Will Mars Astronauts be put in Suspended Animation for the Journey?

Sigourney Weaver in the film Alien (Brandywine Productions Ltd.)

Could you handle six months in space with a tiny handful of crew? Keep in mind you’d be doing everything with them, eating, sleeping, chatting, working, waiting, more sleeping, the occasional emergency, more chatting… If you look around your office now, could you really see yourself spending 24/7 with any of those guys for 24 weeks? Even the happiest, close-knit family would find it hard, especially at the close quarters they are likely to endure. Even if you had to spend that time with your partner, someone you love dearly, there would be stresses… after all you can’t exactly storm out of the spaceship and float home. You’re in it for the long-term.

The solution? Put the astronauts on their way to Mars into a suspended animation state. This not only saves the astronauts from potentially dangerous arguments, it would also save on food, air and water. So how can this be done? Hydrogen sulfide, the gas produced by rotten eggs, may be able to help…

Peggy Whitson, NASA astronaut, spent a record breaking six months on board the International Space Station (she returned on April 19th with a bit of a bump) and it appears she was able to make it through the days on board the ISS with her crew. However, the ISS had a very busy few months, plus it’s had several changes of crew and various new modules have been added. The ISS is a very different environment to work in than on board future missions to Mars. For starters, the main mission is to get to the Red Planet; the transit from Earth will be seen as the “run-up”. Although valuable science will undoubtedly be done, the accommodations are likely to be cramped and Mars astronauts will see the same faces day in and day out. Confrontations could become a serious problem. Supplying the ship with enough food and water for the trip will also be a difficult task. How can all these issues be faced? Put the astronauts in suspended animation.

Probably more familiar in science fiction movies (like the 1979 classic Alien, pictured top), suspended animation has some serious problems. Cooling the human body was thought to be the key to slowing the metabolism down sufficiently so space-bound crews could slip into hibernation for the duration of the long trip, but it seems this interferes with the rhythm of the heart. Now scientists at Harvard believe they have a solution.

Dr Warren Zapol, the head of anaesthesiology at Harvard University’s Massachusetts General Hospital, has been working on the effects that hydrogen sulfide has on the human body. More commonly known for the pungent smell produced by rotten eggs, hydrogen sulphide has been used on mice and the results have been very interesting. When breathed in, the gas slows mouse metabolism, but does not reduce the flow of blood to the brain and doesn’t interfere with the heart.

The mice aren’t asleep. If you pinch their tails they respond. I don’t know what it’s like. Probably some slow-motion world.” – Dr Warren Zapol.

After about ten minutes of inhaling the gas, the mice slipped into a hibernation state. A reduction in oxygen consumption and carbon dioxide production was measured. This reduction continued for as long as hydrogen sulfide was administered and the test subjects recovered fully after normal air flow was supplied for 30 minutes. What’s more, oxygen levels in the blood did not vary, signifying that the major organs were not at risk of being oxygen starved. Mouse heart rate also dropped by 50%.

Of course many tests will be needed before hydrogen sulfide is administered to humans, let alone astronauts, but the preliminary results are encouraging. It looks like mice are joining the monkeys in mankind’s future on Mars…

Source:
ABC Science

Searching for Water and Minerals on Mars – Implications for Colonization

A Vastitas Borealis crater plus ice in the north polar region - reconstructed image by HRSC (ESA)

New results from the The Compact Reconnaissance Imaging Spectrometer for Mars (CRISM) on board the Mars Reconnaissance Orbiter (MRO) reveal the mineral composition of the bottom of Chandor Chasma. There is a rich mix of sulfate and pyroxene-containing deposits in this region and the CRISM instrument continues to find deposits of minerals never thought to exist on the planet’s surface. However, the primary mission objective is to find evidence of water, past and present, aiding the hunt for the best location of the first Mars settlements. SETI Institute principal investigator and CRISM scientist Dr Adrian Brown answers some of my questions about CRISM and how the results may be useful for future manned missions to the Red Planet…

Part of my duties as Communications Officer with the Mars Foundation (a non-profit organization for Mars settlement designers) is to contact and interview key mission scientists working on missions that could be useful for getting us closer to realising the first manned settlement on the Red Planet. Dr Adrian Brown is one such scientist; the CRISM instrument is one such mission. CRISM, an advanced spectrometer, has been looking out for the mineral fingerprint of water since 2006. Minerals will have dissolved in ancient liquid water, so looking for the dry remnants of these minerals today will help to reveal the surface conditions of the past. Another mission objective is to characterize present water on Mars, seeing how surface water ice forms and how it varies with the seasons. Dr Brown’s current project is to map the seasonal variations of water ice in the Martian southern polar region.

Sulfate- and pyroxene-containing deposits in the Candor Chasma region of Mars (NASA/JPL/JHUAPL/ASU)

In a timely news release, the CRISM mission site has announced new results to come from the analysis of the mineral distribution at the bottom of Candor Chasma (pictured), part of the vast Valles Marineris. Candor Chasma is a deep, long and steep-sided valley about 813 km (505 miles) long and has been cited as a possible location for the Hillside Settlement concept as conceived by the Mars Foundation. In fact, this settlement concept was the inspiration behind the first permanent settlement aptly called “Underhill” in Kim Stanley Robinson’s epic novel Red Mars. So, there is obvious interest as to what Candor Chasma can offer the colonists inhabiting the Hillside Settlement with easy access to locally mined minerals.

The CRISM instrument has discovered quantities of sulfate and pyroxene rich deposits in the region, useful for many industrial processes. In our interview, Dr Brown outlined other important minerals that CRISM has found and some of their common uses here on Earth:

These [minerals] include kaolinite (chinaware is made of this mineral), talc (the main constituent of many soaps) and hydrated silica (perhaps like chert, which Indian knives were carved out from). The small amounts of these minerals means it has been impossible to discover them before CRISM, and previously they were discounted in all our modelling of Mars.” – Dr Adrian Brown, SETI Institute principal investigator and CRISM scientist.

For me, the most revealing part of our conversation was Brown’s estimate on the sheer quantity of water held as ice in the north polar cap. The north pole hides under a 1000 km (620 mile) diameter disk of near-pure water ice (with some impurities like sand and dust, giving a pink hue). This disk is 3 km (1.9 miles) high, holding staggering 2.35 million cubic kilometers of water. That’s enough water to cover the continental US to a depth of 200 meters! Throw in the water that is held at the south pole (a carbon dioxide/water ice disk 300 km in diameter and 2 km high) and we’re looking at the equivalent volume of water ice held in the Greenland ice sheet (or 500 times less than the amount of water in our oceans). It’s not that hard to imagine that if a permanent Mars colony is established, mining operations for water ice would be common.

Turning on the Tap - Commissioned artwork - Colonist tapping into a sub-surface aquifer (©Mars Foundation)

But it doesn’t stop there; water could also be extracted from the atmosphere. One of Dr Brown’s studies focus on measuring the variation of water ice crystals in the clouds throughout the seasons. There should also be quantities of water vapour in the warmer equatorial regions.

There is also the possibility of extracting water from the permafrost layers below the Martian regolith. The Phoenix Mars lander (set to arrive at the Red Planet on May 25th) will be able to investigate the possibility of sources of frozen water below the surface. Dr Brown also indicated that the observations by the Mars Orbital Camera (on board NASA’s Mars Global Surveyor, lost in November 2006) of apparent gullies may reveal the location of possible sub-surface aquifers (after gushing across the surface) for future colonists to “tap” into (pictured). However, there have been studies that dispute this in favour of dry debris flows creating the gullies, but a definitive answer will not be arrived at until the gullies are analysed in-situ. And if he had the chance, I think Dr Brown would be the first to look into this exciting possibility after I asked him the question: Would you like to go to Mars?

Of course I would love to travel to Mars, most of all to go to the polar regions and observe them with my own eyes. If I could actually go to the surface of Mars to investigate the fascinating geology of Nili Fossae and Valles Marineris, that would be so awesome. And to visit a gully site and dig behind it to try and find its source… and to witness the cold volcanoes of mud that erupt in the polar cryptic region during springtime… to go and understand these things that have us puzzled at the moment would be so amazing… and of course more questions would be raised, more geological problems unearthed, and the cycle of understanding the Red Planet would continue.” – Dr Adrian Brown

I share his enthusiasm and look forward to more discoveries by CRISM.

For more on Dr Adrian Brown’s work, check out his website: http://abrown.seti.org/

Sources: The Mars Foundation, CRISM

Spirit’s Dust Dilemma

Steve Squyres and the Mars Exploration Rover team knew from the beginning that dust could cause a problem for the rovers, Spirit and Opportunity. When a thick layer of dust coats the solar panels, it blocks the sunlight that generates power for the six-wheeled robots. In the summer of 2007 a huge dust storm blanketed Mars, and deposited a fair amount of dust on solar panels of both rovers. Spirit, especially accumulated a lot of dust on its solar array. Currently, only about one-third of incoming sunlight is able to penetrate dust on Spirit’s solar panels to be converted to electricity. As a result, Spirit is experiencing the lowest energy levels to date and accumulating a backlog of data waiting to be transmitted to Earth. If only a dust devil would come along!

Spirit’s solar array input has been approximately 240 watt-hours per Martian day, or sol (100 watt-hours is the amount of energy needed to light a 100-watt bulb for one hour). The skies in the area are now clear, which means additional dust shouldn’t be accumulating on the solar panels, and sunlight should be abundant. But clear skies also mean lower temperatures on the surface of Mars, increasing the bitter cold experienced by Spirit’s rover electronics module during the current Mars winter. Nighttime temperatures are creeping closer to the point where they will trigger the survival heaters, which draw a large amount of power.

The rover team has been using the strategy of keeping Spirit awake long enough each day to keep the electronics module sufficiently warm with heat from normal operations, providing more time for science observations. However, recently the team has done less science operations in order to allow Spirit’s batteries to recharge. The engineers are being creative in the trade-offs the team makes each day to keep Spirit going through the Martian winter. Another way they are conserving energy is by restricting the number of sols on which Spirit receives direct-from-Earth instructions via the rover’s high-gain antenna and transmits data to Earth via the Odyssey orbiter.

The MER team is hoping for a dust devil event to come and clear off the solar panels, like these dust devils did back in 2005.

This image shows the difference in the dust accumulation before and after the dust-cleaning event back in 2005.

And this is a self-portrait the rover took of its cleaned solar panels in 2005. Here’s hoping Spirit can be wiped clean again, and the sooner the better.

Original News Source: Mars Rover website

Mars Was Recently Blanketed By Glaciers

Mars is a dead world, unchanging for billions of years. Right? Maybe not. Researchers from Brown University have found evidence for thick, recurring glaciers on the surface of Mars. This means that the climate on Mars might be much more dynamic than previously believed. Perhaps the climate could change again. And liquid water underneath these glaciers might have given life a refuge over the eons.

Around 3.5 billion years ago, Mars was a completely different world, with liquid water right there on its surface. And then something happened that made it cold, dry, and quiet – too quiet. Apart from the occasional meteorite impact, planetary geologists thought that very little has happened on Mars since then.

In an article published in the journal Geology, scientists from Brown University released images showing how dynamic Mars might be. They found evidence that thick ice packs, at least 1 km (0.6 miles) thick and maybe 2.5 km (1.6 miles) thick coated Mars’ mid-latitude regions.

These ice sheets weren’t there last year, but they were there 100 million years ago, and maybe localized glaciers were flowing as recently as 10 million years ago. That’s yesterday, geologically speaking.

With activity this recent on Mars, that could mean that its climate might change often, and it could happen again. Maybe Mars wasn’t so dead for the last 3.5 billion years.

The images captured by NASA’s Mars Reconnaissance Orbiter showed a box canyon in a low-lying plain. The canyon clearly has moraines – deposits of rock that mark the end of the glacier, or the path of its retreat.

This discovery increases the possibility of life on the surface of Mars. At the bottom of the glaciers, crushed under kilometres of ice, liquid water would have formed into vast reservoirs. These could have served as sanctuaries for life.

Original Source: Brown University News Release

Opportunity’s Robotic Arm Stalls

NASA engineers say Opportunity’s robotic arm, which has been intermittently problematic since 2005, has worsened recently. A small motor in the shoulder joint of the Mars Exploration Rover’s arm stalled on April 14, and engineers are diagnosing the problem and assessing whether the motor can possibly be used again. They are also trying to determine the impact on Opportunity’s work if the motor were no longer usable.

The motor is one of five in the robotic arm and it controls sideways motion of the shoulder joint. The stall last week occurred after being used briefly, and after much less motion than earlier stalls. Engineers believe the problem is electrical rather than mechanical, and additional tests are being performed to determine whether the is trouble is intermittent or a permanent failure.

The arm is used to place a microscopic imager and spectrometer in contact with rocks and soils to study their composition and texture.

“Even under the worst-case scenario for this motor, Opportunity still has the capability to do some contact science with the arm,” said JPL’s John Callas, project manager for the twin rovers Opportunity and Spirit. “The vehicle has quite a bit of versatility to continue the high-priority investigations in Victoria Crater and back out on the Meridiani plains after exiting the crater.”

The two Mars rovers, Opportunity and Spirit, have been studying the Red Planet since January 2004, and each have shown some signs of aging.

When Opportunity’s shoulder motor began stalling occasionally in November 2005, engineers increased the voltage to the motor, and that allowed the motor to still be operational. Additionally, the engineering changed the standard procedure by unstowing the arm at the end of each day’s drive rather than leaving it stowed overnight. This keeps the arm available for use even if the motor then stops working.

This spring, Opportunity began crossing an inner slope of Victoria Crater to reach the base of a cliff portion of the crater rim, a promontory called “Cape Verde.” On April 14, Opportunity was backing out of a sandy patch encountered on the path toward Cape Verde from the area where the rover descended into the crater. As usual, the commands included unstowing the arm at the end of the day’s short drive. The shoulder motor barely got the arm unstowed before stalling.

“We’ll hold off backing out of the sand until after we’ve completed the diagnostic tests on the motor,” Callas said. “The rover is stable and safe in its current situation, and not under any urgency. So we will take the time to act cautiously.”

Original News Source: JPL Press Release

Mars Express: Looking Beneath Mars’ Surface

MARSIS
MARSIS fully deployed orbiting Mars. Image credit: ESA

To truly know and understand another world, planetary scientists need to look beneath the surface of that planet. This has been done on a small scale by looking inside impact craters, a la Opportunity and Spirit on Mars. But that only provides information for one area on a big planet. To get the global picture of the subsurface, a radar sounder instrument was developed for ESA’s Mars Express spacecraft. The Mars Advanced Radar for Subsurface and Ionosphere Sounding (MARSIS) experiment has now been successfully used for the first time to look beneath Mars’ south polar ice cap, opening up the third dimension for planetary exploration. “We have demonstrated that the polar caps at Mars are mostly water ice, and produced an inventory so now we know exactly how much water there is,” says Roberto Orosei, MARSIS Deputy Principal Investigator.

The data from MARSIS’ probe of the ice cap is still being analyzed, but scientists say they expect some surprising results to be revealed.

MARSIS is built to map the distribution of liquid and solid water in the upper portions of the Martian crust, and can investigate Mars’ subsurface up to a depth of 5 km. If reservoirs of water are detected, it will help us understand the hydrological, geological, climatic and possibly biological evolution of Mars. “At the south pole of Mars, we are seeing through ice 3.7 km thick. A small calculation shows that we could see through ice down to 20 km or more thick at Mars,” says Ali Safaeinili, MARSIS co-investigator.

No one had ever used a radar sounder from orbit on another planet before. So the team was uncertain it would work as planned. The subsurface of the planet might have been too opaque to the radar waves or the upper levels of Mars’ atmosphere (ionosphere) might have distorted the signal too much to be useful.

But, the instrument worked perfectly.

Every time a radar wave crosses a boundary between different substances, it generates an echo that the orbiter detects.

See ESA’s 3-D simulation of the radar instrument.

While MARSIS is still collecting data, a follow-up instrument is already operating at Mars. The Shallow Subsurface Radar (SHARAD) on NASA’s Mars Reconnaissance Orbiter works at higher frequencies than MARSIS and can see more details in the signals it receives from the underground layers, but it can’t penetrate the surface quite as far.

The technique’s success is prompting scientists to think of all the other places in the Solar System where they would like to use radar sounders. One obvious target is Jupiter’s icy moon, Europa. There, a radar sounder could probe the moon’s icy crust to help understand the puzzling features we see on the surface. It may even see the interface at the bottom of the ice where an ocean is expected to begin.

Asteroids and comets could be thoroughly scanned by a radar sounder, producing three-dimensional maps of their interior– perhaps exactly the data we will need if, one day, we have to nudge one out of Earth’s way. Also, this type of radar instrument could be used on our own planet to look inside Earth’s polar caps and ice sheets to determine their stability.

Mars Express has been orbiting the Red Planet since December 2003. It carries seven scientific experiments, including MARSIS, which was built by the Italian Space Agency with cooperation from JPL and the University of Iowa.

Original News Source: ESA press release

Russia to Send Monkeys to Mars

Bion, trying out an orbital module, was one of the first into space, in December 1983. (BBC)

Russia has a long history of scientific discovery and space exploration through the use of animals. Beginning with space dog Laika in 1957, the space program expanded to run tests on other dogs (many returned safely to Earth) and eventually monkeys. Although the monkey testing program was stopped through lack of funding in the mid-1990’s, the nation has announced plans to send the closest relation to humans to a place where no man has gone before: Mars. And here’s us thinking it will be a human first stepping onto the Martian surface…

I must admit, I had to read the story twice before I believed it. Russia wants to send monkeys not only into space, but to Mars. I had an idea that monkeys (or more specifically macaques) were used in space missions in the past, but in my mind this was in the past and would be considered cruel in this day and age. But hold on, aren’t macaques used in medical experiments the world over anyway? Why is it so shocking that macaques should be chosen to pioneer interplanetary travel before mankind?

These questions are emotive (and controversial) and will cause much debate internationally. Many will believe that the experimental testing on animals in the ultra-modern world of space travel will seem barbaric, but there are some serious problems we might definitively answer through the use of macaque space travel. First and foremost, due to the interplanetary radiation we expect to be bathed in during a transit to Mars, by studying a macaque’s physiology during the long journey we may be able to learn how the human body will react to larger than normal doses. The fact remains, monkeys are genetically close to humans, its little wonder that we turn to them for answers.

To this end, monkeys at the Sochi Institute of Medical Primatology, at Vesyoloye near the Black Sea, have begun the selection process for the ultimate medical animal testing experiment. The institute has a long history of involvement in the Russian and Soviet space program. Sochi was the training facility for the first monkeys into space in 1983. Abrek and Bion had a five-day trip around Earth and were returned safely in Kazakhstan and rehabilitated to live “normal lives”. Two years after this historic flight, monkeys Verny and Gordy spent seven days in space. In 1987, Dryoma and Yerosha spent a record breaking (for a monkey-assisted flight) two-weeks in space. Interestingly, Dryoma was given to Cuban leader Fidel Castro as a gift. Following this, in 1989, 1992 and 1996, three two-week flights were carried out until funding for the project ran out. Now experiments have been continued on Earth to simulate weightlessness.

Now, to revitalize Sochi’s history of macaque space flight, they are beginning a two-year program to select 40 monkeys to be sent to the Institute of Biomedical Problems in Moscow so tests can be continued into aerospace biomedicine. This will culminate in a possible primate mission to Mars.

People and monkeys have approximately identical sensitivity to small and large radiation doses, so it is better to experiment on the macaques, but not on dogs or other animals.” Boris Lapin, Institute Director.

Critics of the program are frustrated by the use of animal testing in any capacity, but remain realistic about the situation. “Humanity sacrifices more than 100 million animals a year in the name of health and beauty. It’s time to think of an alternative to experiments with animals,” says Andrei Zbarsky of the conservation group the World Wildlife Fund (WWF).

“…certainly, I feel sorry for the monkeys, they might die, but the experiments are necessary to preserve the lives of the cosmonauts who will fly to Mars in future” – Anaida Shaginyan, Institute Researcher.

This will be a controversial measure by the Russian space program and they are expecting resistance from their European partners. Although monkeys and other animals are used in medical science here on Earth, it might prove too distasteful and cruel for most, but possibly the only means to measure the physical impact on the human body after a long trip to Mars.

Source: BBC

Mars Mesas Stripped of Sand, Forming Dunes: Amazing Images from HiRISE

The mesa (left) and wind-blown sand features (right) (NASA)

There seems to be a never-ending flow of stunning images coming from the High Resolution Imaging Science Experiment (HiRISE) on board NASA’s Mars Reconnaissance Orbiter (MRO). In today’s high-resolution look at the Martian surface, large flat-topped hills (a.k.a. mesas) can be seen to be eroded by the Mars winds, stripping them of their material, creating sand dunes downwind. An incredible sight, it shows just how dynamic and powerful the Martian winds really are…

The down-wind slope of one of the eroded mesas, sand build-up obvious (NASA)

Imaged above the Hellespontus region of Mars, these fluid-like structures trailing across the surface are huge sand banks and sand dunes, built up after years of erosion from mesas upstream. The Mars winds have gradually stripped the large geological structures, allowing sand to build up as dunes in areas of calm. The curious crescent/droplet-shaped dune morphology indicates dominant winds blowing from west to east (left to right). As sand is carried from the mesa, it travels downstream. Where the winds begin to slack, possibly in large turbulent eddies; the suspended sand is dropped to allow dunes to grow.

False color close-up of two sand dunes. Wind flow from left to right (NASA)

The shapes of the Mars dunes bear a striking resemblance to barchan dunes, much like the ones found on Earth. The wind blows up the gentle slope of the dune, allowing sand to gradually build up. As the sand reaches a critical point, it collapses, forming a sharp slope on the downwind-facing side. Horn-like features are evident from above. In addition to the barchans, “seif”-like dunes are evident. Seifs are longitudinal stretches of sand parallel to wind direction. These are most obvious as they trail away from the mesas and stretch toward the clusters of barchan dunes.

See the entire region in a full-resolution projection.

The approximate size of the dunes (NASA)

These new images were captured on March 16th and resolve features to approximately 1.5 meters. At this level of resolution the small ripples in the wind blown sand can even be seen. To give an idea of scale, I’ve included a close up of one of the dunes. As annotated, the larger dunes are approximately 60 meters in length (from east to west) and around 40 meters in width.

Source: HiRISE

Amazing Image of the Martian Moon Phobos

Martian moon Phobos

I think this will easily capture the prize for the best space photo of the month. Check out this amazing picture of Mars’ moon Phobos, captured in colour (and 3D) by NASA’s Mars Reconnaissance Orbiter.

The spacecraft snapped the picture on March 23, 2008 during a flyby. It took two separate images of the moon within 10 minutes of each other, which scientists later merged together into a stereo view.

“Phobos is of great interest because it may be rich in water ice and carbon-rich materials,” said Alfred McEwen, HiRISE principal investigator at the Lunar and Planetary Laboratory at the University of Arizona, Tucson.

Previous spacecraft, like Mars Global Surveyor, have actually flown closer to Phobos, and taken higher resolution images, but according to the researchers, “the HiRISE images are higher quality, making the new data some of the best ever for Phobos.”

When MRO took the first picture, Phobos was 6,800 km (4,200 miles) away, and it was able to resolve features as small as 20 metres (65 feet) across. For the second image, the spacecraft was 5,800 km (3,600 miles) away, and could resolve features down to 15 metres (50 feet) across.

Phobos itself is only 22 km (13.5 miles) in diameter. Since it’s so small, it doesn’t have the gravity to pull itself into a sphere, so it has an oblong shape.

Planetary scientists are hoping to understand if there are reserves of water on the surface of the Martian moon, and to get more clues about its history. Did Phobos form with Mars, or was it captured later on?

If you have a pair of red-blue glasses, you can take a look at the 3D view of Phobos on the HiRISE site. Here’s a link.

Original Source: NASA/JPL/HiRISE News Release

Slowing to Mars Speed

When the Mars Science Laboratory (MSL) goes streaking through the Martian atmosphere at more than twice the speed of sound, it’s going to need one of the largest parachutes ever used in a space mission to successfully land a car-sized rover on the Red Planet. The parachute, built by Pioneer Aerospace, has 80 suspension lines, measures more than 50 meters (165 feet) in length, and opens to a diameter of nearly 17 meters (55 feet). It is the largest so called “disk-gap-band” parachute (more on that in a minute) ever built. To get ready for the scheduled 2009 launch of MSL, engineers have begun testing different parts of the parachute in preparation for the ultimate test of the entire parachute system.

Recent successful trials of two parachute packing techniques were performed in the world’s largest wind tunnel at NASA’s Ames Research Center. Engineers loaded chutes into a cannon and fired them out at 85 mph to simulate events during the real landing, looking for damage to line attachments and other parts. All four tests were successful, and high-speed video data is now being analyzed to select a final parachute design for the mission. But the large parachute is just the beginning of the unique landing technique MSL will use.

MSL will be the first planetary mission to use precision landing techniques, using a rocket-guided entry with a heat shield to steer itself toward the Martian surface similar to the way the space shuttle controls its entry through the Earth’s upper atmosphere. In this way, the spacecraft will fly to a desired location above the surface of Mars before deploying its parachute for the final landing. MSL will use a scaled-up version of parachutes used for the Viking and Mars Exploration Rovers mission. Called a Disk-Gap-Band parachute, the name describes the construction of the parachute: a disk forms the canopy, then a small gap, followed by a cylindrical band.

The parachute is deployed using a mortar that is triggered when the vehicle reaches a fixed planet-relative velocity. The parachute is designed to survive loads in excess of 36,000 kilograms (80,000 pounds).

Twice as long and three times as heavy as the Mars Exploration Rovers, MSL is too massive to use airbags like MER. MSL’s large parachute will only be deployed 3 minutes before touchdown which should slow the incoming vehicle enough for retro rockets to fire for the final 500 meters (1,640 feet) of the descent. But after that is where it gets interesting: In the final seconds, the hovering upper stage would act as a crane, lowering the upright rover on a tether to the surface. This is first the “Sky Crane” system will be used in a space mission.

MSL, a roving analytical laboratory, will collect Martian soil and rock samples and analyze them for organic compounds and environmental conditions that could have supported microbial life now or in the past.

Original News Source: JPL Press Release