Astronomers accidentally discovered the footprints of a monster galaxy in the early universe that has never been seen before. Like a cosmic Yeti, the scientific community generally regarded these galaxies as folklore
Researchers have completed the first-ever, in-depth investigation into how an asteroid would respond to a nuclear deflection attempt, finding that a nuclear device would be able to deflect an asteroid too massive for other approaches. The paper was published by Acta Astronautica on Oct. 15.
Quarks and gluons are elementary particles that make up everything you see before you, including yourself, and Nobuo Sato wants to know how. At the Department of Energy's Thomas Jefferson National Accelerator Facility, he will be tackling this question as the recipient of the JSA/Jefferson Lab Nathan Isgur Fellowship for Nuclear Theory.
At the AVS 66th International Symposium and Exhibition, Oct. 20-25, Daniel Gunlycke will present a study on using symmetry to reduce the effects of random quantum entanglement in quantum computing applications. When deliberate, quantum entanglement can make algorithms more powerful and efficient, but uncontrolled entanglement adds unnecessary additional complexity to quantum computing, making algorithms suboptimal and more prone to error. Gunlycke says by reducing the frequency of accidental entanglements, quantum computing can be improved.
A team led by a University of Hawaii at Manoa chemistry professor and researcher has been able to provide answers to key questions about the surface of Saturn's moon Titan.
This study is the first to confirm dust particles pre-dating the formation of our solar system. Further study of these materials will enable a deeper understanding of the processes that formed and have since altered them.
For the first time, astronomers using ALMA have witnessed 3D motions of gas in a planet-forming disk. At three locations in the disk around a young star called HD 163296, gas is flowing like a waterfall into gaps that are most likely caused by planets in formation. These gas flows have long been predicted and would directly influence the chemical composition of planet atmospheres. This research is published in the latest issue of the journal Nature.
Scientists from the U.S. Department of Energy's (DOE) Brookhaven National Laboratory have garnered two out of five "Distinguished Scientists Fellow" awards announced today by the DOE's Office of Science. Theoretical physicist Sally Dawson, a world-leader in calculations aimed at describing the properties of the Higgs boson, and José Rodriguez, a renowned chemist exploring and developing catalysts for energy-related reactions, will each receive $1 million in funding over three years to pursue new research objectives within their respective fields.
Hubble has taken the sharpest view to date of interstellar comet 2I/Borisov whose speed and trajectory indicate it has come from beyond our solar system. The image, taken October 12, 2019, reveals a central concentration of dust around the comet's nucleus.
Los Alamos National Laboratory scientists Brian Albright, Patrick Chain, Dana Dattelbaum, Michael Hamada, Anna Hayes-Sterbenz, Michael Prime and Laura Smilowitz are being honored as 2019 Laboratory fellows.
At the center of a galaxy called NGC 1068, a supermassive black hole hides within a thick doughnut-shaped cloud of dust and gas. When astronomers used the Atacama Large Millimeter/submillimeter Array (ALMA)
to study this cloud in more detail, they made an unexpected discovery that could explain why supermassive black holes grew so rapidly in the early Universe.
“Thanks to the spectacular resolution of ALMA, we measured the movement of gas in the inner orbits around the black hole,” explains Violette Impellizzeri of the National Radio Astronomy Observatory (NRAO), working at ALMA in Chile and lead author on a paper published in the Astrophysical Journal. “Surprisingly, we found two disks of gas rotating in opposite directions.”
The entry probe of the Galileo mission to Jupiter entered the planet’s atmosphere in 1995 in fiery fashion, generating enough heat to cause plasma reactions on its surface. The data relayed about the burning of its heat shield differed from the effects predicted in fluid dynamics models, and new work examines what might have caused such a discrepancy.
Astronomers at the University of California, Riverside, have discovered that powerful winds driven by supermassive black holes in the centers of dwarf galaxies have a significant impact on the evolution of these galaxies by suppressing star formation.
After its 2021 launch, NASA's James Webb Space Telescope will gather infrared light that has penetrated the dusty veil, revealing the galactic center in unprecedented detail.
The University of Delaware's Swati Singh is using quantum systems to understand astrophysical phenomena and has been awarded a National Science Foundation grant to advance her work.
In a certain sense, physics is the study of the universe’s symmetries. Physicists strive to understand how systems and symmetries change under various transformations.New research from Washington University in St. Louis realizes one of the first parity-time (PT) symmetric quantum systems, allowing scientists to observe how that kind of symmetry — and the act of breaking of it — leads to previously unexplored phenomena.
The surface of Mars was once home to shallow, salty ponds that went through episodes of overflow and drying, according to a paper published today in Nature Geoscience.
A team of scientists, including a researcher from Queen’s University Belfast, have discovered that the fading of infrared light following Type Ia supernovae explosions can be interrupted, with brightness staying the same for up to a year.
The first international mission in the University of North Dakota’s Inflatable Mars/Lunar Habitat (IMLH) was launched Wednesday afternoon when four students from Argentina, Colombia, Mexico and Peru entered the facility to spend two weeks running experiments to help NASA with exploring the moon and Mars.
The two baby stars were found in the [BHB2007] 11 system - the youngest member of a small stellar cluster in the Barnard 59 dark nebula, which is part of the clouds of interstellar dust called the Pipe nebula.
While high-energy physics and cosmology seem worlds apart in terms of sheer scale, physicists and cosmologists at Argonne are using similar machine learning methods to address classification problems for both subatomic particles and galaxies.
An international team of astronomers with participation by researchers from DAWN, Niels Bohr Institute, University of Copenhagen has discovered a protocluster of galaxies 13.0 billion light years away using the Subaru, Keck, and Gemini Telescopes in Hawaii.
Astronomers have uncovered two historic events in which the Andromeda Galaxy underwent major changes to its structure. The findings shed light not only on the evolution and formation of the Andromeda Galaxy, but to our own Milky Way Galaxy as well. Two of the facilities in NSF's National Optical-Infrared Astronomy Research Laboratory, Kitt Peak National Observatory and the International Gemini Observatory, played critical roles in the research, now published in the latest issue of the journal Nature.
On 1 October 2019, the nighttime astronomy facilities supported by the National Science Foundation (NSF) transitioned to operating as one organization, NSF's National Optical-Infrared Astronomy Research Laboratory. The new organization operates five scientific programs: Cerro Tololo Inter-American Observatory, the Community Science and Data Center, Kitt Peak National Observatory (all formerly known as the National Optical Astronomy Observatory); Gemini Observatory and the upcoming Large Synoptic Survey Telescope, and is managed by the Association of Universities for Research in Astronomy.
When he was growing up, Jonathan LeyVa thought he’d follow his passion for race cars and pick a profession in automotive engineering. Instead he’s working on what will become one of the world’s most sensitive searches for dark matter, the invisible substance that accounts for more than 85 percent of the mass of the universe.
The red dwarf GJ 3512 is located 30 light-years from us. Although the star is only about a tenth of the mass of the Sun, it possesses a giant planet - an unexpected observation.
An experiment shows that one of the basic units of life -- nucleobases -- could have originated within giant gas clouds interspersed between the stars.
Missouri University of Science and Technology has joined the Hobby-Eberly Telescope Dark Energy Experiment (HETDEX) as one of 11 international institutions that are collaborating to define the force causing the accelerated expansion of the universe.
The ATLAS experiment at CERN’s Large Hadron Collider (LHC) is ready to begin another chapter in its search for new physics. A significant upgrade to the experiment, called the U.S. ATLAS Phase I Upgrade, has received Critical Decision-4 approval from the U.S. Department of Energy (DOE), signifying the completion of the project and a transition to operations.
Shortly after its launch in 2021, NASA’s James Webb Space Telescope will observe three different types of comets to learn more about them and about the early solar system.
A hypothetical nuclear process known as neutrinoless double beta decay ought to be among the least likely events in the universe. Now the international EXO-200 collaboration, which includes researchers from the Department of Energy’s SLAC National Accelerator Laboratory, has determined just how unlikely it is: In a given volume of a certain xenon isotope, it would take more than 35 trillion trillion years for half of its nuclei to decay through this process – an eternity compared to the age of the universe, which is “only” 13 billion years old.
Barbara Garcia, a Science Undergraduate Laboratory Internship program participant, used the resourcefulness and independence she acquired as a first-generation college student during her summer of research at the Princeton Plasma Physics Laboratory.
Profiled is physicist Gaute Hagen of the Department of Energy’s Oak Ridge National Laboratory, who runs advanced models on powerful supercomputers to explore how protons and neutrons interact to “build” an atomic nucleus from scratch.
Barnes, a UW assistant professor of astrobiology, astronomy and data science, released the first version of VPLanet, his virtual planet simulator, in August. He and his co-authors described it in a paper accepted for publication in the Proceedings of the Astronomical Society of the Pacific.
About 466 million years ago, long before the age of the dinosaurs, the Earth froze. The seas began to ice over at the Earth's poles, and the new range of temperatures around the planet set the stage for a boom of new species evolving.
Berkeley Lab is one of five sites around the globe that is building detector panels for an upgrade project that will improve the performance of a particle detector’s inner tracking system – including its resolution to take snapshots of particle collisions, its durability, and data-collection speed.
An interdisciplinary research team has received a $1 million, two-year grant from the National Science Foundation (NSF) under the “Harnessing the Data Revolution” initiative, to develop computational methods to accelerate data-intensive discovery in astroparticle physics — an important step toward understanding dark matter.
An international team of 30 scientists—led by researchers at McMaster University—is using one of the world’s largest telescopes to investigate and map extreme galaxy environments in brilliant detail.
At the 2019 Topics in Astroparticle and Underground Physics conference in Toyama, Japan, leaders from the KATRIN experiment reported Sept. 13 that the estimated range for the rest mass of the neutrino is no larger than 1 electron volt, or eV.