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NASA’s mission to deflect asteroid is a step towards preparing the world for a potential future asteroid strike like the one which killed the dinosaurs some 66 million years ago, the chances of which are very slim in our lifetime, Indian scientists said.

In a first-of-its-kind mission, the Double Asteroid Redirection Test (DART) spacecraft successfully crashed into an asteroid on Tuesday to test whether space rocks that might threaten Earth in the future could be nudged safely out of the way.

DART – the world’s first planetary defence technology demonstration — targeted the asteroid moonlet Dimorphos, a small body just 160 metres in diameter.

“We are surrounded by several asteroids and comets that orbit our Sun. Very few of them are potentially hazardous to Earth. Hence, It is better to prepare our defenses to avoid such asteroids on a collision course with Earth in the future,” said Chrisphin Karthick, a scientist at the Indian Institute of Astrophysics (IIA), Bengaluru.

Karthick, who is involved in the DART project, noted that the mission “certainly is a step towards” preparing the world for a potential future event like the one which is believed to have led to the extinction of dinosaurs some 66 million years ago.

“This successful DART mission is an example of that. We now know to precisely aim the spacecraft for such a small body. We can also prepare ourselves for the larger body from the post-impact observations of this DART mission,” Karthick told PTI.

Dimorphos orbits a larger 780-metre asteroid called Didymos. Neither asteroid poses a threat to Earth. By comparison, the dinosaur-killing asteroid that hit Earth was about 10 kilometers in diameter.

The DART mission’s one-way trip, confirmed NASA, can successfully navigate a spacecraft to intentionally collide with an asteroid to deflect it, a technique known as kinetic impact.

Goutam Chattopadhyay, a senior scientist at NASA’s Jet Propulsion Laboratory (JPL) in the US also noted that the mission will help to prepare for a future-threatening asteroid.

“DART is an experimental mission to try out a concept of deflecting an asteroid. The idea is, if we can encounter these asteroids whose trajectory is towards us and we do that at a sufficient distance from the Earth, then a minor deflection will be enough to change the path of the asteroid,” he added.

However, scientists noted that most of the asteroids, which are somewhat significant in size and can cause damage on impact with the Earth, have a minuscule chance of hitting the planet.

“However, the probability of that is non-zero and we must always be vigilant. There is always a possibility that a big one might be headed towards us and the question becomes, what would be our approach and how we could mitigate that. That’s why these programs are important,” Chattopadhyay told PTI.

“At least for the next century, there is no such threat from the known asteroids that can cause mass casualties,” said Karthick, adding that this risk assessment is, however, based on the asteroids known to science so far.

Small asteroids are always hitting the Earth all the time but they burn due to the heat generated in the atmosphere. However, for sufficiently large asteroids, that is not the case as the outer core will burn but there will be sufficient mass left to create damage.

The team will now observe Dimorphos using ground-based telescopes to confirm that DART’s impact altered the asteroid’s orbit around Didymos.

Researchers expect the impact to shorten Dimorphos’ orbit by about 1 per cent, or roughly 10 minutes; precisely measuring how much the asteroid was deflected is one of the primary purposes of the full-scale test.

“Post impact, the team will observe Dimorphos using ground-based telescopes to confirm that DART’s impact altered the asteroid’s orbit around Didymos,” Karthick said.

“The expected output of the impact is to shorten Dimorphos’ orbit by about 1 per cent, or roughly 10 minutes. One of the primary goals is to measure the deflection of the asteroid’s orbit,” he added.

However, Chattopadhyay said whether the mission has been able to deflect the orbit of the asteroid will be known only once all the data has been collected.

“I would emphasise that our calculations and small-scale lab experiments show that it might work well,”. he added NASA has a multi prong approach to monitor Near Earth Asteroids (NEAs). The space agency initiated observations program in 1998. Most discoveries are supported by ground-based telescopic surveys, “We primarily use radars and lidars for this. Mostly they are ground-based systems. However, our existing satellites in space are also used to image and track these objects,” the scientist added.

Lidar is a method for determining distance by targeting an object or a surface with a laser and measuring the time for the reflected light.

“The DART mission is humanity’s first attempt to alter the trajectory of an asteroid by crashing a human made object into it. Today’s successful impact is a big step forward in that direction.

“However, to know the eventual success of this concept, we have to wait a few more years by when any significant change in the trajectory would be clearly apparent,” said Dibyendu Nandi, space scientist at Indian Institutes of Science Education and Research, Kolkata.


Buying an affordable 5G smartphone today usually means you will end up paying a “5G tax”. What does that mean for those looking to get access to 5G networks as soon as they launch? Find out on this week’s episode. Orbital is available on Spotify, Gaana, JioSaavn, Google Podcasts, Apple Podcasts, Amazon Music and wherever you get your podcasts.

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Scientists Recreate Cosmic Ray Physics Using Cold Atom in New Laboratory Study

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Scientists Recreate Cosmic Ray Physics Using Cold Atom in New Laboratory Study

For the first time, researchers have managed to simulate a fundamental process of cosmic particle acceleration in a laboratory: the first series of discoveries that will transform our understanding of cosmic rays. Now, scientists from the Universities of Birmingham and Chicago have created a tiny, 100-micrometre Fermi accelerator, in which mobile optical potential barriers collide with trapped atoms, in a partial replica of how cosmic particles pick up energy in space. The technique not only replicates cosmic ray behaviour but also sets a new benchmark in quantum acceleration technology.

Lab-Built Fermi Accelerator Using Cold Atoms Validates Cosmic Ray Theory and Advances Quantum Tech

As per findings published in Physical Review Letters, this fully controllable setup demonstrated particle acceleration through the Fermi mechanism first proposed by physicist Enrico Fermi in 1949. Long theorised to underlie cosmic ray generation, the process had never been reliably replicated in a lab. By combining energy gains with particle losses, researchers created energy spectra similar to those observed in space, offering the first direct validation of Bell’s result, a cornerstone of cosmic ray physics.

In Fermi acceleration, ultracold atoms are accelerated to more than 0.5 metres per second using laser-controlled barriers. Dr Amita Deb, a coauthor and researcher at the University of Birmingham, mentioned, ‘Our chimney is more powerful than conventional quantum nano-measurements, which are the best acceleration tools in the world so far, and while its simplicity and small size can be compelling, its lack of a theoretical speed limit is the most attractive feature.’ The ultracold atomic jets could be readily controlled with high precision in the subsequent experiments.

This progress means that, for the first time, complicated astrophysical events like shocks and turbulence can be studied in a laboratory, lead author Dr Vera Guarrera stated. This opens new avenues for high-energy astrophysics and also for applications in quantum wavepacket control and quantum chemistry.

Researchers plan to find out how different behaviour affects energy cutoffs and acceleration rates. A compact Fermi accelerator of this type could be a cornerstone for studies of fundamental physics and also connect to emerging technologies such as atomtronics.

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Scientists Say Dark Matter Could Turn Failed Stars Into ‘Dark Dwarfs’

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Scientists Say Dark Matter Could Turn Failed Stars Into ‘Dark Dwarfs’

Astronomers now propose that “failed stars” known as brown dwarfs could be powered by dark matter. Dark matter makes up about 85 percent of the universe’s matter but does not shine; it interacts only via gravity. Brown dwarfs form like stars but lack enough mass to ignite fusion. The theory suggests brown dwarfs in galaxy centers might trap dark matter in their interiors. When that dark matter annihilates, it releases energy that heats the star, turning the dwarf into a brighter “dark dwarf.” If such objects exist, finding them would give scientists a new clue to the nature of dark matter.

Dark Matter in Failed Stars

According to the new model, dense brown dwarfs at the centers of galaxies act like gravity wells that accumulate dark matter. Because dark matter interacts only via gravity, it naturally drifts to galactic cores, where it can be captured by star. As University of Hawai‘i physicist Jeremy Sakstein explains, once inside a star dark matter can annihilate with itself, releasing energy that heats the dwarf. The more dark matter a brown dwarf collects, the more energy it outputs. Crucially, this effect only works if dark matter particles self-annihilate (as with heavy WIMPs); lighter or non-interacting candidates like axions would not create dark dwarfs.

They propose using a chemical signature: a dark dwarf should hold on to lithium-7 that normal brown dwarfs burn away. The researchers say powerful telescopes like NASA’s James Webb Space Telescope might already be sensitive enough to spot cool, dim dark dwarfs near the Milky Way’s center. Detecting even one would strongly suggest that dark matter is made of heavy, self-interacting particles (like WIMPs).

In related work, Colgate astrophysicist Jillian Paulin coauthored studies of ancient “dark stars” fueled by dark matter, while SLAC physicist Rebecca Leane and collaborators have shown that dark matter capture could heat brown dwarfs and exoplanets – a process called “dark kinetic heating”. Together, these ideas highlight how even dim, unusual stars could illuminate the nature of dark matter.

For the latest tech news and reviews, follow Gadgets 360 on X, Facebook, WhatsApp, Threads and Google News. For the latest videos on gadgets and tech, subscribe to our YouTube channel. If you want to know everything about top influencers, follow our in-house Who’sThat360 on Instagram and YouTube.


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New Gel-Based Robotic Skin Feels Touch, Heat, and Damage Like Human Flesh

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New Gel-Based Robotic Skin Feels Touch, Heat, and Damage Like Human Flesh

Researchers have created a novel electronic “skin” that could let robots experience a sense of touch. This low-cost, gelatin-based material is highly flexible and durable and can be molded over a robot hand. Equipped with electrodes, the skin detects pressure, temperature changes, and even sharp damage. In tests it responded to pokes, burns and cuts. Unlike conventional designs that use separate sensors for each stimulus, this single “multi-modal” material simplifies the hardware while providing rich tactile data. The findings, published in Science Robotics, suggest it could be used on humanoid robots or prosthetic limbs to give them a more human-like touch.

Multi-Modal Touch and Heat Sensing

According to the paper, unlike typical robotic skins, which require multiple specialized sensors, the new gel acts as a single multi-modal sensor. Its uniform conductive layer responds differently to a light touch, a temperature change or even a scratch by altering tiny electrical pathways. This design makes the skin simpler and more robust: researchers note it’s easier to fabricate and far less costly than conventional multi-sensor skins. In effect, one stretchy sheet of this material can replace many parts, cutting complexity while maintaining rich sensory feedback.

Testing the Skin and Future Applications

The research team tested the skin by casting the gel into a human-hand shape and outfitting it with electrodes. They put it through a gauntlet of trials: blasting it with a heat gun, pressing it with fingers and a robotic arm, and even slicing it open with a scalpel. Those harsh tests generated over 1.7 million data points from 860,000 tiny conductive channels, which fed into a machine-learning model so the skin could learn to distinguish different types of touch.

UCL’s Dr. Thomas George Thuruthel, a co-author of the study, said the robotic skin isn’t yet as sensitive as human skin but “may be better than anything else out there at the moment.” He noted that the material’s flexibility and ease of manufacture as key advantages. Moreover, the team believes this technology could ultimately help make robots and prosthetic devices with a more lifelike sense of touch.

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