Science Goals

Explore the behavior of matter and energy in its most extreme environments

Cosmic rays, high-energy charged particles traveling at velocities that can approach the speed of light, are a rich potential probe of chemical and nuclear in the Universe. The majority of cosmic rays are atomic nuclei from hydrogen to the heaviest elements with energies spanning more than twelve orders of magnitude. In the low energy end, these cosmic rays are most likely accelerated in supernova remnants. Their elemental and isotopic composition probes nucleosynthesis, nuclear interactions with the interstellar medium, the distribution of freshly synthesized elements, and the mechanism of supernova explosions. At energies above roughly 1017 eV a different source dominates. The acceleration engines responsible for such extreme energies are not well understood, but at the highest energies, above about 6 × 1019 eV, the rapid energy loss resulting from interactions with the cosmic microwave background limits sources to within about 100 Mpc. Other cosmic ray components include electrons, positrons and antiprotons. While these are largely the result of interactions of nuclear cosmic rays with the ISM, they may have other origins. Positrons and electrons can be produced directly in astrophysical objects such as pulsars and deviations in their spectra can provide important insights into nearby sources. Cosmic ray particles may also be produced directly by the annihilation of dark matter candidates such as nutralinos and Kaluza-Klein particles. Details of the spectra of the resulting particles would therefore provide important constraints on the nature of the dark matter.

Program News

1 Oct 2014
2014 Program Annual Technology Report (PATR) now available »  [PDF]
9 Sep 2014
Astrophysics Division of NASA's Science Mission Directorate issues open call for nominations to serve on Executive Committee of NASA's Physics of the Cosmos Program Analysis Group »  [PDF]
7 Aug 2014
IPSIG White Paper now available »  [PDF]

Project News

Chandra News
16 Sep 2014
NASA's Chandra X-ray Observatory Finds Planet That Makes Star Act Deceptively Old » Details
Fermi News
31 Jul 2014
NASA's Fermi Space Telescope Reveals New Source of Gamma Rays » Details
Planck News
23 Oct 2013
Last Command Sent to ESA's Planck Space Telescope
» Details
XMM-Newton News
1 Sep 2014
Magnetar discovered close to supernova remnant Kesteven 79 » Details

Related News

NuSTAR News
8 Oct 2014
NASA's NuSTAR Telescope Discovers Shockingly Bright Dead Star » Details
Suzaku News
2 Jul 2014
Iron 'Fingerprints' Point Astronomers to Supernova Suspects » Details
Swift News
30 Sep 2014
NASA's Swift Mission Observes Mega Flares from a Mini Star » Details