Mostrando entradas con la etiqueta NASA’s Johnson Space Center. Mostrar todas las entradas
Mostrando entradas con la etiqueta NASA’s Johnson Space Center. Mostrar todas las entradas

jueves, 4 de agosto de 2016

NASA : Astronauts Test Orion Docking Hatch For Future Missions .- Los astronatuas prueban la escotilla de acoplamiento,de la nave espacial Orión, para futuras misiones...........

http://www.nasa.gov/image-feature/astronauts-test-orion-docking-hatch-for-future-missions

Astronauts Test Orion Docking Hatch For Future Missions
Engineers and astronauts conducted testing in a representative model of the Orion spacecraft at NASA’s Johnson Space Center in Houston to gather the crew's feedback on the design of the docking hatch and on post-landing equipment operations. The testing, shown here with astronauts Stephanie Wilson, Karen Nyberg and Rick Mastracchio (L to R), was done to evaluate the equipment used during egress to ensure that a fully suited crew member carrying survival equipment can get out of the spacecraft through the docking hatch if necessary.
 
While the crew will primarily use the side hatch for entry and exit on Earth and the docking hatch to travel between Orion and a habitation module on long-duration deep space missions, the crew will need to be able to exit out of the docking hatch if wave heights in the Pacific Ocean upon splashdown are too high. The work is being done to help ensure all elements of Orion's design are safe and effective for the crew to use on future missions on the journey to Mars.
Image Credit: NASA
Last Updated: Aug. 3, 2016
Editor: Mark Garcia
NASA
Guillermo Gonzalo Sánchez Achutegui
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domingo, 13 de marzo de 2016

NASA : NASA to Discuss Science Launching on Next Commercial Resupply Space Station Flight.- NASA, discute un lanzamiento desde la ciencia para el reabastecimiento en la Estación Espacial Internacional desde un vuelo

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre sus análisis científicos como llegar al reabastecimiento comercial de la Estación Espacial Internacional, mediante un procedimiento de al vuelo, como se hace en aviones comerciales y militares.
More information....

NASA astronaut Tim Kopra sets up hardware for the Burning and Suppression of Solids – Milliken, or BASS-M, experiment.
NASA astronaut Tim Kopra sets up hardware for the Burning and Suppression of Solids – Milliken, or BASS-M, experiment. The BASS-M investigation tests flame-retardant cotton fabrics to determine how well they resist burning in microgravity. Results benefit research on flame-retardant textiles that can be used on Earth and in space
Credits: NASA
 
NASA is hosting a media teleconference at 1 p.m. EDT Tuesday, March 15, to discuss several science investigations launching on the next Orbital ATK commercial resupply flight to the International Space Station.

The briefing participants will be:
  • Marc Fries, principal investigator for Strata-1 at NASA’s Johnson Space Center in Houston
  • Aaron Parness, principal investigator for Gecko Grippers at NASA's Jet Propulsion Laboratory (JPL) in Pasadena, California
  • Matt Napoli, vice president of in-space operations for the Additive Manufacturing Facility for Made In Space in Moffett Field, California
  • Gary Ruff, co-investigator for Saffire at NASA’s Glenn Research Center in Cleveland
  • Michael Fortenberry, principal investigator for Meteor at Southwest Research Institute in San Antonio  

Cygnus is targeted to launch Tuesday, March 22 on a United Launch Alliance Atlas V rocket from Space Launch Complex 41 at Cape Canaveral Air Force Station in Florida, during a 30-minute launch window that opens at approximately 11 p.m. The spacecraft will carry crew supplies, scientific research and hardware to the orbital laboratory to support the Expedition 47 and 48 crews. 

This launch is the fifth contracted mission by Orbital ATK under NASA’s Commercial Resupply Services contract and will be followed later this year by an Orbital ATK resupply mission launching from the agency’s Wallops Flight Facility in Wallops Island, Virginia.

To participate in the teleconference, reporters must contact Kathryn Hambleton at 202-358-1100 or kathryn.hambleton@nasa.gov by 9 a.m. March 15 for dial-in information.

Audio of the teleconference will be streamed live online at: 


For launch countdown coverage, NASA's launch blog, and more information about the mission, visit:


-end-
Kathryn Hambleton
Headquarters, Washington
202-358-1100
kathryn.hambleton@nasa.gov
Last Updated: March 8, 2016
Editor: Karen Northon
 
NASA
Guillermo Gonzalo Sánchez Achutegui
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jueves, 25 de febrero de 2016

NASA : NASA Astronaut Scott Kelly Talks One-Year Mission in Final In-Space News Conference .- Astronauta de la NASA Scott J. Kelly : Final en el Espacio Conferencia Noticias en conversaciones de un año de misión en

Hola amigos: A VUELO DE UN QUINDE EL BLOG., hemos recibido información de la Agencia Espacial NASA, sobre el final de su permanencia en el espacio del astronauta Scott Kelly.
Kelly regresará a la Tierra el 1° de marzo, marcando la finalización de una misión de 340 días en el espacio.
More information...

NASA astronaut Scott Kelly inside the cupola of the International Space Station
NASA astronaut Scott Kelly inside the cupola of the International Space Station, a special module that provides a 360-degree viewing of the Earth and the station. Kelly will return to Earth on March 1, marking completion of a 340-day mission in space.
Credits: NASA
 
NASA astronaut Scott Kelly’s final news conference from orbit will air live on NASA Television at 12:05 p.m. EST Thursday, Feb. 25.

The 30-minute news conference will take place less than a week before Kelly returns to Earth from the International Space Station, marking the completion of a 340-day mission. Media may ask questions from NASA’s Johnson Space Center in Houston or Kennedy Space Center in Florida, as well as by phone.

To attend the briefing at Johnson, media must request credentials from the Johnson newsroom at 281-483-5111 no later than 9 a.m. on Thursday, Feb. 25. To ask questions by phone, media must call the Johnson newsroom no later than 11:45 a.m. on Thursday, Feb. 25. Accreditation for international media is closed for this event.

All media accreditation requests for Kennedy must be submitted by 2 p.m. on Wednesday, Feb. 24 online at:


All media representatives must present two forms of unexpired legal, government identification to access Kennedy. One form must include a photo, such as a passport or driver’s license. Questions about accreditation should be directed to Jennifer Horner at jennifer.p.horner@nasa.gov or 321-867-6598.

Kelly launched to the space station March 27, 2015, from the Baikonur Cosmodrome in Kazakhstan and is set to return on Tuesday, March 1. He will land in Kazakhstan at 11:27 p.m. (10:27 a.m. Kazakhstan time on March 2) with his one-year crewmate, cosmonaut Mikhail Kornienko of the Russian space agency Roscosmos, and cosmonaut Sergey Volkov, also of Roscosmos. Kelly will return to Houston’s Ellington Field on Wednesday, March 2.

After landing, Kelly will hold the record among U.S. astronauts for cumulative time in space, with 520 days. During their record-setting mission, Kelly and Kornienko participated in a number of studies to provide new insights into how the human body adjusts to weightlessness, isolation, radiation and the stress of long-duration spaceflight, which will include the Journey to Mars. Kelly’s twin brother, former NASA astronaut Mark Kelly, participated in parallel twin studies on Earth to help scientists compare the effects on the body and mind in space.

For NASA TV streaming video, schedule and downlink information, visit:


For more information about the International Space Station and its crew, visit:


-end-
Tabatha Thompson
Headquarters, Washington
202-358-1100
tabatha.t.thompson@nasa.gov

Dan Huot
Johnson Space Center, Houston
281-483-5111
daniel.g.huot@nasa.gov
Last Updated: Feb. 23, 2016
Editor: Karen Northon
NASA
Guillermo Gonzalo Sánchez Achutegui
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sábado, 16 de agosto de 2014

NASA : Stardust Team Reports Discovery of First Potential Interstellar Space Particles


Stardust aerogel collectors
The largest interstellar dust track found in the Stardust aerogel collectors was this 35 micron-long hole produced by a 3 picogram mote that was probably traveling so fast that it vaporized upon impact. The other two likely interstellar dust grains were traveling more slowly and remained intact after a soft landing in the aerogel.
Image Credit: 
Andrew Westphal, UC Berkeley
 
Largest interstellar dust track found in the Stardust aerogel collectors
The largest interstellar dust track found in the Stardust aerogel collectors was this 35 micron-long hole produced by a 3 picogram speck of dust that was probably traveling so fast that it vaporized upon impact. The other two likely interstellar dust grains were traveling more slowly and remained in
Image Credit: 
UC Berkeley/Andrew Westphal.
Seven rare, microscopic interstellar dust particles that date to the beginnings of the solar system are among the samples collected by scientists who have been studying the payload from NASA's Stardust spacecraft since its return to Earth in 2006. If confirmed, these particles would be the first samples of contemporary interstellar dust.
A team of scientists has been combing through the spacecraft's aerogel and aluminum foil dust collectors since Stardust returned in 2006.The seven particles probably came from outside our solar system, perhaps created in a supernova explosion millions of years ago and altered by exposure to the extreme space environment.
The research report appears in the Aug. 15 issue of the journal Science. Twelve other papers about the particles will appear next week in the journal Meteoritics & Planetary Science.
"These are the most challenging objects we will ever have in the lab for study, and it is a triumph that we have made as much progress in their analysis as we have," said Michael Zolensky, curator of the Stardust laboratory at NASA’s Johnson Space Center in Houston and coauthor of the Science paper.
Stardust was launched in 1999 and returned to Earth on Jan. 15, 2006, at the Utah Test and Training Range, 80 miles west of Salt Lake City. The Stardust Sample Return Canister was transported to a curatorial facility at Johnson where the Stardust collectors remain preserved and protected for scientific study.
Inside the canister, a tennis racket-like sample collector tray captured the particles in silica aerogel as the spacecraft flew within 149 miles of a comet in January 2004. An opposite side of the tray holds interstellar dust particles captured by the spacecraft during its seven-year, three-billion-mile journey.
Scientists caution that additional tests must be done before they can say definitively that these are pieces of debris from interstellar space. But if they are, the particles could help explain the origin and evolution of interstellar dust.
The particles are much more diverse in terms of chemical composition and structure than scientists expected. The smaller particles differ greatly from the larger ones and appear to have varying histories. Many of the larger particles have been described as having a fluffy structure, similar to a snowflake.
Two particles, each only about two microns (thousandths of a millimeter) in diameter, were isolated after their tracks were discovered by a group of citizen scientists. These volunteers, who call themselves "Dusters," scanned more than a million images as part of a University of California, Berkeley, citizen-science project, which proved critical to finding these needles in a haystack.
A third track, following the direction of the wind during flight, was left by a particle that apparently was moving so fast -- more than 10 miles per second (15 kilometers per second) -- that it vaporized. Volunteers identified tracks left by another 29 particles that were determined to have been kicked out of the spacecraft into the collectors.
Four of the particles reported in Science were found in aluminum foils between tiles on the collector tray. Although the foils were not originally planned as dust collection surfaces, an international team led by physicist Rhonda Stroud of the Naval Research Laboratory searched the foils and identified four pits lined with material composed of elements that fit the profile of interstellar dust particles.
Three of these four particles, just a few tenths of a micron across, contained sulfur compounds, which some astronomers have argued do not occur in interstellar dust. A preliminary examination team plans to continue analysis of the remaining 95 percent of the foils to possibly find enough particles to understand the variety and origins of interstellar dust.
Supernovas, red giants and other evolved stars produce interstellar dust and generate heavy elements like carbon, nitrogen and oxygen necessary for life. Two particles, dubbed Orion and Hylabrook, will undergo further tests to determine their oxygen isotope quantities, which could provide even stronger evidence for their extrasolar origin.
Scientists at Johnson have scanned half the panels at various depths and turned these scans into movies, which were then posted online, where the Dusters could access the footage to search for particle tracks.
Once several Dusters tag a likely track, Andrew Westphal, lead author of the Science article, and his team verify the identifications. In the one million frames scanned so far, each a half-millimeter square, Dusters have found 69 tracks, while Westphal has found two. Thirty-one of these were extracted along with surrounding aerogel by scientists at Johnson and shipped to UC Berkeley to be analyzed.
NASA's Jet Propulsion Laboratory, Pasadena, California, manages the Stardust mission for NASA's Science Mission Directorate, Washington. Lockheed Martin Space Systems, Denver, developed and operated the spacecraft.
For information about the Stardust mission on the Web, visit:
For information about NASA and agency programs on the Web, visit:
 
NASA
Guillermo Gonzalo Sánchez Achutegui
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viernes, 23 de mayo de 2014

NASA : NASA Teams with Web Tech Company Slooh to Bring Universe to Everyone and Help Protect Earth Too

NASA Astronauts Go Underwater to Test Tools for a Mission to an Asteroid

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Astronauts Stan Love and Steve Bowen discuss their work underwater to test tools and techniques for exploring an asteroid.
Image Credit: 
NASA TV
 
Youtube Override: 
Astronauts Stan Love and Steve Bowen practice climbing out of the Orion spacecraft and taking samples from an asteroid in the Neutral Buoyancy Laboratory at Johnson Space Center.
Image Credit: 
NASA TV
Astronaut Steve Bowen
Steve Bowen is lowered into the Neutral Buoyancy Laboratory at Johnson Space Center to test spacewalk suits and tools for a mission to an asteroid.
Image Credit: NASA
 
 NASA is planning to send astronauts to an asteroid in the 2020s, and preparations are already being made.
Stan Love and Steve Bowen have between them spent more than 62 hours in the vacuum of space on nine shuttle mission spacewalks, and they’re putting that experience to use here on Earth by helping engineers determine what astronauts will need on NASA’s next step toward Deep Space. Wearing modified versions of the orange space shuttle launch and entry suits, the two went underwater on May 9, in the Neutral Buoyancy Laboratory at NASA’s Johnson Space Center, a 40-feet-deep swimming pool that helps provide the lack of gravity needed for astronauts to practice for spacewalks. There a mockup of the Orion spacecraft that will carry astronauts to the asteroid, docked to a mockup of the robotic spacecraft that will be used to capture an asteroid and bring it into a stable orbit near the moon, provided the backdrop for the simulated spacewalk.
“We’re working on the techniques and tools we might use someday to explore a small asteroid that was captured from an orbit around the sun and brought back by a robotic spacecraft to orbit around the moon,” Love said. “When it’s there, we can send people there to take samples and take a look at it up close. That’s our main task; we’re looking at tools we’d use for that, how we’d take those samples.”
For instance, one of the primary goals of visiting an asteroid will be to obtain a core sample that shows its layers, intact – such a sample could provide information on the age of the solar system and how it was formed. But the tools geologist use to collect core samples or even chips of rocks aren’t a good idea in space – swinging a hammer in front of your face isn’t safe when the sheet of glass between you and it is necessary to keep you alive. Instead Love and Bowen tried out a pneumatic hammer to give them a feel for whether a battery-powered version might be useful.
And while they did so, they also evaluated a version of the spacesuit that  could be worn on an asteroid. Orion astronauts already needed a launch and entry suit to protect them during the most dynamic phases of their flights. So, rather than add to the weight Orion has to carry into orbit and take up additional space inside the crew module, engineers have been working to turn the shuttle-heritage Advanced Crew Escape Suit – or ACES – into something suitable for spacewalks.
Gloves, boots from the space station spacesuit and bearings to aid in the kind of moves an astronaut would need to do on a spacewalk are giving the modified ACES new life. But they probably won’t be the last of the modifications, and working through some of the tasks the suit will need to accommodate on an asteroid helps the astronauts advise the engineers on what still needs improvement.
“We need some significant modifications to make it easy to translate,” Bowen said. “I can’t stretch my arms out quite as far as in the [space station space suit]. The work envelop is very small. So as we get through, we look at these tasks. These tasks are outstanding to help us develop what needs to be modified in the suit, as well.”
NASA is already working to identify an asteroid that could be reached by a robotic mission to capture it and bring it into a stable orbit around the moon. Once it’s there, the Orion spacecraft and Space Launch System rocket will launch a crew of astronauts to explore it and gather samples. The strategy makes good use of capabilities NASA already has, while also advancing a number of technologies needed for longer-term plans: sending humans to Mars in the 2030s.
 
NASA
Guillermo Gonzalo Sánchez Achutegui

lunes, 28 de abril de 2014

NASA : Spiders in Space Weave a Web of Scientific Inspiration for Spider-Man Fans


The “Spiders in Space” teacher’s guide is available for free download at bioedonline.org
The “Spiders in Space” teacher’s guide is available for free download at bioedonline.org.
Image Credit:
BioEd Online
 
A female golden orb spider in her web, the same type of spider used in the CSI-05 study that inspired the “Spiders in Space” teacher’s guide.
A female golden orb spider in her web, the same type of spider used in the CSI-05 study that inspired the “Spiders in Space” teacher’s guide.
Image Credit:
Danielle Anthony
 
A golden orb spider and its web inside the Commercial Generic Bioprocessing Apparatus Science Insert-05 (CSI-05) spider habitat aboard the International Space Station
A golden orb spider and its web inside the Commercial Generic Bioprocessing Apparatus Science Insert-05 (CSI-05) spider habitat aboard the International Space Station.
Image Credit:
NASA
 
While spiders were busy spinning webs in space, researchers on Earth weaved their knowledge of this activity into educational materials to inspire and motivate students. Now, this free, Web-based guide is being re-released through Scholastic and Sony Pictures as curriculum for educators to leap on the excitement surrounding the release of the film, “The Amazing Spider-Man 2.”
For those who may have missed it, this guide’s inspiration came from real science using spiders in space. And although the spiders were exposed to microgravity and radiation in space, they did not morph into mutants; rather, they adapted quite well and provided a biology lesson learned around the world.
Using information gleaned from the Commercial Generic Bioprocessing Apparatus Science Insert-05 (CSI-05) investigation conducted aboard the International Space Station, BioServe Space Technologies, Baylor College of Medicine and NASA developed an educational guide for teachers called “Spiders in Space.” The learning tool was also funded by grants from the Howard Hughes Medical Institute and the Houston Endowment Inc., and previous work supported by the National Space Biomedical Research Institute.
“From an educational standpoint, the fact that a large commercial enterprise was willing to work with science institutions to promote lessons that we know are accurate, have been evaluated and are engaging for students, is really valuable,” said Nancy Moreno, Ph.D., professor at Baylor College of Medicine and editorial director of BioEd Online. “To be able to leverage this resource for something like ‘The Amazing Spider-Man 2’ expands the scope and increases the reach of the project. We hope it generates interest in and enthusiasm for research on the space station by new audiences.”
Launched with the STS-134 mission aboard space shuttle Endeavour to the space station in 2011, CSI-05 allowed researchers to observe spiders in a microgravity environment. Two golden orb spiders, or Nephila clavipes, were flown aboard the space station in a special habitat. This allowed researchers to study the spiders’ web-spinning practices to see if that behavior or the characteristics of the web they produced would change over time. The habitat’s cameras collected imagery throughout the spiders’ time in microgravity to document any differences between those in space and the same type of spiders on the ground.
As it turns out, the golden orb spiders’ behavior did not change greatly in microgravity. Their webs looked much like webs spun on Earth, though in space the webs were more circular. The research found that the golden orb spiders liked to spin their webs following a timetable, in contrast to orb spiders from a previous investigation who would spin webs at all times of day.
As the spiders spun their space webs, students were able to use the downlinked imagery to compare the space spiders to golden orb spiders housed in their classrooms on Earth. Educators for grades kindergarten through 12 were able to conduct investigations of these spiders in their classrooms in near real time. Thanks to the “Spiders in Space” teacher’s guide developed during and following the CSI-05 investigation, this curriculum is still in use.
The free guide is available on the BioEd Online website, which provides a plethora of resources to science educators and is run by Baylor College of Medicine. The guide features background information, lesson plans and student activities for conducting a project similar to the space station investigation and adapted for the classroom. The goal of the curriculum is to encourage learning and interest in science, technology, engineering and mathematics (STEM). The guide is accompanied by video, including a demonstration of how to set up classroom spider habitats and other classroom resources.
"Spiders and space are two things that capture the imagination of most kids, so it's a recipe for fascinating science in the schools," said Tara Ruttley, Ph.D., associate program scientist for the International Space Station. "I think this creates great memories for the students, and a way to show them how science can be fun as their science classes become more challenging through the years."
Using this guide, students participate in inquiry-based learning about web spinning and other behaviors of orb weaving spiders on Earth and in microgravity. Students who engage in the scientific process themselves are more likely to be inspired to become the next generation of explorers and researchers. This will likely be their first introduction to an investigation in the space environment and its implications for scientific research. They learn how to conduct a controlled experiment, practice humane animal-handling and experimental procedures, make detailed observations over time and compare their control experiment results to those obtained in the original spaceflight investigation.
With renewed interest in the “Spiders in Space” guide generated by the film, many more educators and students will be exposed to this valuable research activity. Students around the globe will have opportunities to become scientists in the classroom, inspired by a project that gives them the opportunity to create, study and solve problems.
“We hope to generate an appreciation of the unseen natural world and its importance,” said Moreno. “The possibility of students carefully observing the behavior of organisms is a real opportunity. Their ability - based on their own observations - to then ask meaningful questions and collect data to answer those questions helps develop their problem-solving skills.”
With promotion through the release of a new Spider-Man film, these “spidernauts” are recommencing their fame. With the “Spiders in Space” guide, educators are recapturing enthusiasm for these arachnids, and their intricate webs will continue to hold fast on students’ attention long after the closing credits.

Youtube Override:
Laura Niles
International Space Station Program Science Office and Public Affairs Office
NASA’s Johnson Space Center
NASA
Guillermo Gonzalo Sánchez Achutegui
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viernes, 8 de noviembre de 2013

NASA : NASA and International Researchers Obtain Crucial Data from Meteoroid Impact

 
Orbit diagram
This diagram shows the orbit of asteroid 2013 TV135 (in blue), which has just a 1-in-63,000 chance of impacting Earth. Its risk to Earth will likely be further downgraded as scientists continue their investigations.
Image Credit: NASA/JPL-Caltech
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Newly discovered asteroid 2013 TV135 made a close approach to Earth on Sept. 16, when it came within about 4.2 million miles (6.7 million kilometers). The asteroid is initially estimated to be about 1,300 feet (400 meters) in size and its orbit carries it as far out as about three quarters of the distance to Jupiter's orbit and as close to the sun as Earth's orbit. It was discovered on Oct. 8, 2013, by astronomers working at the Crimean Astrophysical Observatory in Ukraine. As of Oct. 14, asteroid 2013 TV135 is one of 10,332 near-Earth objects that have been discovered.
With only a week of observations for an orbital period that spans almost four years, its future orbital path is still quite uncertain, but this asteroid could be back in Earth’s neighborhood in 2032. However, NASA’s Near-Earth Object Program Office states the probability this asteroid could then impact Earth is only one in 63,000. The object should be easily observable in the coming months and once additional observations are provided to the Minor Planet Center in Cambridge, Mass., the initial orbit calculations will be improved and the most likely result will be a dramatic reduction, or complete elimination, of any risk of Earth impact.
"To put it another way, that puts the current probability of no impact in 2032 at about 99.998 percent," said Don Yeomans, manager of NASA's Near-Earth Object Program Office at the Jet Propulsion Laboratory in Pasadena, Calif. "This is a relatively new discovery. With more observations, I fully expect we will be able to significantly reduce, or rule out entirely, any impact probability for the foreseeable future."
NASA detects, tracks and characterizes asteroids and comets passing close to Earth using both ground- and space-based telescopes. The Near-Earth Object Observations Program, commonly called "Spaceguard," discovers these objects, characterizes a subset of them and identifies their orbits to determine if any could be potentially hazardous to our planet.
JPL manages the Near-Earth Object Program Office for NASA's Science Mission Directorate in Washington. JPL is a division of the California Institute of Technology in Pasadena.
More information about asteroids and near-Earth objects is at:
A team of NASA and international scientists for the first time has gathered a detailed understanding of the effects on Earth from a small asteroid impact.
The unprecedented data obtained as the result of the airburst of a meteoroid over the Russian city of Chelyabinsk on Feb. 15, has revolutionized scientists' understanding of this natural phenomenon.
The Chelyabinsk incident was well observed by citizen cameras and other assets. This factor provided a unique opportunity for researchers to calibrate the event, with implications for the study of near-Earth objects (NEOs) and the development of hazard mitigation strategies for planetary defense. Scientists from nine countries now have established a new benchmark for future asteroid impact modeling.
"Our goal was to understand all circumstances that resulted in the shock wave," said meteor expert Peter Jenniskens, co-lead author of a report published in the journal Science.
Jenniskens, a meteor astronomer at NASA’s Ames Research Center and the SETI Institute, participated in a field study led by Olga Popova of the Institute for Dynamics of Geospheres of the Russian Academy of Sciences in Moscow in the weeks following the event.
“It was important that we followed up with the many citizens who had firsthand accounts of the event and recorded incredible video while the experience was still fresh in their minds," said Popova.
By calibrating the video images from the position of the stars in the night sky, Jenniskens and Popova calculated the impact speed of the meteor at 42,500 mph (19 kilometers per second). As the meteor penetrated through the atmosphere, it fragmented into pieces, peaking at 19 miles (30 kilometers) above the surface. At that point the superheated meteor appeared brighter than the sun, even for people 62 miles (100 kilometers) away.
Because of the extreme heat, many pieces of the meteor vaporized before reaching Earth. Scientists believe that between 9,000 to 13,000 pounds (4,000 to 6,000 kilograms) of meteorites fell to the ground. This amount included one fragment weighing approximately 1,400 pounds (650 kilograms). This fragment wasrecovered from Lake Chebarkul on Oct. 16 by professional divers guided by Ural Federal University researchers in Yekaterinburg, Russia.
NASA researchers participating in the 59 member consortium study suspect the abundance of shock fractures in the rock contributed its breakup in the upper atmosphere. Meteorites made available by Chelyabinsk State University researchers were analyzed to learn about the origin of the shock veins and their physical properties. Shock veins are caused by asteroid collisions. When asteroid collide with each other, heat generated by the impact causes iron and nickel components of the objects to melt. These melts cool into thin masses, forming metal veins – shock veins – in the objects.
"One of these meteorites broke along one of these shock veins when we pressed on it during our analysis," said Derek Sears, a meteoriticist at Ames.
Mike Zolensky, a cosmochemist at NASA’s Johnson Space Center in Houston, may have found why these shock veins (or shock fractures), were so frail. They contained layers of small iron grains just inside the vein, which had precipitated out of the glassy material when it cooled.
"There are cases where impact melt increases a meteorite's mechanical strength, but Chelyabinsk was weakened by it," said Zolensky.
The impact that created the shock veins may have occurred as long ago as 4.4 billion years. This would have been 115 million years after the formation of the solar system, according to the research team, who found the meteorites had experienced a significant impact event at that time.
“Events that long ago affected how the Chelyabinsk meteoroid broke up in the atmosphere, influencing the damaging shockwave,” said Jenniskens.
NASA’s Near-Earth Object Program sponsors research to better understand the origin and nature of NEOs. These essential studies are needed to inform our approach to preparing for the potential discovery and deflection of an object on a collision course with the Earth.
NASA's recently announced asteroid initiative includes the first mission to capture and relocate an asteroid, as well as a grand challenge to find and characterize all asteroid threats to human population. It represents an unprecedented technological feat that will lead to new scientific discoveries and technological capabilities that will help protect our home planet.
Aside from representing a potential threat, the study of asteroids and comets represent a valuable opportunity to learn more about the origins of our solar system, the source of water on the Earth, and even the origin of organic molecules that lead to the development of life.
For more information about the Chelyabinsk field study visit:
For more information on asteroids and comets, visit:
For more information about NASA, visit:
NASA
Guillermo Gonzalo Sánchez Acgutegui