the rotation rate of extreme cosmic objects. Consider pulsars. With some rotating at upward of a thousand revolutions per second, we know that they cannot be made of household ingredients, or they would spin themselves apart. In fact, if a pulsar rotated any faster, say 4,500 revolutions per second, its equator would be moving at the speed of light, which tells you that this material is unlike any other. To picture a pulsar, imagine the mass of the Sun packed into a ball the size of Manhattan. If that’s hard to do, then maybe it’s easier if you imagine stuffing about a hundred million elephants into a Chapstick casing. To reach this density, you must compress all the empty space that atoms enjoy around their nucleus and among their orbiting electrons. Doing so will crush nearly all (negatively charged) electrons into (positively charged) protons, creating a ball of (neutrally charged) neutrons with a crazy-high surface gravity. Under such conditions, a neutron star’s mountain range needn’t be any taller than the thickness of a sheet of paper for you to exert more energy climbing it than a rock climber on Earth would exert ascending a three-thousand-mile-high cliff. In short, where gravity is high, the high places tend to fall, filling in the low places—a phenomenon that sounds almost biblical, in preparing the way for the Lord: “Every valley shall be raised up, every mountain and hill made low; the rough ground shall become level, the rugged places a plain” (Isaiah 40:4). That’s a recipe for a sphere if there ever was one. For all these reasons, we expect pulsars to be the most perfectly shaped spheres in the universe.
Neil deGrasse Tyson (Astrophysics for People in a Hurry)
The Himalayas grew against the force of Earth’s gravity because of the resilience of crustal rock. But before you get excited about Earth’s mighty mountains, you should know that the spread in height from the deepest undersea trenches to the tallest mountains is about a dozen miles, yet Earth’s diameter is nearly eight thousand miles. So, contrary to what it looks like to teeny humans crawling on its surface, Earth, as a cosmic object, is remarkably smooth. If you had a super-duper, jumbo-gigantic finger, and you dragged it across Earth’s surface (oceans and all), Earth would feel as smooth as a cue ball. Expensive globes that portray raised portions of Earth’s landmasses to indicate mountain ranges are gross exaggerations of reality.
Neil deGrasse Tyson (Astrophysics for People in a Hurry (Astrophysics for People in a Hurry Series))
Days after the elections of 2016, asha sent me a link to a talk by astrophysicist Neil deGrasse Tyson. We have to have hope, she says to me across 3,000 miles, she in Brooklyn, me in Los Angeles. We listen together as Dr. deGrasse Tyson explains that the very atoms and molecules in our bodies are traceable to the crucibles in the centers of stars that once upon a time exploded into gas clouds. And those gas clouds formed other stars and those stars possessed the divine-right mix of properties needed to create not only planets, including our own, but also people, including us, me and her. He is saying that not only are we in the universe, but that the universe is in us. He is saying that we, human beings, are literally made out of stardust. And I know when I hear Dr. deGrasse Tyson say this that he is telling the truth because I have seen it since I was a child, the magic, the stardust we are, in the lives of the people I come from. I watched it in the labor of my mother, a Jehovah's Witness and a woman who worked two and sometimes three jobs at a time, keeping other people's children, working the reception desks at gyms, telemarketing, doing anything and everything for 16 hours a day the whole of my childhood in the Van Nuys barrio where we lived. My mother, cocoa brown and smooth, disowned by her family for the children she had as a very young and unmarried woman. My mother, never giving up despite never making a living wage. I saw it in the thin, brown face of my father, a boy out of Cajun country, a wounded healer, whose addictions were borne of a world that did not love him and told him so not once but constantly. My father, who always came back, who never stopped trying to be a version of himself there were no mirrors for. And I knew it because I am the thirteenth-generation progeny of a people who survived the hulls of slave ships, survived the chains, the whips, the months laying in their own shit and piss. The human beings legislated as not human beings who watched their names, their languages, their Goddesses and Gods, the arc of their dances and beats of their songs, the majesty of their dreams, their very families snatched up and stolen, disassembled and discarded, and despite this built language and honored God and created movement and upheld love. What could they be but stardust, these people who refused to die, who refused to accept the idea that their lives did not matter, that their children's lives did not matter?
Patrisse Khan-Cullors (When They Call You a Terrorist: A Black Lives Matter Memoir)
The stars of the Milky Way galaxy trace a big, flat circle. With a diameter-to-thickness ratio of one thousand to one, our galaxy is flatter than the flattest flapjacks ever made. In fact, its proportions are better represented by a crépe or a tortilla. No, the Milky Way’s disk is not a sphere, but it probably began as one. We can understand the flatness by assuming the galaxy was once a big, spherical, slowly rotating ball of collapsing gas. During the collapse, the ball spun faster and faster, just as spinning figure skaters do when they draw their arms inward to increase their rotation rate. The galaxy naturally flattened pole-to-pole while the increasing centrifugal forces in the middle prevented collapse at midplane. Yes, if the Pillsbury Doughboy were a figure skater, then fast spins would be a high-risk activity. Any stars that happened to be formed within the Milky Way cloud before the collapse maintained large, plunging orbits. The remaining gas, which easily sticks to itself, like a mid-air collision of two hot marshmallows, got pinned at the mid-plane and is responsible for all subsequent generations of stars, including the Sun. The current Milky Way, which is neither collapsing nor expanding, is a gravitationally mature system where one can think of the orbiting stars above and below the disk as the skeletal remains of the original spherical gas cloud. This general flattening of objects that rotate is why Earth’s pole-to-pole diameter is smaller than its diameter at the equator. Not by much: three-tenths of one percent—about twenty-six miles. But Earth is small, mostly solid, and doesn’t rotate all that fast. At twenty-four hours per day, Earth carries anything on its equator at a mere 1,000 miles per hour. Consider the jumbo, fast-rotating, gaseous planet Saturn. Completing a day in just ten and a half hours, its equator revolves at 22,000 miles per hour and its pole-to-pole dimension is a full ten percent flatter than its middle, a difference noticeable even through a small amateur telescope. Flattened spheres are more generally called oblate spheroids, while spheres that are elongated pole-to-pole are called prolate. In everyday life, hamburgers and hot dogs make excellent (although somewhat extreme) examples of each shape. I don’t know about you, but the planet Saturn pops into my mind with every bite of a hamburger I take.
Neil deGrasse Tyson (Astrophysics for People in a Hurry (Astrophysics for People in a Hurry Series))
Yet, the cosmic view comes with a hidden cost. When I travel thousands of miles to spend a few moments in the fast-moving shadow of the moon during a total solar eclipse, sometimes I lose sight of Earth. When I pause and reflect on our expanding universe with its galaxies hurdling away from one another, embedded within the ever-stretching four-dimensional fabric of space and time, sometimes I forget that uncounted people walk this Earth without food or shelter, and that children are disproportionally represented among them. When I pour over the data that established the mysterious presence of dark matter and dark energy throughout the universe, sometimes I forget that every day, every 24 hour rotation of Earth, people kill and get killed in the name of someone else's conception of God, and that some people who do not kill in the name of God kill in the name of needs or wants of political dogma. When I track the orbits of asteroids, comets, and planets, each one a pirouetting dancer in a cosmic ballet, choreographed by the forces of gravity, sometimes I forget that too many people act in wanton disregard for the delicate interplay of Earth's atmosphere, oceans, and land, with consequences that our children and our children's children will witness and pay for with their health and wellbeing. And sometimes I forget that powerful people rarely do all they can to help those who cannot help themselves. I occasionally forget these things because however big the world is in our hearts, our minds, and our outsized digital maps, the universe is even bigger. A depressing thought to some, but a liberating thought to me.
Neil deGrasse Tyson (Astrophysics for People in a Hurry)
Egg Incubators are used to hatch Pokémon Eggs, which you can find at PokéStops. When an egg is in an incubator, you have to walk a distance of 2 up to 10 kilometers to hatch the egg. The longer the distance you have to cover, the higher the odds are a rare and strong Pokémon is revealed once the egg hatches. Important to note is that you must be traveling slower than 24 kilometers per hour (= 15 miles per hour) to hatch an egg. Traveling any faster will not count towards hatching your egg. You are given one orange Egg Incubator that can be used an infinite amount of times upon registration, while blue Egg Incubators you may purchase in the Shop will only last three hatches. More in depth explanations and strategies on hatching will be revealed later in the book.   Pok
Jeremy Tyson (Pokemon Go: The Ultimate Game Guide: Pokemon Go Game Guide + Extra Documentation (Android, iOS, Secrets, Tips, Tricks, Hints))
Meteor Crater A 150-foot-wide metallic meteor struck the Mogollon Rim in modern-day Arizona 50,000 years ago, leaving a mile-wide hole that’s 60 stories deep.
Neil deGrasse Tyson (StarTalk: Everything You Ever Need to Know About Space Travel, Sci-Fi, the Human Race, the Universe, and Beyond (Astrophysics for People in a Hurry Series))
You know you’re living in the future when you can board a hundred-ton pressurized aluminum tube with wings, fly smoothly in a cushioned chair at 500 miles per hour, 31,000 feet above Earth’s surface, and while crossing the continent, get served a pasta dinner and a mixed drink by someone whose job, in part, is to make you comfortable. And for most of the trip you surf the internet, watch any one of a hundred movies, only to land safely and smoothly a few hours later and complain that the marinara sauce was not to your liking.
Neil deGrasse Tyson (Starry Messenger: Cosmic Perspectives on Civilization)
† A light-year is the distance light travels in one Earth year—nearly six trillion miles or ten trillion kilometers. 2.
Neil deGrasse Tyson (Astrophysics for People in a Hurry (Astrophysics for People in a Hurry Series))
Neil: Were you strapped to a Saturn V rocket, with nine million pounds of thrust, and sent a quarter-million miles away into deep space to witness Earthrise from lunar orbit on Christmas Eve? Madalyn: No. Neil: Then shut the fuck up. In
Neil deGrasse Tyson (Starry Messenger: Cosmic Perspectives on Civilization)
Neil: Were you strapped to a Saturn V rocket, with nine million pounds of thrust, and sent a quarter-million miles away into deep space to witness Earthrise from lunar orbit on Christmas Eve? Madalyn: No. Neil: Then shut the fuck up.
Neil deGrasse Tyson (Starry Messenger: Cosmic Perspectives on Civilization)
I told myself Tyson was going to pick up their laptops, but half a mile later they joined the drive-thru line at an In-N-Out Burger. Tyson. Eating was constant. Maybe he needed sustenance before they retrieved the laptops.
Robert Crais (The Wanted (Elvis Cole, #17; Joe Pike, #6))