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Friday, January 29, 2016

JPL News - Day in Review

 

DAY IN REVIEW
Sandy Selfie Sent from NASA Mars Rover
The latest self-portrait from NASA's Curiosity Mars rover shows the car-size mobile laboratory beside a dark dune where it has been scooping and sieving samples of sand.
› Read the full story
New Animation Takes a Colorful Flight Over Ceres
A colorful new animation shows a simulated flight over the surface of dwarf planet Ceres, based on images from NASA's Dawn spacecraft.
› Read the full story
NASA Damage Maps May Help in Future Quakes
Researchers have developed a way to make maps of natural disaster damage using remote sensing technology.
› Read the full story

 



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Thursday, January 28, 2016

CANCELLED - January Educator Workshop - Space School Musical

 

 

CANCELLED - Space School Musical

When: Saturday, Jan. 30, 9:30 a.m. to 12:30 p.m. (cancelled)

Where: NASA Jet Propulsion Laboratory, Von Karman Auditorium, Pasadena, California

On behalf of the NASA/JPL Educator Resource Center, we wish to apologize for the cancellation of the upcoming Space School Musical Workshop on Saturday, January 30.   We are sorry for any inconvenience this may have caused and look forward to your participation in our upcoming workshops.

Call the Educator Resource Center at 818-393-5917 if you have any questions.

Discover more upcoming educator workshops and events from NASA/JPL Education.

 



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Wednesday, January 27, 2016

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
NASA Radar Brings a New View of World Heritage Site

In just two 10-minute overflights, an airborne NASA synthetic aperture radar proved it could pinpoint areas of disturbance in Peru's Nasca lines World Heritage Site. The data collected on the two flights will help Peruvian authorities fully catalog the thousand-year-old designs drawn on the ground in and around the site for the first time, as well as giving them a new tool for protecting the fragile constructions from both careless humans and natural disturbances such as floods.

The left frame shows a portion of the mesa-top site in a Google Earth image. Drainage gullies circle the mesa where the Nasca people constructed lines several miles long, enormous polygons, and animal figures simply by moving rocks. A shape called the Hummingbird is faintly visible above and to the left of the scale line, its long beak ending below a road that cuts diagonally from the right edge of the image to the center.

In the synthetic aperture radar image of the same site, right, areas of disturbance appear dark. There are extensive areas of disturbance around the Hummingbird as well as a pathway down the gully directly above the glyph. Other small disturbances may have been caused by erosion in the dry creek beds.

NASA's Uninhabited Aerial Vehicle Synthetic Aperture Radar (UAVSAR), developed and managed by the Jet Propulsion Laboratory, Pasadena, California, can record changes on the ground beneath the aircraft that occur between multiple flights, which take exactly the same flight path. The instrument is used to monitor how volcanoes, earthquakes, and other natural hazards are changing Earth. Principal investigator Bruce Chapman of JPL noted that UAVSAR is ideally suited for observing the Nasca site because the region has virtually no vegetation and receives no rainfall whatsoever in most years, meaning that natural disturbances are minimal.

This and other UAVSAR images of the site appear in a paper in the journal Conservation and Management of Archaeological Sites. Chapman's coauthors are Douglas Comer, Cultural Site Research and Management, Baltimore, Maryland; Johny Isla, Ministry of Culture, Peru; and Helaine Silverman, University of Illinois, Urbana-Champaign.

 



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Tuesday, January 26, 2016

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
Ceres: Keeping Well-Guarded Secrets for 215 Years

New Year's Day, 1801, the dawn of the 19th century, was a historic moment for astronomy, and for a space mission called Dawn more than 200 years later. That night, Giuseppe Piazzi pointed his telescope at the sky and observed a distant object that we now know as Ceres.

Today, NASA's Dawn mission allows us to see Ceres in exquisite detail. From the images Dawn has taken over the past year, we know Ceres is a heavily cratered body with diverse features on its surface that include a tall, cone-shaped mountain and more than 130 reflective patches of material that is likely salt. But on that fateful evening in 1801, Piazzi wasn't sure what he was seeing when he noticed a small, faint light through his telescope.

"When Piazzi discovered Ceres, exploring it was beyond imagination. More than two centuries later, NASA dispatched a machine on a cosmic journey of more than 3 billion miles to reach the distant, mysterious world he glimpsed," said Marc Rayman, mission director and chief engineer for Dawn at NASA's Jet Propulsion Laboratory, Pasadena, California.

Piazzi was the director of the Palermo Observatory in Sicily, Italy, which has collected documents and instruments from the astronomer's time, and published a booklet on the discovery of Ceres. According to the observatory, Piazzi had been working on a catalog of star positions on January 1, 1801, when he noticed something whose "light was a little faint and colored as Jupiter." He looked for it again on subsequent nights and saw that its position changed slightly.

What was this object? Piazzi wrote to fellow astronomers Johann Elert Bode and Barnaba Oriani to tell them he had discovered a comet.

"I have presented this star as a comet, but owing to its lack of nebulosity, and to its motion being so slow and rather uniform, I feel in the heart that it could be something better than a comet, perhaps. However, I should be very careful in passing this conjecture to the public," Piazzi wrote to Oriani.

A Missing Planet?

Piazzi didn't entirely keep this secret. He told the press that this object was a comet, but did not provide data from his observations, which generated criticism from other astronomers. Piazzi then became sick for a time, and said he could not observe the object any more.

As newspapers spread the word that a comet had been found, astronomer Jerome de Lalande, based in Paris, wrote to Piazzi requesting relevant data in February. The Italian astronomer obliged in April, after recovering from his illness. One of Lalande's students, Johann Karl Burckhardt, performed calculations that revealed Piazzi's discovery did not have an orbit consistent with a comet's orbit. Instead, the data appeared to better fit a circular orbit.

Of course, there was no email in those days, and letters that Piazzi wrote to his friends Bode and Oriani about the so-called comet were delayed due to the Napoleonic Wars. They finally reached the astronomers in March.

The news was especially interesting to Bode because he had championed the Titius-Bode hypothesis: that the positions of planets in our solar system follow a specific pattern, which predicts each planet's distance from the sun. Uranus, discovered in 1781, fit the prediction, too. But the pattern also demanded that there be a planet, yet undiscovered, between Mars and Jupiter.

To find this missing planet, a group of German astronomers had established a society called the "Celestial Police" (Himmelspolizei in German), with Franz Xaver von Zach as its secretary, in 1800. There were 24 astronomers who each scoured a 15-degree piece of zodiacal sky for the missing object. However, Piazzi did not receive his invitation to join this group until after he had spotted Ceres.

Bode calculated an orbit based on Piazzi's data, and he believed that the object Piazzi saw was the missing planet that fit his formula (which was later discredited). Oriani, meanwhile, also calculated an orbit, and on April 7 asked von Zach to publish the news in his well-known astronomy journal, Monatliche Correspondenz, that such a planet may have been discovered.

Almost a 'Lost Comet'

As of spring 1801, besides Piazzi, no one had been able to observe the new celestial object because of cloudy skies and the object's position in its orbit -- it was no longer visible at night, and the sun blocked astronomers' views. Meanwhile, Piazzi still did not publish anything on the object, while he continued to refine his data. Several of his colleagues grew upset with Piazzi for holding back information. Without the data from his observations that concluded on Feb. 11, confirming his discovery would be more difficult -- since February, Ceres had been lost.

Why did Piazzi hesitate to make his data public? One reason might be that, though Piazzi was a skilled observer, he didn't have a solid theoretical knowledge of astronomy, so he couldn't calculate orbits quickly. Secondly, he risked the credibility and reputation of both himself and the observatory. But while he wavered, colleagues in Germany such as Bode firmly believed that there needed to be a planet between Mars and Jupiter. It was their conviction that helped keep the work going on this object, said Ileana Chinnici, who edited the Palermo Observatory's booklet on Ceres.

"Without the determination of the German astronomers, Piazzi would have been just the discoverer of a lost comet, in the best case. They 'believed' in the existence of the planet and were driven by the endeavor to confirm it. This shows how powerful are ideas, models, theories -- yesterday as well as today," Chinnici said.

The Search for Ceres

At last, in July 1801, Piazzi worked on calculating the object's orbit and made public his data about his observations from earlier in the year. And while other astronomers had already come up with their own names -- such as Juno, Hera and Piazzi (to honor the astronomer) -- Piazzi himself announced that the "new star" was called Ceres Ferdinandea. The "Ferdinandea" part honored King Ferdinand of Sicily.

Ceres, the Roman goddess of agriculture, was also the patron deity of Sicily, where Piazzi then lived and worked. Bode, who had wanted to call the object Juno, agreed on Ceres: "You have discovered it in Taurus, and it was re-observed in Virgo, Ceres of the old times. These two constellations are the symbol of agriculture. This occurrence is quite unique."

By the end of July 1801, many astronomers believed Ceres was a planet, but they needed additional confirmation and observations. Piazzi published his complete data set in von Zach's journal in September and, by doing so, got the attention of a young mathematician who would become instrumental in the fate of Ceres.

Twenty-four-year-old Carl Friedrich Gauss had been experimenting with mathematical methods for which he would later become famous. When he applied those methods to Ceres, he came up with different predictions for its position than what others had calculated. Though some were skeptical about Gauss's results, his calculations enabled von Zach to be the first to see Ceres again, on Dec. 7, 1801, followed by other prominent astronomers of the time, and by Piazzi himself on February 23, 1802.

Asteroids: A New Category of Objects

We credit Gauss for calculating the orbit of Ceres. But he did not resolve a fundamental question: What is Ceres?

In March 1802, Heinrich Wilhelm Matthias Olbers discovered a second, similar object, which later became known as Pallas. William Herschel, one of the most famous astronomers in history, then wrote an essay proposing that both Ceres and Pallas represented an entirely new class of objects: asteroids. Herschel wrote of Ceres: "if we called it planet, it would not fill the space between Mars and Jupiter with the dignity required by that position."

Though Herschel considered it an achievement that Piazzi had encountered the first example of an asteroid, Piazzi was disappointed. He thought that Herschel, who had discovered Uranus, just wanted to downplay Ceres. Piazzi wrote to Oriani: "Be they called planetoides or cometoides then, but never asteroides. [...] If an Asteroid Ceres must be called, so must also be called Uranus."

Nonetheless, the door had opened for many more asteroids to be observed. The discoveries of Juno in 1804 and Vesta in 1807 (which would later become the first target of NASA's Dawn mission) reinforced Herschel's notion that asteroids are a class of their own. Herschel coined the term "asteroid" because of their star-like appearance in telescopes. Today, we know there are hundreds of thousands of asteroids in the main asteroid belt between Mars and Jupiter.

Guess what the bright spots are

Piazzi's Legacy

Piazzi could not have known that NASA's Hubble Space Telescope would one day deliver many intriguing images of Ceres, allowing scientists to confirm that the body is, indeed, round like Earth. He could not imagine that in 2006, long after his death, the International Astronomical Union would upgrade Ceres from asteroid to dwarf planet, receiving the same classification as Pluto, which had not yet been discovered in his lifetime. He did not know that in 2007, NASA's Dawn mission would launch from a place called Cape Canaveral in Florida to embark on an unprecedented journey to orbit Vesta and Ceres.

He likely didn't imagine that a space observatory named after Herschel would find in 2013 that there is water vapor emanating from Ceres, following up on 1992 observations of hydroxide at Ceres from NASA's International Ultraviolet Explorer.

Nor could he have guessed that on March 6, 2015, Dawn would be successfully captured into Ceres' orbit, and would spend the rest of the year sending photos and other valuable data back to Earth. He wouldn't know that scientists would use the Hubble Space Telescope's unique capabilities in November 2015 to observe Ceres in the ultraviolet spectrum, complementing Dawn's observations.

Now, as we commemorate the 215th anniversary of Ceres' discovery this month, Dawn is observing the dwarf planet from its lowest orbit ever: 240 miles (385 kilometers) from the surface. The many craters and other features that Piazzi could not see with his telescope are being named after agricultural deities or festivals, extending the theme that Piazzi began with the name "Ceres."

"Our knowledge, our capabilities, our reach and even our ambition all are far beyond what Piazzi could have imagined, and yet it is because of his discovery that we can apply them to learn more, not only about Ceres itself but also about the dawn of the solar system," Rayman said.

Dawn's mission is managed by the Jet Propulsion Laboratory for NASA's Science Mission Directorate in Washington. Dawn is a project of the directorate's Discovery Program, managed by NASA's Marshall Space Flight Center in Huntsville, Alabama. UCLA is responsible for overall Dawn mission science. Orbital ATK Inc., in Dulles, Virginia, designed and built the spacecraft. The German Aerospace Center, Max Planck Institute for Solar System Research, Italian Space Agency and Italian National Astrophysical Institute are international partners on the mission team. For a complete list of mission participants, visit:

http://dawn.jpl.nasa.gov/mission

More information about Dawn is available at the following sites:

http://dawn.jpl.nasa.gov
http://www.nasa.gov/dawn

 



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Monday, January 25, 2016

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
Galaxy Clusters Reveal New Dark Matter Insights

Dark matter is a mysterious cosmic phenomenon that accounts for 27 percent of all matter and energy. Though dark matter is all around us, we cannot see it or feel it. But scientists can infer the presence of dark matter by looking at how normal matter behaves around it.

Galaxy clusters, which consist of thousands of galaxies, are important for exploring dark matter because they reside in a region where such matter is much denser than average. Scientists believe that the heavier a cluster is, the more dark matter it has in its environment. But new research suggests the connection is more complicated than that.

"Galaxy clusters are like the large cities of our universe. In the same way that you can look at the lights of a city at night from a plane and infer its size, these clusters give us a sense of the distribution of the dark matter that we can't see," said Hironao Miyatake at NASA's Jet Propulsion Laboratory, Pasadena, California.

A new study in Physical Review Letters, led by Miyatake, suggests that the internal structure of a galaxy cluster is linked to the dark matter environment surrounding it. This is the first time that a property besides the mass of a cluster has been shown to be associated with surrounding dark matter.

Researchers studied approximately 9,000 galaxy clusters from the Sloan Digital Sky Survey DR8 galaxy catalog, and divided them into two groups by their internal structures: one in which the individual galaxies within clusters were more spread out, and one in which they were closely packed together. The scientists used a technique called gravitational lensing -- looking at how the gravity of clusters bends light from other objects -- to confirm that both groups had similar masses.

But when the researchers compared the two groups, they found an important difference in the distribution of galaxy clusters. Normally, galaxy clusters are separated from other clusters by 100 million light-years on average. But for the group of clusters with closely packed galaxies, there were fewer neighboring clusters at this distance than for the sparser clusters. In other words, the surrounding dark-matter environment determines how packed a cluster is with galaxies.

"This difference is a result of the different dark-matter environments in which the groups of clusters formed. Our results indicate that the connection between a galaxy cluster and surrounding dark matter is not characterized solely by cluster mass, but also its formation history," Miyatake said.

Study co-author David Spergel, professor of astronomy at Princeton University in New Jersey, added, "Previous observational studies had shown that the cluster's mass is the most important factor in determining its global properties. Our work has shown that 'age matters': Younger clusters live in different large-scale dark-matter environments than older clusters."

The results are in line with predictions from the leading theory about the origins of our universe. After an event called cosmic inflation, a period of less than a trillionth of a second after the big bang, there were small changes in the energy of space called quantum fluctuations. These changes then triggered a non-uniform distribution of matter. Scientists say the galaxy clusters we see today have resulted from fluctuations in the density of matter in the early universe.

"The connection between the internal structure of galaxy clusters and the distribution of surrounding dark matter is a consequence of the nature of the initial density fluctuations established before the universe was even one second old," Miyatake said.

Researchers will continue to explore these connections.

"Galaxy clusters are remarkable windows into the mysteries of the universe. By studying them, we can learn more about the evolution of large-scale structure of the universe, and its early history, as well as dark matter and dark energy," Miyatake said.

 



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Friday, January 22, 2016

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
Voyager Mission Celebrates 30 Years Since Uranus

Humanity has visited Uranus only once, and that was 30 years ago. NASA's Voyager 2 spacecraft got its closest look at the mysterious, distant, gaseous planet on Jan. 24, 1986.

Voyager 2 sent back stunning images of the planet and its moons during the flyby, which allowed for about 5.5 hours of close study. The spacecraft got within 50,600 miles (81,500 kilometers) of Uranus during that time.

"We knew Uranus would be different because it's tipped on its side, and we expected surprises," said Ed Stone, project scientist for the Voyager mission, based at the California Institute of Technology, Pasadena. Stone has served as project scientist since 1972, continuing in that role today.

Uranus revealed itself to be the coldest planet known in our solar system, even though it's not the farthest from the sun. This is because it has no internal heat source.

Scientists determined that the atmosphere of Uranus is 85 percent hydrogen and 15 percent helium. There was also evidence of a boiling ocean about 500 miles (800 kilometers) below the cloud tops.

Scientists found that Uranus has a magnetic field different from any they had ever encountered previously. At Mercury, Earth, Jupiter and Saturn, the magnetic field is aligned approximately with the rotational axis.

"Then we got to Uranus and saw that the poles were closer to the equator," Stone said. "Neptune turned out to be similar. The magnetic field was not quite centered with the center of the planet."

This surface magnetic field of Uranus was also stronger than that of Saturn. Data from Voyager 2 helped scientists determine that the magnetic tail of Uranus twists into a helix stretching 6 million miles (10 million kilometers) in the direction pointed away from the sun. Understanding how planetary magnetic fields interact with the sun is a key part of NASA's goal to understand the very nature of space. Not only does studying the sun-planet connection provide information useful for space travel, but it helps shed light on the origins of planets and their potential for harboring life.

Voyager 2 also discovered 10 new moons (there are 27 total) and two new rings at the planet, which also proved fascinating. An icy moon called Miranda revealed a peculiar, varied landscape and evidence of active geologic activity in the past. While only about 300 miles (500 kilometers) in diameter, this small object boasts giant canyons that could be up to 12 times as deep as the Grand Canyon in Arizona. Miranda also has three unique features called "coronae," which are lightly cratered collections of ridges and valleys. Scientists think this moon could have been shattered and then reassembled.

Mission planners designed Voyager 2's Uranus encounter so that the spacecraft would receive a gravity assist to help it reach Neptune. In 1989, Voyager 2 added Neptune to its resume of first-ever looks.

 

"The Uranus encounter was very exciting for me," said Suzanne Dodd, project manager for Voyager, based at NASA's Jet Propulsion Laboratory, Pasadena, California, who began her career with the mission while Voyager 2 was en route to Uranus." It was my first planetary encounter and it was of a planet humanity had never seen up close before. Every new image showed more details of Uranus, and it had lots of surprises for the scientists. I hope another spacecraft will be sent to explore Uranus, to explore the planet in more detail, in my lifetime."

Voyager 2 was launched on Aug. 20, 1977, 16 days before its twin, Voyager 1. In August 2012, Voyager 1 made history as the first spacecraft to enter interstellar space, crossing the boundary encompassing our solar system's planets, sun and solar wind. Voyager 2 is also expected to reach interstellar space within the next several years.

The Voyagers were built by JPL, which continues to operate both spacecraft. JPL is a division of Caltech. For more information about the Voyager spacecraft, visit:

http://www.nasa.gov/voyager

http://voyager.jpl.nasa.gov

 



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Thursday, January 21, 2016

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
NASA's LISA Pathfinder Thrusters Operated Successfully

While some technologies were created to make spacecraft move billions of miles, the Disturbance Reduction System has the opposite goal: To keep a spacecraft as still as possible.

The thruster system, managed by NASA's Jet Propulsion Laboratory, Pasadena, California, is part of the European Space Agency's LISA Pathfinder spacecraft, which launched from Kourou, French Guiana on Dec. 3, 2015 GMT (Dec. 2 PST). LISA Pathfinder will test technologies that could one day allow detection of gravitational waves, whose effects are so miniscule that a spacecraft would need to remain extremely steady to detect them. Observing gravitational waves would be a huge step forward in our understanding of the evolution of the universe.

Now, LISA Pathfinder is on its way to Lagrange Point L1, about 930,000 miles (1.5 million kilometers) from Earth in the direction of the sun. L1 is a special point that a spacecraft can orbit while maintaining a nearly constant distance to Earth. This month, scientists and engineers have been switching on LISA Pathfinder's instruments to test them in space. This has included the Disturbance Reduction System instrument computer and thrusters.

The system uses colloid micronewton thrusters, which operate by applying an electric charge to small droplets of liquid and accelerating them through an electric field, to precisely control the position of the spacecraft. Thrusters that work this way had never been successfully operated in space before LISA Pathfinder launched.

As of Jan. 10, all eight identical thrusters, developed by Busek Co., Natick, Massachusetts, with technical support from JPL, passed their functional tests. The thrusters achieved their maximum thrust of 30 micronewtons, equivalent to the weight of a mosquito. This level of precision is necessary to counteract small forces on the spacecraft such as the pressure of sunlight, with the result that the spacecraft and the instruments inside are in near-perfect free-fall. A mission to detect gravitational waves would need that level of stability.

"We reached a major milestone with this technology development," said Phil Barela, Disturbance Reduction System project manager at JPL. "The DRS is helping point the way to a system that could be used to detect gravitational waves in the future."

Gravitational waves are one of the last unverified predictions from the theory of General Relativity, which Albert Einstein published about a century ago. Einstein wrote that as massive bodies accelerate, such as black holes, they produce distortions in space-time. Scientists are interested in observing and characterizing these ripples in space-time so that they can learn more about the astrophysical systems that produce them, and about gravity itself. Proposed experiments to detect them from space, such as a future LISA mission, would need to measure how two freely-falling objects move ever so slightly, relative to each other, as a result of gravitational waves. In order to rule out any disturbances that could mask these waves, there must be a system to compensate for solar pressure and other factors. The Disturbance Reduction System on LISA Pathfinder will demonstrate this technology.

The Disturbance Reduction System could also lead to advanced thruster systems for other space applications. Space telescopes need to be very stable to detect distant planets in other solar systems, for example, and could use a similar system. A set of thrusters like the Disturbance Reduction System's could also be used in small satellites to help synchronize flying patterns.

LISA Pathfinder will reach its final orbit on Jan. 22, and begin science operations on March 1. For the first phase of the mission's science operations, a thruster technology system designed by the European Space Agency will be used. JPL's Disturbance Reduction System will then take over in June or July, operating for 90 days.

LISA Pathfinder is managed by the European Space Agency. The spacecraft was built by Airbus Defence and Space, Ltd., United Kingdom. Airbus Defence and Space, GmbH, Germany, is the payload architect for the LISA Technology Package. The DRS is managed by JPL. The California Institute of Technology manages JPL for NASA.

 



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LAST CALL! January Educator Workshop - Space School Musical

 

 

Space School Musical

When: Saturday, Jan. 30, 9:30 a.m. to 12:30 p.m.

Where: NASA Jet Propulsion Laboratory, Von Karman Auditorium, Pasadena, California

Target Audience: Formal and informal educators for grades 3-12

Overview: The solar system comes alive in "Space School Musical," a video series that introduces the planets, moons, asteroids, meteors and more through songs and dance routines. Students watch the videos, learn the songs, do the activities and perform the show themselves.

Call the Educator Resource Center at 818-393-5917 to reserve your spot.

After the workshop, attendees will be able to:

- Show the musical DVD to their students, which stands alone as a basis for engaging learning and discussion opportunities.
- Lead their students in lessons from the activity guide they will receive, reinforcing the learning concepts in the songs through academic, art, fitness and life-skills activities.
- Lead their students in putting on their own production of the musical, allowing students to express their creativity in a variety of ways.
This activity uses arts-based learning to engage students in planetary science through music, art and physical activity. Students' understanding of the content is deepened through activities that encourage creativity, critical thinking, decision-making skills, collaboration and communication.

The Space School Musical video series and activity is also available online, here.

This free workshop is offered through the NASA/JPL Educator Resource Center, which provides formal and informal educators with NASA resources and materials that support STEM learning.

Discover more upcoming educator workshops and events from NASA/JPL Education.


Get Your Free Mars Bulletin Board!

Get the school year back in gear with a Mars-themed bulletin board for your school, classroom, library or educational program. The NASA/JPL Educator Resource Center is offering a set of free posters and lithographs with fun facts about the Red Planet and NASA's Mars missions.

> Learn more

 

 



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Sunday, January 17, 2016

JPL News - Day in Review

 

DAY IN REVIEW
NASA JPL latest news release
Jason-3 Launches to Monitor Global Sea Level Rise

Jason-3, a U.S.-European oceanography satellite mission with NASA participation that will continue a nearly quarter-century record of tracking global sea level rise, lifted off from Vandenberg Air Force Base in California Sunday at 10:42 a.m. PST (1:42 p.m. EST) aboard a SpaceX Falcon 9 rocket.

Jason-3 is an international mission led by the National Oceanic and Atmospheric Administration (NOAA) in partnership with NASA, the French space agency CNES, and the European Organisation for the Exploitation of Meteorological Satellites.

"Jason-3 will take the pulse of our changing planet by gathering environmental intelligence from the world's oceans," said Stephen Volz, assistant administrator for NOAA's Satellite and Information Service.

The mission will improve weather, climate and ocean forecasts, including helping NOAA's National Weather Service and other global weather and environmental forecast agencies more accurately forecast the strength of tropical cyclones.

"Jason-3 is a prime example of how our nation leverages NASA's expertise in space and scientific exploration to help address critical global challenges in collaboration with NOAA and our international partners," said John Grunsfeld, associate administrator for science at NASA Headquarters in Washington. "The measurements from Jason-3 will advance our efforts to understand Earth as an integrated system by increasing our knowledge of sea level changes and the ocean's roles in climate."

Minutes after Jason-3 separated from the rocket's second stage, the spacecraft unfolded its twin sets of solar arrays. Ground controllers successfully acquired the spacecraft's signal, and initial telemetry reports showed the satellite was in good health.

Jason-3 entered orbit about 16 miles (25 kilometers) below Jason-2. The new spacecraft will gradually raise itself into the same 830-mile (1,336-kilometer) orbit and position itself to follow Jason-2's ground track, orbiting about a couple of minutes behind Jason-2. The two spacecraft will fly in formation, making nearly simultaneous measurements for about six months to allow scientists to precisely calibrate Jason-3's instruments.

Jason-3 will begin full science operations after a six-month checkout phase, joining Jason-2, which launched in 2008. From low-Earth orbit, Jason-3 will precisely measure the height of 95 percent of the world's ice-free ocean every 10 days.

Coordinating orbits and combining measurements from Jason-2 and Jason-3 should allow even more frequent coverage of the global ocean. Together, the two spacecraft will double global data coverage. This tandem mission will improve our knowledge of tides in coastal and shallow seas and internal tides in the open ocean, while improving our understanding of ocean currents and eddies.

Measurements of sea-surface height, or ocean-surface topography, reveal the speed and direction of ocean currents and tell scientists how much of the sun's energy is stored by the ocean. Combining ocean current and heat storage data is key to understanding global climate changes.

Since the Topex/Poseidon-Jason satellite missions began in 1992, researchers have observed a total global sea level rise of 2.8 inches (70 millimeters) - an average rate of 0.12 inches (3 millimeters) a year. Because it is a measure of both ocean warming and loss of land ice, sea level rise is an important indicator of human-caused climate change.

"As human-caused global warming drives sea levels higher and higher, we are literally reshaping the surface of our planet," said Josh Willis, NASA project scientist for Jason-3 at NASA's Jet Propulsion Laboratory in Pasadena, California. "These missions tell us how much and how fast."

Data from Jason-3 will be used for other scientific, commercial and operational applications, including modeling of deep-ocean waves; forecasts of surface waves for offshore operators; forecasts of tides and currents for commercial shipping and ship routing; coastal forecasts to respond to environmental challenges such as oil spills and harmful algal blooms; coastal modeling crucial for marine mammal and coral reef research; and forecasts of El Niño and La Niña events.

CNES provided the Jason-3 spacecraft bus. NASA and CNES are jointly providing the primary payload instruments. NASA's Launch Services Program at the Kennedy Space Center in Florida is responsible for launch management and countdown operations for the SpaceX Falcon 9 rocket. JPL manages the mission for NASA's Science Mission Directorate, Washington.

For more information about the Jason-3 mission, visit:

http://www.nesdis.noaa.gov/jason-3

To find out more about NASA's Earth science research, visit:

http://www.nasa.gov/earth

 



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