Space News & Blog Articles

One of the most difficult parts of astronomy is understanding how time affects it. The farther away you look in the universe, the farther back you look in time. One way this complicates things is how objects might change over time. For example, a supermassive black hole at the center of a galaxy in the early universe might appear one way to our modern telescopes, but the same supermassive black hole might appear completely differently a few billion years later. Understanding the connection between the two objects would be difficult to say the least, but a new prerint paper on arXiv from researchers at the University of Science and Technology in South Korea describes one potential parallel, between the recently discovered “Little Red Dots” of the early universe and “BlueDOGs” of the slightly later universe.

In astronomy, some of the most profound discoveries happen by accident. As the saying goes, "The most exciting phrase in science is not 'eureka!' but 'that's funny.'" This was certainly the case with Matus Rybak - a postdoctoral researcher at Leiden University - and his colleagues were observing RXJ1131-1231, a quasar located 6 billion light-years away in the constellation Crater. This active galactic nucleus (AGN) is a favorite among astronomers because of the supermassive black hole (SMBH) at its center and the fact that there is an intervening galaxy between it and Earth.

Water is key to life as we know it. But that doesn’t mean its key to life everywhere. Despite the fact that the ability to house liquid water is one of the key characteristics we look for in potentially habitable exoplanets, there is nothing written in stone about the fact that life has to use water as a solvent as opposed to other liquid options. A new paper from researchers at MIT, including those who are developing missions to look for life on Venus, shows there might be an alternative - ionic liquids that can form and stay stable in really harsh conditions.

The Taurus star-forming region is only a few hundred light-years away, and it may be the nearest star formation region to Earth. It's a stellar nursery with hundreds of young stars, and attracts a lot of astronomers' attention. One of the young stars in Taurus is named IRAS 04302. IRAS 04302 is sometimes called the "Butterfly Star" because of its appearance when viewed edge-on.

Around 11,300 years ago, a massive star teetered on the precipice of annihilation. It pulsed with energy as it expelled its outer layers, shedding the material into space. Eventually it exploded as a supernova, and its remnant is one of the most studied supernova remnants (SNR). It's called Cassiopeia A (Cas A) and new observations with the Chandra X-ray telescope are revealing more details about its demise.

When the James Webb Space Telescope (JWST) began science operations, one of its first tasks was to observe the earliest galaxies in the Universe. These observations revealed a huge population of active galactic nuclei (AGNs) that astronomers nicknamed "Little Red Dots" (LRDs), owing to their small appearance and deep red hue. Based on redshift measurements, these AGNs are estimated to have existed just 0.6 to 1.6 billion years after the Big Bang (13.2 to 12.2 billion years ago). Studying these objects has already triggered some groundbreaking discoveries about the early Universe.

Life is complicated, and not just in a philosophical sense. But one simple thing we know about life is that it requires energy, and to get that energy it needs certain fundamental elements. A new paper in preprint on arXiv from Giovanni Covone and Donato Giovannelli from the University of Naples discusses how we might use that constraint to narrow our search for stars and planets that could potentially harbor life. To put it simply, if it doesn’t have many of the constituent parts of the “building blocks” of life, then life probably doesn't exist there.

What role can the relationship between oxygen (O2) and ozone (O3) in exoplanet atmospheres have on detecting biosignatures? This is what a recent study submitted to Astronomy & Astrophysics hopes to address as an international team of researchers investigated novel methods for identifying and analyzing Earth-like atmospheres. This study has the potential to help scientists develop new methods for identifying exoplanet biosignatures, and potentially life as we know it.

When NASA's OSIRIS-REx spacecraft returned from its mission to asteroid Bennu in 2023, it brought back more than just ancient space rocks, it delivered answers to puzzles that have baffled astronomers for years. Among the most intriguing questions was why asteroids that should look identical through telescopes appear strikingly different colours from Earth.

The Butterfly Nebula, officially known as NGC 6302, earned its name from its distinctive wing like lobes that spread in opposite directions from a central dusty band. This striking shape isn't just beautiful, it’s a natural laboratory where scientists can study the very processes that create the raw materials for rocky planets like Earth.

All (or at least most) astronomical eyes are on 3I/ATLAS, our most recent interstellar visitor that was discovered in early July. Given its relatively short observational window in our solar system, and especially its impending perihelion in October, a lot of observational power has been directed towards it. That includes the most powerful space telescope of them all - and a recent paper pre-printed on arXiv describes what the James Webb Space Telescope (JWST) discovered in the comet’s coma. It wasn’t like any other it had seen before.

The recent discovery of the third known interstellar object (ISO), 3I/ATLAS, has brought about another round of debate on whether these objects could potentially be technological in origin. Everything from random YouTube channels to tenured Harvard professors have thoughts about whether ISOs might actually be spaceships, but the general consensus of the scientific community is that they aren’t. Overturning that consensus would require a lot of “extraordinary evidence”, and a new paper led by James Davenport at the DiRAC Institute at the University of Washington lays out some of the ways that astronomers could collect that evidence for either the current ISO or any new ones we might find.

What processes are responsible for our Sun’s solar wind, heat, and energy? This is what a recent study published in Physical Review X hopes to address as a team of researchers presented evidence for a newly discovered type of barrier that the Sun exhibits that could help explain the transfer of energy to heat within the Sun’s outer atmosphere. This study has the potential to help scientists better understand the underlying mechanisms for what drives our Sun and what this could mean for learning about other suns throughout the cosmos.

What can binary star systems teach astronomers about the formation and evolution of planets orbiting them? This is what a recent study published in Nature hopes to address as a team of scientists investigated past studies that claimed a specific binary star system could host a planet demonstrating a retrograde orbit, meaning it orbits in the opposite direction of the star’s rotation. This study has the potential to help scientists better understand binary and multiple star systems, specifically the formation and evolution of their planets and what this could mean for finding life beyond Earth.

Scientists from the University of Minnesota have discovered something extraordinary in Jupiter's polar regions that has never been seen before, a completely new type of plasma wave that creates aurora unlike anything we observe on Earth.

For astrobiologists, the search for life beyond our Solar System could be likened to where one would look in a vast desert where there's water. The most intriguing targets are planets called sub-Neptunes, which get their name because they're larger than Earth but smaller than Neptune. What makes them fascinating is that their size and mass suggest they're packed with water but not the kind of water we know.

On August 8, 2024, the NSF Daniel K. Inouye Solar Telescope in Hawaii achieved a historic milestone by capturing the sharpest images ever taken of a solar flare. The unprecedented observations revealed coronal loops in stunning detail. The arches of superheated plasma following the Sun's magnetic field lines were captured at such resolution that it’s possible to see individual structures as narrow as 21 kilometres across.

The ESA's JUpiter Icy Moons Explorer (JUICE) is on its way to conduct detailed studies of Jupiter and its three icy moons, Ganymede, Callisto, and Europa. To pick up speed and reach Jupiter by July 2031, the probe will conduct a gravity-assist maneuver with Venus on Sunday, August 31st. According to the ESA, the mission suffered an anomaly with its communications system, which temporarily severed its connection with Earth. Fortunately, a coordinated response by teams at the ESA's European Space Operations Centre (ESOC) and Airbus (JUICE's manufacturer) restored communications in time for the probe's flyby.

Astronomers have observed the distant active galaxy OJ 287 for many years. It's a BL Lac object, a type of active galactic nuclei known for their extreme variability. They display rapid and pronounced variability in their brightness across multiple wavelengths.

What can the Galactic Habitable Zone (GHZ), which is a galaxy’s region where complex life is hypothesized to be able to evolve, teach scientists about finding the correct stars that could have habitable planets? This is what a recent study accepted for publication in Astronomy & Astrophysics hopes to address as an international team of researchers investigated a connection between the migration of stars, commonly called stellar migration, and what this could mean for finding habitable planets within our galaxy. This study has the potential to help scientists better understand the astrophysical parameters for finding habitable worlds beyond Earth and even life as we know it.

In space, the one thing more important than ensuring access to food, water, and waste disposal (combined!) is the need for a steady supply of breathable air. Where the International Space Station (ISS) and other missions in Low Earth Orbit (LEO) can be resupplied regularly, missions operating in deep space will need to produce their own. There are several ways to go about this. One way is to use bioregenerative life support systems (BLSSs), which utilize photosynthetic organisms (like cyanobacteria) that take in carbon dioxide and produce oxygen gas and edible algae.