PS: The nine planets come and go freely, with RLPR crystallization, you can meet as you like, go down to the deep sea to catch turtles, go to the moon for nine days, and ask for a reward!

Chapter 34 Implementation of the Eleventh Dimensional Space Invention III

It wasn't until this time that Gu Xiaohu, a little kid driving his toy-like space vehicle, finally returned, and when he saw his satisfied appearance, he knew that this space trip was really crazy enough. Look at the toy-like space vehicle, it has completely changed its appearance, it has actually become a space train, pulling a section of cargo boxes, each cargo box is full, this trip can be described as quite fruitful, all loaded with all kinds of toys from all over the blue planet, all kinds of toys, even the little girl's Barbie doll has pulled a whole carriage, according to him, to give to the neighbor children. Not to mention the Transformers, all kinds of racing cars, tanks, airplanes, motorcycles and other boys' toys, which are loaded into three compartments.

There is also a carriage filled with all kinds of deep-sea creatures, all kinds of beautiful corals, shells, sea urchins, etc., and I also excitedly conjure up a video camera to show my own images in the deep sea of various oceans, although the photography skills are not good, but it is a very interesting and very scientific value of the image. The deep-sea environment is characterized by high pressure, which increases by about 1 atmosphere for every 10 meters of water depth, and at an abyss of 10,000 meters, the pressure is 1,000 atmospheres. Second, the bottom flow velocity is mostly very slow. The third is plants without light and without photosynthetic nutrition. Fourth, low temperature, except for the high water temperature in individual sea areas (such as the Mediterranean), the average temperature of deep sea water is 1~3 °C, and the lowest can reach -1.8 °C. Fifth, the salinity is high (35‰) and the change is small. Sixth, the oxygen content is relatively abundant, usually the oxygen content of 500~1000 meters of water depth is the lowest, and the oxygen content of the upper and lower aquifers is higher. Seventh, the sediment is mostly soft mud and clay.

Deep-sea organisms can be divided into three categories: planktonic, swimming, and benthic according to their lifestyles. It is composed of some species such as bacteria, protozoa, coelenterates, crustaceans, hairy-jawed animals, etc., and the number of species and organisms is smaller. The number of organisms usually decreases significantly with increasing water depth. The medium-sized plankton mass in the waters of the Pacific Kuril Islands-Kamchatka averages more than 100 mg per cubic meter at a depth of 200~400 meters. But below 3000 meters, it is less than 1 milligram. The same zooplankton. Individuals mostly live in shallow places when they are young. Individuals live in the depths when they are larger. For example, some species of the copepod Daphnia and Daphnia glareus can live up to 17 mm in water at depths of 2,000 meters, and as the water becomes shallower, the size of the individual decreases. Deep-sea zooplankton are mostly omnivorous or carnivorous. The vertical movement of zooplankton plays a positive role in the vertical transfer of nutrients. The main species of zooplankton are: 1. Crustaceans, the most important of which are some species of genera such as Daphnia sage, Daphnia sage, Daphnia sage, Daphnia glabra (the largest individual can reach 17 mm). This is followed by mystic shrimp, krill, amphipods and decapods, as well as mesomorphic animals. Second, coelenterates, there are bowl jellyfish and tube jellyfish. There is no hydrop stage in their life history, and individuals are generally larger. It can be up to 25 centimeters in diameter, mostly maroon and purple, and can emit light. 3. Olive green cells, cells with a length of 10~15 microns. Some scholars believe that they belong to flagellates. At a water depth of 3000~4000 meters, the density of such cells can still reach 25000~50000 cells/liter. It is also commonly found in the intestines of some planktonic crustaceans, and their origin is unknown.

It is mainly fish, followed by squid, octopus and shrimp. Of the more than 1,000 species of oceanic fish, about 150 live in deep waters. Among them, the largest number of species belong to the suborder Horn, with about 80 species. The head of a deep-sea fish has a stalk-like protrusion on the dorsal side, and the top can be used as a bait and lighting. Big mouth. Females can weigh up to 6~8 kg, while males weigh only a few grams. The male's head burrows into the female's epidermis to absorb nutrients. and form a small fissure, the female spawning period. Male fish produce sperm in a bag in preparation for insemination. Fish do not form groups and keep a distance of about 30 meters between individuals. There are also many eels in the deep sea, such as Hastelloy's cystopharyngeal fish and widepharyngeal fish. The fish has a slender body and a particularly large mouth. Some eel larvae swim into shallower water and return to deep water when they become adults. Among the deep-sea fish, the number of individuals of the genus is the largest, the fish is small, only 5~6 cm long, the head is large, dark brown, and its gills can filter feed zooplankton. Do not form groups, keeping a distance of approximately 3 meters between specimens. In the deep sea, there are many species of near-bottom fish, and the individuals are also larger, such as the sleeping shark, which can reach 7 meters in length and live on predation. Some deep-sea fish are often able to swallow foods larger than themselves. There are few species of deep-sea cephalopods, and some octopuses are adapted to deep-sea life and have no eyes.

Adults didn't expect to spoof the superstar little child Gu Xiao, the tiger actually has such a strong desire for knowledge, and it can be seen that it has a strong preference for all kinds of small animals, from the largest carriage can be seen, what little squirrels, parrots, kittens, dogs, etc., I don't know where he collected it, the child's family is going to suffer, such a large car dozens of small guests, but they have to work hard to feed it!

The image shown by the little child Gu Xiaohu is even more amazing, this is the real image of the remaining nine planets in our solar system, this is the dream image of the astronomers of the Blue Planet, but I didn't expect to be preempted by a completely hairy boy. Of course, due to the continuous implementation of the invention of the eleventh dimensional space in the puppet space and the black gold space, these space travels, which seemed to be fantastical in the past, are already just a piece of cake.

Mercury, the first planet of the nine planets, was the god of commerce, travel, and theft in ancient Roman mythology, namely Hermes in ancient Greek mythology, the god of messengers to the gods, perhaps because of the speed at which Mercury moves in the sky, which gave it its name. As early as 3000 BC in Sumerian times, people discovered Mercury, and the ancient Greeks gave it two names: when it first appeared in the early morning it was called Apollo, and when it twinkled in the night sky, it was called Hermes. However, ancient Greek astronomers knew that the two names actually referred to the same star, and Heracletus (a Greek philosopher in the 5th century BC) even believed that Mercury and Venus did not orbit the Earth, but orbited the Sun. Only the Mariner 10 probe visited Mercury three times, in 1973 and 1974. It surveyed only 45% of Mercury's surface (and was unlucky, because Mercury was too close to the Sun. so much so that the Harbour Telescope could not safely photograph it).

Mercury's orbit deviates greatly from the perfect circle. The perihelion is only 46 million kilometers from the Sun. The aphelion is 70 million kilometers, and at perihelion in orbit it orbits the Sun at a very slow rate (precession: a phenomenon in which the precession of the Earth's axis causes the vernal equinox to move slowly westward at a speed of 0.2' per year, about 25,800 years, making the return year shorter than the sidereal year). There are two types of precession, the precession and the precession of the planets, the latter being caused by changes in the ecliptic plane caused by the gravitational pull of the planets. In the nineteenth century, astronomers looked at Mercury's orbital radius very closely, but could not properly explain it using Newtonian mechanics. The subtle discrepancies that exist between the actually observed values and the predicted values are a minor (a difference of one-seventh degree per millennium) but a problem that has plagued astronomers for decades. It has been suggested that there is another planet (sometimes called Vulcan) in orbit close to Mercury. "Zhu Rongxing"), which explains this discrepancy, and the final answer is quite dramatic: Einstein's general theory of relativity. In the early days of acceptance of this theory, the correct prediction of Mercury's orbit was a very important factor. (Mercury orbits the Sun because of its gravitational field, which is extremely large, and according to general relativity, mass produces a gravitational field, which in turn can be regarded as mass, so the giant gravitational field can be regarded as mass, resulting in a small gravitational field.) deviate from its orbit. Similar to the divergence of electromagnetic waves, a changing magnetic field produces an electric field. The changing electric field creates a magnetic field that travels far away. Until 1962, it was thought that Mercury would rotate once and for the same time, so that the side facing the Sun would remain constant. This is very similar to the fact that the Moon always faces the Earth on the same half side. But in 1965, through observations of Doppler radar, it was found that this theory was wrong. Now that we know that Mercury rotates for two and three times at the same time, Mercury is the only known object in the solar system that has a co-motion ratio of 1:1 between its orbital and rotational periods. The temperature difference on Mercury is the largest in the entire solar system, with temperature variations ranging from 90 to 700 Kai. In contrast, Venus is slightly warmer but more stable.

Mercury is similar to the Moon in many ways, with many craters on its surface and very old; It also has no plate movement. Mercury, on the other hand, is much denser than the Moon, (Mercury 5.43 g/cm3 and Moon 3.34 g/cm3). Mercury is the second densest object in the solar system after Earth. In fact, the high density of the earth is partly due to the compression of gravity; Either way, Mercury would be denser than Earth's, suggesting that Mercury's iron core is somewhat larger than Earth's, and most likely makes up most of the planet. As a result, Mercury has only a thin circle of silicate mantle and crust, relatively speaking. The massive iron core, with a radius of 1,800 to 1,900 kilometers, is the dominator of Mercury's interior. The silicate shell is only 500 to 600 kilometers thick, and at least part of the core is probably molten.

In fact, Mercury's atmosphere is thin and made up of destroyed atoms brought by the solar wind. Mercury's temperature is so high that these atoms quickly escape into space, so that Mercury's atmosphere is frequently replenished and replaced compared to the stable atmospheres of Earth and Venus.

The surface of Mercury exhibits huge steep slopes, some reaching hundreds of kilometers long and three kilometers high. Some are transverse at the outer ring of the crater, while others have a sharp slope that suggests that they were formed by compression. It is estimated that Mercury's surface has shrunk by about 0.1% (or about 1 kilometer in the radius of the planet).

One of the largest geomorphic features on Mercury is the Caloris Basin, with a diameter of about 1,300 kilometers, which is thought to be similar to Maria, the largest basin on the Moon. Like the basin of the Moon, the Caloris Basin was most likely formed during the Great Collision in the early solar system, which probably also created the strange terrain of the basin on the other side of the planet. In addition to the crater-ridden terrain, Mercury also has relatively flat plains, some of which may be the result of ancient volcanic activity, but others may be the result of ejecta deposits formed by meteorites. Mercury has a small magnetic field that is about 1% of Earth's.

What is surprising is that Gu Xiaohu, a playful spoof superstar child, actually parked his toy-like space vehicle on the surface of Mercury. Also made a circle around Mercury. Different rock specimens were retrieved. It's incredible.

The second planet, Venus, is the second closest planet to the Sun and the sixth largest planet in the solar system. Of all the planets, Venus has the closest orbit to a circle, with a deviation of less than 1%. Orbital radius: 108,200,000 km (0.72 AU) from the Sun, planetary diameter: 12,103.6 km, mass: 4.869 e24 kg.

Venus (Greek: Aphrodite; Babylonian: Ishtar) is the goddess of beauty and love, and the reason for its name is perhaps to the ancients. It is the brightest of the known planets. (There are also some objections that Venus was named because it resembles a woman's appearance.) Venus has been known since prehistory. Aside from the Sun and Moon, it is the brightest one. Like Mercury, it is often thought to be made up of two separate stars: the morning star is called Eosphorus and the evening star is called Hesperus, which Greek astronomers know better. Since Venus is an inner planet, if you look at it from Earth with a telescope, you will see that it has a phase change. Galileo's observations of this phenomenon are important evidence in favor of Copernicus's heliocentric theory of the solar system.

The rotation of Venus is very unusual in that on the one hand it is very slow (the Venusian day is equivalent to 243 Earth days, which is slightly longer than the Venusian year). On the other hand, it is inverted. In addition, Venus's rotation period coincides with its orbital period. So when it reaches its closest point with the Earth, the side of Venus towards the Earth is always fixed. Whether this is a resonance effect or just a coincidence is unknown.

Venus is sometimes referred to as the sister planet of the Earth, and they are very similar in some ways: First, Venus is slightly smaller than the Earth (95% of the Earth's diameter, 80% of the Earth's mass). Second, there are some roundabouts on the relatively young surface. Third, their density and chemical composition are very similar. Because of these similarities, it is sometimes thought that Beneath its thick clouds Venus may be very similar to Earth and may have life. But unfortunately, many in-depth studies of Venus have shown that Venus is fundamentally different from Earth in many ways.

Venus has an atmospheric pressure of 90 standard atmospheres (equivalent to the pressure at a depth of 1 kilometer in the Earth's oceans), and the atmosphere is mostly composed of carbon dioxide, but also has several layers of clouds thousands of meters thick composed of sulfuric acid. These clouds block our view of the surface of Venus, making it appear very vague. This dense atmosphere also has a greenhouse effect, raising the surface temperature of Venus by 400 degrees Celsius, more than 740 degrees (enough to melt the lead strips). The surface of Venus is naturally hotter than the surface of Mercury, although Venus is twice as far from the Sun as Mercury. There are strong winds at the top of the clouds, about 350 kilometers per hour, but the surface winds are very slow, less than a few kilometers per hour.

It is in this environment of non-human existence that there is no harshness, our naughty spoof master child Gu Xiaohu is still fearless, and happily takes Venus from south to north and from east to west, of course, this is mainly because of the RLPR (human servant) crystal, which can play a protective role in any environment.

The fourth largest planet is the fourth farthest from the Sun and the seventh largest planet in the Solar System, with an orbital orbit of 227,940,000 km (1.52 AU) from the Sun. Planet diameter: 6,794 km. Mass: 6.4219e23 kg. Mars (Greek: Ares) is known as the god of war. This may be due to its bright red color; Mars is sometimes referred to as the "Red Planet". (Fun note: Before the Greeks, the ancient Romans worshipped the Martians as the god of light farming.) The aggressive and expansive Greeks, on the other hand, used Mars as a symbol of war, and the month of March got its name from Mars.

Mars has been known to mankind since prehistoric times. Since it is considered to be the best dwelling place for humans in the solar system (other than Earth), it is loved by science fiction writers. Unfortunately, the famous "canal" that Lowell "saw" and everything else are just fictional like the Barsoomian princesses.

The orbit of Mars is significantly elliptical. Thus, the temperature difference between perihelion and aphelion is almost 30 degrees Celsius in the place where the sun is received. This has a huge impact on the climate of Mars. The average temperature on Mars is about 218 K (-55 °C, -67 degrees Fahrenheit), but it ranges from 140 K (-133 °C to 207 degrees Fahrenheit) in winter to nearly 300 K (27 °C) during the daytime in summer. 80 degrees Fahrenheit). Although Mars is much smaller than Earth. But its surface area is equivalent to the land area of the Earth's surface.

With the exception of Earth, Mars is the solid surface planet with the most interesting terrain of all kinds. Some of them are spectacular, such as the Olympus Mountains: at 24 kilometers (78,000 feet) above the surface, they are the largest mountains in the solar system. Its base is more than 500 kilometers in diameter and is surrounded by a cliff up to 6 kilometers (20,000 feet) high; Then there's Tharsis: a huge bulge on the surface of Mars, about 4,000 kilometers wide and 10 kilometers high; There is also Valles Marineris: canyons 2 to 7 km deep and 4,000 km long; And Hellas Planitia: in the Southern Hemisphere. More than 6,000 meters deep and 2,000 kilometers in diameter, the impact crater.

The surface of Mars has many old craters. But there are also many valleys, ridges, hills and plains that have not been formed for a long time. In the southern hemisphere of Mars, there are curved rings of highlands similar to those on the Moon. On the contrary, its northern hemisphere is mostly made up of newly formed low-lying plains. The formation of these plains is complex. There is a huge change in elevation of several kilometers on the north-south border. The reasons for the great difference in topography between the north and the south and the high degree of upheaval in the border areas are unknown. The interior of Mars is inferred only on the basis of its superficial information and the large amount of data involved. Its core is generally believed to be composed of high-density materials with a radius of 1,700 km; Surrounded by a layer of lava, it is thicker than the Earth's mantle; The outermost layer is a thin shell. Mars is less dense than other solid-state planets, suggesting that the iron (magnesium and iron sulfide) in the Martian core may contain more sulfur.

Like Mercury and the Moon, Mars lacks active plate movements; There is no indication that Mars has had a translational activity in the Earth's crust that would have caused as many folded mountains as Earth's. Since there is no lateral movement, the thermals under the earth's crust are stationary relative to the ground. Add to that the slight gravitational pull of the ground. caused the Tharis bulge and the huge volcano. Although, there may have been a lot of volcanic activity on Mars. But it never seems to have had any tectonic plate movements. There have been floods on Mars, and there are some small rivers on the ground, which is clear evidence that many places have been eroded. In the past, there has been clean water on the surface of Mars, and there may have even been large lakes and oceans. But these things seem to have only existed for a short time, and they are estimated to be about four billion years old.

In the early days of Mars, it was very similar to Earth. Like Earth, almost all of the carbon dioxide on Mars is converted into carbon-containing rocks. But in the absence of Earth's tectonic plate movements, Mars is unable to recycle carbon dioxide into its atmosphere to produce a significant greenhouse effect. Therefore, even if it is pulled to the same distance from the Earth from the Sun, the temperature on the surface of Mars is still much colder than on Earth.

The thin atmosphere of Mars is mainly composed of the remaining carbon dioxide (95.3%) plus nitrogen (2.7%), argon (1.6%) and trace amounts of oxygen (0.15%) and water vapor (0.03%). The average atmospheric pressure on the surface of Mars is only about 7 millibars (less than 1% on Earth), but it varies with altitude and can reach as high as 9 millibars at the deepest point of the basin and only 1 millibar at the top of OlympusMons. But it's also strong enough to support the occasional hurricane and storm that sweeps across the planet throughout the month. The thin layers of Mars' atmosphere can also create a greenhouse effect, but those can only raise the temperature of its surface by 5 K, which is much less than what we know about Venus and Earth.

The poles of Mars are permanently covered with solid carbon dioxide (dry ice). The structure of this ice cover is cascading, which is made up of alternating layers of ice and changing layers of carbon dioxide. In the northern summer, carbon dioxide is completely sublimated, leaving behind a layer of icy water. Since the carbon dioxide in the south has never completely disappeared, it is impossible to know whether there is also an ice water layer under the ice layer in the southern part of the road. The cause of this phenomenon is not known, but it may be due to the long-term change in the angle between the equatorial plane of Mars and its orbit that causes climate change. Perhaps there is also water deeper below the surface of Mars. This change in the cover of the poles due to seasonal changes has changed the pressure of Mars by about 25%.

Gu Xiaohu, the playful spoof superstar child, once again parked his toy-like space vehicle on the surface of Mars, and also circled Mars. Different rock specimens were retrieved. This time, I also went to the north and south poles of Mars. The recovery of a sample of dry ice from Mars made it even more incredible. In fact, Gu Xiaolong is very clear, because the father of the little child Gu Xiaohu is a doctoral supervisor in astronomy at the Capital University of Country C, and the child has been very interested in these astronomical knowledge since he was a child, so he will have such a move.

Jupiter, the fifth planet, is the fifth planet from the Sun and the largest. It is 2 times more massive than all other planets (318 times that of Earth). Orbit: 778,330,000 km (5.20 AU) from the Sun. Planet diameter: 142,984 km (equator). Mass: 1.900e27 kg. Jupiter (a.k.a. Jove; Zeus, as the Greeks called it, was the king of God, the ruler of Mount Olympus and the protector of the Roman state, and it was the son of Cronus (Saturn).

Jupiter is the fourth brightest object in the sky (after the Sun, Moon, and Venus; Sometimes Mars is brighter), Jupiter has been known to mankind since prehistoric times. According to Galileo's 1610 observation of Jupiter's four moons: Europa, Europa, Europa, and Calmede (now often called Galileo's moons), they were the first discoveries that did not orbit around the Earth, and they were the main basis for agreeing with Copernicus's heliocentric theory of planetary motion; Galileo was arrested by the Inquisition for his outspoken support of Copernicus' theories and forced to renounce his faith. He spent the rest of his life in prison. Gas planets do not have a solid surface, and their density of gaseous matter only increases with increasing depth (we calculate their radius and diameter from the equivalent of 1 atmosphere on their surface). What we see is usually the tip of the clouds in the atmosphere. The pressure is slightly higher than 1 atmosphere.

Jupiter is composed of 90% hydrogen and 10% helium (ratio of atomic numbers, 75/25% mass ratio) and trace amounts of methane, water, ammonia and "stones". This is very similar to the composition of the primordial solar system nebulae that formed the entire solar system. Saturn has a similar composition, but Uranus and Neptune have a smaller amount of hydrogen and helium.

Jupiter may have a stony core equivalent to 10-15 Earth's masses. On the inner core, most of the planetary material is concentrated, in the form of liquid metallic hydrogen. These most modest forms on Jupiter may only exist at 4 billion bars of pressure, which is the environment inside Jupiter (and Saturn is too). Liquid metallic hydrogen is made up of ionized protons and electrons (similar to the interior of the sun, but much cooler). At the temperature pressure inside Jupiter, hydrogen is liquid rather than gaseous, making it the electronic conductor and source of Jupiter's magnetic field. Also in this layer may also contain some helium and trace amounts of "ice".

The outermost layer is mainly composed of ordinary hydrogen and helium molecules, which are liquid on the inside and gasified on the outside, and we can see the upper part of this deep layer. Water, carbon dioxide, methane, and other simple gas molecules are also a little bit here.

Ammonia ice, ammonium-water sulphides, and ice-water mixtures are thought to be present in the three distinct layers of the clouds. However, preliminary results from the proof from Galileo indicate that these materials are extremely scarce in the clouds (one instrument appears to have detected the outermost layer, and the other may have detected the second outer layer at the same time). But the surface position of the proof is unusual (left) – Earth-based telescope observations and more recent observations from the Galileo orbiter suggest that the region chosen for this proof is likely to be the warmest and least cloudy region of Jupiter at that time.

Jupiter and other gaseous planets have high-velocity hurricanes on their surfaces and are confined to a narrow range of latitudes, with winds blowing in the opposite direction even near latitudes. Slight changes in the chemical composition and temperature of these bands create colorful surface bands that govern the appearance of the planets. The shiny surface bands are called zones, and the dark ones are called belts. These bands on Jupiter have been known for a long time, but the whirlpools in the boundary zone of the bands were first discovered by the Voyager spacecraft. Data sent back by the Galileo spacecraft indicated that the surface winds were much faster than expected (more than 400 mph) and extended to as deep as the roots could observe, about thousands of kilometers inward. Jupiter's atmosphere has also been found to be quite disordered, suggesting that the hurricane moves at a rapid pace for most of its time due to the heat inside it, unlike Earth, which only gets its heat from the Sun. The colorfulness of the clouds on Jupiter's surface may be caused by subtle differences in the chemical composition of the atmosphere and their effects. It is possible that a mixture of sulfur was mixed in it. The result is a colorful visual effect. However, the details of this are still unknown.

The change in color depends on the height of the clouds: blue at the lowest, followed by brown and white, and red at the highest. We can see the clouds lower through the holes in the clouds above. The Great Red Spot on Jupiter's surface was known to Earth observations as early as 300 years ago (a discovery often attributed to Cassini or Robert Hooke in the 17th century). The Great Red Spot is a 25,000-kilometer-long, 12,000-kilometer-long elliptical that accommodates two Earths. Other, smaller spots have also been seen for decades. Infrared observations and derivation of its rotation trend show that the Great Red Spot is a high-pressure area, where the top of the cloud layer is particularly high and cold compared to the surrounding area. A similar situation is seen on Saturn and Neptune. It is unclear what such structures can last for that long.

Jupiter radiates more energy outward than it receives from the Sun. Jupiter's interior is hot: up to 20,000 open at the inner core. The yield of this heat is generated by the Kelvin-Helmholtz principle (slow gravitational compression of planets). (Jupiter does not produce energy from nuclear reactions like the Sun.) It is too small so that the internal temperature is not sufficient to cause the conditions for a nuclear reaction. This internally generated heat may have greatly triggered convection in Jupiter's liquid layer and caused the complex movement of the cloud tops we are seeing. Saturn and Neptune are similar to Jupiter in this regard, and oddly enough, Uranus is not.

Jupiter coincides with the maximum diameter that a gas planet can reach. If the composition is increased again, it will be compressed by gravity, so that the global radius will increase only slightly. A star can only grow in size because of the internal heat source (nuclear energy), but for Jupiter to become a star, the mass must be at least 80 times larger.

Jupiter has a giant magnetic field, much larger than Earth's, and the magnetosphere extends outward by more than 6.5e7 kilometers (more than Saturn's orbit!). ）。 (Note: Jupiter's magnetosphere is not spherical.) It just stretches in the direction of the sun. As a result, Jupiter's moons remain in Jupiter's magnetosphere, and some of the resulting conditions are partially explained on Europa. Unfortunately. For future spacewalkers and experts dedicated to the design of Voyager and Galileo, the high-energy particles captured by Jupiter's magnetic field in the nearby environment would be a major obstacle. This type of "radiation" is similar, but much more intense than, the Earth's ionospheric belt. It will have a fatal impact on unprotected humanity immediately.

Jupiter has a ring like Saturn's, but small and faint. Their discovery was purely unexpected, except that the scientists of the two Voyager 1 had repeatedly insisted on traveling 1 billion kilometers to see if there was a halo. Everyone else thinks that the chances of finding the auras are zero, but in fact they exist. What a brilliant plan these two scientists came up with. They were later photographed by telescopes on the ground.

Unlike Saturn's, Jupiter's rings are fainter (albedo 0.05). They consist of many granular rocky materials. The particles in Jupiter's rings may not be stable (due to the atmosphere and magnetic fields). In this way, if the auras are to maintain their shape, they need to be replenished constantly. Two small moons orbiting in the Halo, Callisto and Calmede, are the obvious candidates for Halo resources.

Jupiter's moons: Jupiter has 16 known moons, 4 moons discovered by Galileo the Great, and 12 small ones. Jupiter's motion is gradually slowing down due to the gravitational force generated by Galileo's moons. Similarly, the same gravitational force changes the orbits of the moons, causing them to slowly and gradually move away from Jupiter. Europa, Europa, and Europa are affected by the tidal force to fix the co-rotation relationship at 1:2:4 and change together. Ganymede is also part of this. For hundreds of millions of years to come, Europa will also be locked in, running at twice the revolution period of Europa and eight times that of Europa. Jupiter's moons were named after the people Zeus came into contact with during his life (mostly his lovers). (To be continued......)