NASA’s Resilient Rover Opportunity Begins Year 9 On Mars with Audacious Science Ahead

Martian Vista from Opportunity at Endeavour Crater - 8 Years on Mars. NASA’s Opportunity rover celebrated 8 Years on Mars on January 24, 2012. This mosaic shows portions of the segmented rim of Endeavour crater (14 miles, 22 km wide) after the robot arriving at the craters foothills in August 2011. Large ejecta blocks from a smaller nearby crater are visible in the middle. At Endeavour, Opportunity will investigate the oldest minerals deposits she has ever visited from billions of years ago and which may hold clues to environments that were potentially habitable for microbial life. The rover will eventually drive to Cape Tribulation at right after surviving her 5th winter on Mars. Mosaic Credit: NASA/JPL/Cornell/Marco Di Lorenzo/Kenneth Kremer

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Today, the resilient Opportunity robot begins her 9th year roving around beautifully Earth-like Martian terrain where potentially life sustaining liquid water once flowed billions of years ago.

Opportunity celebrates her 8th anniversary on the Red Planet gazing at the foothills of the vast crater named Endeavour, promising a “mother lode” of “watery” science – an unimaginable circumstance since the nail biting landing on the hematite rich plains of Meridiani Planum on 24 January 2004.

“Opportunity is 97 months into the 3 month mission,” team members are proud and universally surprised to say.

“Milestones like 8 years on Mars always make me look forward rather than looking back,” Rover Principal Investigator Prof. Steve Squyres of Cornell University told Universe Today for this article commemorating Opportunity’s landing.

“We’ve still got a lot of exploring to do, but we’re doing it with a vehicle that was designed for a 90-sol mission. That means that every sol is a gift at this point.”

Opportunity has driven more than 21 miles (34 kilometers) across the Red Planet’s surface during what is truly humankind’s first overland expedition on another Planet. See our route map below.

Opportunity Rover Traverse Map at Meridiani Planum on Mars - 2004 to 2012
Traverse map shows the 8 Year Journey of Opportunity from Eagle Crater landing site on Sol 1- Jan. 24, 2004 - to 5th Winter Haven worksite at Greeley Haven at Endeavour Crater rim in January 2012. Opportunity embarked on a crater tour and discovered bountiful evidence for the flow of liquid water on Mars billions of years ago. The robot has shown that ancient ephemeral shallow lakes existed on Mars when the cratered terrain was cut by fluvial channels. Endeavour Crater is 14 miles (22 kilometers) in diameter. Opportunity has so far driven more than 21 miles (34 km) over 8 Years but was only expected to live for 90 Martian days. Credit: NASA/JPL/Cornell/UA/Marco Di Lorenzo/Kenneth Kremer

NASA’s twin rovers Spirit and Opportunity blasted off for Mars atop a pair of Delta II rockets in the summer of 2003 with a mission “warranty” of just 90 Martian days, or Sols.

Today is Sol 2846 of working operations for Opportunity, compared to an anticipated lifetime of only 90 Sols – that amounts to more than 31 times beyond the designer’s expectations.

Indeed, the long lived robot is now enduring her 5th Winter on Mars. And to glimpse the next Martian sunrise, the robo girls manmade components must survive the harsh extremes of frigid Antarctic-like temperatures each and every sol.

“I never thought that we would still be planning sequences for Opportunity today,” Ray Arvidson told Universe Today. Arvidson, of Washington University in St. Louis, is the deputy rover principal investigator.

“I seriously thought both Spirit and Opportunity would be finished by the summer of 2004.”

Opportunity's Eighth Anniversary View From 'Greeley Haven' (False Color). This mosaic of images taken in mid-January 2012 shows the windswept vista northward (left) to northeastward (right) from the location where Opportunity is spending its fifth Martian winter, an outcrop informally named "Greeley Haven. Credit: NASA/JPL-Caltech/Cornell/Arizona State Univ.

But, Opportunity is the gift to science that keeps on giving.

“I am feeling pretty good as the MER rover anniversaries approach,” Arvidson told me.

“Opportunity has shown that ancient ephemeral shallow lakes existed as Mars moved climatically from an early period when the cratered terrain was cut by fluvial channels to the current dry and cold conditions that dominate.”

“Both rovers have conclusively shown the need for lateral mobility to get to relevant outcrops and back out the secrets associated with past conditions,” Arvidson explained.

Barely a month ago the bountiful harvest from mobility was once again demonstrated when the science team lead by Squyres and Arvidson announced that Opportunity had discovered the most scientifically compelling evidence yet for the flow of liquid water on ancient Mars.

Squyres and Arvidson announced that Opportunity had found a bright vein – named “Homestake” – composed of the mineral gypsum located at the Cape York segment of Endeavour Crater where the intrepid robot is currently spending her 5th Martian Winter.

“This gypsum vein is the single most powerful piece of evidence for liquid water at Mars that has been discovered by the Opportunity rover,” Squyres explained.

Veins are a geologic indication of the past flow of liquid water.

See our mosaic below illustrating the exact location of the “Homestake” vein at Endeavour Crater – also published at Astronomy Picture of the Day; 12 Dec 2011.

Opportunity discovers Water related Mineral Vein at Endeavour Crater - November 2011
Opportunity rover discovered Gypsum at the Homestake mineral vein, while exploring around the base of Cape York ridge at the rim of Endeavour Crater. The vein is composed of calcium sulfate and indicates the ancient flow of liquid water at this spot on Mars. This panoramic mosaic of images was taken on Sol 2761, November 2011, and illustrates the exact spot of the mineral vein discovery.
Credit: NASA/JPL/Cornell/Kenneth Kremer/Marco Di Lorenzo
Published on Astronomy Picture of the Day (APOD): 12 Dec 2011

Opportunity just arrived at the rim of the 14 mile (22 kilometer) wide Endeavour Crater in mid-August 2011 following an epic three year trek across treacherous dune fields from her prior investigative target at the ½ mile wide Victoria Crater.

“It’s like a whole new mission since we arrived at Cape York,” says Squyres.

For the next few months of the bitterly cold Martian winter, Opportunity will conduct a vigorous science campaign while remaining mostly stationary at a spot dubbed “Greeley Haven” in honor of Prof. Ronald Greeley, a team member from Arizona State University who recently passed away.

Opportunity Mars Rover at 5th Winter Worksite at Endeavour Crater
This mosaic shows the view of NASA’s Opportunity rover parked at “Greeley Haven” worksite where the robot will spend her 5th Martian Winter. This mosaic of images shows the Winter Haven view from the Cape York Ridge at the western rim of Endeavour Crater looking south along the crater rim. Tire tracks at right. Credit: NASA/JPL/Cornell/ Marco Di Lorenzo/Kenneth Kremer

At this moment Opportunity is snapping a 360 degree panorama, deploying her robotic arm onto nearby outcrops, collecting microscopic images, making measurements of mineral compositions with the Alpha Particle X-Ray Spectrometer and conducting radio science observations to elucidate the unknown structure of the Martian interior and core.

The rover is covered with a significant coating of dust which limits her ability to generate power from the life sustaining solar arrays. Since Opportunity is traversing just south of the equator, engineers have temporarily parked her on a northerly facing slope to maximize the electric power generation.

“Opportunity is currently sitting on an outcrop of impact breccias at Greeley Haven on Cape York,” said Arvidson.

Opportunity will remain at Greeley Haven until some time after the Winter Solstice of southern Martian winter occurs at the end of March.

'Greeley Haven' Site for Opportunity's Fifth Martian Winter. This mosaic of Greeley Haven was acquired by Opportunity on Sol 2793, Dec. 2, 2011. Credit: NASA/JPL-Caltech/Cornell/Arizona State Univ.

Then she’ll head south to further explore the veins and eventually drive to deposits of the clay mineral located a few miles (km) away along the craters rim.

“We’ll do good science while we’re at Greeley Haven. But as soon as we catch a wind gust or the seasons change, we’ll be on our way again,” Squyres told me.

The legendary twins Spirit and Opportunity surely rank as one of the greatest triumphs in space exploration.

Few Details in ESA’s Report on Phobos-Grunt Re-Entry

The map above shows the predicted trajectory of the Fobos-Grunt probe upon reentry. Russian space officials initially said the probe landed at one of the red dots, but later acknowledged that it could have touched down anywhere along the area indicated by the red line segment. Credit: Robert Christy, www.zarya.info

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A week and a half after the re-entry of Russia’s Phobos–Grunt probe, experts have now made an official statement on their determination of where the spacecraft entered Earth’s atmosphere. But their report offers no information regarding if any pieces of the craft made it to Earth and where any remaining debris might be. Consequently, recovery of any pieces, including the Phobos-LIFE biomodule is highly unlikely.

“While this was an uncontrolled reentry, the location of the potential impact area was largely over ocean, with a correspondingly low probability of any detrimental effects,” said Prof. Heiner Klinkrad, Head of ESA’s Space Debris Office in Darmstadt, Germany.

The Inter-Agency Space Debris Coordination Committee (IADC) reports that Phobos–Grunt re-entered on January 15, 2012 at 17:46 GMT, at an altitude of 80 km at 46°S and 87°W, near the South American coastline. About 7 minutes later, the report says, the spacecraft’s altitude was 10 km.

“Within the expected uncertainties, the prediction has been largely confirmed by observations,” ESA’s press release stated.

And that is all the information the IADC has provided, with no details on whether those observations were from observers on the ground or from satellite and radar facilities.

In fact, most of the initial information verifying that Phobos-Grunt was no longer in orbit came from ground observations of not seeing the spacecraft in orbit over Europe after 18:00 UTC on January 15 when it was supposed to have a visible pass.

IADC members include NASA, Roscosmos, the European Space Agency, European national agencies and the space agencies of Canada, China, India, Japan and Ukraine. The group primarily used orbit data from the U.S. Space Surveillance Network and the Russian Space Surveillance System to determine Phobos-Grunt’s path to destruction. Radar systems in Germany and France also provided orbit calculations.

Phobos-Grunt orbiter and lander. Credit: ESA

Before re-entry, predictions from the various agencies differed widely, and initially after the probe was said to have re-entered, there was confusion on when and where the re-entry took place. Roscosmos initially released a statement claiming that the probe had fallen safely in the Pacific, off the coast of Chile, but later there were reports that fragments of the spacecraft had fallen in the south Atlantic Ocean. Officials said the confusion was due to the large number of uncertainties in the spacecraft’s orbit and the space environment affecting the satellite.

Indeed, everyone involved in re-entry calculations acknowledges the problematic nature of trying to monitor things in real-time, such as atmospheric density in the specific location the object is traveling. Most of the time, the details can only be deduced after the time of re-entry, and any unknowns can alter the projected re-entry and impact point by wide margins.

And so it is not entirely surprising that the IADC cannot offer much information beyond the initial entry point and time for Phobos-Grunt.

Although much of the Phobos-Grunt spacecraft was expected to disintegrate upon re-entry, Roscosmos said perhaps 20 to 30 fragments weighing a combined 200 kg (440 lb.) might survive and fall somewhere over a vast strip of the Earth’s surface between 51.4 deg. north and south of the equator.

The cause of the spacecraft’s malfunction has not yet been determined, and Roscosmos has indicated that a full report on the failure will be published on January 26, 2012, although an interim report said to be available by January 20 did not appear. The investigation is being conducted by Yuri Koptev, former head of the Russian Space Agency.

Shortly after launching from the Baikonur Cosmodrome on Nov. 9, 2011, the probe became stuck in low Earth orbit after its upper stage engines repeatedly failed to ignite to send the ship on an unprecedented sample return mission to Mars’ moon Phobos. Later, ESA tracking stations were instrumental in establishing short-lived contact with the probe, leading to hopes the spacecraft could be saved. But subsequent contact was not able to be made, and without contact and inputs from the ground, the spacecraft’s orbit disintegrated.

However, the story of Phobos-Grunt’s malfunctions and demise has included some wild claims ranging from accidental radar interference to outright sabotage, along with intimations of conspiracy theories.

Several times after the malfunction, Russian space officials suggested that US radar emissions may have accidently disabled the spacecraft; at first from a station in Alaska, and then — after it was pointed out that Phobos-Grunt had never flown over that location — another Russian official said it was perhaps radar from a military installation on Kwajalein Atoll in the Marshall Islands.

But these claims were later dismissed by a Russian scientist, Alexander Zakharov from the Russian Academy of Science Space Research Institute, who was involved with the development of Phobos-Grunt. He told the Russian news agency Ria Novosti that the radar theory is “far-fetched,” and suggested instead that issues with the spacecraft itself were likely to blame.

“You can come up with a lot of exotic reasons,” Zakharov told RIA Novosti. “But first you need to look at the apparatus itself. There are problems there,” and he indicated there may have been some known problems with the second stage of the rocket.

Later, after re-entry, links to Phobos-Grunt tracking data on the Space Track website were removed, fueling speculation of a conspiracy to hide in formation of where the probe fell. Space Track is a public website that ordinarily details such events, and is operated by U.S. Strategic Command. The military also did not publish any confirmation of the probe’s fall, which is not the usual protocol.

But later, the US Strategic Command said a human error had accidentally misfiled the information (in the 2011 files instead of 2012). Shortly after the error was discovered, the information was re-posted to the site and is accessible at this time.

The Planetary Society’s Living Interplanetary Flight Experiment (LIFE) capsule, on board the Phobos-Grunt spacecraft. Credit:The Planetary Society

Meanwhile, hopes dim for finding the capsule for the Phobos-LIFE biomodule which included organisms in a small capsule to test the “transpermia” hypothesis –- the possibility that life can travel from planet to planet inside rocks blasted off one planetary surface by impact, to land on another planetary surface. The biomodule would have flown to Phobos and then returned to Earth with the sample return capsule of the Phobos-Grunt spacecraft.

“Because we can’t predict the details of the re-entry, we can’t predict whether the Phobos LIFE biomodule will survive, and certainly we can’t predict whether it will land somewhere it could be recovered,” said Bruce Betts from The Planetary Society, which sponsored the LIFE mission. “In the unlikely event the Phobos LIFE biomodule is recovered, we would want to study the organisms inside. Though not the long deep space experience we had hoped for, there still will be scientific value to study of the organisms even after just two months in low Earth orbit.”

Sources: ESA, ZaryaInfo.com, ieeeSpectrum/Jim Oberg, Ria Novosti. Special thanks to Robert Christy for the lead image, from his website Zarya.info

8 Years on Mars: Downloadable Rover Poster

8 years ago today, January 24, the Opportunity rover landed on Mars. In what has become a tradition, Stu Atkinson and Astro0 from Unmanned Spaceflight have teamed up to create a poster and poem combo to celebrate the occasion. While we fondly remember Spirit’s now-finished journey, the poster features scenes from Opportunity’s view of the ‘Tribulation’ hill and the hills of the crater rim beyond. And no, Oppy didn’t actually spin out in double donuts on Mars to create the ‘figure 8.’

“For a little effect, we’ve added the ‘figure 8’ in the form of the rovers own tracks on Mars,” Astro0 said. “While they may have dreamed of doing it, I’m sure no rover driver would ever be tempted to leave such a mark on Mars for real. So it was only right and proper that I and Photoshop do it for them.”

Click on the image above for a larger version or visit the Astro0 website for higher resolution versions that you can download to print out as a poster or use for your computer wallpaper. Stu’s poem — which both waxes wistful about the year of the MER rovers landing and prognosticates Mars’ future — is written out below:

8 Years on Mars

Hard to believe the Homeworld has circled Sol eight times
Since the first MER bounced and boinged to a historic halt on Mars,
Spirit followed faithfully soon after by her sister, Opportunity,
Just as Clark had followed Lewis two centuries before.
Babies born bloodied and bawling on the day chase girls
In busy schoolyards now; wide-eyed, Star Trek t-shirt wearing
Interns who stumbled along the deer-stalked paths of JPL
Now have interns of their own, and peer at screens painted
Picasso-shades by read date beamed from the true Final Frontier…

In a thousand years, when Mars has oceans of retina-burning blue,
And honeymooning couples crump across the snow-capped summit
Of Olympus, the names ‘Spirit’ and ‘Opportunity’ will still be
Spoken wistfully; and tourists from Titan, explorers from Europa
And Hyperion’s most respected historians will stand before
The rovers, displayed in all their restored gory in the Great
Museum of Mars and envy us, this generation which saw Gusev’s
Rugged Rocks and Meridiani’s misty mountains for the first time,
In 2004, the year Earth finally conquered Mars.

By Stu Atkinson

To see maps of where the rovers are now, see the Mars Rover website.

See more images and musings on space at the Astro0 website, and follow along Oppy’s journey at the Stu’s Road to Endeavour site. For more skillfully mastered images from the MER mission and more, visit Unmanned Spaceflight.

Opportunity arrives at Greeley Haven – 5th Winter Haven Worksite on Mars

Opportunity Mars Rover at Winter Haven Worksite at Endeavour Crater. NASA’s Opportunity rover has parked near this spot at the “Greeley Haven” worksite where the robot will spend her 5th Martian Winter Haven since landing 8 years ago in January 2004. This mosaic of images was snapped in December 2011 and shows the view from the Cape York Ridge at the western rim of Endeavour Crater looking south along the crater rim to a future area that Opportunity will drive to and explore next spring. Credit: NASA/JPL/Cornell/ Marco Di Lorenzo/Kenneth Kremer

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NASA’s seemingly indestructible Opportunity rover has arrived at the breathtaking location where she’ll be working through her unfathomable 5th Martian Winter. The Opportunity Mars Exploration Rover has not only endured, but flourished for 8 years of unending “Exploration & Discovery” on the Red Planet despite having an expected lifetime at landing of just 3 months, way back in January 2004.

Opportunity is parked at a northward facing outcrop dubbed “Greeley Haven” where she can soak up the sun and juice her innards throughout the utterly harsh and Antarctic-like temperatures on tap for the next few months that threaten to kill her each and every Martian day. See our mosaic above around the Greeley Haven area.

Science team members told Universe Today that the rover is sitting at Greeley Haven because the site offers a roughly 15 degree tilt that will maximize the electric output from the life-giving solar arrays and also allow the robot to carry out a vigorous science campaign during the seasonal Martian winter season that officially begins in March.

Greeley Haven is a located at the northern tip of the “Cape York” segment of the western rim of the vast crater named Endeavour, some 14 miles (22 km) wide that’s loaded with a bountiful variety of rocks and soil that neither Opportunity nor her twin Spirit have ever touched and drilled into before and stem from an earlier epoch when liquid water flowed eons ago and perhaps may have been more favorable to sustaining life.

“Opportunity is currently sitting on Saddleback at Greeley Haven, an outcrop of impact breccias on Cape York, Endeavour crater’s rim,” Ray Arvidson told Universe Today. Arvisdon is the mission’s deputy principal investigator, of Washington University in St. Louis.

“Her northerly tilt is about ~15 degrees which is enough to have a vibrant winter campaign. The Martian southern winter solstice occurs at the end of March. A few months after that date we will drive her off the outcrop and further explore Cape York.”

Approaching 'Greeley Haven' on Endeavour Rim
Opportunity captured this view of a northward-facing outcrop, "Greeley Haven," where the rover will work during its fifth Martian winter. This southward-looking image was taken on Sol 2790 on Mars (Nov. 29, 2011). The rover team chose this designation as a tribute to the influential planetary geologist Ronald Greeley (1939-2011), who was a member of the science team for the Mars rovers and many other interplanetary missions. Credit: NASA/JPL-Caltech

“Greeley Haven” is named in tribute to planetary Geologist Ronald Greeley (1939-2011) who was a beloved member of the rover science team and a host of other NASA planetary missions. He taught at Arizona State University and inspired several generations of students and planetary scientists until his recent death on Oct. 27, 2011.

“We’ll hunker down at Greeley Haven as long as we need to, and we’ll do good science while we’re there,” Steve Squyres of Cornell University, Ithaca, N.Y., told Universe Today. Squyres is the Principal Investigator for Opportunity.

Opportunity is collecting a high resolution 360 degree panorama to commemorate Greeley.

Throughout the past 4 Martian winters, Opportunity had continued to traverse without pause. But this winter time it’s different because the solar panels are significantly more coated with an obscuring layer of dust hindering their energy output.

So the rover is parked with a tilt for her 5th Martian winter, mimicking the successful strategy power boosting used by Spirit to survive 3 harsh Martian winters.

And there is a silver lining to sitting mostly still that enables a chance to determine what’s at the core of the Red Planet, a key fact we don’t know.

“This winter science campaign will feature two way radio tracking with Earth to determine the Martian spin axis dynamics – thus the interior structure, a long-neglected aspect of Mars,” Arvidson told me.

I asked Squyres for a progress update and how long would the data collection require ?

Squyres replied that the experiment has already begun and added – “Hard to say how long. It’s months, as opposed to weeks or years, but it depends very much on data quality and the amount of data we get per week. We’re very early in the experiment now… we’ll just see how it goes.”

Locator Map for 'Greeley Haven' on Endeavour Crater Rim
Opportunity will spend its fifth Martian winter working at Greeley Haven on the western rim of Endeavour Crater. Credit: NASA/JPL-Caltech/UA

3 Generations of NASA’s Mars Rovers

Three Generations of Mars Rovers in the Mars Yard. This grouping shows 3 generations of NASA’s Mars rovers from 1997 to 2012 set inside the Mars Yard at the Jet Propulsion Lab in Pasadena, Calif. The Mars Pathfinder Project (front) landed the first Mars rover - Sojourner - in 1997. The Mars Exploration Rover Project (left) landed Spirit and Opportunity on Mars in 2004. The Mars Science Laboratory Project (right) is on course to land Curiosity on Mars in August 2012. Credit: NASA/JPL-Caltech

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NASA Mars rovers have come a long way in terms of size and capability since the rebirth of Red Planet surface exploration just 15 years ago – spanning from 1997 to 2012.

To get a really excellent sense of just how far America’s scientists and engineers have pushed the state of the art in such a short time – when the willpower and funding existed and coincided to explore another world – take a good look at the new pictures here showing 3 generations of NASA’s Mars rovers; namely Mars Pathfinder (MPF), the 1st generation Mars rover, Mars Exploration Rover (MER), the 2nd generation, and Mars Science Laboratory (MSL), the 3rd and newest generation Mars rover.

The newly released pictures graphically display a side by side comparison of the flight spare for Mars Pathfinder (1997 landing) and full scale test rovers of the Mars Exploration Rover (2004 landing) and Mars Science Laboratory (in transit for a 2012 planned landing). The setting is inside the “Mars Yard” at NASA’s Jet Propulsion Laboratory, Pasadena, Calif. where the teams conduct mission simulations.

It’s been nothing less than a quantum leap in advancement of the scientific and technological capability from one generation to the next.

Sojourner - NASA’s 1st Mars Rover
Sojourner takes an Alpha Proton X-ray Spectrometer (APXS) measurement of Yogi rock after Red Planet landing on July 4, 1997 landing. Sojourner was only 2 feet long, the size of a microwave oven.
Credit: NASA

Just consider the big increase in size – growing from a microwave oven to a car !

The “Marie Curie” flight spare and the actual “Sojourner” rover on Mars are 2 feet (65 centimeters) long – about the size of a microwave oven. The MER rovers “Spirit and Opportunity” and the “Surface System Test Bed” rover are 5.2 feet (1.6 meters) long – about the size of a golf cart. The MSL “Curiosity” and the “Vehicle System Test Bed” rover are 10 feet (3 meters) long – about the size of a car.

Side view of Three Generations of Mars Rovers
Front; flight spare for the first Mars rover, Sojourner. Left; Mars Exploration Rover Project test rover. Right; Mars Science Laboratory test rover Credit: NASA/JPL-Caltech

With your own eyes you can see the rapid and huge generational change in Mars rovers if you have the opportunity to visit the Kennedy Space Center Visitor Complex and stroll by the Mars exhibit with full scale models of all three of NASA’s Red Planet rovers.

At the KSC Visitor Complex in Florida you can get within touching distance of the Martian Family of Rovers and the generational differences in size and complexity becomes personally obvious and impressive.

NASA’s Family of Mars rovers at the Kennedy Space Center
Full scale models on display at the Kennedy Space Center Visitor Complex. Curiosity and Spirit/Opportunity are pictured here. Sojourner out of view. Credit: Ken Kremer

All of the Mars rovers blasted off from launch pads on Cape Canaveral Air Force Station, Florida.

Sojourner, Spirit and Opportunity launched atop Delta II rockets at Space Launch Complex 17 in 1996 and 2003. Curiosity launched atop an Atlas V at Space Launch Complex 41 in 2011.

Three Generations of Mars Rovers with Standing Mars Engineers
The rovers are pictured here with real Mars Engineers to get a sense of size and perspective. Front rover is the flight spare for the first Mars rover, Sojourner. At left is a Mars Exploration Rover Project test rover, working sibling to Spirit and Opportunity. At right is a Mars Science Laboratory test rover the size of Curiosity which is targeting a August 2012 Mars landing. The Mars engineers are JPL's Matt Robinson, left, and Wesley Kuykendall. Credit: NASA/JPL-Caltech

Opportunity is still exploring Mars to this day – 8 years after landing on the Red Planet, with a warranty of merely 90 Martian days.

Curiosity is scheduled to touch down inside Gale crater on 6 August 2012.

So, what comes next ? Will there be a 4th Generation Mars rover ?

Stay tuned – only time and budgets will tell.

Rocks From Mars

DARRYL PITT, MACOVICH COLLECTION

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Scientists studying life on Mars got a late Christmas present this year: confirmation that meteorites found in Morocco in December are of Martian origin. It’s a significant discovery; Martian meteorites fall to Earth only about once every 50 years making this a once-in-a-lifetime, and for many a once-in-a-career, event. The Mars rocks are worth more than their weight in gold, but what they can tell us could be even more valuable. 

Astronomers suspect that the meteorite has been wandering around the solar system for millions of years, ever since something big smashed into the red planet and sent debris flying all directions. One of those pieces has wandered its way towards Earth and plunged through the atmosphere.

ALH 84001, the meteorite found in Antarctica in 1984. Evidence of fossilized life inside the rock sparked a search for life on Mars. Image credit: NASA/ JSC

This is only the fifth time scientists have chemically confirmed the Martian origin of meteorites. Rocks found in France in 1815, in India in 1865, in Egypt in 1911, and in Nigeria in 1962 have all been positively identified as being from Mars.

The chemical signature of the Moroccan rocks and the Martian air match said Tony Irving of the University of Washington who did the scientific analysis. But this discovery is different. The rocks weren’t just found, they were seen streaking through the sky in July 2011, which makes them extremely valuable.

These rocks have only had six months to accumulate Earth-based materials and traces of life; typically Martian meteorites found on Earth have been here anywhere from decades to millennia, giving them ample time to become tainted.

These new rocks, while still contaminated because they have been on Earth for months, are relatively pure. “It’s incredibly fresh. It’s highly valuable for that reason,” said Carl Agee, director of the Institute of Meteoritics and curator at the University of New Mexico.

It’s also a rare find. This new sample, about 15 pounds of rocks, brings the total weight of all Martian samples on Earth to just 240 pounds.

Meteorite dealer Darryl Pitt is cashing in on the rocks’ rarity and selling pieces for $11,000 to $22,500 an ounce and has sold most of his supply already. At that price, the Martian meteorite costs about 10 times as much as gold.

An artist's conception of early Mars being hit by an asteroid wider than Texas. Scientists believe the impact melted the planet's crust in its northern hemisphere, flung crust into space, and sent shock wave through the planet's molten core (inset). This explains why Mars' crust is thinner in the northern hemisphere, according to three new studies. Image courtesy Jeff Andrews-Hanna; inset courtesy Francis Nimmo.

Cornell University astronomer Steve Squyres, the principal investigator for NASA’s Mars Exploration Rover Program, is less excited. The rocks, he said, are not the kind scientists are most hoping for. They are hard, igneous or volcanic rock. A softer kind of rock capable of holding water or life would be better. But he also points that these rocks aren’t likely to come streaking through the atmosphere. Any soft rock would be unlikely to survive the fiery entry through Earth’s atmosphere.

Former NASA sciences chief Alan Stern, director of the Florida Space Institute at the University of Central Florida, takes a brighter outlook. “It’s nice to have Mars sending samples to Earth,” he said, “particularly when our pockets are too empty to go get them ourselves.”

Until we manage a sample return mission from Mars, this is the best shot scientists have to study the red planet up close.

Source: physorg.

 

India has Red Planet Fever

Image credit: NASA/

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Mars fever has gripped India. In a recent report from the Planetary Science and Exploration conference that was held in December 2011, scientists from the Indian Space Research Organization (ISRO) are making preliminary plans for a robotic mission to the Red Planet sometime next year. 

The possibility of an Indian mission to Mars first came up during a brainstorming session at the Physical Research Laboratory (PRL), an affiliate of the ISRO, last March. For two days, scientists and students developed their plans and proposals for a mission to the red planet.

A Mars Mission Study Team has been established to review proposed scenarios for the future mission, and an Indian chapter of the Mars Society formed last year at IIT-Mumbai.

Viking 2's view of Mars in 1976. Image credit: NASA/courtesy of nasaimages.org

The report from the meeting last month gives a concrete look at what Indian scientists have on their Martian wish list. In all, ten instruments and experiments comprise the ultimate mission.

En route to Mars, a Mars Radiation Spectrometer (Maris) will measure and characterize background levels of charged particles in interplanetary space. This data will play a vital role in determining radiation levels facing humans going to Mars.

Once at Mars, the proposed Indian mission will focus on the Martian atmosphere.

A Probe For Infrared Spectroscopy for Mars (Prism) is designed to study the spatial and seasonal variations of atmospheric gases on Mars’ atmosphere throughout the mission’s lifetime. The Mars Exospheric Neutral Composition Analyzer (Menca) is designed to analyze the planet’s upper atmosphere-exosphere, the region roughly 400 km (248 miles) above the surface.

Specific instruments are designed to study the composition of the atmosphere. A Methane Sensor For Mars (MSM) has been proposed to detect traces of the gas in the atmosphere. Another instrument, Tis, will measure thermal emissions to help scientists generate a map reflecting the composition and mineralogy of the planet. It will also help the team monitor carbon dioxide levels.

A Plasma and Current Experiment (Pace) will assess the escape rate of the atmosphere and the structure of the “tail” this escaping atmosphere creates. Radio and microwave instruments will also be on board the spacecraft to measure the planet’s surface activity. A suite of instruments will also be on hand to detect plasma waves in the atmosphere.

Mars's atmosphere is only 1 percent as thick as Earth's. Image credit: NASA

Visual measurements are also part of the proposed mission. The Mars Color Camera (MCC) is designed to photograph the Martian surface from a highly elliptical orbit, roughly 500 km by 80,000 km (310 miles by 49,700 miles). The camera will be able to take high resolution images of the topography of the surface and map the polar caps, both of which are expected to help scientists understand surface events like dust storms.

According to ISRO scientists, the proposed mission could launch as early as November 2013, which would have the spacecraft enter into orbit around Mars in September 2014. A launch so relatively soon is appealing to many Indian scientists, many of whom argue that a mission to Mars should take priority over a mission to the Moon.

After all, India has already reached the Moon with the successful Chandrayaan-2 spacecraft. Why not keep the momentum going and aim for a new and exciting target with the next mission?

Source: Asian Scientist

Doomed Phobos-Grunt Mars Mission Destructively Plunges to Earth

Phobos-Grunt plunged to Earth into the Pacific Ocean on Jan 15, 2012 - Crash Zone Map shows orbital track of Phobos-Grunt on Final Orbit before crashing to Earth in the Pacific Ocean west of South America on Jan 15, 2012.

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Story and Crash Zone Map updated 1 p.m. EST Jan 16

Today (Jan. 15) was the last day of life for Russia’s ambitious Phobos-Grunt mission to Mars after a desperate two month race against time and all out attempts to save the daring spaceship by firing up a malfunctioning thruster essential to putting the stranded probe on a trajectory to the Red Planet, failed.

According to the Russian news agency Ria Novosti, the doomed Phobos-Grunt spacecraft apparently plunged into the southern Pacific Ocean today, (Jan. 15) at about 12:45 p.m. EST, 21:45 Moscow time [17:45 GMT] after a fiery re-entry into the Earth’s atmosphere.

“Phobos-Grunt fragments have crashed down in the Pacific Ocean,” Russia’s Defense Ministry official Alexei Zolotukhin told RIA Novosti. He added that the fragments fell 1,250 kilometers to the west of the Chilean island of Wellington.

Universe Today will monitor the developing situation and update this story as warranted. On Jan. 16 Roscosmos confirmed the demise of Phobos-Grunt at 12:45 p.m. EST in the Pacific Ocean – during its last orbit; #1097.

Artist’s concept of Phobos-Grunt re-entry and breakup in the Earth’s atmosphere on Jan 15, 2012

The demise of the Phobos-Grunt spacecraft was expected sometime today, (Jan 15) after a fiery and destructive fall back to Earth, said Roscosmos, the Russian Federal Space Agency, in an official statement released early today before the crash.

Since the re-entry was uncontrolled, the exact time and location could not be precisely calculated beforehand.

Mission Poster for the Russian Phobos-Grunt soil sample return spacecraft that launched to Mars and its moon Phobos on 9 November 2011. The mission did not depart Earth orbit when the upper stage engines failed to ignite. Credit: Roskosmos ( Russian Federal Space Agency)/IKI

The actual crash time of the 13,500 kg space probe was slightly earlier than predicted.

Roscosmos head Vladimir Popovkin had previously stated that perhaps 20 to 30 fragments weighing perhaps 400 pounds (180 kg) might survive and would fall harmlessly to Earth.

The spacecraft burst into a large quantity of pieces as it hit the atmosphere, heated up and broke apart. But the actual outcome of any possible fragments is not known at this time.

Shortly after launching from the Baikonur Cosmodrome on Nov. 9, 2011, the probe became stuck in low Earth orbit after its MDU upper stage engines repeatedly failed to ignite and send the ship on a bold sample return mission to the tiny Martian Moon Phobos.

Phobos-Grunt was loaded with over 11,000 kg of toxic propellants, including dimethylhydrazine and dinitrogen tetroxide, that went unused due to the thruster malfunction and that were expected to be incinerated during the plunge to Earth.

Frictional drag forces from the Earth’s atmosphere had gradually lowered the ship’s orbit in the past two months to the point of no return after all attempts to fire the thrusters and raise the orbit utterly failed.

The audacious goal of Phobos-Grunt was to carry out history’s first ever landing on Phobos, retrieve 200 grams of soil and bring the treasured samples back to Earth for high powered analysis that could help unlock secrets to the formation of Mars, Phobos and the Solar System.

Phobos-Grunt spacecraft being encapsulated inside the nose cone by technicians at the Baikonur Cosmodrome prior to Nov. 9, 2011 blastoff. Credit: Roscosmos

The Holy Grail of planetary science is to retrieve Martian soil samples – and scientists speculated that bits of the Red Planet could be intermixed with the soil of its mini moon Phobos, barely 15 miles in diameter.

The science return from Phobos-Grunt would have been first rate and outstanding.

It’s a sad end to Russia’s attempts to restart their long dormant interplanetary space science program.

The $165 mission was Russia’s first Mars launch in more than 15 years.

Radar image of the Russian Mars orbiter Phobos-Grunt, created with the TIRA space observation radar by researchers at the Fraunhofer Institute in Germany. One can clearly see the extended solar panels (centre) and the tank ring (bottom)
Credit: Fraunhofer FHR
Click to enlarge

Roscosmos had stated that the Atlantic Ocean – to the west of Africa – was at the center of the predicted crash zone. But nothing was certain and the probe had the possibility to crash sooner, perhaps over the Pacific Ocean or South America or later over Africa, Europe or Russia.

Roscosmos had predicted the time of the plunge to Earth to be from 12:50 p.m. EST and 1:34 p.m. EST (1750 to 1834 GMT) or 21:50 to 22: 34 Moscow time on January 15. The last orbit carried the probe over the Pacific Ocean towards South America on a northeasterly heading.

Russia enlisted assistance from ESA and the US in a bid to establish contact with the probe to reorient itself and fire up its engines for a belated journey to the Red Planet. Other than extremely brief signals the efforts proved futile and today’s Pacific plunge is the unfortunate end result.

Hopefully the Russians will not give up in despair, but rather fix the flaws and launch an exciting new Mars mission.

NASA has had better luck with their Mars mission this season.

The Curiosity Mars Science Lab rover is precisely on course to the Red Planet following the Jan 11 firing of the cruise stage thrusters for the first of up to 6 Trajectory Correction Maneuvers – read the details here

Phobos-Grunt imaged while flying over Holland on Dec 28, 2011 by astrophotographer Ralf Vandebergh. Solar panels are deployed. Credit: Ralf Vandebergh

Read Complete Coverage about Phobos-Grunt, Curiosity and the Mars Rovers by Ken Kremer here:
Crucial Rocket Firing Puts Curiosity on Course for Martian Crater Touchdown
8 Years of Spirit on Mars – Pushing as Hard as We Can and Beyond !
2011: Top Stories from the Best Year Ever for NASA Planetary Science!
Opportunity Discovers Most Powerful Evidence Yet for Martian Liquid Water
Curiosity Starts First Science on Mars Sojurn – How Lethal is Space Radiation to Life’s Survival

Russians Race to Save Ambitious Phobos-Grunt Mars Probe from Earthly Demise
Russia’s Bold Sample Return Mission to Mars and Phobos Blasts Off
Russian Mars Moon Sample Probe Poised to Soar atop Upgraded Rocket – Video
Awesome Action Animation Depicts Russia’s Bold Robot Retriever to Mars moon Phobos
Phobos-Grunt and Yinghuo-1 Encapsulated for Voyage to Mars and Phobos
Phobos and Jupiter Conjunction in 3 D and Amazing Animation – Blastoff to Martian Moon near
Russia Fuels Phobos-Grunt and sets Mars Launch for November 9
Phobos-Grunt and Yinghou-1 Arrive at Baikonur Launch Site to tight Mars Deadline
Phobos-Grunt: The Mission Poster
Daring Russian Sample Return mission to Martian Moon Phobos aims for November Liftoff

Scientists Still Searching for the Beagle 2 Crash Site on Mars

An image from the HiRISE camera of the Isidis basin region where the Beagle 2 lander was supposed to touch down. Credit: NASA/JPL/University of Arizona

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Since its disappearance in December 2003, scientists and citizen scientists alike have continued the search for Europe’s Beagle 2 lander which likely crashed on Mars. Its disappearance is a mystery and if the spacecraft could be located, it might be possible to discover what went wrong.

The Mars Reconnaissance Orbiter’s powerful HiRISE camera has been regularly taking high-resolution images of the Isidis basin region where the Beagle 2 lander was supposed to touch down.

“Nothing resembling the Beagle lander has been seen in any of the HiRISE images, although we aren’t sure that they’ve been thoroughly searched,” said HiRISE Principal Investigator Alfred McEwen, writing on the HiRISE website.

So, join in the search and take a look!

Above is the 12th such image taken by HiRISE.

McEwen said the easiest thing to spot would be the bright parachute — if it actually deployed. Remember how HiRISE was able to find the parachutes at the MER landing sites, and even capture the Phoenix lander descending on its parachute? The Beagle 2’s parachute would be a good clue to search for.

(As we reported earlier, the HiRISE team will attempt to image the Mars Science Laboratory during its descent to Mars’ surface in August, as it did for Phoenix.)

Dust should not be a problem as far as hiding the lander or parachutes, McEwen said. “Dust deposition over the past eight years probably would not disguise the bright feature over equatorial regions of Mars,” he said noting that the parachutes are still easy to spot at the MER and Pathfinder landing sites. “At high latitudes the brightness patterns are reset each winter by the seasonal deposits of carbon-dioxide and dust, as seen at the Phoenix landing site.”

All contact with Beagle 2 was lost after its separation from the Mars Express spacecraft, just six days before atmospheric entry. McEwen said the lack of telemetry on its way to the surface means there is little information about where the spacecraft may have landed on the surface, but searching in the region where it was expected to land is a good place to start.

You can download high-resolution version of this images here.

For an idea of what the Beagle 2 hardware might look like, see this web page.

Crucial Rocket Firing Puts Curiosity on Course for Martian Crater Touchdown

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NASA’s car-sized Curiosity Mars Science Lab (MSL) rover is now on course to touch down inside a crater on Mars in August following the completion of the biggest and most crucial firing of her 8.5 month interplanetary journey from Earth to the Red Planet.

Engineers successfully commanded an array of thrusters on MSL’s solar powered cruise stage to carry out a 3 hour long series of more than 200 bursts last night (Jan. 11) that changed the spacecraft’s trajectory by about 25,000 miles (40,000 kilometers) – an absolute necessity that actually put the $2.5 Billion probe on a path to Mars to “Search for Signatures of Life !”

“We’ve completed a big step toward our encounter with Mars,” said Brian Portock of NASA’s Jet Propulsion Laboratory (JPL), Pasadena, Calif., deputy mission manager for the cruise phase of the mission. “The telemetry from the spacecraft and the Doppler data show that the maneuver was completed as planned.”

Mars Science Lab and cruise stage separate from Centaur upper stage just minutes after Nov. 26, 2011 launch. Thrusters on cruise stage performed course correction on Jan. 11, 2012. Up to 6 firings total will put the NASA robot on precision course to Mars.
Credit: NASA TV

This was the first of six possible TCM’s or trajectory correction maneuvers that may be required to fine-tune the voyage to Mars.

Until now, Curiosity was actually on a path to intentionally miss Mars. Since the Nov. 26, 2011 blastoff from Florida, the spacecraft’s trajectory was tracking a course diverted slightly away from the planet in order to prevent the upper stage – trailing behind – from crashing into the Red Planet.

The upper stage was not decontaminated to prevent it from infecting Mars with Earthly microbes. So, it will now sail harmlessly past the planet as Curiosity dives into the Martian atmosphere on August 6, 2012.

The thruster maneuver also served a second purpose, which was to advance the time of the Mars encounter by about 14 hours. The TCM burn increased the velocity by about 12.3 MPH (5.5 meters per second) as the vehicle was spinning at 2 rpm.

“The timing of the encounter is important for arriving at Mars just when the planet’s rotation puts Gale Crater in the right place,” said JPL’s Tomas Martin-Mur, chief navigator for the mission.


Video caption: Rob Manning, Curiosity Mars Science Lab Chief Engineer at NASA JPL describes the Jan. 11, 2012 thruster firing that put the robot on a precise trajectory to Gale Crater on Mars. Credit: NASA/JPL

As of today, Jan. 12, the spacecraft has traveled 81 million miles (131 million kilometers) of its 352-million-mile (567-million-kilometer) flight to Mars. It is moving at about 10,300 mph (16,600 kilometers per hour) relative to Earth, and at about 68,700 mph (110,500 kilometers per hour) relative to the Sun.

The next trajectory correction maneuver is tentatively scheduled for March 26, 2012.

Curiosity rover launches to Mars atop Atlas V rocket on Nov. 26, 2011 from Cape Canaveral, Florida. Credit: Ken Kremer

The goal of the 1 ton Curiosity rover is to investigate whether the layered terrain inside Gale Crater ever offered environmental conditions favorable for supporting Martian microbial life in the past or present and if it preserved clues about whether life ever existed.

Curiosity will search for the ingredients of life, most notably organic molecules – the carbon based molecules which are the building blocks of life as we know it. The robot is packed to the gills with 10 state of the art science instruments including a 7 foot long robotic arm, scoop, drill and laser rock zapper.

Curiosity’s Roadmap through the Solar System-From Earth to Mars
Schematic shows 8.5 month interplanetary trajectory of Curiosity. Credit: NASA/JPL-Caltech

Curiosity Countdown – 205 days to go until Curiosity lands at Gale Crater on Mars !

January 2012 marks the 8th anniversary of the landings of NASA’s Spirit and Opportunity Mars rovers back in January 2004.

Opportunity continues to operate to this day. Read my salute to Spirit here

Read continuing features about Curiosity and Mars rovers by Ken Kremer starting here:
8 Years of Spirit on Mars – Pushing as Hard as We Can and Beyond !
2011: Top Stories from the Best Year Ever for NASA Planetary Science!
Opportunity Discovers Most Powerful Evidence Yet for Martian Liquid Water
Flawlessly On Course Curiosity Cruising to Mars – No Burn Needed Now
NASA Planetary Science Trio Honored as ‘Best of What’s New’ in 2011- Curiosity/Dawn/MESSENGER
Curiosity Mars Rover Launch Gallery – Photos and Videos
Curiosity Majestically Blasts off on ‘Mars Trek’ to ascertain ‘Are We Alone?
Mars Trek – Curiosity Poised to Search for Signs of Life