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NASA’s Double Asteroid Redirection Test (DART) spacecraft is designed to be a one hit wonder. It will end its days by crashing into an asteroid at 24,000 kilometres per hour on September 26. Launched from Earth in November 2021, DART is about the size of a bus and was created to test and prove our ability to defend Earth from a dangerous asteroid.

Landing a direct hit on a target from 11 million kilometres away isn’t easy. But while this sounds far, the asteroid was actually selected by NASA because it is relatively close to Earth. This will give engineers the opportunity to test the spacecraft’s ability to operate itself in the final stages before the impact, as it crashes autonomously.

The target asteroid is called Dimorphos, a body 163 metres in diameter that’s orbiting a 780 metre-wide asteroid called Didymos. This “binary asteroid system” was chosen because Dimorphos is in orbit around Didymos, which makes it easier to measure the result of the impact due to the resulting change in its orbit. However, the Dimorphos system does not currently pose any risk to the Earth.

Regardless, NASA is attempting nothing less than a full scale planetary defence experiment to change an asteroid’s path. The technique being used is called “kinetic impact”, which alters the orbit of the asteroid by crashing into it. That’s essentially what is known as a safety shot in snooker, but played on a planetary level between the spacecraft (as the cue ball) and the asteroid.

A tiny deflection could be sufficient to prove that this technique can actually change the path of an asteroid on a collision path with the Earth.

But the DART spacecraft is going to be completely blown apart by the collision because it will have an impact equivalent to about three tonnes of TNT. In comparison, the atomic bomb dropped on Hiroshima was equal to 15,000 tonnes of TNT.

So, with this level destruction and the distance involved, how will we be able to see the crash? Luckily, the DART spacecraft is not travelling alone on its quest, it is carrying LICIACube, a shoebox-size mini spacecraft, known as a cubesat, developed by the Italian Space Agency and aerospace engineering company Argotec. This little companion has recently separated from the DART spacecraft and is now travelling on its own to witness the impact at a safe distance of 55km.

Never before has a cubesat operated around asteroids so this provides new potential ways of exploring space in the future. The impact will also be observed from Earth using telescopes. Combined, these methods will enable scientists to confirm whether the operation has been successful.

It might, however, take weeks for LICIACube to send all images back to Earth. This period will be utterly nerve wracking – waiting for good news from a spacecraft is always an emotional time for an engineer.

What happens next? An investigation team will look at the aftermath of the crash. These scientists will aim to measure the changes in Dimorphos’ motion around Didymos by observing its orbital period. This is the time during which Dimorphos passes in front and behind Didymos, which will happen every 12 hours.

Ground telescopes will aim to capture images of the Dimorphos’ eclipse as this happens. To cause a significant enough deflection, DART must create at least a 73-second orbital period change after impact – visible as changes in the frequencies of the eclipses.

These measurements will ultimately determine how effective “kinetic impact” technology is in deflecting a potentially hazardous asteroid – we simply don’t know yet.

This is because we actually know very little of the asteroids’ composition. The great uncertainty around how strong Dimorphosis is has made designing a bullet spacecraft a truly enormous engineering challenge. Based on ground observation, the Didymos system is suspected to be a rubble-pile made up of lots of different rocks, but its internal structure is unknown.

There are also great uncertainties about the outcome of the impact. Material ejected afterwards will contribute to the effects of the crash, providing an additional force. We don’t know whether a crater will be formed by the impact or if the asteroid itself will suffer major deformation, meaning we can’t be sure how much force the collision will unleash.

Future missions Our exploration of the asteroid system does not end with DART. The European Space Agency is set to launch the Hera mission in 2024, arriving at Didymos in early 2027 to take a close look at the remaining impact effects.

By observing the deformations caused by the DART impact on Dimorphos, the Hera spacecraft will gain a better understanding of its composition and formation. Knowledge of the internal properties of objects such as Didymos and Dimorphos will also help us better understand the danger they might pose to Earth in the event of an impact.

Ultimately, the lessons from this mission will help verify the mechanics of a high-velocity impact. While laboratory experiments and computer models can already help validate scientists’ impact predictions, full-scale experiments in space such as DART are the closest we will get to the whole picture. Finding out as much as we can about asteroids will help us understand what force we need to hit them with to deflect them.

The DART mission has led to worldwide cooperation among scientists hoping to address the global issue of planetary defence and, together with my colleagues on the DART investigation team, we aim to analyse the impact effects. My own focus will be on studying the motion of the material that is ejected from the impact.

The spacecraft impact is scheduled for September 26 at 19:14 Eastern Daylight Time (00:14 British Summer Time on September 27). You can follow the impact on NASA TV.


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People in Modern Societies Sleep More but Have Irregular Sleep Cycles

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People in Modern Societies Sleep More but Have Irregular Sleep Cycles

A new study challenges the common belief that modern industrialised life results in chronic sleep deprivation. Despite concerns about screen exposure and daily stress impacting sleep quality, findings suggest that individuals in industrialised societies actually sleep longer compared to those in less industrialised settings. Data from multiple studies indicate that sleep duration is higher among people in modern environments, contradicting widely held assumptions. However, while sleep quantity is greater, regular circadian rhythms appear to be more disrupted in these settings.

Study Findings on Sleep Patterns

According to research published in Proceedings of the Royal Society B, anthropologists David Ryan Samson and Leela McKinnon from the University of Toronto Mississauga conducted a meta-analysis of 54 global sleep studies. Their research examined the sleeping habits of 866 healthy adults, revealing that people in hunter-gatherer societies sleep fewer hours on average. Some groups recorded as little as 5.5 hours per night, while the general average in non-industrialised societies was 6.4 hours. In comparison, individuals in industrialised countries averaged over seven hours of sleep nightly.

Efficiency in Sleep and Circadian Rhythm Disruptions

Data also showed that sleep efficiency was higher in industrialised environments. It was reported that 88 percent of time spent in bed was used for sleep, whereas in less-industrialised settings, this figure was lower at 74 percent. Despite this, irregular circadian rhythms were more pronounced in industrialised societies. The circadian function index, which measures regularity in sleep-wake cycles, was recorded at 0.7 in non-industrialised societies but lower at 0.63 in industrialised settings.

Researchers attribute this difference to reduced exposure to natural light cues, which help regulate sleep cycles.

These findings suggest that sleep disturbances in modern environments may not stem from lack of sleep but rather from disrupted biological rhythms.

For details of the latest launches and news from Samsung, Xiaomi, Realme, OnePlus, Oppo and other companies at the Mobile World Congress in Barcelona, visit our MWC 2025 hub.


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New Study Reveals How Pulsars Help Measure Dark Matter in the Milky Way

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New Study Reveals How Pulsars Help Measure Dark Matter in the Milky Way

A new approach to measuring dark matter density in the Milky Way has been introduced by researchers from The University of Alabama in Huntsville (UAH). The study outlines how gravitational acceleration measurements from pulsars can provide insights into the distribution of dark matter in the galaxy. With an expanded dataset including solitary pulsars, scientists have been able to refine their findings, marking a significant advancement in astrophysical research. The ability to measure accelerations at an unprecedented scale has enabled the team to determine local dark matter density with greater accuracy. The findings suggest that in a volume equivalent to Earth, less than 1 kilogram of dark matter is present, highlighting its rarity despite its dominance in the universe’s total mass.

Use of Solitary Pulsars for Dark Matter Measurement

According to the study published on the arXiv preprint server, earlier research relied on binary millisecond pulsars to measure galactic acceleration. Dr. Sukanya Chakrabarti, Pei-Ling Chan Endowed Chair at UAH, explained to Phys.org that most pulsars exist as solitary objects rather than in pairs. By incorporating solitary pulsars into their methodology, the research team has effectively doubled the sample size available for analysis. This expansion allows for a more precise mapping of the Milky Way’s gravitational field, including its dark matter distribution.

Galactic Wobble and Its Role in Measurement

The study also delves into the effects of the Large Magellanic Cloud (LMC) on the Milky Way. Dr. Chakrabarti told Phys.org that the LMC’s gravitational influence creates an imbalance in the Milky Way, leading to an observable wobble. This asymmetry has now been quantified for the first time through pulsar acceleration data. The impact of this gravitational interaction provides further evidence supporting the study’s findings on dark matter distribution.

Addressing Magnetic Braking in Pulsar Acceleration Analysis

A challenge in previous research was accounting for the spindown effect caused by magnetic braking in pulsars. Dr. Tom Donlon, a postdoctoral associate at UAH, explained to Phys.org that binary pulsars were initially used because their orbits remained unaffected by magnetic braking. The latest study has introduced a method to estimate magnetic braking effects with high accuracy, allowing solitary pulsars to be incorporated into acceleration measurements. This advancement broadens the scope of analysis and strengthens the reliability of the findings.

Future Prospects in Dark Matter Research

With the ability to measure accelerations as small as 10 cm/s per decade, the research team believes that mapping the dark matter distribution in the Milky Way with high precision is now within reach. Dr. Chakrabarti stated to Phys.org that while large accelerations near black holes and the galactic center have been measured in the past, this study marks the first time such small accelerations caused by dark matter have been directly observed. The findings contribute significantly to the ongoing efforts to understand the elusive nature of dark matter and its role in shaping the cosmos.

For details of the latest launches and news from Samsung, Xiaomi, Realme, OnePlus, Oppo and other companies at the Mobile World Congress in Barcelona, visit our MWC 2025 hub.


Solar System’s Journey Through Orion Complex May Have Altered Earth’s Climate



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Solar System’s Journey Through Orion Complex May Have Altered Earth’s Climate

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Solar System’s Journey Through Orion Complex May Have Altered Earth’s Climate

The movement of the solar system through the Orion star-forming complex around 14 million years ago may have influenced Earth’s climate, according to scientists. This dense region of space, part of the Radcliffe Wave galactic structure, could have compressed the heliosphere—the protective shield surrounding the solar system—while increasing interstellar dust reaching Earth. Researchers suggest that this influx of cosmic dust might have left traces in geological records, potentially linking galactic activity to past climate changes.

Solar System’s Passage Through the Radcliffe Wave

According to the study published in Astronomy & Astrophysics, an international research team led by the University of Vienna used data from the European Space Agency’s Gaia mission and spectroscopic observations to determine that the solar system moved through the Radcliffe Wave in the Orion constellation between 18.2 and 11.5 million years ago. The most probable period was estimated between 14.8 and 12.4 million years ago. João Alves, Professor of Astrophysics at the University of Vienna and co-author of the study, stated to Phys.org, that this research builds on prior findings regarding the Radcliffe Wave. This structure, made up of interconnected star-forming regions, includes the Orion complex, which the sun is believed to have passed through.

Potential Impact on Earth’s Climate

The study suggests that the increased presence of interstellar dust may have influenced Earth’s atmosphere. Efrem Maconi, lead author and doctoral student at the University of Vienna, said that this dust might have contained traces of radioactive elements from supernovae, which could be detected in geological records using advanced technology in the future.

The solar system’s passage aligns with the Middle Miocene Climate Transition, a period marked by a shift from a warmer, variable climate to a cooler one, leading to the development of Antarctic ice sheets. Scientists highlight that while interstellar dust could have played a role, the dominant factor in this climate change was a long-term decrease in atmospheric carbon dioxide levels.

Not Comparable to Human-Induced Climate Change

Maconi noted that while interstellar dust could have contributed to past climate shifts, the amount required for significant change would need to be much greater than current data suggests. The Middle Miocene Climate Transition unfolded over hundreds of thousands of years, unlike modern climate change, which is occurring rapidly due to human activities

For details of the latest launches and news from Samsung, Xiaomi, Realme, OnePlus, Oppo and other companies at the Mobile World Congress in Barcelona, visit our MWC 2025 hub.

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