Space News & Blog Articles

Earth has a long, 4.5 billion history full of momentous twists and turns. Multiple prominent events played leading roles in Earth's story. One of them is the catastrophic impact with another planetesimal early in Earth's history that not only created the Moon, but altered Earth's chemistry forever.

Dust devils are a regular occurrence on Mars. Similar to Earth, these short-lived whirlwinds emerge when surface heating occurs, causing changes in air pressure and a vertical column of wind to form. As the column pulls in surrounding air, it becomes a vortex that kicks up dust, which it carries with it across the surface. While Mars has a very thin atmosphere, less than 1% that of Earth's, the lower gravity means that its dust devils grow larger than anything we see here. And according to new research by an international research team, these dust devils will reach velocities that are higher than what we expected.

The wavelengths of radio light are so large that you can't capture a high-resolution image with a single dish. To capture an image as sharp as, say, the Hubble telescope, you'd need a radio dish tens of kilometers across. So radio astronomers took a different approach. They used an array of dozens of antennas, each capturing their own signal. Since the antennas not only capture precise data but also the precise timing of that data, astronomers can use a process known as interferometry. Light from a distant radio object reaches each antenna at a slightly different time, and by correlating the arrival times, astronomers can treat the array as a virtual antenna disk the size of the entire array. From many, one, as the saying goes.

The Search For Extra Terrestrial Intelligence (SETI) is evolving. We’ve moved on from the limited thinking of monitoring radio waves to checking for interstellar pushing lasers or even budding Dyson swarms around stars. To match our increased understanding of the ways we might find intelligence elsewhere in the galaxy, the International Academy of Astronautics (IAA) is working through an update to its protocols for what researchers should do after a confirmed detection of intelligence outside of Earth. Their new suggestions are available in a pre-print paper on arXiv, but were also voted on at the 2025 International Astronautical Congress (IAC) in Sydney, with potential full adoption early next year.

Space-based solar power has been gaining more and more traction recently. The recent success of Caltech’s Space Solar Power Project, which demonstrated the feasibility of transmitting power from space to the ground, has been matched by a number of pilot projects throughout the world, all of which are hoping to tap into some of the almost unlimited and constant solar energy that is accessible up in geostationary orbit (GEO). But, according to a new paper from a group of Italian and German researchers, there are plenty of constraints on getting that power down here to Earth - and most of them are more logistical than technical.

What can cryovolcanism on Pluto teach scientists about the dwarf planet’s current geological activity? This is what a recent study published in *The Planetary Science Journal* hopes to address as a team of researchers investigated potential cryovolcanic sites within specific regions on Pluto. This study has the potential to help scientists better understand the current geological activity, including how it can be active while orbiting so far from the Sun.

On the surface of Mars, there are numerous features that tell of a past age when the planet was warmer and wetter, with rivers, lakes, and even an ocean that covered much of its northern hemisphere. These include river channels, delta fans, sedimentary deposits, and low-lying regions rich in clay minerals. The discovery and study of these features over the past fifty years have raised some pressing questions for scientists. These include the question of how much water once flowed on Mars and what led to the gradual transition that left the planet a frigid, desiccated world, where the only water on the surface comes in the form of ice and permafrost.

At the dawn of time, so the theory goes, the cosmos underwent a flash of rapid expansion. Almost instantly the visible Universe grew from a volume smaller than a proton to a spherical region nearly two meters across. It's a moment known as early cosmic inflation. Although Inflation solves several cosmic problems, such as the homogeneity of the Universe and the ratio of hydrogen to helium we observe, we haven't been able to prove it. But we might be able to prove it by looking for a particular type of gravitational wave.

The ice giants remain some of the most interesting places to explore in the solar system. Uranus in particular has drawn a lot of interest lately, especially after the 2022 Decadal Survey from the National Academies named it as the highest priority destination. But as of now, we still don’t have a fully fleshed out and planned mission ready to go for the multiple launch windows in the 2030s. That might actually be an advantage, though, as a new system coming online might change the overall mission design fundamentally. Starship recently continued its recent string of successful tests, and a new paper presented at the IEEE Aerospace Conference by researchers at MIT looked at how this new, much more capable launch system, could impact the development of the Uranus Orbiter and Probe (UOP) that the Decadal Survey suggested.

Is anybody out there? Probably. Most stars have planets; we've discovered more than 6,000 exoplanets thus far, and the most basic statistics point toward the existence of countless potentially habitable worlds in the Universe. But when we have looked for any scrap of evidence for alien civilizations, we have found nothing so far. The question is why?