Hubble tests 16 manas, asteroids worth $ 10,000 billion


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Asteroid 16 Manas (as the name suggests it was the 16th) is believed to have been the now exposed part of the discriminating protoplanet that broke up billions of years ago. Its composition is generally considered to be 90 percent metal and 10 percent silicate rock. It is thought to be much smaller than the typical Stony of the equivalent size, and contains about 1 percent of the entire mass of the planetary belt.

Assuming the core is made of iron and nickel, the total value of the asteroid (if we ignore the effect on market prices) would be ~ 10,000 to r 1 trillion. There are 16 NASA missions expected to begin in 2022 and reach in 2026, and the Hubble Space Telescope spent some time surveying the main body. The composition of the surface of Saiche and the implications of the scientific tests and equipment of the material made from it will be loaded on the probe we send to study the planet.

Researchers in Ultraviolet examined Psyche – one of only a handful of asteroids to examine in this way – to see how light is reflected from its surface. Eclipse signals can reveal details of an asteroid’s internal structure. The information they have found generally supports high iron composition for object objects, but they have found that mixing relatively small amounts of iron in rocky objects such as olivine can produce psychic ultraviolet signature. This “makes it difficult to quantify the amount of iron that appears on the surface of the mind.”

Representation of the mind during Hubble observations. The main part is no field.

There are several theories as to how scientists can create a psyche. It could be a remnant iron protoplanet destroyed in a destructive effect. It may have been the remains of a protoplanet that lost its outer layers in heavy impacts that stripped the surface but also shattered the entire object. There are numerous theories about its formation, and the research to be undertaken by Saich tells us a great deal about the early conditions of the solar system.

The asteroid belt does not really preserve the remains of the ancient solar system as it once was; After the collision the material present there today has been rebuilt and collided again. As we send spacecraft to asteroids like Vesta and dwarf planets like Ceres, we have begun to recreate those collision modes. For example, we know that a massive collision on the asteroid Vesta a billion years ago is responsible for the greater number of Vesta asteroids found on Earth.

This ultraviolet analysis of Saichena does not confirm that asteroids are iron-rich original fossils, but they certainly do not confirm that it suggests other data collected on Psyche, such as its gravitational effect on other nearby bodies (high density). The psyche is the only known metal core-like body from any of the currently known planets that is available for us to access. Put it differently: Before the eclipse is sufficient for a planetary eclipse, the psyche may represent a scale model of the origin of the earth.

This process can fail due to more conflicting gies in the psyche. One of the theories as to why the eclipse belt failed to eclipse the planet is that Jupiter kept the gravitational energy very high to support the planetary eclipse, and the material of the eclipse was either emptied, thrown into the dust, (during the Great Heavy Bombardment). ), Or swallowed only by Jupiter.

The goals of the Psych mission are to determine whether the psyche represents the core of a planet or a group of previously unmelted materials, to gather information about its age, to investigate the structural differences between the minerals in the core of the psyche and the expected contents of the earth under which it forms, And is characteristic of its overall topography.

There are currently no serious plans to mine the mind, but only if the Earth begins to colonize the outer solar system (as shown in the TV show) Expansion), There is no question that we will tap the planet for content one way or another. It is a rock that can teach us about the early days of our solar system, when we need to build its future while providing raw materials.

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