If you happen to be enjoying a sunny day, thank the bright surface of the Sun, known as the photosphere. At a piping hot temperature of about 5,800 K, the photosphere provides nearly all the sunlight Earth receives. But for all its glorious radiance, the photosphere isn't the hottest part of the Sun. That award goes to the diffuse outer atmosphere of the Sun known as the corona, which has a temperature of more than a million Kelvin. Parts of the corona can be as hot as 20 million Kelvin, which is hotter than the Sun's core. Of course, the big mystery is why the corona is so hot.

This week brings the Hubble Space Telescope's 35th birthday — but instead of getting presents, the Hubble team is giving out presents in the form of four views of the cosmos, ranging from a glimpse of Mars to a glittering picture of a far-out galaxy.

Data from the James Webb Space Telescope (JWST) is coming in hot and heavy at this point, with various data streams from multiple instruments being reported in various papers. One exciting one will be released shortly in the Astrophysical Journal from researchers at the University of Kansas (KU), where researchers collected mid-infrared images of a part of the sky that holds galaxies from the time of the "cosmic noon" about 10 billion years ago. Their paper describes this survey and invites citizen scientists to help catalogue and classify some of their findings.

How can we turn the sun into a telescope?

If we need more evidence that our Solar System is not representative of other solar systems, take a look at BD+05 4868. It's a binary star consisting of a K-dwarf and an M-dwarf about 140 light-years away. It's not just the binary star sets the system apart from ours. A small rocky planet is so close to the primary star that it's being vaporized, leaving a trail of debris like a comet.

At some early point in Earth's history, a collection of increasingly complex chemicals performed a new trick. They transformed themselves somehow into an energy-producing and self-replicating cell. The timing of this critical moment in Earth's history is hidden behind the haze of billions of years.

It's a cosmic shame, that we tend to only see flat-looking, 2-dimensional views of deep-sky objects. And while we can't just zoom out past the Andromeda galaxy for another perspective, or see the Crab Nebula from another vantage point in space, we can use existing data to simulate objects in 3D. A recent collection released by Marshall Space Flight Center's Chandra X-ray Center and the Harvard-Smithsonian Center for Astrophysics shows us familiar objects in a new way.

When China's DRO-A and B satellites were launched, their rocket failed to deliver them to their planned orbit. Even worse, the satellites were spinning out of control, unable to properly charge their solar panels. Engineers realized that there was still a way to put them on course again. They executed a series of gravitational slingshots over 123 days, using the Sun, Earth, and the Moon to raise the spacecraft's orbits and put them into their proper trajectory.

The weather gets a little wild and weird on Jupiter. How wild? Spacecraft instruments have measured strong winds, tracked fierce lightning, and found huge methane plume storms rising from deep beneath the clouds. How weird? Think: mushballs raining down like hailstones. They're made of ammonia and water encased in a water ice shell. According to planetary scientists, these mushballs plunge through the Jovian atmosphere. What's more, they probably form on the other gas and ice giants, too.

The evidence is building that the surface of Mars was warm and wet for its early history. But what form did this water take? In a new study, geologists propose that Mars has very similar features to places like Utah on Earth, where precipitation from snow or rain formed the patterns of valleys and headwaters that have been mapped from space. Some of these features would require meters deep of flowing water to deposit large boulders.

Let's turn the sun into a telescope. In fact, we don't have to do any work – we just have to be in the right spot.

Studying the Sun is becoming increasingly important as more and more of our infrastructure moves off the surface and into the realm where coronal mass ejections and the solar wind can begin to affect them. Scientists recognize this problem and have started devoting more and more resources to studying the Sun, specifically the "space weather" that might affect us. Recently, one of the newest members of the group of satellites focused on studying the Sun hit a milestone when the Polarimeter to Unify the Corona and Heliosphere (PUNCH) mission took on its first light.

Planetary scientists have plenty of theories about Mars and its environmental past. Two of the most widely accepted are that there was a carbon dioxide atmosphere and, at one point, liquid water on Mars' surface. However, this theory has a glaring problem: Where should the rocks have formed from the interactions between carbon dioxide and water? According to a new paper by scientists at several NASA facilities using data collected by the rover Curiosity, the answer is right under the rover's metaphorical feet.

The exoplanet K2-18b is generating headlines because researchers announced what could be evidence of life on the planet. The JWST detected a pair of atmospheric chemicals that on Earth are produced by living organisms. The astronomers responsible for the results are quick to remind everyone that they have not found life, only chemicals that could indicate the presence of life. The results beg a larger question, though: Can the JWST really ever detect life?

On any clear, moonless night, the light from the billions of stars in our Milky Way Galaxy can be seen arching across the sky. A large spiral galaxy, the Milky Way we see today is the result of billions of years of galactic evolution. A team of astronomers have announced the discovery of a galaxy very similar to our own but this one is less than a billion years old! Typically galaxies like the Milky Way with a developed central bulge and spiral arms are only seen in nearby galaxies suggesting it's a process that takes time. This latest discovery challenges that theory!

The planets in our Solar System orbit the Sun along a plane extending from the solar equator. That's typically the case for exoplanets too but just recently, a team of astronomers have found a system where a planet is in a perpendicular orbit around a binary pair! The brown dwarf system with its strange planetary companion is likely the result of three-body interactions between the stars and planet, tweaking it into the crazy orbital configuration we see today.

NASA's Lucy spacecraft made a successful flyby of the second asteroid on its must-see list over the weekend, and sent back imagery documenting the elongated object's bizarre double-lobed shape. It turns out that asteroid Donaldjohanson — which was named after the anthropologist who discovered the fossils of a human ancestor called Lucy — is what's known as a contact binary, with a couple of ridges in its narrow neck.

After spending 220 days on board the International Space Station, astronaut Don Pettit is back on Earth. He returned to Earth on Sunday, April 20th, which coincides with his 70th birthday.

Where did the water we believe is on the Moon come from? Most scientists think they know the answer - from the solar wind. They believed the hydrogen atoms that make up the solar wind bombarded the lunar surface, which is made up primarily of silica. When that hydrogen hits the oxygen atoms in that silica, the oxygen is sometimes released and freed to bond with the incoming hydrogen, which in some cases creates water. But no one has ever attempted to replicate that process to prove its feasibility. A new paper by Li Hsia Yeo and their colleagues at NASA's Goddard Space Flight Center describes the first experimental evidence of that reaction.

Just how powerful is the world's most powerful telescope?

Scientists are still trying to understand the origin of multicellular life. It emerged about 1.2 billion years ago (or even earlier, according to some debated evidence). The timing of multicellular life's appearance on Earth is not the only thing being debated; so are the mechanisms behind it. New research supports the idea that multicellular life began when single-celled bacteria started grouping together.

A team of NASA scientists proposed a new initiative at the 56th Lunar and Planetary Science Conference (2025 LPSC). Known as the Commercial Hall Propulsion for Mars Payload Services (CHAMPS), the

How can you fairly compare one telescope to another? It's all in the (angular) resolution.

Scientists have known for a while that Mars currently lacks a magnetic field, and many blame that for its paltry atmosphere - with no protective shield around the planet, the solar wind was able to strip away much of the gaseous atmosphere over the course of billions of years. But, evidence has been mounting that Mars once had a magnetic field. Results from Insight, one of the Red Planet's landers, lend credence to that idea, but they also point to a strange feature - the magnetic field seemed to cover only the southern hemisphere, but not the north. A team from the University of Texas Institute for Geophysics thinks they might know why - in a recent paper, they described how a fully liquid core in Mars could create a lopsided magnetic field like the one seen in Insight's data.

You never know when a central supermassive black hole is going to power up and start gobbling matter. Contrary to the popular view that these monsters are constantly devouring nearby stars and gas clouds, it turns out they spend part of their existence dormant and inactive. New observations from the European Space Agency's XMM-Newton spacecraft opened a window on the "turn on event" for one of these monsters in a distant galaxy.

In a recent paper, a team of researchers indicated that photosynthetic bacteria could exist just beneath the snow and ice around Mars' mid-latitudes. If true, this could be the most easily accessible place to look for present-day life on Mars.

The solar system is currently embedded deep within the Local Bubble, a region of relatively low density stretching for a thousand light-years across. It was carved millions of years ago by a chain of supernova explosions. And the evidence for it is right under our feet.

According to a recent study by the non-profit Explore Titan, a nuclear-fission propulsion spacecraft could enable the first crewed mission to Titan, Saturn's largest moon.

In our neighborhood of the Milky Way, we see a region surrounding the solar system that is far less dense than average. But that space, that cavity, is a very irregular, elongated shape. What little material is left inside of this cavity is insanely hot, as it has a temperature of around a million Kelvin.

Astrobiologists are dying to send another mission to study Enceladus, the icy moon that orbits Saturn and has active plumes emanating from its surface, A team from NASA's Jet Propulsion Laboratory (JPL) proposes an Enceladus Orbitlander that would conduct in-situ measurements of Enceladus' plumes, which could confirm the presence of organics and maybe even life in its interior.

What can Helium-3 (3He) being discharged from the Sun teach us about 3He creation and the Sun's activity? This is what a recent study published in The Astrophysical Journal hopes to address as an international team of researchers investigated 3He-rich solar energetic particles (SEPs) emitted by the Sun in late 2023. This study has the potential to help astronomers better understand how solar activity could contribute to the production of 3He, the latter of which remains one of the most desired substances due to its potential for nuclear fusion technology on Earth.

Two new studies have sparked fresh debate about a faraway planet with a weird atmosphere. One of the studies claims additional evidence for the presence of life on the planet K2-18 b, based on chemical clues. The other study argues that such clues can be produced on a lifeless world.

Sometimes an old telescope can still impress. That is certainly the case for Hubble, which is rapidly approaching the 35th anniversary of its launch. To celebrate, the telescope's operators are collaborating with ESA to release a series of stunning new photographs of some of the most iconic astronomical objects the telescope has observed. As of the time of writing, the latest one to be released is a spectacular new image of a favorite of millions of amateur astronomers - the Sombrero Galaxy.

Who knew that magnetic fields could be so useful?

Everything in the Universe spins. Galaxies, planets, stars, and black holes all rotate, even if just a bit. It comes from the fact that the clouds of scattered gas and dust of the cosmos are never perfectly symmetrical. But the Universe as a whole does not rotate. Some objects spin one way, some another, but add them all up, and the total rotation is zero. At least that's what we've thought. But a new study suggests that the Universe does rotate, and this rotation solves the big mystery of cosmology known as the Hubble tension.

Gamma-ray bursts are the most powerful events in the Universe, briefly outshining the combined light of their entire galaxies. A team of astronomers has figured out a clever technique to use the light from gamma-ray bursts to map out the large-scale structure of the Universe at different ages after the Big Bang. They found that the Universe might be less uniform at large scales than previously thought.

The dream of finding life on an alien Earth-like world is hampered by a number of technical challenges. Not the least of which is that Earth is dwarfed by the size and brightness of the Sun. We might be able to discover evidence of life by studying the molecular spectra of a planet's atmosphere as it passes in front of the star, but those results might be inconclusive. The way to be certain is to observe the planet directly, but that would take a space telescope with a mirror 3–4 times that of Webb.

How can astronomers pierce through the interstellar fog of the Milky Way – not to study distant objects, but to understand the fog itself? It just takes a little light.

If skies are clear, be sure to watch for the April Lyrid meteors this Easter weekend. Spring in the northern hemisphere brings with it the promise for the Lyrids, the first good meteor shower of the season. Weather is just warming up in April, but we're not yet in the midst of summer, waiting up late hours for darkness to fall.

How can we successfully collect and return samples from Mercury and Venus to Earth? This is what a recent study presented at the 56th Lunar and Planetary Science Conference hopes to address as a pair of researchers from the California Institute of Technology (Caltech) discussed how future missions could successfully conduct sample return missions from the two innermost planets in our solar system. This study has the potential to help scientists, engineers, and mission planners better understand new methods for conducting sample returns throughout the solar system, and specifically from hard-to-reach destinations.

Our Sun, like all stars, is made mostly of hydrogen and helium. They are by far the most abundant elements, formed in the early moments of the Universe. But our star is also rich in other elements astronomers call "metals." Carbon, nitrogen, iron, gold, and more. These elements were created through astrophysical processes, such as supernovae and neutron star collisions. The dust of long-dead stars that gathered together into molecular clouds and formed new, younger stars such as the Sun. Stars rich in metals. But there are still stars out there that are not metal rich. These extremely metal-poor stars, or EMPs, hold clues to the origin of stars in the cosmos.

When JWST launched, it found the most distant known galaxy: JADES-GS-z14-0, with a redshift of 14.32, and seen about 290 million years after the Big Bang. Now, a team of astronomers has gone even deeper, searching for galaxies in the redshift 15-30 range, which would be galaxies from 270 to 100 million years after the beginning of the Universe. They've found a few candidates in the 15-20 range, but these could be closer, low-mass dusty galaxies.

It's no surprise that the future of humanity and even Earth's biodiversity hangs in the balance and so the race to preserve life on our planet has never been more urgent. Species and ecosystems are vanishing at alarming rate so teams of scientists are turning to cutting-edge solutions to safeguard the natural world for future generations. A new paper explores cryopreservation as one solution, a technology that allows living cells to be frozen and stored for centuries, preserving genetic material and even entire organisms. This approach comes with its own challenges but as we explore this innovative frontier, it becomes clear that reimagining how and where we protect life is essential to securing the planet's biological legacy.

Jupiter's moon Europa is a fascinating target for study. Data from the Galileo spacecraft's Solid State Imager showed that Europa, one of Jupiter's moons, has a geologically young and varied surface featuring formations like pits, spots, and cryolava domes. A new study has revealed more about the composition of the cryovolcanoes and their domes but also and more excitingly perhaps that they may even provide some form of habitation as we explore the Solar System!

The search for life involves the most sophisticated observational machines known to humanity. They peer out across the light-years, looking for some proof - any proof - that other life exists, out there. What if, despite all our efforts, those observations turn up NO evidence of life elsewhere in our Milky Way Galaxy?

Titan is Saturn's largest moon, with a thick atmosphere and liquid methane lakes, making it the only place besides Earth with stable liquid on its surface. A new paper reveals how a team of researchers have compared real craters on Titan with computer-simulated ones to determine the thickness of its icy shell. This information is important for understanding Titan's interior structure, how it evolved thermally, and its potential to produce organic molecules, making it significant for astrobiological research.

NGC 1514 is a planetary nebula about 1500 light years away. William Herschel discovered it in 1790, and its discovery made him rethink the nature of nebulae. It's been imaged many times by modern telescopes, and each time a more capable one revisits it, astronomers learn more about it. The JWST is the latest to observe the curious nebula, and its observations help explain the unusual object.

We've long known that black holes can produce powerful jets of ionized gas. These jets stream away from the black hole at nearly the speed of light. Jets produced by supermassive black holes are so powerful they are seen as quasars from billions of light-years away. But when you think about it, jets are a bit counterintuitive. Black holes trap and consume material through their tremendous gravity, so how can they push streams of material away? A recent study in Publications of the Astronomical Society of Japan shows how it works.

Whether your views on climate change are informed by politics or science, it's getting harder to ignore it's effects on our lives down here on Earth. But a surprising study reports that increasing concentrations of greenhouse gases in our atmosphere could also be affecting the problem of space junk. As the heat energy stored in our atmosphere increases, its ability to scrub debris from Low-Earth Orbit (LEO) decreases, increasing the risk of satellite collisions and making it more likely that humanity could lose access to space entirely.

One of the challenges of searching for life in the Universe is that there is no single universal biosignature that could reveal its presence. Even if we could tell the difference between chemicals produced by living organisms and those from non-living sources like volcanoes, we're still making the assumption that alien life would resemble life on Earth. A new paper proposes that missions search for "energy-ordered resource stratification" which only happens when both self-replication and ecological competition are present.