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The large asteroid Florence will pass on September 1, 2017 at a distance of 7 million km from our planet. According to the press service of the Jet Propulsion Laboratory at the California Institute of Technology, this celestial body is approximately 4.4 km in diameter, which is comparable to small town, does not pose a threat to humanity: at the moment of Florence’s closest approach to the Earth, the asteroid will be 18 times farther from our planet than the Moon.

Esa and NASA's joint Hades mission, which is applied to asteroid protection, should lead to this knowledge. The distance was about 1.8 million kilometers or 4.6 times the Earth-Moon distance. As dense as the earth's moon. It will be close, explains Wünnemann. But: “Everything that passes is not dangerous.”

By definition, meteorites are more or less large fragments of asteroids or comets that land on Earth. However, most of these bodies burn up upon entering the Earth's atmosphere, the resulting glowing phenomenon is called a meteor. Often, cosmic chunks of rock fall into the sea or float down uninhabited areas, so the consequences often go unnoticed. Here the impact on populated regions is extremely rare. Could this affect the meteorite, as in Chelyabinsk, Germany? "It's not impossible, but it's unlikely," says Manfred Gajda of the German Aerospace Center, "only because of Germany's relatively small area."

To observe the asteroid, a radio telescope in Arecibo (Puerto Rico) with a reflector mirror diameter of 304 m, as well as NASA radars in California, will be used. The data obtained will make it possible to distinguish features on the surface of an asteroid approximately 10 m in size.

As Paul Chodes, head of the US National Aeronautics and Space Administration (NASA) Center for the Study of Celestial Bodies in Near-Earth Space, said, most of the asteroids passed at a closer distance from planet Earth, but they were all smaller in size than Florence. This is the first time since the start of NASA's asteroid observation program that such a large asteroid is getting closer to the Earth.

Most extraterrestrial rocks burn up on their way to Earth

However, in general: a meteorite can fall anywhere in the world. However, the risk of hitting such a stone is very low. He will most likely be killed by lightning. There are several classes of meteorites. They are usually predominantly silicate minerals or an iron-nickel alloy, and many also contain higher amounts of carbon. Large objects with masses of several tons are unlikely to be slowed down by air resistance. The fireball, consisting of frozen gases, must be about 100 meters in diameter to survive its passage through the earth's atmosphere, iron-nickel 30 meters.

The most eminent scientists from the Russian Academy of Sciences have already expressed their opinion on this matter. They believe that the Earth cannot be saved from outside danger in any case, Vlad-Time reports. Thus, out of 15 thousand potentially dangerous celestial bodies, every 9th can actually cause harm to our planet. In addition, the most powerful telescopes in the world can only recognize large celestial bodies, and those meteorites with a diameter of less than 20 m will remain outside the field of view of researchers.

These projectiles hit earth's surface at speeds from 10 to 70 kilometers per second and can penetrate to depths of up to 100 meters. This creates a typical meteorite crater because the surrounding material is blown away by the intense impact energy. The planets and our solar system are literally littered with meteorite craters. Also, the earth is no exception: in the past, it has been hit again and again by meteorites of all size classes. But with erosion and weathering, traces of most impacts were erased from their surface.

Today, about 200 large impact structures are known. The impact was 65 million years ago and likely extinguished. The pollutant was a 10 km class asteroid. Fortunately, such space projectiles rarely hit Earth every 100 million years. There are 1-meter meteorite hits once a year, but most of them land in the sea.


The RAS is confident that falls of this kind celestial body humanity finds out only just before its collision with the planet. As domestic scientists note, so far there is not a single technical device in the world that could protect the Earth from cosmic danger, and who knows when it will appear in the course of technical progress.

We're talking about a rock no more than twenty meters in size that could generate almost thirty times more energy than the Hiroshima bomb, although fortunately almost all of this energy was dissipated in the atmosphere. And this has raised troubling questions: If we didn't see it coming, what are the chances of being surprised by an even bigger and more dangerous meteorite?

The truth is that the proximity of Earth's orbit receives a lot of visits. And then there's this: If you were looking at the lost moon in a dream in May of that year, and you were in a place with little pollution, you might have been able to see with your naked eye a brief flare caused by the impact of an asteroid against our moon.

The Florence asteroid was discovered by Australian astronomers in March 1981. It was named after the prominent British public figure Florence Nightingale (1820-1910), who organized the service medical care wounded during the Crimean War (1853-1856). Astronomers have calculated that the next approach of the Florence asteroid to Earth will occur after 2500.

This is all over the course of a few months, so the threat of an asteroid or comet impact should not be taken as a joke. Interplanetary space is not as empty as we might have assumed, and the transit of material is constant. Space dust: despite the possible double joke reading, we're just talking about large quantities particles less than one millimeter in size. -Steroids: Rocky objects that, although very small compared to planets, can sometimes reach several kilometers in diameter. -Composition: objects containing ice or gases, the evaporation of which leads to coma, this luminous tail, which in exceptional cases is clearly visible from the Earth even in broad daylight and with the naked eye.

The asteroid can be observed using a telescope. In the sky it will take place in such constellations as Southern Pisces, Aquarius, Capricorn and Dolphin.

For the first time, asteroid 2012 TC4 attracted the attention of the general public (the number 2012 in the asteroid’s name indicates the year of its discovery).

Like asteroids, their cores can also measure several kilometers in diameter. -Meteoroids: Small asteroids are generally considered small if they have a diameter of less than 50 meters, like the one that exploded in Russia this year. -Meteor: Any of the above objects that survive impact with the Earth's atmosphere and directly impact the surface. - Meteor: A luminous phenomenon created by the entry of an object into the Earth's atmosphere, but which does not affect the surface.

Recent asteroid impact on the Moon in May. In fact, about a hundred tons of space material fall to Earth every twenty-four hours, attracted by our planet's gravity. Of course, the vast majority are tiny dust particles from comet breakups or collisions between asteroids. Often these tiny particles are enough to create a fleeting but bright trail of light in the night sky, a “shooting star”, before whose vision we smile or even ask for a wish. As we know from this romantic picture, the Earth is bombarded daily by tiny meteors that can never cross the atmosphere without being thrown away and whose ability to harm us is absolutely nil.

Astronomers' interest in the asteroid was caused by the fact that, according to calculations, its next passage near the Earth was supposed to occur on October 12, 2017.

Like all celestial bodies of this kind, the asteroid has a very elongated orbit, so the distance to which it will approach the Earth can never be predicted in advance with great accuracy.

But among all this cosmic dust there are also several objects of noticeable size that could have very serious consequences if they hit Earth, and it is certainly a matter of time before one of these large objects hits our planet. If you prefer to keep the hopeful part of matter, you can take refuge in statistics: for huge sizes solar system we can say that the number of threatening objects is decreasing. In fact, it is estimated that the likelihood of a direct impact from a large asteroid is almost negligible in the temporary conditions of human life.

The generally accepted unit for measuring the distance to asteroids that could threaten the planet is the average distance to the Moon, which is 384,467 km or 30 times the diameter of the Earth. In astronomy, this unit of measurement is designated as LD (Lunar Distance).

During its last pass near the Earth (in 2012), asteroid 2012 TC4 approached the planet at a distance of 0.247 LD (Lunar Distance), which is approximately 94,800 km.

One asteroid with a diameter of one kilometer would impact the Earth every two hundred thousand years at most. A five-kilometer asteroid fell only once every ten million years. And another hundred kilometers, at least once every hundred million years. You might say, "Oh, well, then there's nothing to worry about." The problem is that these statistics tell us the global probability of an impact occurring over a period of time, yes, but it doesn't actually tell us at what point in that period it will occur.

If a stock kilometer mastodon falls every hundred million years, does it do so at the beginning or end of that period? As unlikely as it may seem, it could happen tomorrow. This can happen twice in a row. That's what statistics are: they give us the big picture of a situation, but they don't really help get into the "when will it happen" style details.

According to the calculations of astronomers who observed the orbit of the asteroid in the period 2012-2015, the next time it should approach the Earth on October 12, 2017, passing at the same significant distance as the last time.

If you believe the laws of classical mechanics, which relatively accurately describe the movements of celestial bodies, for an asteroid to fall to Earth it must pass at a distance of 0.079 LD from the planet. Since on October 12, 2017, 2012 TC4 was supposed to be at a much greater distance from Earth, the probability of its collision with the planet was estimated as 0.00055%.

It's completely unpredictable. Apart from what inaccurate statistics always seem to say, the only way to get reliable information about the exact moment during which an object could have hit Earth is to find them using astronomical instruments. In other words, there are thousands of space objects floating around it, the orbit of which will sooner or later pass very close to our planet.

But what will be the consequences of exposure? Obviously, the answer depends on the size of the asteroid, the angle at which it hits, and the exact location in our geography where it hits. Estimates of the destruction potential of these objects are always approximate, since they depend on many factors and necessarily contain errors. But let's try to figure it out, collecting geological data on impacts that occurred earlier, for example. Or observing recent phenomena such as the commented February asteroid.

However, as it now turns out, these were erroneous calculations. According to the latest data, asteroid 2012 TC4 may approach Earth as close as 4,000 miles. This is an almost guaranteed collision of a celestial body with a planet:

The Tunguska episode is attributed to an asteroid, or rather a piece of a medium-sized comet, and is the only historical evidence of such an event in the era of human civilization. Although events such as Tunguska may be relatively frequent, although not always observed by the population, which, as we remember, were very scarce until several centuries ago. Small meteorite impacts, which do not always disintegrate in the atmosphere, are much more common. In the last decade, meteorites have fallen on houses or buildings in Cali, Colombia or Chinese city Zunhua.

In this dramatic situation, it now becomes extremely important for astronomers to accurately determine the size of the asteroid and its composition.

According to official According to 2012 estimates, the size of the asteroid is estimated at 10-40 meters in diameter. For comparison Chelyabinsk meteorite, which fell in February 2013, had a maximum diameter of 20 meters. Therefore, a rock measuring 40 x 40 meters will be quite large.

Obviously, the recovery of these meteorites allows them to be identified as being of extraterrestrial origin. But let's put ourselves in the worst case and imagine a rock that is much larger than the one that erupted a few months ago in Russia and even the famous and mysterious Tunguska site. Imagine that a one kilometer asteroid hits the Earth, for example. This would create the equivalent of an earthquake of magnitude 9.5 on the Richter scale throughout the surrounding region: more or less the intensity of the largest earthquake we have recorded in modern measuring systems.

However, the problem is that Exact size Astronomers can determine an asteroid only by knowing exactly the reflectance of the substance that makes up its surface. If it's a block comet ice, which shines very brightly - the size of the asteroid can be calculated with an accuracy of centimeters. But if it is a huge coal rock, its size will be estimated as the size of a spot of shiny rock coming to the surface.

It would also create a crater twenty-four kilometers in diameter, more than enough to swallow the largest of our cities. The airburst could extend for one hundred and fifty kilometers around, causing various types of damage. Three hundred kilometers away, he could still knock down a few trees and blow out windows. This: if a one kilometer asteroid hits Madrid, it is possible that even in Valencia Zaragoza or Cordoba were injured by glass fragments, breaking the windows of their own houses and vice versa.

But let's be even more pessimistic and imagine a rock ten times larger, ten kilometers in diameter, falling on our planet. This ten-kilometer asteroid will produce a 12-degree Richter earthquake in the area of ​​impact - an intensity we have never recorded in our seismographs - although the region will be completely removed from the map immediately, becoming a crater. about two hundred kilometers. Malasombra's shockwave shook the forests and populations of a thousand kilometers of terrain around him, although he allowed himself to feel one way or another four thousand kilometers away.

It is also very important to know what an asteroid consists of, that is, what is its core? If it is a piece of ice or loose rock, then even with a diameter of 100 meters such an asteroid does not pose a particular threat; it will fall apart when braking against the atmosphere. But if there is a 40-meter piece of refractory rock or even iron inside, almost all of it will reach the surface

This asteroid could hit Warsaw or Athens, and the noise of the impact will wake you from your siesta in almost every corner of Spain, except perhaps Canary Islands. In the case, of course, that he had not yet woken up when he felt a huge earthquake. Thus, during the same exposure, Malasombra could reduce small country to rubble. But the consequences of this impact will also be global and will depend on whether it occurs on land or at sea. To fall into the ocean, a terrible tsunami will occur.

Our hypothetical Malasombra would make waves of unimaginable size; some come to estimate that, given the exact conditions, they could reach thousands of meters in their highest point. Even after they had traveled several thousand kilometers from the point of impact, these waves could continue to measure one hundred meters in height at coastal areas, very far from the epicenter. These regions will be washed away with even worse consequences than those that occurred in the last tsunamis that we can all remember.