lundi 2 mai 2016
The Dew Drop of Saturn
NASA - Cassini International logo.
May 2, 2016
The water-world Enceladus appears here to sit atop Saturn's rings like a drop of dew upon a leaf. Even though it appears like a tiny drop before the might of the giant Saturn, Enceladus reminds us that even small worlds hold mysteries and wonders to be explored.
By most predictions prior to Cassini's arrival at Saturn, a moon the size of Enceladus (313 miles, 504 kilometers across) would have been expected to be a dead, frozen world. But Enceladus displays remarkable geologic activity, as evidenced by the plume emanating from its southern polar regions and its global, subsurface ocean. (For a closer look at individual jets that contribute to the plume, see PIA11688; for more on the subsurface ocean see PIA19656.) The plume, which was discovered in Cassini images, is comprised mostly of water vapor and contain entrained dust particles.
This view looks toward the unilluminated side of the rings from about 0.3 degrees below the ring plane. The image was taken with the Cassini spacecraft wide-angle camera on May 25, 2015 using a spectral filter which preferentially admits wavelengths of near-infrared light centered at 728 nanometers.
The view was obtained at a distance of approximately 930,000 miles (1.5 million kilometers) from Saturn. Image scale is 54 miles (87 kilometers) per pixel.
The Cassini mission is a cooperative project of NASA, ESA (the European Space Agency) and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the mission for NASA's Science Mission Directorate, Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging operations center is based at the Space Science Institute in Boulder, Colorado.
For more information about the Cassini-Huygens mission visit http://saturn.jpl.nasa.gov and http://www.nasa.gov/cassini. The Cassini imaging team homepage is at http://ciclops.org and ESA's website: http://www.esa.int/Our_Activities/Space_Science/Cassini-Huygens
Image, Text, Credits: NASA/JPL-Caltech/Space Science Institute/Tony Greicius.
Greetings, Orbiter.ch
SolarImpulse - Takeoff to Phoenix Confirmed
SolarImpulse - Around The World patch.
May 2, 2016
André Borschberg will takeoff on May 2nd at 12:00PM UTC
After a week of rest at Moffett Airfield, Mountain View, California, Si2 is ready for the next adventure with André Borschberg. André will takeoff on May 2nd at 12:00PM UTC, 2:00PM CET, 5:00AM PT to continue the round-the-world solar flights across America. We have found a clear weather window that will bring us over the Mojave Desert to Phoenix Goodyear Airport. This will take an estimated 16 hours, crossing over 720 miles.
Si2 at Moffett Airfield, Mountain View, California
Step into the shoes of a Solar Impulse team member and watch this 360 video. You no longer have to be a spectator - sit back, plug your headphones in, and immerse yourself in our vision of today as we share our experience at Solar Impulse with you. This will bring you one step closer to flying in a solar airplane and perhaps one day, you will also feel the breeze.
360 video - Solar Impulse, Explorers Of The Impossible
Video above: 360 video: immerse yourself in a Solar Impulse takeoff next to our pilots, Bertrand Piccard and André Borschberg.
For more information about SolarImpulse Around The World, visit: http://blog.solarimpulse.com/
Image, Video, Text, Credits: SolarImpulse.
Best regards, Orbiter.ch
Second ExoMars mission moves to next launch opportunity in 2020
ESA & ROSCOSMOS - ExoMars Mission logo.
2 May 2016
On 14 March 2016, the Roscosmos State Corporation and the European Space Agency (ESA) launched the jointly-developed ExoMars 2016 interplanetary mission, comprising the Trace Gas Orbiter (TGO) and the Schiaparelli lander, on a Proton rocket from Baikonur, thus marking the first phase in the European-Russian ExoMars cooperation programme.
The success achieved by Russian and European experts involved in ExoMars 2016 is the result of long and fruitful cooperation. The ExoMars 2016 spacecraft are due to arrive at Mars in October 2016.
The second ExoMars mission involves a Russian-led surface platform and a European-led rover, also to be launched on a Proton from Baikonur. Russian and European experts made their best efforts to meet the 2018 launch schedule for the mission, and in late 2015, a dedicated ESA-Roscosmos Tiger Team, also including Russian and European industries, initiated an analysis of all possible solutions to recover schedule delays and accommodate schedule contingencies.
Trace Gas Orbiter, Schiaparelli and the ExoMars rover at Mars
The Tiger Team presented its final report during a meeting of the Joint ExoMars Steering Board (JESB) held in Moscow. Having assessed the possible ways to ensure successful mission implementation, the JESB concluded that, taking into account the delays in European and Russian industrial activities and deliveries of the scientific payload, a launch in 2020 would be the best solution.
ESA Director General Johann-Dietrich Woerner and Roscosmos Director General Igor Komarov discussed the ExoMars 2018 situation. After considering the Tiger Team report and the JESB recommendations, they jointly decided to move the launch to the next available Mars launch window in July 2020, and tasked their project teams to develop, in cooperation with the industrial contactors, a new baseline schedule aiming towards a 2020 launch. Additional measures will also be taken to maintain close control over the activities on both sides up to launch.
The successful implementation of both ExoMars missions will allow Russia and Europe to jointly validate cutting-edge technologies for Mars entry, descent, and landing, for the control of surface assets, to develop new engineering concepts and service systems that can be used by other Solar System exploration missions, and to carry out novel science at Mars.
Both Directors General have reiterated their resolve to implement ExoMars programme successfully and step up Russian-European cooperation in Solar System exploration.
Related links:
Robotic exploration of Mars: http://exploration.esa.int/
ExoMars mission: http://www.esa.int/Our_Activities/Space_Science/ExoMars
About ExoMars:
What is ExoMars?: http://www.esa.int/Our_Activities/Space_Science/ExoMars/What_is_ExoMars
Why are we going to Mars?: http://www.esa.int/Our_Activities/Space_Science/ExoMars/Why_are_we_going_to_Mars
More about...
ExoMars Factsheet: http://www.esa.int/Our_Activities/Space_Science/ExoMars/ExoMars_Factsheet
ExoMars frequently asked questions: http://www.esa.int/Our_Activities/Space_Science/ExoMars/ExoMars_frequently_asked_questions
ExoMars brochure: http://www.esa.int/About_Us/ESA_Publications/ESA_Publications_Brochures/ESA_BR-327_EXOMARS_2016
Image, Text, Credits: ESA/ATG medialab.
Greetings, Orbiter.ch
samedi 30 avril 2016
CERN: A weasel puts down the world's largest particle accelerator
CERN - European Organization for Nuclear Research logo.
April 30, 2016
It's not the little beast that will eat the fat, and yet ... Friday at CERN, a weasel has managed to bypass the largest particle accelerator in the world. The animal did not survive.
A weasel was introduced Friday in the Large Hadron Collider (LHC) at CERN in Geneva. It is the cause of a short circuit causing a failure in the largest particle accelerator in the world. The repairs will take several days.
The LHC has experienced "severe electrical disturbance Friday at 5:30," said the CERN (CERN) in his daily activity report. The failure is due to a "short circuit caused by a weasel" on the collider. A transformer 66 kV was damaged.
Large Hadron Collider (LHC) and the guilty of failure: the weasel
Asked by the BBC's Arnaud Marsollier, spokesman for CERN, said the repairs would take several days. The animal did not survive the shock. "It's not the best week for the LHC!" Said CERN's report.
The LHC, located on the French-Swiss border, includes a tunnel-shaped ring of 27 kilometers. This is the most powerful particle accelerator in the world. He has confirmed the existence of the Higgs boson in 2012, considered the cornerstone of the fundamental structure of matter. It could pierce other mysteries of the composition of the Universe.
Note:
CERN, the European Organization for Nuclear Research, is one of the world’s largest and most respected centres for scientific research. Its business is fundamental physics, finding out what the Universe is made of and how it works. At CERN, the world’s largest and most complex scientific instruments are used to study the basic constituents of matter — the fundamental particles. By studying what happens when these particles collide, physicists learn about the laws of Nature.
The instruments used at CERN are particle accelerators and detectors. Accelerators boost beams of particles to high energies before they are made to collide with each other or with stationary targets. Detectors observe and record the results of these collisions.
Founded in 1954, the CERN Laboratory sits astride the Franco–Swiss border near Geneva. It was one of Europe’s first joint ventures and now has 22 Member States.
For more information about the European Organization for Nuclear Research (CERN), visit: http://home.web.cern.ch/
Images, Text, Credits: CERN/ATS/Orbiter.ch Aerospace/Roland Berga.
Greetings, Orbiter.ch
vendredi 29 avril 2016
Pluto: A Global Perspective & New Elevation Map of Pluto’s Sunken ‘Heart’
NASA - Nwe Horizons Mission logo.
April 29, 2016
(Click on the image for enlarge)
Image above: Pluto: A Global Perspective. Image Credits: NASA/JHUAPL/SWRI.
NASA’s New Horizons mission science team has produced this updated panchromatic (black-and-white) global map of Pluto. The map includes all resolved images of Pluto’s surface acquired between July 7-14, 2015, at pixel resolutions ranging from 18 miles (30 kilometers) on the Charon-facing hemisphere (left and right edges of the map) to 770 feet (235 meters) on the hemisphere facing New Horizons during the spacecraft’s closest approach on July 14, 2015 (map center). The non-encounter hemisphere was seen from much greater range and is, therefore, in far less detail.
The latest images woven into the map were sent back to Earth as recently as April 25, and the team will continue to add photos as the spacecraft transmits the rest of its stored Pluto encounter data. All encounter imagery is expected on Earth by early fall. The team is also working on improved color maps.
New Elevation Map of Pluto’s Sunken ‘Heart’. Image Credits: NASA/JHUAPL/SWRI.
This newest shaded relief view of the region surrounding the left side of Pluto’s heart-shaped feature – informally named Sputnik Planum – shows that the vast expanse of the icy surface is on average 2 miles (3 kilometers) lower than the surrounding terrain. Angular blocks of water ice along the western edge of Sputnik Planum can be seen “floating” in the bright deposits of softer, denser solid nitrogen.
Topographic maps of Pluto are produced from digital analysis of New Horizons stereo images acquired during the July 14, 2015 flyby. Such maps are derived from digital stereo-image mapping tools that measure the parallax – or the difference in the apparent relative positions – of individual features on the surface obtained at different times. Parallax displacements of high and low features are then used to directly estimate feature heights.
These topographic maps are works in progress and artifacts are still present in the current version. The map is artificially illuminated from the south, rather than the generally northern solar lighting of landscape during the time of the flyby. One of the many advantages of digital terrain maps is that they can be illuminated from any direction to best bring out different features. North is up and the total relief in the scene is approximately 4 miles (6 kilometers) from the lowest to the highest features.
For more information about New Horizons, visit: http://www.nasa.gov/mission_pages/newhorizons/main/index.html
Images (mentioned), Text, Credits: NASA/Tricia Talbert.
Best regards, Orbiter.ch
NASA Research Gives New Insights into How the Moon Got 'Inked'
NASA - Lunar Reconnaissance Orbiter (LRO) patch.
April 29, 2016
A powerful combination of observations and computer simulations is giving new clues to how the moon got its mysterious "tattoos" -- swirling patterns of light and dark found at over a hundred locations across the lunar surface.
Image above: This is an image of the Reiner Gamma lunar swirl from NASA's Lunar Reconnaissance Orbiter. Image Credits: NASA LRO WAC science team.
"These patterns, called 'lunar swirls,' appear almost painted on the surface of the moon," said John Keller of NASA's Goddard Space Flight Center in Greenbelt, Maryland. "They are unique; we've only seen these features on the moon, and their origin has remained a mystery since their discovery." Keller is project scientist for NASA's Lunar Reconnaissance Orbiter (LRO) mission, which made the observations.
Lunar swirls can be tens of miles across and appear in groups or just as an isolated feature. Previous observations yielded two significant clues about their formation: First, they appear where ancient bits of magnetic field are embedded in the lunar crust (although not every "fossil" magnetic field on the moon has a lunar swirl). Second, the bright areas in the swirls appear to be less weathered than their surroundings. The space environment is harsh; many things can cause material exposed to space to change chemically and darken over time, including impacts from microscopic meteorites and the effects of the solar wind – a million-mile-per-hour stream of electrically conducting gas blown from the surface of the sun.
Those clues led to three prominent theories about how the swirls formed. The swirls and the magnetic fields could both have formed from plumes of material ejected by comet impacts. Alternatively, perhaps when fine dust particles get lofted by micrometeorite impacts, an existing magnetic field over the swirls sorts them according to their susceptibility to magnetism, forming light and dark patterns with different compositions. Finally, since particles in the solar wind (electrons and ions) are electrically charged, they respond to magnetic forces. Perhaps the magnetic field shields the surface from weathering by the solar wind.
In the new research, teams of scientists created computer models that provide new insights into how the magnetic shield hypothesis could work. "The problem with the magnetic shield idea is that the embedded magnetic fields on the moon are very weak – about 300 times weaker than Earth's magnetic field," said Bill Farrell of NASA Goddard. "It's hard to see how they would have the strength to deflect the solar wind ions." Farrell leads Goddard's DREAM-2 Center for Space Environments (Dynamic Response of the Environment at Asteroids, the Moon, and moons of Mars) which is funded by NASA's Solar System Exploration Research Virtual Institute (SSERVI) to conduct the model research.
Lunar Reconnaissance Orbiter (LRO). Image Credit: NASA
The new models reveal that the magnetic field can create a strong electric field when the solar wind attempts to flow through. It is this brawny electric potential of many hundreds of Volts that could deflect and slow particles in the solar wind. This would reduce the weathering from the solar wind, leaving brighter regions over protected areas. The new models are published separately as a series of three papers, one in Icarus on March 1, 2016 by lead author Andrew Poppe of the University of California at Berkeley; one in the Journal of Geophysical Research: Space Physics on June 18, 2015 by lead author Shahab Fatemi of University of California, Berkeley; and one in the Journal of Geophysical Research: Planets on November 25, 2015 by lead author Michael Zimmerman of The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland.
New observations from LRO appear to provide support for the magnetic shield hypothesis, but don't rule out the other ideas. "Until you have somebody making measurements on the lunar surface we may not get a definitive answer, but the new observations that analyze the swirls in ultraviolet and far-ultraviolet light are consistent with earlier observations that indicate the swirls are less weathered than their surroundings," said Keller. The new observations are the subject of two papers published in Icarus by lead author Brett Denevi of The Johns Hopkins University Applied Physics Laboratory, Laurel, Maryland on January 21, 2016 and lead author Amanda Hendrix of the Planetary Science Institute, Tucson, Arizona on February 4, 2016.
The DREAM-2 teams want to continue to develop their models to see how the magnetic shield responds to different strengths of the solar wind and various times of the lunar day, when the solar wind blows from different directions. They also want to model the physical and chemical processes of space weathering to better understand how it can change the lunar surface. The LRO team plans to modify the LAMP instrument (Lyman Alpha Mapping Project) on LRO to improve its signal-to-noise ratio for dayside observations, which will dramatically improve its ability to study this problem.
The research was funded by the LRO mission and the DREAM-2 center. DREAM-2 is part of SSERVI at NASA's Ames Research Center in California’s Silicon Valley. LRO is managed by NASA Goddard for the Science Mission Directorate at NASA Headquarters in Washington.
Related links:
NASA's Lunar Reconnaissance Orbiter (LRO): http://www.nasa.gov/mission_pages/LRO/main/index.html
DREAM-2 Center for Space Environments (Dynamic Response of the Environment at Asteroids, the Moon, and moons of Mars): http://ssed.gsfc.nasa.gov/dream/
NASA's Solar System Exploration Research Virtual Institute (SSERVI): http://sservi.nasa.gov/
Icarus on March 1, 2016: http://www.sciencedirect.com/science/article/pii/S0019103515005096
Journal of Geophysical Research: Space Physics on June 18, 2015: http://onlinelibrary.wiley.com/doi/10.1002/2015JA021027/full
Journal of Geophysical Research: Planets on November 25, 2015: http://onlinelibrary.wiley.com/doi/10.1002/2015JE004865/full
NASA's Ames Research Center: https://www.nasa.gov/centers/ames/home/index.html
Images (mentioned), Text, Credits: NASA's Goddard Space Flight Center/Bill Steigerwald.
Greetings, Orbiter.ch
Hubble Sees Galaxy Hiding in the Night Sky
NASA - Hubble Space Telescope patch.
April 29, 2016
This striking NASA/ESA Hubble Space Telescope image captures the galaxy UGC 477, located just over 110 million light-years away in the constellation of Pisces (The Fish).
UGC 477 is a low surface brightness (LSB) galaxy. First proposed in 1976 by Mike Disney, the existence of LSB galaxies was confirmed only in 1986 with the discovery of Malin 1. LSB galaxies like UGC 477 are more diffusely distributed than galaxies such as Andromeda and the Milky Way. With surface brightnesses up to 250 times fainter than the night sky, these galaxies can be incredibly difficult to detect.
Most of the matter present in LSB galaxies is in the form of hydrogen gas, rather than stars. Unlike the bulges of normal spiral galaxies, the centers of LSB galaxies do not contain large numbers of stars. Astronomers suspect that this is because LSB galaxies are mainly found in regions devoid of other galaxies, and have therefore experienced fewer galactic interactions and mergers capable of triggering high rates of star formation.
LSB galaxies such as UGC 477 instead appear to be dominated by dark matter, making them excellent objects to study to further our understanding of this elusive substance. However, due to an underrepresentation in galactic surveys — caused by their characteristic low brightness — their importance has only been realized relatively recently.
Hubble orbiting Earth
More information:
The Hubble Space Telescope is a project of international cooperation between ESA and NASA.
For images and more information about Hubble Space Telescope:
https://www.spacetelescope.org/
http://hubblesite.org/
http://www.nasa.gov/hubble
Text credits: European Space Agency (ESA)/NASA/Ashley Morrow/Image, Video, Credits: ESA/Hubble & NASA, Acknowledgement: Judy Schmidt.
Greetings, Orbiter.ch
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