Title: The threat from space. Subject(s): EARTH; METEORS; COMETS Source: Earth, Aug96, Vol. 5 Issue 4, p24, 8p, 1 chart, 12c Author(s): Desonie, Dana Abstract: Looks at the potential danger from the cosmic collision involving the planet earth and meteors/comets on the human race. Mass extinction in the earth as the result of a bombardment; Objects which pose a threat to the earth; Odds of a lethal cosmic collision; Possibility of defense against this phenomenon. INSET: Craters, craters everywhere, by Alexandra Witze. AN: 9607032823 ISSN: 1056-148X Note: This title is not owned by Tucson-Pima Public Library. Database: MasterFILE Elite THE THREAT FROM SPACE Asteroids and comets have slammed in to Earth before. They will do so again--but when? And what can we do about it? It could happen to you. Just as a Triceratops may have done some 65 million years ago, you look up and see something strangely bright in the sky. An hour later it appears even more brilliant. Is it a supernova? An alien ship? A comet? Unlike that dinosaur, you might have been warned: A killer meteorite is headed your way. The object grows larger and brighter until, three hour later, it enters Earth's atmosphere. It ignites into a blinding fireball that strikes the surface ten seconds later. By chance, ground zero is shallow water; the impact generates enormous tsunamis that flood coastal regions thousands of miles away. Dust and gas fly heavenward and then coalesce into fireballs that fall back toward Earth. The energy released heats the atmosphere to the temperature of a kitchen oven on broil. Land animals roast. Forests burst into flames. dust particles and smoke block the Sun out and day into night. Earth plunges into a deep freeze. Without sunlight, photosynthesis ends; plants perish and animals starve. Sulfuric gases released from the shattered limestone rock mix with water in the atmosphere to form acid rain. Over the next several months, the rain falls to Earth, dissolving the shells of tiny marine plants with its acidity. The food web of the ocean collapses. Carbon released from the limestone combines to form the greenhouse gas carbon dioxide. Within months the deep freeze ends, and years of intense warming begin. Sound farfetched? This list of horrors was compiled from the work of many scientists to describe the environmental devastation that resulted 65 million years ago when a meteorite six miles across struck Mexico's Yucatan Peninsula with ten billion times the energy of the atomic bomb that destroyed Hiroshima. Although scientists still debate exactly what happened then, many are convinced that the collision triggered a global mass extinction during which roughly two-thirds of Earth's species, including the dinosaurs, were wiped out. If such a cosmic collision were to occur today, life on Earth would once again be utterly changed, with countless species -- including perhaps our own -- being wiped out forever. Any humans who did weather the blast would experience global crop failures and sweeping famine because of the blocking of the Sun's light. "Human civilization would be completely rebooted," says William K. Hartmann of the Planetary Science institute in Tucson, Arizona. Hartmann and many other scientists believe that impacts have played a crucial role in the evolution of life on our planet by wiping out dominant species and giving others a chance to flourish. For example, many paleontologists think that dinosaurs were agile and cunning, that they were well-adapted to their environments and dominated the smaller, less highly specialized mammals. Yet in a geologic instant the dinosaurs' 140-million-year reign ended, and mammals took over the planet. Other extinctions have also been tentatively linked to impacts: Scientists have speculated that the mass extinctions of the late Devonian Period, roughly 365 million years ago, were linked to at least one impact at the same time. Another doomsday may be inevitable. But do we have no more control over our destiny than the dinosaurs had over theirs? Or can we locate our attacker before it strikes and destroy it before it destroys us? Yes, scientists say, there are things we can do to cheat fate. We can search the skies for an object on course to strike our planet; most scientists agree that such a search is wise, but they disagree on whether more should be done. Some say we should construct a defense system now, to be ready to send missiles or even nuclear weapons into space so that we can destroy the object or deflect it from its collision course. Others argue that the risks are so long-term that construction of a defense system can wait until technological advances yield solutions that society can afford. One thing is perfectly clear, however. Another asteroid or comet will hit Earth again. It's only a matter of time. Scientists know Earth has suffered repeated bombardment since it formed 4.5 billion years ago. But this consensus was a long time in coming. In fact, it wasn't until 1957 that scientists even agreed that Earth had a genuine meteorite crater. After decades of debate, a geology graduate student named Eugene Shoemaker argued convincingly that the iron fragments, layers of broken rock and shock-melted glass droplets found at Arizona's Meteor Crater, also known as Barringer Crater, could only have formed by meteorite impact. An asteroid about 200 feet in diameter had broken up in Earth's atmosphere, and some of its fragments and its shock wave slammed into northern Arizona 50,000 years ago, creating one of the best-preserved impact structures on Earth. Since then, scientists have catalogued at least 150 impact structures on Earth, up to 150 miles in diameter, according to impact expert Richard Grieve of the Geological Survey of Canada in Ottawa. The idea that cosmic collisions could shape the evolution of life on Earth gained enormous credibility in 1980 when the father-son team of Luis and Walter Alvarez and two colleagues suggested that a meteorite impact annihilated the dinosaurs and the many other forms of life that became extinct 65 million years ago. The team based their conclusion on rich concentrations of iridium found in layers of rock in many areas of the world, all dating to 65 million years ago. (This element is virtually absent from Earth's surface but is abundant in extraterrestrial rocks.) Since then, other scientists have found the purported crater, buried offshore near its namesake village of Chicxulub in the Yucatan. The Alvarez theory prompted scientists to ask new questions. If a random event could so profoundly alter the course of life on Earth, could it happen again? And if so, when might that happen? Should we be worried about the hazards of extraterrestrial impacts? Such questions became even more pressing after July 1994, when we first witnessed a collision between a large object and a planet. The planet was Jupiter; the object was the shattered comet known as Shoemaker-Levy 9. Over a period of several days, more than 20 comet fragments pummeled Jupiter. Plumes of gas and dust shot thousands of miles into the stratosphere. Astronomers on Earth detected the heat given off as the material fell back. If Earth had been Shoemaker-Levy 9's target, the impact would have been "a globally devastating event," says astronomer Tom Gehrels of the University of Arizona in Tucson. And yet such events are not unlikely. Our solar system is teeming with objects of all sizes, from particles of dust to planets. Most pose no threat to Earth because they are too small or too distant. The two main hazards to Earth, though, are comets and asteroids. Both types of objects can sometimes come perilously close to our planet. On May 19 of this year, for example, an asteroid about one-quarter of a mile across whizzed past only 280,000 miles away --approximately the distance to the Moon. This was the largest object ever to get so close to Earth. Most unsettling, astronomers didn't spot the object until just a few days before it zipped by. Asteroids are rocky or metallic objects ranging in size from particles to tiny planets nearly 600 miles across. Most asteroids orbit the Sun between Mars and Jupiter in what's called the main asteroid belt. They're thought to be debris that didn't coalesce into a planet because of Jupiter's tremendous gravitational pull. Occasionally two main-belt asteroids collide, ejecting fragments that veer into the inner solar system. The fragments thus become near-Earth objects that could intersect our planet's orbit. The gravitational tug of Jupiter can also nudge a main-belt asteroid into a near-Earth path. Comets are composed of rock and dust bound together by ice. (The ice changes directly to vapor when the comet nears the Sun, producing a magnificent tail.) And they're big: The nuclei of comets can measure as large as 150 miles across, though most of them are only about 10 miles across. Comets come from different places. Some orbit the Sun in the Kuiper Belt just beyond the planet Neptune. Others reside in the Oort Cloud, which reaches a fifth of the distance to the next nearest star. Each year, several previously unrecorded comets, such as the recent Comet Hyakutake, blaze through the inner solar system, perhaps dislodged from the Oort Cloud by gravitational interactions with other comets. Between comets and asteroids, Earth faces a pretty good chance of getting walloped. At present, more than 200 noteworthy objects with orbits that cross Earth's orbit have been discovered, though none are predicted to hit anytime soon. However, there is at least one prediction, made recently by Paolo Farinella of the University of Pisa in Italy and colleagues, for a collision between Earth and a large asteroid. In eight computer simulations of possible orbits for a 14-mile-wide asteroid named Eros, one forecast a catastrophic impact with Earth 1.14 million years into the future. According to Gehrels, at the present rate of discovery -- approximately 50 a year and climbing -- it will take about a century to catalog essentially all of the objects that we know could pose a threat. The odds that a lethal cosmic collision will occur in your lifetime are a lot higher than you probably think. "The chances that you'll die from an asteroid impact are the same as [the chances of your] dying in a plane crash if you take one round-trip a year," says David Morrison of NASA's Ames Research Center in California. Large meteorite impacts are extreme cases of low-frequency, high-consequence risks -- events that occur very infrequently but cause enormous numbers of deaths. Many other natural disasters, such as earthquakes, also represent low- frequency, high-consequence risks. Yet most natural disasters are more limited in magnitude than a large collision. For example, geologists believe that Earth's crust can build up only so much stress before that stress must be released in an earthquake; this restricts the size of earthquakes. An Earth-bound asteroid, however, could measure hundreds of miles across. The 1976 Tangshan earthquake in China is thought to have killed as many as three-quarters of a million people, but a collision with an object larger than one mile in diameter could wipe out billions, scientists believe. Fortunately, the more lethal the object is, the less likely it is to strike Earth's surface. Asteroids less than about 160 feet across burn up in the atmosphere. A somewhat larger meteor might explode above ground and damage the surface with its shock wave. Objects measuring between 300 and 3,300 feet are estimated to strike every 1,000 to 200,000 years. If one of these hit the sea, it would send out a 16-foot-high tsunami that would travel thousands of miles and kill millions of people. On land, the same impact would create a three-mile-wide crater and destroy almost 4,000 square miles of property. A hit in New York City's Central Park could kill 25 million. Scientists estimate that it would take a meteorite about one mile across to trigger a catastrophe in which more than one-quarter of the human population dies. An asteroid of that size is thought to strike Earth about once every 300,000 years. Scientists disagree on which objects pose the greatest threat. Many think enormous objects are the most dangerous though they are relatively rare. "The largest -- bigger than a mile across -- are most bothersome because they have the potential for global and catastrophic effects," says Gregory Canavan of Los Alamos National Laboratory in New Mexico. Other scientists think more frequent, smaller collisions are the biggest danger. "What's more of a threat, in terms of global economy, are the smaller objects, most of which we haven't discovered at all," Hartmann says. The first steps in addressing such hazards are to locate Earth-threatening objects and then to calculate their orbits. Today, few scientists are engaged in the effort to find near-Earth objects, though the number is growing. Morrison is fond of saying "The total staff searching worldwide is less than the total staff of one McDonald's restaurant." Gehrels and his colleagues at the Space-watch telescope at Kitt Peak National Observatory near Tucson have discovered about two-thirds of the known near-Earth objects. Other new or updated search programs are based at the Lowell Observatory in Flagstaff, Arizona, and in Haleakala, Hawaii. The Haleakala program alone discovered four new Earth-crossing asteroids and a fast-moving comet last March, the first "good weather" month for observing since the program began in December 1995. "These discoveries certainly suggest that we could face a surprise encounter with a large, unseen object," says lead scientist Eleanor Helin. Still, many scientists think these efforts are not enough. "At present, we know only one to three percent of the objects that could do global damage or even extinguish the human race," says astronomer Brian Marsden of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Massachusetts. If scientists locate an asteroid or comet threatening Earth, it would probably be far enough away that we'd have decades, perhaps centuries, to prepare for its impact, Marsden says. What kind of strategy rye would mount against the hazard depends not only on the length of time available but on the size and makeup of the object. If a meteor were identified that would hit in only a few months, "all we could do would be to plot where the impact would occur and attempt evacuations and civil defense-type measures," says Alan Harris of the Jet Propulsion Laboratory in Pasadena, California. With more advanced warning, it might be possible to deploy specially designed nuclear warheads to blow up the object. But there are drawbacks to such a strategy. The explosives must be enormously powerful or else must bury themselves deep enough in the asteroid to shatter it into fragments less than 160 feet across -- small enough to ensure that they will burn up in Earth's atmosphere. Any large remaining fragments also on a collision course with Earth could be just as serious a threat as the original object. Deflecting the invader from its path appears to be a better strategy. A small nudge, averaging less than half an inch per second over ten years, can push an object six-tenths of a mile in diameter out of a collision course with Earth. The thrust could be provided by a series of one megaton nuclear explosives detonated on the asteroid's side. An asteroid can also be deflected if its mass is decreased enough to change its velocity. A bomb detonated near the body could cause the outer layer to spall off and alter its mass. Some scientists think a nuclear solution is the only sensible way to avoid a collision. They say the technology is understood and could be modified quickly for use. "Nuclear weapons are the highest-energy weapons we know of and the odds-on favorite to intercede and blow the thing up into chunks or slowly deflect it," Harris says. Others support the use of nuclear weapons to deter collisions in only the most extreme cases. They maintain that nuclear weapons may not be as effective as some think because the physical properties of asteroids are poorly understood. In addition, there are inherent risks in the very existence of such a powerful nuclear arsenal, and, by international agreement, it is illegal to detonate nuclear weapons in space. A few scientists, such as Carl Sagan of Cornell University, believe that a nuclear defense system capable of deflecting an approaching object could be used by a terrorist organization to knock a harmless object into a collision course with Earth. Non-nuclear technologies to deflect an asteroid, including Earth-or spacecraft-based lasers, rely on altering the asteroid's mass by incinerating its outer layer. Planetary scientist Jay Melosh of the University of Arizona has proposed vaporizing the object's surface by focusing sunlight from an enormous solar collector. If necessary, a solar collector defense might be realized in a decade. Most scientists involved in these studies agree that humans probably won't be wiped out by an impactor in the next generation. So, they say, it is too dangerous and expensive to develop a full-scale defense system in the absence of an identified threat. "If an asteroid is found to be on a collision course, people will spend anything to defend against it," Melosh says. "But I don't think large sums will be spent to protect against anything purely hypothetical." A very few scientists think the seriousness of the hazard justifies beginning work on a defense system now. Edward Teller, often called the father of the hydrogen bomb, has in recent papers and talks advocated experiments on asteroids and comets, including testing nuclear explosions on asteroids in space. In his opinion, expenditures of roughly $100 million per year are warranted. Meanwhile, Melosh and many others agree that research on defense systems should be maintained at a low level with an emphasis on non-nuclear defenses. They advocate locating and determining orbits for all Earth-crossing asteroids and increasing efforts to search for hazardous comets. "There's a good reason to conduct surveys and to try to determine how much hazard we have and if something is coming our way," Harris says. "I personally don't think it's worth another Cold War build-up just in case." Still, questions about the future of humanity linger. If the impact theory is correct, mammals didn't get ahead because they were better adapted or smarter than reptiles; their rise to power was brought on by a roll of the cosmic dice. Dinosaurs didn't survive the impact, whereas a precious few stocks of mammals did. "It is not some imagined superiority of mammals versus reptiles but much more a matter of sheer chance that finally shifted the balance of control of terrestrial ecosystems from reptiles to mammals," writes paleontologist Niles Eldredge. When the dice are thrown again, our kind may be the next to go. We can allow evolution to take its natural course or we can do what the dinosaurs did not have the capability to do: We can search and, if necessary, we can defend. Marsden suggests that we have a responsibility to do more than just survey for threats to Earth. He points out that it takes only one object hitting Earth to wreak havoc on the planet. "Chances are it will be 100 million years in the future, but it could be tomorrow," he says. "Considering all the tomorrows there are in the next couple of centuries, we owe it to our descendants to do something about it." Meteorites striking Earth are events that don't happen very often, but when they do they can be deadly on a global scale. Your os of dying in a meteorite impact may be higher than you think. Size of impactor Frequency of impact Odds of dying Less than 50 meters Burns up in atmosphere None 50-100 meters Every few centuries or 1 in 3 million 100,000 years in cities. 100 meters-1 kilometer 1,000-2,000 years 1 in 25,000 Greater than 1 km Every 100,000 years 1 in 200,000 or greater PHOTO (COLOR): An asteroid slams into Washington, D.C. in this painting by space artist Michael Carroll. As farfetched as it seems, this scene is entirely plausible: fragments of asteroids and comets have battered Earth repeatedly over its history and will undoubtedly do so again. PHOTO (COLOR): Though buried in Mexico's Yucatan Peninsula, the Chicxulub Crater is visible in this image of the gravity exerted by the crust here. This crater was created when an asteroid slammed into Earth 65 million years ago. The impact may have indirectly killed two-thirds of Earth's species, including the dinosaurs. PHOTO (COLOR): The South Pole-Aitken basin on the Moon, shown here as a purple and blue splotch, is the largest impact crater known in our solar system. An asteroid or comet slammed into the Moon with such force that it penetrated the mantle and left behind this scar, more than 1,300 miles across. PHOTO (COLOR): In this mosaic based on images from the Clementine spacecraft, Earth rises above the pockmarked surface of the Moon. Were it not for the continuous recycling of Earth's crust by plate tectonics, Earth's surface would probably bear many marks from impacts as well. PHOTO (COLOR): Some impact craters on Earth have not yet been recycled by tectonic processes. This is Meteor Crater, also known as Barringer Crater, in northern Arizona -- one of the best-preserved. It was also the first to be recognized as the scar of an extraterrestrial object slamming into our planet. PHOTO (COLOR): The crater known as Manicouagan in eastern Quebec, Canada, measures an impressive 62 miles across. PHOTO (COLOR): This view of Jupiter in 1994 using ultraviolet wavelengths shows the "bruises" left by pieces of the shattered Comet Shoemaker-Levy 9 that punched into the giant gas planet. (The bruises are in the southern hemisphere.) PHOTO (COLOR): This map depicts most of the roughly 150 impact craters that have been discovered on Earth. The apparent concentration of craters in North America, Europe, Australia and Russia is partly due to thorough exploration of these areas by geologists. DIAGRAMS: The two main threats to Earth come from wayward comets or asteroids that are nudged out of their usual paths into Earth-crossing orbits. Asteroids are bits of rock that mainly orbit the sun between Mars and Jupiter (top diagram). They're thought to be debris that never coalesced into a planet because of Jupiter's wrenching gravitational pull. Comets, on the other hand, are bits of rock held together by ice. They reside in two main areas outside our solar system known as the Kuiper Belt and the Oort Cloud. The Kuiper Belt (middle diagram), which includes the planet Pluto, is a disk of rock debris beyond the orbit of Neptune. The Oort Cloud (bottom diagram) stretches as far as one-fifth the distance to our next nearest star, Alpha Centauri. In this diagram, scale is rendered in astronomical units, or a.u. One a.u. is the Earth-Sun distance. GRAPH: The graph at left shows how often meteorites of a certain size smash into Earth today (pink dots) and also how the frequency of impacts has changed over the course of Earth's history. Small rocks hit more frequently and do less damage than large ones. (Anything smaller than about 50 meters across will burn up in the atmosphere and leave no crater on the surface.) In its infancy, Earth was bombarded by meteorites far more often than today. In the first 60 million years of its existence, Earth was struck more often by larger objects (yellow dots). Then, 4 billion years ago, bombardment began to slow down (purple dots), until it reached the present rate. PHOTO (BLACK & WHITE): In 1908, a mysterious object exploded above the Tunguska Valley in Siberia, knocking residents and their reindeer flat. After years of speculating on the cause of the blast, scientists now think that an asteroid about 200 feet in diameter entered the atmosphere and exploded three to six miles above the ground. The force of the blast downed thousands of trees, as shown in this 1929 photo. ~~~~~~~~ by Dana Desonie Dana Desonie teaches geology and oceanography at Arizona State University in Tempe. _________________________________________________________________ Inset Article CRATERS, CRATERS EVERYWHERE There's something to be said for a bird's-eye view, especially when it comes to discovering new impact craters. Scientists have recently been using satellite imagery to identify features that look like possible impact craters from space. On the ground, geologists can then positively identify the crater by finding minerals that are characteristically formed in a high-energy impact. The image at left shows what may be a previously unrecognized meteorite crater in western Wisconsin. Sanjay Limaye of the Space Science and Engineering Center in Madison, Wisconsin, says he has noticed this circular feature, which measures more than 60 miles across, on satellite images of the area for 15 years. This image was taken by NOAA instruments in January 1996. The image below was taken by the SIR-C radar system carried aboard the space shuttle. The ring structure left of center is the previously identified Aorounga crater in Chad. But this new image reveals more details: a possible second and even third impact crater, to the right of and above the confirmed one. NASA scientists speculate that this chain of craters may have formed when a comet or asteroid broke into several pieces before slamming into Earth, just as Comet Shoemaker-Levy 9 did at Jupiter. PHOTOS (COLOR): Different craters on earth cause by slamming comets ~~~~~~~~ By Alexandra Witze _________________ Copyright of Earth is the property of Kalmbach Publishing Co. and its content may not be copied or emailed to multiple sites or posted to a listserv without the copyright holder's express written permission. However, users may print, download, or email articles for individual use. Source: Earth, Aug96, Vol. 5 Issue 4, p24, 8p, 1 chart, 12c. Item Number: 9607032823