Open Category: astronomy, solar system, asteroids, ,],[ 3 http://www.
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xkcq.lamost.org http://www.souezu.cn/Item/50246.aspx dinosaurs have
also died. American scientists in 1991, with the radioisotope method,
the measured Gulf of Mexico, Yucatan Peninsula, a large crater
(diameter about 180 km) of the age of about 6505.18 million years.
Found that the surface crater from the point of view, there is likely
to occur every three million years for the 500-meter diameter asteroid
hitting the Earth event. Greater probability of an asteroid strike,
even smaller. Probability of an asteroid hit the Earth may hit the
Earth in 2014 is 90 parts per million chance BEIJING, Sept. 3, 2003
Xinhua research arm of the United Kingdom and the United States, warned
that an asteroid could hit Earth in 2014, but the probability is 90
more than a million. According to the BBC news, the British
government's Near Earth Objects Research Center, said the U.S.
astronomers discovered a size However, scientists estimate, 杩欓 known
as They further pointed out one after another to collect the latest
data show that the risk of potential impact will continue to decline.
Although the probability of the asteroid hitting Earth is very low,
based on the volume of Fengyun small trekking and speed, it is worth it
for the scientists observed. This However, its speed is 20 miles per
second, per minute at up to 120 miles. As the speed quickly, and if hit
Earth, it can have catastrophic effects on Earth. U.S. astronomers will
be closely observed in the next two months, Asteroid hit the Earth in
the eyes of the artist scene of a British space expert has said that a
giant asteroid named 2002 NT7 will hit the Earth 17 years, when life on
Earth will suffer a devastating blow. The asteroid was allegedly
detected so far the biggest threat to the Earth objects, its diameter
about two kilometers, is expected to hit speeds of up to 28 kilometers
per second, regardless of colliding with the Earth in any one place on
five continents, are sufficient to destroy block the entire continent
and cause global climate upheaval. Atlas Atlas entry for more reference
materials 1 asteroid : The asteroid 75百分之百 of all asteroids, and
therefore the largest number of asteroids. C-asteroid's surface carbon,
albedo is very low, only 0.05 or so. Generally believed that the
composition of C-asteroids and carbonaceous chondrite (a stony
meteorite) the composition of the same. General C-asteroids are
distributed in the outer asteroid belt. S-Asteroids: The Asteroids for
17百分之百 of all asteroids is the second most asteroids. S-asteroids
generally distributed in the inner asteroid belt. S-asteroid albedo is
relatively high, from 0.15 to 0.25. Their composition and similar to
ordinary chondrites. Such meteorites are generally composed of
silicide. M-Asteroids: Most of the rest of the asteroids fall into this
category. These asteroids may be relatively large asteroids in the past
the metal core. Their albedo and S-like asteroids. They may be related
to the composition of nickel - iron meteorite similar. E-asteroids:
asteroid's surface mainly by this type of enstatite composition, their
albedo is relatively high, generally above 0.4. They may be related to
the composition of enstatite chondrites (another type of stony
meteorite) is similar. V-asteroids: This very rare asteroid composition
and S-asteroid almost, the only difference is that they contain more
pyroxene. Astronomers suspect that these asteroids Vesta is in the
upper separated silicide. The surface of Vesta has a very large crater,
possibly formed in the course of its V-asteroid was born. Occasionally,
the earth is very rare to find a stony meteorite, HED-non-chondrites,
their composition may be similar with the V-asteroids, they may also
come from Vesta. G-asteroids: they can be seen as a kind of
C-asteroids. Their spectra are very similar, but in the ultraviolet
part of the G-asteroids have different absorption lines. B-asteroids:
they and G-C-asteroids and asteroids are similar, but different UV
spectrum. F-asteroids: asteroid is a C-. Spectrum in the ultraviolet
part of their different absorption lines and the lack of water.
P-Asteroids: These very low albedo asteroids, but mainly in the red
part of its spectrum. They may be caused by the composition of carbon
silicide. They are generally located in the very outer asteroid belt.
D-asteroid: P-type asteroids and the asteroid is similar to a very low
albedo, spectral red. R-asteroids: V-type asteroids and the asteroid is
similar to their spectra that they contain more pyroxene and olivine.
A-asteroids: asteroid with a lot of this type of olivine, which, mainly
in the inner asteroid belt. T-asteroids: the distribution of these
asteroids in the asteroid belt lining. Their spectrum of dark red, but
with the P-and R-asteroids of different asteroids. The past people
thought that the asteroid is a complete single stone block, but the
asteroid's density, lower than the stone, and they are huge craters on
the surface of the ,
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larger asteroids that organization is relatively loose. They are more
like the enormous combined gravity rubble. This loose objects would not
impact the large fragmentation, and can impact energy absorption over.
Complete a single object in a large shock wave will be crushed under
impact. In addition a large asteroid's rotation speed is very slow. If
the rotation speed of their high, they may be centrifugal
disintegration. Today, astronomers generally believe that asteroids
larger than 200 meters is mainly composed of this rubble. And some
smaller fragments of asteroids have become some of the satellite, for
example: it has two satellites 87 asteroids. Probe into the age of
space travel before the asteroid even the largest telescopes in the
only spot the size of a needle, so their shape and topography are still
unknown mystery. The first is to o变态ain close-up asteroid 1971 Mariner
9 photographed Fu Boss and Dai Mosi photo, the two small bodies, though
they are a satellite of Mars, but may have been asteroid captured by
Mars. These images show "cczwqmddn",
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that the majority of the asteroid with irregular shapes like a potato.
Voyager program after the gas giant plans to get more small satellite
images. The first true asteroid close-up to Jupiter by the Galileo
spacecraft flying in 1991, passing the 951 Gaisipula (Gaspra), then 243
in 1993 and his actress Ai satellite set g Pacific (Dactyl). The first
dedicated asteroid probe space program is the rendezvous - Shoemaker
Road, he was on his way to 433 Eros, taken in 1997 show de 253 M
(Mathilde), in orbit around the probe after the completion, in 2001 The
successful landing on the Eros. Once the spacecraft in the other head
to the flight of asteroids briefly visited there 9969 Blair (Braille)
(Deep Space 1 in 1999) and Anne Frank (Annefrank) (Stardust in 2002).
In September 2005, the Japanese spacecraft Hayabusa arrived at 25143
Itokawa in detail the detection, and may bring back some samples back
to Earth. The Hayabusa mission has encountered some difficulties,
including three guide wheels bad, two, makes it hard to maintain the
direction of the sun to collect solar energy. The next asteroid
detection program is the European Space Agency's Rosetta (launched in
2004), expected in 2008 and 2010 Year 2867 艩teins detection and 21
Lutetia. In 2007, the National Aeronautics and Space Administration
launched the Dawn spacecraft will be in 2011 and 2015 around Ceres and
Vesta, and may extend the mission to probe the Pallas. Asteroids have
been proposed as the future use of Earth resources, the mining of raw
materials as a rare field, or open space station construction
materials. Launch from Earth is very cumbersome and expensive
materials, the future may be able to directly from the space located in
the asteroid factory direct manufacturing and mining. Asteroid belt
asteroid orbit about 90百分之百 of known asteroids orbit in the asteroid
belt. Asteroid belt is located in a fairly wide zone between Mars and
Jupiter. Ceres, Pallas and so the first to be found within the asteroid
belt asteroids are asteroids. Mars orbit of the asteroid asteroids
within the orbit of Mars is divided into three general groups:
Amor-type asteroids: asteroids cross the orbit of Mars in this
category, and came near the Earth's orbit. The representative of the
asteroid was discovered in 1898 asteroid 433 asteroid from the Earth
can reach a distance of 0.15 astronomical units. 1900 and 1931 near
Earth asteroid 433 astronomers to use this opportunity to determine the
size of the solar system. 719 asteroids discovered in 1911 and later
disappeared, until 2000 it was rediscovered. Group named the asteroid
1221 Amor asteroids orbit of stars from the Sun in astronomical units
from 1.08 to 2.76, which is fairly typical of this group as a track.
Apollo asteroids: asteroid groups of asteroids that orbit between Mars
and Earth. Some of the group orbital eccentricity of the asteroid is
very high, they have reached perihelion inside the orbit of Venus.
Typical of this group of asteroids orbit asteroids are discovered in
1932, Apollo 1862, its orbit in between 0.65 to 2.29 astronomical
units. Asteroid 69230 is only 1.5 lunar distances in the fly a little
earth. Aten asteroids: asteroid's orbit in this group generally less
than in Earth orbit. Star named asteroid discovered in 1976, 2062
Arden. Some of this group,
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is relatively high eccentricity of the asteroid, they may be from Earth
orbit to cross the Earth orbit. These asteroids are collectively
referred to as the near-Earth asteroids. In recent years, studies of
these asteroids are better because they at least theoretically possible
to collide with Earth. Compared results of the project are the Lincoln
Near-Earth Asteroid Research Program (LINEAR), Near-Earth Asteroid
Tracking (NEAT) and the Lowell Observatory Near-Earth Object Search
program (LONEOS) and so on. In the other planets orbit the asteroids in
the Lagrangian points of the other planets orbit the asteroid is called
on to run the Trojan asteroids. First to be found in the Jupiter Trojan
asteroids orbit asteroids, some of them before in Jupiter, some run
after Jupiter. Jupiter's Trojan asteroids representative and asteroids
are asteroids 588 1172.1990 on a Mars Trojan asteroid 5261 asteroid was
discovered, then there are other four Martian Trojan asteroids have
been discovered. Asteroid between Saturn and Uranus, Saturn and Uranus
is among a group of asteroids known as the Centaur asteroids asteroids,
and their eccentricities are quite large. Centaur first asteroid
discovered asteroid 2060 asteroid group. Estimated that these asteroids
in the Kuiper belt from the gravitational interference by other planets
fall into an unstable orbit. Kuiper Belt asteroid belt: full name Yiji
Worth - Kuiper Belt (English: Edgeworth-Kuiper belt; EKB, generally
referred to as the Kuiper Belt, Kuiper Belt or translation, Cooper
band, etc.) yellow dot ring as the Kuiper Belt ( Kuiper Belt) TNOs and
similar objects: Centaurs TNOs Kuiper asteroid belt object class
offerings in the object class QB1 2:1 resonant objects Scattered disc
objects Oort cloud beyond Neptune Oort Kuiper belt asteroids are, where
astronomers found that the largest asteroids, such as asteroids 50000
and so on. Asteroids within the orbit of Mercury (water within the
asteroid) Although there has been some speculation within the orbit of
Mercury also has an asteroid group, but so far not confirmed this
speculation. [Line into] some distance from the near-Earth asteroids
close to Earth, they had some small meteorites but after suck the Earth
is gravity, which is near-Earth asteroids. Collision asteroid collision
that said that: about 65 million years ago, about a kilometer in
diameter asteroid collision with Earth, a violent collision rolled up a
lot of dust, so that the earth's atmosphere is filled with dust and
gathered into a dust cloud, a thick cloud of dust enveloped the entire
planet over, blocking the sun, the earth a The lack of sunlight, the
survival
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of plant photosynthesis have been destroyed, a large number of plants
have withered and died, a large herbivorous dinosaur body consume each
day a few h,
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undred kilograms of dry plants, they simply can not adapt to this
flare-up causes variation of the living environment, and only in the
starvation and hopelessness to fall; to herbivorous dinosaur meat for
food sources asteroid quality even smaller than the moon. Astronomers
believe that today the formation of asteroids in the solar system there
is no residue to form planets. Jupiter in the solar system formed when
the quality of the fastest growing, it prevents the asteroid belt
region today the formation of another planet. Asteroid belt region of
the asteroid orbit by Jupiter's interference, they continue to impact
and crushing. Other substances were driven out of their orbits collided
with other planets. Large asteroid in the formation of radioactive
isotopes of aluminum after the 26Al (radioactive isotope of iron and
possible 60Fe) the decay of hot. Heavy elements such as nickel and iron
in this case sank to the asteroid's interior, light elements such as
silicon is floating. As a result of the asteroid on the separation of
the internal material. In the subsequent collision and produced by the
breakdown of the new composition of the asteroid and therefore
different. Some of these pieces was a meteorite landed on Earth.
Structure of the data o变态ained by spectral analysis of the asteroid's
surface composition can prove very different. The characteristics of
their spectral types of asteroids are divided: C-asteroid planet with
15000 CCD 17000 Medvedev (exception) 21000 20000 Varuna encyclopedia
boast aure 25000 56000 50000 astrometry Mesopotamia 71000 Hughdowns
(exception) because permanent number has more than 100,000, some of the
original program to cope with five numbers can not support, so there
are some letters in ten thousand with the number of representation,
that is, A = 10, B = 11 ... ... Z = 35; a = 36 ... ... z = 61, in this
arrangement, the 619,999 the following number of asteroids that can
still be used 5. Well-known part of the asteroid with the Chinese on
Chinese soil on the first one discovered asteroid: 139 Jiuhua stars
(Juewa) (discoverer JC Watson) its first asteroid discovered by the
Chinese people: 1125/3789 Chinese (China) (discoverer Zhang Yu Zhe,
after the 1125 changes to 3789) the first one in China, named after the
asteroid: 1802 Zhang Heng (Zhang Heng) (Purple Mountain Observatory,
discoverer) its first asteroid named after Chinese: Beijing 2045 (
Peking) (Purple Mountain Observatory, discoverer) first named a county
of China's asteroid: 3611 Tai Po (Dabu) (Purple Mountain Observatory,
discoverer) to its first asteroid named after the people of Taiwan:
2240 Cai (Tsai ) (Tsai, Xian) (discoverer of the Harvard Observatory)
spacecraft, the first one to name the asteroid China: 8256 Shenzhou
(Shenzhou) (Purple Mountain Observatory, discoverer) of Hong Kong
secondary school students in recognition of the invention Chan
Yik-hei's achievements in the name of the asteroid: 20780 Chan Yik-hei
stars (Chanyikhei) (discoverer LINEAR team), named to commemorate the
Beijing Olympic Games: the 2008 Beijing Olympic star formation, the
beginning of the asteroid Ida is an asteroid that astronomers in the
planet between Mars and Jupiter from rupture , but all the asteroids in
the asteroid belt's total mass asteroid asteroids are at the
traditional God of the Roman or Greek to name, such as Pallas, Vesta,
Astraea and so on. However, as more and more asteroids were found, the
last classical names of God used up. So was the wife of the discoverer
of asteroids with the names of historical figures or other important
people, cities, fairy tale characters and the name of God or other
mythology named. Such as asteroids Clio 216 is based on the Egyptian
queen named Petra, asteroid 719 Albert was named by Albert Einstein,
asteroid 17744 was named by actress Jodie Foster's , asteroid 1773 is
based on the Brothers Grimm a dwarf named, and so on. As of March 6,
2007, has calculated the orbit (that is, by the temporary number) a
total of 679,373 pieces of asteroids (query), number of asteroids have
been a total of 150,106 permanent teeth (query), the asteroid has been
named a total of 12,712 pieces. For some number is a multiple of 1000
asteroids, it is customary to particularly important people, things to
name. (But occasional exceptions) such as: number is a multiple of 1000
asteroids have been named Herschel 3000 1000 Pia Qi Da Vinci 4000 2000
5000 Hipparch,
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us 7000 United Nations, the International Astronomical Union Curie 8000
6000 Newton 9000 HAL ( exceptions) 10000 Myriostos (exceptions)
asteroid asteroid after the formation of the aluminum in the
radioisotope 26Al (radioactive isotope of iron and possible 60Fe) of
the decay and heat up. Heavy elements such as nickel and iron in this
case sank to the asteroid's interior, light elements such as silicon is
floating. As a result of the asteroid on the separation of the internal
material. In the subsequent collision and produced by the breakdown of
the new composition of the ,
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asteroid and therefore different. Some of these pieces was a meteorite
landed on Earth. Overview of C-type asteroid named 253 Mathilde
asteroid's name consists of two parts: the front part of a permanent
number, a name is part of the back. Each tablet was first confirmed
asteroid will be a permanent number, discoverer of the asteroid can
suggest a name. The name to be approved by the International
Astronomical Union was formally adopted, because the naming of
asteroids have a certain routine. Therefore, some asteroids have no
names, particularly in the permanent number in the tens of thousands of
asteroids. If the asteroid's orbit can be determined accurately enough,
then even if it is confirmed that. Prior to this, it will have a
temporary number, it is found that by the year and two letters, such as
the 2004 DW. Pia Qi is the first asteroid was discovered in 1801 in
Sicily, he gave the stars named Ceres Ferdinand stars. The first part
is the patron saint of Sicily, named Ceres, is the latter part of King
Ferdinand IV of Naples named. However, this international scholars are
not satisfied, so the second part removed. So the first official name
of an asteroid is an asteroid 1 Ceres. Since then discovered the
asteroid Ida It is. October 1991, Galileo Jupiter probe visited the
asteroid 951 Gaspra, the first high-resolution shot of the asteroid
photos. August 1993, Galileo flew another asteroid 243 Ida, making it
the second pieces of asteroids visited by spacecraft. Asteroids Gaspra
and Ida are rich in metals, are S-type asteroids. June 27, 1997, NEAR
asteroid 253 Mathilde pass detector. This rare opportunity allows
scientists to closely observe the first Fengyun C-type asteroids are
rich in carbon. NEAR detector because its not a special inspection that
the visit be carried out so far its only visit. NEAR is used in the
January 1999 inspection of the asteroid Eros. Ground observation of
many asteroid astronomers have made the ground observation. Some
well-known asteroids have Toutais, Castalia, Vesta, and Geographos and
so on. For the asteroid Toutatis, Castalia, and Geographos, astronomers
in their proximity to the sun, on the ground through the observation of
their radio. Vesta asteroid was discovered by the Hubble Space
Telescope. From the beginning of the astronomers that the asteroid is a
planet between Mars and Jupiter from broken, but all the asteroids in
the asteroid belt's total mass much smaller than the quality of the
moon. Astronomers believe that today the formation of asteroids in the
solar system there is no residue to form planets. Jupiter in the solar
system formed when the quality of the fastest growing, it prevents the
asteroid belt region today the formation of another planet. Asteroid
belt region of the asteroid orbit by Jupiter's interference, they
continue to impact and crushing. Other substances were driven out of
their orbits collided with other planets. Large asteroid line, it is
easy to be determined. Moreover, with the film's sensitivity to enhance
their soon to be sensitive than the human eye, even darker asteroids
can be found. The introduction of photography made was found a huge
increase in the number of asteroids. 1990 charge-coupled device
photography technology has been introduced, together with computer
analysis of electronic photography technology have improved the
asteroid makes more in a very short period of time was found. Today,
the number of known asteroid about 22 million. The orbit of an asteroid
has been identified, astronomers can brightness and albedo of its
analysis to estimate its size. In order to analyze the albedo of an
asteroid astronomers generally use both visible light is also used
infrared measurements. However, this method is less reliable, because
each asteroid's surface structure and composition may differ, so the
albedo of the errors are often relatively large. More accurate data can
be used to o变态ain radar. Astronomers use radio telescopes as a
generator of high power radio waves to the strong projection of the
asteroid. By measuring the reflected wave reaches the speed of
asteroid's distance can be calculated. On other data (diffraction data)
of the asteroid can be deduced from the shape and size. In addition,
the observed asteroid occultation can be more precise to calculate the
asteroid's size. Non-manned spacecraft studies of asteroids now have a
series of non-manned spacecraft around the asteroid in a number of them
have studied: in 1991 Galileo Jupiter in its distance on the fly flying
to the asteroid 951 , 1993, asteroid 243 fly. NEAR asteroid No. 253
flew in 1997 and in 2001 landed at the asteroid 433. 1999, Deep Space 1
asteroid flyby in 9969, 26 km away. In 2002, Stardust flew by asteroid
5535 3300 km distance. Because asteroids are left over from the early
solar system material, scientists are very interested in their
composition. After space probe found the asteroid belt, asteroid belt
is actually very spacious, the distance between the asteroid and the
asteroid is very far away. Prior to 1991, it is through ground-based
observations to o变态ain the number of asteroids asteroid
邮件群发 In January 1801 the first
day, Giuseppe Piazzi discovered an object, at first he thinks it will
not again be a comet. But when it was determined orbit, they found it
was not a comet, but rather is a small planet. Piazzi called Ceres
(Ceres, goddess of grain and farming is grain beauty of Sicily), also
known as Ceres. The other three small bodies also were found in
successive years (they are Pallas, Vesta, and Juno). The nineteenth
century have been discovered a few hundred. Has been found more than
7,000 asteroids, and now this figure is still an annual growth rate of
a few hundred. No dou变态, there must be hundreds of asteroids as too
small to observe on Earth. For now known, there are 26 asteroids of
diameter greater than 200 km. Of these visible observations of
asteroids have been basically completed, to our knowledge, about 99百分之百
of the asteroid's diameter is less than 100 kilometers. For those 10 to
100 km in diameter asteroid between the catalog has been completed in
half. But we know there are some smaller, perhaps there are nearly one
million of around 1 km in diameter asteroid. The quality of all the
asteroids and the quality of the moon is smaller than [1]. Early
speculation that the study of history in 1760 there was speculation
within the solar system planets distance from the sun to form a simple
number series. By the series between Mars and Jupiter there is a gap
between these two planets should have a planet. The late 18th century,
many people started looking for Fengyun undiscovered planets.
Well-known Titius - Bode is set is one example. European astronomers at
the world's first international organization of research projects,
under the leadership of the Observatory in Gotha day is divided into 24
districts, the European astronomers who systematically search the area
in the 24 Fengyun known as the But this project without any result,
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s. Pia Qi findings January 1, 1801 the evening, Zhu Se Pupi Aceh
Palermo Observatory in Sicily were found in the inner Taurus in the
chart can not find a star. Pia Qi I did not participate in looking for
He will report his findings to the Gotha Observatory, but at first he
said he found a comet. This Houpi Ya Qi sick, unable to continue his
observations. And report his findings to the use of a very long time Da
Geda, this time the star has been direction to the sun, can not be
found. At this point the research Gauss Gauss invented a method of
calculating orbits of planets and comets method, this method requires
only a few points we can calculate the position of a celestial body's
orbit. Pia homogeneous Gaussian read after the discovery of the
location of the object calculated Fengyun sent Gotha. Olbers on the
evening of 31 December 1801 re-discovered the star. Later it acquired
the name Ceres. 1802, Olbers discovered another one objects, he named
it Pallas. 1803 Juno, Vesta was discovered in 1807. Until 1845, the
fifth asteroid Astraea was discovered, but since then many asteroids
were soon discovered. 1890 so far have been about 300 known asteroids
out. Photography into astronomy photography into astronomy in 1890 for
the development of astronomy given a huge boost. Prior to discover an
asteroid astronomers have suspected for a long time record of each
star's position stars, compare them with the changes between the
location of the surrounding stars. However, photographic film, on an
asteroid relative to the movement of stars on the film pulled out a
asteroid found Ceres close to the sun, on the ground by radio
observations of them. Vesta asteroid was discovered by the Hubble Space
Telescope. The discovery of asteroids with the Titius - Bode set is
closely linked to the proposal, according to the set is, at a distance
of 2.8 astronomical units from the sun should be a planet at the 1801
New Year's Day Piya Qi is really found in the area the first asteroid
Ceres. In the following years with a similar orbit Ceres Pallas, Juno,
Vesta have been found. The introduction of astronomical photography and
flash, as the comparator, it allows the discovery of the asteroid's
rate rose significantly, to 1940, with a permanent number of asteroids
have been 1564. Among them, the German astronomer Encke and longer than
the orbital calculations by Hansen, Wolf and Laiyinmute the observation
that there are many contributions to the discovery of particularly
great. Asteroid naming rights belong to the discoverer. Early like to
use the name of the goddess, and later switched names, nickname and
even the organization name of the acronym to name. Some asteroids and
the asteroid is very famous, such as off Loyang group, Apollo Group,
Icarus, Eros, Hedo Hidalgo and so on. By Orbital for statistical
analysis, at about 5 degrees inclination and eccentricity of about 0.17
the largest number of asteroids. Kirkwood gap is based on the average
heliocentric distance of the asteroid by the best-known statistical
distribution. N and the average number of red asteroid magnitude m at
the statistical relationship between the logN = 0.39m-3.3, an asteroid
with diameter d between the absolute magnitude of g satisfy the
statistical formulas logd (km) = 3.7-0.2g. The distribution of the
number of asteroids with diameters of about 30 km in diameter near the
discontinuity. Ceres Number of asteroids may be about 50 million. The
largest asteroid is only about 1,000 km in diameter, miniature asteroid
the size of pebbles only. Diameter of more than 240 km asteroid about
16. They are located inside Earth's orbit to the orbit of Saturn, the
outer space. The vast majority of asteroids are concentrated in the
orbits of Mars and the asteroid belt between Jupiter. Some of the
asteroid's orbit and the Earth's orbit intersect, there have been some
of the asteroid collision with Earth occurred. Asteroids are remnants
of the material after the formation of the solar system. There is a
speculation that they may be the remains of a mysterious planet, the
planet in ancient times suffered a huge cosmic collision destroyed.
However, the characteristics of these asteroids of view, they do not
like once assembled together. If all the asteroids put together to form
a single object, then it's less than 1500 km in diameter - smaller than
the radius of the moon. Since the early solar system, asteroids are
material, the scientists are very interested in their ingredients.
After a space probe found the asteroid belt, asteroid belt is actually
very open, asteroids and the asteroid separated very far between. In
1991, the asteroid before the data o变态ained only through ground-based
observations. October 1991, Galileo Jupiter probe visited the asteroid
951 Gaspra, which won the first high-resolution photographs of
asteroids. August 1993, Galileo flew by the asteroid 243 Ida, making it
the second pieces of asteroids visited by spacecraft. Asteroids Gaspra
and Ida are rich in metals, are S-type asteroids. We know many of
asteroids falling to Earth's surface through the analysis of space
rubble. The asteroid that collided with the Earth as meteorites. When
high-speed meteoroid broke into our atmosphere, its surface due to
friction with the air temperature and evaporation, and glared, this is
the meteor. If the meteoroid is not completely burned and fell to the
ground, then known as meteorites. After analysis of all the meteorites,
of which 92.8百分之百 of the composition is silicon dioxide (rock), 5.7百分之百
iron and nickel, the remainder is a mixture of these three substances.
Stone meteorites with known large meteorite, a large quantity of iron
meteorites called siderite. Because meteorites and Earth rocks are very
similar, so difficult to identify. June 27, 1997, NEAR asteroid 253
Mathilde pass detector. This opportunity allows scientists to closely
observe the Fengyun first carbon-rich C-type asteroids. Visit the NEAR
detector is not designed to study them and become the only one visit.
NEAR is used in the January 1999 inspection of the asteroid Eros.
Astronomers have already made a lot of ground observation of the
asteroid. Some well-known asteroids have Toutais, Castalia, Vesta, and
Geographos and so on. For the asteroid Toutatis, Castalia, and
Geographos, astronomers in their asteroids Gaspra and Galileo
spacecraft 002 years of glory found in Norbert Ore (Quaoar) diameter is
1280 kilometers, discovered 2004 DW 2004, even up to 1800 kilometers in
diameter. Discovered Sedna in 2003 (asteroid 90377) is located outside
the Kuiper Belt, its diameter is about 1,500 km. According to
estimates, the number of asteroids may be about 50 million. The largest
asteroid is only about 1,000 km in diameter, miniature asteroid the
size of pebbles only. The largest asteroid now reclassified to be
defined as a dwarf planet. Diameter of more than 240 km asteroid about
16. They are located inside Earth's orbit to the orbit of Saturn, the
outer space. The vast majority o,
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f asteroids are concentrated in the orbits of Mars and the asteroid
belt between Jupiter. Some of the asteroid's orbit and the Earth's
orbit intersect, there have been some of the asteroid collision with
Earth occurred. Asteroids are remnants of the material after the
formation of the solar system. There is a speculation that they may be
the remains of a
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mysterious planet, the planet in ancient times suffered a huge cosmic
collision destroyed. However, the characteristics of these asteroids of
view, they do not like once assembled together. If all the asteroids
put together to form a single object, then it's less than 1500 km in
diameter - smaller than the radius of the moon. So far in the solar
system have found a total of about 700,000 asteroids, it could be all
the asteroids is only a small part, only a few of these asteroids
larger than 100 kilometers. Until the 1990s was the largest asteroid
Ceres, but in recent ye,
Tiffany Necklaces,
ars found some of the Kuiper belt asteroid Ceres, the diameter is
larger than, for example discovered in 2000 Varuna (Varuna) 900 km in
diameter, 2002 Norbert Ore found in Quarry (Quaoar) diameter is 1280
kilometers, discovered 2004 DW 2004, even up to 1800 kilometers in
diameter. Discovered Sedna in 2003 (asteroid 90377) is located outside
the Kuiper Belt, its diameter is about 1,500 km. According to
estimates, asteroid Toutatis Introduction to the History of early
speculation that the discovery of homogeneous Gaussian Pia research
into astronomy, photography unmanned spacecraft on the asteroid named
an overview of sources of ground observation number 1000 multiples of
some asteroids have been named with the Chinese on the formation of
structures known asteroids orbit the asteroid belt asteroid probe
orbits Mars on other planets within the asteroid orbit asteroid
collision asteroid that hit Earth Introduction chance asteroid, minor
planet or planetoid in the solar system planets around the sun like
sports, but the volume and quality of much smaller objects than
planets. So far in the solar system have found a total of about 700,000
asteroids, it could be all the asteroids is only a small part, only a
few of these asteroids larger than 100 kilometers. Until the 1990s was
the largest asteroid Ceres, but in recent years found some of the
Kuiper belt asteroid Ceres, the diameter is larger than, for example
discovered in 2000 Varuna (Varuna) 900 km in diameter, 2 < p>
Asteroid directory 锘?p> asteroid (asteroid) is similar to the solar
system planets around the Sun campaign, but much smaller volume and
mass ratio of planetary objects. Most asteroids in our solar system
orbit between Mars and Jupiter called the asteroid belt. Also outside
the orbit of Neptune is also the distribution of asteroids, this area
called the Kuiper belt (Kuiper Belt).
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