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MID
QUOTE (Bulldog1974 @ Jun 23 2008, 05:00 AM) *
http://phoenix.lpl.arizona.edu/

that should work....

more than likely, we are seeing water ice and it is subliming into the air. Dry ice would have already sublimed at those temps.




I tend to agree with the assessment.
But as usual, I'm careful about a declaration until further tests have been done...although there's probably little doubt left.


QUOTE
(stevewinn...)sound great doesn't it it must be water (ice) surely but i guess we just have to wait and see if Phoenix detects water, and if it does will it be the first time water has been detected on Mars?



If so, steve, it will merely pinpoint water-ice precisely.
We know water ice is present, without much doubt at all, since the Mars Oddysey's GRS detected quantities of it in the subsurface of the Martian polar regions in 2002.


We know it's there.



stevewinn
Cheers for the reply MID,

Phoenix takes it time analysing the samples doesn't it, i thought we'd have results back by now, these missions take too bloody long, we should be in and out like the SAS. grin2.gif
MID
QUOTE (stevewinn @ Jun 24 2008, 08:09 AM) *
Cheers for the reply MID,

Phoenix takes it time analysing the samples doesn't it, i thought we'd have results back by now, these missions take too bloody long, we should be in and out like the SAS. grin2.gif



You're welcome, steve..

You know it takes a while to actually do the testing on board a lander that's 35-40 million miles away.

There is a large matrix of procedures and commands and verifications that must be completed thoroughly for every single thing Phoenix does. The team needs to verify everything's ready prior to issuing a single command, then wait for at least 8 minutes, while the command goes up there, gets executed (which might take a few minutes, depending on what it is), and the telemetry is sent back so it can be analyzed to determine if things went as planned.

Then, there's a status check for the next phase, and the process will repeat itself. It can take hours just to make it's robotic arms reach down and scoop up a little dirt.

Further, we have to be in a position to have these commands and data streams relayed through the orbiting vehicles we have in place. There are times when we can't communicate with Phoenix directly, which adds to the timeline, of course.


We've delivered some of a scoop of dirt into the Phoenix optical microscope, and today, the procedures are being done to actually look at it, and start sending the data back to Earth. I venture a guess there's dozens of pages of procedures and commands involved in this process.

They also yesterday ran a full diagnostic on the wet chemistry laboratory, and sent the commands to thaw water ice that we brought along, which of course is the essential solvent that will be used in the experiments on another portion of that dirt sample in the scoop. We'll be putting that part of the sample into the wet chemistry module in the next day or so, and will then prepare to run the experiments there.


...by the way, the water did all melt and we're good to go!

Once that's done, and data streams start coming back, scientists will begin the analysis of the results...which of course also takes some time.


Basically, it's kinda tough running your laboratory when it's about 40 million miles away, and you can't actually do anything with it hands on.

There are a whole series of questions that need to be answered prior to doing anything, and everything from that distance with an automated piece of engineering.


The simple act of reaching down and scooping up a little dirt, and dumping it proportionately into a couple of experiment modules, can take a whole day for a team of engineers and technicians to accomplish. This is something that a man, standing there, could accomplish in a matter of 30 seconds.


Un-manned missions are cool as cool can be...and a testimony to the capabilities of the people who design and build the spacecraft. Often, however, especially at such distances, the price you pay is time, and that's just necessary to make sure everything works right from start to finish (i.e., we cannot screw this up!).


Look at it this way: Phoenix took 10 months to get where it is, 10 months of travel and a painstaking (as well as nerve wracking) descent and landing, so it can do it's 3 month science mission. There's a hell of a lot packed into the mission--painstaking, precise scientific work. It's difficult, and requires profound attention to detail. After 10 months of transit, I feel we can wait a while for good data.


I am absolutely confident that this team of very fine people will get the data they're looking for and will be able to make substantive conclusions based on them. It may take some time, however! It's the nature of the beast!


thumbsup.gif
Incorrigible1
QUOTE (MID @ Jun 24 2008, 04:46 PM) *
I am absolutely confident that this team of very fine people will get the data they're looking for and will be able to make substantive conclusions based on them. It may take some time, however! It's the nature of the beast!


thumbsup.gif

MID, perhaps you should stop bye the control room and bust some chops. Give 'em some hell, and let them know how it was done in the old days!
MID
QUOTE (Incorrigible1 @ Jun 24 2008, 05:50 PM) *
MID, perhaps you should stop bye the control room and bust some chops. Give 'em some hell, and let them know how it was done in the old days!




Well, you know, back in the "old days" folks took their time too...when they could.
Of course, on a manned mission where crap could hit the fan and threaten the lives of human folk...it was more like, "OK, let's fix the problem, NOW, and not screw it up."

...coffee and cigarettes were staples in those days, for good reason!

With Phoenix, we do have some time constraints, but not quite like those on something like Apollo 13, or the descent to lunar landing on Apollo 11... I'm perfectly content to wait for things to get done properly, since we've got the time, and it's built into the plans.


I think the controllers on today's missions rather reflect the ethic present back in days of yore. I remember seeing John Lewellyn, one of Gene Kranz' control team on Apollo 13 saying something to the effect of,


"I didn't give a sh** what I'd been thinkin', how many problems I had...when I walked through those doors and I shut 'em behind me, I was in the control center and I'd better get my act together because what I was goin' to be doing was important."

I think that same ethic is posessed by all the fine people today that man the operations, be it manned or unmanned...(in fact, I know it is. I been watchin' em. They make me proud as hell...)


I don't think they need a kick in the a**. I think they could kick all of our asses!
They are the best there are...and as always, that's what's necessary!

I'd just be thankful for the luxury of time!






stevewinn
so what's the latest news from the red planet?

i have a question, you know the ovens on the phoenix, if they heat the samples up and if water is present in the sample will it become liquid or will it be vapour, if it does end up in a liquid form how will they empty the "testing" chamber?
Incorrigible1
QUOTE (stevewinn @ Jun 26 2008, 05:49 AM) *
so what's the latest news from the red planet?

i have a question, you know the ovens on the phoenix, if they heat the samples up and if water is present in the sample will it become liquid or will it be vapour, if it does end up in a liquid form how will they empty the "testing" chamber?

I don't believe the chambers are emptied. There are several chambers to perform several tests. Eight, I believe.
stevewinn
QUOTE (Incorrigible1 @ Jun 26 2008, 05:16 PM) *
I don't believe the chambers are emptied. There are several chambers to perform several tests. Eight, I believe.


cheers for the reply,
Bulldog1974
http://www.comcast.net/articles/news-scien...-SPACE-MARS-DC/

Some interesting results...
Slave2Fate
QUOTE (Bulldog1974 @ Jun 27 2008, 12:38 AM) *


yea, I read that in another post, very interesting. thumbsup.gif

BTW, did they ever find out what that was under the lander that looked like ice?
stevewinn
hey, that's great news, so the soil isn't toxic? so does that mean you could grow some sort of plant life?
MID
QUOTE (stevewinn @ Jun 27 2008, 08:46 AM) *
hey, that's great news, so the soil isn't toxic? so does that mean you could grow some sort of plant life?



steve,

I think that's precisely what the preliminary results are indicating. It's pretty friendly looking stuff. It has nutrients, minerals, etc, and an appropriate Ph to grow Earth plants in it. It appears completely benign, no toxins...

Almost garden soil.
stevewinn
QUOTE (MID @ Jun 27 2008, 03:15 PM) *
steve,

I think that's precisely what the preliminary results are indicating. It's pretty friendly looking stuff. It has nutrients, minerals, etc, and an appropriate Ph to grow Earth plants in it. It appears completely benign, no toxins...

Almost garden soil.



its amazing isn't it, so do you reckon if we took some plant from earth that could withstand the cold temperatures and has long as we provided it with water it would grow wouldnt it?
MID
QUOTE (stevewinn @ Jun 27 2008, 01:15 PM) *
its amazing isn't it, so do you reckon if we took some plant from earth that could withstand the cold temperatures and has long as we provided it with water it would grow wouldnt it?




Personally, I would not be inclined to speculate on that possibility.
There are of course very hearty species of plants here on Earth that are able to thrive in environments that one would never expect. Antarctica, for one, is an area where we are researching some of these types of plants.

However, based upon initial results of the surface layer of soil in one location on Mars' surface, and realizing that the conditions on Mars are hostile to life as we know it (think of Antarctica at 100,000 feet altitude and it's somewhat similar), to say I think so would be somewhat nonsensical and utterly speculative on my part. What we know is that this particular sample of soil seems to be Earth-like, and , if we had it here on Earth, we could likely grow something in it.

But as to Mars? Well, maybe. But I have no idea at this point. There's alot more data to be collected and research to be done.
The Maharaja
I KNEW IT I KNEW IT what else are we going to discover i can't wait
stevewinn
QUOTE (MID @ Jun 28 2008, 05:33 PM) *
Personally, I would not be inclined to speculate on that possibility.
There are of course very hearty species of plants here on Earth that are able to thrive in environments that one would never expect. Antarctica, for one, is an area where we are researching some of these types of plants.

However, based upon initial results of the surface layer of soil in one location on Mars' surface, and realizing that the conditions on Mars are hostile to life as we know it (think of Antarctica at 100,000 feet altitude and it's somewhat similar), to say I think so would be somewhat nonsensical and utterly speculative on my part. What we know is that this particular sample of soil seems to be Earth-like, and , if we had it here on Earth, we could likely grow something in it.

But as to Mars? Well, maybe. But I have no idea at this point. There's alot more data to be collected and research to be done.



cheers MID,

just on the off chance you might know, how deep can phoenix dig?
MID
QUOTE (stevewinn @ Jun 28 2008, 03:11 PM) *
cheers MID,

just on the off chance you might know, how deep can phoenix dig?




I honestly don't, steve...


But I cannot imagine it's much more than a few inches...



stevewinn
QUOTE (MID @ Jun 29 2008, 07:42 PM) *
I honestly don't, steve...


But I cannot imagine it's much more than a few inches...


i was thinking the same, any way lets hope the next load of NEWS from Phoenix is even better, keep up the good work MID. thumbsup.gif
Incorrigible1
QUOTE (stevewinn @ Jun 28 2008, 02:11 PM) *
cheers MID,

just on the off chance you might know, how deep can phoenix dig?

And did it bring any turnip seeds?
ROGER
The Phoenix sight says the just under 8 foot robotic arm can dig 0.5 meters (1.6 Feet) and in tests in Death Valley in the year 2000 , made a 10 inch trench in 4 hours.

Pretty good for little fella! yes.gif
stevewinn
QUOTE (ROGER @ Jun 30 2008, 07:17 AM) *
The Phoenix sight says the just under 8 foot robotic arm can dig 0.5 meters (1.6 Feet) and in tests in Death Valley in the year 2000 , made a 10 inch trench in 4 hours.

Pretty good for little fella! yes.gif


cheers Roger, like you say that's pretty deep, thumbsup.gif
MID
QUOTE (stevewinn @ Jun 29 2008, 05:05 PM) *
i was thinking the same, any way lets hope the next load of NEWS from Phoenix is even better, keep up the good work MID. thumbsup.gif




Thanks, steve...and


QUOTE
The Phoenix sight says the just under 8 foot robotic arm can dig 0.5 meters (1.6 Feet) and in tests in Death Valley in the year 2000 , made a 10 inch trench in 4 hours.



Thanks ROG, for digging that tid-bit up!


You're right, that's a hell of a machine if it can do that!


Ghost Ship
What's the latest news about the white stuff? Were is waspie?

Hello everyone.
stevewinn
QUOTE (Ghost Ship @ Jul 8 2008, 01:23 AM) *
What's the latest news about the white stuff? Were is waspie?

Hello everyone.



Waspie has deserted us, the mission has been going now for 42 days and all we have to show for it, is one scoop of soil which turned out to be similar to garden soil, which is great news, but for the last few days they've been repeating the process of digging/scooping a second sample of soil for analysis, to compare to the first sample,....................the mission is only 3 months long and its took 42 days for one scoop, so if NASA dont hurry up by the missions end we'll have just 3 scoops, i was hoping for a lot more.
Waspie_Dwarf
QUOTE (Ghost Ship @ Jul 8 2008, 01:23 AM) *
Were is waspie?



QUOTE (stevewinn @ Jul 8 2008, 03:13 PM) *
Waspie has deserted us,

I haven't deserted anyone. If you want to know where I've been then you can find the answer in my blog HERE, which is more appropriate than discussing it here. As soon as I get a chance I will post the missing NASA announcements, news releases and pictures, but there is a lot of catching up to do, so please bae with me.


QUOTE
the mission is only 3 months long and its took 42 days for one scoop, so if NASA dont hurry up by the missions end we'll have just 3 scoops, i was hoping for a lot more.

It is not the number of scoops that matters, it is the quality of the analysis that is carried out on them. It is better to have 3 good sets of results than 100 useless ones. These things take time. The most important discoveries will be made long after this mission has ended, as the scientists review the vast amount of data returned.
Waspie_Dwarf
Here, as promised, are the images and news releases from NASA which I missed as a result of my forced abscence. Some of them will be covering ground already discussed in this thread, but I hope no one objects too much to that - Waspie.
_______________________________


NASA's Phoenix Mars Lander Delivers Soil Sample to Microscope
06.13.08

TUCSON, Ariz. -- New observations from NASA's Phoenix Mars Lander provide the most magnified view ever seen of Martian soil, showing particles clumping together even at the smallest visible scale.

In the past two days, two instruments on the lander deck -- a microscope and a bake-and-sniff analyzer -- have begun inspecting soil samples delivered by the scoop on Phoenix's Robotic Arm.

linked-image
This photograph shows the Robotic Arm on NASA's
Phoenix Mars Lander carrying a scoop of Martian
soil bound for the spacecraft's microscope.
Image credit: NASA/JPL-Caltech/University of
Arizona


"This is the first time since the Viking missions three decades ago that a sample is being studied inside an instrument on Mars," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson.

Stickiness of the soil at the Phoenix site has presented challenges for delivering samples, but also presents scientific opportunities. "Understanding the soil is a major goal of this mission and the soil is a bit different than we expected," Smith said. "There could be real discoveries to come as we analyze this soil with our various instruments. We have just the right instruments for the job."

Images from Phoenix's Optical Microscope show nearly 1,000 separate soil particles, down to sizes smaller than one-tenth the diameter of a human hair. At least four distinct minerals are seen.

"It's been more than 11 years since we had the idea to send a microscope to Mars and I'm absolutely gobsmacked that we're now looking at the soil of Mars at a resolution that has never been seen before," said Tom Pike of Imperial College London. He is a Phoenix co-investigator working on the lander's Microscopy, Electrochemistry and Conductivity Analyzer.

The sample includes some larger, black, glassy particles as well as smaller reddish ones. "We may be looking at a history of the soil," said Pike. "It appears that original particles of volcanic glass have weathered down to smaller particles with higher concentration of iron."

The fine particles in the soil sample closely resemble particles of airborne dust examined earlier by the microscope.

Atmospheric dust at the Phoenix site has remained about the same day-to-day so far, said Phoenix co-investigator and atmospheric scientist Nilton Renno of the University of Michigan, Ann Arbor.

"We've seen no major dust clouds at the landing site during the mission so far," Renno said. "That's not a surprise because we landed when dust activity is at a minimum. But we expect to see big dust storms at the end of the mission. Some of us will be very excited to see some of those dust storms reach the lander."

Studying dust on Mars helps scientists understand atmospheric dust on Earth, which is important because dust is a significant factor in global climate change.

"We've learned there is well-mixed dust in the Martian atmosphere, much more mixed than on Earth, and that's a surprise," Renno said. Rather than particles settling into dust layers, strong turbulence mixes them uniformly from the surface to a few kilometers above the surface.

Scientists spoke at a news briefing today at the University of Arizona, where new color views of the spacecraft's surroundings were shown.

"We are taking a high-quality, 360-degree look at all of Mars that we can see from our landing site in color and stereo," said Mark Lemmon, Surface Stereo Imager lead from Texas A&M University, College Station.

"These images are important to provide the context of where the lander is on the surface. The panorama also allows us to look beyond our workspace to see how the polygon structures connect with the rest of the area. We can identify interesting things beyond our reach and then use the camera's filters to investigate their properties from afar."

The Phoenix mission is led by Smith at the University of Arizona with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For more about Phoenix, visit: http://www.nasa.gov/phoenix and http://phoenix.lpl.arizona.edu.

Media contacts: Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu

2008-109


Source: NASA - Phoenix - News
Waspie_Dwarf
Microscopic Comparison of Airfall Dust to Martian Soil
06.13.08

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This pair of images taken by the Optical Microscope on NASA's Phoenix Mars Lander offers a side-by-side comparison of an airfall dust sample collected on a substrate exposed during landing (left) and a soil sample scooped up from the surface of the ground beside the lander. In both cases the sample is collected on a silicone substrate, which provides a sticky surface holding sample particles for observation by the microscope.

Similar fine particles at the resolution limit of the microscope are seen in both samples, indicating that the soil has formed from settling of dust.

The microscope took the image on the left during Phoenix's Sol 9 (June 3, 2008), or the ninth Martian day after landing. It took the image on the right during Sol 17 (June 11, 2008).

The scale bar is 1 millimeter (0.04 inch).

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image NASA/JPL-Caltech/University of Arizona

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Robotic Arm Camera Image of the South Side of the Thermal and Evolved-Gas Analyzer (Door TA4 receiving sample)
06.13.08

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The Thermal and Evolved-Gas Analyzer (TEGA) instrument aboard NASA's Phoenix Mars Lander is shown with one set of oven doors open and dirt from a sample delivery. After the "seventh shake" of TEGA, a portion of the dirt sample entered the oven via a screen for analysis. This image was taken by the Robotic Arm Camera on Sol 18 (June 13, 2008), or 18th Martian day of the mission.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Max Planck Institute

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
First Sample Delivery to Mars Microscope
06.13.08

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The Robotic Arm on NASA's Phoenix Mars Lander has just delivered the first sample of dug-up soil to the spacecraft's microscope station in this image taken by the Surface Stereo Imager during the mission's Sol 17 (June 11, 2008), or 17th Martian day of the mission.

The scoop is positioned above the box containing key parts of Phoenix's Microscopy, Electrochemistry and Conductivity Analyzer, or MECA, instrument suite. It has sprinkled a small amount of soil into a notch in the MECA box where the microscope's sample wheel is exposed. The wheel turns to present sample particles on various substrates to the Optical Microscope for viewing.

The scoop is about 8.5 centimeters (3.3 inches) wide. The top of the MECA box is 20 centimeters (7.9 inches) wide. This image has been lightened to make details more visible.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image Credit: NASA/JPL-Caltech/University of Arizona/Texas A&M

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
"Dodo" and "Goldilocks" Trenches
06.13.08

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This image of the informally named "Dodo" (on left) and "Goldilocks" (on right) trenches was taken by the Surface Stereo Imager (SSI) aboard NASA's Phoenix Mars Lander on Sol 17 (June 11, 2008) the 17th Martian day of the mission. "Baby Bear" is the name of the sample taken from "Goldilocks." This sample was delivered to the Thermal and Evolved- Gas Analyzer (TEGA) instrument for analysis.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University/SSV

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Looking North from Phoenix
06.13.08

linked-image

This series of images, taken by NASA's Phoenix Mars Lander's Surface Stereo Imager, has been combined into a panoramic view looking north from the lander. The area depicted is beyond the immediate workspace of the lander and shows a system of polygons and troughs that connect with the ones Phoenix will be investigating in depth. The images in the panorama were taken on Sol 14 (June 8, 2008), or the 14th Martian day after landing.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA’s Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Panorama of Phoenix Landing Area Looking Southeast
06.13.08

linked-image

This image was taken by NASA’s Phoenix Mars Lander’s Surface Stereo Imager on Sol 15 (June 9, 2008), the 15th Martian day after landing. This panorama looks to the southeast and shows rocks casting shadows, polygons on the surface and in the far horizon, Phoenix’s backshell gleams in the distance.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA’s Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

NASA/JPL-Caltech/University of Arizona

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Phoenix's Solar Panel and Robotic Arm
06.13.08

linked-image

This image shows NASA’s Phoenix Mars Lander’s solar panel and the lander’s Robotic Arm with a sample in the scoop. The image was taken by the lander’s Surface Stereo Imager looking west during Phoenix’s Sol 16 (June 10, 2008), or the 16th Martian day after landing. The image was taken just before the sample was delivered to the Optical Microscope. This view is a part of the "mission success" panorama that will show the whole landing site in color.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

NASA/JPL-Caltech/University of Arizona.

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Zooming in on the Martian Soil
06.13.08

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Three zoomed-in portions are shown with an image of Martian soil particles taken by the Optical Microscope on NASA's Phoenix Mars Lander.

The left zoom box shows a composite particle. The top of the particle has a green tinge, possibly indicating olivine. The bottom of the particle has been reimaged at a different focus position in black and white (middle zoom box), showing that this is a clump of finer particles.

The right zoom box shows a rounded, glassy particle, similar to those which have also been seen in an earlier sample of airfall dust collected on a surface exposed during landing.

The shadows at the bottom of image are of the beams of the Atomic Force Microscope.

The microscope took this image during Phoenix's Sol 17 (June 11, 2008), or the 17th Martian day after landing. The scale bar is 1 millimeter (0.04 inch).

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA’s Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image Credit: NASA/JPL-Caltech/University of Arizona/Imperial College London.

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Microscopic Image of Martian Surface Material on a Silicone Substrate
06.13.08

linked-image

This image taken by the Optical Microscope on NASA's Phoenix Mars Lander shows soil sprinkled from the lander's Robot Arm scoop onto a silicone substrate. The substrate was then rotated in front of the microscope. This is the first sample collected and delivered for instrumental analysis onboard a planetary lander since NASA's Viking Mars missions of the 1970s. It is also the highest resolution image yet seen of Martian soil.

The image is dominated by fine particles close to the resolution of the microscope. These particles have formed clumps, which may be a smaller scale version of what has been observed by Phoenix during digging of the surface material.

The microscope took this image during Phoenix's Sol 17 (June 11), or the 17th Martian day after landing. The scale bar is 1 millimeter (0.04 inch).

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image NASA/JPL-Caltech/University of Arizona.

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Sol 17 Weather Report
06.13.08

linked-image

Another sunny and relatively clear day at NASA’s Phoenix Mars Lander site. Atmospheric pressure on Sol 17 (June 11, 2008) was 8.35 millibars, with a maximum of minus 26 degrees Celsius (-15 Fahrenheit and a low of minus 82 Celsius (minus 116 Fahrenheit). Winds were calm at 14 km/h (8.7 miles per hour) from the southwest.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA’s Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Canadian Space Agency. Wind by Denmark’s University of Aarhus.

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Early Spring Dust Storms at the North Pole of Mars
06.13.08

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Early spring typically brings dust storms to northern polar Mars. As the north polar cap begins to thaw, the temperature difference between the cold frost region and recently thawed surface results in swirling winds. The choppy dust clouds of at least three dust storms are visible in this mosaic of images taken by the Mars Global Surveyor spacecraft in 2002. The white polar cap is frozen carbon dioxide.

Image NASA/JPL/Malin Space Science Systems.

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
Nanobuckets
06.13.08

linked-image

Microscopic View of Soil on a Micromachined Silicone Substrate

This image taken by the Optical Microscope on NASA's Phoenix Mars Lander on Sol 17 (June 11, 2008) shows soil sprinkled from the lander's Robot Arm scoop onto a substrate that has been micromachined to produce different patterns of pegs and holes to capture the smallest particles in the Martian soil.

The micromachined substrates are designed to tightly hold particles for imaging using the Atomic Force Microscope on Phoenix, which should be able to zoom in another 40 times beyond the magnification in this Optical Microscope image. Each stripe has a different spacing of pegs and holes. The strip third from the left, with a peg spacing of 5 micrometers, has been most successful in collecting the particles. These substrates were fabricated by Imperial College London as the United Kingdom hardware contribution to the Phoenix mission.

For scale, each strip is 0.4 millimeter (0.016 inch) wide.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image NASA/JPL-Caltech/University of Arizona/Imperial College London

› Full Resolution

Source: NASA - Phoenix - Images
Waspie_Dwarf
First Dodo Trench with White Layer Visible in Dig Area
06.13.08

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This color image was taken by NASA's Phoenix Mars Lander's Stereo Surface Imager on the ninth Martian day of the mission, or Sol 9 (June 3, 2008). This image of the trench shows a white layer that has been uncovered by the Robotic Arm (RA) scoop and is now visible in the wall of the trench. This trench was the first one dug by the RA to understand the Martian soil and plan the digging strategy.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image Credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

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Source: NASA - Phoenix - Images
Waspie_Dwarf
Blowing in the Wind Animations
06.13.08

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These are two separate, side-by-side animations made from the same nine images the Surface Stereo Imager (SSI) on NASA's Phoenix Mars Lander took looking into the sky after 5:17 p.m. local time on Sol 8 (June 2, 2008), the eighth Martian day of the mission. The SSI was pointed almost straight up, toward the southwest. Zenith is near the top of the center frame.

In the left animation, the images were stretched to enhance contrast. The right animation highlights variations between each image and the next. The variations are likely dust blown by winds passing through the SSI's field of view. The images suggest the dust is blowing from west to east.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image Credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

Source: NASA - Phoenix - Images
Waspie_Dwarf
Digging Movie from Phoenix's Sol 18
06.13.08

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The Surface Stereo Imager on NASA's Phoenix Mars Lander recorded the images combined into this movie of the lander's Robotic Arm enlarging and combining the two trenches informally named "Dodo" (left) and "Goldilocks."

The 21 images in this sequence were taken over a period of about 2 hours during Phoenix's Sol 18 (June 13, 2008), or the 18th Martian day since landing.

The main purpose of the Sol 18 dig was to dig deeper for learning the depth of a hard underlying layer. A bright layer, possibly ice, was increasingly exposed as the digging progressed. Further digging and scraping in the combined Dodo-Goldilocks trench was planned for subsequent sols.

The combined trench is about 20 centimeters (about 8 inches) wide. The depth at the end of the Sol 18 digging is 5 to 6 centimeters (about 2 inches).

The Goldilocks trench was the source of soil samples "Baby Bear" and "Mama Bear," which were collected on earlier sols and delivered to instruments on the lander deck. The Dodo trench was originally dug for practice in collecting and depositing soil samples.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image Credit: NASA/JPL-Caltech/University of Arizona/Texas A&M

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Source: NASA - Phoenix - Images
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'Dodo-Goldilocks' Trench Dug by Phoenix
06.13.08

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This color image was acquired by NASA's Phoenix Mars Lander's Surface Stereo Imager on the 19th day of the mission, or Sol 19 (June 13, 2008), after the May 25, 2008, landing. This image shows one trench informally called "Dodo-Goldilocks" after two digs (dug on Sol 18, or June 12, 2008) by Phoenix's Robotic Arm. The trench is 22 centimeters (8.7 inches) wide and 35 centimeters (13.8 inches) long. At its deepest point, the trench is 7 to 8 centimeters (2.7 to 3 inches) deep.

White material, possibly ice, is located only at the upper portion of the trench, indicating that it is not continuous throughout the excavated site. According to scientists, the trench might be exposing a ledge, or only a portion of a slab, of the white material.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

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Source: NASA - Phoenix - Images
Waspie_Dwarf
NASA's Phoenix Lander Bakes Sample, Arm Digs Deeper
06.16.08

TUCSON, Ariz. – One of the ovens on NASA's Phoenix Mars Lander continued baking its first sample of Martian soil over the weekend, while the Robotic Arm dug deeper into the soil to learn more about white material first revealed on June 3.

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This color-coded elevation map shows the "Dodo
-Goldilocks" trench dug by the Robotic Arm on
NASA's Phoenix Mars Lander.
Image credit: NASA/JPL-Caltech/University of
Arizona/Texas A&M University/NASA Ames
Research Center


"The oven is working very well and living up to our expectations," said Phoenix co-investigator Bill Boynton of the University of Arizona, Tucson. Boynton leads the Thermal and Evolved-Gas Analyzer (TEGA), or oven instrument, for Phoenix.

Phoenix has eight separate tiny ovens to bake and sniff the soil and look for volatile ingredients, such as water. This baking is performed at three different temperature ranges.

On Sol 18 (June 12), the lander's Robotic Arm dug deeper into the two trenches, informally called "Dodo" and "Goldilocks," where white material was previously found. This created one large trench, now called "Dodo-Goldilocks."

"We have continued to excavate in the Dodo-Goldilocks trench to expose more of the light-toned material, and we will monitor the site," said Robotic Arm lead scientist Ray Arvidson of the University of Washington, St. Louis. "If the material is ice, it should change with time. Frost may form on it, or it could slowly sublimate." Sublimation is the process where a solid changes directly into gas.

The Dodo-Goldilocks trench is 22 centimeters wide (8.7 inches) and 35 centimeters long (13.8 inches). The trench is seven to eight centimeters (2.7 to 3 inches) deep at its deepest. The deepest portion is closest to the lander.

The white material is located only at the shallowest part of the trench, farthest from the lander, indicating that it is not continuous throughout the excavated site. The trench might be exposing a ledge, or only a portion of a slab, of the white material, according to scientists.

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For more about Phoenix, visit: http://www.nasa.gov/phoenix and http://phoenix.lpl.arizona.edu.

Media contacts: Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu


Source: NASA - Phoenix - News
Waspie_Dwarf
'Dodo-Goldilocks' Trench Elevation Map
06.16.08

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This color-coded elevation map shows the "Dodo-Goldilocks" trench dug by the Robotic Arm on NASA's Phoenix Mars Lander. The trench, originally two separate trenches nicknamed "Dodo" (left) and "Goldilocks" (right), became one after further digging on the 18th Martian day, or Sol 18, of the mission (June 12, 2008). The trench is 7 to 8 centimeters (2.7 to 3 inches) at its deepest (blue). Because the terrain itself is inclined at a 14-degree angle, the highest areas (pink) are about 20 centimeters (7.8 inches) above the lowest areas.

The trench is 22 centimeters (8.7 inches) wide and 35 centimeters (13.8 inches) long. Its deepest portion is closest to the lander.

This picture was taken by Phoenix's Surface Stereo Imager on Sol 19 (June 13, 2008).

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University/NASA Ames Research Center

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Source: NASA - Phoenix - Images
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Phoenix Makes First Trench in Science Preserve
06.17.08

NASA's Phoenix Mars Lander began digging in an area called "Wonderland" early Tuesday, taking its first scoop of soil from a polygonal surface feature within the "national park" region that mission scientists have been preserving for science.

The lander's Robotic Arm created the new test trench called "Snow White" on June 17, the 22nd Martian day, or sol, after the Phoenix spacecraft landed on May 25. Newly planned science activities will resume no earlier than Sol 24 as engineers look into how the spacecraft is handling larger than expected amounts of data.

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NASA's Phoenix Mars Lander began excavating a
new trench, dubbed "Snow White," in a patch
of Martian soil located near the center of a
polygonal surface feature, nicknamed "Cheshire
Cat."
Image credit: NASA/JPL-Caltech/University of
Arizona/Texas A&M University


During Tuesday’s dig, the arm didn't reach the hard white material, possibly ice, that Phoenix exposed previously in the first trench it dug into the Martian soil.

That's just what scientists both expected and wanted. The Snow White trench is near the center of a relatively flat hummock, or polygon, named "Cheshire Cat," where scientists predict there will be more soil layers or thicker soil above possible white material.

The Snow White trench is about two centimeters deep (about three-quarters of an inch) and 30 centimeters (about a foot) long. The Phoenix team plans at least one more day of digging deeper into the Snow White trench.

They will study soil structure in the Snow White trench to decide at what depths they will collect samples from a future trench planned for the center of the polygon.

Meanwhile, the Thermal and Evolved-Gas Analyzer (TEGA) instrument continues its ongoing experiment in the first of its eight ovens.

TEGA has eight separate tiny ovens to bake and sniff the soil to look for volatile ingredients, such as water. The baking is performed at three different temperature ranges.

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For more about Phoenix, visit: http://www.nasa.gov/phoenix and http://phoenix.lpl.arizona.edu.

Media contacts: Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu


Source: NASA - Phoenix - News
Waspie_Dwarf
Digging of 'Snow White' Begins
06.17.08

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NASA's Phoenix Mars Lander began excavating a new trench, dubbed "Snow White," in a patch of Martian soil near the center of a polygonal surface feature, nicknamed "Cheshire Cat." The "dump pile" is located at the top of the trench, the side farthest away from the lander, and has been dubbed "Croquet Ground." The digging site has been named "Wonderland."

The trench is about 2 centimeters (.8 inches) deep and 30 centimeters (about 12 inches) long.

At this early stage of digging, the Phoenix team did not expect to find any of the white material seen in the mission's first trench, now called "Dodo-Goldilocks." That trench showed white material at a depth of about 5 centimeters (2 inches). More digging of Snow White is planned for coming sols, or Martian days.

Snow White was dug on Sol 22 (June 17, 2008) with Phoenix's Robotic Arm. This picture was acquired on the same day by the lander's Surface Stereo Imager.

This image has been enhanced to brighten shaded areas.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University/NASA Ames

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Source: NASA - Phoenix - Images
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NASA Mars Lander to Dig; Team Probes Flash Memory
06.18.08

TUCSON, Ariz. -- NASA's Phoenix Mars Mission generated an unusually high volume of spacecraft housekeeping data on Tuesday causing the loss of some non-critical science data. Phoenix engineers are analyzing why this anomaly occurred. The science team is planning spacecraft activities for Thursday that will not rely on Phoenix storing science data overnight but will make use of multiple communication relays to gain extra data quantity.

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This photograph shows the Robotic Arm on NASA's
Phoenix Mars Lander carrying a scoop of Martian
soil bound for the spacecraft's microscope"
Image credit: NASA/JPL-Caltech/University of
Arizona

"The spacecraft is healthy and fully commandable, but we are proceeding cautiously until we understand the root cause of this event," said Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory.

Usually Phoenix generates a small amount of data daily about maintaining its computer files, and this data gets a high priority in what gets stored in the spacecraft's non-volatile flash memory. On Tuesday, the quantity of this data was so high that it prevented science data from being stored in flash memory, so the remaining science data onboard Wednesday, when the spacecraft powered down for the Martian night after completing its 22nd Martian day, or sol, since landing, was not retained. None of that science data was high-priority data. Almost all was imaging that can be retaken, with the exception of images taken of a surface that Phoenix's arm dug into after the images were taken.

To avoid stressing Phoenix's capacity for storing data in flash memory while powered off for overnight sleeps, the team commanded Phoenix Tuesday evening to refrain from any new science investigations on Wednesday and to lower the priority for the type of file-housekeeping data that exceeded expected volume on Tuesday.

"We can continue doing science that does not rely on non-volatile memory," Goldstein said. Most science data collected during the mission has been downlinked to Earth on the same sol it has been collected, not requiring overnight storage, but on some sols the team has intentionally included imaging that yields more data than can fit in the afternoon communication passes. This has been done in order to take advantage of the capacity to downlink additional data during communications passes on the following Martian mornings. In the short term, while the root cause of the unexpected amount of housekeeping data is being determined, the science team will forgo that strategy of storing data overnight.

Meanwhile, extra communication-relay opportunities have been added to Thursday's schedule, so the science plan for the day will be able to generate plentiful data without needing overnight storage. Trench-digging, imaging and weather monitoring are in the plan.

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For more about Phoenix, visit: http://www.nasa.gov/phoenix and http://phoenix.lpl.arizona.edu.

Media contacts: Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu


Source: NASA - Phoenix - News
Waspie_Dwarf
Bright Chunks at Phoenix Lander's Mars Site Must Have Been Ice
06.19.08

TUCSON, Ariz. – Dice-size crumbs of bright material have vanished from inside a trench where they were photographed by NASA's Phoenix Mars Lander four days ago, convincing scientists that the material was frozen water that vaporized after digging exposed it.

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See below to see images that show sublimation of
ice in the trench informally called "Dodo-Goldilocks"
over the course of four days.
Image credit: NASA/JPL-Caltech/University of
Arizona/Texas A&M University


"It must be ice," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson. "These little clumps completely disappearing over the course of a few days, that is perfect evidence that it's ice. There had been some question whether the bright material was salt. Salt can't do that."

The chunks were left at the bottom of a trench informally called "Dodo-Goldilocks" when Phoenix's Robotic Arm enlarged that trench on June 15, during the 20th Martian day, or sol, since landing. Several were gone when Phoenix looked at the trench early today, on Sol 24.

Also early today, digging in a different trench, the Robotic Arm connected with a hard surface that has scientists excited about the prospect of next uncovering an icy layer.

The Phoenix science team spent Thursday analyzing new images and data successfully returned from the lander earlier in the day.

Studying the initial findings from the new "Snow White 2" trench, located to the right of "Snow White 1," Ray Arvidson of Washington University in St. Louis, co-investigator for the robotic arm, said, "We have dug a trench and uncovered a hard layer at the same depth as the ice layer in our other trench."

On Sol 24, Phoenix extended the first trench in the middle of a polygon at the "Wonderland" site. While digging, the Robotic Arm came upon a firm layer, and after three attempts to dig further, the arm went into a holding position. Such an action is expected when the Robotic Arm comes upon a hard surface.

Meanwhile, the spacecraft team at Lockheed Martin Space Systems in Denver is preparing a software patch to send to Phoenix in a few days so scientific data can again be saved onboard overnight when needed. Because of a large amount a duplicative file-maintenance data generated by the spacecraft Tuesday, the team is taking the precaution of not storing science data in Phoenix's flash memory, and instead downlinking it at the end of every day, until the conditions that produced those duplicative data files are corrected.

"We now understand what happened, and we can fix it with a software patch," said Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena. "Our three-month schedule has 30 days of margin for contingencies like this, and we have used only one contingency day out of 24 sols. The mission is well ahead of schedule. We are making excellent progress toward full mission success."

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For more about Phoenix, visit: http://www.nasa.gov/phoenix and http://phoenix.lpl.arizona.edu.

Media contacts: Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu


Source: NASA - Phoenix - News
Waspie_Dwarf
Disappearing Ice
06.19.08

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These images were acquired by NASA's Phoenix Mars Lander's Surface Stereo Imager on the 21st and 25th days of the mission, or Sols 20 and 24 (June 15 and 19, 2008).

These images show sublimation of ice in the trench informally called "Dodo-Goldilocks" over the course of four days.

In the lower left corner, lumps disappear, similar to the process of evaporation.

The Phoenix Mission is led by the University of Arizona, Tucson, on behalf of NASA. Project management of the mission is by NASA's Jet Propulsion Laboratory, Pasadena, Calif. Spacecraft development is by Lockheed Martin Space Systems, Denver.

Image credit: NASA/JPL-Caltech/University of Arizona/Texas A&M University

Source: NASA - Phoenix - Images
Waspie_Dwarf
NASA Phoenix Mars Lander Confirms Frozen Water
06.20.08

TUCSON, Ariz. -- Scientists relishing confirmation of water ice near the surface beside NASA's Phoenix Mars Lander anticipate even bigger discoveries from the robotic mission in the weeks ahead.

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These color images were acquired by NASA's
Phoenix Mars Lander's Surface Stereo Imager on
the 21st and 25th days of the mission, or Sols 20
and 24 (June 15 and 18, 2008).
Image credit: NASA/JPL-Caltech/University of
Arizona/Texas A&M University


"It is with great pride and a lot of joy that I announce today that we have found proof that this hard bright material is really water ice and not some other substance," said Phoenix Principal Investigator Peter Smith of the University of Arizona, Tucson, during a Friday news briefing to announce the confirmation of water ice.

"The truth we're looking for is not just looking at ice. It is in finding out the minerals, chemicals and hopefully the organic materials associated with these discoveries," said Smith

The mission has the right instruments for analyzing soil and ice to determine whether the local environment just below the surface of far-northern Mars has ever been favorable for microbial life. Key factors are whether the water ever becomes available as a liquid and whether organic compounds are present that could provide chemical building blocks and energy for life. Phoenix landed on May 25 for a Mars surface mission planned to last for three months.

"These latest developments are a major accomplishment and validation of the Mars Program's 'follow-the-water' exploration framework," said Doug McCuistion at NASA Headquarters, Washington, director of the space agency's Mars Program. "This specific discovery is the result of an outstanding team working with a robust spacecraft that has allowed them to work ahead of their original science schedule."

The key new evidence is that chunks of bright material exposed by digging on June 15 and still present on June 16 had vaporized by June 19. "This tells us we've got water ice within reach of the arm, which means we can continue this investigation with the tools we brought with us," said Mark Lemmon of Texas A&M University, College Station, lead scientist for Phoenix's Surface Stereo Imager camera. He said the disappearing chunks could not have been carbon-dioxide ice at the local temperatures because that material would not have been stable for even one day as a solid.

The disappearing chunks were in a trench to the northwest of the lander. A hard material, possibly more ice, but darker than the bright material in the first trench, has been detected in a second trench, to the northeast of the lander. Scientists plan next to have Phoenix collect and analyze surface soil from a third trench near the second one, and later to mechanically probe and sample the hard layer.

"We have in our ice-attack arsenal backhoeing, scraping and rasping, and we'll try all of these," said Ray Arvidson of Washington University in St. Louis, lead scientist for Phoenix's Robotic Arm.

Phoenix Project Manager Barry Goldstein of NASA's Jet Propulsion Laboratory, Pasadena, reported that an issue reported earlier this week related to producing thousands of duplicate copies of some file-maintenance data files has been diagnosed, and a corrective software patch will be sent to Phoenix within a few days. Science operations continue in the meantime, though all data collected must be relayed to Earth on the same Martian day it is collected, instead of being stored to non-volatile memory when Phoenix powers down to conserve energy during the Martian night.

Images sent back Friday morning from Mars showed that the doors to the Number 5 oven on the Thermal and Evolved-Gas Analyzer opened part way. The instrument team is working to understand the consequences of this action.

The Phoenix mission is led by Peter Smith at the University of Arizona with project management at JPL and development partnership at Lockheed Martin, Denver. International contributions come from the Canadian Space Agency; the University of Neuchatel, Switzerland; the universities of Copenhagen and Aarhus, Denmark; Max Planck Institute, Germany; and the Finnish Meteorological Institute. For more about Phoenix, visit: http://www.nasa.gov/phoenix and http://phoenix.lpl.arizona.edu.

Media contacts: Guy Webster 818-354-6278
Jet Propulsion Laboratory, Pasadena, Calif.
guy.webster@jpl.nasa.gov

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
dwayne.c.brown@nasa.gov

Sara Hammond 520-626-1974
University of Arizona, Tucson
shammond@lpl.arizona.edu


Source: NASA - Phoenix - News
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