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Home https://server7.kproxy.com/servlet/redirect.srv/sruj/smyrwpoii/p2/ Science https://server7.kproxy.com/servlet/redirect.srv/sruj/smyrwpoii/p2/ The small object first discovered on the edge of the Solar System. Object of the Cuiper belt, which is only 2.6 km away

The small object first discovered on the edge of the Solar System. Object of the Cuiper belt, which is only 2.6 km away



The Bay of Keiper, or Edward-Kupper's belt, is home to ancient rocks. The sites of the Kaiper belt or the CBO are the remains of the early days of a planetary formation of our solar system. Small KBOs in 1 km. The diameter range has been theorized for decades, but no one has been discovered.

So far

Planets form when the pieces of powder conglomerate into rocks that conglomerate into stones that conglomerate into larger and larger objects. In our inner solar system we can see many of these larger rocks or asteroids. We can study them, but they are not the same as the distant, ancient CBA. The asteroids in our neighborhood have been altered by exposure to solar radiation, collisions, and interaction with the gravity of the planets.

But CBOs are more virgin. They are a more accurate representation of the state of things in the early solar system. That is why finally confirming the existence of one of them creates so much interest.

<img src = "https://www.universetoday.com/wp-content/uploads/201
6/10/Kuiper-Belt-with-New-Horizon-traj-1024×580.jpg" alt = "Kuiper Belt was named in honor of the Dutch-American astronomer Gerard Keiper, who postulated a reservoir of icy bodies beyond Neptune.The first object of the Kuiper Belt was discovered in 1992. We now know about more than a thousand sites there and are estimated to live in more than 100,000 asteroids and comets located more than 100 km, was named in honor of the Dutch-American astronomer Gerard Keiper, who postulated a reservoir of icy bodies beyond Neptune. Kupper was discovered in 1992. We now know about more than a thousand sites there, and it is believed that over 100,000 asteroids and comets lying there are more than 100 kilometers long. but they are so far away, so small and so incredibly dark that there is no way a telescope can see one. But a research team led by Co Arimatsu of Japan's National Astronomical Observatory found a way to find them: an eclipse.

In the same way we can find exoplanets around distant stars by watching dims in the starlight, Arimatsu and his team. motivated, we can observe distant stars and look for dips caused by CBC in our solar system. They started the OASES project (Organized Auto-Telescopes for Random Events) to do so.

"This is a real victory for small projects."

They placed two small (28 cm) telescopes on the roof of Miyako's Miyakojima-shi, Okinawa Prefecture, Japan, and observed about 2000 stars for a total 60 hours.

When analyzing the 60 hours of data, the team found a star that looked obscured as it was sunk in the 1.3 km radius of the Edgeworth-Kuiper Belt Object. Their work shows that the kilometric Edgeworth-Kuiper Belt objects are more numerous than previously thought. He also supports planetary patterns of formation where planesimaths first develop slowly into miles of objects, before their growth unites them into planets.

In a press release, Arimatsu explains: "This is a real victory for small projects. Our team had less than 0.3% of the budget of major international projects. We did not even have enough money to build a second dome to protect our second telescope! Still, we were able to make a discovery that is impossible for big projects. Now that we know our system is working, we will study the Edgeworth-Kuiper Belt in more detail. We also have our sights on the still uncovered Oort Cloud beyond that. "

More discoveries will confirm the team's findings, and when they do, they will fill in gaps in our understanding of the formation of the planet. As the team says in their report, "If this is a true CBC detection, it means that planetside before their growth phase has become objects of a kilometer size in the original external solar system and remain as the main population in today's Kuiper.

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