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Research Campaign: Lunar Gravitational-wave AntennaThe Lunar Gravitational-wave Antenna (LGWA) is a mission conceived as a network of stations to measure the vibrations of the Moon caused by gravitational waves (GWs). The long-term vision is to accomplish ground-breaking, paradigm shifting science in the coming decades on the Moon. LGWA will lead to the first observation of GW signals in the decihertz band greatly expanding our understanding of the universe and laying out a path to eventually probe the moment of its creation. LGWA stations will also be unique contributions to a lunar geophysical network shedding light on the Moon’s formation history. LGWA is a project of inclusion and international collaboration, where space-faring and space-aspiring nations can contribute to the LGWA network with their own stations whose cost depends on the targeted station lifetime and deployment location. With respect to the baseline concept proposed here, different sensor technologies can be implemented over time with the goal to continually increase the performance of the LGWA network. The broader context of lunar GW detection and its long-term vision are outlined in an accompanying topical white paper.
Document ID
20210026530
Acquisition Source
Goddard Space Flight Center
Document Type
White Paper
Authors
Lorella Angelini
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Francesca Badaracco
(Université Catholique de Louvain Louvain-la-Neuve, Belgium)
Stefano Benetti
(Osservatorio Astronomico di Padova Padova, Italy)
Alessandro Bertolini
(National Institute for Subatomic Physics Amsterdam, Netherlands)
Stefano Benetti
(Osservatorio Astronomico di Padova Padova, Italy)
Xing Bian
(Chinese Academy of Sciences Beijing, Beijing, China)
Alessandro Bonforte
(National Institute of Geophysics and Volcanology Rome, Italy)
Enrico Bozzo
(University of Geneva Geneva, Switzerland)
Marcel ter Brake
(University of Twente Enschede, Overijssel, Netherlands)
Marica Branchesi
(Gran Sasso Science Institute L’Aquila, Italy)
Enrico Cappellaro
(Osservatorio Astronomico di Padova Padova, Italy)
Christophe Collette
(Universite de Liege)
Michael Coughlin
(University of Minnesota Minneapolis, Minnesota, United States)
Stefano Covino ORCID
(Brera Astronomical Observatory Milan, Italy)
Roberto Della Ceca
(Brera Astronomical Observatory Milan, Italy)
Riccardo De Salvo
(Riclab LLC)
Gianluca Di Rico
(Collurania Teramo Observatory Teramo, Italy)
Alessandro Frigeri
(Istituto di Astrofisica e Planetologia Spaziali Roma, Italy)
Carlo Giunchi
(National Institute of Geophysics and Volcanology Rome, Italy)
Joris van Heijningen
(Université Catholique de Louvain Louvain-la-Neuve, Belgium)
Vuk Mandic
(University of Minnesota Minneapolis, Minnesota, United States)
Szabolcs Marka
(Columbia University New York, New York, United States)
Andrea Maselli
(Osservatorio Astronomico di Padova Padova, Italy)
Daniele Melini
(National Institute of Geophysics and Volcanology Rome, Italy)
Ana Carolina Silva Oliveira
(Columbia University New York, New York, United States)
Marco Olivieri
(National Institute of Geophysics and Volcanology Rome, Italy)
Andrea Perali
(University of Camerino Camerino, Marche, Italy)
Roberto Serafinelli
(Istituto di Astrofisica e Planetologia Spaziali Roma, Italy)
Paola Severgnini
(Brera Astronomical Observatory Milan, Italy)
Date Acquired
January 7, 2022
Publication Date
January 31, 2022
Subject Category
Communications And Radar
Funding Number(s)
WBS: 070146.02.07.02.11
CONTRACT_GRANT: SPEC5732
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
External Peer Committee
No Preview Available