In Memoriam: Spirit Rover, 2004-2010

Mars
The sun has set for the Spirit rover on Mars. Credit: NASA

If you’re feeling a little sad today at the news that the Spirit rover is “dead,” you’re not alone. And we all know we’re anthropomorphizing here, but it is hard not to. As MER project manager John Callas said at yesterday’s press conference, the MER rovers are “the cutest darn things out in the solar system,” and yes, we’ve become attached to them. Below are a few quotes we’ve gathered from Steve Squyres, Scott Maxwell, and some of the other people who have been involved with the MER mission in various capacities.

Feel free to add your best memories of Spirit’s mission in the comment section.

Rover Driver Scott Maxwell with a model of MER. Photo courtesy Scott Maxwell

Rover Driver Scott Maxwell. Maxwell has been part of the rover driving team since before the MER rovers lauched. He is publishing the diary he has kept, five years delayed on his Mars and Me blog.

“My take on this is that I know I’m supposed to be sad and I know that at some point I will be really sad, but at the moment it is hard to be sad because that feeling is overwhelmed by the pride of what Spirit accomplished,” Maxwell told Universe Today. “She accomplished an enormous amount in the six years plus that she was active on Mars, and we have every good reason to be proud of her. That is dominating my reaction to this announcement today. It terrible that she’s gone but I’m so proud of her, she did so much, she lived so long and accomplished such great things it’s hard to feel any other way.”

Will Spirit’s official loss put a big hole in Maxwell’s day?

“In terms of my practical day to day operations, not so much,” he said. “My day is filled with taking care of Opportunity and working on the upcoming Mar Science Lab mission, so actually I didn’t have that much to do with Spirit the past year. The way it will affect me is that I won’t be getting the weekly planning schedule for Spirit anymore, so in that way Spirit is going to disappear out of my world.”

Maxwell’s cat died a few months ago he finds he sometimes has an unconscious expectation that the cat will greet him when Maxwell returns home, but then he realizes the cat isn’t there anymore. “That’s the kind of hole that Spirit will leave in my life, where I’ll be unconsciously looking for scheduling emails, or data or information about Spirit, and it is not going to be there, and that place that she has occupied in my life is just not going to be there anymore. I’ve had time to get used to that over the past year, of not actively driving her, so I’ve gone through that transition and I’ll go through this transition next.”

MER PI Steve Squyres. Credit: NASA

Steve Squyres, MER Principal Investigator

“What’s most remarkable to me about Spirit’s mission is just how extensive her accomplishments became,” Squyres said in a JPL press release. “What we initially conceived as a fairly simple geologic experiment on Mars ultimately turned into humanity’s first real overland expedition across another planet. Spirit explored just as we would have, seeing a distant hill, climbing it, and showing us the vista from the summit. And she did it in a way that allowed everyone on Earth to be part of the adventure.”

Squyres said Spirit’s unexpected discovery of concentrated silica deposits was one of the most important findings by either rover.

“It showed that there were once hot springs or steam vents at the Spirit site, which could have provided favorable conditions for microbial life,” he said.

The silica-rich soil was next to a low plateau called Home Plate, which was Spirit’s main destination after the traverse long distances and climbed up and down Husband Hill. “What Spirit showed us at Home Plate was that early Mars could be a violent place, with water and hot rock interacting to make what must have been spectacular volcanic explosions. It was a dramatically different world than the cold, dry Mars of today,” said Squyres.

Chris Potts points to Gusev Crater on Mars on January 4, 2004, after the MER navigation team landed the Spirit rover on Mars with unprecedented accuracy. Photo courtesy of Chris Potts

Chris Potts was the Deputy Navigation Team Chief for both MER rovers.

“My thoughts immediately go back to the night Spirit landed in Gusev Crater on Jan. 3, 2004,” Potts told Universe Today. “It was a nerve wracking evening, thinking about the dangers involved with bringing Spirit from 12,000 mph to a safe landing via menacing bounces inside the airbags. No one could dare imagine that Spirit would continue on to explore Mars for over 6 years. Such an engineering feat requires the best from everyone involved, from the early designers to the operations team that extracted every last bit that Spirit had to offer. Spirit overcame so many obstacles on the journey, that the rover seemed to have a destiny that would not be denied. Spirit has finally reached the inevitable mission end, but I like to imagine the future when space tourists will follow Spirit’s tracks and continue to marvel at what the rover was able to accomplish.”

Doug Ellison, founder of UnmannedSpaceflight.com, where imaging enthusiasts get together to work with data being produced by robotic missions. He started the website, in part, because of the remarkable images being returned by the MER mission.

“I’ve been trying to figure out the words to describe how it feels,” Ellison told Universe Today. “Like losing a family member isn’t that short of the mark. When those early raw JPG’s were put onto their website so quickly I just couldn’t help myself. I found myself making color composites, panoramas, anaglyphs…and that’s what triggered the making of what became UMSF. It’s been a 7 year adventure that’s been shared through more than 125,000 images. We all lived that adventure through those pictures, together.”

Ellison said it is heartbreaking to see Spirit’s part of the mission come to an end. “Mars always had the power to end things, and she did, on her terms and not ours,” he said. “That’s as it should be, Spirit went down fighting in the battle against freezing temperatures on a barren near airless planet. My only regret is that we’ll never truly know exactly what caused Spirit to stay quiet.”

“We think of ‘Spirit’ as that robot on Mars,” he continued. “Without the team of scientists and engineers here on the ground who figured out what to do with that robot, the adventure we’ve been on, together, would never have happened. She’s part of this large team. She’s the teams feet with every drive she made. She’s their eyes with every picture she took. She’s their hands with every rock she studied. And, for many of us, she’s also its heart. The sol-to-sol rhythm of seeing new pictures and planning new adventures was the heartbeat of this large family that wasn’t just the mission personnel at JPL, Cornell and elsewhere – it wasn’t even just Spirit – it was all of us. That family was the thousands and thousands of people who followed along all over the world, it was the robot that did the dirty work, the engineers who kept her safe and the scientists who made the most of her. That family is now one member short – but it still exists. It formed around this little robot called Spirit, and will carry on through other projects.”

“Spirit didn’t die. She just moved on. I feel so very very sorry for the engineers who spent so long designing, building, and then for more than 6 years, using that little robot. But most of all, I feel sorry for Curiosity. As someone at UMSF suggested – that rover’s now sat in the clean room thinking ‘How the heck am I supposed to follow an act like that?'”

Neil Mottinger.

Neil Mottinger from JPL worked on the navigation team for the launch and trajectory of the two spacecraft that brought Spirit and Opportunity to Mars.

“It’s an incredible testimony to engineering that this plucky little craft survived 3 winters, when it wasn’t designed to survive any such weather conditions at all,” Mottinger told Universe Today. “Dust storms didn’t drown its ability to generate electricity thanks to the dust devils that repeatedly cleaned the panels. May its tenacity remind us all to strive for greater goals and push on way beyond the immediate horizons before us.”

Stu Atkinson, member of UMSF, poet and writer penned this poem about the end of Spirit’s mission. You can also read a short story he wrote about a year ago of what could have happened in some households when Spirit died.

MER Project Manager John Callas. Credit: JPL

John Callas has written a letter to his MER team, and in part said, “But let’s remember the adventure we have had. Spirit has climbed mountains, survived rover-killing dust storms, rode out three cold, dark winters and made some of the most spectacular discoveries on Mars. She has told us that Mars was once like Earth. There was water and hot springs, the conditions that could have supported life. She has given us a foundation to further explore the Red Planet and to understand ourselves and our place in the universe.

“But in addition to all the scientific discoveries Spirit has given us in her long, productive rover life, she has also given us a great intangible. Mars is no longer a strange, distant and unknown place. Mars is now our neighborhood. And we all go to work on Mars every day. Thank you, Spirit. Well done, little rover. And to all of you, well done, too.”

We’ll be adding more quotes about Spirit as they come in.

End of the Road for Spirit Rover

A composite image of how the Spirit rover probably looks, stuck in Gusev Crater. Credit: NASA, image editing by Stu Atkinson.

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In the wee hours of May 25, 2011 the scientists and engineers of the Mars Exploration Rover team will send the last command in attempt to contact the Spirit rover. Over the past year, they have sent over 1,200 commands and haven’t heard anything in reply from the stuck and likely frozen rover. “We have exhausted all the likely scenarios for contacting Spirit, and the likelihood of success is now practically zero,” said John Callas, Project Manager for the Mars Exploration Rover mission. “And at this point, the season is declining and we couldn’t do any of the planned science objectives even if we heard from her now. The Deep Space Network will occasionally listen for Spirit when resources permit, but we have decided not to do anything past the last commands that will done tonight.”

The Spirit rover, as seen by the HiRISE camera on the Mars Reconnaissance Orbiter. Credit: NASA, image enhanced by Stu Atkinson.

Spirit, the plucky rover that landed on Mars on January 3, 2004, overcame many difficulties and endured waaay past her 90-day warranty. For nearly six years, she traveled long distances, climbed hills — something the rovers weren’t really designed to do — she roved and stopped at interesting rocks along the way, all the while beaming back the information she garnered, enlightening us all about the nature of Mars, past and present.

Spirit became embedded in soft Martian soil in May of 2009 and that was the beginning of the end. The team spent months planning for her extrication, and then months again attempting to drive her out, but they ran out of time and power in the approaching Martian winter. The team was unable to put the rover in a favorable position to catch rays of sunlight on her solar panels, and after another freezing, grueling winter, Spirit has now likely succumbed to the harsh environment on Mars.

“We drove it, literally, until its wheels came off and at the beginning of the mission, we never expected that would be the way this project would end up,” said Dave Lavery, MER program director at NASA Headquarters.

The last commands will be sent early on May 25, 0700 UTC, which is just after midnight at JPL in Pasadena, California.

So, this is it. This is end of the Spirit rover mission.

“We always knew we would get to this point,” Callas said during a teleconference with the press, “and really, that’s what we wanted to do, to utilize these rovers as much as possible and wear them out. We are here today because we really wore Spirit out. If on sol 90 (the 90th Martian day of the mission) someone would have said this was going to last another 6 years, we just wouldn’t have believed it.”

The MER Spirit Rover (credit: NASA)

Asked what Spirit’s lasting legacy would be, Callas told Universe Today, “In addition to the great exploration and scientific discoveries, I think the great intangible that goes with Spirit is that she has made Mars a familiar place for us. It is no longer a mysterious location. For six years we’ve had people who go to work on Mars every day, via the rovers.”

The original plan was to try and contact Spirit once a week through the end of 2011, but the team has come to realize that the probability of success was practically zero and they would be wasting valuable resources, both human time and listening resources from the DSN. So the decision was made to end the attempts to contact Spirit.

The Spirit rover's solar panels were covered with dust until a gust of wind blew it off in 2006. Credit: NASA.

One of the challenges that Spirit faced is that it always had dust on the solar arrays, Callas said, even during the first winter on the Columbia Hills. After a timely dust cleaning event by a dust devil, the team was able tilt Spirit to gather sunshine and she survived. The second winter she achieved a 10% tilt and survived; the third winter, the team was able to find a 30% tilt – again she survived. But the 4th winter, there just wasn’t the right geography in the sand pits of Troy that would enable Spirit to survive after it became embedded.

What is the mood of the rover team? “We all are taking realistic look, as this mission was originally supposed to last only 90 sols, and we thought if we were extraordinarily lucky we’d get twice that much time and that the first Martian winter would be the end of the mission” said Lavery. “Realistically, in every possible definition of the word, we looking at this as a massive success in terms of longevity and the massive science return we got out of the project. As this particular chapter of Spirit’s mission comes to a close, this is very much a celebration of the accomplishments of the rover and the success it has had, and looking forward to the next steps of Mars exploration.”

Lavery added that the teams are not looking at this as a funeral, but more like an Irish wake. “I’m sure we’ll be telling stories of when Spirit was a wee little rover,” he said. There will be a science team meeting in July and they will use that opportunity to bring together all who were involved in development and science planning to come together and have some sort of event at that time.

“They are cutest darn things out in the solar system,” Callas said. “Yes, we are attached to these beautiful, accomplished little proxies out on the surface of Mars. We have sadness that we have to say goodbye to Spirit, but we have to remember the great accomplishments and the blessings we’ve received for having this rover operate for all this time, for over six years.”

A look at the nearly buried wheels on the Spirit rover on Mars. Credit: NASA/JPL

Spirit made many discoveries – finding carbonates which told scientists much about the past habitability of Mars and that it likely had a thicker atmosphere at one point. Then, even failure brought discovery, as the malfunction of the right front wheel in 2004 meant the team had to relearn to drive the rover, driving it backwards, dragging the wheel behind. This churned up the top soil and revealed what was under the surface: amorphous silica, which is evidence for an ancient hydrothermal system on Mars, which means not only water but an energy source that could have been driving a type of ecosystem in one particular location on Mars.

“There’s an enormous amount that can and still will be written about Spirit and the discoveries she’s made. The science team will be writing papers for a long while,” said Lavery. “But there’s also the inspiration that the rover provided to the team and really to the entire country that we were able to put together a project that went to another planet and survived well past its designed lifetime. The sense of wonder and sense of accomplishments go well beyond the mission itself.”

Yes, we knew this day was coming. Spirit roved her way into our hearts and into the science books. She will not be forgotten.

Spirit at work on Mars. Credit: NASA/JPL

Mars Science Lab Backshell Damaged (Updated)

The aeroshell for the Mars Science Laboratory. Credit: Lockheed Martin

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UPDATE: According to JPL’s Scott Maxwell on Twitter, the aeroshell was not damaged during the improper lifting, which is good news, as there should be no impact to the launch schedule.

The backshell for the Mars Science Laboratory was damaged last week at Kennedy Space Center when it was lifted improperly, according to Aviation Week. Engineers are now examining the backshell to determine the nature of the damage and how serious it is. There is no word yet on whether this could impact the launch of the Curiosity rover, which is currently set for November 25 of this year. The launch window extends to December 18, but after that the mission would have to wait about 26 months for the next favorable launch window.

An agency spokesman was quoted as saying the damage to the backshell did not appear to be serious. An Air Force C-17 carrying the backshell, cruise stage and heat shield arrived at Kennedy Space Center on May 12, while the rover and its unique the descent stage scheduled to arrive in June. The accident apparently involved the backshell being lifted with a crane in the wrong attitude, placing out-of-specification strain on clamps holding it together.

We’ll keep you posted.

Source: Aviation Week, h/t Stu Atkinson

Swirls, Gullies and Bedrock Create Two Jaw-Dropping Ethereal Mars Landscapes

A new image from the HiRISE camera on the Mars Reconnaissance Orbiter shows an ethereal landscape near Mars north pole. Credit: NASA/HiRISE team

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Wow! These two latest images from the HiRISE Camera on the Mars Reconnaissance Orbiter are simply amazing. I couldn’t decide which to post on top as the lead image, so did a coin flip. This observation shows dune gullies laced with beautiful swirls of tracks left by dust devils. Just like on Earth, dust devils move across the Martian surface and expose the underlying darker material, creating a striking view. The HiRISE team has been tracking changes in this location (-70.3 degrees latitude and 178.2 degrees Longitude East), and they also compare it with dune gully activity going on in other regions. The science team says the activity here is rather anomalous for their high altitude location.

And the other image….

Dunes and bedrock near Noachis Terra on Mars. Credit: NASA/HiRISE team.

This HiRISE image shows a very unique butter brickle-like landscape — it is actually dunes and bedrock on the floor of a crater near Noachis Terra. What strikes me most is the clarity of the detail in this image — it is absolutely stunning.

Scientifically, this crater is unique because it has been very well characterized as being olivine-rich. Olivine is a magnesium-iron silicate that is very common on Earth. There are other regions of Mars that are also rich in olivine, and since olivine turns into other minerals in the presence of water, scientists are interested in looking for those minerals as well.

The science team says that while the large scale morphology of these craters is well characterized, this is not the case with fine scale layering and fracturing, such as what is seen here. Studying landscapes like this could help the understanding of large scale crustal processes on Mars, including the genesis of magmas and the creation of regolith.

All I know is that it is just plain pretty.

See more images at the HiRISE website.

Guest Post: Drifting on Alien Winds: Exploring the Skies and Weather of Other Worlds

Triton Probe: Neptune’s blue skies may be visited by beachball-sized methane raindrops. (painting ©Michael Carroll)

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Editor’s note: We all want to explore other worlds in our solar system, but perhaps you haven’t considered the bizarre weather you’d encounter — from the blistering hurricane-force winds of Venus to the gentle methane rain showers of Saturn’s giant moon Titan. Science journalist Michael Carroll has written a guest post for Universe Today which provides peek at the subject matter for his new book, “Drifting on Alien Winds: Exploring the Skies and Weather of Other Worlds.

It’s been a dramatic year for weather on Earth. Blizzards have blanketed the east coast, crippling traffic and power grids. Cyclone Tasha drenched Queensland, Australia as rainfall swelled the mighty Mississippi, flooding the southern US. Eastern Europe and Asia broke high temperature records. But despite these meteorological theatrics, the Earth’s conditions are a calm echo of the weather on other worlds in our solar system.


Take our nearest planetary neighbor, Venus. Nearly a twin of Earth in size, Venus displays truly alien weather. The hurricane-force Venusian winds are ruled not by water (as on Earth), but by battery acid. Sunlight tears carbon dioxide molecules (CO2) apart in a process called photodissociation. Leftover bits of molecules frantically try to combine with sulfur and water to become chemically stable, resulting acid hazes. Temperatures soar to 900ºF at the surface, where air is as dense as the Earthly oceans at a depth of X feet.

Venus is the poster child of comparative planetology, the study of other planets to help us understand our own. Earth’s simmering sibling has taught us about greenhouse gases, and gave us an even more immediate cautionary tale in 1978. The Pioneer Venus orbiter discovered that Venus naturally generates chlorofluorocarbons (CFCs) in its atmosphere. These CFCs were tearing holes in the planet’s ozone. At the same time, a wide variety of industries were preparing to use CFCs in insecticides, spray paints, and other aerosol products. Venus presented us with a warning that may have averted a planet-wide crisis.

In the same way, Mars has provided insights into long-term climate change. Its weather is a simplified version of our own. Locked within its rocks and polar caps lie records of changing climate over eons.

Jupiter’s Great Red Spot is a cyclone larger than two Earths. (photomontage ©Michael Carroll)

But fans of really extreme weather must venture further out, to the outer planets. Jupiter and Saturn are giant balls of gas with no solid surface, and are known as the “gas giants.” They are truly gigantic: over a thousand Earths could fit within Jupiter itself.

The skies of Jupiter and Saturn are dominated by hydrogen and helium, the ancient building blocks of the solar system. Ammonia mixes in to produce a rich brew of complex chemistry, painting the clouds of Jupiter and Saturn in tans and grays. Lightning bolts sizzle through the clouds, powerful enough to electrify a small city for weeks. Ammonia forms rain and snow in the frigid skies. Jupiter’s Great Red Spot is a centuries-old cyclone large enough to swallow three Earths. Saturn has its own bizarre storms: a vast hexagon-shaped trough of clouds races across the northern hemisphere. Over the south pole, a vast whirlpool gazes from concentric clouds like a Cyclops.

Clouds tower into a twilight sky on Saturn. The planet’s glowing rings seem to bend at the horizon because of the dense air. (painting ©Michael Carroll)

Beyond Jupiter and Saturn lie the “ice giants”, Uranus and Neptune. These behemoths host atmospheres of poisonous brews chilled to cryogenic temperatures. Methane tints Uranus and Neptune blue. Neptune’s clear air reveals a teal cloud deck. Hydrocarbon hazes tinge Uranus to a paler shade of blue-green. Neptune’s clear air is somewhat of a mystery to scientists. This may be because cloud-forming particles can’t stay airborne long enough to become visible clouds. Some scientists propose that Neptune’s abundant methane rains may condense so rapidly that within a few seconds tiny methane raindrops swell to something the size of a beachball. There are no clouds adrift, because methane rains out of the atmosphere too quickly.

One of the strangest cases of bizarre weather comes to us from Neptune’s moon Triton. Triton’s meager nitrogen air is tied to the freezing and thawing of polar ices, also composed of nitrogen. Triton’s entire atmosphere collapses twice a year, when it’s winter on one of the poles. At that time of year, all of Triton’s air migrates to the winter pole, where it freezes to the ground. The moon only has “weather” during the spring and fall; its atmosphere exists only during those seasons.

So, the next time you contemplate complaining about the heat, think of Venus. And if it’s blizzards you worry about, find comfort in Triton: at least our atmosphere doesn’t disappear in winter!

For more on the subject, see Michael Carroll’s newest book, Drifting on Alien Winds: Exploring the Skies and Weather of Other Worlds from Springer.

More Evidence of Liquid Erosion on Mars?

Possible water-formed gullies cut through sedimentary layers in Terby Crater

 

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Terby Crater, a 170-km-wide (100-mile-wide) crater located on the northern edge of the vast Hellas Planitia basin in Mars’ southern hemisphere, is edged by variable-toned layers of sedimentary rock – possibly laid down over millennia of submersion beneath standing water. This image (false-color) from the HiRISE camera aboard the Mars Reconnaissance Orbiter shows a portion of Terby’s northern wall with what clearly looks like liquid-formed gullies slicing through the rock layers, branching from the upper levels into a main channel that flows downward, depositing a fan of material at the wall’s base.

But, looks can be deceiving…

 

Terby Crater. Credit: NASA/JPL/University of Arizona

Dry processes – especially on Mars, where large regions have been bone-dry for many millions of years – can often create the same effects on the landscape as those caused by running water. Windblown Martian sand and repetitive dry landslides can etch rock in much the same way as liquid water, given enough time. But the feature seen above in Terby seem to planetary scientists to be most likely the result of liquid erosion… especially considering that the sedimentary layers themselves seem to contain clay materials, which only form in the presence of liquid water. Is it possible that some water existed beneath Mars’ surface long after the planet’s surface dried out? Or that it’s still there? Only future exploration will tell for sure.

“While formation by liquid water is one of the proposed mechanisms for gully formation on Mars, there are others, such as gravity-driven mass-wasting (like a landslide) that don’t require the presence of liquid water. This is still an open question that scientists are actively pursuing.”

– Nicole Baugh, HiRISE Targeting Specialist

Terby Crater was once on the short list of potential landing sites for the new Mars Science Laboratory (aka Curiosity) rover but has since been removed from consideration. Still, it may one day be visited by a future robotic mission and have its gullies further explored from ground level.

Click here to see the original image on the HiRISE site.

Image credit: NASA / JPL / University of Arizona

Mars’ Underground Atmosphere

Pitted "swiss cheese" terrain at Mars' south pole hints at sublimation of underground CO2

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Scientists have spotted an underground reservoir near Mars’ south pole the size of Lake Superior… except that this lake is filled with frozen carbon dioxide – a.k.a. “dry ice”!

A recent report by scientists at the Southwest Research Institute in Boulder, CO reveals variations in Mars’ axial tilt can change how much carbon dioxide gets released into the atmosphere, affecting factors from the stability of water on its surface to the power and frequency of dust storms.

Thickness Map of Buried CO2 Ice Deposit
Thickness Map of Buried CO2 Ice Deposit

The Mars Reconnaissance Orbiter’s ground-penetrating Shallow Radar identified a subsurface deposit of frozen material, confirmed as carbon dioxide ice by its radar signature and visual correlation to the surface pitting seen above. As the polar surface warms during the Martian spring, underground CO2 deposits evaporate (or “sublime”) leaving behind round depressions in the frozen ground. (This has been aptly dubbed “swiss cheese terrain” by researchers on the HiRISE imaging team.)

While scientists were aware of seasonal CO2 ice layers atop the water ice this new discovery brings to light nearly 30 times more frozen CO2 than was previously believed to exist. In fact this particular deposit alone contains 80% the amount of CO2 currently present in the planet’s entire atmosphere.

The importance of this finding is how the carbon dioxide ultimately affects the global Martian climate as it freezes and thaws. When the CO2 is frozen and locked away in subsurface deposits like this, it’s not free to enter the atmosphere and do what CO2 does best: warm the planet… as well as increase atmospheric pressure. This means that liquid water cannot last as readily on the surface since it will either freeze or boil away. Also with less air pressure the strength of wind is decreased, so dust storms are less frequent and less severe.

When factored in with the axial tilt difference – and thus variations in the amount of sunlight hitting the poles – researchers’ models show that Mars’ average atmospheric pressure may at times be 75% higher than it is today.

These shifts in the orientation of the Red Planet’s axis occur on 100,000-year intervals… long by human standards but geologically very frequent. Mars may have had liquid water existing on its surface fairly recently!

Mars' south polar ice cap, seen in April 2000 by Mars Odyssey. NASA/JPL/MSSS

Although this may sound that Mars has had its own share of global warming due to CO2 emissions in its history, it must be remembered that Mars and Earth have very different atmospheric compositions. Earth’s atmosphere is much thicker and denser than Mars’, so even when doubling its CO2 content Mars’ atmosphere is still too thin and dry to create a strong greenhouse effect… especially considering that the polar caps on Mars increase cooling more than additional CO2 in the atmosphere raises global temperature. Without oceans and atmosphere to collect and distribute heat, the effect of any warming quickly radiates out into space…and eventually the planet swings back into a freeze-dried state.

“Unlike Earth, which has a thick, moist atmosphere that produces a strong greenhouse effect, Mars’ atmosphere is too thin and dry to produce as strong a greenhouse effect as Earth’s, even when you double its carbon-dioxide content.”

– Robert Haberle, planetary scientist at NASA’s Ames Research Center

Read the full news release on the NASA Missions site.

Image credit: NASA / JPL / University of Arizona

 

Solar Powered Jupiter bound JUNO lands at Kennedy Space Center for blastoff

The Juno spacecraft passes in front of Jupiter in this artist's depiction. Juno, the second mission in NASA's New Frontiers program, will improve our understanding of the solar system by advancing studies of the origin and evolution of Jupiter. The spacecraft will carry eight instruments to investigate the existence of a solid planetary core, map Jupiter's intense magnetic field, measure the amount of water and ammonia in the deep atmosphere, and observe the planet's auroras. Credit: NASA/JPL-Caltech

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Juno, NASA’s next big mission bound for the outer planets, has arrived at the Kennedy Space Center to kick off the final leg of launch preparations in anticipation of blastoff for Jupiter this summer.

The huge solar-powered Juno spacecraft will skim to within 4800 kilometers (3000 miles) of the cloud tops of Jupiter to study the origin and evolution of our solar system’s largest planet. Understanding the mechanism of how Jupiter formed will lead to a better understanding of the origin of planetary systems around other stars throughout our galaxy.

Juno will be spinning like a windmill as it fly’s in a highly elliptical polar orbit and investigates the gas giant’s origins, structure, atmosphere and magnetosphere with a suite of nine science instruments.

Technicians at Astrotech's payload processing facility in Titusville, Fla. secure NASA's Juno spacecraft to the rotation stand for testing. The solar-powered spacecraft will orbit Jupiter's poles 33 times to find out more about the gas giant's origins. Credit: NASA/Jack Pfaller

During the five year cruise to Jupiter, the 3,600 kilogram probe will fly by Earth once in 2013 to pick up speed and accelerate Juno past the asteroid belt on its long journey to the Jovian system where it arrives in July 2016.

Juno will orbit Jupiter 33 times and search for the existence of a solid planetary core, map Jupiter’s intense magnetic field, measure the amount of water and ammonia in the deep atmosphere, and observe the planet’s auroras.

The mission will provide the first detailed glimpse of Jupiter’s poles and is set to last approximately one year. The elliptical orbit will allow Juno to avoid most of Jupiter’s harsh radiation regions that can severely damage the spacecraft systems.

Juno was designed and built by Lockheed Martin Space Systems, Denver, and air shipped in a protective shipping container inside the belly of a U.S. Air Force C-17 Globemaster cargo jet to the Astrotech payload processing facility in Titusville, Fla.

Juno undergoes acoustics testing at Lockheed Martin in Denver where the spacecraft was built. Credit: NASA/JPL-Caltech/Lockheed Martin

This week the spacecraft begins about four months of final functional testing and integration inside the climate controlled clean room and undergoes a thorough verification that all its systems are healthy. Other processing work before launch includes attachment of the long magnetometer boom and solar arrays which arrived earlier.

Juno is the first solar powered probe to be launched to the outer planets and operate at such a great distance from the sun. Since Jupiter receives 25 times less sunlight than Earth, Juno will carry three giant solar panels, each spanning more than 20 meters (66 feet) in length. They will remain continuously in sunlight from the time they are unfurled after launch through the end of the mission.

“The Juno spacecraft and the team have come a long way since this project was first conceived in 2003,” said Scott Bolton, Juno’s principal investigator, based at Southwest Research Institute in San Antonio, in a statement. “We’re only a few months away from a mission of discovery that could very well rewrite the books on not only how Jupiter was born, but how our solar system came into being.”

Juno is slated to launch aboard the most powerful version of the Atlas V rocket – augmented by 5 solid rocket boosters – from Cape Canaveral, Fla. on August 5. The launch window extends through August 26. Juno is the second mission in NASA’s New Frontiers program.

NASA’s Mars Curiosity Rover will follow Juno to the Atlas launch pad, and is scheduled to liftoff in late November 2011. Read my stories about Curiosity here and here.

Because of cuts to NASA’s budget by politicians in Washington, the long hoped for mission to investigate the Jovian moon Europa may be axed, along with other high priority science missions. Europa may harbor subsurface oceans of liquid water and is a prime target in NASA’s search for life beyond Earth.

Technicians inside the clean room at Astrotech in Titusville, Fla. guide NASA's Juno spacecraft, as it is lowered by overhead crane, onto the rotation stand for testing. Credit: NASA/Jack Pfaller
Technicians at Astrotech unfurl solar array No. 1 with a magnetometer boom that will help power NASA's Juno spacecraft on a mission to Jupiter. Credit: NASA
Juno's interplanetary trajectory to Jupiter. Juno will launch in August 2011 and fly by Earth once in October 2013 during its 5 year cruise to Jupiter. Click to enlarge. Credit: NASA/JPL

Curiosity Mars Rover Almost Complete

Curiosity Mars Rover almost complete at NASA’s Jet Propulsion Laboratory – Side View. The rover for NASA's Mars Science Laboratory mission, named Curiosity, is about 3 meters (10 feet) long, not counting the additional length that the rover's arm can be extended forward. The front of the rover is on the left in this side view. The arm is partially raised but not extended. Rising from the rover deck just behind the front wheels is the remote sensing mast. Credit: NASA/JPL-Caltech

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NASA’s massive ‘Curiosity’ rover is almost ready to begin the first leg of its long trek to the surface of the Red Planet. Engineers at NASA’s Jet Propulsion Laboratory in California are nearly finished with assembling and testing all the components of the Mars Science Laboratory (MSL) mission (see photos above and below).

The MSL team plans to ship Curiosity as well as the cruise stage, descent stage and back shell to the Kennedy Space Center (KSC) in May and June. After arriving at KSC, all the pieces will be integrated together and tested during final assembly in a clean room. The rover will then be installed inside a 5 meter diameter nose cone, shipped the short distance to Cape Canaveral and then bolted atop an Atlas V rocket (photo below).

Top of Mars Rover Curiosity's Remote Sensing Mast.
The remote sensing mast on NASA Mars rover Curiosity holds two science instruments for studying the rover's surroundings and two stereo navigation cameras for use in driving the rover and planning rover activities. Credit: NASA/JPL-Caltech

The launch window for Curiosity extends from Nov. 25 to Dec. 18, 2011. The first stage of the powerful Atlas V rocket will be augmented with four solid rocket boosters. The Atlas V has previously launched two planetary missions; the Mars Reconnaissance Orbiter (MRO) and the New Horizons mission to Pluto.

Take a long gander at the 3 meter long rover because its appearance is now very much how it will look while it’s roving along intriguing martian landscapes for at least two earth years after landing in August 2012.

NASA Mars Rover Curiosity at JPL, View from Front Left Corner.
Support equipment is holding the Mars rover Curiosity slightly off the floor. When the wheels are on the ground, the top of the rover's mast is about 2.2 meters (7 feet) above ground level. Credit: NASA/JPL-Caltech

The mini-Cooper sized Curiosity rover is equipped with 10 science instruments to investigate Martian soil and rock samples in far greater detail than ever before. Curiosity’s science payload weighs ten times more than any prior Mars rover mission.

The goal is to search for clues to environmental conditions favorable for microbial life and for preserving evidence about whether Martian life ever existed in the past or today. NASA is scrutinizing a list of four potential landing sites for the best chance of finding a habitable zone.

Arm and Mast of Curiosity Mars Rover.
Curiosity's arm and remote sensing mast carry science instruments and other tools for the mission. This image, taken April 4, 2011, inside the Spacecraft Assembly Facility at JPL shows the arm on the left and the mast just right of center. Credit: NASA/JPL-Caltech
Atlas V rocket at pad 41 at Cape Canaveral Air Force Station.
An Atlas V rocket similar to this one with a 5 meter diameter nose cone – but with 4 solid rocket boosters added - will launch Curiosity to Mars in late 2011. Credit: Ken Kremer
Atlas V launch vehicle will blast Curiosity to Mars

10 Years of the Mars Odyssey

This view across western Candor Chasma on Mars was created with data from the 2001 Mars Odyssey. Credit: NASA/JPL/Arizona State University, R. Luk

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A 2001 space odyssey indeed! On this day in 2001, the Mars Odyssey spacecraft launched, and now, 3,333 days later, the robotic spacecraft is still going strong. In orbit around the Red Planet, Mars Odyssey has collected more than 130,000 images and continues to send information to Earth about Martian geology, climate, and mineralogy. Last December, Mars Odyssey broke the record for the longest-serving spacecraft at Mars, besting the Mars Global Surveyor, which operated in orbit of Mars from 1997 to 2006.

An artist's impression of the Odyssey orbiter around Mars. . Image Credit: NASA

Measurements by Odyssey have enabled scientists to create maps of minerals and chemical elements and identify regions with buried water ice. Images that measure the surface temperature have provided spectacular views of Martian topography.

Early in the mission, Odyssey determined that radiation in low-Mars orbit is twice that in low-Earth orbit. This is an essential piece of information for eventual human exploration because of its potential health effects — Odyssey has provided vital support to ongoing exploration of Mars by relaying data from the Mars rovers to Earth via the spacecraft’s UHF antenna.

Odyssey will support the 2012 landing of the Mars Science Laboratory and surface operations of that mission. Mars Science Laboratory, a.k.a Curiosity, will assess whether its landing area has had environmental conditions favorable for microbial life and preserving evidence about whether life has existed there. The rover will carry the largest, most advanced set of instruments for scientific studies ever sent to the Martian surface.

Mars Odyssey carries three main science instruments: The Gamma Ray Spectrometer (GRS), the Thermal Emission Imaging System (THEMIS), and the Mars Radiation Environment Experiment (MARIE).

More info: Mars Odyssey website, THEMIS website (tons of great images)