jeudi 16 mars 2017

ESA’s Jupiter mission moves off the drawing board

ESA - JUICE Mission logo.

16 March 2017

Demanding electric, magnetic and power requirements, harsh radiation, and strict planetary protection rules are some of the critical issues that had to be tackled in order to move ESA’s Jupiter Icy Moons Explorer – Juice – from the drawing board and into construction.

Scheduled for launch in 2022, with arrival in the Jovian system in 2029, Juice will spend three-and-a-half years examining the giant planet’s turbulent atmosphere, enormous magnetosphere, its set of tenuous dark rings and its satellites.

Juice’s journey to Jupiter

It will study the large icy moons Ganymede, Europa and Callisto, which are thought to have oceans of liquid water beneath their icy crusts – perhaps even harbouring habitable environments.

The mission will culminate in a dedicated, eight-month tour around Ganymede, the first time any moon beyond our own has been orbited by a spacecraft.

Juice will be equipped with 10 state-of-the-art instruments, including cameras, an ice-penetrating radar, an altimeter, radio-science experiments, and sensors to monitor the magnetic fields and charged particles in the Jovian system.

In order to ensure it can address these goals in the challenging Jovian environment, the spacecraft’s design has to meet stringent requirements.

Jupiter's largest moons

An important milestone was reached earlier this month, when the preliminary design of Juice and its interfaces with the scientific instruments and the ground stations were fixed, which will now allow a prototype spacecraft to be built for rigorous testing.

The review also confirmed that the 5.3 tonne spacecraft will be compatible with its Ariane 5 launcher.

Operating in the outer Solar System, far from the Sun, means that Juice needs a large solar array: two wings of five panels each are foreseen, which will cover a total surface area of nearly 100 sq m, capable of providing 820 W at Jupiter by the end of the mission.

After launch, Juice will make five gravity-assist flybys in total: one each at Mars and Venus, and three at Earth, to set it on course for Jupiter. Its solar panels will have to cope with a range of temperatures such that when it is flying closer to the Sun during the Venus flyby, the solar wings will be tilted to avoid excessive temperatures damaging the solar cells.

The spacecraft’s main engine will be used to enter orbit around the giant planet, and later around Jupiter’s largest moon, Ganymede. As such, the engine design has also been critically reviewed at this stage.

Special measures will allow Juice to cope with the extremely harsh radiation that it must endure for several years around Jupiter. This means careful selection of components and materials, as well as radiation shielding.

One particularly important topic is Juice’s electromagnetic ‘cleanliness’. Because a key goal is to monitor the magnetic fields and charged particles at Jupiter, it is imperative that any electromagnetic fields generated by the spacecraft itself do not interfere with the sensitive scientific measurements.

Juice

This will be achieved by the careful design of the solar array electrical architecture, the power distribution unit, and the reaction wheels – a type of flywheel that stabilises the attitude.

The review also ensured that Juice will meet strict planetary protection guidelines, because it is imperative to minimise the risk that the potentially habitable ocean moons, particularly Europa, might be contaminated by viruses, bacteria or spores carried by the spacecraft from Earth. Therefore, mission plans ensure that Juice will not crash into Europa, on a timescale of hundreds of years.

“The spacecraft design has been extensively and positively reviewed, and confirmed to address the many critical mission requirements,” says Giuseppe Sarri, Juice project manager. “So far we are on schedule, and are delighted to begin the development stage of this ambitious large-class mission.”

ESA’s industrial partners, led by Airbus, now have the go-ahead to start building the prototype spacecraft units that will subjected to tough tests to simulate the conditions expected during launch, as well as the extreme range of environmental conditions.

Once the design is proved beyond doubt, the flight model – the one that will actually go into space – will be built.

Related links:

ESA' JUICE: http://sci.esa.int/juice/

JUICE in depth: http://sci.esa.int/science-e/www/area/index.cfm?fareaid=129

Images, Video, Text, Credits: ESA/Markus Bauer/Giuseppe Sarri/Olivier Witasse/AOES/NASA/JPL/DLR.

Best regards, Orbiter.ch

MRO: A Closer Look at Holden Crater & Bedrock Outcrops in Kaiser Crater












NASA - Mars Reconnaissance Orbiter (MRO) logo.

March 15, 2017

A Closer Look at Holden Crater


Holden Crater in southern Margaritifer Terra displays a series of finely layered deposits on its floor (white and light purple in an enhanced color image). The layered deposits are especially well exposed in the southwestern section of the crater where erosion by water flowing through a breach in the crater rim created spectacular outcrops.

In this location, the deposits appear beneath a cap of alluvial fan materials (tan to brown in this image). Within the deposits, individual layers are nearly flat-lying and can be traced for hundreds of meters to kilometers. Information from the CRISM instrument on the Mars Reconnaissance Orbiter suggests that at least some of these beds contain clays.

By contrast, the beds in the overlying alluvial fan are less continuous and dip in varying directions, showing less evidence for clays. Collectively, the characteristics of the finely bedded deposits suggest they may have been deposited into a lake on the crater floor, perhaps fed by runoff related to formation of the overlying fans.

The map is projected here at a scale of 25 centimeters (9.8 inches) per pixel. [The original image scale is 25.9 centimeters (10.2 inches) per pixel (with 1 x 1 binning); objects on the order of 78 centimeters (30.7 inches) across are resolved.] North is up.

Bedrock Outcrops in Kaiser Crater


This enhanced-color image shows a patch of well-exposed bedrock on the floor of Kaiser Crater.

The wind has stripped off the overlying soil, and created grooves and scallops in the bedrock. The narrow linear ridges are fractures that have been indurated, probably by precipitation of cementing minerals from groundwater flow. The rippled dark blue patches consist of sand.

The map is projected here at a scale of 25 centimeters (9.8 inches) per pixel. [The original image scale is 25.3 centimeters (9.9 inches) per pixel (with 1 x 1 binning); objects on the order of 76 centimeters (29.9 inches) across are resolved.] North is up.

This is a stereo pair with http://www.uahirise.org/ESP_012516_1330

Mars Reconnaissance Orbiter (MRO)

The University of Arizona, Tucson, operates HiRISE, which was built by Ball Aerospace & Technologies Corp., Boulder, Colo. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, California, manages the Mars Reconnaissance Orbiter Project for NASA's Science Mission Directorate, Washington.

Mars Reconnaissance Orbiter (MRO): http://www.nasa.gov/mission_pages/MRO/main/index.html

Images, Text, Credits: NASA/Tony Greicius/JPL-Caltech/Univ. of Arizona.

Greetings, Orbiter.ch

ExoMars: science checkout completed and aerobraking begins









ESA & ROSCOSMOS - ExoMars Mission patch.

16 March 2017

Trace Gas Orbiter (TGO)

The ExoMars Trace Gas Orbiter has completed another set of important science calibration tests before a year of aerobraking gets underway.

The mission was launched a year ago this week, and has been orbiting the Red Planet since 19 October. During two dedicated orbits in late November, the science instruments made their first calibration measurements since arriving at Mars.

 Flying over Mellish crater

The latest tests were carried out 5–7 March from a different orbit, and included checking procedures associated with taking images and collecting data on the planet’s atmosphere.

For example, the Nadir and Occultation for Mars Discovery (NOMAD) instrument made test observations to help determine the best settings to make future measurements of trace gases in the atmosphere.

Methane in particular is of high interest. On Earth it is produced primarily by biological activity, and to a smaller extent by geological processes, such as some hydrothermal reactions. Understanding how the Red Planet’s methane is produced therefore has extremely exciting implications.

NOMAD also had the opportunity to test joint measurements with the Atmospheric Chemistry Suite, which together will take highly sensitive measurements of the atmosphere to determine its constituents.

 Water vapour

Meanwhile, the FREND detector continued to collect more on the flow of neutrons from the surface. Eventually, these data will be used to identify sites where water or ice might be hidden just below the surface.

The high-resolution Colour and Stereo Surface Imaging System was commanded to take a number of images, including star calibrations, and several pointing at Mars.

An example is presented here, taken just as the orbiter was crossing the boundary between day and night, over the southern hemisphere.

“These dress rehearsals enable our science teams to fine-tune their data acquisition techniques including pointing commands, iron out any software bugs, and get used to working with the data, well in advance of the start of the main mission starting next year,” says Håkan Svedhem, ESA’s project scientist. “What we’re seeing so far is really promising for our science goals.”

 Carbon dioxide

Starting next year, the craft will make its observations from a near-circular 400 km-altitude orbit, circling the planet every two hours.

It is currently in a one-day, 200 x 33 000 km orbit but will use the atmosphere to adjust the orbit gradually by ‘aerobraking’. It will repeatedly surf in and out of the atmosphere at closest approach, pulling down its furthest point over the course of the year.

Earlier this week, the first commands for aerobraking were uploaded, ready to be executed starting yesterday. Over the next few weeks it will make seven engine burns that will adjust its orbit as part of a ‘walk-in’ period before the main aerobraking. This will first see the closest point of the orbit reduced to about 113 km.

“It’s not ESA’s first experience with aerobraking, but it is the first time we’ve used this technique to achieve a planned science orbit, repeating it for such a long duration,” says flight director Michel Denis.

“The mission controllers have worked intensively with our flight dynamics experts to prepare for this challenging phase – we’re go for aerobraking.

Neutron detections

“We’ll closely monitor the solar array temperature and the acceleration of the spacecraft, not only during the first few passages through the atmosphere but throughout the rest of 2017, and adjust the trajectory as needed.”

The final orbit is also designed for relay and communications with rovers and landers on the surface. In particular it will act as a relay for the 2020 ExoMars mission of a stationary surface platform and a rover.

ExoMars is a joint endeavour between ESA and Roscosmos.

Related links:

ExoMars: http://www.esa.int/Our_Activities/Space_Science/ExoMars

Robotic exploration of Mars: http://exploration.esa.int/

Roscosmos: http://en.federalspace.ru/

ExoMars at IKI: http://exomars.cosmos.ru/

Thales Alenia Space: https://www.thalesgroup.com/en/worldwide/space/space

NASA In 2016 ExoMars orbiter (Electra radio): http://mars.nasa.gov/programmissions/missions/future/exomarsorbiter2016/

Where on Mars?: http://whereonmars.co/

ExoMars for broadcasters: http://www.esa.int/esatv/Transmissions/2016/10/ExoMars_at_Mars_live_coverage

Images, Graphics, Text, Credits: ESA/Markus Bauer/Håkan Svedhem/Roscosmos/CaSSIS , CC BY-SA 3.0 IGO/NOMAD/BISA/IAA/INAF/OU/ACS/IKI/FREND.

Best regards, Orbiter.ch

mercredi 15 mars 2017

NASA's ICESat-2 to Provide More Depth to Sea Ice Forecasts












NASA - ICESat-2 Mission patch.

March 15, 2017

In March, the Arctic sea ice pack is supposed to reach its greatest extent — but this year it’s far below average, off by an area about the size of Texas and New Mexico combined.

Satellite observations currently reveal how much of the ocean surface is covered by ice, but there is another critical measurement to make. Researchers are already anticipating using NASA’s Ice, Cloud and land Elevation Satellite-2, or ICESat-2, to measure sea ice in the third dimension.

Satellites have been continuously measuring sea ice since 1979, and have mapped the downward trend of ice extent. Determining the thickness of the remote sea ice pack, however, is difficult with existing tools. And it’s an essential measurement. Thicker ice is more resilient to storms, and can take years to build up. Changes in the depth of sea ice alters the water’s salinity and temperature, which can alter oceanic and atmospheric currents.  Sea ice also acts as a cap on the ocean — insulating it from the atmosphere — and plays a key role in cooling down the planet.


Image above: Ice can switch from thick to thin over short distances, as seen in this photo taken form Operation IceBridge’s campaign over the Chukchi Sea in March 2017. Image Credit: NASA.

Some scientists have used the available satellite data to monitor the ice’s age, determining which has survived and built up through more than two summers. They found that the amount of older, thicker ice is declining. But with ICESat-2, scientists will be able to measure the height of the sea ice directly, and from that calculate the thickness.

ICESat-2, slated to launch in 2018, will use a laser instrument to measure the height of Earth’s surfaces globally. It will monitor vegetation, bodies of water and more, but with a focus on measuring ice and snow cover. By taking a dense set of measurements, the satellite will collect enough precise information for scientists to measure how far sea ice floats above the ocean surface, down to about 1 inch (3 centimeters).

“The question we want to ask with ICESat-2 is what’s happening to the thickness of the ice,” said Sinead Farrell, a member of the ICESat-2 science definition team and polar scientist at the University of Maryland, College Park, Maryland. “We’re trying to monitor the health of the ice pack, and one of the things we’re really keen on doing is making sure we get the ICESat-2 data into the hands of scientists and the scientific community as quickly as possible.”

The influx of data from ICESat-2, managed by NASA’s Goddard Space Flight Center in Greenbelt, Maryland, will be a boon to sea ice forecasters. These researchers use observations of the ice to improve computer models that simulate the extent, thickness and other conditions of Arctic ice cover.


Image above: Young sea ice in the Chukchi Sea, north of the Bering Sea, as seen by Operation IceBridge in March 2017. IceBridge measures ice thickness along its flight lines. Once ICESat-2 launches, it will greatly increase sea ice coverage with a dense grid of measurements, taken year-round. Image Credit: NASA.

“It’s difficult to take measurements to validate our model against — it’s expensive to get to the Arctic and conditions aren’t too friendly up there,” said Pamela Posey, computer scientist and sea ice modeler with the U.S. Naval Research Laboratory in NASA's Stennis Space Center, Mississippi. She is also a principal investigator with ICESat-2’s Early Adopter program, which is part of an effort to reach out to the stakeholder community before the satellite launches, enabling the mission scientists to understand what is possible, or not, for other researchers to do with the data. The program also aims to help people put the data to use faster, after the satellite launches.

Posey works on a model that takes in information about current Arctic conditions, and predicts sea ice characteristics for the coming week. The Navy provides that information to submarines and surface ships — if subs have an emergency and need to surface, they need to know the thickness of the ice above them, she noted. And surface ships need to know how thick ice is to determine whether or not they can break a path through a particular area.

“Our models run daily and produce out to a seven-day forecast,” Posey said. “The more observations you get into a model, the more accurate your forecast is going to be.”

She is currently using a derived ice thickness product from the ESA’s (European Space Agency) Cryosat satellite to plug into the model, to determine how to use ICESat-2’s data once they are available. She plans to compare ICESat-2’s measurements with the ice conditions predicted by the model, to validate the computer model and reset it to improve accuracy going forward.

Andrew Roberts, a researcher and Early Adopter principal investigator with the Naval Postgraduate School in Monterey, California, is also working to see how ICESat-2 could improve computer simulations of sea ice in distant regions. He’s working on several problems to get ready for the influx of sea ice height data — one being that while models simulate what the sea ice is doing across the entire Arctic, ICESat-2 will take individual point measurements along the satellite’s path, creating tracks of information that need to be reconciled with the data from models, which is in a grid.

ICESat-2 satellite. Image Credit: NASA

So Roberts is creating a program for the computer model that will produce a simulation of sea ice only where ICESat-2 is measuring, to better compare the two sets of numbers.

“We’ve effectively simulated what ICESat-2 would see,” Roberts said. “It’s actually very finicky to do, and you’ve got to come up with an efficient way to do it.”

Roberts is also working on isolating the height of the sea ice above the ocean surface in the computer model — the basic measurement that ICESat-2 will take — to be able to compare the satellite and computer-simulated data. It’s all to be able to improve models of what’s going on in the Arctic, he said.

The models are used by the Navy, shipping companies and others, but also provide a window into a remote, complex part of the world. And sea ice has impacts that stretch beyond its boundaries. It acts as an air conditioner for the globe, reflecting sunlight that would otherwise be absorbed into the ocean. It interacts with the atmosphere and ocean currents, impacting weather and climate systems that reach down to lower latitudes. It provides seasonal habitat for wildlife, and hunting grounds for indigenous populations.

“The Arctic sea ice is changing extremely rapidly, and we’re trying to understand why that is the case,” Roberts said.

For more information about NASA's ICESat-2 mission:

http://www.nasa.gov/icesat-2 or http://icesat-2.gsfc.nasa.gov/

Images (mentioned), Text, Credits: NASA's Goddard Space Flight Center, by Kate Ramsayer/Karl Hille.

Greetings, Orbiter.ch

Relativistic Electrons Uncovered with NASA’s Van Allen Probes










NASA - Van Allen Probes Mission patch.

March 15, 2017

Earth’s radiation belts, two doughnut-shaped regions of charged particles encircling our planet, were discovered more than 50 years ago, but their behavior is still not completely understood. Now, new observations from NASA’s Van Allen Probes mission show that the fastest, most energetic electrons in the inner radiation belt are not present as much of the time as previously thought. The results are presented in a paper in the Journal of Geophysical Research and show that there typically isn’t as much radiation in the inner belt as previously assumed — good news for spacecraft flying in the region.

Leaky Radiation Belts

Video above: Since their discovery at the dawn of the Space Age, Earth's radiation belts continue to reveal new complex structures and behaviors. This visualization shows how the radiation belts change in response to the injection of electrons from a storm in late June 2015. Red colors indicate higher numbers of electrons. Video Credits: NASA's Goddard Space Flight Center/Tom Bridgman.

Past space missions have not been able to distinguish electrons from high-energy protons in the inner radiation belt. But by using a special instrument, the Magnetic Electron and Ion Spectrometer — MagEIS — on the Van Allen Probes, the scientists could look at the particles separately for the first time. What they found was surprising —there are usually none of these super-fast electrons, known as relativistic electrons, in the inner belt, contrary to what scientists expected.

“We’ve known for a long time that there are these really energetic protons in there, which can contaminate the measurements, but we’ve never had a good way to remove them from the measurements until now,” said Seth Claudepierre, lead author and Van Allen Probes scientist at the Aerospace Corporation in El Segundo, California.

Of the two radiation belts, scientists have long understood the outer belt to be the rowdy one. During intense geomagnetic storms, when charged particles from the sun hurtle across the solar system, the outer radiation belt pulsates dramatically, growing and shrinking in response to the pressure of the solar particles and magnetic field.  Meanwhile, the inner belt maintains a steady position above Earth’s surface. The new results, however, show the composition of the inner belt isn’t as constant as scientists had assumed.

Ordinarily, the inner belt is composed of high-energy protons and low-energy electrons. However, after a very strong geomagnetic storm in June 2015, relativistic electrons were pushed deep into the inner belt.

The findings were visible because of the way MagEIS was designed. The instrument creates its own internal magnetic field, which allows it to sort particles based on their charge and energy. By separating the electrons from the protons, the scientists could understand which particles were contributing to the population of particles in the inner belt.

“When we carefully process the data and remove the contamination, we can see things that we’ve never been able to see before,” said Claudepierre. “These results are totally changing the way we think about the radiation belt at these energies.”

(Click on the image for enlarge)

Image above: During a strong geomagnetic storm, electrons at relativistic energies, which are usually only found in the outer radiation belt, are pushed in close to Earth and populate the inner belt. While the electrons in the slot region quickly decay, the inner belt electrons can remain for many months. Image Credits: NASA’s Goddard Space Flight Center/Mary Pat Hrybyk-Keith.

Given the rarity of the storms, which can inject relativistic electrons into the inner belt, the scientists now understand there to typically be lower levels of radiation there — a result that has implications for spacecraft flying in the region. Knowing exactly how much radiation is present may enable scientists and engineers to design lighter and cheaper satellites tailored to withstand the less intense radiation levels they’ll encounter.

In addition to providing a new outlook on spacecraft design, the findings open a new realm for scientists to study next.

“This opens up the possibility of doing science that previously was not possible,” said Shri Kanekal, Van Allen Probes deputy mission scientist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, not involved with the study. “For example, we can now investigate under what circumstances these electrons penetrate the inner region and see if more intense geomagnetic storms give electrons that are more intense or more energetic.”

Van Allen Probes in orbit. Image Credit: NASA

The Van Allen Probes is the second mission in NASA’s Living with a Star Program and one of many NASA heliophysics missions studying our near-Earth environment. The spacecraft plunge through the radiation belts five to six times a day on a highly elliptical orbit, in order to understand the physical processes that add and remove electrons from the region.

Related links:

Journal of Geophysical Research: http://onlinelibrary.wiley.com/doi/10.1002/2016JA023719/abstract

NASA's Van Allen Probes website: http://www.nasa.gov/van-allen-probes/

Images (mentioned), Video (mentioned), Text, Credits: NASA's Goddard Space Flight Center, by Mara Johnson-Groh/Rob Garner.

Best regards, Orbiter.ch

Experiments Show Titan Lakes May Fizz with Nitrogen












NASA & ESA - Cassini-Huygens Mission to Saturn & Titan patch.

March 15, 2017

A recent NASA-funded study has shown how the hydrocarbon lakes and seas of Saturn's moon Titan might occasionally erupt with dramatic patches of bubbles.

For the study, researchers at NASA's Jet Propulsion Laboratory in Pasadena, California, simulated the frigid surface conditions on Titan, finding that significant amounts of nitrogen can be dissolved in the extremely cold liquid methane that rains from the skies and collects in rivers, lakes and seas. They demonstrated that slight changes in temperature, air pressure or composition can cause the nitrogen to rapidly separate out of solution, like the fizz that results when opening a bottle of carbonated soda.


Image above: Cassini captured this mosaic of images showing the northern lakes and seas of Saturn's moon Titan on Feb. 17, 2017. The mission's final close Titan flyby is planned for April 22. Image Credits: NASA/JPL-Caltech/Space Science Institute.

NASA's Cassini spacecraft has found that the composition of Titan's lakes and seas varies from place to place, with some reservoirs being richer in ethane than methane. "Our experiments showed that when methane-rich liquids mix with ethane-rich ones -- for example from a heavy rain, or when runoff from a methane river mixes into an ethane-rich lake -- the nitrogen is less able to stay in solution," said Michael Malaska of JPL, who led the study.

The result is bubbles. Lots of bubbles

The release of nitrogen, known as exsolution, can also occur when methane seas warm slightly during the changing seasons on Titan. A fizzy liquid could also cause problems, potentially, for a future robotic probe sent to float on or swim through Titan's seas. Excess heat emanating from a probe might cause bubbles to form around its structures -- for example, propellers used for propulsion -- making it difficult to steer or keep the probe stable.

Cassini Titan flyby. Image Credits: NASA/JPL-Caltech

Magic Island Mechanism?

The notion of nitrogen bubbles creating fizzy patches on Titan's lakes and seas is relevant to one of the more enchanting unsolved mysteries Cassini has investigated during its time exploring Titan: the so-called "magic islands." During several flybys, Cassini's radar has revealed small areas on the seas that appeared and disappeared, and then (in at least one case) reappeared. Researchers proposed several potential explanations for what could be creating these seemingly island-like features, including the idea of fields of bubbles. The new study provides details about the mechanism that could be forming such bubbles, if they are indeed the culprit.


Image above: Radar images from Cassini showed a strange island-like feature in one of Titan's hydrocarbon seas that appeared to change over time (series of images at left). One possible explanation for this "magic island" is bubbles. Image Credits: NASA/JPL-Caltech/Space Science Institute.

"Thanks to this work on nitrogen's solubility, we're now confident that bubbles could indeed form in the seas, and in fact may be more abundant than we'd expected," said Jason Hofgartner of JPL, who serves as a co-investigator on Cassini's radar team and was a co-author of the study.

Freezing Fizz and Breathing Lakes

In characterizing how nitrogen moves between Titan's liquid reservoirs and its atmosphere, the researchers also coaxed nitrogen out of a simulated ethane-rich solution as the ethane froze to the bottom of their tiny, simulated Titan lake. Unlike water, which is less dense in its solid form than its liquid form, ethane ice would form on the bottom of Titan's frigid pools. As the ethane crystalizes into ice, there's no room for the dissolved nitrogen gas, and it comes fizzing out.

Nitrogen Fizzing Out of Ethane Slush

While the thought of hydrocarbon lakes bubbling with nitrogen on an alien moon is dramatic, Malaska points out that the movement of nitrogen on Titan doesn't just move in one direction. Clearly, it has to get into the methane and ethane before it can get out.

"In effect, it's as though the lakes of Titan breathe nitrogen," Malaska said. "As they cool, they can absorb more of the gas, 'inhaling.' And as they warm, the liquid's capacity is reduced, so they 'exhale.'"

A similar phenomenon occurs on Earth with carbon dioxide absorption by our planet's oceans.

Results of the study were published online in February by the journal Icarus.

Final Titan Flyby Nears

Cassini will make its final close flyby of Titan -- its 127th targeted encounter -- on April 22. During the flyby, Cassini will sweep its radar beam over Titan's northern seas one final time. The radar team designed the upcoming observation so that, if magic island features are present this time, their brightness may be useful for distinguishing between bubbles, waves and floating or suspended solids.

The flyby also will bend the spacecraft's course to begin its final series of 22 plunges through the gap between Saturn and its innermost rings, known as Cassini's Grand Finale. The 20-year mission will conclude with a dive into Saturn's atmosphere on Sept. 15.

The Cassini-Huygens mission is a cooperative project of NASA, ESA (European Space Agency) and the Italian Space Agency. NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. JPL designed, developed and assembled the Cassini orbiter.

More information about Cassini:

http://www.nasa.gov/cassini

http://saturn.jpl.nasa.gov

http://www.esa.int/Our_Activities/Space_Science/Cassini-Huygens

Images (mentioned), Text, Credits: NASA//JPL/Preston Dyches.

Greetings, Orbiter.ch

GRACE Mission: 15 Years of Watching Water on Earth











NASA - GRACE Mission patch.

March 15, 2017

Fast Facts:

- In 15 years of operations, the GRACE satellite mission has revolutionized our view of how water moves and is stored on Earth.

- GRACE measures changes in the local pull of gravity as water shifts around Earth due to changing seasons, weather and climate processes.

- Among other innovations, GRACE gave us the first space-based view of water beneath Earth's surface, giving insight into where aquifers may be shrinking or dry soils contributing to drought.

- The GRACE Follow-On mission, launching in early 2018, will extend GRACE's innovative measurements.


"Revolutionary" is a word you hear often when people talk about the GRACE mission. Since the twin satellites of the U.S./German Gravity Recovery and Climate Experiment  launched on March 17, 2002, their data have transformed scientists' view of how water moves and is stored around the planet.

"With GRACE, we effectively created a new field of spaceborne remote sensing: tracking the movement of water via its mass," said Michael Watkins, the original GRACE project scientist and now director of NASA's Jet Propulsion Laboratory, Pasadena, California.

Like many other transformations, GRACE began with an insight. "The completely new idea about GRACE was the perception that measuring mass gives you a way to probe the Earth system," said Principal Investigator Byron Tapley, director of the Center for Space Research and professor in the Cockrell School of Engineer at The University of Texas at Austin. Measuring changes in mass has been a key to discovering how water and the solid Earth are changing in places humans can't go or can't see.

15 Years of GRACE Earth Observations

The Weight of Water

The greater an object's mass, the greater its gravitational pull. For example, the massive Rocky Mountains exert more gravitational pull than the flat plains of the Midwest. Humans don't notice the tiny difference, but satellites do. While orbiting Earth, satellites accelerate very slightly as they approach a massive feature, and slow down as they move away.

The vast majority of Earth's gravitational pull is due to the mass of Earth's interior. A small part, however, is due to the mass of water on or near Earth's surface. The ocean, rivers, glaciers and underground water change much more rapidly than Earth's interior does, responding to changing seasons, storms, droughts and other weather and climate effects. GRACE grew from the recognition that a specially designed mission could observe these changes in water from space, revealing hidden secrets of the water cycle.

GRACE measures changes in mass through their effects on twin satellites orbiting one behind the other about 137 miles apart (220 kilometers). The small accelerations and decelerations caused by changing mass below the spacecraft alter the distance between them very slightly -- by a few microns (a fraction of the diameter of a human hair). To measure this ever-changing distance, the spacecraft constantly beam microwave pulses at each other and time the arrival of returning signals. GPS keeps track of where the spacecraft are relative to Earth's surface, and onboard accelerometers record forces on the spacecraft other than gravity, such as atmospheric drag and solar radiation. Scientists process these data to produce monthly maps of regional variations in global gravity, showing how water on or near Earth's surface has moved every month.

When NASA selected this complex, high-precision mission for launch under its Earth System Science Pathfinder program, "A lot of people thought it was a bit improbable that we could actually bring it off," Tapley said. He credits the mission's success to a close collaboration between NASA and two German partners, the Deutsches Zentrum für Luft- und Raumfahrt (DLR, the German Aerospace agency) and the Helmholtz Centre Potsdam German Research Centre for Geosciences (GFZ), with leadership from original co-principal investigator Christoph Reigber and project manager Frank Flechtner of GFZ. The collaboration has run very smoothly, according to Flechtner, who has now taken the role of GRACE's German co-principal investigator. "It's as if we are one family on both sides of the Atlantic."

GRACE was built in Germany at Airbus Defense and Space. DLR procured a Russian "Rockot" as the launch vehicle. GFZ is involved in the U.S./German Science Data System and mission operations at DLR´s German Space Operations Center. GRACE ground segment operations are currently co-funded by GFZ and the European Space Agency (ESA). NASA, ESA, GFZ and DLR are supporting the continuation of the measurements of mass redistribution in the Earth system.

What GRACE Has Taught Us

Here are a few highlights of discoveries from GRACE during its 15 years of operation. These discoveries reflect the work of researchers worldwide, who have developed innovative techniques to use the data and combine it with other observations and models for new insights into the Earth system.

Underground water: Water stored in soil and aquifers below Earth's surface is very sparsely measured worldwide. In describing GRACE's contribution to understanding this life-giving resource, JPL Senior Water Scientist Jay Famiglietti said, "I can't think of another set of measurements that have so revolutionized the science."

Hydrologist Matt Rodell of NASA's Goddard Space Flight Center, Greenbelt, Maryland, did his doctoral research on GRACE's hydrological uses. Rodell said no one guessed before launch that GRACE would reveal unknown groundwater depletion, but over the last decade, he, Famiglietti and other researchers have found more and more locations where humans are pumping out groundwater faster than it is replenished. In 2015, their team published a comprehensive survey showing a third of Earth's largest groundwater basins are being rapidly depleted.

Dry soils can add to drought risk or increase the length of a drought. Rodell and his team provide GRACE data on deep soil moisture and groundwater to the National Drought Mitigation Center each week, using a hydrology model to calculate how the moisture is changing throughout the month between one map and the next. The data are used in preparing weekly maps of U.S. drought risk.

Artist's concept of Grace. Image credits: NASA/JPL

Melting ice sheets: Antarctica is one of the world's toughest places to collect data, and Greenland isn't far behind. Yet we need to know how fast these ice sheets are melting to better understand rates and variations of sea level rise around the world. Scientists studying ice sheets and glaciers were among the first to start working with GRACE data to extract the information they needed. In the mid-2000s, Jianli Chen (University of Texas at Austin); Isabella Velicogna (University of California, Irvine); and the late John Wahr showed that ice losses from Greenland and Antarctica were dramatically larger than previously estimated, using estimates of the changing height of the ice sheets and other types of data. Since GRACE launched, its measurements show Greenland has been losing about 280 gigatons of ice per year on average -- a bit less than twice the weight of Mt. Everest -- and Antarctica has lost slightly under 120 gigatons a year. There are indications that both melt rates are increasing.

Sea level: The sea level is rising both because melting ice from land is flowing into the ocean and because seawater is expanding as it warms. Scientists have a very precise, continuous measurement of sea level heights worldwide beginning in 1992 with the NASA-French Topex-Poseidon mission and continuing through the Jason series of sea level altimetry missions. The altimeter measurements, however, see only the full effect of ocean height changes from all causes -- warming, ice melting and runoff from land. To get an in-depth view of the processes responsible for the changes, scientists need to know how much of the full effect is due to each one.

With GRACE, scientists are able to distinguish between changes in water mass and changes in ocean temperatures. An example of the value of this ability is a study led by GRACE Project Scientist Carmen Boening of JPL, which both documented and explained a significant drop in sea level with the 2011 La Niña event. The study showed that the water that left the ocean, causing the drop in sea level, was rained out over Australia, South America and Asia. The finding gave scientists a new view on the global water cycle.

Solid Earth changes: The viscous mantle under Earth's crust is also moving ever so slightly in response to mass changes from water near the surface. GRACE has a community of users that calculate these shifts for their research. JPL scientists Surendra Adhikari and Erik Ivins recently used GRACE data to calculate how ice sheet loss and groundwater depletion have actually changed the rotation of Earth as the system adjusts to these movements of mass.

GRACE's planners didn't have much hope that the mission's measurement could be used to pinpoint the abrupt changes in mass associated with large earthquakes because of the difference in scale: earthquakes are sudden and local, whereas GRACE's monthly maps average over an area the size of Illinois and an entire month of time. However, by devising new data processing and modeling techniques, researchers have found a way to isolate the earthquake effects. "We're able to measure the instantaneous mass shift in an earthquake, and we've found there's a very measurable relaxation that goes on for one or two months after the earthquake," Tapley said. These measurements provide unprecedented insights into what is happening far below Earth's surface in big quakes such as the 2004 Sumatra event and 2011 Tohuku (Japan) quake, both of which caused devastating tsunamis.

The Future

At 15 years, GRACE has lasted three times as long as originally planned. Project managers have done everything possible to extend its life, but the spacecraft will run out of fuel soon -- probably this summer. NASA and GFZ have been working since 2012 on a second GRACE mission called GRACE Follow-On (GRACE-FO), with Germany again procuring a launch vehicle and the twin satellites built at Airbus in Germany. "With GRACE, we have gained new insight into how global and regional water resources are evolving," said Frank Webb, the GRACE-FO project scientist. "Through GRACE-FO, we will extend into the next decade our capacity to gain an accurate picture of the global water cycle."

GRACE-FO is scheduled for launch between December 2017 and February 2018. The new mission focuses on continuing GRACE's successful data record. The new satellites use similar hardware to GRACE and will also carry a technology demonstrator with a new laser ranging instrument to track the separation distance between the satellites.  The laser instrument has the potential to produce an even more accurate measurement.

"GRACE-FO allows us to continue the revolutionary legacy of GRACE," said JPL's Watkins. "There are sure to be more unexpected and innovative findings ahead."

Related links:

Weekly maps of U.S. drought risk: http://droughtmonitor.unl.edu/

GRACE data on deep soil moisture and groundwater: http://drought.unl.edu/MonitoringTools/NASAGRACEDataAssimilation.aspx

National Drought Mitigation Center: http://drought.unl.edu/

Topex-Poseidon: https://sealevel.jpl.nasa.gov/missions/topex/

GRACE Follow-On (GRACE-FO): https://gracefo.jpl.nasa.gov/

For more information on GRACE:

http://grace.jpl.nasa.gov

http://www.csr.utexas.edu/grace

Images (mentioned), Video, Text, Credits: NASA Earth Science News Team, written by Carol Rasmussen/JPL/Alan Buis/University of Texas/Sandra Zaragoza.

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