NASA, Partners Announce LAUNCH: Systems Challenge Forum

NASA, the U.S. Agency for International Development (USAID), the U.S. State Department and Nike Inc. will host the fifth forum of the LAUNCH initiative at NASA's Jet Propulsion Laboratory in Pasadena, Calif. Friday, Sept. 27 and Saturday, Sept. 28.

This year's forum, LAUNCH: Systems Challenge, seeks to identify and accelerate solutions in futuristic materials that will help enable exploration beyond our atmosphere and reduce humanity's harmful footprint on our planet. Ten finalists were chosen to attend the forum to work with experts from government and industry.

During the forum, LAUNCH innovators will discuss their most pressing business and program issues with LAUNCH Council members, who represent the business, textile, investment, international development, policy, engineering, science, communications and sustainability sectors. The sessions are designed to identify key challenges and opportunities for the entrepreneurs' innovations in an effort to accelerate their solutions toward greater global impact.

Innovators were chosen for their groundbreaking technologies and programs. Considerations included the potential to revolutionize the future of fabrics and low-impact production; demonstration of a clear commitment to positive social and environmental impact and reducing the harmful consumption of planetary resources; and the potential to help unlock a new era of exploration.

A link to live video of the conference, along with additional information on the innovations, is available online at:

Welcome

Media interested in attending the forum should contact Molly Conroy at Molly.Conroy@nike.com.

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NASA, Partners Announce LAUNCH: Systems Challenge Forum

NASA Picks 10 Innovative Space Tech Ideas for Funding

NASA has awarded grants 10 innovative university projects that promise to help the space agency develop the advanced technologies it needs for future long-duration manned spaceflights and research.

The agency's Space Technology Research Grants Program will give about $250,000 to each of the one-year projects, with the possibility of another year of funding contingent on technical progress, NASA officials announced Wednesday (Sept. 25).

Some projects are aimed at developing the space technologies NASA needs for lengthy manned space missions beyond low-Earth orbit, including proposals to improve the recovery ofoxygen from carbon dioxide for astronaut life-support systems, and enhancing the storage and transfer of cryogenic fuel in a zero gravity environment. [NASA's Space Tech Goals for 2014 (Gallery)]

Other projects will explore advanced optics technologies that could help scientists obtain better measurements of distant cosmic objects, which could lead to a better understanding of exoplanets, galaxy evolution and the early moments of the universe, NASA officials said in a statement.

Still other projects will explore new ways to trackasteroidsthat could pose a threat to humanity.

These early stage innovation grants are given out under NASA's relatively newSpace Technology Program, which was born out of President Barack Obama's fiscal year 2011 budget request. The program is intended to spur innovative ideas from commercial industries, universities and even citizens.

"A critical element of America's space technology pipeline rests in the cutting edge research in the early stage technologies conducted at the nation's universities," NASA's Associate Administrator for Space Technology, Michael Gazarik, said in a statement. "Through this investment NASA will continue to benefit from university-led R and D."

Below is a list of the universities and proposal titles that NASA selected:

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NASA Selects Early Stage Innovation Proposals from 10 Universities

NASA has selected 10 university-led proposals for study of innovative, early stage space technologies that address high priority technical needs America's space program must master to enable future missions.

The one-year grants from NASA's Space Technology Research Grants Program are worth about $250,000 each, with an additional year of research possible. Selected proposals address technology challenges that may improve astrophysics scientific instruments, oxygen recovery for space life support systems, cryogenic propellant storage for long-duration space exploration, our identification, characterization and protection from near-Earth asteroids.

"A critical element of America's space technology pipeline rests in the cutting edge research in the early stage technologies conducted at the nation's universities," said NASA's Associate Administrator for Space Technology, Michael Gazarik, in Washington. "Through this investment NASA will continue to benefit from university-led R and D."

The selected technology research areas require dramatic improvements over existing capabilities for future science and human exploration missions. Early stage, or low technology readiness level, technologies could mature into tools that solve the difficult challenges facing future NASA missions.

Universities selected for NASA's early stage innovation grants and the titles of their proposals are:

- Johns Hopkins University, Baltimore; "Detection, tracking, and identification of asteroids through on-board image analysis" - Michigan Technological University, Houghton, Mich.; "A new experiment for determining evaporation and condensation coefficients of cryogenic propellants and development of an efficient computational model of cryogenic film stability in microgravity" - Northwestern University, Evanston, Ill.; "Broadband electrically tunable monolithic mid-infrared laser" - Purdue University, West Lafayette, Ind.; "Innovations in understanding and modeling cryogenic propellants for long-duration spaceflight" - University of Arkansas, Fayetteville; "Asynchronous A/D converter for in situ instruments operating under extreme environments" - University of Colorado, Boulder; "Comprehensive modeling of the effects of hazardous asteroid mitigation techniques" - University of Florida, Gainesville; "Bio-inspired broadband antireflection coatings at long wavelengths for space applications" - University of Michigan, Ann Arbor; "Broad bandwidth metamaterial antireflection coatings for measurement of the cosmic microwave background" - University of South Carolina, Columbia; "Oxygen recovery via carbon dioxide electrolysis with microtubular solid oxide cells" - University of Utah, Salt Lake City; "A lightweight compact multi-spectral imager using novel computer-generated micro-optics and spectral-extraction algorithms"

The selected efforts will explore new science instrument technologies to better understand the history, climates, evidence of past life and future potential habitability of planets and moons within our solar system.

Researchers will investigate advances in optics technologies. These could enable the challenging science measurements that may contribute to the understanding of the first moments of the universe, the characterization of galaxy evolution over time and the characterization of newly found exoplanets, which are planets outside our solar system.

Researchers also will explore technologies that are needed for future long duration human space exploration beyond low-Earth orbit, including improvements in the recovery of oxygen from carbon dioxide, as well as greatly increasing the capability to store and transfer cryogenic fluids in a zero gravity environment.

In addition, researchers will develop technologies to better understand and protect our planet from near-Earth asteroids. Advancing early stage technologies will help with characterizing, understanding, and planning how to mitigate the threat of near-Earth asteroids.

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NASA Selects Early Stage Innovation Proposals from 10 Universities

NASA radar device detects heartbeats in disaster rubble

NASA is collaborating with the US Department of Homeland Security on a portable radar device that can detect heartbeats and breathing after a disaster.

The Finder unit during a test.

When a disaster strikes, there's a very short window of time in which to locate and free survivors trapped under rubble. The Finder portable radar system, developed through a collaboration between NASA and the US Department of Homeland Security, could make it much easier for emergency responders to find victims.

"Finder" is short for "Finding Individuals for Disaster and Emergency Response." The device works by sending a low-power microwave radar signal through the rubble. The signals that bounce back are analyzed for patterns that indicate a person's breathing or heartbeat.

The technology is related to radar systems NASA uses to locate spacecraft on their missions. "Detecting small motions from the victim's heartbeat and breathing from a distance uses the same kind of signal processing as detecting the small changes in motion of spacecraft like Cassini as it orbits Saturn," says James Lux, the Finder task manager at NASA's Jet Propulsion Lab.

The heavy lifting for this technology is done on the data processing side. It takes advanced algorithms to differentiate between a human's chest moving versus a rat scurrying, or a plant's leaves waving.

Finder can see through up to 20 feet of solid concrete. The device has been in testing for about a year. The whole unit weighs less than 20 pounds and could be useful for a variety of disaster scenarios, from tornadoes to earthquakes.

Locating disaster victims is Finder's first purpose, but NASA is looking ahead at potential uses in space. The system could be adapted to monitor astronauts without the need for wires. Meanwhile, on Earth, the technology could be ready and available for wider use by spring of 2014.

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NASA radar device detects heartbeats in disaster rubble

NASA Media Resources Available on New International Climate Report

NASA will make scientists and data visualizations available to journalists Friday, Sept. 27, with the release of a portion of the Fifth Assessment Report from the United Nations' Intergovernmental Panel on Climate Change (IPCC).

The IPCC will issue the "Summary for Policymakers" of the "Physical Science Basis of Climate Change" section of the report in Stockholm on Friday and the full text of that section Monday, Sept. 30. Additional sections will be released in the coming months.

More than 25 NASA scientists helped author and review the Fifth Assessment Report. NASA also will provide unique data visualizations of projected temperature and precipitation changes for the 21st century, based on climate models referenced in the report.

NASA satellite observations, scientific analysis and climate modeling contributed to the report's conclusions on such topics as temperature change, sea level rise, changes to glaciers and ice sheets, and Earth's global energy balance. NASA climate models contributed to the international modeling effort to project climate change throughout the 21st century. NASA scientists also played a key role in evaluating climate model accuracy by comparing models to NASA satellite observations.

The following NASA scientists -- listed with their hosting NASA facilities and points of contacts for media interviews -- participated in the "Physical Science Basis of Climate Change" and the "Summary for Policymakers":

Goddard Institute for Space Studies, New York: Drew Shindell, coordinating lead author, Chapter 8: Anthropogenic and Natural Radiative Forcing; drafting author, Summary for Policymakers Gavin Schmidt, expert reviewer, Chapters: 1: Introduction; 5: Information from Paleoclimate Archives; 8: Anthropogenic and Natural Radiative Forcing, and; 9: Evaluation of Climate Models Media contact: Leslie McCarthy at leslie.m.mccarthy@nasa.gov or 212-678-5507.

Goddard Space Flight Center, Greenbelt, Md.: Joey Comiso, coordinating lead author, Chapter 4: Observations: Cryosphere Peter Hildebrand, expert reviewer, Chapter 4: Observations: Cryosphere Media contact: Rani Gran at rani.c.gran@nasa.gov or 301-286-2483.

Jet Propulsion Laboratory, Pasadena, Calif.: Graeme Stephens, contributing author, Chapter 7: Clouds and Aerosols; lead author, Chapter 8: Anthropogenic and Natural Radiative Forcing; expert reviewer, Chapter 9: Evaluation of Climate Models Eric Rignot (JPL/University of California-Irvine), lead author, Chapter 4: Observations: Cryosphere Duane Waliser, expert reviewer, Chapter 9: Evaluation of Climate Models Media contact: Alan Buis at alan.d.buis@jpl.nasa.gov or 818-354-0474.

The visualizations of climate model projections show how global temperature and precipitation patterns are expected to change through the year 2100. The projections are based on the carbon emissions scenarios used in "Physical Science Basis of Climate Change." The visualizations will be available online at 8 a.m. EDT Sept. 27 at: http://go.nasa.gov/18rLWnq

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Space Station Astronaut Demonstrates the COLBERT Treadmill | NASA Science Video – Video


Space Station Astronaut Demonstrates the COLBERT Treadmill | NASA Science Video
Visit my website at http://www.junglejoel.com - Expedition 37 flight engineer Karen Nyberg demonstrates how astronauts use the COLBERT treadmill in the weigh...

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Space Station Astronaut Demonstrates the COLBERT Treadmill | NASA Science Video - Video

NASA's Hubble and Chandra Find Evidence for Densest Nearby Galaxy

WASHINGTON, Sept. 24 -- NASA issued the following news release:

Astronomers using NASA's Hubble Space Telescope and Chandra X-ray Observatory and telescopes on the ground may have found the most crowded galaxy in our part of the universe.

The ultra-compact dwarf galaxy, known as M60-UCD1, is packed with an extraordinary number of stars and may be the densest galaxy near Earth. It is providing astronomers with clues to its intriguing past and its role in the galactic evolutionary chain.

M60-UCD1, estimated to be about 10 billion years old, is near the massive elliptical galaxy NGC 4649, also called M60, about 54 million light years from Earth. It is the most luminous known galaxy of its type and one of the most massive, weighing 200 million times more than our sun, based on observations with the W.M. Keck Observatory 10-meter telescope in Hawaii.

What makes M60-UCD1 so remarkable is that about half of this mass is found within a radius of only about 80 light years. The density of stars is about 15,000 times greater -- meaning the stars are about 25 times closer to each other -- than in Earth's neighborhood in the Milky Way galaxy.

"Traveling from one star to another would be a lot easier in M60-UCD1 than it is in our galaxy, but it would still take hundreds of years using present technology," said Jay Strader of Michigan State University in Lansing. Strader is the lead author of a paper about the research, which was published Sept. 20 in The Astrophysical Journal Letters.

The 6.5-meter Multiple Mirror Telescope in Arizona was used to study the amount of elements heavier than hydrogen and helium in stars in M60-UCD1. The values were found to be similar to our sun.

"The abundance of heavy elements in this galaxy makes it a fertile environment for planets and, potentially, for life to form," said co-author Anil Seth of the University of Utah.

Another intriguing aspect of M60-UCD1 is the presence of a bright X-ray source in its center, revealed in Chandra data. One explanation for this source is a giant black hole weighing in at about 10 million times the mass of our sun.

Astronomers want to find out whether M60-UCD1 was born as a jam-packed star cluster or became more compact as stars were ripped away from it. Large black holes are not found in star clusters, so if the X-ray source is in fact due to a massive black hole, it was likely produced by collisions between M60-UCD1 and one or more nearby galaxies. M60-UCD1's great mass and the abundances of elements heavier than hydrogen and helium are also arguments for the theory it is the remnant of a much larger galaxy.

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NASA's Hubble and Chandra Find Evidence for Densest Nearby Galaxy

12 NASA Explorer Schools Receive Honor Awards and Grants

NASA has recognized 12 NASA Explorer Schools from 11 U.S. states for their contributions to science, technology, engineering or mathematics (STEM) education in the 2012-2013 school year.

All 12 schools will receive a NASA certificate of recognition that includes an American flag that was flown in space. Six of the 12 also submitted successful proposals to a recent NASA Explorer Schools solicitation and will receive a $5,000 grant to help implement a STEM project in their classrooms by April 2014.

The schools identified as leaders in STEM education and selected to receive a NASA Explorer Schools Honor Award are:

Forest Lake Technology Magnet, Columbia, S.C. Academy of Information Technology and Engineering, Stamford, Conn. Woodrow Wilson Middle School, Glendale, Calif. Mack Benn Jr. Elementary School, Suffolk, Va. Franke Park Elementary School, Fort Wayne, Ind. Ferndale Middle School, High Point, N.C.

The six schools also receiving a $5,000 grant are:

Cardinal Gibbons High School, Raleigh, N.C. Northland Preparatory Academy, Flagstaff, Ariz. Stoney Creek High School, Rochester Hills, Mich. St. Marys Visitation School, Elm Grove, Wis. Corpus Christi Catholic School, Chambersburg, Pa. Our Lady of Perpetual Help, Germantown, Tenn.

"Congratulations to the 2012-2013 honor award and grant winners," said Diane DeTroye, NASA's director of STEM engagement in Washington. "By using NASA educational resources, innovative teachers brought new approaches to their classrooms to engage their students in STEM studies."

A team of NASA education professionals selected these 12 schools for their exemplary classroom practices and innovative uses of NASA educational content to engage a broad school population in STEM activities.

The NASA Explorer Schools project infuses STEM content related to the agency's missions and programs into classroom lessons for students in grades 4-12.

For more information about NASA Explorer Schools visit: http://explorerschools.nasa.gov

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12 NASA Explorer Schools Receive Honor Awards and Grants