Monster Volcano Gave Mars Extreme Makeover
Half the size of France, the volcano spewed so much lava 3.5 billion years ago that the weight displaced the Red Planet’s outer layers.
A volcano on Mars half the size of France spewed so much lava 3.5 billion years ago that the weight displaced the Red Planet's outer layers, according to a study released Wednesday.
Mars' original north and south poles, in other words, are no longer where they once were.
The findings explain the unexpected location of dry river beds and underground reservoirs of water ice, as well as other Martian mysteries that have long perplexed scientists, the lead researcher told AFP.
"If a similar shift happened on Earth, Paris would be in the Polar Circle," said Sylvain Bouley, a geomorphologist at Universite Paris-Sud.
"We'd see Northern Lights in France, and wine grapes would be grown in Sudan."
The volcanic upheaval, which lasted a couple of hundred million years, tilted the surface of Mars 20 to 25 degrees, according to the study.
The lava flow created a plateau called the Tharsis dome more than 5,000 square kilometers (2,000 square miles) wide and 12 km (7.5 mi) thick on a planet half the diameter of Earth.
"The Tharsis dome is enormous, especially in relation to the size of Mars. It's an aberration," Bouley said.
This outcropping - upward of a billion billion tonnes in weight - was so huge it caused Mars' top two layers, the crust and the mantle, to swivel around, like the skin and flesh of a peach shifting in relation to its pit.
Already in 2010, a theoretical study showed that if the Tharsis dome were removed from Mars, the planet would shift on its axis.
Bouley and colleagues matched these computer models with simulations and observations - their own and those of other scientists.
Many things on Mars that begged explanation suddenly make sense in light of the new paradigm.
"Scientists couldn't figure out why the rivers" - dry riverbeds today - "were where they are. The positioning seemed arbitrary," Bouley told AFP.
"But if you take into account the shift in the surface, they all line up on the same tropical band."
Likewise the huge underground reservoirs of frozen water ice that should be closer to the poles. Once upon a time, we now know, they were.
The new theory also explains why the Tharsis dome is situated on the "new" equator, exactly where it would need to be for the planet to regain its equilibrium.
The findings, published in Nature, likewise challenge the standard chronology which assumes the Red Planet's rivers were formed after the Tharsis dome.
Most of these ancient waterways would have flowed from the cratered highlands of the Red Planet's southern hemisphere to the low plains of the north even without the massive lava fields, the study concluded.
"But there are still a lot of unanswered questions," cautioned Bouley.
"Did the tilt cause the magnetic fields to shut down? Did it contribute to the disappearance of Mars' atmosphere, or cause the rivers to stop flowing? These are things we don't know yet."
How does the wind blow on Mars? It sounds like a simple question, but scientists are still learning a lot about how that happens. With few meteorological stations on the surface, one of the best
-- vast formations that march across the Martian surface, sometimes as much as several feet per year. In recent months,
for an unprecedented close-up look at these dunes to see, in great detail, how the grains of sand shift. Scientists are trying to figure out mysteries such as why ripples appear larger on some Martian dunes than Earth ones, and why they're of a different texture. Read on to explore some of the most recent findings and past observations of Mars' mysterious dunes.
Image: This observation was imaged by Curiosity's front Hazard Avoidance Camera (Hazcam) on Sol 1184 (Dec. 5) as it carried out a closeup investigation of dunes on the slopes of Mount Sharp.
This is one of the first images ever of a rover next to a large dune on Mars. Previously, NASA Mars Exploration Rovers Spirit and Opportunity were by much smaller ripples. NASA is trying to learn more about how dunes, which are distinguished by steep flanks like the one pictured here, move about on Mars. The challenge is modelling Martian winds and sands, which are obviously not as well-known as what is found on Earth. Curiosity is on the lookout for evidence of sand slides,
-- a season ago in Martian terms.
Image: Panoramic image of the Curiosity rover next to "Namib Dune" on Dec. 18, 2015.
In 2009, the Spirit rover was exploring Gusev Crater -- filled with fluffy regolith -- when it became mired in a sand trap nicknamed "Troy." While not technically a dune, scientific investigations of the region before Spirit got stuck and eventually died showed what sand can hide underneath. In this case, the rover was sitting atop a sulfate deposit, associated with a hydrothermal (steam) vent. The rover's demise showed how difficult it is to predict the composition of sand in even flat regions on Mars.
Image: The Spirit rover captured the region where it got stuck, nicknamed "Troy", in April 2009.
For the last few years, Opportunity has been exploring Endeavour crater on Mars.
, in April 2010. The dunes pictured here are relatively modest -- just 20 centimeters (8 inches) tall. The brighter spot in the foreground is a rock outcrop. Opportunity's controllers changed its route to Endeavour after discovering sand ripples (larger than the ones pictured here) that could have posed a threat to the rover.
Image: Ripples in Endeavour crater as seen by the Opportunity rover in April 2010.
In 2014, the Mars Reconnaissance Orbiter's powerful camera, HiRISE, captured dunes in the extremely active area of Nili Patera. The dunes have been tracked moving an average of 1.7 meters (5.5 feet) in less than four Earth months, according to
. What's even more astonishing is just how big these dunes are: up to 50 meters (164 feet) high. You can see more
Image: Nili Patera, a very active dune field on Mars, caught by the HiRISE camera on the Mars Reconnaissance Orbiter.
Once again, this image shows the amazing extent of dunes on Mars. This image is of the formations in Bunge Crater, taken by NASA Mars Odyssey's thermal emission imaging system in 2006, covering a region about 14 kilometers (9 miles) wide. The dunes are moving towards the left of the picture in this perspective. Scientists are doing their best to understand these processes by using computer models and comparing these dunes with ones on Earth.
Image: Bunge Crater dunes -- described as "fans and ribbons" of dunes by NASA -- take on the appearance of a rough skin on the surface of Mars. Picture taken by Mars Odyssey in January 2006.
This ESA Mars Express picture shows dunes towering in Rabe Crater as high as 200 meters (656 feet) high, nearly twice the height of the Empire State Building. They're mostly made up of basalt (volcanic rock) and have complex geology, according to the European Space Agency: "Its flat floor has a number of smaller craters and large sunken pits within it. The bulk of the dune material sits atop the flat remnant of the original crater floor, but then some of it spills dramatically down into the pits below."
Image: Ripples of dunes inside a crater are visible in this 3-D view based on Mars Express data on Rabe Crater. Images to construct this view were taken in 2005 and 2014.