Mars Express Captures Dozens of Dust Devils in Mars Valley
The European Space Agency’s Mars Express has captured part of Mars’s Mamers Valles: a fascinating valley system speckled with brief, tornado-like whirlwinds known as dust devils.
Key points
- Focus: The European Space Agency’s Mars Express has captured part of Mars’s Mamers Valles: a fascinating valley system speckled with brief, tornado-like
- Detail: Science reporting: verify primary technical documentation
- Editorial reading: science reporting; whenever possible, verify the cited primary source.
The European Space Agency’s Mars Express has captured part of Mars’s Mamers Valles: a fascinating valley system speckled with brief, tornado-like whirlwinds known as dust devils. The science-journalism coverage adds useful context, while the strongest evidential footing still comes from the underlying data, papers or institutional documentation.
That matters because astronomy does not advance on single detections. The field builds confidence by accumulating independent observations across different wavelengths, instruments and epochs until isolated signals become defensible conclusions. What looks convincing in one dataset can dissolve when a second instrument looks at the same target, and what looks marginal can solidify when follow-up campaigns confirm the original reading. The current standard requires that a result survive this triangulation before the community treats it as settled. Dust devils are a regular feature on Mars. Just like those found on Earth, these mini whirlwinds form when parts of Mars are warmed by the Sun, causing air above the surface to swirl upward, carrying dust with it.
But in Mars' lower gravity (38% that of Earth), these devils grow much larger, reaching up to 8 km (5 mi) in height and achieving speeds of up to 45 meters per second (150 ft/s). They are also a major part of Mars' meteorological cycles, playing a key role in distributing dust across the planet.
When passing above Mamers Valles, a set of channels in a winding canyon system etched into the cratered northern uplands of Arabia Terra, the ESA's Mars Express probe spotted. The image (shown above) was taken by the High Resolution Stereo Camera (HRSC), one of eight instruments aboard the *Mars Express* that has been mapping the surface of the Red.
The image (at top) was created by combining sequential views from the High Resolution Stereo Camera (HRSC), using up to nine separate camera channels. The channels in Mamers Valles extend for around 1, 000 km (660 mi) from Mars's ancient southern highlands into the planet's northern lowlands and measure up to 25 km (15.
What gives the story weight is not just the object itself, but the way the measurement trims the range of plausible physical explanations. Astronomy has accumulated enough cases to know that the most interesting results are rarely the ones that confirm expectations cleanly; they are the ones that confirm some expectations while complicating others, or that open a parameter space that previous instruments could not reach. The scientific community evaluates these contributions by asking whether the new data constrain a model in a way that older data could not, and whether those constraints survive systematic review.
Some of the channels are lined with dark material, which is believed to be volcanic sands, some of which may have been deposited by wind. This is consistent with the valley's age, which is dated to the late Noachian period (ca.
Because this item comes through Universe Today as science journalism, it should be treated as contextual reporting rather than primary evidence. Good science reporting can identify why a result matters, connect it to the wider literature and make technical work readable, but the decisive evidence remains in the original paper, dataset, mission release or technical record. That distinction is especially important when a story is later repeated by aggregators, because repetition increases visibility, not evidential strength.
The next step is to see whether other instruments and other wavelengths tell the same story. Campaigns with JWST, the VLT, the forthcoming Extremely Large Telescopes and radio arrays will provide the spectral coverage and spatial resolution needed to move from detection to physical characterization. The timeline for that kind of confirmation is typically measured in years, not months, which is worth keeping in mind when reading the current result.
Original source: Universe Today