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NASA on Tuesday celebrated exceeding expectations during a mission to deflect a distant asteroid, in a sci-fi like test of humanity’s ability to stop an incoming cosmic object from devastating life on Earth.

The fridge-sized Double Asteroid Redirection Test (DART) impactor deliberately smashed into the moonlet asteroid Dimorphos on September 26, pushing it into a smaller, faster orbit around its big brother Didymos, NASA chief Bill Nelson announced.

That changed its orbital period by four percent, or 32 minutes — from 11 hour 55 minutes to 11 hours 23 minutes, bettering an expectation of 10 minutes.

“At some point in the future, if we find an asteroid that is threatening to hit Earth, and would be large enough to really do some damage, thank goodness that we will have had this successful test,” Nelson told AFP.

The asteroid pair loop together around our Sun every 2.1 years, and pose no threat to our planet.

But they are ideal for studying the “kinetic impact” method of planetary defense.

DART’s success as a proof-of-concept has made a reality what was once science fiction — notably films such as “Armageddon,” “Deep Impact,” and “Don’t Look Up.”

Never actually photographed before, Dimorphos, which is 530 feet (160 meters) in diameter or roughly the size of a big Egyptian pyramid, appeared as a speck of light around an hour before impact.

Its egg-like shape and craggy, boulder-dotted surface finally came into clear view in the last few moments, as DART raced toward it at roughly 14,500 miles (23,500 kilometres) per hour.

Pseudo-comet 

In the days that followed, astronomers rejoiced in stunning images of matter spreading out thousands of miles — pictures collected by Earth and space telescopes, as well as a tiny companion satellite that traveled to the zone with DART.

Thanks to its temporary new tail, Dimorphos has turned into a man-made comet.

But quantifying just how well the test worked required an analysis of light patterns from ground telescopes, which took a few weeks to become apparent.

The binary asteroid system, which was around 6.8 million miles (11 million kilometres) from Earth at impact, is visible only as a single dot from the ground.

The dot’s brightness changes as Dimorphos passes in front of Didymos, which is significantly bigger at half-a-mile wide.

Four optical telescopes were involved in measuring the orbital period — all in Chile and South Africa — while two US-based radar telescopes helped confirm the finding, said NASA planetary scientist Nancy Chabot.

The test also showed scientists that the asteroid is less like a solid rock, and more like a “rubbish pile” of boulders bound by mutual gravity.

If an asteroid is more solid, the momentum imparted by a spaceship will be limited. But if significant mass is pushed at high velocity in the opposite direction to impact, there will be an additional boost.

“It looks like the recoil from the ejecta blast off the surface was a substantial contributor to the overall push given to the asteroid,” said NASA scientist Tom Statler at a briefing.

The test will serve as an “anchor point” for simulations and calculations about the outcome of future impacts, he added.

Mass extinction

No known asteroid larger than 140 meters (460 feet) in size — big enough to devastate a city — has a significant chance to hit Earth for the next 100 years, according to NASA.

But wait long enough, and it will happen.

The geological record shows, for example, that a six-mile wide asteroid struck Earth 66 million years ago, plunging the world into a long winter that led to the mass extinction of the dinosaurs along with 75 percent of all species.

The agency plans to launch in 2026 a telescope called the Near-Earth Object (NEO) Surveyor to better characterize potentially hazardous 140-meter asteroids and comets that come within 30 million miles.

So far, less than half of the estimated 25,000 NEOs of 140 meters have been discovered.

Kinetic impact with a spaceship is just one way to defend the planet, albeit the only method possible with current technology.

Should an approaching object be detected early, a spaceship could be sent to fly alongside it for long enough to divert its path via using the ship’s gravitational pull, creating a so-called gravity tractor.

Another option would be launching nuclear explosives to redirect or destroy an asteroid.

NASA believes the best way to deploy such weapons would be at a distance, to impart force without blowing the asteroid to smithereens, which could further imperil Earth.


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Is the Wheel of Ghosts an Ancient Observatory? New Study Suggests Otherwise

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Is the Wheel of Ghosts an Ancient Observatory? New Study Suggests Otherwise

The ancient Rujm el-Hiri site, situated in the Golan Heights and often referred to as the “Wheel of Ghosts,” has been re-evaluated, with its long-standing identification as an astronomical observatory coming under scrutiny. Researchers have determined that geodynamic changes over millions of years have altered the site’s orientation, raising questions about its original purpose. These findings, derived from advanced geophysical and remote sensing techniques, provide a new perspective on this enigmatic archaeological structure.

Geophysical Insights Challenge Established Theories

According to the study published in Remote Sensing, geodynamic movements averaging 8–15 millimetres per year over 150 million years shifted the site’s alignment significantly. Researchers from Tel Aviv University and Ben-Gurion University, led by Dr Olga Khabarova and Prof Lev Eppelbaum, concluded that the structure’s current orientation does not match celestial patterns, contradicting earlier interpretations of its function. The entrances and radial walls, when reconstructed to their original positions, were shown to lack alignment with solstices, equinoxes, or other astronomical markers.

Advanced Techniques Reveal Archaeological Landscape

As reported by SciTech Daily, the researchers employed geomagnetic analysis and satellite technology to document the surrounding archaeological features within a 30-kilometre radius of the Sea of Galilee. Unique circular structures, some up to 90 metres in diameter, were identified alongside burial mounds and round enclosures. These findings suggest agricultural and herding purposes rather than purely ceremonial or observational roles.

A Broader Perspective on Rujm el-Hiri’s Role

Dr Michal Birkenfeld of Ben-Gurion University emphasised in his statement to SciTech Daily that this reassessment enriches understanding of ancient life in the Golan Heights. The research team noted that the study reopens debates about the site’s purpose while highlighting its integration into a broader archaeological landscape. By questioning past assumptions, the study encourages further exploration of how ancient communities interacted with their environment.

Catch the latest from the Consumer Electronics Show on Gadgets 360, at our CES 2025 hub.


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Scientists Investigate Hypernuclei To Understand Subatomic Forces and Neutron Stars

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Scientists Investigate Hypernuclei To Understand Subatomic Forces and Neutron Stars

A breakthrough has been reported in particle physics, focusing on hypernuclei—rare atomic systems that form through the inclusion of hyperons, particles containing at least one “strange” quark. Unlike the ordinary nuclei of atoms made of protons and neutrons, hypernuclei exhibit unique properties that may offer insights into subatomic forces and the extreme conditions present in neutron stars. Scientists aim to deepen the understanding of these fleeting structures and their implications for astrophysics and nuclear physics.

Insights from Advanced Research

According to a study published in The European Physical Journal A, researchers led by Ulf-G. Meißner from the Institute for Advanced Simulation in Jülich and the University of Bonn applied nuclear lattice effective field theory to investigate hypernuclei. This approach simplifies the study of nuclear interactions by focusing on protons, neutrons, and hyperons rather than quarks and gluons, providing a computationally feasible way to study these particles.

This study specifically examined Λ-hyperons, one of the lightest hyperons, and their interactions within hypernuclei. A lattice-based model was utilised, where particles are simulated within a discrete grid, reducing the complexity of the calculations. Forces governing the structure of hypernuclei were calculated, achieving agreement with experimental data within a 5 percent margin of accuracy. The method also allowed the study of hypernuclei with up to 16 constituents, expanding the scope of earlier models.

Implications for Neutron Stars

Hypernuclei are theorised to form in neutron stars due to the immense pressure and density in their cores. The measurable properties of neutron stars, such as mass and radius, could be influenced by the presence of hyperons. By using advanced X-ray telescopes and gravitational wave detectors, scientists hope to detect deviations from existing models, potentially confirming hyperons’ role in these environments.

Further research is required to refine models and explore pion exchanges, which may alter the forces within hypernuclei. Enhanced experimental data and precision in accelerator experiments are expected to contribute to this field in the future.

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Mathematicians Uncover Science Behind Hula Hooping and Body Dynamics

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Mathematicians Uncover Science Behind Hula Hooping and Body Dynamics

The mechanics of hula hooping have been analysed by researchers, uncovering how body shapes and motions influence the ability to keep a hoop spinning against gravity. Insights from the study have raised intriguing questions about body dynamics, energy efficiency, and potential engineering applications. The findings, based on experiments and mathematical modelling, offer new perspectives on an activity often overlooked in scientific research. Key revelations include the role of body curvature and slope in maintaining the hoop’s motion.

Study Details Dynamics of Hula Hooping

According to research published in the Proceedings of the National Academy of Sciences, experiments were conducted using miniature robotic models at New York University’s Applied Mathematics Laboratory. Different shapes, such as cylinders, cones, and hourglasses, were replicated at one-tenth human scale to examine their impact on hula hooping efficiency. Motorised motions were applied to these models, and high-speed cameras captured the behaviour of hoops launched onto the robotic forms.

Findings indicated that successful twirling could be achieved without significant variation based on body cross-section shapes, such as circles or ellipses. However, maintaining the hoop’s height against gravity required specific physical attributes, particularly sloping hips and a curvy waist. These characteristics provided the necessary angles for upward thrust and stability, helping to keep the hoop in motion.

Mathematical Modelling and Broader Applications

Senior researcher and associate professor Leif Ristroph explained in a press release that mathematical models were developed to explain the physical principles observed. These models offered insight into the interaction between body motion and hoop dynamics, which could be extended to applications such as energy harvesting and robotics.

The researchers highlighted that the work bridges a gap in the understanding of a popular activity, while also demonstrating its relevance to technology. Ristroph noted that these findings could lead to improvements in robotic systems used in manufacturing, as well as innovative ways to utilise energy generated by vibrations.

This research sheds light on the science behind hula hooping, offering practical applications while enhancing the understanding of human and mechanical motion.

Catch the latest from the Consumer Electronics Show on Gadgets 360, at our CES 2025 hub.

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