Space News & Blog Articles

Mars, often called the Red Planet due to its rusty iron oxide covered surface, is Earth's smaller, colder neighbour. Orbiting the Sun at an average distance of 228 million kilometres, Mars shares remarkable similarities with Earth; a 24.6 hour day, polar ice caps, seasons driven by a 25.2 degree axial tilt, and evidence of ancient rivers and lakes that once flowed across its surface. Yet Mars today is a harsh world with a thin atmosphere just 1% the density of Earth's, average temperatures of -63°C, and no liquid water on its surface. It has an incredibly thin atmosphere composed primarily of carbon dioxide (95%) which is so tenuous that liquid water cannot exist on the surface, yet it’s still thick enough to generate global dust storms.

The search for extraterrestrial life may soon get a revolutionary new tool which is no bigger than a soft drink can. A team of Dutch scientists are developing the (Origin of) Life Marker Chip (LMCOOL), a device that could detect signs of life on distant worlds. The LMCOOL is best described as a tiny yet complete laboratory in the form of a computer chip. This device is being developed by a Dutch consortium led by TU Delft, with researcher Jurriaan Huskens and his team working to make the optical sensor particularly sensitive for the required biomarkers.

Tumbleweeds offer iconic visual depictions of desolate landscapes. Though typically associated with the American West, the most common type of tumbleweed actually originated in Europe, and is known scientifically as salsola targus, or more commonly as Russian thistle. So its only fitting that a team led by European scientists has some up with an idea based on the tumbleweed’s unique properties that could one day have groups of them exploring Mars.

The James Webb Space Telescope (JWST) has revealed some amazing things about the Universe. From the earliest galaxies and planet-forming disks to characterizing exoplanet atmospheres, there is virtually no corner of the cosmos that Webb has not observed in extremely high resolution. This includes the Solar System, where Webb has used its sophisticated infrared instruments and spectrometers to provide the most detailed images ever taken of Jupiter, Saturn, the ice giants, and smaller objects like Dimorphos and the latest cosmic interloper detected, 3I/ATLAS.

Radio astronomy began in the 1930s when Karl Jansky, an engineer at Bell Telephone Laboratories, accidentally discovered radio waves coming from the Milky Way. He was investigating sources of interference in transatlantic radio communications, no-one expected this to be the birth of radio astronomy. The finding opened an entirely new window on the universe, one that could peer through clouds, dust and observe phenomena invisible to optical telescopes. The field really took off after World War II when surplus military radar equipment became available to scientists with major discoveries following rapidly from pulsars to quasars, the cosmic microwave background radiation and the detailed structure of galaxies. Today's radio telescopes, from giant single dishes like the 500 metre FAST telescope in China to vast interferometer arrays like the Square Kilometre Array, continue to revolutionise our understanding of the universe.

Rocket propulsion technology has evolved from ancient Chinese gunpowder filled bamboo tubes that shot off into opposing armies to the powerful engines of Saturn V and more recently the Space Launch Vehicle and Falcon 9. The journey progressed through centuries of experimentation by pioneers like Konstantin Tsiolkovsky, Robert Goddard, and Hermann Oberth who laid the foundations for modern rocketry. The space race dramatically accelerated development of new technology, producing the liquid fuelled engines that launched Sputnik, sent humans to the Moon, and built the International Space Station.

Star formation is a fundamental physical process in our Universe. Stars light up the cosmos, and give rise to planets, some of which may support life. While humans have no doubt wondered about stars since prehistoric times, new technological tools like the Milky Way have taken our natural curiosity to a whole new level. Now we can peer inside obscured regions and detect young stars in their dusty cocoons.

Interference from human activity has always been a sticking point in astronomical observations. Radio astronomy is notoriously sensitive to unintentional interference - hence why there are “radio silent” zones near telescopes where cell phones are banned. But gravitational wave astronomy is affected to an even worse degree than radio astronomy, according to a new paper pre-published on arXiv by Reed Essick of the University of Toronto, and it’s not clear there’s much we can do about it.

The heliosphere is a giant bubble created by the Sun, extending far beyond Neptune's orbit and out into interstellar space. Voyager 1 crossed the boundary of the heliosphere (known as the heliopause) in August 2012 and Voyager 2 followed later in November 2018. They were 119 astronomical units from the Sun at the time, that’s 119 times further from the Sun than Earth. It protects us from dangerous levels of radiation and without it, life on Earth would be unlikely to have evolved.

Mysteries abound in the Solar System. Though it can sometimes seem like we've learned a lot, you can pick any object in the Solar System and quickly come up with unanswered questions. That's certainly true of tiny Mercury.

What can exoplanets orbiting M-dwarf stars teach scientists about planetary formation and evolution? This is what a recent study submitted to the American Astronomical Society journals hopes to address as a team of researchers investigated the possibility of exo-Titans, exoplanets with atmospheres comprised of nitrogen and methane like Saturn’s moon Titan, orbiting M-dwarf stars, which are smaller and cooler than our Sun. this study has the potential to help scientists better understand the formation and evolution of exoplanets orbiting M-dwarf stars and whether they could possess life as we know it.

Thanks to missions that have been exploring the Red Planet since the 1970s, it has been established that Mars was once a much different place than what we see there today. Instead of an extremely cold, extremely dry, and irradiated planet with a very thin atmosphere, Mars once has a warmer, denser atmosphere and flowing water on its surface. Between 4.2 and 3.7 billion years ago, the planet began to undergo a transition whereby its atmosphere was slowly tripped by solar wind, causing its water to escape into space, collect in the polar ice caps, and retreat underground.

What is the meaning of life? Even the best of us couldn’t hope to answer that question in a universe today article. But there are those who would try to “constrain” it, at least in terms of physics. A new paper from Pankaj Mehta of Boston University of Jané Kondev of Brandeis that was recently pre-published on arXiv looks at how the fundamental constants of physics might be applied to life as we know it - and even life as we don’t know it yet. Their idea doesn't necessarily give the answer to the ultimate question, but it does tie two seemingly disparate fields nicely together.

One of the JWST's most startling discoveries was that black holes were extremely massive in the early Universe, less than one billion years after the Big Bang. The discovery defied explanation, since astrophysicists thought that it would take much more time for black holes to accrete so much mass. An explanation for this discrepancy may lie in a massive black hole observed with NASA's Chandra X-ray Observatory.

Asteroids are rocky remnants from the early Solar System, chunks of stone and metal that range in size from pebbles to mountains. Most of them orbit peacefully in the asteroid belt between Mars and Jupiter, but occasionally gravitational forces can nudge them toward Earth. The largest asteroid, Ceres, is almost 1,000 km across, while the one that likely killed the dinosaurs was roughly 10 km wide. Even relatively small asteroids can cause tremendous damage for example, the space rock that created Arizona's famous Meteor Crater was only about 45 metres across, yet it generated a crater just over 1km wide.

Exoplanets aren’t the only objects floating around other stars - they likely have comets and asteroids as well. Even some of the exoplanets themselves will have “exomoons”, at least according to our current understanding of the physics of planetary formation. However, we have yet to find any of these other objects conclusively, though there has been some hint at the presence of exomoons in the last ten years. A new paper from astronomers at the European Southern Observatory (ESO), recently pre-published on arXiv, suggests a way in which we might be able to finally detect the presence of an exomoon - using a technique that is also commonly used to find exoplanets themselves.

Some NASA missions are designed for very specific tasks, but all of them help feed into our understanding of our universe, and in some cases our pale blue dot, work. A new mission to study one of the more esoteric parts of the atmosphere is scheduled to launch today, and over the next 2-3 years will monitor the outer reaches of our planet’s atmosphere.

Small fragments of rock can reveal a lot when they're analyzed with powerful laboratory instruments. New research into tiny fragments of the asteroid Ryugu sampled by JAXA's Hayabusa2 mission showed that water flowed through it more than one billion years after it formed. This new insight overturns the previous understanding that asteroids only experienced water activity in the very earliest stages of solar system formation.

How does spaceflight influence sarcopenia, which is a common age-related muscle decline, specifically for elder adults? This is what a recent study published in Stem Cell Reports hopes to address as a team of researchers investigated how microgravity influences muscle cell function. This study has the potential to help scientists, mission planners, astronauts, and the public better understand the long-term health impacts of microgravity on muscle decline and the steps that can be taken to mitigate it.

Space agencies like NASA, the European Space Agency (ESA), the China National Space Agency (CNSA), and others are working to return astronauts to the Moon for the first time since the Apollo Era. Mounting missions beyond Low Earth Orbit (LEO), something that has not happened in over 50 years, presents several major challenges. One of the biggest is that resupply missions take much longer to send to the Moon and require heavier launch vehicles. Whereas the International Space Station can be resupplied in a matter of hours by a Falcon 9, missions bound for the Moon take about three days and require a Space Launch System (SLS) or the Starship.

For over a century, scientists have known that the Universe is rapidly expanding. This phenomenon, named in honor of the astronomers who independently confirmed it (Edwin Hubble and Georges Lemaître), is known as the Hubble-Lemaitre Constant (or the Cosmological Constant). By the 1990s, the Hubble Space Telescope (designed to measure this constant) revealed that the rate at which the Universe was expanding was slower during the early Universe, which was in "tension" with measurements of recent cosmic epochs. This is what led to the "Hubble Tension" in astrophysics and cosmology, and the theory of Dark Energy (DE) as a possible means of explaining the discrepancy.