Answering the question "how did we get here?" is one of the key goals in NASA's Astrophysics Division, and is the prime objective of its Cosmic Origins (COR) Program. The subject of Origins is a very broad one. Some of the questions and topic areas are:
No one space or airborne observatory can provide all the answers. The COR Program includes telescopes-both present and future-that together operate across a wide swath of the electromagnetic spectrum, from the far-ultraviolet through the far-infrared and sub-millimeter. Currently operating facilities in COR are Hubble Space Telescope (HST), Spitzer Space Telescope (SST) and the Herschel Space Observatory. Future facilities and efforts within or with COR related science include the James Webb Space Telescope (JWST), currently in implementation and the #1 recommendation of the 2001 Decadal Survey; advanced future instruments for SOFIA; and studies of a UV-optical successor to HST. Advances in key technologies will enable the building of powerful future facilities.
An exciting aspect of the Program is that the telescopes of the future are significantly more capable than those that have flown before. HST, currently in orbit and at the peak of its scientific powers, has observed galaxies as long ago as only 500-600 million years after the Big Bang. Yet it will take JWST-with a larger mirror and a longer reach into the infrared-to see all the way back to when the first star systems formed, perhaps only 200 million years after the birth of the universe. In science, the past and present inform the dreams and efforts of the future, and that is certainly true in NASA's Cosmic Origins Program.
The inaugural Cosmic Origins Program Annual Technology Report (PATR) - the annual summary of the technology development activities in support of the Cosmic Origins (COR) Program for FY11 - is now available for viewing and download. It provides an overview of the status of prior COR-supported technologies and delineates priorities for future investments.
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NASA will host an open session devoted to encouraging interaction between the astronomical community and the Program Analysis Groups (PAGs). Held at the AAS in Austin on 10 January 2012, this session will provide information illustrating how community members have a voice in coordinating the Astrophysics Division's strategic objectives.
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The COPAG will be holding a splinter meeting on Sunday, 8 January 2012 at the AAS Meeting, Austin, TX. This meeting will provide opportunities for the community to present further science needs and related technologies to augment the COR technology needs list.
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