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In a world first, NASA has crashed a spacecraft into an asteroid in an attempt to push the rocky traveler off its trajectory. The Double Asteroid Redirection Test – or DART – is meant to test one potential approach that could prevent an asteroid from colliding with Earth. David Barnhart is a professor of astronautics at the University of Southern California and director of the Space Engineering Research Center there. He watched NASA’s live stream of the successful mission and explains what is known so far.

1. What do the images show?

The first images, taken by a camera aboard DART, show the double asteroid system of Didymos – about 2,500 feet (780 meters) in diameter – being orbited by the smaller asteroid Dimorphos that is about 525 feet (160 meters) long.

As the targeting algorithm on DART locked onto Dimorphos, the craft adjusted its flight and began heading towards the smaller of the two asteroids. The image taken at 11 seconds before impact and 42 miles (68 kilometers) from Dimorphos shows the asteroid centered in the camera’s field of view. This meant that the targeting algorithm was fairly accurate and the craft would collide right at the center of Dimorphos.

The second-to-last image, taken two seconds before impact shows the rocky surface of Dimorphos, including small shadows. These shadows are interesting because they suggest that the camera aboard the DART spacecraft was seeing Dimorphos directly on but the Sun was at an angle relative to the camera. They imply the DART spacecraft was centred on its trajectory to impact Dimorphos at the moment, but it’s also possible the asteroid was slowly rotating relative to the camera.

The final photo, taken one second before impact, only shows the top slice of an image but this is incredibly exciting. The fact that NASA received only a part of the image implies that the shutter took the picture but DART, traveling at around 14,000 miles per hour (22,500 kilometers per hour) was unable to transmit the complete image before impact.

2. What was supposed to happen?

The point of the DART mission was to test whether it is possible to deflect an asteroid with a kinetic impact – by crashing something into it. NASA used the analogy of a golf cart hitting the side of an Egyptian pyramid to convey the relative difference in size between tiny DART and Dimorphos, the smaller of the two asteroids. Prior to the test, Dimorphos orbited Didymos in roughly 16 hours. NASA expects the impact to shorten Dimorphos’ orbit by about 1 percent or roughly 10 minutes. Though small, if done far enough away from Earth, a nudge like this could potentially deflect a future asteroid headed towards Earth just enough to prevent an impact.

3. What do we know already?

The last bits of data that came from the DART spacecraft right before impact show that it was on course. The fact that the images stopped transmitting after the target point was reached can only mean that the impact was a success.

While there is likely a lot of information to be learned from the images taken by DART, the world will have to wait to learn whether the deflection was also a success. Fifteen days before the impact, DART released a small satellite with a camera that was designed to document the entire impact. The small satellite’s sensors should have taken images and collected information, but given that it doesn’t have a large antenna onboard, the images will be transmitted slowly back to Earth, one by one, over the coming weeks.

4. What does the test mean for planetary defense?

I believe this test was a great proof-of-concept for many technologies that the US government has invested in over the years. And importantly, it proves that it is possible to send a craft to intercept with a minuscule target millions of miles away from Earth. From that standpoint DART has been a great success.

Over the course of the next months and years, researchers will learn just how much deflection the impact caused – and most importantly, whether this type of kinetic impact can actually move a celestial object ever so slightly at a great enough distance to prevent a future asteroid from threatening 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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