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A Whiff of Dark Matter on the ISS
Presented by Science at NASA
In science fiction movies, 
finding antimatter on board your spaceship is not good news. 
Usually, it means you're moments away from an explosion.
In real life, though, 
finding antimatter could lead to a Nobel Prize.
On April 3rd, 
researchers led by Nobel Laureate Samuel Ting of MIT 
announced that the Alpha Magnetic Spectrometer, 
a particle detector 
operating onboard the International Space Station since 2011, 
has counted more than 400,000 positrons, 
the antimatter equivalent of electrons. 
There's no danger of an explosion, 
but the discovery is sending shock waves through the scientific community.
'These data show the existence of a new physical phenomenon,' 
wrote Ting and colleagues 
in an article published in the Physical Review Letters. 
'It could be a sign of dark matter.'
The Alpha Magnetic Spectrometer 
('AMS' for short) 
was delivered to the ISS by the space shuttle Endeavour 
on its final flight in May 2011. 
In its first 18 months of operations, 
from May 19, 2011 to December 10, 2012, 
the AMS analyzed 25 billion cosmic ray events. 
Of these, an unprecedented number 
were unambiguously identified as positrons.
Cosmic rays are subatomic particles 
such as protons and helium nuclei 
accelerated to near-light speed by supernova explosions 
and other violent events in the cosmos. 
Researchers have long thought 
that cosmic rays contain a sprinkling of antimatter. 
Italy's PAMELA satellite detected high-energy positrons in 2009, 
and NASA's Fermi gamma-ray observatory 
confirmed the find two years later.  
But where do the positrons come from? 
The Universe is almost completely devoid of antimatter, 
so the positron fraction of cosmic ray electrons
--as much as 10%--
is a little surprising. 
One idea is dark matter. 
Astronomers know that the vast majority of the material Universe 
is actually made of dark matter 
rather than ordinary matter. 
They just don't know what dark matter is. 
It exerts gravity, 
but emits no light, 
which makes it devilishly difficult to study.
A leading theory holds 
that dark matter is made of a particle called the neutralino. 
Collisions between neutralinos 
should produce a large number of high-energy positrons, 
which the AMS should be able to detect with unprecedented sensitivity.
'The accuracy of our measurements is 1%, 
which is excellent, 
and we have statistics unmatched by any other spacecraft,' 
says Ting.
'So far the evidence supports the hypothesis of dark matter. 
But,' he cautions, 'it does not rule out another possibility--pulsars.'
Pulsars are strongly-magnetized neutron stars 
formed in the aftermath of supernova explosions. 
They can spin on their axes thousands of times a second, 
flinging particles into space with fantastic energies 
that accelerators on Earth can't match. 
Among these particles are pairs of electrons and positrons.
AMS can distinguish between pulsars and dark matter
--but not yet. 
'We need more data at higher energies 
to decide which is the correct explanation,' says Ting. 
'It is only a matter of time, 
perhaps months or a few years.'
Built by scientists from 16 countries 
with support from the US Dept. of Energy, 
the Alpha Magnetic Spectrometer will continue operating 
for the rest of the life of the space station 
at least until 2020. 
Between now and then, 
the mystery of dark matter could be solved, 
once and for all.
Stay tuned for updates from science.nasa.gov
