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NASA Participation in ESA-Led L3 Gravitational Wave Mission

The L3 Study was active from 2016 to 2018

NASA intends to partner with ESA on the third Large-Class mission (L3) in ESA's Cosmic Vision 2015-2025 Programme, planned for launch in 2034. ESA has selected a gravitational wave observatory as the science theme. 

About the NASA L3 Study

Detecting and Measuring Gravitational Waves in Space

ESA has selected a gravitational wave observatory as the science theme for the third Large-Class mission (L3) in ESA's Cosmic Vision 2015-2025 Programme.

To this end, NASA has formed an L3 Study Team (L3ST) composed of selected members of the community. A Dear Colleague Letter was issued on December 7, 2015, soliciting nominations and self-nominations for the L3ST, with due date December 21, 2015. Submitted applications were reviewed by members of the NASA HQ Astrophysics Division and of the PCOS Program office, who then made selection recommendations.

US LISA Project about Detecting and Measuring Gravitational Waves in Space
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

The purpose of the "L3 Study" is to understand how NASA might participate in ESA's L3 Gravitational Wave mission, to inform our engagement through its earliest stages and to prepare for the 2020 decadal survey.

The L3 Study Team (L3ST)

NameInstitution
Baker, JohnNASA Goddard Space Flight Center
Bender, PeterUniversity of Colorado at Boulder
Berti, EmanueleUniversity of Mississippi
Conklin, JohnUniversity of Florida
Cornish, Neil
Montana State University
Cutler, CurtJet Propulsion Laboratory
Holley-Bockelman, KellyVanderbilt University
Larson, ShaneNorthwestern University
McWilliams, SeanWest Virginia University
Miller, ColeUniversity of Maryland
Robertson, NornaCalifornia Institute of Technology
Shoemaker, David (Chair)Massachusetts Institute of Technology
Vallisneri, MicheleJet Propulsion Laboratory
Note: Ex-Officio NASA members of the L3ST: R. Sambruna, A. Hornschemeier, and I. Thorpe. In addition, A. Parmar has been appointed by ESA as an observer on the L3ST.

The Technology Analysis Group

The L3ST is assisted by a Technology Analysis Group (TAG) who provide expert knowledge of the technology associated with NASA's possible hardware contributions to ESA.

NameInstitution
Camp, JordanNASA Goddard Space Flight Center
Klipstein, WilliamJet Propulsion Laboratory
Livas, JeffreyNASA Goddard Space Flight Center
McKenzie, KirkJet Propulsion Laboratory
Mueller, GuidoUniversity of Florida
Ziemer, JohnJet Propulsion Laboratory

Technology Presentations

TitlePresenterPresentation
Mission Architecture OverviewIra Thorpe[PDF]
Colloid Micro-Newton Thrusters for the Space Technology 7 Mission and BeyondJohn Ziemer[PDF]
Telescope Design for a Space-based Gravitational Wave MissionJeffrey Livas[PDF]
Phasemeter Development for LISA at JPLWilliam Klipstein[PDF]
eLISA Laser Development in the US Jordan Camp[PDF]

L3 Study Team (L3ST) Events

Meetings, Conferences, Seminars, Workshops and other events.

Chandra/Hubble/Spitzer X-ray/Visible/Infrared Image of M82

14 – 17 April 2018

Fifth Meeting (Tentative) at APS April Meeting 2018

NASA scientists used supercomputers to solve Einstein’s equations for a merging black hole binary to predict the precise gravitational wave output.

9 – 14 July 2017

Fourth Meeting at Edoardo Amaldi Conference on Gravitational Waves

A bright white point of light is surrounded by ten to fifteen regularly spaced, hazy rings at its bottom, right, and upper right. The central point, where the stars are located, has a rough hexagon shape. The innermost ring is highlighted blueish white and is much brighter to the right. The outer rings fade from view to the upper left, with only a few close rings visible there. The central light seems to highlight the misshapen rings like a spotlight, with rays coming out diagonally from the upper left to lower right. One ray illuminates even more rings as it travels to the upper right.

28 – 31 January 2017

Third Meeting at APS April Meeting 2017

Simulated LISA sky

4 – 9 September 2016

Second Meeting at 11th International LISA Symposium

Hubble Sees a Horsehead of a Different Color

16 – 19 April 2016

First Meeting at APS April Meeting 2016

Telecon Schedule

The GW community holds a regular weekly telecon on Mondays at 11:00 AM Eastern. Other telecons are scheduled as needed. For telecon connection information, please contact both PCOS Chief Scientist Ann Hornschemeier and Deputy PCOS Chief Scientist Terri Brandt.

Documents

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