To understand how chaotic the early Solar System was, we need only gaze at the Moon. Its cratered surface bears the scars from multitudes of collisions. The early Solar System was like a debris field where objects smashed into each other in cascades of collisions. The same must be true in all young solar systems, and in a new paper, researchers simulated a collision between two massive planets to see what would happen.
Researchers have identified several features on Mars that look surprisingly similar to conditions on Earth. One notable feature is giant wave-like landforms called solifluction lobes, which are in cold, mountainous regions of Earth, like the Arctic or Rocky Mountains. These are slow-moving patterns similar to fluids running downhill, but on Mars, they're 2.6 times larger because of its lower gravity. They can grow much taller before collapsing on Mars.
There is a supermassive black hole at the center of our galaxy, and it's not alone. There is also likely a forest of binary black holes, neutron stars, and white dwarfs. All of these emit gravitational waves as they gradually spiral ever closer together. These gravitational waves are too faint for us to detect at the moment, but future observatories will be able to observe them. This poses an interesting astronomical challenge.
A new space mission is open for business. Last week, we got a look at science images from NASA’s SPHEREx (Spectro-Photometer for the History of the Universe, Epoch of Re-ionization, and Ices Explorer) mission. The mission will now begin science operations, taking 3,600 unique images a day in an effort to create a 3D map of the sky.
The JWST continues to live up to its promise by revealing things hidden from other telescopes. One of its lesser-known observations concerns Free-Floating Planets (FFP). FFPs have no gravitational tether to any star and are difficult to detect because they emit so little light. When the JWST detected 42 of a particular type of FFP in the Orion Nebula Cluster, it gave astronomers an opportunity to study them more closely.
When astronomers want to understand brown dwarfs, they often turn to WISE 1049AB. It's a benchmark brown dwarf in astronomy, and the closest and brightest brown dwarf we know of. The binary pair, which is also known as Luhman 16, is about 6.5 light-years away. Brown dwarfs are a crucial bridge between planets and stars, and understanding them helps astronomers understand the dynamics of both exoplanets and stars.
What new technologies or methods can be developed for more efficient in-situ planetary subsurface analyses? This is what a recent study presented at the 56th Lunar and Planetary Science Conference hopes to address as a team of researchers investigated how a novel instrument called OptiDrill could fill existing technological voids regarding the sampling and collection of regolith (top dust layer) and subsurface samples on a myriad of planetary bodies throughout the solar system.
The idea that our Solar System is representative of other solar systems hasn't survived the age of exoplanet discovery. Kepler and TESS have shown us that our system doesn't even contain the most common type of planet: sub-Neptunes. These planets pose a mystery to planetary scientists, and the JWST is helping unravel the mystery.
New Horizons' primary mission is complete. It's already completed its pass through the Pluto system and even stopped by 486958 Arrokoth, a Kuiper belt object on its way out of the solar system. But that doesn't mean it's done providing new scientific insights. A new paper looks at data collected by its ultraviolet spectrograph, which looked at one particular wavelength and helped provide context to a few different questions about the solar system.
The center of the Milky Way is a busy place, tightly packed with stars and dominated by the supermassive black hole Sagittarius A*. It also features powerful magnetic fields that regulate star production, influence gas dynamics and gas cloud formation, and even affect the accretion processes around Sagittarius A*. Gigantic filaments of gas that look like bones form along the magnetic field lines, and one of them appears to be fractured.
On 20 April, 2025, the African Space Agency (AfSA) was formally launched at an inauguration ceremony in Cairo, Egypt. The decision to create AfSA was made by the African Union (AU) in 2016 to coordinate the continent's approach to space, and enact the African Space Policy and Strategy. AfSA will coordinate African space cooperation with Europe and other international partners.
The solar gravitation lens (SGL) has much potential as a telescope. This point in space, located about 650 AU away from the Sun, uses fundamental properties of physics to amplify the light from extremely far-away objects, allowing us to see them at a level of detail unachievable anywhere else. However, any SGL mission would face plenty of technical and physical challenges. A new paper by independent researcher Viktor Toth is the latest in a series that discusses those challenges when imaging a far-away exoplanet, and in particular, looks at the difficulties in dealing with potential moving cloud cover. He concludes that using the SGL might not be the most effective way of capturing high-resolution images of an exoplanet, after all.
How do you distinguish a galaxy from a mere cluster of stars? That's easy, right? A galaxy is a large collection of millions or billion of stars, while a star cluster only has a thousand or so. Well, that kind of thinking won't get you a Ph.D. in astronomy! Seriously, though, the line between galaxy and star cluster isn't always clear. Case in point, UMa3/U1.
In a recent paper, a team of engineers from Purdue University describes how sandbox video games that offer players a high degree of freedom and creativity, like the popular Kerbal Space Program (KSP), could be used by space agencies to assist the early-mission development process.
Since the discovery of the first exoplanet in 1992 astronomers have now found over 5,000 alien worlds around other stars. With the discoveries of exoplanets came an entirely new classification of worlds known as the super-Earth; terrestrial planets more massive than Earth but smaller than Neptune. Sadly we don’t have any such planets in our Solar System but a new report suggests planets like this are surprisingly common with at least as many as there are Neptune sized planets.
Magnetars are among the rarest - and weirdest - denizens of the galactic zoo. They have powerful magnetic fields and may be the source of fast radio bursts (FRBs). A team of astronomers led by European Space Agency researcher Ashley Chrimes recently used the Hubble Space Telescope to track one of these monsters called SGR 0501+4516 (SGR0501, for short, and SGR stands for Soft Gamma Repeater). It's whipping through the Milky Way at a rate that could be as high as 65 kilometers per second. The big challenge was to find its birthplace and figure out its origin.
A few years ago, astronomers discovered an exoplanet orbiting the white dwarf 1856+534 b. Now they've used the mighty JWST to do follow-up observations and made some exciting discoveries. It's definitely a planet and not a brown dwarf, with a temperature of 186 K (-87°C/-125°F) and about 6 times the mass of Jupiter. This makes it the coldest exoplanet ever detected, and it's orbiting in the "forbidden zone," which should have been engulfed during the red giant phase.
Since the invention of the telescope, astronomers have been hunting for objects in our Solar System in particular and more recently, for the theorised 9th planet. Observations of Kuiper Belt objects suggest a large object might be lurking in the depths of the Solar System but to date, it hasn’t been directly observed. A team of researchers have analysed infrared sky surveys and found 13 objects that matched the estimated flux and motion of Planet Nine! Further analysis ruled out 12 leaving a single object. Is this Planet Nine?
What kind of spacecraft can be used to explore and study the subsurface lunar environment? This is what a recent study presented at the 56th Lunar and Planetary Science Conference (LPSC) hopes to address as an international team of researchers discussed the benefits of a mission concept called LunarLeaper, which will be designed to traverse and analyze the various aspects of the lunar subsurface environment, including moon pits and lava tubes.
NASA's Psyche mission launched in 2023 and has now successfully demonstrated that laser technology can transmit high-bandwidth data across millions of kilometres in space, making it promising for communications from Mars. However, researchers simulating Martian conditions found that while this optical communication works well under normal circumstances, performance degrades during dustier periods and fails completely during global dust storms.
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