Archive for high resolution imaging science experiment – Page 3

NASA Spacecraft Detects Changes in Martian Sand Dunes

NASA’s Mars Reconnaissance Orbiter has revealed that movement in sand dune fields on the Red Planet occurs on a surprisingly large scale, about the same as in dune fields on Earth. This is unexpected because Mars has a much thinner atmosphere than Earth, is only about one percent as dense, and its high-speed winds are less frequent and weaker than Earth’s.

For years, researchers debated whether sand dunes observed on Mars were mostly fossil features related to past climate, rather than currently active. In the past two years, researchers using images from Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE) camera have detected and reported sand movement.

Now, scientists using HiRISE images have determined that entire dunes as thick as 200 feet (61 meters) are moving as coherent units across the Martian landscape. The study was published online by the journal Nature.

“This exciting discovery will inform scientists trying to better understand the changing surface conditions of Mars on a more global scale,” said Doug McCuistion, director, NASA’s Mars Exploration Program, Washington. “This improved understanding of surface dynamics will provide vital information in planning future robotic and human Mars exploration missions.”

Researchers analyzed before-and-after images using a new software tool developed at the California Institute of Technology (Caltech) in Pasadena, Calif. The tool measured changes in the position of sand ripples, revealing the ripples move faster the higher up they are on a dune.

The study examined images taken in 2007 and 2010 of the Nili Patera sand dune field located near the Martian equator. By correlating the ripples’ movement to their position on the dune, the analysis determined the entire dunes are moving. This allows researchers to estimate the volume, or flux, of moving sand.

“We chose Nili Patera because we knew there was sand motion going on there, and we could quantify it,” said Nathan Bridges, a planetary scientist at Johns Hopkins University Applied Physics Laboratory in Laurel, Md., and lead author of the Nature paper. “The Nili dunes also are similar to dunes in places like Antarctica and to other locations on Mars.”

The study adds important information about the pace at which blowing sand could be actively eroding rocks on Mars. Using the new information about the volume of sand that is moving, scientists estimate rocks in Nili Patera would be worn away at about the same pace as rocks near sand dunes in Antarctica, where similar sand fluxes occur.

“Our new data shows wind activity is indeed a major agent of evolution of the landscape on Mars,” said Jean-Philippe Avouac, Caltech team leader. “This is important because it tells us something about the current state of Mars and how the planet is working today, geologically.”

Scientists calculate that if someone stood in the Nili Patera dunes and measured out a one-yard (one-meter) width, they would see more than two cubic yards (1,500 liters) of sand pass by in an Earth year, about as much as in a child’s sand box.

“No one had estimates of this flux before,” said Bridges. “We had seen with HiRISE that there was dune motion, but it was an open question how much sand could be moving. Now, we can answer that.”

Scientists will use the information to understand broader mysteries on Mars, like why so much of the surface appears heavily eroded, how that occurred, and whether it is a current process or it was done in the past. Scientists can now point to sand flux as a mechanism capable of creating significant erosion today on the Red Planet.

The HiRISE camera provides unprecedented resolution in studying the Martian landscape. NASA’s Jet Propulsion Laboratory, Pasadena, Calif., a division of Caltech, manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate in Washington. Lockheed Martin Space Systems, Denver, built the spacecraft. HiRISE is operated by the University of Arizona and was built by Ball Aerospace and Technologies Corp., Boulder, Colo.

Article source: http://www.marsdaily.com/reports/NASA_Spacecraft_Detects_Changes_in_Martian_Sand_Dunes_999.html

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NASA Spacecraft Detects Changes in Martian Sand Dunes

ScienceDaily (May 9, 2012) — NASA’s Mars Reconnaissance Orbiter has revealed that movement in sand dune fields on the Red Planet occurs on a surprisingly large scale, about the same as in dune fields on Earth.

This is unexpected because Mars has a much thinner atmosphere than Earth, is only about one percent as dense, and its high-speed winds are less frequent and weaker than Earth’s.

For years, researchers debated whether sand dunes observed on Mars were mostly fossil features related to past climate, rather than currently active. In the past two years, researchers using images from Mars Reconnaissance Orbiter’s High Resolution Imaging Science Experiment (HiRISE) camera have detected and reported sand movement.

Now, scientists using HiRISE images have determined that entire dunes as thick as 200 feet (61 meters) are moving as coherent units across the Martian landscape. The study was published online May 9 by the journal Nature.

“This exciting discovery will inform scientists trying to better understand the changing surface conditions of Mars on a more global scale,” said Doug McCuistion, director, NASA’s Mars Exploration Program, Washington. “This improved understanding of surface dynamics will provide vital information in planning future robotic and human Mars exploration missions.”

Researchers analyzed before-and-after images using a new software tool developed at the California Institute of Technology (Caltech) in Pasadena, Calif. The tool measured changes in the position of sand ripples, revealing the ripples move faster the higher up they are on a dune.

The study examined images taken in 2007 and 2010 of the Nili Patera sand dune field located near the Martian equator. By correlating the ripples’ movement to their position on the dune, the analysis determined the entire dunes are moving. This allows researchers to estimate the volume, or flux, of moving sand.

“We chose Nili Patera because we knew there was sand motion going on there, and we could quantify it,” said Nathan Bridges, a planetary scientist at Johns Hopkins University Applied Physics Laboratory in Laurel, Md., and lead author of the Nature paper. “The Nili dunes also are similar to dunes in places like Antarctica and to other locations on Mars.”

The study adds important information about the pace at which blowing sand could be actively eroding rocks on Mars. Using the new information about the volume of sand that is moving, scientists estimate rocks in Nili Patera would be worn away at about the same pace as rocks near sand dunes in Antarctica, where similar sand fluxes occur.

“Our new data shows wind activity is indeed a major agent of evolution of the landscape on Mars,” said Jean-Philippe Avouac, Caltech team leader. “This is important because it tells us something about the current state of Mars and how the planet is working today, geologically.”

Scientists calculate that if someone stood in the Nili Patera dunes and measured out a one-yard (one-meter) width, they would see more than two cubic yards (1,500 liters) of sand pass by in an Earth year, about as much as in a child’s sand box.

“No one had estimates of this flux before,” said Bridges. “We had seen with HiRISE that there was dune motion, but it was an open question how much sand could be moving. Now, we can answer that.”

Scientists will use the information to understand broader mysteries on Mars, like why so much of the surface appears heavily eroded, how that occurred, and whether it is a current process or it was done in the past. Scientists can now point to sand flux as a mechanism capable of creating significant erosion today on the Red Planet.

The HiRISE camera provides unprecedented resolution in studying the Martian landscape. NASA’s Jet Propulsion Laboratory, Pasadena, Calif., a division of Caltech, manages the Mars Reconnaissance Orbiter for NASA’s Science Mission Directorate in Washington. Lockheed Martin Space Systems, Denver, built the spacecraft. HiRISE is operated by the University of Arizona and was built by Ball Aerospace Technologies Corp., Boulder, Colo.

For related images and more information about Mars Reconnaissance Orbiter, visit: http://www.nasa.gov/mro .

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Story Source:

The above story is reprinted from materials provided by NASA/Jet Propulsion Laboratory.

Note: Materials may be edited for content and length. For further information, please contact the source cited above.


Journal Reference:

  1. N. N. Bridges, F. Ayoub, J-P. Avouac, S. Leprince, A. Lucas, S. Mattson. Earth-like sand fluxes on Mars. Nature, 2012; DOI: 10.1038/nature11022

Note: If no author is given, the source is cited instead.

Disclaimer: Views expressed in this article do not necessarily reflect those of ScienceDaily or its staff.

Article source: http://www.sciencedaily.com/releases/2012/05/120509171230.htm

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NASA Mars Spacecraft Detects Large Changes In Martian Sand Dunes


WASHINGTON, May 9, 2012 /PRNewswire via COMTEX/ –
NASA’s Mars Reconnaissance Orbiter (MRO) has revealed that movement in sand dune fields on the Red Planet occurs on a surprisingly large scale, about the same as in dune fields on Earth.

http://photos.prnewswire.com/prnthumb/20081007/38461LOGO

This is unexpected because Mars has a much thinner atmosphere than Earth, is only about one percent as dense, and its high-speed winds are less frequent and weaker than Earth’s.

For years, researchers debated whether or not sand dunes observed on Mars were mostly fossil features related to past climate, rather than currently active. In the past two years, researchers using images from MRO’s High Resolution Imaging Science Experiment (HiRISE) camera have detected and reported sand movement.

Now, scientists using HiRISE images have determined that entire dunes as thick as 200 feet are moving as coherent units across the Martian landscape. The study was published online today by the journal Nature.

“This exciting discovery will inform scientists trying to better understand the changing surface conditions of Mars on a more global scale,” said Doug McCuistion, director of NASA’s Mars Exploration Program in Washington. “This improved understanding of surface dynamics will provide vital information in planning future robotic and human Mars exploration missions.”

Researchers analyzed before-and-after images using a new software tool developed at the California Institute of Technology (Caltech) in Pasadena. The tool measured changes in the position of sand ripples, revealing the ripples move faster the higher up they are on a dune.

The study examined images taken in 2007 and 2010 of the Nili Patera sand dune field located near the Martian equator. By correlating ripples’ movement to their position on the dune, the analysis determined the entire dunes are moving. This allows researchers to estimate the volume, or flux, of moving sand.

“We chose Nili Patera because we knew there was sand motion going on there, and we could quantify it,” said Nathan Bridges, a planetary scientist at Johns Hopkins University Applied Physics Laboratory in Laurel, Md., and lead author of the Nature paper. “The Nili dunes also are similar to dunes in places like Antarctica and to other locations on Mars.”

The study adds important information about the pace at which blowing sand could be actively eroding rocks on Mars. Using the new information about the volume of sand that is moving, scientists estimate rocks in Nili Patera would be worn away at about the same pace as rocks near sand dunes in Antarctica, where similar sand fluxes occur.

“Our new data shows wind activity is indeed a major agent of evolution of the landscape on Mars,” said Jean-Philippe Avouac, Caltech team leader. “This is important because it tells us something about the current state of Mars and how the planet is working today, geologically.”

Scientists calculate that if someone stood in the Nili Patera dunes and measured out a one-yard width, they would see more than two cubic yards of sand pass by in an Earth year, about as much as in a children’s sand box.

“No one had estimates of this flux before,” said Bridges. “We had seen with HiRISE that there was dune motion, but it was an open question how much sand could be moving. Now, we can answer that.”

Scientists will use the information to understand broader mysteries on Mars, like why so much of the surface appears heavily eroded, how that occurred, and whether it is a current process or it was done in the past. Scientists can now point to sand flux as a mechanism capable of creating significant erosion today on the Red Planet.

The HiRISE camera provides unprecedented resolution in studying the Martian landscape. NASA’s Jet Propulsion Laboratory manages MRO for NASA’s Science Mission Directorate in Washington. Lockheed Martin Space Systems, Denver, built the spacecraft. HiRISE is operated by the University of Arizona and was built by Ball Aerospace Technologies Corp., Boulder, Colo.

For related images and more information about MRO, visit:

http://www.nasa.gov/mro

SOURCE NASA

Copyright (C) 2012 PR Newswire. All rights reserved

Article source: http://www.marketwatch.com/story/nasa-mars-spacecraft-detects-large-changes-in-martian-sand-dunes-2012-05-09

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Trio of twisters spotted on Mars

NASA / JPL-Caltech / ASU

Three Martian whirlwinds, known as dust devils, whirl in this picture captured by NASA’s Mars Reconnaissance Orbiter on Feb. 11.

It’s eerie enough to see one whirlwind swirling across the Martian surface, but three? Get out your 3-D glasses and spot the three dust devils rising from Amazonis Planitia, as seen by the high-resolution camera aboard NASA’s Mars Reconnaissance Orbiter.

These mini-twisters are analogous to the dust devils that are whipped up on sunny afternoons on Earth, due to the rise of hot air through a low-pressure pocket of cooler air above it. In February, the Mars orbiter spotted a couple of prominent examples of the phenomenon that rose as high as 12 miles into the Red Planet’s thin atmosphere. These three dust devils aren’t nearly as big, but seeing them simultaneously in one 3-D picture gives you an idea just how active the wind patterns on Mars can get.

“The active dust devils seem to float above the surface,” says Arizona State University’s Alfred McEwen, principal investigator for the camera, known as the High Resolution Imaging Science Experiment or HiRISE. “There are also some bright lines present … those are the tracks of dust devils that passed through this region in the prior two weeks.”

For more from Mars, check out the HiRISE website — and as long as you have your 3-D glasses out, take a look at HiRISE’s 3-D image gallery. What? You don’t have your 3-D glasses yet? This NASA webpage lists some online vendors. While you’re at it, think about picking up some sun-viewing spectacles for the May 20 annular solar eclipse. On Friday, I’ll be giving away a combo pack of 3-D glasses and eclipse glasses as the prize in our weekly “Where in the Cosmos” photo contest; watch for that on the Cosmic Log Facebook page.

More about Mars:


Alan Boyle is msnbc.com’s science editor. Connect with the Cosmic Log community by “liking” the log’s Facebook page, following @b0yle on Twitter or adding Cosmic Log’s Google+ page to your circle. You can also check out “The Case for Pluto,” my book about the controversial dwarf planet and the search for other worlds.

Article source: http://photoblog.msnbc.msn.com/_news/2012/05/07/11584846-trio-of-twisters-spotted-on-mars?chromedomain=cosmiclog

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NASA budget impacts UA projects

While some programs slip through, others have been cut entirely

With one project already halted, a proposed NASA budget cut stands to hurt the UA’s planetary science research.

President Barack Obama’s proposal, delivered on Feb. 13, suggested cutting NASA funding by $58.6 million. The area facing the largest cut is planetary science, which, according to the proposal, will drop by $300 million.

Since the UA receives about $18 million from NASA annually, according to planetary sciences department head Tim Swindle, the proposal significantly impacts the UA’s planetary science research and could limit what the department is able to do in the future.

“If the budget stands as proposed, it certainly will not be good for us,” Swindle said in an email. “Since we compete very successfully in virtually every program in NASA planetary science, it is inevitable that we will be hurt in ways we can’t predict.”

The Senate and House of Representatives proposed that funds to planetary science only drop by about $1 million on Thursday, but the proposal is still up in the air.

Alfred McEwen, a professor of planetary geology and the principal investigator for the High Resolution Imaging Science Experiment, has taken the biggest hit from the proposal at the UA level. He had to halt nearly all production on his latest project, the High Resolution Stereo Color Imager (HiSCI).

The project includes the construction of a camera similar to HiRISE. While it would take photos at a lower resolution than its predecessor, it would be capable of full-color imaging and stereo mapping. The instrument would attach to the ExoMars Trace Gas Orbiter, which is being built by the European Space Agency, and is due to launch in 2016.

HiSCI’s funding comes from a joint venture between NASA and the European Space Agency, with the former pitching in about $30 million. Since the proposal, McEwen said the project had lost $25 million of its tentative funding, and can no longer proceed with the construction phase of HiSCI. This phase would have started around this time after a final design review in February, which also failed to come to fruition.

“It’s not a big economic impact to the U of A,” McEwen said. “But it’s an important experiment that we want to complete.”
McEwen added that HiSCI was one of the first steps leading to sample return — literally bringing back a sample from Mars for research in a number of facets — which is a roughly $10-billion, multi-project undertaking for NASA.

“They didn’t want to make that commitment at this time,” he said.
Despite the expense of such a lengthy series of projects, McEwen said the ExoMars Trace Gas Orbiter stood independent from the overall idea of sample return, and shouldn’t have been cut.
“It’s unclear how well they understood that, or whether they were just looking for excuses to cut something,” he said.

Following NASA’s withdrawal, the European Space Agency partnered with Russia in completing the mission, and hope to restore HiSCI is quickly dimming.

In an effort to get HiSCI into space regardless of the vehicle it’s attached to, McEwen is working on design concepts for an entirely different NASA-led mission with a proposed launch in 2018, which remains completely open. How the association can afford this project but not the original is anyone’s guess, McEwen said.

While HiSCI is facing harsh affects from the proposal, OSIRIS-REx has avoided any major funding changes.

OSIRIS-REx began in 2008, winning about $800 million, the highest-paying contract in the UA’s history. It involves taking a sample from an asteroid to be used for research to explore the solar system’s history and discover the potential benefits and dangers of asteroids surrounding Earth, said Dante Lauretta, an associate professor of cosmochemistry and planet formation and the project’s principal investigator.

OSIRIS-REx is funded through NASA’s New Frontiers program, a competitive program that aims to fund roughly two high-profile missions every 10 years, Lauretta said. Similar to other projects of its kind, OSIRIS-REx is a collaborative effort between the UA as well as other institutions and companies.

Each of the partners will receive a certain portion of the funding, with the UA collecting about $225 million by the end of the project.

While the terms of funding for OSIRIS-REx have already been negotiated, Lauretta said that anything can change at this point, and the proposal process is always ongoing. Furthermore, he said the budgeting process is often an unorganized one, with the largely bipartisan Congress that typically doesn’t line out the official budget until several months into the fiscal year. When this happens, Lauretta said, Congress usually reverts back to the previous year’s budget until next year’s can be determined.
Regardless of how the budget for 2013 turns out, Lauretta said his project is well off for the months to come. Its roots in both science and homeland security give it an edge that not every project has.

“It’s a real challenge for the people who work at NASA headquarters to keep projects like this moving forward,” he said, “when your budget is constantly a moving target, the subject of a political battle and not getting done by the deadlines that things are supposed to get done by.”

Article source: http://www.wildcat.arizona.edu/index.php/article/2012/04/nasa_budget_impacts_ua_projects

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Elephant on Mars — sculpted by lava flow

The dried flood of lava over the surface of Mars has created the spitting image of the eye and trunk of an elephant.

The curve of the animal’s forehead and the dent of an ear also appear in a new photo taken by the High Resolution Imaging Science Experiment (HiRISE) on NASA’s Mars Reconnaissance Orbiter.

“This is a good example of the phenomena ‘pareidolia,’ where we see things (such as animals) that aren’t really there,” University of Arizona planetary geologist Alfred McEwen wrote in an update posted on the university’s HiRISE website.

The Mars elephant illusion photo shows a region of the Red Planet called the Elysium Planitia, which is the youngest flood-lava province on Mars.

Scientists aren’t sure if the lava flows on Mars were deposited quickly, or over a longer time period, as is the case on Earth, where most lava floods were put in place over years to decades.

“This is probably true for much of the lava on Mars as well,” McEwen wrote. “An elephant can walk away from the slowly advancing flow front. However, there is also evidence for much more rapidly flowing lava on Mars, a true flood of lava. In this instance, maybe this elephant couldn’t run away fast enough.”

The Mars Reconnaissance Orbiter, which has been circling the Red Planet since 2006, was launched in 2005. The orbiter, currently in an extended phase of its mission, has transmitted more data to Earth than all other interplanetary missions combined, NASA officials have said.

Copyright 2012 SPACE.com, a TechMediaNetwork company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

Article source: http://www.foxnews.com/scitech/2012/04/10/elephant-on-mars-sculpted-by-lava-flow/

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NASA | JPL… A Devil On Mars (Imagery)

Satnews Daily
April 09, 2012


NASA | JPL… A Devil On Mars (Imagery)


[SatNews] A Martian dust devil roughly 12 miles high (20 kilometers) was captured…

…whirling its way along the Amazonis Planitia region of Northern Mars on March 14th. It was imaged by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA‘s Mars Reconnaissance Orbiter. Despite its height, the plume is little more than three-quarters of a football field wide (70 yards, or 70 meters).


A Martian dust devil roughly 12 miles (20 kilometers) high was captured winding its way along the Amazonis Planitia region of Northern Mars on March 14, 2012 by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter. Despite its height, the plume is little more than three-quarters of a football field wide (70 yards, or 70 meters).

Image credit: NASA/JPL-Caltech/UA

Dust devils occur on Earth as well as on Mars. They are spinning columns of air, made visible by the dust they pull off the ground. Unlike a tornado, a dust devil typically forms on a clear day when the ground is heated by the sun, warming the air just above the ground. As heated air near the surface rises quickly through a small pocket of cooler air above it, the air may begin to rotate, if conditions are just right. This image was taken during late northern spring, two weeks short of the northern summer solstice, a time when the ground in the northern mid-latitudes is being heated most strongly by the sun.

The Mars Reconnaissance Orbiter has been examining the Red Planet with six science instruments since 2006. Now in an extended mission, the orbiter continues to provide insights into the planet’s ancient environments and how processes such as wind, meteorite impacts and seasonal frosts continue to affect the Martian surface today. This mission has returned more data about Mars than all other orbital and surface missions combined. More than 21,700 images taken by HiRISE are available for viewing on the instrument team’s website: http://hirise.lpl.arizona.edu. Each observation by this telescopic camera covers several square miles, or square kilometers, and can reveal features as small as a desk.

HiRISE is operated by the University of Arizona, Tucson. The instrument was built by Ball Aerospace Technologies Corp., Boulder, Colorado. The Mars Reconnaissance Orbiter Project and the Mars Exploration Rover Project are managed by NASA‘s Jet Propulsion Laboratory, Pasadena, Calif., for NASA’s Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena. Lockheed Martin Space Systems, Denver, built the orbiter.



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Article source: http://www.satnews.com/cgi-bin/story.cgi?number=1343869367

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On Mars, all is extreme: Witness the 12-mile-high dust devil

Mars doesn’t have tornadoes. It doesn’t have thunderstorms. But the Red Planet can kick up a truly unholy dust devil.

Such a phenomenon — 12 miles high in fact — was photographed last month on the surface of the planet.

“It really is the size of it that is the unique thing,” said Jet Propulsion Laboratory scientist Ashwin Vasavada. “Conditions allowed this single giant vortex to form and survive to suck up dust all the way to that height.”

The sun beats down on the desert-like surface of Mars and — with the lack of water and the “extremely thin atmosphere” — convection begins, said  Vasavada, deputy project scientist for the Mars Science Laboratory. “Roiling, turbulent air” forms at the planet’s surface in a layer five to 10 miles thick, he added. 

These types of conditions can send dust devils spinning, Vasavada said Thursday in an interview with The Times.

Arguably as impressive as the natural phenomenon is the technology that allowed it to be photographed for us to see back on Earth.

The $720-million Mars Reconnaissance Orbiter is the latest orbiter that NASA has sent to Mars.  It was launched in August 2005 and began mapping Mars in March 2006, Vasavada said.  The mission is managed by the California-based Jet Propulsion Laboratory.

“One of its key capabilities is this camera,” he added, “the size of a big telescope.” The high-tech, high-resolution piece of equipment — “like a spy camera on Mars” — allows scientists to see details on the surface of the planet to about 30 centimeters (11.8 inches) across.

From orbit, HiRISE (for High Resolution Imaging Science Experiment, seriously) was able to see the “golf-cart-size rovers” Spirit and Opportunity, Vasavada said, even picking out their tracks. 

The camera has helped scientists pinpoint a spot for the upcoming landing of the Curiosity rover, set for Aug. 5. Curiosity is part of the Mars Science Laboratory project, which will follow up on the discovery of clays — minerals that need liquid water to form — on Mars. 

Reconnaissance’s CRISM (for Compact Reconnaissance Imaging Spectrometer for Mars) revealed to scientists the colors of minerals. And clays were seen at sites all around the planet, particularly in terrain that dated from the earliest 1 billion or 2 billion years of the planet’s existence, Vasavada said.

Curiosity will land at Gale Crater, where a mound exists that the scientist likened to “a book that has chapters from all the major parts of Mars history.”

Studying this mound will help scientists explore theories on the history of the planet — the “clay area early on,” Vasavada said, with its hints at surface water “and the best chance of supporting life if there ever was life.”

The next, higher layer in the mound is “sulfates” at the point in Mars history when it was drying out. The most recent history, he said, is “characterized by a lot of boring dust.”

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amy.hubbard@latimes.com 

Article source: http://www.latimes.com/news/nation/nationnow/la-na-nn-mars-dust-devil-20120405,0,4097816.story

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Is That an Elephant on Mars?

Mars-elephant

Once you see it, you can’t shake it; there is indeed an elephant on Mars! Well, it’s actually a Martian lava flow in the shape of an elephant’s head, but it is also a fantastic opportunity to discuss some Mars geology and why the human brain seems so easily tricked into seeing large mammals in alien landscapes.

First, a little Mars geology.

As photographed by the High-Resolution Imaging Science Experiment (HiRISE) camera aboard NASA’s Mars Reconnaissance Orbiter (MRO), this geological feature was spotted in Elysium Planitia, a Martian plain that exhibits some of the youngest lava flows on the Red Planet’s surface.

PHOTOS: Weirdest Mars Craters

Mars is largely geologically inactive, so active volcanoes and flowing lava are a thing of the past. But the ‘young’ lava flows that cover Elysium Planitia may have been emplaced within the last 100 million years — potentially as recent as the last 10 million years. This may not sound recent, but when chronicling billions of years of Mars geological history, a hundred million years is no time at all.

TumbleweedWATCH VIDEO: New concepts for Mars-probing rovers would use Martian wind to move around the planet.

According to University of Arizona planetary geologist Alfred McEwen, when the lava flow was hot and spewing out of Mars’ interior, its advancing flow front would have most likely been so slow that an elephant could have out-walked its glacial pace — not too dissimilar to lava flows on Earth.

“However, there is also evidence for much more rapidly flowing lava on Mars, a true flood of lava,” McEwen points out. “In this instance, maybe this elephant couldn’t run away fast enough.”

Whether or not an elephant could outrun a lava flow on Mars isn’t the focus of this HiRISE photograph, however. It’s actually a vivid example of “pareidolia” — a psychological phenomenon that tricks our brains into seeing familiar objects in random shapes.

ANALYSIS: Sadly, There’s No Secret Base On Mars

A popular everyday example of pareidolia is seeing shapes of bunnies in clouds. But pareidolia can take on all shapes and sizes (pun intended). People see religious symbols in potatoes and “Angry Birds” in astronomical observations of deep space. What about the “Man in the Moon”? Yep, that’s pareidolia. So is the “Face on Mars” that was captured by early observations of the Red Planet (and spawned the punchline of the terrible Hollywood movie “Mission to Mars”).

Mars is often the subject of some great popular culture pareidolia, like the “Martian Yeti.” Surface missions to Mars often come under close scrutiny after conspiracy theorists and the tabloid press interpret random shapes in rocks as being somehow artificial.

While writing about an apparent “Egyptian statue” carved into the side of a rocky outcrop at Victoria Crater as photographed by Mars Rover Opportunity, I decided to go on a “pareidolia hunt” of my own. Taking the Opportunity photo (including two “alien artifacts” as detailed on conspiracy websites — pictured below), I used a bit of imagination and spotted a huge number of shapes that looked familiar. (I was particularly impressed to see “Star Wars” Admiral Ackbar etched into one outcrop.)

ANALYSIS: Angry Bird in the Sky? Face on Mars?

So it goes to show, whether you’re orbiting Mars or roving across its surface, there is an endless supply of randomly shaped rocks and geological features to trick your brain into thinking its seeing elephant heads. But also watch out for those pesky cosmic rays, they might give you the impression that we already have bases on Mars.

Image credits: NASA/JPL/University of Arizona

Mars_faces1




Article source: http://news.discovery.com/space/is-that-an-elephant-on-mars-120405.html

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Mars Water? Odd ‘Flowing’ Features On Red Planet’s Surface Stir Debate

By: Leonard David
Published: 04/02/2012 07:34 AM EDT on SPACE.com

Flow-like features on Mars are a source of debate among scientists. While some experts say they are likely produced by liquid water or brine on the Red Planet’s surface today, other investigations interpret some of these features as dry mass movements, stirred up by various other processes.

Whatever the cause, these slope streaks — called Recurring Slope Lineae — represent the movement of mass down slopes on the surface of our neighboring planet. They are among the few known examples of current geologic activity on Mars.

Many scientists agree that water likely flowed across ancient Mars. However, whether it exists as a liquid on the planet’s surface today is arguable.

Recurring Slope Lineae are dark, narrow features that extend on steep, equator-facing, mid-latitude rocky slopes of Mars. Furthermore, they form and grow during multiple warm seasons, and fade in cold seasons.

The head-scratching phenomenon sparked a lively debate on what’s behind the strange slope processes on Mars during last week’s 43rd Lunar and Planetary Science Conference in The Woodlands, Texas. [Photos: The Search for Water on Mars]

SPACE.com spoke to several scientists involved in the research, who gave us a glimpse into what may be happening on Mars.

Ongoing drainage system

Conditions are such on present-day Mars that, at certain locations at certain times of year, liquid water should be capable of existing for short amounts of time, according to Jim Head and Jay Dickson of the department of geological sciences at Brown University in Rhode Island.

The best evidence that water currently exists there comes from the recent discovery in the southern mid-latitudes of Recurring Slope Lineae, or RSL for short.

Dickson and Head described their research findings, showing that identical features are found on the equator-facing wall of the South Fork of Upper Wright Valley in the McMurdo Dry Valleys of Antarctica.

“If this is correct, then RSL on Mars may represent the surface expression of a far more significant ongoing drainage system on steep slopes in the mid-latitudes,”  the team said.

Islands of persistence

In research led by Norbert Schörghofer, of the University of Hawaii’s Institute for Astronomy in Honolulu, a selected study site on Mars revealed the coming-and-going nature of slope streaks.

“For the first time we see an approximate balance between faded and new streaks,” Schörghofer said. “The rate of formation and rate of fading are nearly equal, revealing that the number of slope streaks on the surface of Mars is approximately constant rather than increasing with time. This indicates the streak population is balanced.”

The average lifetime of slope streaks, from time of formation until they disappear, and the turnover time of the slope streak population, are estimated to be four decades, Schörghofer said. Slope streaks fade gradually over time, with “islands of persistence,” and are not obliterated by planet-encircling dust storms.

Rolling and tumbling

So, what on Mars is actually going on?

A formidable tool in helping to spot and catalog these confounding features is NASA’s Mars Reconnaissance Orbiter, or MRO, now circling the Red Planet.

“This is complicated,” said Alfred McEwen, a planetary geologist and director of the Planetary Image Research Laboratory at the University of Arizona in Tucson.”Lots of stuff moves down steep slopes on both Earth and Mars.” McEwen is principal investigator of the High Resolution Imaging Science Experiment (HiRISE) on the MRO.

On Mars, there are several rolling and tumbling categories, McEwen told SPACE.com:

  • Slope streaks on dusty equatorial slopes. These are fully explained as dust avalanches.
  • Slope streaks associated with the presence — especially defrosting — of carbon dioxide (CO2) frost, so CO2-aided mass wasting explains this. This category includes active gullies. The only distinction is whether or not HiRISE images can resolve the topographic changes.
  • Lineaments associated with dry boulder/debris falls.
  • Recurring Slope Lineae may look superficially similar to the other categories, but form only under very particular environmental conditions, in places where there is no CO2 frost. They grow incrementally, and they recur each summer. So far, only the flow of briny water seems to be able to explain these.

“Folks can invoke water for all of the above if they like water. But given the thermodynamics,” McEwenadded, “it is extremely unlikely except, maybe, for the RSL. They all have excellent non-water explanations except the RSL. Maybe the RSL will eventually prove to have a dry explanation as well.”

Leonard David has been reporting on the space industry for more than five decades. He is a winner of last year’s National Space Club Press Award and a past editor-in-chief of the National Space Society’s Ad Astra and Space World magazines. He has written for SPACE.com since 1999.

Copyright 2012 SPACE.com, a TechMediaNetwork company. All rights reserved. This material may not be published, broadcast, rewritten or redistributed.

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Article source: http://www.huffingtonpost.com/2012/04/02/mars-water-features-debate_n_1396233.html

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