Space News & Blog Articles

Tracking down resources on the Moon is a critical process if humanity decides to settle there permanently. However, some of our best resources to do that currently are orbiting satellites who use various wavelengths to scan the Moon and determine what the local environment is made out of. One potential confounding factor in those scans is “space weathering” - i.e. how the lunar surface might change based on bombardment from both the solar wind and micrometeroid impacts. A new paper from a researchers at the Southwest Research Institute adds further context to how to interpret ultra-violet data from one of the most prolific of the resource assessment satellites - the Lunar Reconnaissance Orbiter (LRO) - and unfortunately, the conclusion they draw is that, for some resources such as titanium, their presence might be entirely obscured by the presence of “old” regolith.

Radio astronomy has a pollution problem. Satellites thousands of kilometres overhead, designed to broadcast communications or relay data, are increasingly contaminating the frequencies astronomers use to study the universe. While much attention has focused on SpaceX's Starlink and other low Earth orbit constellations, but what about the satellites much farther away?

(This is Part 1 of a series exploring the mythic side of the Big Bang!)

When astronauts finally set foot on Mars, they'll arrive carrying the weight of centuries of speculation about whether life exists beyond Earth. Now a new report from the National Academies has settled a fundamental question about priorities: searching for evidence of past or present Martian life should be the primary science objective for humanity's first crewed mission to the red planet, ranking above all other scientific goals including understanding the effects of Mars on human health.

On July 1st, 2025, the third interstellar object (ISO) ever detected was seen making its way through our Solar System. Shortly after being alerted by automated detection systems, astronomers at the European Space Agency (ESA) began using observatories in Hawaii, Chile, and Australia to get a better look at the interstellar interloper. Since then, 3I/ATLAS has been observed by multiple space observatories, including the venerable NASA/ESA Hubble Space Telescope. On Nov. 30th, Hubble viewed the ISO again, which is about to make its closest approach to Earth.

What could force a supermassive black hole (SMBH) out of its host galaxy? They can have hundreds of millions, even billions of solar masses? What's powerful enough to dislodge one of these behemoths?

The Hubble Tension is one of the great mysteries of cosmology. Solving it might require a fundamental change in how we understand the universe - but scientists have to prove it actually exists first. A new paper from a collective of cosmologist researchers known as the TDCOSMO Collaboration adds further fuel to that first with updated measurements of the “Late Universe” measurement of the Hubble Constant using gravitational lenses of quasars, which shows that the Tension might exist after all.

How did life begin on Earth? Based on studies of fossilized bacteria, scientists theorize that life first emerged on Earth over 4 billion years ago as simple, single-celled organisms. Over time, these organisms evolved to incorporate photosynthesis and sexual reproduction, eventually giving rise to more complex multicellular organisms, plants, and, eventually, mammals. Despite this scientific consensus, the question of how inorganic chemicals came together to form organic molecules that gradually evolved into self-replicating systems remains unclear.

What geological features on Earth can be used to better understand unique geological features on Jupiter’s icy moon, Europa? This is what a recent study published in *The Planetary Science Journal* hopes to address as a team of researchers investigated potential Earth analogs for studying a unique geological feature on Europa scientists identified almost 30 years ago. This study has the potential help scientists gain insights into Europa’s unique geological features, some of which scientists hypothesize are caused by the moon’s internal liquid water ocean.

(This is Part 4 of a series on primordial black holes. Check out Part 1, Part 2, and Part 3!)

Looking at an X-ray image of a galaxy cluster is like watching fireworks frozen in time. You see swirls and arcs, bubbles and filaments, structures that hint at past violence but don't explain what actually happened. Astronomers have puzzled over these features for decades, trying to determine which came from shock waves, which from cooling gas, and which from bubbles blown by black holes. Now a team led by Hannah McCall at the University of Chicago has developed a technique that answers these questions directly, creating images that classify the structures by their physics rather than their appearance.

Imagine trying to spot a single firefly orbiting a lighthouse from hundreds of kilometres away. That's essentially the challenge astronomers face when attempting to study Proxima b, an Earth sized exoplanet orbiting Proxima Centauri, the closest star to our Solar System. The star shines 10 million times brighter than its planet, drowning out any hope of detecting the faint light reflected from that distant world. Now scientists at the University of Geneva have successfully tested key components of an instrument designed specifically to solve this seemingly impossible problem.

How to see the best meteor shower of the year.

The Large and Small Magellanic Clouds are irregular dwarf galaxies and satellites of the Milky Way. The LMC is about 163,000 light-years away and the SMC is about 206,000 light-years away, and their close proximity makes them excellent laboratories for the study of galaxies in general. The Clouds are the focus of a new research group being formed at the Leibniz Institute for Astrophysics Potsdam (AIP).

There are already tens of thousands of pieces of large debris in orbit, some of which pose a threat to functional satellites. Various agencies and organizations have been developing novel solutions to this problem, before it turns into full-blown Kessler Syndrome. But many of them are reliant on understanding what is going on with the debris before attempting to deal with it. Gaining that understanding is hard, and failure to do so can cause satellites attempting to remove the debris to contribute to the problem rather than alleviating it. To help solve that conundrum, a new paper from researchers at GMV, a major player in the orbital tracking market in Europe, showcases a new algorithm that can use ground-based telescopes to try figure out how the debris is moving before a deorbiter gets anywhere near it.

The hunt is on for terrestrial exoplanets in habitable zones, and some of the most promising candidates were discovered almost a decade ago about 40 light-years from Earth. The TRAPPIST-1 system contains seven terrestrial planets similar to Earth, and four of them may be in the habitable zone. The star is a dim red dwarf, so the habitable zone is close to the star, and so are the planets. For that reason, astronomers expect them to be tidally-locked to the star.

(This is Part 3 of a series on primordial black holes. Check out Part 1 and Part 2!)

Supernovae aren't one of the JWST's main science themes, but the perceptive telescope is full of surprises. Recently, it pinpointed a single star in a galaxy when the Universe was only about 730 million years old. It wasn't just any random star; this one was a supernovae responsible for a gamma-ray burst (GRB) detected back in March, 2025.

Astronomers have found a unique blast coming from a distant supermassive black hole (SMBH). The SMBH is in a barred spiral galaxy about 135 million light-years away named NGC 3783. The Hubble recently imaged this face-on galaxy, showing its beautiful spiral arms and its center, tightly-packed with shining stars.

In 2017, astronomers using the TRAnsiting Planets and PlanetesImals Small Telescope (TRAPPIST) in Chile and NASA’s Spitzer Space Telescope confirmed the presence of seven rocky planets orbiting TRAPPIST-1, an M-type red dwarf star located about 39 light-years from Earth. What made the system especially intriguing was that three of these planets orbited within (or straddled) the system's habitable zone (HZ): TRAPPIST-1d, e, and f. Since then, scientists have been busy conducting follow-up observations of this system to learn as much as possible about its seven planets and whether they could be habitable.

Almost every massive galaxy is has a supermassive black hole at its core, an object containing millions or even billions of times the mass of our Sun. Most of these giants simply lurk in the darkness, quietly consuming material from their surroundings while emitting barely a hint of radiation. But a small fraction shine brilliantly, pumping out enormous amounts of energy as active galactic nuclei (AGN). For decades, astronomers have debated what triggers this dramatic awakening. Now, a new dataset from the Euclid space telescope provides evidence that violent collisions between galaxies are the primary culprit.