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Phoenix is dead...long live Phoenix!

Posted by Emily Lakdawalla

2010/06/02 03:11 CDT

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The latest HiRISE images of the Phoenix polar lander, taken near Mars' northern summer solstice, show why we haven't heard from the spacecraft since it fell silent on November 2, 2008: it appears the solar panels have collapsed. No solar panels means no power; Phoenix is now silent forever.

In a previous post, I showed views of the Phoenix landing site taken during the active mission and also right after the mission ended; in addition, I showed two pictures taken just as spring's first sunlight was arriving at the landing site. Those pictures were very difficult to interpret because of the extremely low angle of the sunlight. Now I have two more pictures to add, taken as spring was giving way to summer; with better lighting, the changes that have come to the landing site are obvious and surprising. To give away the punch line, I'll quote Peter Smith from this week's Planetary Radio interview with Mat Kaplan: the spacecraft parts "are now turned into a Martian red. Mars is taking back the spacecraft."

As a reminder, here's the view from sol 55 of the mission, when Phoenix was still active:

NASA / JPL / UA / annotations by Emily Lakdawalla

Phoenix landing site monitoring from HiRISE: July 20, 2008 (Phoenix sol 55)

Image scale is 25 cm/pixel. North is to the left. Source page

Seen at low resolution, the most obvious features of the lander are the brilliant white parachute and the dark splat of the heat shield, as well as a subtler dark spray left behind by the retrorockets on the lander and backshell. Now look at the same area in January of this year, before the seasonal carbon dioxide frost had completely sublimated away:

NASA / JPL / UA / annotations by Emily Lakdawalla

Phoenix landing site monitoring from HiRISE: January 6, 2010

Image scale is 25 cm/pixel. North is to the left. As spring comes to Mars, the area is illuminated by a Sun that is a reasonable 30 degrees above the horizon; still, not all of the seasonal carbon dioxide frost has yet sublimated. It is especially concentrated in the topographic lows between the polygonal patterns in the polar soil. Source page

I was only able to locate the spacecraft in this view using the distinctive pattern of the large east-west trough located just to the north of the lander -- that is, I had to know where it was in order to find it. Now look at the same site on May 7, just before the summer solstice:

NASA / JPL / UA / annotations by Emily Lakdawalla

Phoenix landing site monitoring from HiRISE: May 7, 2010

Image scale is 25 cm/pixel. North is to the left. Just before the summer solstice, the Sun is 40 degrees above the horizon. The dark bounce mark and bright parachute that originally made the landing site easy to spot have apparently vanished. Now the best way to recognize the landing site is from the dark shadows thrown by the lander and backshell. Source page

The change from last Mars year is really quite shocking. The parachute and dark backshell splat seem to be totally gone. Now, the most distinctive things about the site seen at low resolution are the shadows thrown by the spacecraft and backshell. While they are not hard to see against the background plains, they are much smaller than the parachute and heat shield splat were, so it was much harder to spot the landing site location at low resolution.

Let's compare the two images taken a Mars year apart at much higher resolution.

NASA / JPL / UA / Emily Lakdawalla

Phoenix lander before and after a Martian winter

Two images of the Phoenix lander taken by the HiRISE camera on Mars Reconnaissance Orbiter on July 20, 2008 (top) and May 7, 2010 (bottom) document the damage done to the lander by the intervening Martian polar winter. The images are enlarged by a factor of three. The two most obvious differences are a lack of bright reflection from the metal surfaces of the lander's main body -- which suggest that it is covered with dust -- and the disappearance of the solar panels and their accompanying shadows -- which suggest that the panels collapsed over the winter.

Wow. That's a sobering view. Asked during the radio interview how he felt about seeing what Mars has done to his spacecraft, Peter told Mat "It doesn't feel good at all." Poor Phoenix!

The changes to the heat shield, backshell, and parachute are just as stark. The lesson that Mars enthusiasts should take away from this comparison is that it will be exceedingly difficult indeed to locate the missing Mars Polar Lander, even with the incredible eyesight of HiRISE. Even if Mars Polar Lander's entry, descent, and landing worked almost flawlessly, leaving it fairly intact on the surface with a heat shield, backshell, and parachute nearby, the intervening Martian polar winters may well have acted quickly to hide the spacecraft and its associated hardware from view.

NASA / JPL / UA / Emily Lakdawalla

Phoenix heat shield before and after a Martian winter

Two images of the Phoenix heat shield taken by the HiRISE camera on Mars Reconnaissance Orbiter on July 20, 2008 (top) and May 7, 2010 (bottom) show how rapidly the Martian polar environment acts to hide human artifacts sent there. When Phoenix approached for landing, this round heat shield protected the spacecraft during its fiery entry into the Martian atmosphere. Shortly before landing, Phoenix ejected the heat shield, which fell to the ground a short distance away from the lander. When it bounced, it deposited a splash of sooty material, flipped, and landed with its sooty side up, making a distinctive dark circle on the ground. Following the Martian winter, the dark bounce mark is invisible -- probably covered with a layer of dust -- and the heat shield itself is only barely discernible from the surrounding terrain.

NASA / JPL / UA / Emily Lakdawalla

Phoenix backshell and parachute before and after a Martian winter

Two images of the Phoenix bakcshell and parachute taken by the HiRISE camera on Mars Reconnaissance Orbiter on July 20, 2008 (top) and May 7, 2010 (bottom) make it clear that searching for the missing Mars Polar Lander will be exceedingly difficult. Shortly after Phoenix' landing, the bright parachute was the easiest thing to spot in a low-resolution view of the landing area; its brilliantly reflective whiteness saturated the HiRISE camera detector. A year later, the parachute has apparently vanished; no sign of it remains. It is most likely still there, but the thin material has conformed to the shape of the soil below it, and it has been coated with dust, camouflaging it into the surroundings. The backshell also appears less bright because it is coated with dust, but its shadow has not changed, indicating that the backshell has survived the winter more or less unchanged from its condition and position when it landed.

I sent emails to Peter as well as to Mark Lemmon (head of the camera team) expressing my surprise at the rapidity of the changes, and both of them replied. Peter wrote:

The rate of change surprised me also. I would have thought that one year would bring a dusting to the exposed surfaces -- look at the rovers for instance. But to have the solar panels become essentially invisible against the background and the parachute to disappear is a big departure from a slight dusting. One imagines the parachute fluffed by winds and dust devils with some surfaces peeking through the dust mantle. You are right, it has completely returned to Martian red. This leaves little hope for finding MPL [Mars Polar Lander] in the southern polar region.

Mark wrote the following -- if you don't recall what "tau" means, here's an explainer:

I'm a little surprised I cannot make something out even as a texture change. A tau=4.4 dust storm in there would collapse to about a 6 micron thick layer of dust, give or take, and be almost as hard to see through. Remember that one of the most predictable types of dust storms on Mars is the receding-cap storm. As that CO₂ goes away, a lot of dust is kicked up locally, and settles back down without going very far.
I'm curious if [the parachute] rotated around the backshell downwind, and maybe a purely textural feature could be found. However, the dust coating is most plausible if it has been immobilized, as it seemed to be during the mission.

So the Phoenix spacecraft really has sent its last data to Earth. But that doesn't mean that Phoenix has finished teaching us about Mars; far from it. Peer-reviewed science results are only beginning to be published from the mission. The things that Phoenix' instruments uncovered -- like the perchlorate salts just below the surface -- are stimulating research into the possibility for Martian life. And Phoenix' experiences -- both the successes and the challenges -- are informing the development of the next Mars mission, the Curiosity rover. Phoenix was the first of the new, low-cost "Scout" line of Mars missions, and it did its job, exploring a previously unexplored landscape, using previously untried methods (untried, at least, on Mars), succeeding at many things, failing at a few, developing valuable lessons to help us move forward in our exploration of the most Earthlike of alien worlds.

Meanwhile, Mars will continue to take back the cold, still piles of metal and glass that is all that remains of the Phoenix spacecraft. One thing that is still there, though probably covered now with a coating of dust, is the Phoenix DVD. Peter wrote to me about that too: "One thing that will remain under the protective dust cover is our DVD of Martian literature. Someday it will be uncovered by a future team of archeologists. I wonder what they will think of us?"

NASA / JPL / UA / Texas A & M / color mosaic by James Canvin

Amateur version of the Phoenix Mission Success Panorama (the 'Peter Pan')

This is James Canvin's version of Phoenix' Mission Success Panorama, which includes 150 separate camera pointings taken from sols 13 to 43. Canvin produces his mosaics using software he developed for Mars Exploration Rover panoramas. The DVD, encoded with the names of more than 250,000 Earthlings who signed up to ride along with Phoenix to the surface of Mars, is located on the lander deck just below the scoop on the end of the robotic arm. (The robotic arm appears disembodied because the lander did not take a photo of the arm higher in the air.)

The Planetary Society's Director of Projects, Bruce Betts, reflected on the end of Phoenix this way:

by Bruce Betts

On the Phoenix spacecraft, a message to the future sits waiting on Mars. Now is a good time to remember that, as NASA has ended operations on the Phoenix mission due to their inability to contact it, and now HiRISE images show likely damage due to winter carbon dioxide ice accumulation.

NASA / JPL / U. Arizona

Visions of Mars, on Mars

This image shows the DVD provided by The Planetary Society to the Phoenix mission, which contains 250,000 names of people who signed up to send their names to Mars. It also contains "Visions of Mars," messages to future Martian explorers, science fiction stories and art inspired by the Red Planet. The DVD is mounted on the deck of the lander, which sits about one meter above the Martian surface, visible in the background.

We congratulate the Phoenix team for a hugely successful mission that lasted longer than designed, and returned engineering triumphs and science discoveries. As part of our Messages from Earth program, The Planetary Society provided the Phoenix mission with a silica glass mini-DVD that was attached to the deck of the spacecraft. On that mini-DVD are a quarter million names of those who wanted to send their names to the surface of Mars including all Planetary Society members (if you haven't already, you can print your certificate here). Also, on board is Visions of Mars: the first library on Mars. It includes science fiction and science writing about Mars, Mars art, radio shows including War of the Worlds, and audio-visual greetings from Carl Sagan, Arthur C. Clarke, Louis Friedman, and Judith Merrill, as well as a greeting from Phoenix Principal Investigator Peter Smith.

The Planetary Society

Phoenix DVD

This mini-DVD made of silica glass now sits on Mars as part of the Phoenix spacecraft.

The DVD's greetings and historical documents are a time capsule, waiting for future explorers to find and decode it. When they do so, they will look back into the past, seeing, hearing, and reading the impressions their ancestors had of Mars. Thanks to the silica mini-DVD technology, provided by Plasmon OMS, the archive should last at least hundreds of years. Even as carbon dioxide ice seems to be collapsing solar panels on the spacecraft, our message to the future sits safely waiting for the future. Thank you, Phoenix!

NASA / JPL / UA / Texas A & M

The Phoenix DVD gets even dirtier

During the mission, Mars reached out and touched our DVD when the robotic scoop dropped Mars dirt onto the DVD. On sol 28 (June 22, 2008), Phoenix used the scoop on its robotic arm to deliver a sample of soil from the Snow White / Rose Red trench to the first of its four wet chemistry laboratory cells. In so doing it spilled more dirt on the lander deck, including on top of the Phoenix DVD.

ere is a roundup of The Planetary Society's coverage of some of the exciting events from this mission. There is also an extensive section about Phoenix, including a sol-by-sol summary of its operational activities.

January 25, 2007, feature story:A Green Valley for Phoenix
uly 12, 2007, feature story:Phoenix Prepares for August Launch to Mars' Northern Plains
ugust 4, 2007, feature story:Phoenix Launches to Mars
ugust 5, 2007, blog: Phoenix launch wrapup
eptember 7, 2007, blog: Phoenix returns its first photo
ovember 15, 2007, blog: No descent images or sounds from Phoenix
ay 13, 2008, blog: Landing ellipses
ay 24, 2008, blog: Inspired by Phoenix: "Arrival," by Stuart Atkinson
ay 25, 2008, blog: Have some courage, NASA!
ay 25, 2008, blog: Entry, Descent, and Landing events...
ay 25, 2008, blog: First images from Phoenix! - Solar Panel Deployed - Footpads - Color
ay 25, 2008, blog: Phoenix: last press briefing of the day after the successful landing
ay 25, 2008, feature story:Phoenix Lands Flawlessly on Mars and Sends Home First Postcards
ay 26, 2008, blog: OMG!! Parachute!!!! Photo!!!!!
ay 26, 2008, blog: Visions of Mars, on Mars
ay 27, 2008, blog: The HiRISE parachute image just got even better
ay 27, 2008, blog: HiRISE images of the Phoenix landing site
ay 28, 2008, blog: A full panorama and an unstowed arm
une 1, 2008, feature story:Holy Cow, Snow Queen! Phoenix Landed on Ice, Team Thinks
une 21, 2008, feature story:Phoenix Scientists Confirm Water-Ice on Mars
une 26, 2008, blog: Phoenix sol 30 update: Alkaline soil, not very salty, "nothing extreme" about it!
une 27, 2008, blog: Strange things under Phoenix
uly 10, 2008, blog: More things to see in the amazing HiRISE image of Phoenix' descent
uly 17, 2008, blog: Danes on Mars
uly 23, 2008, blog: How are we coming on Phoenix mission success?
uly 31, 2008, blog: Highlights of the Phoenix sol 64 press conference
ugust 3, 2008, blog: Apparently there's something more exciting yet to be announced by Phoenix
ugust 4, 2008, blog: The Phoenix flap
ugust 6, 2008, feature story:Alien Rumors Quelled as NASA Announces Phoenix Perchlorate Discovery
ugust 6, 2008, blog: Phoenix perchlorate kerfuffle
ugust 15, 2008, blog: First image of a speck of Mars dust from the Atomic Force Microscope
eptember 29, 2008, blog: Phoenix Update, Sol 123: Press briefing with carbonates, clays, and snow!
eptember 30, 2008, feature story:Phoenix Detects Falling Snow, Digs Up Evidence for Past Water, and Snares Mission Extension
ctober 28, 2008, blog: The beginning of the end for Phoenix: No more robotic arm operations
ctober 30, 2008, feature story:Phoenix Enters Safe Mode
ctober 31, 2008, blog: A brief Phoenix update
ovember 4, 2008, blog: Phoenix update: Not dead yet; still in "Lazarus mode;" one attempt at microphone use did not work
ovember 11, 2008, feature story:Sun Sets on Phoenix, NASA Declares End of Mission
ovember 11, 2008, blog: The end of Phoenix
ecember 11, 2008, blog: Some interesting information in a Nature story about Phoenix
ecember 15, 2008, blog: AGU: Some first impressions from today's Phoenix sessions
ecember 19, 2008, blog: AGU: Wrapping up my notes on Phoenix
arch 23, 2009, blog: LPSC, Day 1: Phoenix, morning session
arch 25, 2009, blog: LPSC: Saltwater at the Phoenix landing site?
ctober 28, 2009, blog: HiRISE sees Phoenix in the Martian spring
anuary 11, 2009, blog: Odyssey's going to start listening for Phoenix
arch 2, 2010, blog: LPSC, Day 1: Spirit and Phoenix
pril 13, 2010, blog: No signal from Phoenix