Universe Today

Frozen in time, ancient microbes or their remains could be found in Martian ice deposits during future missions to the red planet. By recreating Mars-like conditions in the lab, a team of researchers from NASA Goddard Space Flight Center and Penn State demonstrated that fragments of the molecules that make up proteins in E. coli bacteria, if present in Mars' permafrost and ice caps, could remain intact for over 50 million years, despite harsh and continuous exposure to cosmic radiation.

In a recent study, theoretical physicists at Goethe University Frankfurt described the origin of powerful jets emanating from the core regions of galaxies using a series of complex simulations.

Use cases for smart materials in space exploration keep cropping up everywhere. They are used in everything from antenna deployments on satellites to rover deformation and reformation. One of the latest ideas is to use them to transform the solar sails that could primarily be used as a propulsion system for a mission into a heat shield when that mission reaches its final destination. A new paper from Joseph Ivarson and Davide Guzzetti, both of Auburn’s Department of Aerospace Engineering, and published in Acta Astronautica, describes how the idea might work and lists some potential applications exploring various parts of the solar system.

Rather randomly I’ve just returned from a theatre tour where my science show featured yeast in one of the experiments, so when research about yeast surviving Martian conditions crossed my desk, it immediately piqued my interest. These microscopic fungi that help our bread rise and our beer ferment might just have what it takes to endure one of the Solar System's harshest environments.

Mars is a planet of mystery! Its surface today is cold and dry, yet evidence suggests it was once home to flowing water. Most of the planet's remaining ice sits locked away at the poles, but recent observations have detected signals of hydrogen in equatorial regions that could indicate buried ice deposits where the environment should be too warm for ice to survive. How did frozen water end up at Mars's equator? It seems we might find the answer in Martian volcanoes.

White dwarfs are stellar corpses, the slowly cooling remnants of stars that ran out of fuel billions of years ago. Our Sun will eventually share this fate, collapsing into a compact object so dense that the heavier it becomes, the smaller it shrinks. This rather strange property is just one of the aspects of white dwarfs that makes them utterly fascinating and occasionally, utterly baffling. Sometimes we find white dwarfs as part of binary systems and they are usually cool and gently radiating their energy out into space. A team of astronomers have recently discovered a peculiar class of these binary systems that defies expectations. The pair of white dwarfs are orbiting each other faster than once per hour and exhibiting temperatures between 10,000 and 30,000 degrees Kelvin, significantly hotter than expected and twice their usual size.

It rains on the Sun! Although not in any way we'd recognise from Earth. In the Sun's corona, the superheated atmosphere that extends millions of kilometres above its visible surface, cooler blobs of plasma occasionally form and fall back downward in what astronomers are calling coronal rain. Until now, the mechanism behind the rain has remained a mystery especially during solar flares where it seems to accelerate but researchers at the University of Hawaii Institute for Astronomy have finally cracked the puzzle.

Scientists have begun to piece together the origin story of a cataclysmic collision between two black holes that met their fate on an unusual orbital path. The merger, designated GW200208_222617 (that really rolls of the tongue,) stands out among gravitational wave detections as one of the rare events showing clear signs of orbital eccentricity, meaning the black holes followed a squashed, oval shaped orbit rather than a circular one as they spiralled toward their final encounter.

Impulse Space, the California-based venture founded by veteran SpaceX engineer Tom Mueller, has unveiled its proposed architecture for delivering medium-sized payloads to the moon, starting as early as 2028.

Modularity is taking off in more ways than one in space exploration. The design of the upcoming “Lunar Gateway” space station is supposed to be modular, with different modules being supplied by different organizations. In an effort to extend that thinking down to rovers on the ground, a new paper from researchers at Germany’s space agency (DLR), developed an architecture where a single, modular rover could be responsible for both exploration and carrying payloads around the Moon or Mars.

It’s great to see old astronomical observations come to light. Not only can these confirm or refute what’s known about historic astronomical events, but they can describe what early observers actually saw. A recent study cites two Arabic texts that may refer to accounts of two well-known supernovae seen in our galaxy: one in 1006 AD and another in 1181 AD.

We know lots about our Galaxy yet still, some regions still hold countless secrets. Recently, a team of astronomers using South Africa's MeerKAT radio telescope uncovered 164 of them, compact radio rings. Each one smaller than an arcminute across, were hiding along the plane of the Milky Way, and were just waiting for a telescope powerful enough to reveal them.

For millions of years, a fragment of ice and dust drifted through interstellar space, its origin, a distant planetary system. This summer, that fragment finally entered our Solar System, becoming only the third confirmed interstellar visitor and earning the designation 3I/ATLAS. When astronomers at Auburn University pointed NASA's Swift Observatory toward this icy chunk, they detected water vapour streaming from its surface. It was revealed through the faint ultraviolet glow of hydroxyl molecules and was completely unexpected.

SpaceX closed out a dramatic chapter in the development of its super-heavy-lift Starship launch system with a successful flight test that mostly followed the script for the previous flight test.

Earth's atmosphere has always been the enemy of ground based astronomy and don’t I know it. What would otherwise be crisp, clean datasets gets turned into blurry smudges. Space telescopes avoid the problem entirely but can only photograph tiny fragments of sky. Now, a team of mathematicians has cracked the code with an elegant algorithm that strips away atmospheric interference in seconds, potentially giving ground based observatories space quality vision whilst keeping their ability to survey great regions of sky.

When I spotted a headline about Earth's ancient oceans and urea, my brain immediately went to the obvious place. Urea, the same compound found in urine. Yes, scientists are telling us that a component of wee played a crucial role in one of the most important events in our planet's history. Sometimes science really does have a sense of humour.

Avoiding, or at least limiting the damage from, geomagnetic storms is one of the most compelling arguments for why we should pay attention to space. Strong solar storms can have an impact on everything from air traffic to farming, and we ignore them at our own peril and cost. Despite that threat, the tools that we have applied to tracking and analyzing them have been relatively primitive. Both simulations and the physical hardware devoted to it require an upgrade if we are to accurately assess the threat a solar storm poses. As a first step, a new paper from a group led by researchers at the University of Michigan created a much more detailed simulation that shows how important it is that we also have the appropriate sensing hardware in place to detect these storms as they happen.

In a newly published novel titled “Hole in the Sky,” Cherokee science-fiction author Daniel H. Wilson blends Native American tales about alien civilizations with up-to-date speculation about UFOs, now also known as unidentified anomalous phenomena or UAPs.

For decades, the dramatic difference between the Moon's two faces has been the subject of much debate. Now, a fresh look at the Moon's largest and oldest impact crater has revealed something quite unexpected. The asteroid that formed it seems to have hit from the opposite direction than everyone thought, and it created a radioactive splash zone that may finally explain the mystery. Even better, NASA's Artemis astronauts are about to land right in the middle of it.

When two galaxies merge, the supermassive black holes at their centres should eventually find each other and begin a gravitational dance that lasts millions of years. Despite decades of predictions, astronomers are still hunting for definitive proof these binary systems exist. A new review examines the clues scattered across the universe, from wobbling jets spanning hundreds of thousands of light years to specific spectral signatures, and explores why finding these black hole pairs matters for understanding both the past and future of our own Galaxy.