Universe Today

What imaging systems can NASA’s Artemis astronauts use on the Moon to conduct groundbreaking science and efficient documentation on the lunar surface? This is what a recent study presented at the 56th Lunar and Planetary Science Conference (LPSC) aspired to address as a team of researchers from the University of Texas at El Paso and Johns Hopkins University Applied Physics Laboratory investigated using next-generation cameras on the Artemis III mission, which is slated to be the first lunar surface mission of the Artemis program.

Astronomers have found a new way of accurately mapping the outer gas disk of the Milky Way using the positions of young stars. In the process, they've also discovered that our galaxy's structure is more complex than everyone thought, complete with tufty-looking "flocculent" gas clouds.

A new solar observing telescope on the exterior of the International Space Station is open for business. NASA recently released images from the newly commissioned Coronal Diagnostic Experiment (CODEX) mounted on the station.

The observed exoplanet population contains a large number of solar systems where multiple exoplanets follow short orbital periods. The most well-known example of a compact solar system is the TRAPPIST-1 system. There are many others, and exoplanet scientists are trying to understand how they form. Scientists at the Southwest Research Institute (SwRI) may have figured it out.

Mercury doesn't give up its secrets easily. The smallest planet in our Solar System is also one of the most extreme, a sun-scorched, metal-rich world with a puzzling magnetic field and lavas unlike anything found on Earth. Now, groundbreaking laboratory experiments are finally beginning to unlock these mysteries, revealing how this planetary oddball could hold the key to understanding rocky planets throughout the universe.

Pulsars are spinning neutron stars, with several times the mass of the Sun compressed into a sphere just 10 km across. They have a theoretical "death line,” a point where pulsars should stop emitting radio waves as they slow down. But researchers have detected two pulsars still beaming radio signals despite being below this death line. One explanation is that there are tiny irregularities on their surfaces, mountains just 1 cm tall. These peaks amplify local electric fields, making it easier for the pulsars to accelerate particles and produce radio emissions that should be impossible.

The Japanese ispace HAKUTO-R Mission 2 was supposed to touch down gently on the Moon on June 5, 2025. Unfortunately, communications with the RESILIENCE lander were lost about 90 seconds before it should have landed, and it was assumed to have crashed on the lunar surface. Now, NASA's Lunar Reconnaissance Orbiter has captured the crash site from orbit at an altitude of 80 km and confirmed where it smashed into the Moon.

Since 2025, Solar Orbiter is the first Sun-watching spacecraft to ever get a clear look at the Sun's poles. It discovered that at the south pole, the Sun’s magnetic field is currently a mess.  This image shows a magnetic field map from Solar Orbiter's Polarimetric and Helioseismic Imager (PHI) instrument, centred on the Sun's south pole. Blue indicates positive magnetic field, pointing towards the spacecraft, and red indicates negative magnetic field.  There are clear blue and red patches vi...

After years of research, and a completed pathfinder mission, the European Space Agency has officially begun the construction of the Laser Interferometer Space Antenna (LISA). This will consist of three spacecraft flying in formation, sending laser signals back and forth to detect passing gravitational waves - including previously undetected supermassive black hole mergers. ESA has chosen OHB System AG to construct the spacecraft, which are due to launch in 2035 on an Ariane 6 rocket.

I can recall the excitement of waiting for the first CCD Image I had taken to download, THAT was exciting. I was using a Starlight Express MX716 for those who can remember. This however is far more exciting. The Vera C. Rubin Observatory has officially come online and now we're looking at its first pictures. The telescope has completed ten hours of test observations, viewing millions of galaxies and Milky Way stars. It found thousands of new asteroids in just a few hours of observations, and took incredible pictures of the Triffid and Lagoon Nebulae. Over the course of its 10-year primary mission, it'll capture 800 images of every spot in the southern sky.

Mars holds two of humanity's greatest space ambitions, discovering alien life and establishing our first foothold on another world. Key to both is the discovery of water. We know it's at the poles, but where could we find it at lower latitudes? In a new paper, researchers carefully examined images of Mars taken by the Mars Reconnaissance Orbiter. They found examples of features, like "brain coral terrain", expanded craters, and ridges which are evidence of water ice just under the surface.

The Solar System lacks hot-jupiters, intensely hot gas giant planets, so close to their stars they take just days or even hours to orbit once. But there are some systems that have not one, but two hot-jupiters. In a new study, researchers show the long-term gravitational interactions with binary stars that can push multiple gas giants into these extremely close orbits around their stars. Both stars can end up with hot-jupiters.

The Earth's magnetosphere is a giant magnetic field that arises from the flow of material deep inside the planet. Because the flow of material isn't constant, the strength and shape of the magnetosphere can change over geologic time. But researchers have found that changes in the magnetosphere seem to be correlated with fluctuations in the amount of oxygen in the Earth's atmosphere. Both could be responding to a single underlying process.

Just when you thought the race to reusable rockets was all wrapped up, a new competitor emerges from the shadows. Honda R&D Co (a subsidiary of Honda Motor Co) successfully tested their new experimental reusable rocket. The 6.3-meter rocket blasted off, reached an altitude of 271.4 m, and then landed within 37 cm of their touchdown point. The flight lasted for 56.6 seconds.

The early Universe was a busy place some 13 billion years ago. That's when countless young galaxies began to evolve and birthed stars at a prodigious rate. The hearts of those very distant galaxies show turbulent, lumpy disks studded with even thicker clumps of dust and gas that spawned huge batches of stars. Astronomers want to understand what's driving the clumping, so they've turned to recent surveys of closer galaxies in the "local Universe" that contain similar lumpy regions.

More than one third of the regular matter in the Universe is missing (we're not talking about dark matter, just regular matter). It's needed to make the current cosmological models work, so astronomers continue to search for it, and have found many indirect examples of it. Now a team of astronomers has directly observed it as a huge filament of hot gas bridging four galaxy clusters and containing 10 times the mass of the Milky Way.

Solar eclipses are beautiful, but they're a valuable chance to study the Sun's atmosphere as its surface is blocked by the Moon. Now, ESA can generate artificial solar eclipses from space with the Proba-3 mission. The two satellites fly in formation 150 meters apart. One spacecraft occults the Sun, while the other observes the faint solar corona. They can produce a new 6-hour eclipse every 19.6-hour orbit around the Earth. Solar eclipses on demand.

Comet C/2014 UN271 is one of the largest Oort Cloud comets ever observed, measuring 140 km across. It's currently at a distance of 16.5 AU from the Sun, which makes it tough to observe with all but the largest telescopes. Astronomers have used ALMA in Chile to observe the comet, watching as jets of carbon monoxide gas are erupting from its nucleus. This is a surprising level of activity for a comet that's so far from the Sun.

Scientists are using a new approach to find the mysterious - if it exists - Planet Nine by hunting for its heat signature instead of reflected light. Using data from Japan's AKARI space telescope, a team of researchers identified two promising candidates using their thermal detection method which is more effective than optical searches alone. But could these distant heat sources finally prove the existence of our Solar System's most elusive world, or will they turn out to be yet another false alarm in the decades long search?