More incredible imagery from Mars. This time it is a nice detail image of Ius Chasma, an area within Valles Marineris which is believed to be the largest canyon in the solar system. This recently released image by NASA was snapped by the Mars Reconnaissance Orbiter, one of the many robotic explorers working for us on Mars right now, and shows in pretty stunning detail the stratigraphic layers believed to have been created by both wind and water. I am in awe of the detail of this image and with the frequency and quality of images available to us from Mars. Nice work NASA, the ESA, and all of your partners for all of the Mars missions. I’m a fan.
Definitely a highlight of my rather long day today was seeing these images taken by the ESA’s Mars Express robotic probe. The images depict the Echus Chasma series of canyons mentioned in the title, and I find them absolutely stunning. Planetary geologists believe that these chasms were formed by flowing ground water, and that they were carved over thousands of years. More images:
I absolutely geek out seeing the surface of Mars in such incredible detail. Our base of knowledge for Mars is growing rapidly, and it seems that with the Phoenix Mars Explorer, Mars Surveyor, and ESA’s Mars Express we have a trifecta of data and images streaming to us from the red planet.
The Phoenix Mars mission team released some incredible news on June 20th. The Phoenix Mars explorer, since landing on Mars on May 25th, had definitively established that the white material exposed with its digging tool earlier is in fact frozen water. Phoenix had found water ice just below the Martian regolith. That was a significant part of the mission, and to accomplish it so quickly and efficiently is a big win for NASA, JPL, and the whole mission team. The proof is represented in the image above. If you watch the image you see the white material begin to shrink and disappear. That is called sublimination, which is the transition of an element or compound from solid to gas without the intermediary liquid step. Given the atmospheric conditions on Mars, you are seeing evidence above of the frozen water on mars subliming.
Identifying water ice was the first important step in the mission team’s “follow-the-water” mission framework. Knowing that they are working with water ice now triggers a series of analyses that will help identify the mineral components and chemicals in that water ice, and also look for any organic materials. This investigation will help determine if the conditions just below the Martian surface are conducive to microbial life, and if that life exists or has existed on Mars.
This image is the result of the Mars Phoenix mission team instructing the robotic arm camera to look under the vehicle. What you are looking at is the surface of Mars, and it shows that the Martian soil has been displaced by the landing thrusters on Phoenix to expose what is most probably ice. The simple action of Phoenix landing on Mars has potentially exposed polar ice directly under the vehicle, ice that was covered by a very loose and thin layer of soil.
There is a rumor that when the mission leaders saw this image the first words uttered were “Holy cow!”
The Phoenix robotic explorer has been on Mars now for about 27 hours after an incredibly successful entry, descent and landing. It has been very busy. Incredible images are already streaming to Earth, and those of us geeked out by things of this nature are absolutely riveted. I was excited to discover how many people I know were following @MarsPhoenix on Twitter.
Many images are coming back, and most right now are of the explorer itself and the immediate vicinity as the mission managers check systems and get their bearings. The above image of one of the craft’s landing pads is one of my favorites because that image is of the pad of a man-made robotic explorer sitting on the surface of Mars millions of miles away from Earth, and it was taken in the last 24 hours. Astounding. Even more astounding is this video composite of the Martian surface, terrain and horizon taken by Phoenix today.
We are at just under four hours before Phoenix lands on the surface of Mars. I am checking periodically at the Phoenix mission control website in anticipation of this event. Martian weather is clear and the landing later today is green for go. I suspect there are a lot of very excited and anxious people at JPL right now.
The above animation is of weather on Mars around its north pole from 5/16 through 5/22. The small cigar shaped outline in the upper left quadrant is the planned landing zone.
It’s not just a big day for race fans, its a big day for science and space enthusiasts. In August of last year the Mars Phoenix Explorer left Earth to start its journey to Mars. Its mission is to arrive safely, land on the Martian North Pole, and dig into the soil there begin looking for the building blocks of life. It arrives today at around 4:45PM PDT. Arriving is the hardest part, as now the explorer has to successfully enter the Martian atmosphere (at 12,000mph) using parachutes to slow the rapid descent from 900mph to 250mph, and then fire landing rockets to prevent it from slamming into the Martian surface (see the video above). Its a complex landing, and the mission control team probably hasn’t been sleeping much these last few days, as the last five years of their work culminates today in about seven minutes of anxiety. That’s okay, though, as they have a number of ways they can distract themselves while keeping us updated on the the mission’s progress. For instance, you can follow the Phoenix mission on Twitter and get frequent updates and mission facts. The mission team also has a blog that is full of information and that will be used to post what the mission team is thinking and what Phoenix sees and discovers, as well as an information rich mission website.
So, the entire Phoenix mission is going to be captured for us via an array of online tools. This is incredibly exciting, and it serves to connect us to the exploration and science that NASA leads in a way that is not only meaningful, but also basically real time.
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