NASA Spacecraft Reveals New Observations of Interstellar Matter

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Jan. 31, 2012

Dwayne Brown                                    
Headquarters, Washington                                     
202-358-1726 
dwayne.c.brown@xxxxxxxx 

Susan Hendrix 
Goddard Space Flight Center, Greenbelt, Md. 
301-286-7745 
susan.m.hendrix@xxxxxxxx 

RELEASE: 11-036

NASA SPACECRAFT REVEALS NEW OBSERVATIONS OF INTERSTELLAR MATTER

WASHINGTON -- NASA's Interstellar Boundary Explorer (IBEX) has 
captured the best and most complete glimpse yet of what lies beyond 
the solar system. The new measurements give clues about how and where 
our solar system formed, the forces that physically shape our solar 
system, and the history of other stars in the Milky Way. 

The Earth-orbiting spacecraft observed four separate types of atoms 
including hydrogen, oxygen, neon and helium. These interstellar atoms 
are the byproducts of older stars, which spread across the galaxy and 
fill the vast space between stars. IBEX determined the distribution 
of these elements outside the solar system, which are flowing charged 
and neutral particles that blow through the galaxy, or the so-called 
interstellar wind. 

"IBEX is a small Explorer mission and was built with a modest 
investment," said Barbara Giles, director of the Heliophysics 
Division at NASA Headquarters in Washington. "The science 
achievements though have been truly remarkable and are a testament to 
what can be accomplished when we give our nation's scientists the 
freedom to innovate." 

In a series of science papers appearing in the Astrophysics Journal on 
Jan. 31, scientists report finding 74 oxygen atoms for every 20 neon 
atoms in the interstellar wind. In our own solar system, there are 
111 oxygen atoms for every 20 neon atoms. This translates to more 
oxygen in any part of the solar system than in nearby interstellar 
space. 

"Our solar system is different than the space right outside it, 
suggesting two possibilities," says David McComas, IBEX principal 
investigator, at the Southwest Research Institute in San Antonio. 
"Either the solar system evolved in a separate, more oxygen-rich part 
of the galaxy than where we currently reside, or a great deal of 
critical, life-giving oxygen lies trapped in interstellar dust grains 
or ices, unable to move freely throughout space." 

The new results hold clues about the history of material in the 
universe. While the big bang initially created hydrogen and helium, 
only the supernovae explosions at the end of a star's life can spread 
the heavier elements of oxygen and neon through the galaxy. Knowing 
the amounts of elements in space may help scientists map how our 
galaxy evolved and changed over time. 

Scientists want to understand the composition of the boundary region 
that separates the nearest reaches of our galaxy, called the local 
interstellar medium, from our heliosphere. The heliosphere acts as a 
protective bubble that shields our solar system from most of the 
dangerous galactic cosmic radiation that otherwise would enter the 
solar system from interstellar space. 

IBEX measured the interstellar wind traveling at a slower speed than 
previously measured by the Ulysses spacecraft, and from a different 
direction. The improved measurements from IBEX show a 20 percent 
difference in how much pressure the interstellar wind exerts on our 
heliosphere. 

"Measuring the pressure on our heliosphere from the material in the 
galaxy and from the magnetic fields out there will help determine the 
size and shape of our solar system as it travels through the galaxy," 
says Eric Christian, IBEX mission scientist, at NASA's Goddard Space 
Flight Center in Greenbelt, Md. 

The IBEX spacecraft was launched in October 2008. Its science 
objective is to discover the nature of the interactions between the 
solar wind and the interstellar medium at the edge of our solar 
system. 

The Southwest Research Institute developed and leads the IBEX mission 
with a team of national and international partners. The spacecraft is 
one of NASA's series of low-cost, rapidly developed missions in the 
Small Explorers Program. Goddard manages the program for the agency's 
Science Mission Directorate at NASA Headquarters in Washington. 

For more information about IBEX, visit: 

http://www.nasa.gov/ibex 

	
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