JPL Home NASA Home Caltech Home
Follow this link to skip to the main content
NASA Logo - Jet Propulsion Laboratory
JPL Home Earth Solar System Stars & Galaxies Technology
Science Visitor and Colloquium Program
SVCP Home
Meetings
Information for Visiting Speakers
Contact
Restricted
 
Astrophysics Colloquium

The Laser Interferometer Space Antenna: Observing mHz Gravitational Waves from Space
Presented by John Conklin
University of Florida

Thursday, July 18, 2019
11:00 A.M. in 169-336

Abstract
Gravitational wave detection is one of the most compelling problems in science today. It represents an entirely new way of observing our universe and therefore provides enormous potential for scientific discovery. The first direct detection in 2016 by the ground-based LIGO observatory has already brought new insights into the population of black holes and the evolution of our Universe.

The Laser Interferometer Space Antenna (LISA), a joint venture between NASA and the European Space Agency, will be the first mission to detect and observe low-frequency gravitational waves from space, complementing observatories on the ground. LISA will be the largest instrument ever constructed, consisting of three Sun-orbiting spacecraft that form an equilateral triangle, with each side measuring 2.5 million kilometers in length. Each spacecraft houses two free-floating test masses (TM), which are protected from all disturbing forces so that they follow pure geodesics in spacetime. A "drag-free" control system is supplied with measurements of the TM position and commands external micronewton thrusters to force the spacecraft to fly in formation with the test masses. Laser interferometry is used to measure the minute variations in the distance, or light-travel time, between these purely free-falling TMs, caused by gravitational waves. LISA represents the ultimate engineering challenge in precision ranging between spacecraft and precision accelerometry. Variations in the distance between test masses, spaced millions of km apart, must be measured to 1011 m/Hz1/2, and the test masses must experience free fall at a level below 31016 g/Hz1/2. This talk will present the LISA project and the key contributions made by the University of Florida Precision Space Systems Lab to realize this ground-breaking mission.

JPL Contact: Graca Rocha (3-0095)

About the Speaker
John Conklin a University Term Professor in Mechanical and Aerospace Engineering at the University of Florida (UF). He joined the UF faculty in 2012 after a three-year research associateship at the W.W. Hansen Experimental Physics Laboratory at Stanford. He received his BS and MEng degrees from Cornell and PhD from Stanford in 2009. In 2011, John was the Fulbright Junior Lecturer at the University of Trento in Italy. He is the chair of NASA's Physics of the Cosmos Program Analysis Group and a member of NASA's Astrophysics Advisory Committee. He has led the Technology Working Group for NASA's Gravitational Wave L3 Study Team. John has been awarded the NASA Group Achievement Award (2005) for the Gravity Probe B science team, the Balhaus Prize (2009) for best PhD thesis in Aeronautics and Astronautics at Stanford, the Zeldovich Medal (2010) from COSPAR and the Russian Academy of Sciences, the NASA Early Career Faculty Award (2014), NASA's Nancy Grace Roman Technology Fellowship in Space Astrophysics for Early Career Researchers (2015), Teacher of the Year Award (2015) in Mechanical and Aerospace Engineering at UF, and the Space Science Award from AIAA (2016) for the Gravity Probe B science team.


SVCP Astrophysics


Privacy / Copyrights
  NASA Home Page
Site Manager:
Webmaster:

CL 08-3220