Slashdot Mirror


Vast Subsurface Martian Ice Discovered

The Fun Guy writes to tell us New Scientist is reporting that deep-scan radar results from ESA's Mars Express spacecraft have revealed vast amounts of subsurface ice. From the article: "Intriguingly, the signal reflected from the bottom of the crater is so strong and appears so flat that it may be liquid water. 'If you put water there, that's what the signal might look like,' Johnson told New Scientist. But he cautions the data is based on only one pass over the region and could be caused by another material."

20 of 308 comments (clear)

  1. oblig ERB by opencity · · Score: 5, Funny

    also found was John Carter, slightly the worse for wear.

    --
    Physics is like sex: sure, it may give some practical results, but that's not why we do it.
  2. Terraforming by richcoder · · Score: 4, Interesting

    To anyone in the know, what implications would this have on the possible terraforming of mars to have a hospitable atmosphere?

    1. Re:Terraforming by Anonymous Coward · · Score: 5, Funny

      The implications are that there will likely be further implications

    2. Re:Terraforming by MightyMartian · · Score: 4, Interesting

      I really can't imagine how the terraforming idea is going to be tenable over the long term. Even if you can figure out a way to bulk-up the atmosphere to raise surface temperatures sufficiently for water to exist in a liquid state, the gravity of Mars is to weak to sustain such an atmosphere, which will leak off over time. You would essentially have to keep adding to the atmosphere.

      --
      The world's burning. Moped Jesus spotted on I50. Details at 11.
    3. Re:Terraforming by drinkypoo · · Score: 4, Funny

      Depends on if we can send the governator to mars to reactivate the alien machines...

      --
      "You're right," Fisheye says. "I should have set it on 'whip' or 'chop.'"
    4. Re:Terraforming by FridayBob · · Score: 4, Insightful

      Also, since Mars has no magnetic field to speak of, any bulked-up the atmosphere would be lost even faster. Forget terraforming. We might some day figure out how to live there, but it'll never look like home. Then again, home is what you make it, right?

    5. Re:Terraforming by nappingcracker · · Score: 5, Funny

      Ice makes terraforming quite easy.

      • 1. Get your ass to mars
      • 2. Enlist help of little people, mutants, and three breasted women
      • 3. Take Johnnycab to local Martian artifact/ruins
      • 4. Locate martian touchpad
      • 5. insert "spock-live-long-and-prosper" hand to lower alien reactor rods into ice
      • 6. Immediately play outside without EV suit, the planet will be completely pressurized and habitable before your head explodes.

      Cohagen, give those people air!

      --
      |plastic....or gasoline?|
    6. Re:Terraforming by jafac · · Score: 4, Funny

      but the point where the atmosphere is lost again is so far in the future as to be meaningless.

      Here we go again.

      I can see Mars, in the future - the environmentalists will be warning everyone of the danger of atmospheric depletion and the need to invest in replenishment, and the conservatives will claim it's hogwash and that paying for replenishment would be a drain on the economy and cost jobs. . .

      UNTIL THEY ALL CHOKE AND DIE!

      --

      These are my friends, See how they glisten. See this one shine, how he smiles in the light.
  3. Most Puzzling Clue by Waffle+Iron · · Score: 5, Funny

    More detailed analysis of the radar image indicates that the shape of the flat region actually appears to be almost perfectly rectangular, with an aspect ratio of 4:9. Nobody is quite sure what to make of that.

  4. Definately A Big Deal by PlayfullyClever · · Score: 4, Insightful

    This is a big deal. You don't find raw metal much on Mars; most of it is tied up with oxygen. Raw metal has many implications: if it is common, it can be a great source of base building. If the metals are rare on Earth as well, and they're common on Mars, they could provide a potential export source. If it is a meteor, and they're common, it could affect our models of how often Mars gets struck by meteors. Since the rock isn't buried, it could provide clues as to how long it's been on Mars, how fast Meridiani Planum is eroding, and give us dataon how metals wear over time on Mars.

    Any time you find something you've never found before, it's a big deal. Honestly, to people who've been following the mission, it looked like Opportunity was pretty much wrapping things up. It just left a geological treasure trove and there isn't much more "on the map", so to speak. It's neat to see it continue making nice finds.

    --
    Check out my website: Playfully Clever
  5. headline creep by mcguyver · · Score: 5, Insightful

    Actual Scientist - If you put water there, that's what the signal might look like.
    newscientist.com - Radar reveals ice deep below Martian surface
    Slashdot.com - Vast Subsurface Martian Ice Discovered

    The headlines gets better and better!

  6. Little if any by everphilski · · Score: 4, Informative

    To terraform you need to make an atmosphere. You need greenhouse gasses to do this. Water generally doesn't factor into the equation. A good reference is "The case for Mars" by Robert Zubrin (although I don't totally agree with him)

    -everphilski-

  7. Detecting Water by Matts · · Score: 4, Funny

    Everyone knows that to detect water in a deep crater you drop a stone in it and wait for the plopping noise.

    Jeez, and these guys call themselves scientists!

    --

    Matt. Want XML + Apache + Stylesheets? Get AxKit.
  8. Turn your volume up! by Volanin · · Score: 5, Informative

    This sounds very interesting!
    Click here for an audio interview about the finding.

    --
    If I clone myself, can I call it a thread?
    If a girl winks to us, can I call it a race condition?
  9. A solution to global warming... by mustafap · · Score: 4, Funny


    All this moaning about the ice caps melting, lets just nip over there and bring some back!

    --
    Open Source Drum Kit, LPLC deve board - mjhdesigns.com
  10. On the right track by everphilski · · Score: 5, Informative

    Its too thin. That's the problem, trying to make the atmosphere thicker. You basically have to import gasses one way or another. Gasses are bulky though, there are better ways to do it, like plants, biomass, etc. that can break down matter from a solid state into gas. Martian rock is actually rather rusty and carbonaceous (sp?) if you had a good cheap source of heat you could heat it up and get some carbon dioxide and oxygen off of it... its not an easy problem to tackle. Other methods that have been suggested have been bombarding the surface with asteroids from the asteroid belt (many of them have a lot of solid gasses on them) or detonating nuclear bombs (bad idea IMO).

    -everphilski-

  11. Official news from ESA by Volanin · · Score: 4, Informative

    From ESA:

    For the first time in the history of planetary exploration, the MARSIS radar on board ESA's Mars Express has provided direct information about the deep subsurface of Mars.

    First data include buried impact craters, probing of layered deposits at the north pole and hints of the presence of deep underground water-ice.

    The subsurface of Mars has been so far unexplored territory. Only glimpses of the Martian depths could be deduced through analysis of impact crater and valley walls, and by drawing cross-sections of the crust deduced from geological mapping of the surface.

    With measurements taken only for a few weeks during night-time observations last summer, MARSIS - the Mars Advanced Radar for Subsurface and Ionospheric Sounding - is already changing our perception of the Red Planet, adding to our knowledge the missing 'third' dimension: the Martian interior.

    First results reveal an almost circular structure, about 250 km in diameter, shallowly buried under the surface of the northern lowlands of the Chryse Planitia region in the mid-latitudes on Mars. The scientists have interpreted it as a buried basin of impact origin, possibly containing a thick layer of water-ice-rich material.

    To draw this first exciting picture of the subsurface, the MARSIS team studied the echoes of the radio waves emitted by the radar, which passed through the surface and then bounced back in the distinctive way that told the 'story' about the layers penetrated.

    These echo structures form a distinctive collection that include parabolic arcs and an additional planar reflecting feature parallel to the ground, 160 km long. The parabolic arcs correspond to ring structures that could be interpreted as the rims of one or more buried impact basins. Other echoes show what may be rim-wall 'slump blocks' or 'peak-ring' features.

    The planar reflection is consistent with a flat interface that separates the floor of the basin, situated at a depth of about 1.5 to 2.5 km, from a layer of overlying different material. In their analysis of this reflection, scientists do not exclude the intriguing possibility of a low-density, water-ice-rich material at least partially filling the basin.

    "The detection of a large buried impact basin suggests that MARSIS data can be used to unveil a population of hidden impact craters in the northern lowlands and elsewhere on the planet," says Jeffrey Plaut, Co-Principal Investigator on MARSIS. "This may force us to reconsider our chronology of the formation and evolution of the surface."

    MARSIS also probed the layered deposits that surround the north pole of Mars, in an area between 10 and 40 East longitude. The interior layers and the base of these deposits are poorly exposed. Prior interpretations could only be based on imaging, topographic measurements and other surface techniques.

    Two strong and distinct echoes coming from the area correspond to a surface reflection and subsurface interface between two different materials. By analysis of the two echoes, the scientists were able to draw the likely scenario of a nearly pure, cold water-ice layer thicker than 1 km, overlying a deeper layer of basaltic regolith. This conclusion appears to rule out the hypothesis of a melt zone at the base of the northern layered deposits.

    To date, the MARSIS team has not observed any convincing evidence for liquid water in the subsurface, but the search has only just begun. "MARSIS is already demonstrating the capability to detect structures and layers in the subsurface of Mars which are not detectable by other sensors, past or present," says Giovanni Picardi, MARSIS Principal Investigator.

    "MARSIS holds exciting promise to address, and possibly solve, a number of open questions of major geological significance," he concluded.

    --
    If I clone myself, can I call it a thread?
    If a girl winks to us, can I call it a race condition?
  12. Re:Yup by BarryNorton · · Score: 5, Informative

    NASA did not "find water" years ago... or ever! They found the gamma-ray spectrometry signature for hydrogen and proposed this was likely locked up in ice. Now a different means has been used to measure the subsurface (much more effectively in terms of depth, if less conclusively in terms of composition) and also found results not inconsistent with ice. We will probably not 'find ice' until someone goes there and drills. Until then, different means of measurement are a good idea (even though the media, and worse the bottom-feeding pseudo-journalism of sites like Slashdot, will misinterpret the conclusions that can be drawn).

  13. Re:Yup by tntguy · · Score: 5, Funny

    NASA did not "find water" years ago... or ever!

    Lies! Definitive proof of water on Mars.

  14. Since when is water vapor not a greenhouse gas? by Shivetya · · Score: 4, Informative

    I have always been under the impression that it is a greenhouse gas, probably one of the most popular ones at that.

    I would go find some good sources but will settle for Wiki...

    http://en.wikipedia.org/wiki/Greenhouse_gas

    --
    * Winners compare their achievements to their goals, losers compare theirs to that of others.