Growing plants in space? Yes indeed! NASA astronauts are conducting botany experiments aboard the International Space Station (ISS).

What is it?

In this snapshot — captured by NASA astronaut Jessica Watkins, commander of SpaceX's Crew-13 mission to the ISS — we can see fellow NASA spaceflyer Luke Delaney hard at work aboard the ISS. And while he's orbiting around our planet aboard a laboratory in the vacuum of space, he's also growing plants.

In the photo, Delaney is working petri dishes and experiment modules that support our growing understanding of how plants grow in the microgravity environment aboard the station. Specifically, the experiments Delaney is working on will investigate the genetic responses of plants in this environment.

This is not the first time that researchers have studied plants in space. In fact, ISS astronauts have conducted a wide variety of plant experiments and investigations over the years. They've grown peppers and other edible produce and even proved that moss can survive outside the station, in the harsh environment of space.

Why is it incredible?

When you picture the inside of an orbiting space station, you might imagine the white and gray walls with computers, buttons, switches and other such tech speckling the scene. But the space station is also full of (non-astronaut) life, thanks to the incredible variety of biological experiments onboard.

While space is "the final frontier," and we look outward to study everything from black holes to exploding stars, outer space can also help teach us about own planet. Satellites look back at Earth, studying its changing landforms, migrating wildlife, diminishing glaciers and natural disasters. Onboard the ISS, astronauts conduct experiments with plants, animals, microscopic organisms and an incredible amount of studies supporting human health and medical care. While space might be the final frontier, so much of the work done in space is designed to benefit us back here on Earth.

HAWTHORNE, Calif. — A moon buggy carrying a history-making supercomputer is ready to launch to the lunar surface. And it's taking some inspiration from Mars.

Later this year, Astrolab will launch its uncrewed moon rover FLIP to the lunar south pole as part of the Griffin Mission 1, or Griffin-1. The California company is one of two that NASA has selected to develop a drivable rover for the agency's Artemis program. On board FLIP will be Hewlett Packard Enterprise's (HPE) Spaceborne Computer-4, an advanced computer module built to be used in space.

This will be the first time that high-performance computing and artificial intelligence will be tested on the lunar surface. As NASA gets closer to landing humans back on the moon with Artemis, advancements like this aim to support future human habitation as well as economic activity on and around the moon.

"We're sending the first supercomputer from HPE to the lunar surface later this year, doing the first GPU [graphics processing unit] on the moon [and the] first AI experiments on the moon," Jaret Matthews, founder and CEO of Astrolab, said during an Oct. 14 media event here at Astrolab's headquarters. "They're breaking new ground, and they're ahead of the curve."

The computer is designed to be lightweight, compact, self-contained and fanless. It has a low-power 64-bit CPU (central processing unit) with a GPU. The computer will be attached to FLIP's cooling system and will be powered by a system supported by both batteries and solar cells on the rover. The computer will also be paired with solid state drives from the company KIOXIA that will allow for memory storage.

So, what will a supercomputer and AI accomplish on this uncrewed mission? First and foremost, the flightwill test how the computer works in this extreme environment. The computer is built with heat-conductive aluminum and is designed with the specific conditions of the lunar south pole in mind. But while it was designed and tested to be able to withstand the extreme temperatures and conditions on the moon's surface, the upcoming mission seeks to show that this advanced technology can actually work in this environment.

"NASA's given us a real challenge," Matthews told Space.com at the media event. "We have to design for a full year on the lunar surface. So that means surviving multiple lunar nights, upwards of 150 hours of complete darkness where we're not receiving energy or warmth from the sun. And then, also, there's going to be a long period [in] which we're operating semi-autonomously for [when] the astronauts are not there … and so we're having to develop a semi-autonomous platform that will spend many months [and] travel hundreds of kilometers [on the moon]."

But the computer will more than just prove its durability, if all goes to plan. It will also analyze visual data captured on the mission and enable autonomous observations, process navigation, mapping and terrain analysis. The mission also promises to test AI capabilities, though it's unclear what exact applications we'll see with this lunar AI. HPE shared in a statement that "an AI services container will demonstrate reliable deployment of scalable AI service applications on the moon."

It is also to be determined exactly how, once tested, these capabilities might be used with future crewed missions. Astronauts aboard the International Space Station already use computers for communications, science experiments and other daily tasks while living in space, but we can't say yet exactly how future astronauts might use these capabilities, especially with the addition of AI, on the moon.

From Mars to the moon

One interesting aspect of this new development is where it came from. While HPE has provided computing power to NASA for decades, Matthews is also bringing his previous experience working at NASA's Jet Propulsion Laboratory (JPL) into this new venture.

"One of the experiments [that will be] running on the spaceborne computer on the moon is a localization software experiment from JPL. It has been used on Mars, and this will be the first time it's used on the moon," Matthews said.

"The challenge with the moon and Mars is that there's no GPS, so locating yourself and knowing where you are on the surface [can be difficult]," he added. "So we're going to be running what is essentially a machine learning algorithm that JPL developed to take a map that's stored in memory … and compare it to the local terrain we see around us, and then do a match. So essentially, match features of the local terrain to the map that's stored in memory to help find ourselves on the map and keep ourselves away from dangerous craters."

As its name suggests, Griffin-1 will be the first mission for the robotic Griffin moon lander, which was developed by Astrobotic. The Pittsburgh company is flying Griffin-1 for NASA, under the agency's CLPS (Commercial Lunar Payload Services) program. In addition to FLIP, the mission will carry Astrobiotic's CubeRover, a small, uncrewed rover; LandCam-X, an optical navigation system; and Nanofiche GLPH (Galactic Library to Preserve Humanity), a tiny archive of human history, to the moon's surface.

"The moon presents a challenging environment for advanced computing, and we’re pleased to provide HPE with an opportunity to demonstrate its technology on the lunar surface," Matthews added in a statement. "Our FLIP rover is designed to accommodate a variety of payloads, and this mission will demonstrate how commercial lunar mobility platforms can support technology development and scientific research."

If you were approaching the edge of a spiral galaxy, arriving from afar through the cosmos, it might look something like this.

What is it?

In this new snapshot by the Hubble Space Telescope's Advanced Camera for Surveys (ACS), we can see the edge of the spiral galaxy NGC 1827. Found about 37 million light-years from Earth, this galaxy sparkles in this side-on view.

Not all spiral galaxies are the same. This galaxy is what is known as an "intermediate" spiral, which means that its structure sits somewhere between that of a barred and unbarred spiral galaxy. Barred galaxies have a distinctive central, bar-shaped structure, while the unbarred variety lacks this bar and can look more like circular spirals.

NGC 1827's spiral shape isn't clear from the side, however. From this perspective, we see its twinkling edge, speckled with stars and woven together with brown ribbons of dust.

Why is it incredible?

Beneath the beauty of this spiral edge lies an expansive, cosmic landscape. Bright blue stars dot the spiral's side, with one particularly luminous star taking the spotlight with four diffraction spikes — created by light bending through the inner workings of Hubble's camera — emanating from its center.

This image was captured as part of a larger Hubble survey that's exploring 260 satellite galaxies, which are galaxies gravitationally bound to larger hosts. Hubble is specifically looking to survey satellite galaxies that lie near host galaxies similar to our own Milky Way.

So far, Hubble has spotted 111 such satellites and will continue to observe, hunting for the rest.

By studying satellite galaxies like this one, which also happens to be an especially low-mass galaxy, researchers could better understand the complicated dynamics both within the galaxies themselves and between them and their host galaxies.

The moon is shrinking, and scientists are narrowing in on exactly how much our natural satellite has dwindled over the years.

The moon is thought to have formed from a violent collision between a massive object and our young Earth roughly 4.5 billion years ago, and its interior is still gradually cooling off from this ancient collision. As it cools, the moon contracts, leading to a long, slow shrinking process. Now, in a new study, scientists think that they have figured out how much smaller the moon is actually getting.

In this new study, scientists analyzing images snapped by the Lunar Reconnaissance Orbiter Camera (LROC) have spotted over 10,000 young faults, or cracks across the moon's surface. This helped them to figure out how much the moon has contracted over time, and they now estimate that the moon's radius has decreased by about 148 feet (45 meters) over the past 400 to 800 million years.

"The number of these young faults revealed in LROC images is much greater than I ever imagined," study lead Thomas Watters, a geologist and scientist emeritus at the Center for Earth and Planetary Studies at the Smithsonian's National Air and Space Museum, said in a statement. "As the interior of the moon continues to cool and contract, it is expected that the growth of existing faults and formation of new faults continues today."

With these LROC observations, researchers in this study saw a variety of different types of cracks and landforms across the lunar surface. This included lobate scarps, or long, curved structures that form when the moon's surface contracts, cracks and is pushed upwards; and small mare ridges, or narrow "wrinkles" in the lunar surface, across the dark plains on the moon.

Tectonic activity on the moon looks a lot different than it does on Earth. On our own planet, there are about 15 major tectonic plates. On the moon, there are no tectonic plates at all. Instead, the moon has a single-plate body meaning its outer shell is a single piece only broken by faults or other such cracks created by the moon contracting. This means that instead of faults or cracks appearing at tectonic plate boundaries, they are instead scattered all over the moon.

By mapping these thousands of different features, all created from the moon cooling and contracting over time, the researchers are piecing together lunar history. In addition to finding the extent to which the moon has shrunk over time, they also found that some areas of the moon are covered in many more faults than other areas, and the areas with fewer cracks and faults have thicker moon crust.

This led them to conclude that not only are these areas with thicker crust more stable, but they suggest that a great deal of the widespread cracks in the lunar surface were created later in the moon's history as, in its earlier years, its thick crust would have insulated the moon's warm interior and prevented cooling, contracting and cracking.

This work was described in a study published Oct. 14 in The Planetary Science Journal.

Antarctica is a magnificent sight, and that beauty is visible all the way from space.

What is it?

Orbiting planet Earth, the European Space Agency's (ESA) Copernicus Sentinel-3 mission captured a close-up of West Antarctica.

Winter is ending in the Southern Hemisphere, meaning this is the peak of icy weather and sea ice in the Arctic.

In this image snapped by Sentinel-3, you can see a massive swath of ice which includes Elephant Island on the left-hand side. An ice-covered island off the Antarctic coast, Elephant Island floats in the Southern Ocean. It got its name both from the island's shape, which some liken to that of an elephant's head, and the fact that the island is home to a community of elephant seals.

Why is it incredible?

While a seal-inhabited island on the left floats near the Antarctic coast, across the water is a vast, frozen landscape. In just this snapshot, you can see about between 746 and 1,056 miles (1,200 to 1,700 kilometers) of the icy continent.

This image was captured on Sept. 30, 2026. In the Southern Hemisphere, that was just past the end of winter. The absolute peak for sea ice in Antarctica fell just a couple weeks before, on Sept. 14, according to the National Snow and Ice Data Center, ESA reported.

So in this one snapshot, we can see a near-maximum for sea ice in the Antarctic, spanning hundreds of miles. In observing our own planet from space, we are able to peer across vast landscapes, capturing important observational data. This is especially critical for the Antarctic as, with the progression of climate change, this sea ice continues to dwindle, adding to sea level rise among other serious consequences across the planet.

What looks like a neon pink treble clef floating out in space is actually a bizarre source of radio waves spotted deep in the cosmos.

What is it?

Scientists using NASA's Chandra X-ray Observatory have peered far out into space to look at strange radio waves coming from what they have nicknamed the "treble clef" because of its distinct shape, which looks a lot like the musical notation.

Using Chandra, as well as the German Extended RÖntgen Survey with an Imaging Telescope Array (eROSITA) X-ray telescope, researchers looking at this strange sight spotted a big cloud of blue gas, which we can see in this image, along with radio signals (seen here in bright pink). They think that this object is actually a huge galaxy cluster made up of two different clusters that are in the process of merging.

Why is it incredible?

The researchers think they may have gotten to the bottom of where these radio waves are coming from, they report in a new study.

The team thinks that the treble clef-shaped radio signals were created by an outburst from a supermassive black hole. They believe that this outburst pushed clouds of charged particles and magnetic fields away from the galaxy cluster's center, producing bright radio waves.

According to the scientists, following this bright outburst, there was likely an extreme collision between two galaxy clusters. This cosmic smash-up either compressed or somehow reenergized these charged particles to amplify the radio signal.

When we see beautiful images of objects in space such as this, they can seem just like peaceful, colorful, cosmic clouds. But when you look a bit deeper, these spectacular scenes can actually be evidence of violent, chaotic events.

This work was described in a study published in the journal Astronomy & Astrophysics.