Explore the Universe with Science@ESA

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If you’re looking for some superb space and astronomy vodcasts, ESA has produced a series of informative video podcasts that explore our Universe as seen through the “eyes” of ESA’s fleet of science spacecraft. “The Science@ESA podcast series was started as part of an education and public outreach project for the International Year of Astronomy,” said Dr. Salim Ansari, from ESA’s Directorate of Science and Robotic Exploration, “but it will continue on past IYA, continuing to cover more missions and discoveries.”

The series is a high quality video podcast with HD graphics and stunning visuals. Ansari said the production all done in house.

“One of my favorites is actually the first podcast that shows how with our eyes we see just a small portion of the electromagnetic spectrum,” Ansari said. “But we demonstrate how the different spacecraft can provide insight across the whole spectrum.”
ESA podcast screenshot.
Other podcasts delve into specifics of the electromagnetic spectrum that will be explored by the new Planck (microwave) and Herschel (infrared) spacecraft, to learning about the Gaia galaxy mapper mission that will determine the position of a billion stars.

A new 7th podcast will be released next week that introduces the solar system as seen by the Venus Express, Mars Express, Rosetta, Cassini-Huygens, SoHO and Cluster.

See the Science@ESA page for a complete list of podcasts.

NASA and ESA Sign Mars Exploration Joint Initiative

NASA and the European Space Agency (ESA) have officially agreed to combine their efforts in the exploration and study of Mars. The heads of both agencies, NASA administrator Charles Boden and ESA director-general Jean-Jacques Dordain signed an agreement that officially binds the two agencies together for upcoming orbiter and rover missions. Discussions of this cooperation began in December of 2008, and culminated in a meeting in June 2009, out of which came the official agreement signed last week.

The new “letter of intent” outlines the Mars Exploration Joint Initiative (MEJI), under which mission engineers will cooperate in the design and launch of rovers, orbiters and landers into the 2020s, with the ultimate goal of returning rocks from Mars to Earth for study. The first collaborative mission is a European-led orbiter that will also place a meteorological station on Mars planned for 2016. This will be followed by surface rovers to keep Spirit and Opportunity company (c’mon, you know they’ll still be ticking!) in 2018, and possibly a network of landers shortly after in 2018, one of which will include the ESA’s ExoMars Lander.

NASA will take care of the launching rockets for 2016 and 2018, and the ESA will cover the entry, descent and landing for the first mission in 2016.

The signing of this document makes official the talks held in Plymouth, UK this past June. Since the talks, most of the fine print has been worked out on the collaboration – this signing just seals the deal.

The ESA and NASA, both under financial constraints in their Mars exploration programs, envision this new union to allow both to to launch vehicles in the window that opens every 26 months for missions to Mars. NASA’s most recently planned mission to the Red Planet, the Mars Science Laboratory, missed the October 2009 window because of technical problems, so will have to be launched in 2011 instead. The same fate befell the ESA ExoMars lander, which has been postponed three times – until 2018 – from the initial launch date of 2009. This joint initiative aims at preventing such delays by sharing both engineering and financial responsibilities.

NASA’s associate administrator for science, Dr Ed Weiler, told the BBC back in July,”We have very similar scientific goals, maybe we ought to consider working together jointly on all our future Mars missions, so that we can do more than either one of us can do by ourselves.”

Hopefully, this collaboration will provide both administrations with the opportunity to get more science done for cheaper, and extend further the already amazing capabilities of proposed missions to the Red Planet.

Source: BBC, ESA

Rosetta to Make Final Earth Flyby Nov. 13th

The comet chasing spacecraft Rosetta will make its third and final swing by the Earth on November 13th to pick up more speed for the last part of a 10-year journey that lies ahead. Its mission is to place a lander on comet 67P/Churyumov-Gerasimenko and chase the comet for an entire year on its orbit around the Sun. The spacecraft will be visible to observers from the ground in certain locations on the Earth. This last flyby will increase the spacecraft’s speed by 3.6 km/s (2.2 miles/s) with respect to the Sun, giving Rosetta the energy it needs to boost it to the outer regions of the Solar System.

Rosetta was launched March 2nd, 2004, and will visit a host of targets on its way to comet 67P/Churyumov-Gerasimenko. Rosetta already paid a visit to asteroid 2867 Steins in September 2008. It will visit comet 21 Lutetia 10 June 2010, after which it will go into hibernation until it reaches its final destination in May 2014.

Once Rosetta arrives at 67P/Churyumov-Gerasimenko, it will deploy its Philae lander on the comet’s nucleus, and continue to orbit and study the comet for an entire year during its closest orbit of the Sun. This is the first mission ever to orbit and land on a comet, and promises to return a wealth of data on cometary interaction with the Sun. Comets also contain mostly undisturbed materials from the formation of the Solar System in their nuclei, so studying their composition gives scientists an look into how our Solar System developed.

During the flyby of Earth in November of 2007, Rosetta took the breathtaking image of the Earth pictured here. This next flyby will give observers on the ground a chance to take a look back at Rosetta. The closest approach will occur on November 13th at 8:45 Central European Time (07:45 UT).

Unfortunately, the spacecraft will only be visible from parts of Europe, South America and Africa, as can be seen in the image below. If you are in these regions during the approach, and have favorable conditions, there is a wealth of observing information on the Rosetta blog, specifically on the posts Tips for Sky Junkies I and Tips for Sky Junkies II. They will also be closely following the flyby on the blog, so you can check there for updates on the eve of the event if you are outside the observable range of the spacecraft.The regions where Rosetta will be visible to observers from the ground. Image Credit: ESA

As always, you can check back with us on Universe Today for more coverage of Rosetta’s journey!

Source: ESA

New ESA Rover Will Look For Life On Mars

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NASA’s Mars Exploration Rovers (MER) have been an outstanding success in their longevity and helping us to understand the role of water in Mars’ past. But Spirit and Opportunity don’t have the instruments on board to answer the question foremost in many people’s minds: Is there, or was there ever life on Mars?

A new spacecraft being readied by the European Space Agency (ESA) will have that ability. The rover for the ExoMars 2013 mission will have an on-board subsurface radar, a drill, and life-detection equipment as part of the scientific payload.

To help prepare for the mission, scientists at Aberystwyth University in Wales have simulated the surface of Mars in their lab to test the “roving” capabilities of the vehicle. Also being tested are the robotic arm for collecting samples and a panoramic camera.

The ExoMars mission will also have an orbiter that will scan for the best landing site for the rover. The rover is slated to travel to ten different locations in 6 months. The rover will use a radar system that can scan the surface and subsurface, a drill that can dig down 1-2 meters below the surface and gather a sample that will be brought to the onboard instruments that will look for life, past or present, in the Mars landscape.

A robotic arm that is part of this system is similar to arm that was part of the ill-fated Beagle 2 lander, that crashed on Mars surface in 2003. But the new arm has been improved, and it is hoped the arm will work with on-board cameras and to be able to acquire rock samples autonomously.

The rover will weigh about 140-180 kg, comparable to the NASA’s MER. The main scientific objectives of the ExoMars mission are to study the biological environment of Mars surface, to characterize the Mars geochemistry and water distribution and to identify possible surface hazards to future human missions.

The mission is scheduled to launch in 2013 and land on Mars in 2014.

Original News Source: BBC

A New Supply Ship for the ISS

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The International Space Station (ISS) depends on regular deliveries of food, air and water, as well as equipment and spare parts to keep the station and its occupants happy and in peak operating condition. Of course, the space shuttle brings supplies on its visits for construction and crew exchange missions, and the Russian Progress spacecraft faithfully brings supplies and equipment to the station approximately every six months. But beginning in February 2008 the ISS will have a new supply ship: Europe’s Automated Transfer Vehicle (ATV). The first of seven planned ships, known as the “Jules Verne,” is currently undergoing fueling to ready the craft for its journey to the space station. Launch is tentatively scheduled for February 22.

The ATV pressurized cargo carrier is based on the Italian-built Multi-Purpose Logistics Module (MPLM), (aka Leonardo, Donatello and Raffaello) which has already been carried to the station via the space shuttle as a “space barge,” transporting equipment to and from the station. The ATV, which is equipped with its own propulsion and navigation systems combines full automatic capabilities of an unmanned vehicle with human spacecraft safety requirements. Its mission in space will resemble the combination of a tugboat and a river barge.

Every 12 months or so, the ATV will haul 7.5 tons of cargo to the Station 400 km above the Earth. The ATV will launch on board a Arianne 5 rocket from Kourou, French Guiana. An automatic navigation system will guide the ATV on a rendezvous trajectory towards ISS, to automatically dock with the station’s Russian service module. The ATV will remain docked to the station as a pressurized “waste basket” for up to six months until its final mission: a fiery one-way trip into the Earth’s atmosphere to dispose of up to 6.5 tons of station waste.

The ATV is a cylinder 10.3 meters long and 4.5 meters in diameter. The exterior is covered with an insulating foil layer on top of anti-meteorite Whipple Shields. The X-shaped extended solar arrays look like a metallic blue wings. Inside, the ATV consists of two modules, the propulsion spacecraft and the integrated cargo carrier which docks with the ISS.

The ATV’s will become especially important during the time period between after the shuttles are retired and before the next generation of US space craft, can bring supplies and crew to the station. The ESA also sees the ATVs as a way for Europe to pay its share in ISS running costs. Depending on the operational lifetime of the Space Station, ESA will build at least 7 ATVs.

Original News Source: ESA Press Release

Ulysses Passes Over Sun’s North Pole

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Continuing on its epic journey around the Sun, Ulysses has reached the Sun’s north pole just in the nick of time. In fact, its timing couldn’t be better, just as the Sun begins “Solar Cycle 24”. The probe is in a unique orbit, passing over the solar north and south poles, out of the ecliptic plane of the solar system, giving it an unprecedented view of parts of the Sun we cannot observe on Earth. “Graveyards for sunspots” and mysterious coronal holes lurk in these regions and Ulysses will be perfectly placed, directly above.

The joint NASA and ESA Ulysses mission has been a resounding success in its 18 years of operation since launch on board Space Shuttle Discovery (STS-41) in October 1990. The intrepid spacecraft was helped on it’s way by a gravitational assist by the planet Jupiter which flung it over the poles of the Sun. Quietly travelling in a perpendicular orbit (space missions and the planets usually orbit around the Sun’s equator), Ulysses has been measuring the distribution of solar wind particles emanating from latitudinal locations for one and a half orbits.

As Ulysses passes over the north polar region, the Sun will be observed during a period of minimum activity at this location for the first time. The poles of the Sun are of particular interest to scientists as this is where the fast solar wind originates from open magnetic field lines reaching into space. The dynamics of solar material in this location provides information on how the Sun interacts with interplanetary space and how the solar wind is generated. Observing the solar wind at “solar minimum” will be of massive interest as it may provide some answers as to why the solar wind is accelerated hundreds of kilometers per hour even when activity is at its lowest.

Just as Earth’s poles are crucial to studies of terrestrial climate change, the sun’s poles may be crucial to studies of the solar cycle.” – Ed Smith, Ulysses project scientist, NASA Jet Propulsion Laboratory.

The dynamics of low altitude magnetic fields in polar regions are also a focus for interest. As 11-year solar cycles progress, sunspot population increase near the solar equator. As the magnetic field is “wound up”, sunspots (and their associated magnetic flux) drift toward the poles where they slowly disappear as the old magnetic field sinks back into the Sun, quite accurately described as sunspot graveyards. Understanding how this cycle works will help to reveal the secrets of the solar cycle and ultimately help us understand the mechanisms behind Space Weather.

Source: NASA Featured News