Tiny Object Found at the edge of the solar system for the first time. Kuiper Belt subject of just 2.6km



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Kuiper Belt, not an Edgeworth-Kuiper Belt, is home to ancient rocks. Kuiper Belt Objects, or KBOs, are the remains of early days and planet creation of our solar system. Small KBOs, in 1 km. a range of diameter, has been indicated about ten years, but not everyone is detected.

So far.

Planets will be created when fragments of sediment are made; Going into rocks, which enters into boulders, which are go into larger and larger objects. In the Internal Solar System, we see many of these larger rocks, or asteroids. We can check it out, but they are not the same as the old KBOs, old. Our neighborhood asteroids have changed by looking at the sun's radiation, through accidents, and by interacting with planets' trauma.

But KBOs are safer. Stronger representation of the state of the things in the Solar System is in the early stages. That's why finally it is confirmed that one of them is in a & # 39; creating as much interest.

The Kuiper Belt was named in honor of the American-American geologist Gerard Kuiper, who made a shelf of a peat corpse outside Neptune. The first thing to find Kuiper Belt was found in 1992. We now know more than a thousand items there, and it's It is estimated to be home to more than 100,000 asteroids and comets there over 62 miles (100 km). Credit: JHUAPL
The Kuiper Belt was named in honor of the American-American geologist Gerard Kuiper, who made a shelf of a peat corpse outside Neptune. The first thing to find Kuiper Belt was found in 1992. We now know more than a thousand items there, and it's It is estimated to be home to more than 100,000 asteroids and comets there over 62 miles (100 km). Credit: JHUAPL

Scientists have predicted that KBOs were between 1 km and a diameter of several kilometers. But they are so far away, how small, the most amazing thing is that there is no way to find one telescope. But finding a research team led by Ko Arimatsu at the Japanese National Astronomy Theater found a way: harassment.

In the same way in which we can find exoplanets about long stars by looking for a split in the starlight, Arimatsu and his team will be reasonable, we can look at the stars in the distance and their # 39; Look for KBO splitting in our Solar System. They started the OASES (Organized self-telegopy for Serendipitous Event Survey) project to do.

"This is really true for small projects."

Ko Arimatsu, Japanese Geographical National Review

They put two small telegopic (28 cm) on the Miyako open school top on Miyako Island, Miyakojima-shi, Okinawa Prefecture, Japan, and looked at around 2000 stars for a total of 60 hours.

When they analyzed 60 hours of data, the star team found its appearance as Objective radius 1.3 km Edgeworth-Kuiper. Their work shows that the Edgeworth-Kuiper Belt Objects kilometers are much larger than expected. It also supports the formulation of planet modules where planetesimals are first; grow slowly in kilometer causes before growing growth causes them to go with planets.

In a press release, Arimatsu explains: "This is really true for small projects. Our team was less than 0.3% of the budget of major international projects. We did not even have a & # 39; It's enough money to build a second ridge to protect our second telescope! However, we have made a search that the projects are not possible. Now we know that Our system works, we will investigate the Edgeworth-Kuiper Grid in a more detailed way. We have also set our scenes on Oort Cloud that are still uncovered. "

More detailed analysis of the team's results, and when they do, will fill an attractive gap in our understanding of the creation of a planet. As the team says in their paper, "If this is true for a KBO search, this means that they have a planetimals before they grow their level of growth. ; grow to become a knitting element in the main solar system outside and to remain a prime population in the current Kuiper belt. "

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