Freitag, 9. Oktober 2015 - 20:30 Uhr

Mars-Chroniken - Mars Rover Curiosity befindet sich vermutliche auf Überresten eines ca. 3.5 Milliarden Jahre alten Seebettes


The dry, dusty crater that NASA’s Mars rover Curiosity is exploring was once filled with a series of lakes that together may have lasted for millions of years, scientists at Jet Propulsion Laboratory say. 
The findings, published by the journal Science, show that liquid water may have existed for long enough on the planet for life to (hypothetically) begin and thrive.
"We as a science community have to come to grips with the fact that, sometime between 3.2 and 3.8 billion years ago, water was really stable on the surface of Mars," said lead author John Grotzinger, a Caltech geologist and Curiosity's former project scientist.
Since landing in Gale Crater in 2012, snapping pictures and drilling rocks, Curiosity has found plenty of evidence that liquid water was present in the rust-hued planet’s distant past. In Yellowknife Bay, the rover even discovered clear signs of a past habitable environment, filled with life-friendly chemicals. 
“The geology of Mars still holds the tantalizing possibility that extraterrestrial life might exist or have been preserved, because the evidence of water is so plentiful,” Marjorie Chan of the University of Utah, who was not involved in the paper, wrote in a commentary.  
But how long did this wet, life-friendly environment stick around? It would have to last long enough for life to emerge. Scientists don’t know how long that might take, but it could be on the order of millions of years. A lake that lasted a mere millennium simply wouldn't cut it.
The newly published research takes into account observations from across Curiosity’s journey, from its landing site all the way to the base of Mt. Sharp, the 3-mile-high mountain in the middle of Gale Crater.
Over about 9 kilometers and about 75 meters of elevation, the rover examined dozens of outcrops, the study authors wrote. They looked at the size and patterns of grain in the rock and found signs of sediments deposited by streams. Closer to the middle of the crater, they found even smaller sand-sized grains – the kind you would see in delta deposits, where the streams should meet a lake. They found evidence for just such a lake, with even finer mud-sized grains.
Gale Crater, the scientists say, probably held a series of lakes over time that rose and fell before and filled again, connected through a shared groundwater table.  
“This intracrater lake system probably existed intermittently for thousands to millions of years, implying a relatively wet climate that supplied moisture to the crater rim and transported sediment via streams into the lake basin,” the study authors wrote. 
Scientists have recently found evidence for extremely briny water flowing on present-day Mars, but pure liquid water couldn’t really survive on the planet today; the atmosphere is so thin that the water would either boil off or freeze solid, depending on the temperature. 
So if there is evidence for long-lived bodies of standing water, that means the atmosphere must have been much thicker, perhaps filled with puffy clouds, able to support a water cycle that might have included precipitation (rain or snow). This world would have looked, in short, a lot more like our own planet. 
“The more the geology looks like Earth, the more likely it seems that some life-form(s) could have developed in the martian waters,” Chan wrote.
Quelle: Los Angeles Times
Wet Paleoclimate of Mars Revealed by Ancient Lakes at Gale Crater
A paper published on Oct. 9 in Science by members of the Mars Science Laboratory team describes ancient water flows and lakes on Mars, and what this might mean about the ancient climate.
We have heard the Mars exploration mantra for more than a decade: follow the water. In a new paper published October 9, 2015, in the journal Science, the Mars Science Laboratory (MSL) team presents recent results of its quest to not just follow the water but to understand where it came from, and how long it lasted on the surface of Mars so long ago.
The story that has unfolded is a wet one: Mars appears to have had a more massive atmosphere billions of years ago than it does today, with an active hydrosphere capable of storing water in long-lived lakes. The MSL team has concluded that this water helped to fill Gale Crater, the MSL rover Curiosity's landing site, with sediment deposited as layers that formed the foundation for the mountain found in the middle of the crater today.
Curiosity has been exploring Gale Crater, which is estimated to be between 3.8 billion and 3.6 billion years old, since August 2012. In mid-September 2014, the rover reached the foothills of Aeolis Mons, a three-mile-high layered mountain nicknamed "Mount Sharp" in honor of the late Caltech geologist Robert Sharp. Curiosity has been exploring the base of the mountain since then.
"Observations from the rover suggest that a series of long-lived streams and lakes existed at some point between 3.8 billion to 3.3 billion years ago, delivering sediment that slowly built up the lower layers of Mount Sharp," says Ashwin Vasavada (PhD '98), MSL project scientist. "However, this series of long-lived lakes is not predicted by existing models of the ancient climate of Mars, which struggle to get temperatures above freezing," he says.
This mismatch between the predictions of Mars's ancient climate that arise from models developed by paleoclimatologists and indications of the planet's watery past, as interpreted by geologists, bears similarities to a century-old scientific conundrum—in this case, about Earth's ancient past.
At the time, geologists first began to recognize that the shapes of the continents matched each other, almost like scattered puzzle pieces, explains John Grotzinger, Caltech's Fletcher Jones Professor of Geology, chair of the Division of Planetary and Geological Sciences, and lead author of the paper. "Aside from the shapes of the continents, geologists had paleontological evidence that fossil plants and animals in Africa and South America were closely related, as well as unique volcanic rocks suggestive of a common spatial origin. The problem was that the broad community of earth scientists could not come up with a physical mechanism to explain how the continents could plow their way through Earth's mantle and drift apart. It seemed impossible. The missing component was plate tectonics," he says. "In a possibly similar way, we are missing something important about Mars."
As Curiosity has trekked across Gale Crater, it has stopped to examine numerous areas of interest. All targets are imaged, and soil samples have been scooped from some; the rocks in a select few places have been drilled for samples. These samples are deposited into the rover's onboard laboratories. Using data from these instruments, as well as visual imaging from the onboard cameras and spectroscopic analyses, MSL scientists have pieced together an increasingly coherent and compelling story about the evolution of this region of Mars.
Before Curiosity landed on Mars, scientists proposed that Gale Crater had filled with layers of sediments. Some hypotheses were "dry," implying that the sediments accumulated from wind-blown dust and sand, whereas others focused on the possibility that sediment layers were deposited in ancient streams and lakes. The latest results from Curiosity indicate that these wetter scenarios were correct for the lower portions of Mount Sharp. Based on the new analysis, the filling of at least the bottom layers of the mountain occurred mostly by ancient rivers and lakes.
"During the traverse of Gale, we have noticed patterns in the geology where we saw evidence of ancient fast-moving streams with coarser gravel as well as places where streams appear to have emptied out into bodies of standing water," Vasavada says. "The prediction was that we should start seeing water-deposited, fine-grained rocks closer to Mount Sharp. Now that we've arrived, we're seeing finely laminated mudstones in abundance." These silty layers in the strata are interpreted as ancient lake deposits.
"These finely laminated mudstones are very similar to those we see on Earth," says Woody Fischer, professor of geobiology at Caltech and coauthor of the paper. "The scale of lamination—which occurs both at millimeter and centimeter scale—represents the settling of plumes of fine sediment through a standing body of water. This is exactly what we see in rocks that represent ancient lakes on Earth." The mudstone indicates the presence of bodies of standing water in the form of lakes that remained for long periods of time, possibly repeatedly expanding and contracting during hundreds to millions of years. These lakes deposited the sediment that eventually formed the lower portion of the mountain.
"Paradoxically, where there is a mountain today there was once a basin, and it was sometimes filled with water," says Grotzinger. "Curiosity has measured about 75 meters of sedimentary fill, but based on mapping data from NASA's Mars Reconnaissance Orbiter and images from Curiosity's cameras, it appears that the water-transported sedimentary deposition could have extended at least 150–200 meters above the crater floor, and this equates to a duration of millions of years in which lakes could have been intermittently present within the Gale Crater basin," Grotzinger says. Furthermore, the total thickness of sedimentary deposits in Gale Crater that indicate interaction with water could extend higher still—up to perhaps 800 meters above the crater floor, and possibly representing tens of millions of years.
But layers deposited above that level do not require water as an agent of deposition or alteration. "Above 800 meters, Mount Sharp shows no evidence of hydrated strata, and that is the bulk of what forms Mount Sharp. We see another 4,000 meters of nothing but dry strata," Grotzinger says. He suggests that perhaps this segment of the crater's history may have been dominated by eolian, or wind-driven, deposition, as was once imagined for the lower part explored by Curiosity. This occurred after the wet period that built up the base of the mountain.
A lingering question surrounds the original source of the water that carried sediment into the crater. For flowing water to have existed on the surface, Mars must have had a thicker atmosphere and warmer climate than has been theorized for the time frame bookending the intense geological activity in Gale Crater. Evidence for this ancient, wetter climate exists in the rock record. However, current models of this paleoclimate—factoring in estimates of the early atmosphere's mass, composition, and the amount of energy it received from the sun—come up, quite literally, dry. Those models indicate that the atmosphere of Mars could not have sustained large quantities of liquid water.
Yet the rock record discovered at Gale Crater suggests a different scenario. "Whether it was snowfall or rain, you have geologic evidence for that moisture accumulating in the highlands of the Gale Crater rim," Grotzinger says. In the case of Gale Crater, at least some of the water was supplied by the highlands that form the crater rim, but groundwater discharge—a standard explanation to reconcile wet geologic observations with dry paleoclimatic predictions—is unlikely in this area. "Right on the other side of Gale's northern rim are the Northern Plains. Some have made the argument that there was a northern ocean sitting out there, and that's one way to get the moisture that you need to match what we are seeing in the rocks." Pinpointing the possible location of an ocean, however, does not help to explain how that water managed to exist as a liquid for extended periods of time on the surface.
As climatologists try to develop new atmospheric models, help should be coming from the continuing explorations by Curiosity. "There are still many kilometers of Mars history to explore," says Fischer. He thinks that some of the most exciting data yet may come in the next few years as Curiosity climbs higher on Mount Sharp. "The strata will reveal Gale's early history, its story. We know there are rocks that were deposited underwater, in the lake. What is the chemistry of these rocks? That lake represented an interface between the water and the atmosphere, and should tell us important things about the environment of the time."
"We have tended to think of Mars as being simple," adds Grotzinger. "We once thought of the earth as being simple, too. But the more you look into it, questions come up because you're beginning to fathom the real complexity of what we see on Mars. This is a good time to go back to reevaluate all our assumptions. Something is missing somewhere." 
Quelle: Caltech

Tags: Mars-Chroniken