Due to the lapse in federal government funding, NASA is not updating this website.

Suggested Searches

Gravitational Wave Mission Concepts Study

2012 Architecting Study

A study initiated by NASA's Physics of the Cosmos Program to develop mission concepts that could meet some or all of the objectives outlined in the New Worlds, New Horizons decadal report.

About Gravitational Wave Mission Concepts Study

New Mission Concepts to Meet New Objectives

The study began with the release of a formal Request for Information (RFI). In parallel, NASA released an open solicitation inviting members of the science community to participate in a Community Science Team (CST) for the X-ray mission.

A Physics of the Cosmos Program study team working with the CST identified the requirements relevant to each concept, defined the mission configuration options, executed mission design runs at mission design laboratories, refined the mission concepts, and drafted a mission concept study reports.

The Gravitational Wave Mission Concepts Workshop about New Mission Concepts to Meet New Objectives
The LISA (Laser Interferometer Space Antenna) mission, led by ESA (European Space Agency) with NASA contributions, will detect gravitational waves in space using three spacecraft, separated by more than a million miles, flying in a triangular formation. Lasers fired between the satellites, shown in this artist’s concept, will measure how gravitational waves alter their relative distances.
AEI/MM/Exozet

NASA's Request for Information

The RFI, "Concepts for the NASA Gravitational Wave Mission," was released in the NASA NSPIRES Web site on 27 September 2011, as solicitation number NNH11ZDA019L. Responses were due by 20 November 2011. The full text of this NASA research opportunity is posted on the NASA NSPIRES web site.

JPL Team X for Gravitational Wave Mission Study

Study Summaries

TitleDatesPresentation
Team X Study of the SGO-Mid and SGO-High Options 5-8 March 2012[PDF]
Team X Study of the LAGRANGE Mission20-22 March 2012[PDF]
Team X Study of the OMEGA Mission 26-28 March / 3-5 April 2012[PDF]

Final Study Reports

TitleDatesPresentation
Team X SGO-Mid and SGO-High Study Report 6 September 2012[PDF]
Team X LAGRANGE Study Report6 September 2012[PDF]
Team X OMEGA Study Report 6 September 2012[PDF]

Community Science Team

NASA issued a call for Letters of Application for Membership in the Community Science Team (CST) for Gravitational Wave Mission Concepts. The "Dear Colleague" letter can be found HERE. The deadline for responding was 25 October at 4:30pm EST.

Community Science Team Members

NameInstitution
Peter BenderJILA / NIST
Joan CentrellaNASA / GSFC
Neil CornishMontana State University
Jens GundlachUniversity Washington
Ronald HellingsMontana State University
Guido MuellerUniversity of Florida
Holger MuellerU. C. Berkeley
Thomas PrinceCalTech
Rainer WeissMIT (Co-Chair)
Edward WrightUCLA (Co-Chair)

Mission Concepts Submissions in Response to the RFI

TitleSubmitted byPresentation
Instrument Control Unit (ICU) Fritz, Hans[PDF]
Space Communication Rates at Multi-GBPSMcIntyre, Todd[PDF]
A non-drag-free gravitational wave mission architectureFolkner, W.M.[PDF]
A Geostationary Gravitational Wave Interferometer (GEOGRAWI)Tinto, Massimo[PDF]
Interferometer in Space for Detecting Gravity Wave Radiation using Lasers (InSpRL) Saif, Babak N.[PDF]
Interferometer in Space for Detecting Gravity Wave Radiation using Lasers (InSpRL), Updated Dec 9, 2011Saif, Babak N.[PDF]
Simplified optical payload with digital interferometry de Vine, Glenn[PDF]
A Low-Cost, High-Performance Space Gravitational Astronomy Mission Hellings, Ronald[PDF]
Drag-Free Atomic Disturbance Reduction System for LISA-like Gravitational Wave DetectionYu, Nan[PDF]
Concept of Compact Highly-Sensitive Superconducting Antenna for Gravitational Wave RadiationGulian, A.[PDF]
LAGRANGE: LAser GRavitational-wave ANtenna at GEo-lunar L3, L4, L5Conklin, John W.[PDF]
New Sciencecraft and Test Mass Concepts for the LISA MissionShao, Michael[PDF]
SGO Low: A LISA-Like Concept for the Space-based Gravitational-wave Observatory (SGO) at a Low Price-PointThorpe, J.I.[PDF]
Lowest: A LISA-Like Concept for the Space-based Gravitational-wave Observatory (SGO) at the Lowest Cost-PointBaker, John SGO[PDF]
SGO High: A LISA-Like Concept for the Space-based Gravitational-wave Observatory (SGO) at a High Cost-PointStebbins, Robin[PDF]
SGO Mid: A LISA-Like Concept for the Space-based Gravitational-wave Observatory (SGO) at a Middle Price-PointLivas, Jeff[PDF]
LAGRANGE:A Space-Based Gravitational Wave Detector with Geometric Suppression of Spacecraft NoiseMcKenzie, Kirk[PDF]
Geostationary Antenna for Disturbance-Free Laser Interferometry (GADFLI)McWilliams, Sean T.[PDF]

The 2012 Architecting Studies

NASA's Physics of the Cosmos (PhysCOS) Program initiated two studies to develop mission concepts that could meet some or all of the objectives outlined in the New Worlds, New Horizons decadal report for the areas of X-ray astronomy and gravitational-wave science. The PhysCOS Program worked with these communities to define mission concepts that achieve these science objectives at multiple price points.

This began with the release of a formal Request for Information (RFI) on each topic. In parallel, NASA released an open solicitation inviting members of the science community to participate in a Community Science Team (CST) for the X-ray mission or the gravitational-wave mission. The Program Office worked with each CST to review the RFI responses. In December 2012, workshops, which were open to the community, were held to discuss the RFI responses and define the mission concepts to be studied.

A PhysCOS Program study team, working with each CST, identified the requirements relevant to each concept, defined the mission configuration options, executed mission design runs at mission design laboratories, refined the mission concepts, and drafted a mission concept study reports.

News Straight to Your Inbox

Subscribe to your community email news list

We will never share your email address.

Sign Up