This just in: The Solar System is different from the space just outside it.
Researchers announced the finding at a press conference on Jan. 31, 2012. Its based on data from NASAs IBEX spacecraft, which is able to sample material flowing into the solar system from interstellar space.
Weve detected alien matter that came into our solar system from other parts of the galaxy--and, chemically speaking, its not exactly like what we find here at home. says David McComas the principal investigator for IBEX at the Southwest Research Institute in San Antonio, Texas.
Our solar system is surrounded by the heliosphere, a magnetic bubble that separates us from the rest of the Milky Way. Outside the heliosphere lies the realm of the stars or interstellar space; inside lies the sun and all the planets. The sun blows this vast magnetic bubble using the solar wind to inflate the suns own magnetic field. Its a good thing: The heliosphere helps protect us from cosmic rays that would otherwise penetrate the solar system.
Launched in 2008, the IBEX spacecraft spins in Earth orbit scanning the entire sky. IBEXs special trick is detecting neutral atoms that slip through the heliospheres magnetic defenses. Without actually exiting the solar system, IBEX is able to sample the galaxy outside.
The first two years of counting these alien atoms have led to some interesting conclusions:
"We've directly measured four separate types of atoms from interstellar space and the composition just doesn't match up with what we see in the solar system," says Eric Christian, mission scientist for IBEX at NASA's Goddard Space Flight Center in Greenbelt, Md.
Among the four types of atoms detectedH, He, O and Nethe last one, neon, serves as a particularly useful reference. Neon is a noble gas, so it doesnt react with anything. And its relatively abundant, so we can measure it with good statistics, explains McComas.
Using data from IBEX, the researchers team compared the neon-to-oxygen ratio inside vs. outside the heliosphere. In a series of six science papers appearing in the Astrophysical Journal, they reported that for every 20 neon atoms in the galactic wind, there are 74 oxygen atoms. In our own solar system, however, for every 20 neon atoms there are 111 oxygen atoms.
That translates to more oxygen in any given slice of the solar system than in local interstellar space.
Where did the extra oxygen come from?
There are at least two possibilities," says McComas. "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 spaceand thus undetectable by IBEX."
Either way, this affects scientific models of how our solar system and life formed.
Its a real puzzle, he says.
While IBEX samples alien atoms from Earth orbit, NASAs Voyager spacecraft have been traveling to the edge of the heliosphere for nearly 40 yearsand they could soon find themselves on the outside looking in. Researchers expect Voyager 1 to exit the solar system within the next few years. The new data from IBEX suggest the Voyagers are heading for a new frontier, indeed.
Explore further: Going a long way to do a quick data collection