HEAD High Energy Astrophysics Division

HEADNEWS: THE ELECTRONIC NEWSLETTER OF THE HIGH ENERGY ASTROPHYSICS DIVISION OF THE AAS




Newsletter No. 98, June 2011

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14. NASA Gravitational Wave News (Formerly LISA News) - Michele Vallisneri (JPL)

Based on discussions with the European Space Agency (ESA) at the spring ESA-NASA bilateral meeting, the LISA project can provide the following information. Readers are advised to refer to ESA postings for details and clarifications regarding the Cosmic Vision Programme.

LISA was competing with X-ray and outer-planets missions for the L1 opportunity in ESA's Cosmic Vision Programme (2015-2025). The U.S. decadal survey rankings and NASA's constrained out-year resources, as projected in the President's FY12 Budget Request, have led ESA to conclude that none of the three mission concepts were feasible within the Cosmic Vision L1 schedule.

ESA has ended the study of LISA and the other concepts as partnerships at the scale proposed in the New Worlds New Horizons decadal survey (NWNH). ESA has begun a rapid definition effort that includes the formation of a new science team. That effort will identify science goals and a mission concept that can be implemented as part of an ESA-led mission launching in the early 2020's. Revised mission concepts from the three science areas will be considered in a selection process commencing in February 2012. A future minor role for NASA in the ESA-led mission has not been ruled out. NASA is participating in the new ESA science team through a NASA civil servant scientist who will act as conduit for input from and information to the US science community.

NASA's Astrophysics Division is continuing basic funding for the LISA study team through FY11. The Division will engage the community about strategic investments in gravitational-wave astrophysics and possible solicitations for new concept studies, in the context of NWNH recommendations and projected resources. A US science team will be asked to provide input from the community on the way forward in gravitational-wave astronomy including scientific and technical assessments.

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