Mostrando entradas con la etiqueta Astronomy. Mostrar todas las entradas
Mostrando entradas con la etiqueta Astronomy. Mostrar todas las entradas

domingo, 22 de julio de 2012

Astronomy: Celebrating Apollo 11

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG.,
Apollo 11 was the spaceflight which landed the first humans, Americans Neil Armstrong and Buzz Aldrin, on the Moon on July 20, 1969, at 20:18 UTC. Armstrong became the first to step onto the lunar surface 6 hours later on July 21 at 02:56 UTC. A third member of the mission, Michael Collins, remained alone in lunar orbit until they returned from the surface about 15 hours later. All 3 returned to Earth safely after travelling in space for 8 days.
Launched by a Saturn V rocket from Kennedy Space Center in Merritt Island, Florida on July 16, Apollo 11 was the fifth manned mission of NASA's Apollo program. The Apollo spacecraft had three parts: a Command Module with a cabin for the three astronauts which was the only part which landed back on Earth; a Service Module containing propulsion, electrical power, oxygen and water; and a Lunar Module for landing on the Moon. After being sent to the Moon by the Saturn V's upper stage, the astronauts separated the spacecraft from it and travelled for three days until they entered into lunar orbit. Armstrong and Aldrin then moved into the Lunar Module and landed in the Sea of Tranquility. They stayed a total of about 21½ hours on the lunar surface, including about 2½ hours outside the spacecraft. After lifting off in the upper part of the Lunar Module and rejoining Collins in the Command Module, they returned to Earth and landed in the Pacific Ocean on July 24.
Broadcast on live TV to a world-wide audience, Armstrong stepped onto the lunar surface and described the event as "one small step for [a] man, one giant leap for mankind." Apollo 11 effectively ended the Space Race and fulfilled a national goal proposed in 1961 by the late U.S. President John F. Kennedy in a speech before the United States Congress, "before this decade is out, of landing a man on the Moon and returning him safely to the Earth."[3] W
Wikipedia.
Landing site of Apollo 11 at Sea of Tranquility. Wikipedia
The Saturn V carrying Apollo 11 slowly rises past the launch tower camera. Wikipedia
The Eagle in lunar orbit after separating from Columbia. Wikipedia
A mounted slowscan TV camera shows Armstrong as he climbs down the ladder to surface. Wikipedia

Aldrin bootprint; part of an experiment to test the properties of the lunar regolith. Wikipedia.

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 Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com 
ayabaca@hotmail.com 
ayabaca@yahoo.com 

miércoles, 25 de abril de 2012

Astronomy: NASA Scientists Find History of Asteroid Impacts in Earth Rocks

Hi My Friends: A VUELO DE UN QUINDE EL BLOG., Research by NASA and international scientists concludes giant asteroids, similar or larger than the one believed to have killed the dinosaurs, hit Earth billions of years ago with more frequency than previously thought.

NASA Scientists Find History of Asteroid Impacts in Earth Rocks :
WASHINGTON -- Research by NASA and international scientists concludes giant asteroids, similar or larger than the one believed to have killed the dinosaurs, hit Earth billions of years ago with more frequency than previously thought.

To cause the dinosaur extinction, the killer asteroid that impacted Earth 65 million years ago would have been almost 6 miles (10 kilometers) in diameter. By studying ancient rocks in Australia and using computer models, researchers estimate that approximately 70 asteroids the same size or larger impacted Earth 1.8 to 3.8 billion years ago. During the same period, approximately four similarly-sized objects hit the moon.

"This work demonstrates the power of combining sophisticated computer models with physical evidence from the past, further opening an important window to Earth's history," said Yvonne Pendleton, director of NASA's Lunar Science Institute (NLSI) at NASA's Ames Research Center at Moffett Field, Calif.

Evidence for these impacts on Earth comes from thin rock layers that contain debris of nearly spherical, sand-sized droplets called spherules. These millimeter-scale clues were formerly molten droplets ejected into space within the huge plumes created by mega-impacts on Earth. The hardened droplets then fell back to Earth, creating thin but widespread sedimentary layers known as spherule beds.
The new findings are published today in the journal Nature.

"The beds speak to an intense period of bombardment of Earth," said William Bottke principal investigator of the impact study team at the Southwest Research Institute (SwRI) in Boulder, Colo. "Their source long has been a mystery."

The team's findings support the theory Jupiter, Saturn, Uranus and Neptune formed in different orbits nearly 4.5 billion years ago, migrating to their current orbits about 4 billion years ago from the interplay of gravitational forces in the young solar system. This event triggered a solar system-wide bombardment of comets and asteroids called the "Late Heavy Bombardment." In the paper, the team created a model of the ancient main asteroid belt and tracked what would have happened when the orbits of the giant planets changed. They discovered the innermost portion of the belt became destabilized and could have delivered numerous big impacts to Earth and the moon over long time periods.

At least 12 mega-impacts produced spherule beds during the so-called Archean period 2.5 to 3.7 billion years ago, a formative time for life on Earth. Ancient spherule beds are rare finds, rarer than rocks of any other age. Most of the beds have been preserved amid mud deposited on the sea floor below the reach of waves.

The impact believed to have killed the dinosaurs was the only known collision over the past half-billion years that made a spherule layer as deep as those of the Archean period. The relative abundance of the beds supports the hypothesis for many giant asteroid impacts during Earth's early history.

The frequency of the impacts indicated in the computer models matches the number of spherule beds found in terrains with ages that are well understood. The data also hint at the possibility that the last impacts of the Late Heavy Bombardment on Earth made South Africa's Vredefort crater and Canada's Sudbury crater, both of which formed about 2 billion years ago.

"The Archean beds contain enough extraterrestrial material to rule out alternative sources for the spherules, such as volcanoes," said Bruce Simonson, a geologist from Oberlin College in Oberlin, Ohio.

The research was funded by NLSI and conducted by members or associates of NLSI's Center of Lunar Origin and Evolution, based at SwRI.

The impact study team also includes scientists from Purdue University in West Lafayette, Ind.; Charles University in Prague, Czech Republic; Observatorie de la Cote d'Azur in Nice, France; and Academia Sinica in Taipei, Taiwan.

To learn about the NLSI, visit:
http://lunarscience.arc.nasa.gov/
Guillermo Gonzalo Sánchez Achutegui

lunes, 23 de abril de 2012

Astronomy: A New View of the Tarantula Nebula


Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., To celebrate its 22nd anniversary in orbit, the Hubble Space Telescope released a dramatic new image of the star-forming region 30 Doradus, also known as the Tarantula Nebula because its glowing filaments resemble spider legs. A new image from all three of NASA's Great Observatories--Chandra, Hubble, and Spitzer--has also been created to mark the event.
The Tarantula Nebula

To celebrate its 22nd anniversary in orbit, the Hubble Space Telescope released a dramatic new image of the star-forming region 30 Doradus, also known as the Tarantula Nebula because its glowing filaments resemble spider legs. A new image from all three of NASA's Great Observatories--Chandra, Hubble, and Spitzer--has also been created to mark the event.

The nebula is located in the neighboring galaxy called the Large Magellanic Cloud, and is one of the largest star-forming regions located close to the Milky Way. At the center of 30 Doradus, thousands of massive stars are blowing off material and producing intense radiation along with powerful winds. The Chandra X-ray Observatory detects gas that has been heated to millions of degrees by these stellar winds and also by supernova explosions. These X-rays, colored blue in this composite image, come from shock fronts--similar to sonic booms--formed by this high-energy stellar activity.

The Hubble data in the composite image, colored green, reveals the light from these massive stars along with different stages of star birth, including embryonic stars a few thousand years old still wrapped in cocoons of dark gas. Infrared emission data from Spitzer, seen in red, shows cooler gas and dust that have giant bubbles carved into them. These bubbles are sculpted by the same searing radiation and strong winds that comes from the massive stars at the center of 30 Doradus.

Image Credits: X-ray: NASA/CXC/PSU/L.Townsley et al.; Optical: NASA/STScI; Infrared: NASA/JPL/PSU/L.Townsley et al.
Guillermo Gonzalo Sánchez Achutegui

domingo, 22 de abril de 2012

Astronomy: NASA's SOFIA Featured in the Astrophysical Journal Special Edition

http://www.nasa.gov/mission_pages/SOFIA/12-122HQ.html
Cornell University’s Faint Object Infrared Camera for the SOFIA Telescope, or FORCAST, is mounted on the telescope during preparation leading to Short Science flights. (NASA photo)  › View Larger Image
With the sliding door over its 17-ton infrared telescope wide open, NASA's Stratospheric Observatory for Infrared Astronomy – or SOFIA – soars over California's snow-covered Southern Sierras on a test flight in 2010 (NASA / Jim Ross) › View Larger Image

NASA's SOFIA Featured in the Astrophysical Journal Special Edition :

MOFFETT FIELD, Calif. -- The Astrophysical Journal, a leading professional astronomy research publication, will issue a special edition of its Letters volume on April 20 with papers about observations made with NASA's Stratospheric Observatory for Infrared Astronomy (SOFIA) airborne telescope.

SOFIA is a highly modified Boeing 747SP aircraft that carries a telescope with a 100-inch (2.5-meter) diameter reflecting mirror that conducts astronomy research not possible with ground-based telescopes. By operating in the stratosphere at altitudes up to 45,000 feet, SOFIA can make observations above the water vapor in Earth's lower atmosphere.

"This is really SOFIA's debut on the world scientific stage," said Chris Davis, SOFIA program scientist at NASA Headquarters in Washington. "World-class observatories such as the Hubble, Chandra and Spitzer space telescopes had their Astrophysical Journal special editions, and now SOFIA joins their prestigious ranks."

The eight SOFIA papers featured in the special edition cover diverse research on topics including SOFIA's capabilities as a flying observatory and its study of star formation in our galaxy and beyond.

Studies of star and planet formation processes are one of SOFIA's 'sweet spots,'" said SOFIA Science Mission Director Erick Young. "SOFIA's infrared instruments can see into the dense clouds where stars and planets are forming and detect heat radiation from their construction material. By getting above the Earth's atmospheric water vapor layer that blocks most of the infrared band, SOFIA's telescope can view the glow from forming stars at their strongest emission wavelengths."

The infrared images analyzed in these papers were obtained with the FORCAST (Faint Object Infrared Camera for the SOFIA Telescope) instrument during SOFIA's first science observations in December 2010. Papers based on observations with SOFIA and the GREAT spectrometer (German Receiver for Astronomy at THz Frequencies) will be published in a May 2012 special volume of the European journal Astronomy and Astrophysics.

SOFIA is a joint project of NASA and the German Aerospace Center and is based and managed at NASA's Dryden Aircraft Operations Facility in Palmdale, Calif. NASA's Ames Research Center at Moffett Field, Calif., manages the SOFIA science and mission operations in cooperation with the Universities Space Research Association, headquartered in Columbia, Md., and the German SOFIA Institute at the University of Stuttgart.

For more information about SOFIA, visit:
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com



La Tierra: Investigation on Envisat continues

On 15 April, the French space agency CNES rotated the Pleiades Earth observation satellite to capture this image of Envisat. At a distance of about 100 km, Envisat’s main body, solar panel and radar antenna were visible.
Credits: CNES
Optical, radar and laser observations of the Envisat satellite show that it is still in a stable orbit. Efforts to regain contact with the satellite have been under way since 8 April, when it unexpectedly stopped sending data to Earth.
 To determine if Envisat has entered its ‘safe mode’ – which would be a starting point for revival – the recovery team is drawing on every information source available.
Valuable help is coming from many European and international partners. France’s new Pleiades satellite normally provides very high-resolution images of Earth, but is now focusing on Envisat to shed more light on the situation.
On 15 April, the French space agency turned Pleiades to capture images of Envisat passing within about 100 km. This remarkable feat was possible thanks to the exceptional agility of Pleiades.
Flight specialists and engineers are using the images to determine the orientation of Envisat’s solar panel – the satellite’s power source.
If the panel is in a suitable position for sufficient exposure to the Sun, enough power is being generated to put Envisat into safe mode, and could allow for re-establishing communications with Earth.
“We are really grateful to CNES for offering to acquire images of Envisat using their Pleiades and Spot satellites,” said Volker Liebig, ESA’s Director of Earth Observation Programmes.  

This radar image showing the Envisat satellite in orbit was produced by the ground-based tracking and imaging radar, TIRA, of the Fraunhofer Institute for High Frequency Physics and Radar Techniques in Wachtberg, Germany, on 10 April 2012.
Credits: Fraunhofer FHR
Investigation on Envisat continues :“Additional observations being acquired across the globe show how the international space community has come together to track this veteran satellite.”
The Fraunhofer Institute for High Frequency Physics and Radar Techniques in Wachtberg, Germany, is also providing images to help determine Envisat’s orientation.
Images from the TIRA ground-based tracking and imaging radar show the satellite’s body, solar panel and radar antenna.
“These unique images will enable us to analyse Envisat’s orientation, which will indicate whether we are able to regain contact with the satellite,” said Manfred Warhaut, Head of ESA’s Mission Operations Department.
Information on Envisat’s orbit is being provided by the US Joint Space Operations Center. In addition, multiple laser ranging stations on the ground are providing information to verify the stability of the satellite’s orbit.
The sudden interruption of Envisat services has disrupted data provision to the international Earth observation user community, which relies on data continuity.
The launch of the upcoming Sentinel series being developed for Europe’s Global Monitoring for Environment and Security (GMES) programme has become even more urgent.
The Sentinels will provide the data needed for information services to improve the management of the environment, understand and mitigate the effects of climate change and ensure civil security.
Guillermo Gonzalo Sánchez Achutegui 
 ayabaca@gmail.com

miércoles, 18 de abril de 2012

Astronomy: Rings, Titan and Enceladus

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., Saturn’s icy moon Enceladus hangs below the gas giant’s rings while Titan lurks in the background, in this new image taken by the Cassini spacecraft. Saturn’s icy moon Enceladus hangs below the gas giant’s rings while Titan lurks in the background, in this new image taken by the Cassini spacecraft.

Faint detail of the tiger stripe markings can be seen on Enceladus’ surface, which is framed against Titan, Saturn’s largest moon. With jets of water ice and vapour streaming from Enceladus’ south pole, and liquid hydrocarbon lakes pooling beneath Titan’s thick atmosphere, these are two of Saturn’s most enigmatic moons.

The northern, sun-lit side of Saturn’s rings are seen from just above the ring plane in this image, which was taken in visible green light by Cassini’s narrow-angle camera on 12 March while it was approximately one million kilometres from Enceladus. The image scale is six kilometres per pixel on Enceladus.

Credits: NASA/JPL-Caltech/Space Science Institute
http://www.esa.int/SPECIALS/Cassini-Huygens/SEMNUCKWZ0H_0.html

Guillermo Gonzalo Sánchez Achutegui



Astronomy: Preparing MAVEN for Mars

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., MAVEN's hydrazine propellant tank is shown prior to it being installed in the core structure of the MAVEN spacecraft at a Lockheed Martin clean room near Denver in this image taken in April 2012. Preparing MAVEN for Mars
MAVEN's hydrazine propellant tank is shown prior to it being installed in the core structure of the MAVEN spacecraft at a Lockheed Martin clean room near Denver in this image taken in April 2012. The goal of the Mars Atmosphere And Volatile EvolutioN program, or MAVEN, is to determine the role that loss of atmospheric gas to space played in changing the Martian climate through time. The mission will determine how much of the Martian atmosphere has been lost over time by measuring the current rate of escape to space and gathering enough information about the relevant processes to allow extrapolation backward in time.

Built of composite panels comprised of aluminum honeycomb sandwiched between graphite composite face sheets, the entire structure only weighs 275 pounds. MAVEN is scheduled to launch in November 2013 and will be the first mission devoted to understanding the Martian upper atmosphere.

Image Credit: Lockheed Martin
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

Astronomy: Space technology landing in Hanover at largest trade fair

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., Propelling the Ariane 5 rocket into space, the Vulcain engine truly reflects Europe’s impressive aerospace achievements. The giant engine will flag ‘ESA Space Apps’ at this year’s Hannover Messe trade fair showcasing impressive space technology spin-offs and their terrestrial potential.

The Vulcain engine of the Ariane 5 launcher during a test run at the German Space Agency DLR Credits: DLR
Propelling the Ariane 5 rocket into space, the Vulcain engine truly reflects Europe’s impressive aerospace achievements. The giant engine will flag ‘ESA Space Apps’ at this year’s Hannover Messe trade fair showcasing impressive space technology spin-offs and their terrestrial potential. Organised by ESA’s Technology Transfer Programme Office and German MST Aerospace, the ESA Space Apps stand will illustrate how striking product developments and innovative advances are possible in a variety of fields through the transfer of ready available space technologies.
ESA Space Apps stand at Hannover Messe 2011 Credits: Hannover Messe

On the opening day – 23 April – the winner of this year’s ESA Space Spin-off Award will be announced. It goes to individuals or an organisation that have carried out a space technology transfer of extraordinary success with significant economic impact and remarkable results in a non-space sector.

ESA Space Apps visitors can discuss with MST and ESA representatives how space technologies can be employed in their fields.

Spin-offs on display by companies

ESA’s Technology Transfer Programme Office has invited several industrial partners to present their products and services, all based on space spin-offs.

Trude, the world´s largest tunnel boring machines (TBMs) with a diameter of 14.2m, excavated the 4th pipe Elbe Tunnel in Hamburg, Germany. It took two years and five months to drill the 2,561 metres underground tunnel.
The German tunnelling company, Herrenknecht AG, responsible for this achievement is now applying a new technique with space origin in order to be able to drill tunnels even better. The German company Astro- und Feinwerktechnik Adlershof GmbH has produced a new transmitter for Herrenknecht AG based upon their know-how gained from their work for ESA on the Cassini-Huygens spacecraft.
A number of these transmitters are now mounted on a TBM and provides a look into the ground in front of the TDB. Every second the transmitters send sound waves into the ground, microphones receive the reflecting signals which are data processed and visualizes important geologic changes up to 40 m in front of the rotary shear blade.

Credits: Herrenknecht AG.

From the Cassini-Huygens Saturn mission, Astro- and Feinwerktechnik Adlershof derived a technology for seismic soft-ground probing to predict geological changes in front of the rotary shear blades of underground drilling machines. This is now used by the machine manufacturer Herrenknecht.

Thermal silicon-carbide protection shield technologies developed by IABG for the Hermes spaceplane were adapted for high-performance carbon ceramic brake discs by Brembo SGL Carbon Ceramic Brakes.

Based on spacecraft equipment, Tecnalia Research and Innovation is developing a telecare fall-detector device and an intelligent assistance system for mountaineers and search and rescue teams.

The German start-up company PiMON develops a fiber optic based monitoring technology for pipelines. Space expertise from very similar technologies used in structural elements in the aerospace industry, e.g. in the Ariane launch system or in satellites to monitor the integrity of cryogenic propellant tanks, have been used in the development by PiMON.
The publication presents a selection of the latest space technology transfers assisted by ESA’s Technology Transfer Programme Office.

Credits: ESA
The space expertise of PiMON has lead to the development of novel fibre optics-based sensor monitoring systems for oil and gas pipelines. Vibration and other changes along the lines – such as leaks or illegal tapping – are immediately detected and reported to service personnel.

Special ball-bearing cages developed for space missions like the BepiColombo Mercury probe are now offered by AAC for terrestrial applications.

Fire Suppression Inside is spinning off a technology from ESA’s Proba-2 satellite to suppress overheating and fire in electrical equipment like servers, switches, power distribution units and backup generators.

‘mobile life‘ is developing GPS/Galileo-based high accuracy positioning monitoring systems with wireless telemetric sensors for easy location and monitoring of people, animals and freight.
“Europe’s space programmes are important economic drivers, also when leading-edge space technology is transferred to non-space systems and sectors,” explains Werner Dupont of MST Aerospace.

MST is co-organiser of the ESA Space Apps stand and the manager of ESA’s Technology Transfer Broker Network.

“Space technologies enable in many cases everyday products in sectors like automotive, health and household without users and consumers being aware of it.”

At the Hannover Messe, ESA Space Apps is located at stand D56 in hall 2, 23–27 April.

ESA is also present with its ESA Career Info stand at Hall 6, J24/40.
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com


martes, 27 de marzo de 2012

Astronomy: Lighting the Sky

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., ATREX, the Anomalous Transport Rocket Experiment successfully launched five suborbital sounding rockets in the early morning hours of March 27, 2012, from the Wallops Flight Facility in Virginia as part of a study of the upper level jet stream. The first rocket launched at 4:58 a.m. EDT and each subsequent rocket launched 80 seconds apart.Lighting the Sky
ATREX, the Anomalous Transport Rocket Experiment successfully launched five suborbital sounding rockets in the early morning hours of March 27, 2012, from the Wallops Flight Facility in Virginia as part of a study of the upper level jet stream.

The first rocket launched at 4:58 a.m. EDT and each subsequent rocket launched 80 seconds apart.

Each of the rockets released a chemical tracer that created milky, white clouds at the edge of space.

The launches and clouds were reported to be seen from as far south as Wilmington, N.C., west to Charlestown, W. Va., and north to Buffalo, N.Y.The mission will gather information that will assist researchers to better understand the process responsible for the high-altitude jet stream located 60 to 65 miles above the surface of the Earth.

Image Credit: NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

domingo, 25 de marzo de 2012

Astronomy: Hubble Sees Glittering Jewels of Messier 9

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., The Hubble Space Telescope has produced the most detailed image so far of Messier 9, a globular star cluster located close to the center of the galaxy. This ball of stars is too faint to see with the naked eye, yet Hubble can see over 250,000 individual stars shining in it. Hubble Sees Glittering Jewels of Messier 9
The Hubble Space Telescope has produced the most detailed image so far of Messier 9, a globular star cluster located close to the center of the galaxy. This ball of stars is too faint to see with the naked eye, yet Hubble can see over 250,000 individual stars shining in it.

Messier 9, pictured here, is a globular cluster, a roughly spherical swarm of stars that lies around 25,000 light-years from Earth, near the center of the Milky Way, so close that the gravitational forces from the galactic center pull it slightly out of shape.

Globular clusters are thought to harbor some of the oldest stars in our galaxy, born when the universe was just a small fraction of its current age. As well as being far older than the sun -- around twice its age -- the stars of Messier 9 also have a markedly different composition, and are enriched with far fewer heavier elements than the sun.

In particular, the elements crucial to life on Earth, like oxygen and carbon, and the iron that makes up our planet’s core, are very scarce in Messier 9 and clusters like it. This is because the universe’s heavier elements were gradually formed in the cores of stars, and in supernova explosions. When the stars of Messier 9 formed, there were far smaller quantities of these elements in existence.

As well as showing the individual stars, Hubble’s image clearly shows the different colors of the stars. A star’s color is directly related to its temperature -- counter-intuitively, perhaps, the redder it is, the cooler it is; and the bluer it is, the hotter. The wide range of stellar temperatures here is clearly displayed by the broad palette of colors visible in this image.

Image Credit: NASA and ESA

Guillermo Gonzalo Sánchez Achutegui



Astronomy: Cassini Mission Receives Air and Space Museum Award

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., The Smithsonian's National Air and Space Museum has bestowed its highest group honor, the Trophy for Current Achievement, on NASA's Cassini mission to Saturn. The annual award recognizes outstanding achievements in the fields of aerospace science and technology. National Air and Space Museum Award for Cassini-Huygens
NASA's Cassini-Huygens mission to Saturn was awarded the 2012 National Air and Space Museum Trophy for Current Achievement on March 21 at a black-tie dinner in Washington, D.C. Pictured (from left to right) - Wayne Clough, secretary of the Smithsonian; Robert Mitchell, Cassini program manager based at NASA's Jet Propulsion Laboratory, Pasadena, Calif.; and Gen. Jack Dailey, director of the museum.

Image credit: Smithsonian National Air and Space Museum


Cassini Mission Receives Air and Space Museum Award.

PASADENA, Calif. -- The Smithsonian's National Air and Space Museum has bestowed its highest group honor, the Trophy for Current Achievement, on NASA's Cassini mission to Saturn. The annual award recognizes outstanding achievements in the fields of aerospace science and technology.
The trophy was presented Wednesday, March 21, during an evening ceremony at the museum in Washington. Established in 1985, the award has been presented to seven NASA planetary mission teams.
"This joint mission has produced an unprecedented science return," said William Knopf, Cassini program executive at NASA Headquarters in Washington. "Missions like Cassini pave the way for future robotic and human exploration throughout our solar system and beyond."
Launched in 1997, the Cassini spacecraft entered Saturn's orbit in June 2004 with the European Space Agency's (ESA) Huygens probe bolted to its side. In December 2004, the spacecraft successfully released Huygens, which entered the atmosphere of Saturn's largest moon, Titan. Cassini completed its prime mission in 2008 and has been extended twice. It is now in its so-called solstice mission, which will enable scientists to observe seasonal changes in Saturn and its moons during the planet's northern summer solstice. The mission will last through September 2017.
"We look forward to sailing around the Saturn system for several more years to see how our views of the planet and its magnificent moons change as we get into northern summer solstice," said Robert Mitchell, the Cassini program manager at NASA's Jet Propulsion Laboratory in Pasadena, Calif., who accepted the award on behalf of the team.
The Cassini spacecraft carries 12 science instruments and investigations, with an additional six aboard Huygens. Cassini mission highlights to date include the discovery of four new moons and two new rings around Saturn. Cassini observed spraying water vapor and icy particle jets from the moon Enceladus. In Saturn's northern hemisphere, the spacecraft watched the evolution of a monster storm, a sign of seasonal change from northern winter into northern spring.
Cassini and Huygens has also revealed new characteristics about Titan, the only body in the solar system other than Earth with stable liquid on its surface.
The Cassini-Huygens mission is a cooperative project of NASA, ESA and the Italian Space Agency. JPL manages the mission for NASA's Science Mission Directorate in Washington. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. JPL is managed for NASA by the California Institute of Technology in Pasadena.
For more information about the mission,

visit: http://www.nasa.gov/cassini
Images of the award and a Cassini historical video are available

at: http://go.nasa.gov/GH6qbA
For a full listing of previous awardees,

visit: http://www.nasm.si.edu/research/aero/trophy/nasm.cfm
More Cassini information is available at and http://saturn.jpl.nasa.gov .

Guillermo Gonzalo Sánchez Achutegui



Astronomy: NASA'S Grail MoonKam Returns First Student-Selected Lunar Images

http://images.moonkam.ucsd.edu/main.php?g2_itemId=321


NASA'S Grail MoonKam Returns First Student-Selected Lunar Images

WASHINGTON -- One of two NASA spacecraft orbiting the moon has beamed back the first student-requested pictures of the lunar surface from its onboard camera. Fourth grade students from the Emily Dickinson Elementary School in Bozeman, Mont., received the honor of making the first image selections by winning a nationwide competition to rename the two spacecraft. The image was taken by the MoonKam, or Moon Knowledge Acquired by Middle school students. Previously named Gravity Recovery And Interior Laboratory (GRAIL) A and B, the twin spacecraft are now called Ebb and Flow. Both washing-machine-sized orbiters carry a small MoonKAM camera. Over 60 student-requested images were taken aboard the Ebb spacecraft from March 15-17 and downlinked to Earth on March 20.

"MoonKAM is based on the premise that if your average picture is worth a thousand words, then a picture from lunar orbit may be worth a classroom full of engineering and science degrees," said Maria Zuber, GRAIL mission principal investigator from the Massachusetts Institute of Technology in Cambridge, Mass. "Through MoonKAM, we have an opportunity to reach out to the next generation of scientists and engineers. It is great to see things off to such a positive start."

GRAIL is NASA's first planetary mission to carry instruments fully dedicated to education and public outreach. Students will select target areas on the lunar surface and request images to study from the GRAIL MoonKAM Mission Operations Center in San Diego.

The MoonKAM program is led by Sally Ride, America's first woman in space, and her team at Sally Ride Science in collaboration with undergraduate students at the University of California in San Diego. More than 2,700 schools spanning 52 countries are using the MoonKAM cameras. "What might seem like just a cool activity for these kids may very well have a profound impact on their futures," Ride said. "The students really are excited about MoonKAM, and that translates into an excitement about science and engineering."

Launched in September 2011, Ebb and Flow will answer longstanding questions about the moon and give scientists a better understanding of how Earth and other rocky planets in the solar system formed.

NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the GRAIL mission for NASA's Science Mission Directorate in Washington. GRAIL is part of the Discovery Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems in Denver built the spacecraft. To view the student-requested images, visit:
http://images.moonkam.ucsd.edu
For more information about MoonKAM, visit:
https://moonkam.ucsd.edu

For more information about GRAIL, visit:
http://www.nasa.gov/grail
Guillermo Gonzalo Sánchez Achutegui



martes, 20 de marzo de 2012

Astronomy: Spider Web of Stars

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., At a distance of about 10 million light-years, IC 342 is relatively close by galactic standards, however our vantage point places it directly behind the disk of our own Milky Way. The intervening dust makes it difficult to see in visible light, but infrared light penetrates this veil easily. IC 342 belongs to the same group as its even more obscured galactic neighbor, Maffei 2. Spider Web of Stars
Looking like a spider's web swirled into a spiral, Galaxy IC 342 presents its delicate pattern of dust in this image from NASA's Spitzer Space Telescope. Seen in infrared light, faint starlight gives way to the glowing bright patterns of dust found throughout the galaxy's disk.

At a distance of about 10 million light-years, IC 342 is relatively close by galactic standards, however our vantage point places it directly behind the disk of our own Milky Way. The intervening dust makes it difficult to see in visible light, but infrared light penetrates this veil easily. IC 342 belongs to the same group as its even more obscured galactic neighbor, Maffei 2.

IC 342 is nearly face-on to our view, giving a clear, top-down view of the structure of its disk. It has a low surface brightness compared to other spirals, indicating a lower density of stars (seen here as a blue haze). Its dust structures show up much more vividly (red). Blue dots are stars closer to us, in our own Milky Way.

New stars are forming in the disk at a healthy rate. The very center glows especially brightly in the infrared, highlighting an enormous burst of star formation occurring in this tiny region. To either side of the center, a small bar of dust and gas is helping to fuel this central star formation.

Data from Spitzer's infrared array camera are shown in blue (3.6 microns), green (4.5 microns) and red (5.8 and 8.0 microns).

Image Credit: NASA/JPL-Caltech

Guillermo Gonzalo Sánchez Achutegui



jueves, 15 de marzo de 2012

Astronomy: Compact Planetary System

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., This artist's concept depicts a planetary system so compact that it's more like Jupiter and its moons than a star and its planets. Astronomers using data from NASA's Kepler mission and ground-based telescopes recently confirmed that the system, called KOI-961, hosts the three smallest exoplanets currently known to orbit a star other than our sun. An exoplanet is a planet that resides outside of our solar system.Compact Planetary System
This artist's concept depicts a planetary system so compact that it's more like Jupiter and its moons than a star and its planets. Astronomers using data from NASA's Kepler mission and ground-based telescopes recently confirmed that the system, called KOI-961, hosts the three smallest exoplanets currently known to orbit a star other than our sun. An exoplanet is a planet that resides outside of our solar system.

The star, which is located about 130 light-years away in the Cygnus constellation, is a red dwarf that is one-sixth the size of the sun, or just 70 percent bigger than Jupiter. The star is also cooler than our sun, and gives off more red light than yellow.

The smallest of the three planets, called KOI-961.03, is actually located the farthest from the star, and is pictured in the foreground. This planet is about the size of Mars, with a radius of 0.57 times that of Earth. The next planet to the upper right is KOI-961.01, which is 0.78 times the radius of Earth. The planet closest to the star is KOI-961.02, with a radius 0.73 times the Earth's.

All three planets whip around the star in less than two days, with the closest planet taking less than half a day. Their close proximity to the star also means they are scorching hot, with temperatures ranging from 350 to 836 degrees Fahrenheit (176 to 447 degrees Celsius). The star's habitable zone, or the region where liquid water could exist, is located far beyond the planets.

The ground-based observations contributing to these discoveries were made with the Palomar Observatory, near San Diego, Calif., and the W.M. Keck Observatory atop Mauna Kea in Hawaii.

Image Credit: NASA/JPL-Caltech
NASA.

Guillermo Gonzalo Sánchez Achutegui



domingo, 11 de marzo de 2012

Astronomy: Hubble Image of Galaxies' El Dorado

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., NASA's Hubble Space Telescope has produced this beautiful image of the galaxy NGC 1483. NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado — the dolphinfish (or Mahi-mahi fish) in Spanish. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star-forming regions. In the background, many other distant galaxies can be seen. Hubble Image of Galaxies' El Dorado
NASA's Hubble Space Telescope has produced this beautiful image of the galaxy NGC 1483. NGC 1483 is a barred spiral galaxy located in the southern constellation of Dorado — the dolphinfish (or Mahi-mahi fish) in Spanish. The nebulous galaxy features a bright central bulge and diffuse arms with distinct star-forming regions. In the background, many other distant galaxies can be seen.

The constellation Dorado is home to the Dorado Group of galaxies, a loose group comprised of an estimated 70 galaxies and located some 62 million light-years away. The Dorado group is much larger than the Local Group that includes the Milky Way (and which contains around 30 galaxies) and approaches the size of a galaxy cluster. Galaxy clusters are the largest groupings of galaxies (and indeed the largest structures of any type) in the universe to be held together by their gravity.

Barred spiral galaxies are so named because of the prominent bar-shaped structures found in their center. They form about two thirds of all spiral galaxies, including the Milky Way. Recent studies suggest that bars may be a common stage in the formation of spiral galaxies, and may indicate that a galaxy has reached full maturity.

Image Credit: ESA/Hubble & NASA
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com
ayabaca@hotmail.com
ayabaca@yahoo.com

miércoles, 7 de marzo de 2012

Astronomy: Firestorm of Star Birth in Galaxy Centaurus A

Hi My Friends: AL VUELO DE UN QUIND EL BLOG., Hubble's panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, reveals the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by the dust.Firestorm of Star Birth in Galaxy Centaurus A
Resembling looming rain clouds on a stormy day, dark lanes of dust crisscross the giant elliptical galaxy Centaurus A.

Hubble's panchromatic vision, stretching from ultraviolet through near-infrared wavelengths, reveals the vibrant glow of young, blue star clusters and a glimpse into regions normally obscured by the dust.The warped shape of Centaurus A's disk of gas and dust is evidence for a past collision and merger with another galaxy. The resulting shockwaves cause hydrogen gas clouds to compress, triggering a firestorm of new star formation. These are visible in the red patches in this Hubble close-up.

At a distance of just over 11 million light-years, Centaurus A contains the closest active galactic nucleus to Earth. The center is home for a supermassive black hole that ejects jets of high-speed gas into space, but neither the supermassive black hole or the jets are visible in this image.

This image was taken in July 2010 with Hubble's Wide Field Camera 3.Image Credit: NASA, ESA, and the Hubble Heritage (STScI/AURA)-ESA/Hubble CollaborationAcknowledgment: R. O'Connell (University of Virginia) and the WFC3 Scientific Oversight Committee. NASA
Guillermo Gonzalo Sánchez Achutegui



Astronomy: NASA's Twin GRAIL Spacecraft Begin Collecting Lunar Science Data

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., NASA's Gravity Recovery And Interior Laboratory (GRAIL) spacecraft orbiting the moon officially have begun their science collection phase. During the next 84 days, scientists will obtain a high-resolution map of the lunar gravitational field to learn about the moon's internal structure and composition in unprecedented detail. The data also will provide a better understanding of how Earth and other rocky planets in the solar system formed and evolved. Artist concept of GRAIL mission. GRAIL will fly twin spacecraft in tandem orbits around the moon to measure its gravity field in unprecedented detail. Image credit: NASA/JPL .

PASADENA, Calif. -- NASA's Gravity Recovery And Interior Laboratory (GRAIL) spacecraft orbiting the moon officially have begun their science collection phase. During the next 84 days, scientists will obtain a high-resolution map of the lunar gravitational field to learn about the moon's internal structure and composition in unprecedented detail. The data also will provide a better understanding of how Earth and other rocky planets in the solar system formed and evolved.
"The initiation of science data collection is a time when the team lets out a collective sigh of relief because we are finally doing what we came to do," said Maria Zuber, principal investigator for the GRAIL mission at the Massachusetts Institute of Technology in Cambridge, "but it is also a time where we have to put the coffee pot on, roll up our sleeves and get to work."
The GRAIL mission's twin, washing-machine-sized spacecraft, named Ebb and Flow, entered lunar orbit on New Year's Eve and New Years Day. GRAIL's science phase began yesterday at 5:15 p.m. PST (8:15 p.m. EST). During this mission phase, the spacecraft will transmit radio signals precisely defining the rate of change of distance between the two. The distance between the spacecraft will change slightly as they fly over areas of greater and lesser gravity caused by visible features such as mountains, craters and masses hidden beneath the lunar surface. Science activities are expected to conclude on May 29, after GRAIL maps the gravity field of the moon three times.
"We are in a near-polar, near-circular orbit with an average altitude of about 34 miles (55 kilometers) right now," said David Lehman, GRAIL project manager from NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif. "During the science phase, our spacecraft will orbit the moon as high as 31 miles (51 kilometers) and as low as 10 miles (16 kilometers). They will get as close to each other as 40 miles (65 kilometers) and as far apart as 140 miles (225 kilometers)."
The two spacecraft were previously named GRAIL A and B. The names Ebb and Flow were the result of a nationwide student contest to choose new names for them. The winning entry was submitted by fourth graders from the Emily Dickinson Elementary School in Bozeman, Mont. Nearly 900 classrooms with more than 11,000 students from 45 states, Puerto Rico and the District of Columbia, participated in the contest.
JPL manages the GRAIL mission for NASA's Science Mission Directorate in Washington. The GRAIL mission is part of the Discovery Program managed at NASA's Marshall Space Flight Center in Huntsville, Ala. Lockheed Martin Space Systems in Denver built the spacecraft.
For more information about GRAIL,


Guillermo Gonzalo Sánchez Achutegui



domingo, 4 de marzo de 2012

Astronomy: NASA's Kepler Releases New Catalog- 2,321 Planet Candidates

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., The histogram summarizes the findings in the Feb. 27, 2012 Kepler Planet Candidate catalog release. The catalog contains 2,321 planet candidates identified during the first 16 months of observation conducted May 2009 to September 2010. Of the 46 planet candidates found in the habitable zone, the region in the planetary system where liquid water could exist, ten of these candidates are near-Earth-size. Kepler Planet Candidates by Size, Feb. 27, 2012
The histogram summarizes the findings in the Feb. 27, 2012 Kepler Planet Candidate catalog release. The catalog contains 2,321 planet candidates identified during the first 16 months of observation conducted May 2009 to September 2010. Of the 46 planet candidates found in the habitable zone, the region in the planetary system where liquid water could exist, ten of these candidates are near-Earth-size.

Credit: NASA Ames/Wendy Stenzel.


Since science operations began in May 2009, the Kepler team has released two catalogs of transiting planet candidates. The first catalog (Borucki et al, 2010), released in June 2010, contains 312 candidates identified in the first 43 days of Kepler data. The second catalog (Borucki et al, 2011), released in February 2011, is a cumulative catalog containing 1,235 candidates identified in the first 13 months of data.

Today the team presents the third catalog containing 1,091 new planet candidates identified in the first 16 months of observation conducted May 2009 to September 2010. These are the same candidates that the team discussed at the Kepler Science Conference held at NASA Ames Research Center in December 2011.

Here are the highlights of the new catalog:
A.- Planet candidates smaller than twice the size of Earth increased by 197 percent, compared to 52 percent for candidates larger than twice the size of Earth.
B.- Planet candidates with orbital periods longer than 50 days increased by 123 percent, compared to 85 percent for candidates with orbital periods shorter than 50 days. Since the last catalog was released in February 2011, the number of planet candidates identified by Kepler has increased by 88 percent and now totals 2,321 transiting 1,790 stars.

The cumulative catalog now contains well over 200 Earth-size planet candidates and more than 900 that are smaller than twice Earth-size. Of the 46 planet candidates found in the habitable zone, the region in the planetary system where liquid water could exist, ten of these candidates are near-Earth-size.

The number of planetary systems found with more than one planet candidate also has increased. Last year, 17 percent, or 170 stars, had more than one transiting planet candidate. Today, 20 percent, or 365, stars have more than one.

"With each new catalog release a clear progression toward smaller planets at longer orbital periods is emerging, " said Natalie Batalha, Kepler deputy science team lead at San Jose State University in California. "This suggests that Earth-size planets in the habitable zone are forthcoming if, indeed, such planets are abundant.

"Nearly 5,000 periodic transit-like signals were analyzed with known spacecraft instrumentation and astrophysical phenomena that could masquerade as transits, which can produce false positives. The most common false positive signatures are associated with eclipsing binary stars- a pair of orbiting stars that eclipse each other from the vantage point of the spacecraft.

The Kepler space telescope identifies planet candidates by repeatedly measuring the change in brightness of more than 150,000 stars in search of planets that pass in front, or "transit," their host star. Kepler must record at least three transits to verify a signal as a planet.


The catalog is available at the Kepler data archive at the Space Telescope Science Institute and can be downloaded from the NASA Exoplanet Archive.

NASA's Ames Research Center in Moffett Field, Calif., manages Kepler's ground system development, mission operations and science data analysis. NASA’s Jet Propulsion Laboratory, Pasadena, Calif., managed the Kepler mission's development.

Ball Aerospace and Technologies Corp. in Boulder, Colo., developed the Kepler flight system and supports mission operations with the Laboratory for Atmospheric and Space Physics at the University of Colorado in Boulder.

The Space Telescope Science Institute in Baltimore archives, hosts and distributes Kepler science data. Kepler is NASA's 10th Discovery Mission and is funded by NASA's Science Mission Directorate at the agency's headquarters in Washington.

For information about the Kepler Mission,

visit: http://www.nasa.gov/kepler
Guillermo Gonzalo Sánchez Achutegui
ayabaca@gmail.com


Astronomy: Dark Matter Core Defies Explanation

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., Astronomers using data from NASA's Hubble Telescope have observed what appears to be a clump of dark matter left behind from a wreck between massive clusters of galaxies. The result could challenge current theories about dark matter that predict galaxies should be anchored to the invisible substance even during the shock of a collision.

Abell 520 is a gigantic merger of galaxy clusters located 2.4 billion light-years away. Dark matter is not visible, although its presence and distribution is found indirectly through its effects. Dark matter can act like a magnifying glass, bending and distorting light from galaxies and clusters behind it. Astronomers can use this effect, called gravitational lensing, to infer the presence of dark matter in massive galaxy clusters.

This technique revealed the dark matter in Abell 520 had collected into a "dark core," containing far fewer galaxies than would be expected if the dark matter and galaxies were anchored together. Most of the galaxies apparently have sailed far away from the collision. This composite image shows the distribution of dark matter, galaxies, and hot gas in the core of the merging galaxy cluster Abell 520, formed from a violent collision of massive galaxy clusters. The natural-color image of the galaxies was taken with NASA's Hubble Space Telescope and with the Canada-France-Hawaii Telescope in Hawaii. Superimposed on the image are "false-colored" maps showing the concentration of starlight, hot gas, and dark matter in the cluster. Starlight from galaxies, derived from observations by the Canada-France-Hawaii Telescope, is colored orange. The green-tinted regions show hot gas, as detected by NASA's Chandra X-ray Observatory. The gas is evidence that a collision took place. The blue-colored areas pinpoint the location of most of the mass in the cluster, which is dominated by dark matter. Dark matter is an invisible substance that makes up most of the universe's mass. The dark-matter map was derived from the Hubble Wide Field Planetary Camera 2 observations, by detecting how light from distant objects is distorted by the cluster galaxies, an effect called gravitational lensing.

The blend of blue and green in the center of the image reveals that a clump of dark matter resides near most of the hot gas, where very few galaxies are found. This finding confirms previous observations of a dark-matter core in the cluster. The result could present a challenge to basic theories of dark matter, which predict that galaxies should be anchored to dark matter, even during the shock of a collision. Abell 520 resides 2.4 billion light-years away.

Credit: NASA, ESA, CFHT, CXO, M.J. Jee (University of California, Davis), and A. Mahdavi (San Francisco State University)

"This result is a puzzle," said astronomer James Jee of the University of California in Davis, lead author of paper about the results available online in The Astrophysical Journal.

"Dark matter is not behaving as predicted, and it's not obviously clear what is going on. It is difficult to explain this Hubble observation with the current theories of galaxy formation and dark matter.

"Initial detections of dark matter in the cluster, made in 2007, were so unusual that astronomers shrugged them off as unreal, because of poor data. New results from NASA's Hubble Space Telescope confirm that dark matter and galaxies separated in Abell 520.

One way to study the overall properties of dark matter is by analyzing collisions between galaxy clusters, the largest structures in the universe. When galaxy clusters crash, astronomers expect galaxies to tag along with the dark matter, like a dog on a leash. Clouds of hot, X-ray emitting intergalactic gas, however, plow into one another, slow down, and lag behind the impact.

That theory was supported by visible-light and X-ray observations of a colossal collision between two galaxy clusters called the Bullet Cluster. The galactic grouping has become an example of how dark matter should behave.Studies of Abell 520 showed that dark matter's behavior may not be so simple.

Using the original observations, astronomers found the system's core was rich in dark matter and hot gas, but contained no luminous galaxies, which normally would be seen in the same location as the dark matter. NASA's Chandra X-ray Observatory was used to detect the hot gas. Astronomers used the Canada-France-Hawaii Telescope and Subaru Telescope atop Mauna Kea to infer the location of dark matter by measuring the gravitationally lensed light from more distant background galaxies.

The astronomers then turned to the Hubble's Wide Field Planetary Camera 2, which can detect subtle distortions in the images of background galaxies and use this information to map dark matter. To astronomers' surprise, the Hubble observations helped confirm the 2007 findings. "We know of maybe six examples of high-speed galaxy cluster collisions where the dark matter has been mapped," Jee said.

"But the Bullet Cluster and Abell 520 are the two that show the clearest evidence of recent mergers, and they are inconsistent with each other. No single theory explains the different behavior of dark matter in those two collisions. We need more examples."

The team proposed numerous explanations for the findings, but each is unsettling for astronomers. In one scenario, which would have staggering implications, some dark matter may be what astronomers call "sticky." Like two snowballs smashing together, normal matter slams together during a collision and slows down.

However, dark matter blobs are thought to pass through each other during an encounter without slowing down. This scenario proposes that some dark matter interacts with itself and stays behind during an encounter.

Another possible explanation for the discrepancy is that Abell 520 has resulted from a more complicated interaction than the Bullet Cluster encounter. Abell 520 may have formed from a collision between three galaxy clusters, instead of just two colliding systems in the case of the Bullet Cluster.

A third possibility is that the core contained many galaxies, but they were too dim to be seen, even by Hubble. Those galaxies would have to have formed dramatically fewer stars than other normal galaxies. Armed with the Hubble data, the group will try to create a computer simulation to reconstruct the collision and see if it yields some answers to dark matter's weird behavior.

The Hubble Space Telescope is a project of international cooperation between NASA and the European Space Agency. NASA's Goddard Space Flight Center in Greenbelt, Md., manages the telescope. The Space Telescope Science Institute (STScI) in Baltimore, Md., conducts Hubble science operations. STScI is operated by the Association of Universities for Research in Astronomy, Inc., in Washington, D.C.For images and more information about Abell 520’s dark core,


For more information about dark matter,

visit:http://go.nasa.gov/dJzOp1
Guillermo Gonzalo Sánchez Achutegui



miércoles, 22 de febrero de 2012

Astronomy: NASA'S Spitzer Finds Solid Buckyballs in Space

Hi My Friends: AL VUELO DE UN QUINDE EL BLOG., Astronomers using data from NASA's Spitzer Space Telescope have, for the first time, discovered buckyballs in a solid form in space. Prior to this discovery, the microscopic carbon spheres had been found only in gas form. Formally named buckminsterfullerene, buckyballs are named after their resemblance to the late architect Buckminster Fuller's geodesic domes. They are made up of 60 carbon molecules arranged into a hollow sphere, like a soccer ball. Their unusual structure makes them ideal candidates for electrical and chemical applications on Earth, including superconducting materials, medicines, water purification and armor.

Space Balls
NASA's Spitzer Space Telescope has at last found buckyballs in space, as illustrated by this artist's conception showing the carbon balls coming out from the type of object where they were discovered -- a dying star and the material it sheds, known as a planetary nebula.

Buckyballs are made up of 60 carbon atoms organized into spherical structures that resemble soccer balls. They also look like Buckminister Fuller's architectural domes, hence their official name of buckministerfullerenes. The molecules were first concocted in a lab nearly 25 years ago, and were theorized at that time to be floating around carbon-rich stars in space.

But it wasn't until now that Spitzer, using its sensitive infrared vision, was able to find convincing signs of buckyballs. The telescope found the molecules -- as well as their elongated, rugby-ball-like relatives, called C70 -- in the material around a dying star, or planetary nebula, called Tc 1. The star at the center of Tc 1 was once similar to our sun but as it aged, it sloughed off its outer layers, leaving only a dense white-dwarf star. Astronomers believe buckyballs were created in shed layers of carbon that blew off the star. Tc 1 does not show up that well in images, so a picture of the NGC 2440 nebula, taken by NASA's Hubble Space Telescope, was used in this artist's conception.

Image credit: NASA/JPL-Caltech Hubble image credit: NASA, ESA, STScI

Jiggling Soccer-Ball Molecules in Space
These data from NASA's Spitzer Space Telescope show the signatures of buckyballs in space. Buckyballs, also called C60 or buckministerfullerenes, after architect Buckminister Fuller's geodesic domes, are made of 60 carbon atoms structured like a black-and-white soccer ball. They were first discovered in a lab in 1985, but could not be definitively identified in space until now. Spitzer was able to find their spectral signatures -- along with the signatures of their rugby-ball-like relatives, called C70 -- by analyzing the infrared light from Tc 1, a planetary nebula consisting of material shed by a dying star.

Buckyballs jiggle, or vibrate, in a variety of ways -- 174 ways to be exact. Four of these vibrational modes cause the molecules to either absorb or emit infrared light. All four modes were detected by Spitzer.

The space telescope first gathered light from the area around the dying star -- specifically a region rich in carbon -- then, with the help of its spectrograph instrument, spread the light into its various components, or wavelengths. Astronomers studied the data, a spectrum like the one shown here, to identify signatures, or fingerprints, of molecules. The four vibrational modes of buckyballs are indicated by the red arrows. Likewise, Spitzer identified four vibrational modes of C70, shown by the blue arrows.

Image credit: NASA/JPL-Caltech/University of Western Ontario

NASA'S Spitzer Finds Solid Buckyballs in Space

WASHINGTON -- Astronomers using data from NASA's Spitzer Space Telescope have, for the first time, discovered buckyballs in a solid form in space. Prior to this discovery, the microscopic carbon spheres had been found only in gas form.

Formally named buckminsterfullerene, buckyballs are named after their resemblance to the late architect Buckminster Fuller's geodesic domes. They are made up of 60 carbon molecules arranged into a hollow sphere, like a soccer ball.

Their unusual structure makes them ideal candidates for electrical and chemical applications on Earth, including superconducting materials, medicines, water purification and armor. In the latest discovery, scientists using Spitzer detected tiny specks of matter, or particles, consisting of stacked buckyballs.

They found them around a pair of stars called "XX Ophiuchi," 6,500 light-years from Earth. "These buckyballs are stacked together to form a solid, like oranges in a crate," said Nye Evans of Keele University in England, lead author of a paper appearing in the Monthly Notices of the Royal Astronomical Society.

"The particles we detected are miniscule, far smaller than the width of a hair, but each one would contain stacks of millions of buckyballs." Buckyballs were detected definitively in space for the first time by Spitzer in 2010. Spitzer later identified the molecules in a host of different cosmic environments. It even found them in staggering quantities, the equivalent in mass to 15 Earth moons, in a nearby galaxy called the Small Magellanic Cloud. In all of those cases, the molecules were in the form of gas.

The recent discovery of buckyballs particles means that large quantities of these molecules must be present in some stellar environments in order to link up and form solid particles. The research team was able to identify the solid form of buckyballs in the Spitzer data because they emit light in a unique way that differs from the gaseous form.

"This exciting result suggests that buckyballs are even more widespread in space than the earlier Spitzer results showed," said Mike Werner, project scientist for Spitzer at NASA's Jet Propulsion Laboratory in Pasadena, Calif.

"They may be an important form of carbon, an essential building block for life, throughout the cosmos." Buckyballs have been found on Earth in various forms. They form as a gas from burning candles and exist as solids in certain types of rock, such as the mineral shungite found in Russia, and fulgurite, a glassy rock from Colorado that forms when lightning strikes the ground. In a test tube, the solids take on the form of dark, brown "goo."

"The window Spitzer provides into the infrared universe has revealed beautiful structure on a cosmic scale," said Bill Danchi, Spitzer program scientist at NASA Headquarters in Washington. "In yet another surprise discovery from the mission, we're lucky enough to see elegant structure at one of the smallest scales, teaching us about the internal architecture of existence."

NASA's Jet Propulsion Laboratory (JPL) in Pasadena, Calif., manages the Spitzer Space Telescope mission for NASA's Science Mission Directorate in Washington. Science operations are conducted at the Spitzer Science Center at the California Institute of Technology in Pasadena. Caltech manages JPL for NASA. For information about previous Spitzer discoveries of buckyballs,


Guillermo Gonzalo Sánchez Achutegui