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New dwarf planet solar system's 2nd most distant

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Diagram showing the orbits of the newly-discovered dwarf planet 2014 UZ224, together with the present positions of Uranus, Neptune, and Pluto. The dot indicates the present position of the 2014 UZ224 in its orbit. Image credit: JPL Horizons, Sky and TelescopeDiagram showing the orbits of the newly-discovered dwarf planet 2014 UZ224, together with the present positions of Uranus, Neptune, and Pluto. The dot indicates the present position of the 2014 UZ224 in its orbit. Image credit: JPL Horizons, Sky and TelescopeANN ARBOR—Astronomers at the University of Michigan and their colleagues on the Dark Energy Survey have discovered a new dwarf planet that's more than 90 times farther from the sun than Earth is, making it the second-most distant minor planet in the known solar system.

The Dark Energy Survey, which uses a powerful digital camera called DECam on a 4-meter telescope in Chile, was designed to capture images of distant galaxies to understand why the expansion of the universe is accelerating.

"But the same sensitivity that makes this a state-of-the-art survey of the distant universe also makes it a powerful tool to look for new objects in our own cosmic backyard," said David Gerdes, the U-M physics and astronomy professor who led the planet-finding team.

The DES images are sensitive enough to detect the reflected sunlight from the new object, which is as faint as a single candle 100,000 miles away.

The researchers say the discovery of the icy, faraway world shows that their technique is a promising approach for finding "Planet Nine"—a massive body hypothesized to reside around 600 times farther from the sun than Earth. The existence of Planet Nine would explain the elongated, aligned orbits of a group of distant minor planets similar to, but not including, this newly discovered one.

The U-M team submitted observations of the object to the Minor Planet Center, an international organization that designates and tracks minor planets, comets and moons. The center gave it a designation—2014 UZ224—but after its orbit has been refined for several more years, the researchers can propose an official name. In the meantime, they've dubbed it DeeDee, short for distant dwarf.

At this point in its orbit, DeeDee is more than 8.5 billion miles from the sun, or 92 astronomical units. One astronomical unit is the distance from the sun to Earth. Only the Pluto-sized dwarf planet Eris is currently more distant, though other minor planets with off-centered orbits spend most of their time even further out. On DeeDee, the sun would look like a very bright star.

The data indicate that DeeDee is between 200 and 800 miles in diameter, meaning it is probably large enough to qualify as a dwarf planet. The researchers expect to obtain a much better estimate of its size from an image they recently obtained with the Atacama Large Millimeter/submillimeter Array telescope in Chile. The researchers expect to complete this analysis and publish the results by mid-November.

To identify DeeDee, the researchers looked through thousands of images to find moving objects in orbit around the sun, against the background of millions of stars and galaxies that remain in the same place from night to night. Gerdes likens this to "finding a really small needle in a really big haystack."

The researchers don't look for planets with their eyes. Thousands of computers at Fermilab were used to analyze hundreds of terabytes of data, a process that would have taken more than 300 years on a single computer.

Even with a powerful instrument like DECam, distant minor planets look like points.

"Every image taken by DECam is subtracted from every other image from the same piece of the sky. That way, we can find moving solar system objects even if they happen to lie right in front of a background galaxy or star," said Masao Sako, a physicist at the University of Pennsylvania who was also involved in the search.

This analysis still left the researchers with millions of "dots," and many more possible ways to connect them. Computer programs developed by the U-M team took several more months to perform that task. Their code identified DeeDee this summer.

Minor planet "DeeDee" discoverers undergraduate Tali Khain, Physics and astronomy professor David Gerdes, doctoral student Stephanie Hamilton and undergraduate Lynus Zullo, all in the U-M College of Literature, Science and the Arts. Image credit: Eric Bronson, Michigan PhotographyMinor planet "DeeDee" discoverers undergraduate Tali Khain, Physics and astronomy professor David Gerdes, doctoral student Stephanie Hamilton and undergraduate Lynus Zullo, all in the U-M College of Literature, Science and the Arts. Image credit: Eric Bronson, Michigan PhotographyMichigan undergraduates played important roles on the team.

"I'm so grateful to have been given the opportunity to work with Professor Gerdes and contribute to this project," said Tali Khain, a sophomore majoring in physics and math whose work for this project involves analyzing the long-term behavior of minor planets beyond Neptune. "It's extremely exciting."

Even more exciting would be identifying the elusive Planet Nine. Its existence was recently suggested as a way to explain the off-kilter orbit of the dwarf planet Sedna, which crosses through the plane of the solar system, but swings far out of it. More objects with similar orbits have been discovered since.

"The discovery of DeeDee is a promising sign of our ability to find distant new worlds," Gerdes said. "If more things like this are in our data, the tools we've built will find them."

But on its own, the new discovery tells us a bit more about where we came from.

"All the bodies that make up our solar system came from the same cloud of gas and dust that began to collapse over 4 billion years ago," said Stephanie Hamilton, a doctoral student in physics who was involved in this discovery.

"The smallest bodies in the solar system are the ones that preserve its history. They have been knocked around and strewn about through interactions with larger planets, and by studying lots of them we can try to learn how that happened."

The Dark Energy Survey
The Dark Energy Survey is a collaboration of more than 400 scientists from 26 institutions in seven countries. Its primary instrument, the 570-megapixel Dark Energy Camera, is mounted on the 4-meter Blanco telescope at the National Optical Astronomy Observatory's Cerro Tololo Inter-American Observatory in Chile, and its data are processed at the National Center for Supercomputing Applications at the University of Illinois.

Funding for the DES Projects has been provided by the U.S. Department of Energy Office of Science, U.S. National Science Foundation, Ministry of Science and Education of Spain, Science and Technology Facilities Council of the United Kingdom, Higher Education Funding Council for England, ETH Zurich for Switzerland, National Center for Supercomputing Applications at the University of Illinois, Kavli Institute of Cosmological Physics at the University of Chicago, Center for Cosmology and Astro-Particle Physics at Ohio State University, Mitchell Institude for Fundamental Physics and Astronomy at Texas A&M University, Financiadora de Estudos e Projetos, Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro, Conselho Nacional de Desenvolvimento Científico e Tecnológico and the Ministério da Ciência e Tecnologia, Deutsche Forschungsgemeinschaft and collaborating institutions in the Dark Energy Survey, the list of which can be found at www.darkenergysurvey.org/collaboration.

The search for solar system objects in DES is funded by a National Science Foundation grant to researchers at the University of Michigan and the University of Pennsylvania.

 

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