화성’ surface was carved by fast and furious floods from overflowing craters 3.5 billion years ago – with enough water released in a matter of weeks to completely fill Lake Superior, 연구 결과
화성’ surface was carved by fast and furious floods from overflowing crater lakes 3.5 billion years ago, a new study says.
Researchers in 텍사스 have used satellite images to determine how 262 breached lakes on the Red Planet shaped the Martian surface.
The floods, which probably lasted mere weeks, eroded more than enough sediment to completely fill Lake Superior and Lake Ontario, 그들은 말한다.
Although there’s no liquid water on Mars today, 약 4.3 billion years ago the Red Planet had enough water to cover its entire surface in a liquid layer about 450 피트 (137 미터) deep, 에 따르면 NASA.
Fast forward to 3.5 billion years ago, and this water was more scarce – channeled around the planet between crater lakes via rivers, much like on Earth today.
Floods at these lakes created river valleys with high walls of jagged rock on either side, much like Earth’s own impressive modern-day canyons.
A coloured topographical image showing river valleys on Mars. The outlet canyon Loire Vallis (white line) formed from the overflow of a lake in Parana Basin (outlined in white). Black lines indicate other river valleys formed by processes other than lake overflows. Image is approximately 400 마일 (650 킬로미터) 건너서
Mars was not always a big dry rusty rock like it is today. Perhaps about 4.3 billion years ago, Mars would have had enough water to cover its entire surface in a liquid layer about 450 피트 (137 미터) deep
RIVER VALLEYS ON MARS
The cratered highlands of Mars have many river valleys that formed in a water-rich environment about 4.5 ...에 3.7 billion years ago.
Erosion since then has been slow, leaving these old features preserved.
나중, massive outflows of groundwater formed flood channels tens to hundreds of kilometers wide and perhaps over 1,000 kilometers (620 마일) 긴.
River valley networks begin near crater rims and other high ridges and wind through the cratered landscape.
출처: Smithsonian National Air and Space Museum
‘If we think about how sediment was being moved across the landscape on ancient Mars, lake breach floods were a really important process globally,’ said lead author Tim Goudge, an assistant professor at the UT Jackson School of Geosciences, the University of Texas at Austin.
‘And this is a bit of a surprising result because they’ve been thought of as one-off anomalies for so long.’
On Earth, river erosion – the constant wearing away of the river bed and banks by the force of water – is usually a slow-going process.
Over years and years, coastal land recedes as the force of the water breaks off sediment.
But on Mars, massive floods from overflowing crater lakes had an outsized role in shaping the Martian surface, carving deep chasms and moving vast amounts of sediment.
Crater lakes were common on Mars billions of years ago when the Red Planet had liquid water on its surface. Some craters could hold a small sea’s worth of water.
But when the water became too much to hold, it would breach the edge of the crater, causing catastrophic flooding that carved river valleys in its wake.
ㅏ 2019 연구 led by Goudge, published in the in the journal Geology, determined that these events happened rapidly.
Remote sensing images taken by satellites orbiting Mars have allowed scientists to study the remains of breached Martian crater lakes.
The remains of a former crater lake on Mars surrounded by other smaller craters. The large outlet canyon (the spindly blue dent in the upper left) formed during a crater breach event
A global map of Mars showing river valleys around the Red Planet. River valleys formed by crater lake breaches are in white. River valleys that formed gradually over time are in black
MARS IS ‘TOO SMALL’ TO RETAIN LQUID WATER, SAYS STUDY
Mars once had flowing liquid water, but is now a dry desert landscape – and this could be because it is too small to retain moisture, ㅏ 2021 study said.
About half the size of Earth, Mars sits at the very outer edge of the habitable zone where liquid water ‘could flow’.
Researchers at Washington University in St Louis studied the chemical makeup of Mars meteorites.
These rocks revealed Mars didn’t have the necessary chemistry in its structure to hold onto water long-term.
하나, the crater lakes and their river valleys have mostly been studied on an individual basis, Goudge said.
This is the first study to investigate how the 262 breached lakes across the Red Planet shaped the Martian surface as a whole.
연구를 위해, the researchers reviewed a preexisting catalog of river valleys on Mars and classifying them into two categories – valleys that got their start at a crater’s edge and valleys that formed elsewhere on the landscape.
Valleys that got their start at a crater’s edge indicates they formed during a lake breach flood, while valleys that formed elsewhere on the landscape suggests a more gradual formation over time.
From there, the scientists compared the depth, length and volume of the different valley types and found that river valleys formed by crater lake breaches erode nearly a quarter of the Red Planet’s river valley volume despite making up only 3 per cent of total valley length.
‘This discrepancy is accounted for by the fact that outlet canyons are significantly deeper than other valleys,’ said study co-author Alexander Morgan, a research scientist at the Planetary Science Institute in Tucson, 애리조나.
에서 559 피트 (170.5 미터), the median depth of a breach river valley is more than twice that of other river valleys created more gradually over time, which have a median depth of about 254 피트 (77.5 미터).
게다가, although the chasms appeared in a geologic instant, they may have had a lasting effect on the surrounding landscape.
Floods at Martian lakes created river valleys with high walls of jagged rock on either side, much like the impressive canyons on Earth today. 사진, the Colorado River as it flows through Marble Canyon prior to entering the infamous Grand Canyon in northern Arizona
The study suggests that the breaches scoured canyons so deep they may have influenced the formation of other nearby river valleys.
The authors said this is a potential alternative explanation for unique Martian river valley topography that is usually attributed to climate.
On Earth, river erosion is a slow and steady process in most cases, but that doesn’t mean it will work that way on other worlds, according to Goudge.
‘When you fill [the craters] with water, it’s a lot of stored energy there to be released,’ Goudge said. ‘It makes sense that Mars might tip, in this case, toward being shaped by catastrophism more than the Earth.’
The new study has been published today in the journal 자연.
WAS MARS EVER HOME TO LIQUID WATER?
Evidence of water on Mars dates back to the Mariner 9 mission, which arrived in 1971. It revealed clues of water erosion in river beds and canyons as well as weather fronts and fogs.
Viking orbiters that followed caused a revolution in our ideas about water on Mars by showing how floods broke through dams and carved deep valleys.
Mars is currently in the middle of an ice age, and before this study, scientists believed liquid water could not exist on its surface.
6 월 2013, Curiosity found powerful evidence that water good enough to drink once flowed on Mars.
In September of the same year, the first scoop of soil analysed by Curiosity revealed that fine materials on the surface of the planet contain two per cent water by weight.
에 2017, Scientists provided the best estimates for water on Mars, claiming it once had more liquid H2O than the Arctic Ocean – and the planet kept these oceans for more than 1.5 억년.
The findings suggest there was ample time and water for life on Mars to thrive, but over the last 3.7 billion years the red planet has lost 87 per cent of its water – leaving it barren and dry.