Characteristics and information of the moon

The Moon The Moon is commonly known as the Moon or the Lunar Moon. The moon is also about 4.6 billion years old. It is closely related to the earth. The moon also has a layered structure such as crust, mantle, and core. The average thickness of the outermost lunar crust is about 60-65 kilometers. Below the lunar crust to a depth of 1,000 kilometers is the lunar mantle, which accounts for most of the moon's volume. Below the lunar mantle is the lunar core. The temperature of the lunar core is about 1,000 degrees, and it is likely to be in a molten state. The diameter of the moon is about 3476 kilometers, which is 3/11 of the earth. The volume is only 1/49 of the Earth, and the mass is about 735 billion tons, which is equivalent to 1/81 of the Earth's mass. The gravity of the moon is almost equivalent to 1/6 of the Earth's gravity. There are dark parts and bright areas on the moon. When early astronomers observed the moon, they thought that the dark areas were covered with sea water, so they called them "sea". The famous ones include the Sea of ​​Clouds, the Sea of ​​Shit, the Sea of ​​Tranquility, etc. The bright part is the mountains, where there are many mountains, criss-crossing mountains, and dotted craters everywhere. Bailey Crater, located near the South Pole, has a diameter of 295 kilometers and can fit the entire Hainan Island into it. The deepest mountain is Newton Crater, which is 8,788 meters deep. In addition to craters, there are also ordinary mountains on the moon. High mountains and deep valleys appear one after another, creating a unique scenery. The front side of the moon always faces the Earth. On the other hand, most of the far side of the moon cannot be seen from the Earth, except for an area near the edge of the moon that is occasionally visible due to the movement of the scales. In the era before detectors, the far side of the moon has always been an unknown world. One of the unique features of the far side of the Moon is that it has almost no darker lunar surface features such as maria. When the probe moves to the far side of the moon, it will not be able to communicate directly with the earth. Orbital data: Average orbit radius: 384,400 kilometers; Orbital eccentricity: 0.0549; Perigee distance: 363,300 kilometers; Apogee distance: 405,500 kilometers; Average orbital period: 27 days, 7 hours, 43 minutes, 11.559 seconds; Average orbital speed: 1.023 kilometers/second; Orbital inclination: between 28.58° and 18.28° Interchange (the angle with the ecliptic plane is 5.145°) Ascending node right ascension 125.08° Perigee argument 318.15° Physical characteristics Equator diameter 3,476.2 kilometers Pole diameter 3,472.0 kilometers Oblateness 0.0012 Surface area 3.976×107 square kilometers Oblateness 0.0012 Volume 2.199 × 1010 cubic kilometers Mass 7.349 × 1022 kg Average density of water 3.350 times Equator gravity acceleration 1.62 m/s2 1/6 of Earth Escape velocity 2.38 km/s Rotation period 27 days, 7 hours, 43 minutes, 11.559 seconds (synchronous rotation) Rotation speed 16.655 m/s (at the equator) Rotation axis inclination angle varies between 3.60° and 6.69° (the angle with the ecliptic is 1.5424°) Albedo 0.12 Apparent magnitude at full moon -12.74 Surface temperature (t) -233~123 ℃ (average -23℃) Atmospheric pressure 1.3×10-10 kPa The moon orbits the earth once in about one lunar month, and moves half a degree relative to the background starry sky every hour, which is similar to the apparent diameter of the moon. Unlike other satellites, the Moon's orbital plane is closer to the ecliptic plane than to the Earth's equatorial plane. Relative to the background starry sky, the time it takes for the Moon to orbit the Earth (moon revolution) once is called a sidereal month; and the time it takes for a new moon to the next new moon (or between two identical moon phases) is called a synodic month. The synodic moon is longer than the sidereal moon because the earth itself advances a certain distance in its orbit around the sun during the movement of the moon. Because the moon's rotation period is exactly the same as its revolution period, we can only see the same side of the moon always facing the earth. Since the early formation of the Moon, the Moon has been affected by a torque that causes its rotation to slow down. This process is called tidal locking. Therefore, part of the angular momentum of the Earth's rotation is converted into the angular momentum of the Moon's revolution around the Earth. As a result, the Moon moves away from the Earth at a speed of about 38 mm per year. At the same time, the Earth's rotation is getting slower and slower, and the length of the day is getting longer by 15 microseconds every year.

The gravitational pull exerted by the moon on the earth is one of the causes of tides. The Moon's orbit around the Earth is a synchronous orbit, and the so-called synchronous rotation is not strictly enforced. Since the moon's orbit is elliptical, when the moon is at perihelion, its rotation speed cannot catch up with its revolution speed. Therefore, we can see the area in the eastern part of the moon reaching 98 degrees east longitude. On the contrary, when the moon is at aphelion, its rotation speed is faster than its revolution speed. The speed is fast, so we can see the area in the western part of the moon up to 98 degrees west longitude. This phenomenon is called Libra movement. And because the moon's orbit is tilted toward the Earth's equator, when the moon moves in the starry sky, its polar regions will wobble by about 7 degrees. This phenomenon is called libra movement. Furthermore, since the moon is only 60 earth radii away from the earth, if an observer observes from moonrise to moonset, the observation point will have a displacement of one earth diameter, and the area on the moon's surface with a longitude of 1 degree can be seen. This phenomenon is called Libra movement. Strictly speaking, the earth and the moon revolve around the center of homogeneity, which is 4,700 kilometers away from the center of the earth (that is, 2/3 of the radius of the earth). Since the center of gravity is below the surface of the earth, the movement of the earth around the center of mass seems to be "rocking". Viewed from above the Earth's North Pole, both the Earth and the Moon rotate in a clockwise direction; the Moon also orbits the Earth in a clockwise direction; and even the Earth orbits the Sun in a clockwise direction. Many people don't understand why the values ​​of the Moon's orbital inclination and the Moon's rotational axis have changed so much. In fact, the orbital inclination is relative to the central celestial body (i.e. the Earth), while the rotation axis inclination is relative to the orbital plane of the satellite (i.e. the Moon) itself. While this definition is customary for general cases (such as the orbits of artificial satellites) and is fairly fixed in value, this is not the case for the Moon. The moon's orbital plane (the ecliptic plane) maintains an angle of 5.145 396° with the ecliptic plane (the earth's orbital plane), while the moon's rotation axis forms an angle of 1.5424° with the normal to the ecliptic plane. Because the Earth is not a perfect sphere, but rather bulges at the equator, the ecliptic plane is constantly precessing (that is, the intersection with the ecliptic rotates clockwise), completing one cycle every 6793.5 days (18.5966 years). During this period, the angle between the ecliptic plane and the equatorial plane of the Earth (the Earth's equatorial plane is tilted at 23.45° to the ecliptic plane) will change from 28.60° (i.e. 23.45° + 5.15°) to 18.30° (i.e. 23.45°- 5.15°). Similarly, the angle between the moon's axis of rotation and the ecliptic plane will also be between 6.69° (i.e. 5.15° + 1.54°) and 3.60° (i.e. 5.15° - 1.54°). These changes in the moon's orbit will in turn affect the inclination of the earth's rotation axis, causing it to wobble by ±0.002 56°, which is called nutation. The two intersections of the ecliptic plane and the ecliptic plane are called lunar nodes - the ascending node (north point) refers to the point where the moon passes to the north of the ecliptic plane; the descending node (south point) refers to the point where the moon passes to the south of the ecliptic. When the new moon happens to be on the lunar nodes, a solar eclipse will occur; and when the full moon happens to be on the lunar nodes, a lunar eclipse will occur; the moon's period name Value (d) defines the sidereal month 27.321 661 Synodic month relative to the background stars 29.530 588 Relative to the Sun (moon phase) Equinox month 27.321 582 Relative to the vernal equinox periapsis month 27.554 550 Relative to the perigee nodal month 27.212 220 Other characteristics of the lunar orbit relative to the ascending node Name Value (d) Definition Metonic Chapter (repeat phase) /day) 19-year average moon-to-earth distance ~384 400 kilometers Perigee distance ~364 397 kilometers Apogee distance ~406 731 kilometers Average orbital eccentricity 0.0549003 Node retrograde period 18.61 years Perigee motion period 8.85 eclipse years 346.6 Tiansara period (repeat eclipses) The average inclination angle between the moon's equator and the ecliptic is 5°9' in 10/11 days of 2018. The average inclination angle between the moon's equator and the ecliptic is 1°32'. The first man-made object to reach the moon in human lunar exploration was the unmanned landing of the former Soviet Union Luna 2, which crashed into the moon on September 14, 1959.

Luna 3 took photos of the far side of the moon on October 7 of the same year. Luna 9 was the first lander to soft-land on the moon. It sent back photos taken on the lunar surface on February 3, 1966. In addition, Luna 10 successfully entered orbit on March 31, 1966, becoming the first man-made satellite on the moon. During the Cold War, the United States of America and the former Soviet Union always wanted to lead each other in space technology. This space race reached its climax when the first man landed on the moon on July 20, 1969. Neil Armstrong, commander of Apollo 11 of the United States of America, was the first man to set foot on the moon, while Eugene Cernan was the last man to stand on the moon during the Apollo 17 mission in December 1972. members. See: List of Lunar Astronauts The Apollo 11 astronauts left a 9-inch by 7-inch stainless steel plaque on the lunar surface to commemorate the landing and provide information for other creatures who might discover it. Six Helios missions and three unmanned Lunar missions (Lunar 16, 20, and 24) brought rock and soil samples from the moon back to Earth. In February 2004, President George W. Bush of the United States of America proposed sending people to the moon again by 2020. The European Space Agency and the People's Republic of China also have plans to launch probes to the moon. Europe's Smart 1 probe was launched on September 27, 2003, and entered orbit around the moon on November 15, 2004. It will survey the lunar environment and produce X-ray maps of the lunar surface. The People's Republic of China is also actively carrying out lunar exploration programs and seeking the feasibility of mining lunar resources, especially the helium isotope helium-3, an element that is expected to become the earth's energy source in the future. For information about the People's Liberation Army and the country's lunar exploration program, see the Chang'e Project entry. Japan and India are also unwilling to follow suit. Japan has initially set out its future lunar exploration missions. Japan's Aerospace Exploration Agency has even begun planning a manned lunar base. India will first launch the unmanned moon orbiter Chandrayan. Myths about the Moon In the ancient mythology of the Republic of China, there are countless stories about the moon. In ancient Greek mythology, the name of the moon goddess is Artemis. She is the twin sister of the sun god Apollo and she is also the goddess of hunting. The astronomical symbol of the moon is like a crescent moon, symbolizing the bow of Artemis. The moon is the earth's only natural satellite and the closest celestial body to us. Its average distance from the earth is about 384,401 kilometers. Its average diameter is about 3476 kilometers, which is slightly larger than 1/4 of the Earth's diameter. The surface area of ​​the moon is 38 million kilometers, which is not as large as the area of ​​Asia. The mass of the moon is about 735 billion tons, which is equivalent to 1/81 of the mass of the earth. The gravity of the moon is almost equivalent to 1/6 of the earth's gravity. Orbital Movement of the Moon The Moon moves around the Earth in an elliptical orbit. The great circle intercepted by this orbital plane on the celestial sphere is called the "white path". The ecliptic plane does not coincide with the celestial equator, nor is it parallel to the ecliptic plane, and its spatial position is constantly changing. Period 173 days. The rotation of the moon The moon rotates while revolving around the earth, with a period of 27.32166 days, which is exactly one sidereal month, so we cannot see the back side of the moon. We call this phenomenon "synchronous rotation", and it is almost a universal law in the satellite world. It is generally believed to be the result of the long-term tidal effect of the planet on the satellite. Libra motion is a wonderful phenomenon that allows us to see 59% of the moon. The main reasons are as follows: 1. In different parts of the elliptical orbit, the rotation speed does not match the revolution angular speed. 2. The angle between the white equator and the equator. Physical Conditions of the Moon The main topography of the moon are: Craters. This name was given by Galileo. It is a prominent feature of the lunar surface, covering almost the entire lunar surface. The largest crater is Bailey Crater near Antarctica, with a diameter of 295 kilometers, which is slightly larger than Hainan Island. A small ringed mountain may even be a crater of tens of centimeters. There are approximately 33,000 with a diameter of not less than 1,000 meters. It accounts for 7-10% of the moon's surface area.

A Japanese scholar proposed a crater classification in 1969, which was divided into Clavian type (old craters, which are generally unrecognizable, and some still have mountains within mountains), and Copernican type (young craters, which often have "radiation patterns" and inner walls Generally with concentric circular mounds, usually with a central peak in the center) Archimedes-shaped (lower ring walls, may have evolved from the Copernican type) bowl-shaped and dimple-shaped (small craters, some with a diameter less than one meter). The dark part of the moon visible to the naked eye is actually a vast plain on the moon. Due to historical reasons, this unworthy name has remained until now. There are 22 lunar maria that have been identified, and there are also some landforms called "lunar maria" or "lunar maria". Most of the 22 recognized ones are distributed on the near side of the moon. There are 3 on the back and 4 on the edge area. The area of ​​the maria on the front side is slightly more than 50%, and the largest "Ocean Procellarum" covers an area of ​​more than 5 million square kilometers, which is almost the total area of ​​nine France. Most lunar maria are roughly circular or oval in shape, and are mostly enclosed by mountains, but there are also some seas that are connected into one piece. In addition to the "sea", there are five "lakes" with similar topography - Meng Lake, Dead Lake, Summer Lake, Autumn Lake, and Spring Lake. However, some lakes are larger than the sea, such as the area of ​​Meng Lake. 70,000 square kilometers, much larger than Qihai and others. The parts of the lunar sea that extend to the land are called "bays" and "marshes", both of which are distributed on the front. There are five bays: Dew Bay, Summer Bay, Central Bay, Rainbow Bay, and Meiyue Bay; there are three marshes: Rotting Marsh, Plague Marsh, and Meng Marsh. In fact, there is no difference between marshes and bays. The terrain of the lunar maria is generally low, similar to basins on the earth. The lunar maria is 1-2 kilometers lower than the lunar mean level. Some of the lowest seas, such as the southeastern part of the Imbrium, are even 6,000 meters lower than the surrounding area. The moon's albedo (a physical measure of its ability to reflect sunlight) is also relatively low, so it appears darker. Lunar Land and Mountains The area on the lunar surface that is higher than the lunar sea is called the lunar land. It is generally 2-3 kilometers higher than the level of the lunar sea. Because of its high albedo, it looks brighter. On the far side of the moon, the land area is roughly equal to the maria, but on the far side, the land area is much larger than the maria. It is known from isotope measurements that the lunar continent is much older than the lunar maria and is the oldest topographic feature on the moon. On the moon, in addition to the numerous jagged craters, there are also some mountains similar to those on the earth. Mountains on the moon often borrow the names of mountains on the earth, such as the Alps, Caucasus Mountains, etc. The longest mountain range is the Apennine Mountains, which stretches for 1,000 kilometers, but its height is only three or four kilometers higher than the level of the lunar sea. There are also some steep peaks on the mountain range, and their heights were estimated to be too high in the past. It is now believed that the height of most mountain peaks is similar to that of the Earth's peaks, and the highest peaks (also near the moon's south pole) are only 9,000 meters and 8,000 meters high. There are 6 peaks on the moon above 6,000 meters, 20 between 5,000 and 6,000 meters, 80 between 4,000 and 5,000 meters, and 200 above 1,000 meters. Mountains on the moon have a common feature: the slopes on both sides are very asymmetrical. The seaward side has a very steep slope, sometimes in the shape of a cliff, while the other side is quite gentle. In addition to mountains and mountain groups, there are four cliffs hundreds of kilometers long on the moon. Three of them protrude into the moon sea. This kind of cliff is also called "moon chasm". Radiation Patterns on the Moon Another main feature on the moon is that some "younger" craters often have beautiful "radiation patterns", which are bright bands that extend in all directions with the craters as radiating points. A straight direction passes through mountain systems, maria and craters. Radiation patterns vary in length and brightness. The most eye-catching is the radiation pattern in Tycho crater. The longest one is 1,800 kilometers long and is particularly spectacular during the full moon. Secondly, the two craters Copernicus and Kepler also have quite beautiful radiation patterns. According to statistics, there are 50 craters with radiating patterns. The reason for the formation of radial patterns has not yet been determined. In essence, it is closely related to the theory of crater formation. Nowadays, many people are inclined to the theory of meteorite impact, believing that on the moon, which has no atmosphere and little gravity, meteorite impact may cause high-temperature fragments to fly very far. Some other scientists believe that the role of volcanoes cannot be ruled out, and the jets from volcanic eruptions may also form radiation patterns that scatter in all directions. Lunar Valleys (lunar gaps) There are many famous rift valleys on the earth, such as the East African Rift Valley.

There is also this kind of structure on the moon - those large black cracks that appear to be curved are lunar valleys. Some of them extend for hundreds to thousands of kilometers, and their widths range from a few kilometers to tens of kilometers. . Those wider valleys are found mostly in flatter areas of the moon, while those narrower, smaller valleys (sometimes called moon creeks) are found everywhere. The most famous lunar valley is the Alpine Great Lunar Valley, which connects the Mare Imbrium and the Mare d'Arc in the southeast of Plato Crater. It cuts off the Alps on the lunar surface, which is very spectacular. Photos taken from space estimate that it is 130 kilometers long and 10-12 kilometers wide. Where did it come from? ---The Mystery of the Moon's Formation The moon is an alien spacecraft: This is not nonsense, because the driving force of science lies in bold imagination. Without originality, there will be no new breakthroughs. The theory of relativity proposed by Einstein was It's not nonsense. What the Chinese lack in science is this kind of bold originality. Why can't we see the far side of the moon? The moon always faces the earth with one side. This is because the moon's autobiography and revolution periods are the same. (27.32166) To understand this phenomenon, you can do an experiment. Draw a circle and mark the directions of true east, west, north and south. You stand in the center of the circle (representing the earth), find another friend, stand on the circle, let him face forward (that is, without twisting his neck), move counterclockwise along the circle, and ask him to keep moving while moving along the circle. Always face towards the center of the circle, which is you. Then such a process basically simulates the rotation process of the moon and the earth. Obviously, in such a process, your friend will always face you with one side (the front). Let’s understand why in such a process, the revolution period is equal to the rotation period. Your friend starts from your due north and revolves around you. When he appears due north again, he completes a revolution cycle. (Similar to the time it takes the moon to make one revolution around the earth.) Let’s take a look at its rotation time. We might as well set the posture when your friend is due north of you and faces due south as the initial posture. Then we can find that when your friend moves counterclockwise to your due west position, his rotation posture rotates 90 degrees counterclockwise. (If your friend does not "rotate" during the process, then when he is at this position, he is not facing you, but is still facing the south direction. However, during the actual experiment, your friend is facing the right direction at this position. East, so he rotates 90 degrees counterclockwise relative to his initial position. Similarly, when he walks to your south, he rotates 180 degrees relative to his initial position. When it reaches the direction of your true north, it has rotated 360 degrees relative to its initial attitude. That is to say, it has completed a revolution. It has just completed a rotation process, so from a time perspective, this rotation period is equal to the revolution period, because during the whole process, your friend always faces you with his body and face. In other words, the moon always faces one side. Earth. Guanghan Palace - Moon Whenever night falls, a bright moon rises in the night sky, and the clear moonlight fills the earth, making people have countless thoughts and reveries. The literati and poets are even more fond of the moon. The poet Zhang Ruoxu of the Tang Dynasty wrote "On the River." "When does a person first see the moon? When does the river moon shine on people for the first time?" and "When will the bright moon come? Ask the blue sky with wine" by Su Shi, a writer of the Song Dynasty, which can be regarded as popular moon chants. The moon is commonly known as the moon, also known as the lunar moon. . In ancient Chinese mythology, there are countless stories about the moon. In ancient Greek mythology, the moon goddess’s name is Artemis, and she is also the goddess of hunting. The astronomical symbol of the moon is like a curved eyebrow, which also symbolizes Art. The Divine Bow of Mis. When the moon is bright in the sky, we can clearly see the dark parts and bright areas on it. When early astronomers observed the moon, they thought that the dark areas were covered with sea water, so they called them. "Sea". The famous ones are the Sea of ​​Clouds, the Sea of ​​Moisture, and the Sea of ​​Tranquility. The bright part is the mountains, which are crisscrossed by mountains and dotted with craters. The Bailey crater located near the South Pole has a diameter of 295 kilometers, which can cover the entire area. Hainan Island is included. The deepest crater is Newton Crater, which is 8,788 kilometers deep. There are also ordinary mountains and deep valleys on the moon. The moon is about 4.6 billion years old. The moon also has a layered structure such as crust, mantle, and core.

The average thickness of the outermost lunar crust is about 60 to 65 kilometers. Below the lunar crust to a depth of 1,000 kilometers is the lunar mantle, which accounts for most of the moon's volume. Below the lunar mantle is the lunar core. The temperature of the lunar core is about 1,000 degrees, and it is likely to be in a molten state. The diameter of the moon is about 3476 kilometers, which is 3/11 of the earth. The volume is only 1/49 of the Earth, and the mass is about 735 billion tons, which is equivalent to 1/81 of the Earth's mass. The gravity of the moon is almost equivalent to 1/6 of the Earth's gravity. Views on the formation of the moon 1. Split theory. This is one of the earliest hypotheses to explain the origin of the moon. As early as 1898, George Darwin, the son of the famous biologist Darwin, pointed out in the article "Tides and Similar Effects in the Solar System" that the moon was originally a part of the earth. Later, due to the rapid rotation of the earth, part of the material on the earth was thrown away. When it came out, these materials separated from the earth to form the moon, and the large crater left on the earth is now the Pacific Ocean. This view quickly received some objections. They believe that with the speed of the earth's rotation, it is impossible to throw a piece of something that big. Besides, if the moon was thrown out by the earth, then the material composition of the two should be the same. However, through laboratory analysis of the rock samples brought back from the moon by the "Apollo 12" spacecraft, it was found that the two are very different. 2. Capture theory. This hypothesis holds that the moon was originally just an asteroid in the solar system. Once, it moved near the earth and was captured by the earth's gravity. It has never left the earth since. There is also a view close to the capture theory that the earth continues to accretion matter that enters its orbit together. Over time, more and more things are accreted, and eventually the moon is formed. But some people point out that the earth may not have that much power to capture a planet as big as the moon. 3. Theory of homology. This hypothesis holds that the Earth and the Moon are both floating nebulae in the solar system, which formed stars at the same time through rotation and accretion. During the accretion process, the Earth corresponds a little faster than the Moon and becomes the "elder brother". This assumption has also been challenged objectively. Through laboratory analysis of rock samples brought back from the moon by the Apollo 12 spacecraft, it was discovered that the moon is much older than the earth. Some people believe that the moon is at least 7 billion years old. 4. Big collision theory. This is a new hypothesis about the formation of the moon in recent years. On March 20, 1986, at the Moon and Planets Symposium held at the Johnson Space Center in Houston, Benz and Slattery of the Los Alamos National Laboratory in the United States and Cameron* of the Smith Center for Astrophysics of Harvard University ** also proposed the giant collision hypothesis. This hypothesis holds that in the early stages of the evolution of the solar system, a large number of "planet particles" were formed in the interstellar space, and the planet particles grew up through mutual collision and accretion. The planetesimals merged to form a primitive Earth, and also formed a celestial body equivalent to 0.14 times the mass of the Earth. During their respective evolution processes, these two celestial bodies formed a metallic core mainly composed of iron and a mantle and shell composed of silicate. Since the two celestial bodies are not far apart, the chance of encountering them is high. By chance, the small celestial body hit the earth at a speed of about 5 kilometers per second. The violent collision not only changed the motion of the Earth and tilted its axis, but also caused the small celestial body to be shattered by the impact. The silicate shell and mantle were heated and evaporated, and the expanding gas and high speed carried a large amount of crushed dust flying away. Earth. The material flying away from the earth is mainly composed of the mantle of the collision object, and also contains a small amount of material on the earth. The ratio is roughly 0.85:0.15. The metal core separated from the mantle when the impactor broke up was decelerated by the expanding and flying gas, and was accreted to the Earth in about 4 hours. The gas and dust flying away from the earth are not completely separated from the gravitational control of the earth. They are combined by mutual accretion to form a completely molten moon, or they first form several separate small moons, and then gradually accrete to form a part. The big molten moon. Moon Composition 4.5 billion years ago, the surface of the moon was still a liquid magma ocean. Scientists believe that KREEP, the mineral that makes up the moon, exhibits chemical clues left behind by magma oceans. KREEP is actually a composite of what scientists call "incompatible elements"—materials that couldn't fit into the crystal structure and were left behind, floating to the surface of the magma. For researchers, KREEP is a handy clue to the volcanic history of the moon's crust and to infer the frequency and timing of impacts from comets or other celestial bodies.

The lunar crust is composed of a variety of major elements, including: uranium, thorium, potassium, oxygen, silicon, magnesium, iron, titanium, calcium, aluminum and hydrogen. When bombarded by cosmic rays, each element emits specific gamma radiation. Some elements, such as uranium, thorium and potassium, are inherently radioactive and can emit gamma rays on their own. But regardless of the cause, each element emits different gamma rays. Each element has unique spectral line characteristics and can be measured with a spectrometer. Until now, humans have not made comprehensive measurements of the abundance of lunar elements. Currently, spacecraft measurements are limited to only part of the lunar surface. Libra Movement Since the moon's orbit is elliptical, when the moon is at perihelion, its rotation speed cannot keep up with its revolution speed. Therefore, we can see the area in the eastern part of the moon reaching 98 degrees east longitude. On the contrary, when the moon is at aphelion, its rotation speed Faster than the revolution speed, so we can see the area in the western part of the moon reaching 98 degrees west longitude. This phenomenon is called meridian movement. The front and back of the moon: Front:

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