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Researchers have teased out the details of how sound behaves at various times and place onMars — and the results are very different from what we are used to on Earth .

NASA’sPerseverance roveron Mars carry several microphone . These devices , think to study the properties of materials on the Red Planet , have picked up all sorts of additional sound , include the eery spluttering of Martiandust monster .

A top down photograph of a large purple-colored mountain on the surface of Mars

Sound on Mars may be the most Earth-like on mountaintops, like the purple mountain seen in this Mars Reconnaissance Orbiter image, according to new research. Elsewhere, the speed of sound varies greatly by location, time of day, and temperature.

Recordings have already shown thatsound behaves peculiarlyon Mars . For example , resound below 240 hertz — around a piano ’s halfway C — travel about 30 feet per 2d ( 10 meters per second ) slower than higher - pitched sound do . This is because C dioxide molecules , which take over some of speech sound ’s energy at grim oftenness , make up 95 % of Mars ' atmosphere . Such flakey properties , if unaccounted for , could compromise communications on next Mars missions , specially crewed ones .

With this in mind , a team of scientists from French and U.S. initiation set out to canvas the speed of sound and its fading — its inclination to die down over distance — within the first 60 foot ( 20 G ) of Mars ' atmosphere .

To commence , the team collate values of different parameter — include atmospheric atmospheric pressure , temperature and chemical substance typography — at various pip on the Red Planet from theMars Climate Database . change in these parameter can stretch or quail sound waves , making these factors essential in predicting sound ’s properties .

A panorama of the surface of mars taken by NASA’s curiousity rover

A composite panorama of Mars taken by NASA’s Curiosity rover at two different times of day — 8:30 a.m. and 4:10 p.m., local Mars time. New research finds that sound moves differently at different times of the day on Mars, as well as at different times of year and at different locations.

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The team calculated profound speed and attenuation at different points of time in the planet ’s year ( which is about 687 Earth days ) and in various spots across the Martian landscape , including mountain peaks and valley . This approaching was necessary because the underlying factor alter massively over space and time .   In the polar neighborhood , for model , noontide temperature can waver by 108 degrees Fahrenheit ( 60 degrees Celsius ) , and carbon dioxide level by 30 % , across seasons .

The figuring turn up several interesting determination , which were published May 7 in theJGR : major planet . For one , debris does n’t seem to impact sound propagation , the writer say in a joint electronic mail to Live Science — standardized to on Earth , where a rubble storm between you and an drome , for deterrent example , would n’t obstruct your power to pick up the planes taking off . The modification in the speed of sound with temperature ( about 0.5 meter / s for every degree Celsius ) is also similar to that on Earth .

a photo of an eye looking through a keyhole

Unlike on Earth , though , legal speed and attenuation look greatly on carbon dioxide levels . Additionally , while the speed of audio rises abruptly at around 240 hertz , the extent of the shimmy is less marked at lower temperatures than at higher ones .

The big difference from Earth , though , stems from the enormous fluctuations in temperature — and , to a lesser extent , the concentration of carbon dioxide — day by day . In the area where the Perseverance roamer currently dwell , for case , mercury level shift by about 90 degrees Fahrenheit ( 50 degrees Celsius ) during the daytime . This causes sound to travel up to 100 feet per second ( 30 m / s ) and choke down three times faster in the hotter hours compare with the stale ones . modification in temperature and C dioxide levels also cause variation in sound hurrying and attenuation across seasons , although this upshot is more marked in the polar realm .

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The consequence permit scientists to " predict the healthy speed and attenuation for any location at the Martian surface at any time of year and any time of day , " the researchers told Live Science . The model can also ameliorate scientists ' understanding of what sound - grow objects on Mars really sound like .

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" We only hear it [ a sound ] after the sound has propagated through the atmosphere , " the writer said . " Our model can help to retrieve the characteristic of the original sound sources . "

Additionally , the model bring home the bacon a coup d’oeil of animation for future human residents on Mars : morning on mountaintops may be the snug thing to the way sound behaves on Earth . At other times and places , like afternoons at the Perseverance web site , a jarring burden will fall out as high up - pitched noises at confining distance arrive at the spike quicker than lower - pitched single ; more distant noises ordinarily audible on Earth wo n’t be heard at all .

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