By Andy Tomaswick May 29, 2025
We've been gazing at the Moon for a long time, yet it's still mysterious. We've sent numerous orbiters and landers to our satellite, and even brought some of it back to our labs. Those rocks only presented more mysteries, in some ways. Lunar rocks are magnetic, yet the Moon doesn't have a magnetosphere. How did this happen?
By Andy Tomaswick May 29, 2025
Just because we can find ozone in the atmosphere of other planets doesn't mean there's life. Ozone is a sign of life on Earth, but its detection on Venus shows that it can also be produced abiotically. This indicates that there are different pathways for its creation, not only on Venus but also on other Venus-like exoplanets.
What happens when you see something that just doesn’t make sense? Perhaps you rub your eyes and consider it an anomaly. But what if you see it in an experiment? Say, travelling electrons that make different patterns depending upon whether they were detected? Then, you might want to change your sense of reality. Now, if you can develop a theory for the observations, then maybe you can start a new field of science. It has happened. Quantum mechanics is the name given to this relatively new field and it’s the topic that Sean Carroll writes in his book, “The Biggest Ideas in the Universe – Quanta and Fields”. In his book, there’s much ado about particles, fields, groups and diagrams; all with the aim of enabling any reader to make sense of it.
Asteroids are the ancient remnants of our Solar System's birth, rocky fragments that never formed into planets. Most of these celestial wanderers inhabit the asteroid belt between Mars and Jupiter, where Jupiter's immense gravitational influence prevented them from assembling into a single world. Ranging from house-sized boulders to Ceres, a dwarf planet nearly 1,000 kilometres across, asteroids preserve pristine records of the early Solar System's composition and conditions.
Lunar exploration is entering a new era. Long after the Apollo missions, a renewed international interest comes with ambitious plans for a long-term presence on the Moon. NASA’s Artemis program is leading efforts to return humans to the lunar surface, with Artemis III aiming to land astronauts near the Moon’s South Pole as early as 2026. Meanwhile, countries like China and India have successfully conducted robotic missions, including landings and sample returns, while private companies are increasingly involved through partnerships and commercial lander missions. The focus has shifted from short visits to sustainable exploration, with goals that include building lunar habitats, developing on-site resource utilisation, and establishing infrastructure to support future crewed missions to Mars.
By Matthew Williams May 28, 2025
For centuries, astronomers have sought to understand the formation and evolution of the Solar System and the dynamics that govern it. In particular, there is the long-standing question of whether or not the planets' orbits will remain stable over time. However, these studies have generally treated the Solar System as an isolated system, focusing solely on the gravitational interactions between the planets. This is in spite of the fact that astronomers have known for some time that stars in the Milky Way make close passes to each other every so often.
Some parts of the Moon are more interesting than others, especially when searching for future places for humans to land and work. There are also some parts of the Moon that we know less about than others, such as the Irregular Mare Patches (IMPs) that dot the landscape. We know very little about how they were formed, and what that might mean for the history of the Moon itself. A new mission, called the LUnar Geology Orbiter (LUGO), aims to collect more data on the IMPs and search for lava tubes that might serve as future homes to humanity.
Extraordinary claims require extraordinary evidence. That truism, now known as the "Sagan standard" after science communication Carl Sagan, has been around in some form since David Hume first published it in the 1740s. But, with modern-day data collection, sometimes even extraordinary evidence isn't enough - it's how you interpret it. That's the argument behind a new pre-print paper by Luis Welbanks and their colleagues at Arizona State University and various other American institutions. They analyzed the data behind the recent claims of biosignature detection in the atmosphere of K2-18b and found that other non-biological interpretations could also explain the data.
Most astronomers agree that life is likely common throughout the Universe. While Earth is the only world known to have life, we know that life arose early on our world, and the building blocks of life, including amino acids and sugars, form readily. We also know there are countless worlds in the cosmos that might be home for life. But just because life is likely, that doesn't mean proving it will be easy. Many of the biosignatures we can observe can also have abiotic origins. So how can we be sure? One way is to compare our observations of a habitable world with other worlds in the system.
We tend to think of habitability in terms of individual planets and their potential to host life. But barring outliers like rogue planets with internal heating or icy moons with subsurface oceans created by tidal heating, it's exoplanet/star relationships that generate habitability, not individual planets. New research emphasizes that fact.
Supermassive Black Holes reside at the center of large galaxies, where they dominate their surroundings and sometimes eat stars. When they gobble up a star, they emit a distinctive light flare. This makes it easier for astronomers to pinpoint their location. Astronomers have detected one of these flares offset from a galactic center. Is the black hole shifting its location?
Over the past decade or so, astronomers have speculated about the characteristics of rogue planets in the Milky Way Galaxy. These "free-floating" worlds don't orbit stars, but instead roam the spaceways. They're hard to spot with current technology, but the upcoming Nancy Grace Roman Space Telescope (Roman) will be a perfect instrument to find them and give insights into the history and features they may have in common with Solar System worlds.
One of the unanswered questions in astronomy is just how supermassive black holes grew so big, so quickly. A team of astronomers have tried to answer this question by searching for actively feeding supermassive black holes (aka quasars) as a way to measure how much material material they are actually accumulating. They studied nebulae near the quasars that light up with the quasar is releasing radiation and found that many of the more distant quasars have only been active for a few hundred thousand years, not long enough to grow to the size we see today.
The most massive stars in the Milky Way contain one hundred times more mass than the Sun, even more in some cases. These O-type stars are extremely hot, luminous, and blue, and often die in supernova explosions. Astrophysicists want to know how they get so big, and a simple household chemical might hold the answer.
The Fermi Paradox presents us with a striking contradiction: despite the high probability of numerous civilizations existing throughout the Universe, we've encountered no evidence or communication from any alien intelligence. A new paper just published calculates that we should have a 99% chance of detecting at least one signal from another civilisation—assuming they survive for several hundred years and could be distributed anywhere across the Milky Way galaxy. This calculation further deepens the mystery of our apparent cosmic solitude.
On May 7th, the Japanese space exploration company ispace announced that its HAKUTO-R RESILIENCE lander entered lunar orbit after completing a 9-minute thruster burn. It's now in a stable lunar orbit, and operators will spend the next month testing and preparing for its landing attempt on June 5. This is the company's second attempt at landing on the Moon, after the first attempt crashed in 2023. It's carrying a micro-rover and several science experiments.
All Rights Reserved. 2026. SpaceZE.com
