Space News & Blog Articles

Random flashes of radiation in the sky are not all that unusual. A few years ago, once such flash was detected coming from a star that at the time, was believed to be from a star consuming a planet! The exact mechanism was unsure though for example; was it the star bloating up as a red giant and engulfing the planet or did the planet spiral in toward the star? The answer was until now, a little elusive. Observations from the James Webb Space Telescope showed the environment around the star didn’t match a red giant so it must have been the planet crashing into the star!

Promoting Substainable Lunar Bases With Bio-Concrete

The two most prominent satellite galaxies of the Milky Way are the Large and Small Magellanic Clouds. A team of astronomers have recently tracked the movements of 7,000 stars in the Small Magellanic Cloud (SMC) and found that many of them are being pulled away towards the Large Magellanic Cloud! It seems the SMC is being pulled apart, perhaps leading to its eventual destruction as the tidal forces strip away its stars!

One of the things about astronomy that captivates me is that for every question we answer, we open up a whole bunch of other questions. Dark matter and dark energy are one such phenomenon that rather continues to confound us. There’s also the mystery of missing infrared light too but a team of astronomers think they may have found it! The team examined a region of sky using the Herschel Space Telescope and, by staking 141 images, found where individual dust-rich galaxies appeared blended together. The galaxies are absorbing starlight and re-emitting infrared radiation, and is this that may well account for the missing light.

Exploring the Moon with Biologically-Inspired Subsurface Robots

What can exozodiacal dust, also called exozodi, teach astronomers about identifying Earth-like exoplanets? This is what a recently submitted NASA white paper—which highlights key findings from the annual Architecture Concept Review—hopes to address as a team of researchers discussed how exozodi orbiting within a star’s habitable zone (HZ) could interfere with detecting Earth-like exoplanets. This study has the potential to help scientists better understand observational constraints of observing Earth-like exoplanets and what improvements could be made for future telescopes and instruments to overcome these constraints.

The widespread use of low Earth orbit (LEO), especially by thousands of CubeSats, has opened up many opportunities in research and business applications. One particular field that has benefited from the data that CubeSats provide is farming. Precision agriculture (PA) is a technique that uses advanced sensors, including the remote ones on CubeSats, to determine the health and productivity of a farm. A recent review paper from Lamia Rahali and her co-authors at the Mediterranea University of Reggio Calabria's Department of Agriculture looks at how CubeSats have been changing the practice of precision agriculture - and how they may continue to do so.

Newly discovered comet C/2025 F2 SWAN could put on a brief dawn display over the next few weeks. Discovered thanks to the hard work of online sleuths and amateur astronomers, the comet may brighten towards perihelion on May 1st.

Astronomers are on the hunt for those in-between black holes, not the small stellar ones or the supermassive ones, but something right in the middle. Recently, a group of scientists spotted a star travelling at high velocity out of the globular cluster M15. This speedy star got kicked out about 20 million years ago and is now zooming along at an incredible 550 km/s, fast enough that it's actually escaping our entire Galaxy! The researchers think this stellar ejection might have happened because of some cosmic game of pool - basically a three-body interaction involving one of those middle-sized black holes they've been trying to find!

The search for life in our Solar System, however primitive, past or present has typically focussed upon Mars and a select few moons of the outer Solar System. Saturn’s moon Titan for example has all the raw materials for life scattered across its surface, rivers and lakes of methane along with rock and sand containing water ice. There’s even a sprinkling of organic compounds too but according to a new study, Titan can probably only support a few kilograms of biomass overall, that’s just one cell per litre of water across Titan’s ocean.

What kind of mission would be best suited to sample the plumes of Saturn’s ocean world, Enceladus, to determine if this intriguing world has the ingredients to harbor life? This is what a recent study presented at the 56th Lunar and Planetary Science Conference hopes to address as a team of researchers investigated the pros and cons of an orbiter or flyby mission to sample Enceladus’ plumes. This study has the potential to help scientists, engineers, and mission planners design and develop the most scientifically effective mission to Enceladus with the goal of determining its potential habitability.

In the great tug-of-war between the Sun and its planets, Jupiter, Saturn, and Uranus are much more susceptible to solar activities than scientists thought. Jupiter itself has an interesting reaction as it gets pummeled several times a month by solar wind bursts. They compress its magnetosphere and create a huge "hot spot" with temperatures over 500C.

Up until recently, astronomy was reliant entirely on electromagnetic waves. While that changed with the confirmation of gravitational waves in 2016, astronomers had developed fundamental frameworks in the electromagnetic spectrum by that point. One critical framework broke the spectrum into three categories based on their wavelength - infrared, optical, and ultraviolet. To astronomers, each of these categories was created by a different physical phenomenon, and monitoring each gave its insight into what that phenomenon was doing, no matter what the other spectra said. This was especially prevalent when researching galaxies, as infrared and optical wavelengths were used to analyze different aspects of galaxy formation and behavior. However, Christian Kragh Jespersen of Princeton's Department of Astrophysics and his colleagues think they have found a secret that breaks the entire electromagnetic framework - the optical and infrared are connected.

It’s easy to measure the rotation rate of terrestrial planet by tracking surface features but the gas and ice giants pose more of a problem. Instead, previous studies have relied upon indirect measures like measuring the rotation of their magnetic fields. Now a team of astronomers have used the Hubble Space Telescope to refine the rotation rate of Uranus with an incredible level of accuracy. This time though, instead of studying the rotation of the magnetic field, they tracked aurora to measure one rotation!

We all know that black holes can devour stars. Rip them apart and consume their remnants. But that only happens if a star passes too close to a black hole. What if a star gets close enough to a star to experience strong tidal effects, but not close enough to be immediately devoured? This scenario is considered in a recent paper on the arXiv.

In 2021, the Office of the Director of National Intelligence (ODNI) released a report detailing recently-declassified information on Unidentified Aerial Phenomena (UAP). Since then, the Department of Defense has released annual reports on UAP through the All-domain Anomaly Resolution Office (AARO). Nevertheless, there is still a lack of publicly available scientific data on the subject. To address this, a new study led by the Harvard-Smithsonian Center for Astrophysics (CfA) and the Galileo Project proposes an All-Sky Infrared Camera to search for potential indications of extraterrestrial spacecraft.

Familiar Saturn currently provides dawn observers with a bizarre, ‘ring-less’ view.

NGC346 is a young star cluster in the Small Magellanic Clouds with an estimated 2,500 stars. It’s about 200,000 light years away and this image, taken by the Hubble Space Telescope reveals a beautiful region of star formation. The bright blue stars are many times more massive than the Sun and will live short lives ending in spectacular supernova explosions. The image helps us to understand the stellar formation process in a galaxy that has fewer metals than our own Galaxy.

Astronomers have discovered a remarkable star system just 150 light-years from Earth that's destined for a spectacular cosmic display. The system contains a white dwarf star drawing material from its companion star, with the pair orbiting at just 1/60th of the Earth-Sun distance. With their combined mass reaching 1.56 times that of our Sun, these stars are gradually spiralling toward each other, setting the stage for a spectacular explosion. Fortunately, scientists estimate this cataclysmic event won't occur for roughly 23 billion years, long after our own Sun will have reached the end of its life cycle.

Although astronomers have ruled out a smash-up between Earth and an asteroid known as 2024 YR4 in the year 2032, the building-sized space rock still has a chance of hitting the moon. In fact, the chances — slight as they are — have doubled in the past month.

Despite their name, black holes can sometimes emit radiation. A team of astronomers has recently detected a flicker of X-ray radiation from the supermassive black hole at the center of the Andromeda Galaxy. This flicker was identified using 15 years of data from the Chandra X-ray Observatory, revealing two distinct flashes in 2006 and 2013. Interestingly, these flashes coincided with bursts of neutrinos detected by the IceCube Neutrino Observatory, offering exciting new insights into the extreme conditions surrounding the black hole.