What are comets mainly made of? Solar system. Comets. Heavenly Wanderers

Comets- (from Greek kometes - “star with a tail”, “comet”, “shaggy”; literally - "long-haired"), small bodies of the Solar System, revolving around the Sun in elongated orbits and having the appearance of nebulous objects, usually with a light clump - a core in the center and a tail. As it approaches the Sun, the comet's tail, formed by gases evaporating under the sun's heat, enlarges.

A few days ago, the area of ​​the comet where Rosetta will descend became known. This is Maat, in the smallest lobe of the two, consisting of a comet where some active regions are observed. Seriously, the Sun is a star that shines with its own light and was formed about 5 billion years ago and will continue to live for probably another 5 billion years.

The distance of the Sun from the Earth is about 150 million kilometers and is considered an astronomical unit. The distance of the Sun from other stars is measured in light years. A light year is the distance traveled by a ray of light per year traveling at about a thousand times the speed of the Earth. It is made up of 75 percent hydrogen, 20 percent helium and traces of other elements such as oxygen, carbon and nitrogen.

Comet Hale-Bopp 1996

Presumably, long-period comets come to us from the “Oort Cloud,” located on the outer boundaries of the Solar System, in which millions of cometary nuclei circulate.

Comets are shapeless blocks only a few kilometers in size, consisting of ice mixed with dust particles. Comets move in very elongated orbits, spending most of the time far from the Sun, where they remain invisible, and when they approach the Sun, ice begins to melt under the influence of solar heat, evaporating and escaping into interplanetary space along with other gases. As a result, many comets, passing near the Sun, take on a very unusual appearance.

Such high values ​​depend on the enormous amount of heat generated by the nuclear fusion process occurring inside the Sun. In this process, four hydrogen nuclei fuse to form a helium nucleus. During nuclear fusion, a small amount of a substance produces great amount energy. Nuclear reactions occur in the central region of the Sun, called the core.

Energy is transferred by irradiation and conditionally from the center to the surface. The surface of the Sun is called the photosphere and emits visible radiation, or radiation that can be seen as bright. The photosphere often exhibits darker areas caused by lower temperature gas vortices called sunburns.

Most comets that periodically appear in the vicinity of the Sun are rather faint objects. The exception is Halley's Comet, which appears before us as a very bright and impressive object on almost every return to the Sun.

In fact, the brightest and most spectacular comets appear unexpectedly in the sky, many of them perhaps approaching the Sun for the first time. Those few weeks during which a bright comet quickly circles the Sun, then disappearing forever or, perhaps, for many millennia in space, are the hottest time for cometary astronomers. In rare cases, especially if a comet comes too close to the Sun, it can break into pieces that are later observed as separate bodies (comet nuclear decay).

A thin, colored layer called the chromosphere marks the boundary between the photosphere and the corona. The corona is the outermost region of the solar atmosphere, visible only during eclipses. At this point the Sun is at what should be its maximum, although it appears quite calm.

Comets are composed of gas masses mixed with dust, ice and fragments stone material. Comets are believed to originate from regions of the solar system far beyond Pluto, where a cloud formed from billions of protocomets would be located.



Orbit of a periodic comet and tail formation

What are they made of?

Comets look different. Everyone has a foggy gas envelope - coma, which together with the nucleus forms the head of the comet. Even if the comet is in close proximity from the Sun, her head appears to be nothing more than a hazy speck. The most remarkable feature of most comets is tail. It is brightest when the comet is near the perihelion of its orbit. Here, the heat flow from the Sun is especially significant, under the influence of which gases and dust evaporate from the comet into outer space. Some comets have two tails: one is curved, consisting of dust particles; the other is straight, gaseous, elongated in the direction exactly opposite to the direction of the Sun. A number of comets have been observed to have multiple (dust) tails.

Protocoms are nuclei consisting of solid particles, which, after penetrating into the Solar System and approaching the Sun, undergo partial evaporation under the influence of solar energy. More specifically, as the protometer approaches the Sun, some of the frozen material from which it is formed evaporates, forming a gaseous cloud called a hair and tail. The comet then forms a head, formed in turn by a nucleus, surrounded by hair and a tail, which always turns on the opposite side of the Sun.

Length comet tails can reach tens and hundreds of millions of kilometers; comets were observed whose tails stretched almost half the sky. It is assumed that dust lost by comets, entering interplanetary space, gives rise to meteor bodies, which later, colliding at great speed with the earth’s atmosphere, are detected in the form of meteors. Dust grains from comet tails also replenish interplanetary dust clouds, which, scattering the sun's rays, give rise to a phenomenon called zodiacal light.

Comets orbit the Sun in very elongated elliptical orbits and can be seen from Earth at controlled intervals. When a comet's orbit is relatively short, it appears after short intervals; if instead it is very long, the comet takes many years before passing through the inner solar system. It may happen that a comet, having presented itself at regular intervals, disappears and no longer appears for a ritual purpose.

The disappearance may be due to the fact that it escaped the sun's gravity and is lost in interstellar space, or that, passing too close to the Sun, it simply disintegrated. According to many theories, comets contributed to the formation of water on our planet.

Core comets are sometimes visible inside the coma as a bright star-shaped object in which no details can be discerned even with the largest telescopes. Sometimes the nucleus can be confused with various structural formations in a coma - such as a shell or ejections of matter from the comet's nucleus. Comet nuclei were studied in detail by spacecraft that approached comets.

Additional information about stars. The star comes from a cloud of gas and cosmic dust that takes its name as a nebula. Mana, that particles of the cloud matter attract each other, forming more and more masses, the temperature of the nebula rises, and the star begins to glow.

When the temperature reaches approximately 10 million degrees Celsius in the stellar core, nuclear fusion occurs, creating a huge amount of energy that reaches the surface of the star and is radiated into space. A star's life depends on its size. When a small or medium-sized star runs out of hydrogen present in its core, it undergoes rapid contraction accompanied by a rise in temperature. The heat that is heated warms the surrounding gases, causing the formation of helium.

In 2005, NASA's Deep Impact spacecraft rammed Comet Tempel 1 and transmitted images of its surface.


The nucleus of Comet Tempel 1 (photo by the Deep Impact apparatus)

Comet observations

Any instrument can be used to observe comets. Experience shows that giant comet tails can be detected with the naked eye, binoculars and telescopes with a wide field of view. But to see the complex structure of a comet near its nucleus, telescopes with large apertures and high magnification are needed.

A star at this stage is called a giant or supergiant star and is at the end of its existence. A white dwarf is nothing more than the dying core of a giant star, so called by astronomers for the faint white light it emits. When a white dwarf has exhausted all its energy, it turns into a black dwarf. It may happen that in an area of ​​the sky where a star has never been observed, it may suddenly appear very bright, which disappears after a certain period of time.

A star of this type is called a nova. According to astronomers, the nova is the product of a violent stellar explosion, during which the material that forms the outer layer of the star is dispersed into space. After the explosion, the remaining gas, once cooled, wraps around what is left of the star, forming a nebula visible to telescopes for many years.

Sketches of comets can be made during observations using any instruments; the technique is the same as for sketching planets.

Photographing comets

Photographs help not only determine the exact position of the comet's head, but also provide an image of its tail, as well as see fine details that, due to their low brightness, cannot be seen in other ways.

However, not all stars become white dwarfs. In fact, if the star's mass is large enough, the star can explode, leaving behind a cloud of gas and forming a neutron star. In a neutron star, matter is so compressed that it has a density of a billion tons per cubic centimeter. Therefore, its mass can be no more than two to three times higher than that of the Sun and its gravity and 100 billion times higher than that of the Earth.

When you have a supernova, you can also form a pulsar, which is a neutron star that spins rapidly on its axis. These stars emit radio waves that allow astronomers to determine their rotation speed using telescopic radio receivers.

With an instrument equipped with a clock mechanism, you can try to take a photograph of the comet. With a long-focus refractor, sometimes a shutter speed of 5-10 minutes is enough to get a clear image of the comet's nucleus.

To track a comet, taking into account its own movement among the stars, the telescope (or camera) must be equipped with a guidance system. In this case, the images of stars in the photographs will appear in the form of dashes. When using short-focus lenses, guiding can be done directly by the stars.

If the process of contraction of a neutron star or pulsar, such a gravitational collapse, never stops, the star can be reduced to a single point. These points are called black holes. In a black hole, the material is so compacted that the force of gravity is so strong that it cannot escape the light either. Black holes are therefore invisible. Thanks to new technologies, astronomers have now identified a large number of black holes.

Comets, those lonely vagabonds of space, attracted to the Sun like butterflies of night lights, were born at the same time as our solar system about four and a half billion years ago, but, unlike the planets, the ancient ice and dust of comets have remained motionless since then .

For photographing a comet's tail, a short-focus fast camera is preferable. A large aperture makes it possible, with a not very long shutter speed, to get the tail of a comet far from the head in the photograph. Such a photograph can give an idea of ​​the structure of the comet.

Comet designations

Until 1995, the order in which comets were designated was as follows. At the beginning, the comet was designated by the year of discovery and a small letter of the Latin alphabet (in order of discovery). The final designation of the comet consisted of the year, the number (Roman numeral) in the order of the moments of perihelion passage, and the surname of the discoverer (or two or three surnames of the persons who independently discovered the comet). For example, comet 1957f=1957 IX was called comet Latyshev-Wild-Burnham.

So there are windows to the past through which we can look at when it all began. Comets are associated with our history and our legends, and have been feared for centuries because they were guilty of bad luck and unbelief. Their passage was met with superstitious concern, but while many feared these mysterious strings of light that moved across the night sky, others, not blinded by superstition, considered them part of the nature they were trying to understand.

Among them is the English astronomer Edmund Halley. For this prediction, Halley laughed, but a subsequent passage of the comet confirmed his intuition. The largest comets were then intensively studied by scientists. Comets are a very mysterious small body in the solar system that mostly move along elliptical curves. They are actually "dirty ice balls". They come from rocks, dust and dirt that contain water ice and frozen gases. The name of these pseudosciences comes from the Hebrew word for "comets" or long-haired.

Since January 1995, a new rule for naming comets has been in effect, and it extends back to all comets of the past with well-known orbits. Now after the year number they put a Latin letter (from A to Y), indicating in which half of which month the discovery took place: A - from January 1 to 15, B - from January 16 to 31, C - from February 1 to 15, etc. .d. The letter I is not used so as not to confuse it with the number 1 and the letter J. After the letter they put a number - the serial number of the opening in this half of the month.

In Czech sources the name “hairy” appears most often. Observation of comets From the beginning to the present, comets have already been considered the bearer of life and death. Perhaps this is the reason for life and perhaps the end different years on the ground. These small bodies are considered to be the objects of origin of the solar system. They were certainly observed in our prehistoric times, and the oldest records of their injections can be found in archival documents from the East. The oldest document is from internal sources from 240 BC. This discovery was Halley's Comet.

But hundreds of scientists believed that these were just “exhausts” in the Earth’s atmosphere. By the end of the century, a total of 150 comets had been recorded, but there were repeated recoils on a number of occasions cometary comets. Over the centuries, the most successful comet hunter, Jean-Louis Pons, discovered 37 comets. Johann Enck helped Laplace's theory identify the comet with the shortest period of 3.3 years. Named after Enck, which did not belong to the discoverers. This was the first time a comet was associated with meteor shower, which later managed to prove a majority for all large meteor swarms.

Before the opening date, one letter indicates the “status” of the object:

P (periodic) - a comet with an orbital period of less than 200 years;
C (comet) - long period comet, with a period of more than 200 years;
D (disappear) - disappeared comet;
X is a comet for which it was not possible to calculate the orbit accurately enough.
For periodic comets, instead of the discovery date, there is a serial number in front of the calculation of the exact orbit (this is reminiscent of the designation system for asteroids), for example, Halley's comet now has a permanent designation: IP/Halley, and comet Encke - 2P/Enske.

This team's discovery contributed significantly to the understanding of the physics of comets. The capture of the photographs was a result of the upcoming discovery and better understanding of the morphology of comets. Regardless of this, Gerard Kuiper came up with the idea of ​​a cometary disk beyond the outer edge of a planetary system.

This verse with a giant planet shows that our planet can pose a threat to our comets. Parts of this comet created Earth-sized crumbs on Jupiter that would have catastrophic consequences for our planet. Although Jupiter acts as a "planetary vacuum" in our system, sometimes a comet breaks up and lands on Earth. Many scientists agree that comets are more dangerous to us than asteroids. The reason is the late observation of comets. They are visible until they approach the Sun to begin releasing gases.

Now the names of astronomers need not be written, although traditionally they still do this and sometimes even put them in front, for example, Tempel-Tuttle (55Р). The old designation for Comet Shoemaker-Levy 9 (which fell on Jupiter) was 1993e, and the new one is D/1993 F2.

Finally

The masses of comets are very small - about a billion times less than the mass of our Earth, and the density of matter in their tails is practically zero. Therefore, “heavenly guests” do not in any way affect the planets of the solar system, much less the lives of people. In May 1910, for example, the Earth passed through the tail of Comet Halley, but no changes in the movement of our planet occurred and no clearly related phenomena were noticed on Earth. However, history preserves the fear and fear of our ancestors before these heavenly wanderers. And very often one can find in ancient chronicles and chronicles references to the appearance bright comets in the sky and the connection of these phenomena with earthly incidents - fires, wars and even the deaths of individual people.

In the future he is considering sending spacecraft to become cometary satellites or take samples of cometary rock. Documentary: Vesmer - a trip to the comet. Description of the comet This is a very dark body that reflects 3 to 4% of the light. A comet consists of a nucleus, a coma, and a ponytail. The nucleus is the solid part of the comet that is likely to be produced during gravitational impacts from icy planes at the edge of the system. The comet's nucleus is essentially permanent until it approaches the Sun, causing gravitational destruction.


Vintage image of a comet

On the other hand, the collision of a large comet with a planet can cause large-scale effects in the atmosphere and magnetosphere of the planet. A good and fairly well-studied example of such a collision was the collision of debris from comet Shoemaker-Levy 9 with Jupiter in July 1994.

Let us hope that the growing scientific and technical potential of our civilization will help in the future to protect Earthlings from death in the event of a dangerous collision with the Earth of a large nucleus of a comet.

Materials used:

Kulikovsky P. G. Handbook for an Astronomy Amateur / Ed. V. G. Surdina. Ed. 5th, revised and full updated - M.: Editorial URSS, 2002. - 688 p.
- Dunlop S. ABC of the starry sky: Trans. from English/Ed. and with a preface. A. V. Kozenko. M.: Mir, 1990. - 238 pp., ill.
- Website astropage.ru
- Wikipedia website