SWIFT: A modern highly-parallel gravity and smoothed particle hydrodynamics solver for astrophysical and cosmological applications Matthieu Schaller (Lorentz Institute & Leiden Observatory), Josh Borrow, Peter W. Draper, Mladen Ivkovic, Stuart McAlpine, Bert Vandenbroucke, Yannick Bah’e, Evgenii Chaikin, Aidan B. G. Chalk, Tsang Keung Chan, Camila Correa, Marcel van Daalen, Willem Elbers, Pedro Gonnet, Lo"ic Hausammann, John Helly, Filip Huv{s}ko, Jacob A. Kegerreis, Folkert S. J. Nobels, Sylvia Ploeckinger, Yves Revaz, William J. Roper, Sergio Ruiz-Bonilla, Thomas D. Sandnes, Yolan Uyttenhove, James S. Willis, Zhen Xiang arXiv:2305.13380v2 Announce Type: replace Abstract: Numerical simulations have become one of the key tools used by theorists in all theRead More →

21-cm fluctuations from primordial magnetic fields Hector Afonso G. Cruz, Tal Adi, Jordan Flitter, Marc Kamionkowski, Ely D. Kovetz arXiv:2308.04483v2 Announce Type: replace Abstract: The fluid forces associated with primordial magnetic fields (PMFs) generate small-scale fluctuations in the primordial density field, which add to the $mathrm{Lambda CDM}$ linear matter power spectrum on small scales. These enhanced small-scale fluctuations lead to earlier formation of galactic halos and stars and thus affect cosmic reionization. We study the consequences of these effects on 21 cm observables using the semi-numerical code 21cmFAST v3.1.3. We find the excess small-scale structure generates strong stellar radiation backgrounds in the early Universe, resultingRead More →

EIGER V. Characterizing the Host Galaxies of Luminous Quasars at $zgtrsim6$ Minghao Yue, Anna-Christina Eilers, Robert A. Simcoe, Ruari Mackenzie, Jorryt Matthee, Daichi Kashino, Rongmon Bordoloi, Simon J. Lilly, Rohan P. Naidu arXiv:2309.04614v2 Announce Type: replace Abstract: We report {em JWST}/NIRCam measurements of quasar host galaxy emissions and supermassive black hole (SMBH) masses for six quasars at $5.9arXiv:2309.04614v2 Announce Type: replace Abstract: We report {em JWST}/NIRCam measurements of quasar host galaxy emissions and supermassive black hole (SMBH) masses for six quasars at $5.9Read More →

Astronomaly at scale: searching for anomalies amongst 4 million galaxies Verlon Etsebeth, Michelle Lochner, Mike Walmsley, Margherita Grespan arXiv:2309.08660v2 Announce Type: replace Abstract: Modern astronomical surveys are producing datasets of unprecedented size and richness, increasing the potential for high-impact scientific discovery. This possibility, coupled with the challenge of exploring a large number of sources, has led to the development of novel machine-learning-based anomaly detection approaches, such as Astronomaly. For the first time, we test the scalability of Astronomaly by applying it to almost 4 million images of galaxies from the Dark Energy Camera Legacy Survey. We use a trained deep learning algorithm to learn usefulRead More →

Extremophiles: Why study them? What can they teach us about finding life beyond Earth? Universe Today has conducted some incredible examinations regarding a plethora of scientific fields, including impact craters, planetary surfaces, exoplanets, astrobiology, solar physics, comets, planetary atmospheres, planetary geophysics, cosmochemistry, meteorites, and radio astronomy, and how these disciplines can help scientists and the public gain greater insight into searching for life beyond Earth. Here, we will discuss the immersive field of extremophiles with Dr. Ivan Paulino-Lima, who is a Senior Research Investigator at Blue Marble Space Institute of Science and the Co-Founder and Chief Science Officer for Infinite Elements Inc., including why scientists study extremophiles, the benefits and challenges, finding lifeRead More →

It Takes a Supercomputer to Properly Simulate a Neutron Star’s Surface Neutron stars, the remains of massive stars that have imploded and gone supernova at the end of their life, can still create massive flares. These incredible bursts of energy release X-rays that propagate through space. It is a complex process to simulate but astronomers have turned to a supercomputer to help. Modelling the twisting magnetic fields, the interaction with gas and dust, the surface of flaring neutron stars has been revealed in incredible 3D. Throughout a stars life, the inward force of gravity is balanced by the outward pushing thermonuclear force. Stars like ourRead More →

Against all Odds. Japan’s SLIM Lander Survived a Second Lunar Night Upside Down You might remember the SLIM lunar lander that managed to land upside-down! The probe from the Japanese Space Agency has survived its second night on the Moon and returns a new photograph. Despite the solar panels pointing away from the Sun during the day it was still able to capture the image and transmit to Earth. All that while surviving the harsh -130C lunar night.  The Japanese Space Agency (JAXA) sent SLIM (the Smart Lander for Investigating the Moon) back in January but the lightweight spacecraft landed completely wrong. Despite the wonkyRead More →

Radio Astronomy: Why study it? What can it teach us about finding life beyond Earth? Universe Today has investigated the significance of studying impact craters, planetary surfaces, exoplanets, astrobiology, solar physics, comets, planetary atmospheres, planetary geophysics, cosmochemistry, and meteorites, and how these scientific fields contribute to researchers and the public gain greater insight into our place in the universe and finding life beyond Earth. Here, will discuss the field of radio astronomy with Dr. Wael Farah, who is a research scientist at the SETI Institute, about how radio astronomy teaches us about the myriad of celestial objects that populate our universe, along with the benefits and challenges, finding life beyond Earth, andRead More →

The Search for the Perfect Coronagraph to Find Earth 2.0 Studying exoplanets is made more difficult by the light from the host star. Coronagraphs are devices that block out the star light and both JWST and Nancy Grace Roman Telescope are equipped with them. Current coronagraphs are not quite capable of seeing other Earths but work is underway to push the limits of technology and even science for a new, more advanced device. A new paper explores the quantum techniques that may one day allow us to make such observations.  Coronagraphs are devices that attach to telescopes and were originally designed to study the coronaRead More →

A Supermassive Black Hole with a Case of the Hiccups Can binary black holes, two black holes orbiting each other, influence their respective behaviors? This is what a recent study published in Science Advances hopes to address as a team of more than two dozen international researchers led by the Massachusetts Institute of Technology (MIT) investigated how a smaller black hole orbiting a supermassive black hole could alter the outbursts of the energy being emitted by the latter, essentially giving it “hiccups”. This study holds the potential to help astronomers better understand the behavior of binary black holes while producing new methods in finding moreRead More →

Meteorites: Why study them? What can they teach us about finding life beyond Earth? Universe Today has explored the importance of studying impact craters, planetary surfaces, exoplanets, astrobiology, solar physics, comets, planetary atmospheres, planetary geophysics, and cosmochemistry, and how this myriad of intricately linked scientific disciplines can assist us in better understanding our place in the cosmos and searching for life beyond Earth. Here, we will discuss the incredible research field of meteorites and how they help researchers better understand the history of both our solar system and the cosmos, including the benefits and challenges, finding life beyond Earth, and potential routes for upcoming studentsRead More →

China’s Relay Satellite is in Lunar Orbit On March 20th, China’s Queqiao-2 (“Magpie Bridge-2”) satellite launched from the Wenchang Space Launch Site LC-2 on the island of Hainan (in southern China) atop a Long March-8 Y3 carrier rocket. This mission is the second in a series of communications relay and radio astronomy satellites designed to support the fourth phase of the Chinese Lunar Exploration Program (Chang’e). On March 24th, after 119 hours in transit, the satellite reached the Moon and began a perilune braking maneuver at a distance of 440 km (~270 mi) from the lunar surface. The maneuver lasted 19 minutes, after which theRead More →

The Hubble Aims Its Powerful Ultraviolet Eye at Super-Hot Stars Some stars are so massive and so energetic that they’re a million times brighter than the Sun. This type of star dominated the early Universe, playing a key role in its development and evolution. The first of its kind are all gone now, but the modern Universe still forms stars of this type. These hot, blue stars emit powerful ultraviolet energy that the Hubble can detect from its perch in Low-Earth Orbit. In December 2023, astronomers completed a three-year survey of these hot stars. It’s one of the Hubble’s largest and most ambitious surveys. It’sRead More →

Search for Life on Mars Could Level-Up with MARSE Mission Concept A recent study presented at the 55th Lunar and Planetary Science Conference (LPSC) discusses the Mars Astrobiology, Resource, and Science Explorers (MARSE) mission concept and its Simplified High Impact Energy Landing Device (SHIELD), which offers a broader and cheaper method regarding the search for—past or present—life on the Red Planet, specifically by using four rovers at four different landing sites across Mars’ surface instead of just one-for-one. This concept comes as NASA’s Curiosity and Perseverance rovers continue to tirelessly explore the surface of Mars at Gale Crater and Jezero Crater, respectively. Here, Universe TodayRead More →

The Milky Way’s Smallest, Faintest Satellite Galaxy Found The Milky Way has many satellite galaxies, most notably the Large and Small Magellanic Clouds. They’re both visible to the naked eye from the southern hemisphere. Now astronomers have discovered another satellite that’s the smallest and dimmest one ever detected. It may also be one of the most dark matter-dominated galaxies ever found. The galaxy is called Ursa Major III / UNIONS 1 (UMa3/U1), and it contains very few stars. In fact, its luminosity is so low that it’s gone undetected until new, even though it’s in our neighbourhood. The discovery is in a new paper titledRead More →

Thermal Modeling of a Pulsed Plasma Rocket Shows It Should Be Possible To Create One We’ve reported on a technology called pulsed plasma rockets (PPRs) here at UT a few times. Several research groups have worked on variations of them. They are so popular partly because of their extremely high specific impulse and thrust levels, and they seemingly solve the trade-off between those two all-important variables in space exploration propulsion systems. Essentially, they are an extremely efficient propulsion methodology that, if scaled up, would allow payloads to reach other planets in weeks rather than months or years. However, some inherent dangers still need to beRead More →

Civilizations Could Time Their Communications Based on the Movement of a Single Star The Search for Extraterrestrial Intelligence has been ongoing for decades at this point. Despite that, we have yet to find any rock-hard evidence of a signal from an alien civilization. When asked about this, experts point out just how little of the overall signal space we’ve analyzed. A signal could be coming from anywhere in the sky, at any frequency, and might not be continuous. Constraining the “search space” could help us find a signal faster, but what could we use to constrain it? It’s hard to think like an alien intelligence,Read More →

Astronomers only knew of a single binary Cepheid system—they just found nine more Measuring the distance to far away objects in space can be tricky. We don’t even know the precise distance to even our closest neighbors in the universe—the Small and Large Magellanic Clouds. But, we’re starting to get to the tools to measure it. One type of tool is a Cepheid Variable—a type of star that varies its luminosity in a well-defined pattern. However, we don’t know much about their physical properties, making utilizing them as distance markers harder. phys.org Go to SourceRead More →