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Planck Space Telescope Sees Light Billions of Years Old

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The Planck space telescope has begun to collect light left over from the Big Bang explosion that created our universe.

The mission, which is led by the European Space Agency with important participation from NASA, will help answer the most fundamental of questions: How did space itself pop into existence and expand to become the universe we live in today? The answer is hidden in ancient light, called the cosmic microwave background, which has traveled more than 13 billion years to reach us. Planck will measure tiny variations in this light with the best precision to date.

The mission officially started collecting science data on Aug. 13, as part of a test period. If all goes as planned, these observations will be the first of 15 or more months of data gathered from two full-sky scans. Science results are expected in about three years.

Read about NASA and JPL’s role in the mission at http://www.nasa.gov/mission_pages/planck/overview.html
More information about the mission is also online at http://www.esa.int/SPECIALS/Planck/index.html .


ESA Astronaut Roberto Vittori to fly to ISS in 2010

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ESA astronaut Roberto Vittori from Italy has been assigned as a Mission Specialist to Space Shuttle mission STS-134, which is currently scheduled for launch to the International Space Station (ISS) in July or September 2010. This mission will deliver the Alpha Magnetic Spectrometer (AMS) to the Station.

Vittori’s flight opportunity stems from a bilateral agreement between the Italian space agency (ASI) and NASA involving the utilisation of the Italian-built Multi Purpose Logistics Modules.

It will be Roberto Vittori’s third flight into space and to the International Space Station, but his first on the Space Shuttle. In April 2002, Vittori spent 10 days on the ISS performing a concise experimental programme. Three years later, he returned to the Station for another 10 days this time to conduct an extensive programme consisting of 22 experiments. On both missions Roberto Vittori flew as a Flight Engineer on the Russian Soyuz spacecraft.

“This assignment underlines once again the strong and long-lasting cooperation between the European Space Agency and the Italian space agency,” said ESA Director General Jean-Jacques Dordain. “The choice of Roberto Vittori for this mission fits well with ESA’s plans for the utilisation of its astronaut corps, with an experienced astronaut capable of performing missions that suit the needs of both ESA and ASI, as well as those of the Italian Air Force.”

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(Above) Alpha Magnetic Spectrometer (AMS-02) integration activities in Geneva, Switzerland. AMS will be launched on STS-134.

“Roberto Vittori’s mission,” said Enrico Saggese, ASI President, “represents a further achievement resulting from the bilateral cooperation between ASI and NASA, in the framework of the agreement on the utilisation of the Italian modules Leonardo, Raffaello and Donatello, with the important support of the European Space Agency, and confirms Italy’s key role in what is such an ambitious international undertaking: the ISS programme.”

“After the two Soyuz flights in 2002 and 2005, I am now looking forward to flying in 2010 on the Space Shuttle,” said Roberto Vittori, adding, ”The ISS has changed considerably in the last few years. Most importantly, Europe’s Columbus space laboratory has been attached, allowing European scientists to conduct more and more experiments in conditions of weightlessness.” Vittori will be the first ESA astronaut from Italy to have flown on both the Shuttle and Soyuz.

“I am very satisfied with Roberto Vittori’s assignment to STS-134 along with the AMS experiment,” said ESA’s Director of Human Spaceflight Simonetta Di Pippo. “This is an important mission for science, for human spaceflight and for Europe and Italy in particular. As we demonstrate how critical the ISS can be in supporting great scientific quests, we are also marking two important achievements rooted in international cooperation: AMS, which is supported by 16 countries worldwide, and Vittori’s assignment, which is made possible by the cooperation between ASI, which owns the flight opportunity, ESA and NASA.”

“This is the second flight of a European astronaut scheduled for 2010,” Di Pippo added. “We have flown astronauts regularly in the last few years, even flying two missions a year since 2008. We are working very hard to secure and carry out those missions for the benefit of Europe and ESA’s Member States, and are committed to obtaining additional flight opportunities so as to exploit all our potential in terms of research, training and to gain even more experience. This assignment is further recognition of the level we and the European Astronaut Corps have attained and demonstrates the maturity human spaceflight has acquired in Europe. It is a very solid basis on which to prepare future cooperative undertakings in human spaceflight and exploration.”

The STS-134 mission will be commanded by NASA astronaut Mark Kelly. NASA astronaut Gregory H. Johnson will serve as the pilot. Mission Specialists are NASA astronauts Michael Fincke, Greg Chamitoff and Andrew Feustel. ESA astronaut Roberto Vittori will also serve as a Mission Specialist.

The flight will include three spacewalks and the installation of AMS to the exterior of the Space Station. Once attached to the right side of the Station’s truss, AMS will collect information from cosmic sources to search for evidence of anti-matter and further advance our knowledge of the Universe. Before its flight, AMS will arrive at ESA’s research and technology centre, ESTEC, in the Netherlands, in November 2009 to undergo an extensive three-month test campaign.


Ariane 5′s potential role in U.S. Human Space Flight

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Ariane 5 is available to support the future of U.S. space exploration, including cargo resupply flights for the International Space Station, along with missions to the Moon and Mars.

This was the message of Arianespace Chairman & CEO Jean-Yves Le Gall in a presentation to the Review of U.S. Human Space Flight Plans Committee, which was created to evaluate America’s future human spaceflight operations after the National Aeronautics and Space Administration’s (NASA) planned retirement of the Space Shuttle.

“Originally human-rated, the Ariane 5 has adapted to its present day role as the leading large capacity launch vehicle for satellite operators and international partners the world over,” Le Gall explained during his committee presentation in Washington, D.C. “The Ariane 5 can reach lunar orbit, the lunar surface, and Mars – objectives that are compatible with NASA’s exploration missions.”

Le Gall underscored Ariane 5’s payload capabilities and its maturity as a proven, capable heavy-lift launch vehicle. He noted that Ariane 5 has performed 45 launches to date, with 31 consecutive successes since 2003. The vehicle’s heavy-lift payload capacity enables it to deliver 20 metric tons to low Earth orbit, seven metric tons to lunar transfer orbit, and five metric tons to Mars.

Arianespace’s ability to meet customers’ mission timing requirements also was highlighted by Le Gall, who underscored the company’s flight rate of seven Ariane 5 missions per year, and the sustained manufacturing output – with 46 launch vehicles currently in production.

One key issue to be reviewed by the Review of U.S. Human Space Flight Plans Committee is resupply support for the International Space Station after the Space Shuttle’s removal from service. NASA has selected U.S. contractors to develop commercial cargo resupply services (CRS) to replace the capacity provided by Space Shuttle flights – but there is concern of a possible gap if these new systems cannot be ready in time. The result could be a shortfall of 3-12 metric tons in annual cargo delivery from 2010 to 2015.

Ariane 5 is able to offer gap-filler resupply services, Le Gall explained, having already demonstrated its capabilities by launching Europe’s first Automated Transfer Vehicle (ATV) to the International Space Station last year. With a liftoff mass of approximately 20,750 kg., the ATV is able to deliver 7,750 kg. of cargo to the orbital station – providing cargo, fuel, water, air and supplies for its crew.

“Ariane 5-ATV cargo resupply can offer gap-filler services until CRS providers fully meet NASA requirements, and this approach can sustain the architecture for future U.S. human spaceflight by ensuring utilization of the completed International Space Station,” Le Gall said. “Ariane 5 is fully available with 31 successes in a row – including last year’s perfect flight with the first ATV – which I feel is quite important, and this flight-proven system meets NASA’s space station resupply requirements.”

He added that Ariane 5 also continues the application of international collaboration for International Space Station operations, which is a point that has been stressed by at least one member of the Review of U.S. Human Space Flight Plans Committee.

Le Gall noted that Ariane 5’s operating base at the Spaceport is a modern facility that meets all Western safety standards. Located on NATO territory, its security is maintained at the same level as for NATO allies’ nuclear forces.


Reconciling Methane Variations on Mars

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Since the discovery of its presence in the Martian atmosphere, methane has remained an intriguing atmospheric component which source (either of biotic or abiotic origin) is not yet fully understood. The recently reported variations in the concentration of atmospheric methane have proven difficult to explain with 3-D numerical models of the atmosphere that include the known chemical and physical processes.

In a paper published this week in Nature, Franck Lefèvre and François Forget present their study to derive the implications of the observed methane concentrations on Mars and their variability. They conclude that there needs to be both an intense localised source of methane and a destruction mechanism that is much more efficient than the known atmospheric processes that break down methane.

Further, if this efficient destruction of methane occurs only close to the surface, these findings imply a very harsh environment for organic molecules to survive on the surface of Mars.

The Martian atmosphere is composed mainly of CO2 (95%), with nitrogen and argon forming the largest contributions to the remainder. Methane (CH4) was discovered to be among the other trace components as reported in 2004 from observations by both the PFS instrument on board Mars Express (Formisano et al.) and ground based telescopes (Krasnopolsky et al.). These observations also indicated that the distribution of methane was not uniform across the planet.

Explore this topic further at ESA.


SPACE WALLPAPER: Soyuz Docks with ISS Against Lunar Backdrop

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(Above) This digital painting is an ESA artist’s impression showing the Soyuz docking with ISS against a Lunar background.

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NASA & ESA Establish Joint Mars Exploration Initiative

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Last month the ESA Director of Science and Robotic Exploration, David Southwood, met NASA’s Associate Administrator for Science, Ed Weiler, in Plymouth, UK, to establish a framework for future exploration of the Red Planet.

The outcome of the bilateral meeting was an agreement to create a Mars Exploration Joint Initiative (MEJI) that will provide a framework for the two agencies to define and implement their scientific, programmatic and technological goals at Mars.

Discussions between ESA and NASA began in December 2008, driven by the ESA Ministerial Council’s recommendation to seek international cooperation to complete the ExoMars mission and to prepare further Mars robotic exploration missions. At the same time, NASA was reassessing its Mars Exploration Program portfolio after the launch of its Mars Science Laboratory was delayed from 2009 to 2011.

This provided ESA and NASA with an opportunity to increase cooperation and expand collective capabilities. To investigate the options in depth, a joint ESA/NASA engineering working group was established, along with a joint executive board to steer the efforts and develop final recommendations on how to proceed.

At the bilateral meeting in Plymouth, the executive board recommended NASA and ESA establish MEJI spanning launch opportunities in 2016, 2018 and 2020, with landers and orbiters conducting astrobiological, geological, geophysical and other high-priority investigations, and leading to the return of samples from Mars in the 2020s. The Director and Associate Administrator agreed, in principle, to establish the Initiative and continue studies to determine the most viable joint mission architectures.

ESA and NASA also agreed to establish a joint architecture review team to assist the agencies in planning the mission portfolio. As plans develop, they will be reviewed by ESA member states for approval and by the US National Academy of Sciences. This unique collaboration of missions and technologies will pave the way for exciting discoveries at Mars.


European ATV-2 bears the name ‘Johannes Kepler’

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In Bremen on Tuesday 7 July 2009, the second European space transporter, ATV-2 – developed in association with, and with the support of, the German Aerospace Center (Deutsches Zentrum für Luft- und Raumfahrt; DLR) – was presented to the public. It was officially given the name of the German astronomer and scholar Johannes Kepler.

In connection with the naming ceremony, the European Space Agency (ESA) and Astrium GmbH signed a contract for studying the further development of ATV technology. The Advanced Re-entry Vehicle (ARV) will have, in contrast to the ATV, the capability of performing a controlled re-entry into Earth’s atmosphere. The goal is that ARV should enable the return of freight and experiments from the ISS to Earth.

The European ATV space vehicles are carried into space by Ariane 5 ES launch vehicles and give the European spaceflight programme increased independence. The development of ARV would secure the operation and provisioning of the ISS. This will become important after the cessation of the NASA Space Shuttle program in 2010, when provisioning of the ISS will become dependent on the Russian Cosmodrome at Baikonur.

European contribution to the provisioning of the space station

Among others, the event was attended by the Chairman of the DLR Executive Board, Prof. Dr-Ing Johann-Dietrich Wörner, the Director General of the European Space Agency, Jean-Jacques Dordain, ESA Director of Human Spaceflight, Simonetta Di Pippo, the Mayor of Bremen, Jens Böhrnsen, and the head of the space transport division at EADS Astrium, Alain Charmeau. Frank de Winne, the first European commander of the International Space Station (ISS), was also involved in the event.

The ATV-2 ‘Johannes Kepler’ is currently being completed at Astrium in Bremen and is scheduled to lift off in November 2010 from Kourou, French Guiana, en route to the ISS. These ATV flights are the European contribution towards keeping the ISS provisioned. The bulk of Europe’s share of the ISS operating costs is being met through these practical contributions rather than through foreign currency payments to NASA. Following the successful and spectacular premiere of the ATV-1 ‘Jules Verne’ on 9 March 2008, a further four ATV flights are scheduled between now and 2013.


Ulysses Spacecraft Ends Historic Mission of Discovery

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(Above) Ulysses team members bid the spacecraft a fond farewell.

Ulysses, a joint NASA and European Space Agency mission, officially ceased operations today, after receiving commands from ground controllers to do so. The spacecraft, which operated for more than 18 years, charted the unexplored regions of space above the poles of the sun.

As planned via commands beamed to the spacecraft earlier in the day, Ulysses switched to its low-gain antenna at 1:09 p.m. PDT (4:09 p.m. EDT, or 2009 UTC). As a result, ground controllers were no longer able to pick up a signal from Ulysses, which had also been commanded to switch off its transmitter completely at 1:15 p.m. PDT (4:15 p.m. EDT, or 2015 UTC).

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When space shuttle Discovery launched Ulysses on Oct. 6, 1990, it had an expected lifetime of five years. The mission gathered unique information about the heliosphere, the bubble in space carved by the solar wind, for nearly four times longer than expected.

“This has been a remarkable scientific endeavor,” said Richard Marsden, Ulysses mission manager and project scientist at the European Space Agency. “The results Ulysses obtained have exceeded our wildest dreams many times over.”

Ulysses made nearly three complete orbits of the sun. The probe revealed for the first time the three-dimensional character of galactic cosmic radiation, energetic particles produced in solar storms and the solar wind. Not only has Ulysses allowed scientists to map constituents of the heliosphere in space, its longevity enabled them to observe the sun over a longer period of time than ever before.

“The sun’s activity varies with an 11-year cycle, and now we have measurements covering almost two complete cycles,” said Marsden. “This long observation has led to one of the mission’s key discoveries, namely that the solar wind has grown progressively weaker during the mission and is currently at its weakest since the start of the Space Age.”

In addition to measuring the solar wind and charged particles, Ulysses instruments measured small dust particles and neutral gases from local interstellar space that penetrate into the heliosphere. Ulysses had an unprecedented three chance encounters with comet tails, registered more than 1,800 cosmic gamma-ray bursts, and provided findings for more than 1,000 scientific articles and two books.

“The breadth of science addressed by Ulysses is truly astonishing,” said Ed Smith, Ulysses project scientist at NASA’s Jet Propulsion Laboratory in Pasadena, Calif. “The data acquired during the long lifetime of this mission have provided an unprecedented view of the solar activity cycle and its consequences and will continue to keep scientists busy for many years to come.”

Ulysses’ successes have not been confined to scientific data. The extended mission presented significant challenges to the NASA-European operations team. In particular, critical parts of the spacecraft became progressively colder with time. In recent years, a major effort was needed to prevent the onboard hydrazine fuel from freezing. The operations team continually created methods to allow the aging space probe to continue its scientific mission.

Earlier this month, the Ulysses mission team received a NASA Group Achievement Award. Another milestone was reached on June 10 when Ulysses became the longest-running ESA-operated spacecraft, overtaking the International Ultraviolet Explorer which logged 18 years and 246 days of operations.

“The Ulysses team performed exceptionally by building and operating a research probe that would return scientific data for analysis no matter what challenges it encountered,” said Arik Posner, Ulysses program scientist at NASA Headquarters in Washington. “The knowledge gained from Ulysses proves what can be achieved through international cooperation in space research.”

The Ulysses orbital path is carrying the spacecraft away from Earth. The ever-widening gap has progressively limited the amount of data transmitted. Ulysses project managers, with the concurrence of ESA and NASA, decided it was an appropriate time to end this epic scientific adventure.

ESA Ulysses Mission Operations Manager Nigel Angold points out that more than a year ago, “We had estimated Ulysses would not survive further than July 2008. However, the spacecraft didn’t stop surprising us and kept working a full year, collecting invaluable science data. It’s nice to be going out in style.”

After the spacecraft was placed into low Earth orbit in 1990, a combination of solid fuel motors propelled Ulysses toward Jupiter. Ulysses swung by Jupiter on Feb. 8, 1992. The giant planet’s gravity bent the spacecraft’s flight path southward and away from the ecliptic plane, putting the probe into a final orbit that would take it over the sun’s south and north poles.

The European Space Agency’s European Space Research and Technology Centre and European Space Operations Centre managed the mission in coordination with the Jet Propulsion Laboratory. Ulysses is tracked by NASA’s Deep Space Network. A joint ESA/NASA team at JPL oversaw spacecraft operations and data management. Teams from universities and research institutes in Europe and the United States provided the 10 instruments on board.


Herschel Space Observatory Opens Its Infrared Eyes

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(Above) Glowing light from clouds of dust and gas around and between the stars is visible clearly. These clouds are a reservoir of raw material for ongoing star formation in this galaxy. Blue indicates regions of warm dust that is heated by young stars, while the colder dust shows up in red.

The Herschel Space Observatory has snapped its first picture since blasting into space on May 14, 2009. The mission, led by the European Space Agency with important participation from NASA, will use infrared light to explore our cosmic roots, addressing questions of how stars and galaxies are born.

The new “sneak preview” image was taken in an early attempt to demonstrate that Herschel works, and, in particular, that its telescope is focused and correctly aligned with the science instruments, and to whet our appetites for what’s yet to come. It shows the Whirlpool galaxy, which lies relatively nearby, about 35 million light-years away, in the constellation Canes Venatici.

The galaxy was first observed by Charles Messier in 1773, who gave the beauty its official name of Messier 51. Back then, astronomers, including William Herschel, the observatory’s namesake, catalogued objects like these as fuzzy nebulae without knowing their true nature. Later, Messier 51 became one of the first of these fuzzy objects observed to have a spiral structure, a finding that eventually led to the revelation that galaxies full of stars exist far from our own.

The image is a composite of infrared light captured with Herschel’s Photoconductor Array Camera and Spectrometer at three wavelengths: 70, 100 and 160 microns. Herschel’s full wavelength range spans 55 to 672 microns. The blue and white areas show where stars are actively forming, while the brown regions contain cold dust. The brightest blue dot at top left is a smaller, companion galaxy.

Longer-wavelength light inherently does not produce pictures with resolution as high as those obtained at shorter wavelengths, such as visible light. However, because Herschel’s mirror is the largest infrared astronomy mirror ever launched in space (3.5 meters, or about 11.5 feet across), it can take the sharpest pictures to date at the particular wavelengths it observes.

During its prime mission phase, NASA’s Spitzer Space Telescope, also a space-based infrared telescope, could see shorter-wavelength light, with wavelengths ranging from 3.6 to 160 microns. Because the two telescopes are able to see, for the most part, different wavelengths of light, their results complement each other, highlighting the multifaceted features of cosmic objects. Spitzer’s shorter-wavelength infrared view of the Whirlpool galaxy, in comparison to a visible-light view, can be seen here.

Herschel is in the final stretches of its journey to the second Lagrange point of the Earth-sun system. The observatory will spend its lifetime, estimated to be at least three-and-a-half-years, orbiting this point, which is about 1.5 million kilometers (930,000 miles) from Earth on the opposite side of our planet from the sun. After a cover protecting the telescope’s instruments was popped open on June 14, engineers and scientists commanded the telescope to take its first test picture. The telescope is still being commissioned, with science observations expected to begin later this year.

Herschel is a European Space Agency cornerstone mission, with science instruments provided by a consortia of European institutes and with important participation by NASA. NASA’s Herschel Project Office is based at NASA’s Jet Propulsion Laboratory. JPL contributed mission-enabling technology for two of Herschel’s three science instruments. The NASA Herschel Science Center, part of the Infrared Processing and Analysis Center at the California Institute of Technology in Pasadena, supports the United States astronomical community. Caltech manages JPL for NASA.


Joint ESA/NASA Ulysses Mission to End

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(Above) Artist’s concept of Ulysses moving towards the Sun

Upon receipt of the last command from Earth, the transmitter on Ulysses will switch off on 30 June, bringing one of the most successful and longest missions in spaceflight history to an end.

After 18.6 years in space and defying several earlier expectations of its demise, the joint ESA/NASA solar orbiter Ulysses will achieve ‘end of mission’ on 30 June 2009. The final communication pass with a ground station will start at 17:35 CEST and run until 22:20 CEST (15:35-20:20 UTC) or until the final command is issued to switch the satellite’s radio communications into ‘monitor only’ mode. No further contact with Ulysses is planned.

Ulysses is the first spacecraft to survey the environment in space above and below the poles of the Sun in the four dimensions of space and time. Among many other ground-breaking results, the hugely successful mission showed that the Sun’s magnetic field is carried into the Solar System in a more complicated manner than previously believed. Particles expelled by the Sun from low latitudes can climb up to high latitudes and vice versa, even unexpectedly finding their way down to planets.

Expanding our understanding of the Sun

This is very important as regions of the Sun not previously considered as possible sources of hazardous particles for astronauts and satellites must now be taken into account and carefully monitored.

“Ulysses has taught us far more than we ever expected about the Sun and the way it interacts with the space surrounding it,” said Richard Marsden, ESA’s Ulysses Project Scientist and Mission Manager.

The shut-down of the satellite is a joint decision of the two agencies and comes a year after the mission was expected to end.

Weakened power supply

A year ago, the satellite’s power supply had weakened to the point that it was thought the low temperatures would cause the fuel lines to freeze up, rendering Ulysses uncontrollable.

This didn’t happen immediately and spacecraft controllers realised that they could keep the fuel warm and circulating by performing a short thruster burn every two hours, an ingenious solution that has enabled Ulysses’ science mission to continue. It was decided to maintain the spacecraft in operation using NASA’s 70 m-diameter ground station network allocated on a ‘spare-capacity’ basis.

But as Ulysses has moved further from Earth, the communications bit-rate has gone down while other demands for the 70 m-diameter Deep Space Network stations have gone up. Most importantly, the overall return of scientific data has decreased to a level where it is hard to justify the cost of keeping Ulysses in operation.

Longevity a tribute to builders and operators

“We expected the spacecraft to cease functioning much earlier. Its longevity is a tribute to Ulysses’s builders and the people involved in operations over the years,” says Paolo Ferri, Head of the Solar & Planetary Missions Division at ESA’s European Space Operations Centre, Darmstadt, Germany.

He added that, “Although it is always hard to take the decision to terminate a mission, we have to accept that the satellite is running out of resources and a controlled switch-off is the best ending.”

Final mission operations will be conducted from the Ulysses Mission Support Area (MSA) located at NASA’s Jet Propulsion Laboratory in California, USA. The joint team will include Nigel Angold, ESA Mission Operations Manager, and Ed Massey, NASA Project Manager, as well as a number of engineers and analysts from both Agencies.

“Tuesday will be a very sad day when we send the last commands to Ulysses,” said Angold. “But I’m very proud that we have overcome the many challenges that have come our way over the course of nearly two decades. Its longevity is an indication of the desire for international collaboration on space missions. ESA and NASA are to be commended for supporting this unique mission until the very end,” he added.

After shut-off, Ulysses will continue to orbit the Sun, becoming in effect a man-made ‘comet’.

“Whenever any of us look up in the years to come, Ulysses will be there, silently orbiting our star, which it studied so successfully during its long and active life,” said Marsden.


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