All the news about DES that’s fit to print!
The paper’s authors describe the new object as the “most extreme” Trans-Neptunian Object “discovered to date.” In plain English, that means it has the wonkiest orbit of any object past Neptune.
The new object was discovered using data from The Dark Energy Survey, an ongoing project investigating the expansion of our universe by looking deep into space.
The planets we know about all orbit the sun at the same angle, called the orbital plane, because of the sun’s gravitational pull. Because The Dark Energy Survey is examining a different plane, scientists did not expect to find any orbiting objects in the data.
The orbit of 2015 BP519 is tilted 54 degrees from our orbital plane, according to the paper. A likely explanation is that a giant ghost planet is tilting the object’s orbit.
Models suggest it would take this hypothetical Planet Nine 10,000 to 20,000 years to complete one rotation around the sun.
Two years ago, scientists from the California Institute of Technology (Caltech) found evidence to suggest that a mysterious planet larger than Earth could be hiding beyond the orbit of Pluto, in the furthest reaches of the Solar System.
While the researchers didn’t directly observe the hypothetical ninth planet—otherwise known as Planet Nine—they did predict its existence based on the strange orbits of a handful of so-called Trans-Neptunian objects (TNOs)—distant, icy worlds located beyond the orbit of Neptune. These TNOs are clustered together in a way that is extremely unlikely to have occurred by chance, indicating the presence of a planet-sized object that is influencing their orbits through its gravitional pull, the theory goes.
Since this discovery, scientists around the world have scrambled to investigate the predictions, but Planet Nine has remained elusive. Now, an international team of researchers has reported the discovery of another distant world with an extraordinary orbit—referred to as 2015 BP519—which, they say, bolsters the case for the ninth planet.
In a new paper, published on the online preprint server arXiv.org, the team described how it uncovered the space object in 2014 using data from the Dark Energy Survey (DES)—an international, collaborative effort to map a vast region of the skies and reveal the nature of the mysterious force that is accelerating the expansion of the universe, known as dark energy.
Astronomers have lost track of nearly 900 asteroids that could be on a deadly collision course with Earth
These space rocks, which orbit uncomfortably close to our planet, were spotted just once by scientists.
Researchers were unable to continue tracking them, which means they have no way of knowing if they are on a collision course with Earth.
Despite fears they could smash into Earth, experts say there is a ‘low chance’ of of surprise near-Earth asteroids causing damage.
To make their finding the team looked at data from some of Earth’s most prolific asteroid hunting systems, including Pan-STARRS, the Catalina Sky Survey, the Dark Energy Survey, and the Space Surveillance Telescope.
In early 2016, two planetary scientists declared that a ghost planet is hiding in the depths of the solar system, well beyond the orbit of Pluto. Their claim, which they made based on the curious orbits of distant icy worlds, quickly sparked a race to find this so-called Planet Nine — a planet that is estimated to be about 10 times the mass of Earth. “It has a real magnetism to it,” said Gregory Laughlin, an astronomer at Yale University. “I mean, finding a 10-Earth-mass planet in our own solar system would be a discovery of unrivaled scientific magnitude.”
Gerdes and his colleagues spotted the new object in data from the Dark Energy Survey, a project that probes the acceleration in the expansion of the universe by surveying a region well above the plane of the solar system. This makes it an unlikely tool for finding objects inside the solar system, since they mostly orbit within the plane. But that is exactly what makes the new object unique: Its orbit is tilted 54 degrees with respect to the plane of the solar system. It’s something Gerdes did not expect to see. Batygin and Brown, however, predicted it.
Brian Nord works in the deep skies lab on gravitational lensing at Fermilab. A gravitational lens is formed between a distant light source and an observer that bends the light from the source as it travels towards the observer. The amount of bending is one of the predictions of Albert Einstein’s general theory of relativity. Researchers can also use “lensing” as a measurement of how much dark matter there is in the universe. Between 1979 and now, only 1,000 such “lenses” have been discovered, but they predict significantly more of these observations will be found. The Dark Energy Survey (DES) uses the dark energy camera, and is predicted to have over 2,000 galaxy scale lenses in this survey. LSST was hinted to find potentially 120,000 of these types of events. This team also didn’t want to reinvent the wheel, and they also turned to AI techniques to help them. Using deep learning they found 8 new confirmed lenses, by looking at 100’s of square degrees of images. They use “ensembles of networks” and then use a simple majority vote to decide on which are lenses and which are not lenses. This specific technique of “jury vote” or consensus prediction is becoming very popular in a variety of fields to improve the quality of AI systems.
A supernova is one of the most impressive natural phenomena in the Universe. Unfortunately, such events are often brief and transient, temporarily becoming as bright as an entire galaxy and then fading away. But given what these bright explosions – which occur when a star reaches the end of its life cycle – can teach us about the Universe, scientists are naturally very interested in studying them.
Using data from the Dark Energy Survey Supernova (DES-SN) program, a team of astronomers recently detected 72 supernovae, the largest number of events discovered to date. These supernovae were not only very bright, but also very brief – a finding which the team is still struggling to explain. The results of their study were presented on Tuesday, April 3rd, at the European Week of Astronomy and Space Science in Liverpool.
The team was led by Miika Pursiainen, a PhD researcher from the University of Southampton. For the sake of their study, the team relied on data from the 4-meter telescope at the Cerro Tololo Inter-American Observatory (CTIO). This telescope is part of the Dark Energy Survey, a global effort to map hundreds of millions of galaxies and thousands of supernovae in to find patterns int he cosmic structure that will reveal the nature of dark energy.
Professor Bob Nichol and Dr David Bacon, from the Institute of Cosmology and Gravitation, have played key roles in the Dark Energy Survey (DES).
Kick-started in 2003, the project has united more than 400 scientists from institutions in the United States, the United Kingdom, Brazil, Spain, Germany, Switzerland and Australia. And together, with internationally-sourced government and university funding, this crack team has built and used a 570-megapixel digital camera to carry out a deep probe of 5,000 square degrees – or one eighth – of the southern sky.
Scientists working on the Dark Energy Survey (DES), an international project mapping a few hundred million distant galaxies to learn more about dark energy, discovered the most distant supernova ever detected.
Designated DES16C2nm, the supernova took place 10.5 billion years ago when a massive star exploded at the end of its life. It is classed as a superluminous supernova (SLSN), the brightest and most rare of all supernovae.
“Such supernovae were not thought of when we started DES over a decade ago,” explained Bob Nichol, Director of the Institute of Cosmology and Gravitation at the University of Portsmouth in the UK.
“Such discoveries show the importance of empirical science; sometimes, you just have to go out and look up to find something amazing.”
Mathew Smith of the University of Southampton, also in the UK, and lead author of a paper on the findings published in the Astrophysical Journal, noted the rare finding gives astronomers better understanding of the rare superluminous supernovae.
The colossal cosmic blast happened only 3.3billion years after the Big Bang, when the universe was a quarter of its current age, and light from the supernova has taken 10.5billion years to reach Earth – the Universe itself is thought to be 13.8billion years old.
The supernova, named DES16C2nm, was identified by a team led by Southampton University for the Dark Energy Survey (DES) – an international collaboration mapping far-off galaxies.
The team confirmed it is a superluminous supernova (SLSN) which is the brightest and rarest class and up to 100 times brighter than other types of stellar blasts.
Lead author Dr Mathew Smith said: “DES16C2nm is extremely distant, extremely bright and extremely rare – not the sort of thing you stumble across every day as an astronomer.
“It’s thrilling to be part of the survey that has discovered the oldest known supernova.
“As well as being a very exciting discovery in its own right the extreme distance of DES16C2nm gives us a unique insight into the nature of SLSN.”
An international team of astronomers has discovered the oldest supernova ever detected — a huge cosmic explosion that took place 10.5 billion years ago. A supernova is the explosion of a massive star at the end of its life cycle.
The exploding star, named DES16C2nm, was detected by the Dark Energy Survey (DES), an international collaboration to map several hundred million galaxies in order to find out more about dark energy — the mysterious force believed to be causing the accelerated expansion of the universe.
As detailed in a new study published in The Astrophysical Journal, light from the event has taken 10.5 billion years to reach Earth, making it the oldest supernova ever discovered and studied.