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A dust devil looks a bit like a tornado, but is weaker and rarely lasts more than about a minute.

It is a twisting column of warmed air scooting across sun-heated ground, made visible by the dust that it lofts upwards. Although usually benign, occasionally dust devils can kill.

Dust devils have been known to appear on Mars since the 1970s. They have been observed both from the ground and from orbit.

The more dust in the Martian atmosphere, the warmer and more agitated it becomes, and this can escalate into a global dust storm.

When the dust settles, it can coat and disable the solar panels that are essential for many of the instruments we’ve landed on the planet.

There’s a lot we don’t know about how these devils function. But new research, published this week in Nature Communications, has recorded what dust devils sound like – giving fresh insights into how they operate.

But it also raises questions about how future astronauts would detect and interpret sounds on the red planet.

There has been a vast amount of erosion on Mars since the last rivers and lakes vanished, including at the landing sites of both Nasa’s current rovers Curiosity and Perseverance.

Although the erosive power of an individual dust devil is tiny, a billion years worth of dust devils could potentially have worn away kilometres of rock.

There are thus many reasons for wanting to better understand how dust devils function.

And we now know what a Martian dust devil sounds like thanks to the new study led by Naomi Murdoch of Toulouse University in France.

Many passing dust devils have been imaged by cameras on Mars landers and rovers, but Murdoch and her team report a dust devil that luckily passed exactly over the Perseverance rover on September 27, 2021, which was on the floor of Jezero crater.

The rover’s masthead camera, named SuperCam, includes a microphone, and this recorded the sound of the wind rising and falling as the dust devil passed over.

In detail, the wind noise rose when the leading wall of the vortex arrived, followed by a lull representing the calm air in the eye of the vortex, before a second episode of wind noise as the trailing wall of the vortex passed over.

This took less than ten seconds, and you can hear the sound recording here(https://jirafeau.isae-supaero.fr/f.php?h=2JWSkdJR&p=1) (turn your volume to max). Other sensors gave information too. They showed that the pressure fell to a minimum between the two bursts of wind noise – which to me is consistent with sucking rather than blowing – and also recorded impacts of individual dust grains onto the rover.

The dust devil was about 25 metres in diameter, at least 118 metres tall, and was tracking across the ground at about five metres per second.

The maximum wind speed in the rotating vortex was probably just under 11 metres per second, equating to a “fresh” to “strong” breeze on Earth.

Did it really sound like that? Listening to a recording purporting to be the sound of Martian wind is all very well, but is this really what we would hear if we were there ourselves? The first thing to note is that this does genuinely originate as “real sound”, unlike other data such as images or radio signals turned into sound (a process known as sonification), such as the so-called sound of two black holes colliding or radio noise from from Venus’s atmosphere.

The dust devil audio file contains actual sound waves picked up by a microphone on Mars.

There the atmosphere is much thinner than on Earth (Martian surface pressure is less than a hundredth of ours), so the high frequency component of sound hardly carries (scientists say it’s “attenuated”).

The result is that the wind sounds much lower in pitch than a similar wind on Earth.

The only other planetary body from which we have genuine sound recordings is Venus, where in 1982 two Soviet “Venera” landers recorded wind and lander operation noises.

However, if you were on Mars you could never hear the wind directly with your own ears.

If you were foolish enough to expose your ears to Mars’s atmosphere, the low external pressure would cause your eardrums to burst, and you would be instantly deaf as well as having no air to breathe.

If you were to go outside in a pressurised spacesuit (a much more sensible idea), what you would hear would depend on how well the sound waves were transmitted through the solid shell of your helmet, and then on how these were turned back into sound waves in the air inside your helmet.

In other words, you would hear a distorted version of what an external microphone would pick up. Imagine walking round on Earth with your head inside a goldfish bowl and you’ll get part of the idea.

If future human explorers on Mars want to hear what’s going on in the external environment, I suspect they will rely on a suit-mounted microphone feeding to wireless ear buds, although I can’t find any evidence that that this has yet been factored into Mars suit design.

This all boils down to a recording from external microphone being the best way to represent sounds on Mars, or indeed any other planet that has an atmosphere.

If you want to hear some more sounds from Mars, NASA has a collection of audio recordings you can listen to.


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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.

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

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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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