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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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A Nearby Supernova May End Dark Matter Search, Claims New Study

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A Nearby Supernova May End Dark Matter Search, Claims New Study

The pursuit of understanding dark matter, which comprises 85 percent of the universe’s mass, could take a significant leap forward with a nearby supernova. Researchers at the University of California, Berkeley, led by Associate Professor of Physics Benjamin Safdi, have theorised that the elusive particle known as the axion might be detected within moments of gamma rays being emitted from such an event. Axions, predicted to emerge during the collapse of a massive star’s core into a neutron star, could transform into gamma rays in the presence of intense magnetic fields, offering a potential breakthrough in physics.

Potential Role of Gamma-Ray Telescopes

The study was published in Physical Review Letters and revealed that the gamma rays produced from axions could confirm the particle’s mass and properties if detected. The Fermi Gamma-ray Space Telescope, currently the only gamma-ray observatory in orbit, would need to be pointed directly at the supernova, with the likelihood of this alignment estimated at only 10 percent. A detection would revolutionise dark matter research, while the absence of gamma rays would constrain the range of axion masses, rendering many existing dark matter experiments redundant.

Challenges in Catching the Event

For detection, the supernova must occur within the Milky Way or its satellite galaxies—an event averaging once every few decades. The last such occurrence, supernova 1987A, lacked sensitive enough gamma-ray equipment. Safdi emphasised the need for preparedness, proposing a constellation of satellites, named GALAXIS, to ensure 24/7 sky coverage.

Axion’s Theoretical Importance

The axion, supported by theories like quantum chromodynamics (QCD) and string theory, bridges gaps in physics, potentially linking gravity with quantum mechanics. Unlike neutrinos, axions could convert into photons in strong magnetic fields, providing unique signals. Laboratory experiments like ABRACADABRA and ALPHA are also probing for axions, but their sensitivity is limited compared to the scenario of a nearby supernova. Safdi expressed urgency, noting that missing such an event could delay axion detection by decades, underscoring the high stakes of this astrophysical endeavour.

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

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Fastest-Moving Stars in the Galaxy May be Piloted by Aliens, New Study Suggests

Intelligent extraterrestrial civilisations might be utilising stars as massive interstellar vehicles to explore the galaxy, according to a theory proposed by Clement Vidal, a philosopher at Vrije Universiteit Brussel in Belgium. His research suggests that alien species could potentially accelerate their binary star systems to traverse vast cosmic distances. While such a concept is purely hypothetical and unproven, Vidal’s recent paper, which has not undergone peer review, raises intriguing possibilities about advanced extraterrestrial engineering.

Concept of Moving Star Systems

The study was published in the Journal of the British Interplanetary Society. As per a report by LiveScience, the idea revolves around the notion that alien civilisations, instead of building spacecraft for interstellar travel, might manipulate entire star systems to travel across the galaxy. Vidal highlights binary star systems, particularly those involving neutron stars and smaller companion stars, as ideal candidates. Neutron stars, due to their immense gravitational energy, could serve as anchors for devices designed to propel the system by selectively ejecting stellar material.

Vidal explained in the paper that uneven heating or manipulation of magnetic fields on a star’s surface could cause it to eject material in one direction. This process would create a reactionary thrust, propelling the binary system in the opposite direction. The concept provides a way to travel while preserving planetary ecosystems, making it a theoretically viable method for species reliant on their home systems.

Known Examples with High Velocities

Astronomers have identified hypervelocity stars, such as the pulsars PSR J0610-2100 and PSR J2043+1711, which exhibit high accelerations. While their movements are believed to be natural phenomena, Vidal suggests they could be worth further investigation to rule out potential artificial influences.

This theory adds an unconventional angle to the search for intelligent life, expanding possibilities beyond traditional methods of exploration like searching for signals or probes. The research underscores the importance of considering advanced and unconventional methods aliens might employ to navigate the galaxy.

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

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Hubble Telescope Finds Unexpectedly Hot Accretion Disk in FU Orionis

NASA’s Hubble Space Telescope has provided new insights into the young star FU Orionis, located in the constellation Orion. Observations have uncovered extreme temperatures in the inner region of its accretion disk, challenging current models of stellar accretion. Using Hubble’s Cosmic Origins Spectrograph and Space Telescope Imaging Spectrograph, astronomers captured far-ultraviolet and near-ultraviolet spectra, revealing the disk’s inner edge to be unexpectedly hot, with temperatures reaching 16,000 kelvins—almost three times the Sun’s surface temperature.

A Star’s Bright Outburst Explained

First observed in 1936, FU Orionis became a hundred times brighter in months and has remained a unique object of study. Unlike typical T Tauri stars, its accretion disk touches the stellar surface due to instabilities. These are caused by the disk’s large mass, interactions with companion stars, or material falling inwards. Lynne Hillenbrand, a co-author from Caltech, in a statement said that the ultraviolet brightness seen exceeded predictions, revealing a highly dynamic interface between the star and its disk.

Implications for Planet Formation

As per a report by NASA, the study holds significant implications for planetary systems forming around such stars. The report further quoted Adolfo Carvalho, lead author of the study, saying that while distant planets in the disk may experience altered chemical compositions due to outbursts, planets forming close to the star could face disruption or destruction. This revised model provides critical insights into the survival of rocky planets in young star systems, he further added.

Future Investigations on FU Orionis

The research team continues to examine spectral emission lines in the collected data, aiming to map gas movement in the star’s inner regions. Hillenbrand noted that FU Orionis offers a unique opportunity to study the mechanisms at play in eruptive young stars. These findings, published in The Astrophysical Journal Letters, showcase the ongoing value of Hubble’s ultraviolet capabilities in advancing stellar science.

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