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LISA Telescope Development Status and Flight DesignThe study of the universe through gravitational waves will yield a revolutionary new perspective on the universe, which has been intensely studied using electromagnetic waves in many wavelength bands. A space based gravitational wave observatory will enable access to a rich array of astrophysical sources in the measurement band from 0.1 to 100 mHz. A space based mission complements ground based gravitational wave observatories, which typically search for signals at higher frequencies. LISA is a space based gravitational wave mission. Telescopes are one of the technology contributions from NASA to the European Space Agency (ESA) for the Laser Interferometer Space Antenna (LISA) Mission. We will describe the key requirements and interfaces for the flight telescopes. We will also discuss the expected schedule for the Mission and delivery of the telescopes and summarize the current status of the technology development effort.
Document ID
20230016663
Acquisition Source
Goddard Space Flight Center
Document Type
Presentation
Authors
Ritva Keski-kuha
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Ryan T Derosa
(Goddard Space Flight Center Greenbelt, Maryland, United States)
Date Acquired
November 15, 2023
Subject Category
Optics
Meeting Information
Meeting: SPIE Astronomical Telescopes + Instrumentation
Location: Yokohama
Country: JP
Start Date: June 16, 2024
End Date: June 21, 2024
Sponsors: International Society for Optics and Photonics
Funding Number(s)
PROJECT: 244904.04.09.05.05.01
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
Technical Review
Single Expert
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