Rover Driver Scott Maxwell with a model of MER. Photo courtesy Scott Maxwell
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How often have you wanted to be a fly on the wall during media interviews of top scientists and engineers? Here’s your chance! On Friday, February 10, we’ll be having our first live interview via a Google+ Hangout On Air. We’ve done the weekly Space Hangout for several weeks now and Fraser has done multiple virtual star parties via a Hangout On Air. Now we’ll start the first of what we hope are many live interviews that we’ll share with our readers and fans. We’re excited that Mars rover driver Scott Maxwell, will be joining us, and he will provide insight on the plans for the Opportunity rover’s upcoming winter, a look back at the 8 years and counting for the rovers, a look ahead to the future, and more.
The Hangout On Air will start at 18:00 UTC (1 pm EST,12 noon CST, 10 am PST) or you can check here at the fancy-schmancy time and date announcement Scott put together that shows the time in almost every time zone possible.
How do you find the Hangout? The best way is to join Google+ and “circle” Fraser and the Hangout On Air will show up in his timeline. You can also circle Nancy, who will also provide a link, but within Fraser’s timeline there will also be the opportunity for you to post questions that we can ask Scott during the live interview.
If you can’t watch live, the Hangout will be recorded and we’ll post it later on Friday on Universe Today.
An astronaut once told me that fellow space flier Don Pettit could fix anything with a paper clip. Indeed, Pettit has nicknames like Mr. Wizard and Mr. Fixit, and he is well-known for his Saturday Morning Science videos during his first stay on the International Space Station and his “Zero G Coffee Cup” from a space shuttle mission he was on in 2008. Now in his second long-duration stint on the ISS, Pettit has a new video series called “Science off the Sphere” and the first video is above. Pettit uses “knittin” needles (watch the video to hear Pettit’s pronunciation) and water droplets to demonstrate physics in space, and shows what fun astronauts can have with water in zero-G with his ‘dancing’ water droplets.
This new video series is partnership between NASA and the American Physical Society. But there’s more than just videos, as at the end of each video Pettit poses a challenge question. Submit your answers at the Science Off the Sphere website for a chance to have your name read from space and receive a snazzy t-shirt from Earth.
Visualization of the GPM Core Observatory and Partner Satellites. Credit: NASA
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An international plan is unfolding that will launch satellites into orbit to study global snowfall precipitation with unprecedented detail. With the upcoming Global Precipitation Measurement (GPM) satellites, for the first time we will know when, where and how much snow falls on Earth, allowing greater understanding of energy cycles and how best to predict extreme weather.
Snow is more than just a pretty winter decoration… it’s also a very important contributor to fresh water supply in many regions around the world, especially those areas that rely on spring runoff from mountains.
The snowmelt from the Sierra Nevadas, for example, accounts for a third of the water supply for California.
But changing climate and recent drought conditions have affected how much snow the mountains receive in winter… and thus how much water is released in the spring. Unfortunately, as of now there’s no reliable way to comprehensively detect and measure falling snow from space… whether in the Sierras or the Andes or the Alps.
Engineers are building and testing the GPM Core Observatory at Goddard Space Flight Center. (NASA/GSFC)
The GPM Core satellite, slated to launch in 2014, will change that.
“The GPM Core, with its ability to detect falling snows, it’s one of the very first times that we’ve put sensors in space to specifically look at falling snow,” said GPM Deputy Project Scientist Gail Skofronick-Jackson in an online video. “We’re at that edge where rain was fifty years ago. We’re still figuring out how to measure snow.”
And why is snow such a difficult subject to study?
“Rain tends to be spherical like drops,” says Skofronick-Jackson. “But if you’ve ever been out in a snowfall and you’ve looked at your shirt, you see the snow comes in all different forms.”
Once GPM scientists calculate all the various types of snowflake shapes, the satellite will be able to detect them from orbit.
“The GPM Core, with its additional frequencies and information on the sensors, is going to be able to provide us for the first time a lot more information about falling snow than we’ve ever done before.”
Knowing where and how much snow and rain falls globally is vital to understanding how weather and climate impact both our environment and Earth’s energy cycles, including effects on agriculture, fresh water availability, and responses to natural disasters.
Snowfall is a missing part of the puzzle, and GPM will fill those pieces in.
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.
Ebb and Flow - New Names for the GRAIL Twins in Lunar Orbit. 4th Grade Students from Montana win NASA’s contest to rename the GRAIL A and GRAIL B spacecraft. Artist concept of twin GRAIL spacecraft flying in tandem orbits around the Moon to measure its gravity field in unprecedented detail and unravel the hidden mysteries of the lunar interior’s composition. Credit: NASA/JPL Montage:Ken Kremer
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A classroom of America’s Youth from an elementary school in Bozeman, Montana submitted the stellar winning entry in NASA’s nationwide student essay contest to rename the twin GRAIL lunar probes that just achieved orbit around our Moon on New Year’s Eve and New Year’s Day 2012
“Ebb” & “Flow” – are the dynamic duo’s official new names and were selected because they clearly illuminate the science goals of the gravity mapping spacecraft and how the Moon’s influence mightily affects Earth every day in a manner that’s easy for everyone to understand.
“The 28 students of Nina DiMauro’s class at the Emily Dickinson Elementary School have really hit the nail on the head,” said GRAIL principal investigator Prof. Maria Zuber of the Massachusetts Institute of Technology in Cambridge, Mass.
“We asked the youth of America to assist us in getting better names.”
“We chose Ebb and Flow because it’s the daily example of how the Moon’s gravity is working on the Earth,” said Zuber during a media briefing held today (Jan. 17) at NASA Headquarters in Washington, D.C. The terms ebb and flow refer to the movement of the tides on Earth due to the gravitational pull from the Moon.
“We were really impressed that the students drew their inspiration by researching GRAIL and its goal of measuring gravity. Ebb and Flow truly capture the spirit and excitement of our mission.”
Leland Melvin, NASA Associate Administrator for Education, left, Maria Zuber, GRAIL Prinicipal Investigator at the Massachusetts Institute of Technology, and James Green, Director of the Planetary Science Division in the Science Mission Directorate at NASA Headquarters, right, applaud students from Emily Dickinson Elementary School in Bozeman, Mont. during a news conference, Tuesday, Jan. 17, 2012, at NASA Headquarters in Washington. Nine hundred classrooms and more than 11,000 students from 45 states, as well as Puerto Rico and the District of Columbia, participated in a contest that began in October 2011 to name the twin lunar probes. Credit: NASA/Paul E. Alers
Ebb and Flow are flying in tandem around Earth’s only natural satellite, the first time such a feat has ever been attempted.
As they fly over mountains, craters and basins on the Moon, the spaceships will move back and forth in orbit in an “ebb and flow” like response to the changing lunar gravity field and transmit radio signals to precisely measure the variations to within 1 micron, the width of a red blood cell.
The breakthrough science expected from the mirror image twins will provide unprecedented insight into what lurks mysteriously hidden beneath the surface of our nearest neighbor and deep into the interior.
The winning names from the 4th Graders of Emily Dickinson Elementary School were chosen from essays submitted by nearly 900 classrooms across America with over 11,000 students from 45 states, Puerto Rico and the District of Columbia, Zuber explained.
The students themselves announced “Ebb” and “Flow” in a dramaric live broadcast televised on NASA TV via Skype.
“We are so thrilled that our names were chosen and excited to share this with you. We can’t believe we won! We are so honored. Thank you!” said Ms. DiMauro as the very enthusiastic students spelled out the names by holding up the individual letters one-by-one on big placards from their classroom desks in Montana.
Watch the 4th Grade Kids spell the names in this video!
Until now the pair of probes went by the rather uninspiring monikers of GRAIL “A” and “B”. GRAIL stands for Gravity Recovery And Interior Laboratory.
The twin crafts’ new names were selected jointly by Prof. Zuber and Dr. Sally Ride, America’s first woman astronaut, and announced during today’s NASA briefing.
NASA’s naming competition was open to K-12 students who submitted pairs of names and a short essay to justified their suggestions.
“Ebb” and “Flow” (GRAIL A and GRAIL B) are the size of washing machines and were launched side by side atop a Delta II booster rocket on September 10, 2011 from Cape Canaveral, Florida.
They followed a circuitous 3.5 month low energy path to the Moon to minimize the fuel requirements and overall costs.
So far the probes have completed three burns of their main engines aimed at lowering and circularizing their initial highly elliptical orbits. The orbital period has also been reduced from 11.5 hours to just under 4 hours as of today.
“The science phase begins in early March,” said Zuber. At that time the twins will be flying in tandem at 55 kilometers (34 miles) altitude.
The GRAIL twins are also equipped with a very special camera dubbed MoonKAM (Moon Knowledge Acquired by Middle school students) whose purpose is to inspire kids to study science.
“GRAIL is NASA’s first planetary spacecraft mission carrying instruments entirely dedicated to education and public outreach,” explained Sally Ride. “Over 2100 classrooms have signed up so far to participate.”
Thousands of middle school students in grades five through eight will select target areas on the lunar surface and send requests for study to the GRAIL MoonKAM Mission Operations Center in San Diego which is managed by Dr. Ride in collaboration with undergraduate students at the University of California in San Diego.
By having their names selected, the 4th graders from Emily Dickinson Elementary have also won the prize to choose the first target on the Moon to photograph with the MoonKam cameras, said Ride.
Zuber notes that the first MoonKAM images will be snapped shortly after the 82 day science phase begins on March 8.
Ebb & Flow Achieve Lunar Orbit on New Year’s Weekend 2012
NASA’s twin GRAIL-A & GRAIL-B spacecraft are orbiting the Moon in this astrophoto taken on Jan. 2, 2012 shortly after successful Lunar Orbit Insertions on New Year’s Eve and New Year’s Day 2012.
Credit: Ken Kremer
Wrinkle ridges, like this one in the northern part of Mare Imbrium, were studied using telescopic observations, as early as the 1880's. Data from the Apollo era refined our understanding of these interesting features. More recently, data from the Lunar Reconnaissance Orbiter Camera is calling that understanding into question. Image credit: NASA/GSFC/Arizona State University and the author Click on the image to explore the LROC data from this area in greater detail
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Wrinkle ridges have been seen on the surface of the Moon for over a century. Studies of these interesting features began as early as 1885, with telescopic photographs, and continued beyond the Apollo era, with satellite and lander observations. Scientists thought they understood them, but the latest images from the Lunar Reconnaissance Orbital Camera (LROC) suggest we may not know the whole story.
By definition, wrinkle ridges are narrow, steep-sided ridges that form predominantly in volcanic regions. They are very complex features, which can be either straight or curved, or even be braided and zig-zagged. Their width can be anything from less than 1 km to over 20 km. And their heights range from a few meters (say the height of an average room) to 300 meters (about the height of a 100-story sky scraper). They are also asymmetric, with one side of the ridge being higher than the other. Often, these things sit on top of a gentle swell in the landscape. Features like this have been found on a number of planets throughout the Solar System, including the Moon, Mars, Mercury, and Venus.
Wrinkle ridges, like this one in the northern part of Mare Imbrium, were studied using telescopic observations, as early as the 1880's. Data from the Apollo era refined our understanding of these interesting features. More recently, data from the Lunar Reconnaissance Orbiter Camera is calling that understanding into question.
Image credit: NASA/GSFC/Arizona State University and the author
Click on the image to explore the LROC data from this area in greater detail
The earliest researchers of lunar wrinkle ridges saw them through telescopes. When looking at the terminator (the line between the dark side and the lit side of the Moon), the angle of the Sun causes spectacular shadows to highlight the topography, allowing these otherwise subtle features to be seen. Scientists in the late 19th century believed that these wrinkle ridges, which were found predominantly in the volcanic mare regions, formed when the cooling magma shrank. The chilled crust at the very top of this magma body was now too large, and wrinkles had to form to accommodate the difference. This process was often compared to the wrinkled skin of a shriveled apple, or the skin on our hands as we age.
The dawn of the space age introduced orbiting satellites, which circled the Moon collecting images that were more detailed than had been possible ever before. Data from the 1960’s the Lunar Orbiter (LO) program, whose mission was to photograph the Moon in preparation for the Apollo missions, showed many more of these wrinkle ridge features.
Some researchers felt the LO data pointed to a volcanic origin for wrinkle ridges. They saw lava flows emanating from the wrinkle ridges and embaying impact craters. They suggested that lava flowed to the surface along linear fractures that exploited zones of weakness in the lunar crust (presumably, these weaknesses formed when impacts created the basins that lunar mare occupy). Lava that extruded onto the surface formed the wrinkle ridge features, while magma that intruded below the surface formed the regional swell the ridges sit on.
The Apollo missions, however, were able to provide information about what was happening below the surface, with the Apollo Lunar Sounder Experiment (ALSE). Data collected over a wrinkle ridge in the southeastern portion of Mare Serenitatis showed that there was some kind of topographic structure beneath the thin mare layers in this area. This suggested that wrinkle ridges were the surface expressions of thrust faults in the underlying crust. This interpretation was appealing because it explained why some wrinkle ridges are found outside of mare areas.
Wrinkle ridges are generally steep-sided, asymmetric structures, displaying complex braiding or zig-zag patterns. This wrinkle ridge, in the northern mare of Tsiolkovskiy crater, is very different. Described as "bulging", it has a gently curved uniform shape. It is also much smaller than the wrinkle ridges seen before. This unusual wrinkle ridge suggests we may not understand the formation of these features as well as we thought.
Image credit: NASA/GSFC/Arizona State University
Click on the image to learn more about this discovery from NASA's LROC team.
Later, studies of wrinkle-like features on Earth refined our understanding of how these features form. Now the thinking is that wrinkle ridges form by tectonic buckling of the mare areas and their surroundings. When mare lavas are extruded on the surface of the Moon, they fill up the impact basins in a series of basalt layers. The thinned crust left by the basin-forming process can’t support the weight of the mare, so the entire structure sags. The mare layer can become decoupled from the underlying regolith (the “soil” layer that impacts created between the time the basin was formed and when the first mare lavas extruded) and slide towards the sagging centre. As it does so, it bunches up in places where the decoupling is not complete. This creates a series of thrust faults at the base of the mare layer, which show up as wrinkle ridges at the surface. This decoupling process is more pronounced for thinner mare layers, which explains why we often see wrinkle ridges at the edges of a mare.
Recent findings from the Lunar Reconnaissance Orbiter Camera (LROC) may challenge this current understanding of wrinkle ridge formation. LROC images from the mare in Tsiolkovskiy crater have identified wrinkle ridges that are considerably different from the ones seen before. For one, these wrinkle ridges are not asymmetrical in profile, but have a uniformly curved shape. Also, they are much smaller, measuring less than 100 meters in width, as opposed to the 1-20 km widths seen for other wrinkle ridges.
It remains to be seen if these new wrinkle ridges will again change our understanding of how these enigmatic features form. The discovery of these particular ridges is so new that there is nothing yet published about them! Perhaps this image and others like it will help us learn more about these enigmatic features and answer questions such as: does this new wrinkle ridge represent the beginnings of their formation process and that all such ridges started out so small and symmetrical? Or maybe we’ll find that they are extrusions of particularly viscous lava, which have barely protruded above the surface along a linear fault.
Scientists plan to target this area for further data acquisition, because only more data from LRO and further research will help solve the mysteries of the wrinkled Moon.
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
Spirit Mars rover - view from Husband Hill summit. Spirit snapped this view self portrait from the summit of Husband Hill inside Gusev crater on Sol 618 on 28 September 2005. The rovers were never designed or intended to climb mountains. It took more than 1 year for Spirit to scale the Martian mountain. This image was created by an international team of astronomy enthusiasts and appeared on the cover of the 14 November 2005 issue of Aviation Week & Space Technology magazine and the April 2006 issue of Spaceflight magazine. Also selected by Astronomy Picture of the Day (APOD) on 28 November 2005. Credit: Marco Di Lorenzo, Douglas Ellison, Bernhard Braun and Kenneth Kremer. NASA/JPL/Cornell/Aviation Week & Space Technology
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January 2012 marks the 8th anniversary since of the daring landing’s of “Spirit” and “Opportunity” – NASA’s now legendary twin Mars Exploration Rovers (MER), on opposite sides of the Red Planet in January 2004. They proved that early Mars was warm and wet – a key finding in the search for habitats conducive to life beyond Earth.
I asked the leaders of the MER team to share some thoughts celebrating this mind-boggling milestone of “8 Years on Mars” and the legacy of the rovers for the readers of Universe Today. This story focuses on Spirit, first of the trailblazing twin robots, which touched down inside Gusev Crater on Jan. 3, 2004. Opportunity set down three weeks later on the smooth hematite plains of Meridiani Planum.
“Every Sol is a gift. We push the rovers as hard as we can,” Prof. Steve Squyres informed Universe Today for this article commemorating Spirit’s landing. Squyres, of Cornell University, is the Scientific Principal Investigator for the MER mission.
“I seriously thought both Spirit and Opportunity would be finished by the summer of 2004,” Ray Arvidson told Universe Today. Arvidson, of Washington University in St. Louis, is the deputy principal investigator for the MER rovers.
'Calypso' Panorama of Spirit's View from 'Troy'
This full-circle view from the panoramic camera (Pancam) on NASA's Mars Exploration Rover Spirit shows the terrain surrounding the location called "Troy," where Spirit became embedded in soft soil during the spring of 2009. The hundreds of images combined into this view were taken beginning on the 1,906th Martian day (or sol) of Spirit's mission on Mars (May 14, 2009) and ending on Sol 1943 (June 20, 2009). Credit: NASA/JPL-Caltech/Cornell University
click to enlarge
Spirit endured for more than six years and Opportunity is still roving Mars today !
The dynamic robo duo were expected to last a mere three months, or 90 Martian days (sols). In reality, both robots enormously exceeded expectations and accumulated a vast bonus time of exploration and discovery in numerous extended mission phases.
Spirit survived three harsh Martian winters and only succumbed to the Antarctic-like temperatures when she unexpectedly became mired in an unseen sand trap driving beside an ancient volcanic feature named ‘Home Plate’ that prevented the solar arrays from generating life giving power to safeguard critical electronic and computor components.
Spirit was heading towards another pair of volcanic objects named von Braun and Goddard and came within just a few hundred feet when she died.
Everest Panorama from Husband Hill summit
It took Spirit three days, sols 620 to 622 (Oct. 1 to Oct. 3, 2005), to acquire all the images combined into this mosaic, called the "Everest Panorama". Credit: NASA/JPL-Caltech/Cornell University
Click to enlarge
“I never thought that we would still be planning sequences for Opportunity today and that we only lost Spirit because of her limited mobility and bad luck of breaking through crusty soil to get bogged down in loose sands,” said Arvidson
By the time of her last dispatch from Mars in March 2010, Spirit had triumphantly traversed the red planets terrain for more than six years of elapsed mission time – some 25 times beyond the three month “warranty” proclaimed by NASA as the mission began back in January 2004.
The "Columbia Hills" in Gusev Crater on Mars
Husband Hill is 3.1 kilometers distant. Spirit took this mosaic of images with the panoramic camera at the beginning of February, 2004, less than a month after landing on Mars. Image credit: NASA/JPL-Caltech/Cornell
“I am feeling pretty good as the MER rover anniversaries approach in that Spirit had an excellent run, helping us understand without a doubt that early Mars had magmatic and volcanic activity that was “wet”, Arvidson explained.
“Magmas interacted with ground water to produce explosive eruptions – at Home Plate, Goddard, von Braun – with volcanic constructs replete with steam vents and perhaps hydrothermal pools.”
Altogether, the six wheeled Spirit drove over 4.8 miles (7.7 kilometers) and the cameras snapped over 128,000 images. NASA hoped the rovers would drive about a quarter mile during the planned 90 Sol mission.
“Milestones like 8 years on Mars always make me look forward rather than looking back,” Squyres told me.
Carbonate-Containing Martian Rocks discovered by Spirit Mars Rover
Spirit collected data in late 2005 which confirmed that the Comanche outcrop contains magnesium iron carbonate, a mineral indicating the past environment was wet and non-acidic, possibly favorable to life. This view was captured during Sol 689 on Mars (Dec. 11, 2005). The find at Comanche is the first unambiguous evidence from either Spirit or Opportunity for a past Martian environment that may have been more favorable to life than the wet but acidic conditions indicated by the rovers' earlier finds. Credit: NASA/JPL-Caltech/Cornell University
Spirit became the first robotic emissary from humanity to climb a mountain beyond Earth, namely Husband Hill, a task for which she was not designed.
“No one expected the rovers to last so long,” said Rob Manning to Universe Today. Manning, of NASA’s Jet Propulsion laboratory, Pasadena, CA. was the Mars Rover Spacecraft System Engineering team lead for Entry, Descent and Landing (EDL)
“Spirit surmounted many obstacles, including summiting a formidable hill her designers never intended her to attempt.”
“Spirit, her designers, her builders, her testers, her handlers and I have a lot to be thankful for,” Manning told me.
After departing the Gusev crater landing pad, Spirit traversed over 2 miles to reach Husband Hill. In order to scale the hill, the team had to create a driving plan from scratch with no playbook because no one ever figured that such a mouthwatering opportunity to be offered.
Spirit Rover traverse map from Gusev Crater landing site to Home Plate: 2004 to 2011
It took over a year to ascend to the hill’s summit. But the team was richly rewarded with a science bonanza of evidence for flowing liquid water on ancient Mars.
Spirit then descended down the other side of the hill to reach the feature dubbed Home Plate where she now rests and where she found extensive evidence of deposits of nearly pure silica, explosive volcanism and hot springs all indicative of water on Mars billions of years ago.
“Spirit’s big scientific accomplishments are the silica deposits at Home Plate, the carbonates at Comanche, and all the evidence for hydrothermal systems and explosive volcanism, Squyres explained. “ What we’ve learned is that early Mars at Spirit’s site was a hot, violent place, with hot springs, steam vents, and volcanic explosions. It was extraordinarily different from the Mars of today.”
“We’ve still got a lot of exploring to do [with Opportunity], but we’re doing it with a vehicle that was designed for a 90-sol mission,” Squyres concluded. “That means that ever sol is a gift at this point, and we have to push the rover and ourselves as hard as we can.”
NASA concluded the last attempt to communicate with Spirit in a transmission on May 25, 2011.
Spirit Rover traverse map from Husband Hill to resting place at Home Plate: 2004 to 2011The Last View Ever from Spirit rover on Mars
Spirit’s last panorama from Gusev Crater was taken during February 2010 before her death from extremely low temperatures during her 4th Martian winter. Spirit was just 500 feet from her next science target - dubbed Von Braun – at center, with Columbia Hills as backdrop.
Mosaic Credit: Marco De Lorenzo/ Kenneth Kremer/ NASA/JPL/Cornell University
Mosaic featured on Astronomy Picture of the Day (APOD) on 30 May 2011 - http://apod.nasa.gov/apod/ap110530.html
Meanwhile, the Curiosity Mars Science Lab rover, NASA’s next Red Planet explorer, continues her interplanetary journey on course for a 6 August 2012 landing at Gale Crater.
Jan 11: Free Lecture by Ken Kremer at the Franklin Institute, Philadelphia, PA at 8 PM for the Rittenhouse Astronomical Society. Topic: Mars & Vesta in 3 D – Plus Search for Life & GRAIL
A mineral brought back to Earth by the first men on the Moon and long thought to be unique to the lunar surface has been found in Australian rocks more than one billion years old, scientists say. Image Credit: Birger Rasmussen
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When it comes to our natural human curiosity, we want to know if there’s something new out there… something we haven’t discovered yet. That’s why when lunar rock samples were returned, geologists were thrilled to find very specific minerals – armalcolite, pyroxferroite and tranquillityite – which belonged only to our Moon. However, over the years the first two were found here on Earth and tranquillityite was disclosed in specific meteorites. Named for Tranquility Base, site of the first Moon landing, tranquillityite was supposed to be the final hold-out… the last lunar unique mineral… until now.
Birger Rasmussen, paleontologist with Curtin University in Perth, and colleagues report in their Geology paper that they’ve uncovered tranquillityite in several remote locations in Western Australia. While the samples are incredibly small, about the width of a human hair and merely microns in length, their composition is undeniable. What’s more, tranquillityite may be a lot more common here on Earth than previously thought.
Rasmussen told the Sydney Morning Herald, “This was essentially the last mineral which was sort of uniquely lunar that had been found in the 70s from these samples returned from the Apollo mission.The mineral has since been found exclusively in returned lunar samples and lunar meteorites, with no terrestrial counterpart. We have now identified tranquillityite in six sites from Western Australia.”
Why has this remote mineral stayed hidden for so long? One major reason is its delicate structure. Composed of iron, silicon, oxygen, zirconium, titanium and a tiny bit of yttrium, a rare earth element, tranquillityite erodes at a rapid pace when exposed to natural environmental conditions. Another explanation is that tranquillityite can only form through a unique set of circumstance – through uranium decay. Rasmussen explains it’s evidence these minerals were ‘always’ located here on Earth and we share the same chemical processes as our satellite.
“This means that basically we have the same chemical phenomena on the Moon and on Earth.” says Rasmussen. And one of the reasons it has taken so long to be found is, “No one was looking hard enough.”
Image Credit: Birger RasmussenAnd exactly what does it take to locate it? More than a billion years old, the only sure way to identify tranquillityite is to subject it to a series of electron blasts. By exposing it to a high-energy accelerating electron beam, it produces spectra. From there “an elemental composition in combination with back-scattered electron (BSE) brightness and x-ray count rate information is converted into mineral phases.” According to Rasmussen’s paper, “Terrestrial tranquillityite commonly occurs as clusters of fox-red laths closely associated with baddeleyite and zirconolite in quartz and K-feldspar intergrowths in late-stage interstices between plagioclase and pyroxene.”
While it has no real economic value, terrestrial tranquillityite is another good reason mankind should try to preserve pristine regions such as the northeast Pilbara Region and the Eel Creek formation. Who knows what else we might find?
Take a good close look at the Moon today and consider this; Two new Moon’s just reached orbit.
NASA is ringing in the New Year with a double dose of champagne toasts celebrating the back to back triumphal insertions of a pair of tiny probes into tandem lunar orbits this weekend that seek to unravel the hidden mysteries lurking deep inside the Moon and figure out how the inner solar system formed eons ago.
Following closely on the heels of her twin sister, NASA’s GRAIL-B spacecraft ignited her main braking rockets precisely as planned on New Year’s Day (Jan.1) to go into a formation flying orbit around the Moon, chasing behind GRAIL-A which arrived on New Year’s Eve (Dec. 31).
“Now we have them both in orbit. What a great feeling!!!!” NASA manager Jim Green told Universe Today just minutes after the thruster firing was done. Green is NASA’s Director of Planetary Science and witnessed the events inside Mission Control at the Jet Propulsion Laboratory (JPL) in Pasadena, Ca.
“It’s the best New Year’s ever!!” Green gushed with glee.
GRAIL-B spacecraft entered Lunar Orbit on New Year’s Day 2012. Artist concept of GRAIL-B performing its lunar orbit insertion burn. Credit: NASA/JPL-Caltech
The new lunar arrivals of GRAIL-A and GRAIL-B capped a perfect year for NASA’s Planetary Science research in 2011.
“2011 began the Year of the Solar System – which is a Mars year (~670 Earth days long)… and includes Grail B insertion, Dawn leaving Vesta this summer … And the landing of MSL! ,” Green said.
NASA’s GRAIL-A & GRAIL-B are orbiting the Moon in this image taken on Jan. 2, 2012 after Lunar Orbit Insertions on New Year’s Weekend. Click to enlarge.
Credit: Ken Kremer
“Cheers in JPL mission control as everything is looking good for GRAIL-B. It’s going to be a great 2012!!” JPL tweeted shortly after confirming the burn successfully placed GRAIL-B into the desired elliptical orbit.
After years of hard work, GRAIL principal investigator Maria Zuber of MIT told Universe Today that she was very “relieved”, soon after hearing the good news at JPL Mission Control.
“Since GRAIL was originally selected I’ve believed this day would come,” Zuber told me shortly after the GRAIL-B engine firing was declared a success on New Year’s Day.
“But it’s difficult to convey just how relieved I am right now. Time for the Science Team to start their engines !”
Artist's concept depicts how the science instrument on the mirror image twin GRAIL spacecraft will send signals to each other to map the Moon's gravity and then transmit the data to Earth. Credit: NASA
At 2:43 p.m. PST (5:43 p.m. EST) on New Year’s Day, the main thruster aboard GRAIL-B automatically commenced firing to slow down the spacecraft’s approach speed by about 430 MPH (691 kph) and allow it to be captured into orbit by the Moon’s gravity. The preprogrammed maneuver lasted about 39 minutes and was nearly identical to the GRAIL-A firing 25 hours earlier.
The hydrazine fueled main thrusters placed the dynamic spacecraft duo into near-polar, highly elliptical orbits.
Over the next two months, engineers will trim the orbits of both spacecraft to a near-polar, near-circular formation flying orientation. Their altitudes will be lowered to about 34 miles (55 kilometers) and the orbital periods trimmed from their initial 11.5 hour duration to about two hours.
The science phase begins in March 2012. For 82 days, the mirror image GRAIL-A and GRAIL-B probes will be flying in tandem with an average separation of about 200 kilometers as the Moon rotates beneath.
“GRAIL is a Journey to the Center of the Moon,” Zuber explained at a media briefing. “It will use exceedingly precise measurements of gravity to reveal what the inside of the Moon is like.”
As one satellite follows the other, in the same orbit, they will perform high precision range-rate measurements to precisely measure the changing distance between each other to within 1 micron, the width of a red blood cell, using a Ka-band instrument.
When the first satellite goes over a higher mass concentration, or higher gravity, it will speed up slightly. And that will increase the distance. Then as the second satellite goes over, that distance will close again.
The data returned will be translated into gravitational field maps of the Moon that will help unravel information about the makeup of the Moon’s mysterious core and interior composition. GRAIL will gather three complete gravity maps over the three month mission.
“There have been many missions that have gone to the Moon, orbited the Moon, landed on the Moon, brought back samples of the Moon,” said Zuber. “But the missing piece of the puzzle in trying to understand the Moon is what the deep interior is like.”
“Is there a core? How did the core form? How did the interior convect? What are the impact basins on the near-side flooded with magma and give us this Man-in-the-Moon shape whereas the back side of the Moon doesn’t have any of this? These are all mysteries that despite the fact we’ve studied the Moon before, we don’t understand how that has happened. GRAIL is a mission that is going to tell us that.”
“We think the answer is locked in the interior,” Zuber elaborated.
How will the twins be oriented in orbit to gather the data ?
“The probes will be pointed at one another to make the highly precise measurements,” said GRAIL co-investigator Sami Asmar of JPL to Universe Today. “The concept has heritage from the US/German GRACE earth orbiting satellites which mapped Earth’s gravity field. GRACE required the use of GPS satellites for exactly knowing the position, but there is no GPS at the Moon. So GRAIL was altered to compensate for no GPS at the Moon.”
GRAIL will map the gravity field by 100 to 1000 times better than ever before.
“We will learn more about the interior of the Moon with GRAIL than all previous lunar missions combined,” says Ed Weiler, the recently retired NASA Associate Administrator of the Science Mission Directorate in Washington, DC.
The GRAIL twins blasted off from Florida mounted side by side atop a Delta II booster on September 10, 2011 and took a circuitous 3.5 month low energy path to the Moon to minimize the overall costs.
So when you next look at the sky tonight and in the coming weeks just imagine those mirror image GRAIL twins circling about seeeking to determine how we all came to be !
GRAIL Project manager David Lehman cuts the cake for team members at JPL to celebrate 2 for 2 at the Moon. Credit: NASA/Jim GreenGRAIL team at JPL toasts success as twin spacecraft both went into orbit around the Moon on New Year’s weekend.
