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The James Webb Space Telescope • Physics Seminar

June 12 @ 12:00 pm - 1:00 pm

The James Webb Space Telescope: Characteristics, Instruments, Main Missions, and Dusty Galaxies

Dr. Gerardo Vazquez (Salisbury University Physics Department) discusses the James Webb Space Teloscope (JWST), successor of the Hubble Space Telescope, its characteristics, instruments, main missions, dusty galaxies, and his research on active galaxies.  All are welcome (especially students).  Refreshments will be available in the Dana Lobby starting at 11:45 am.

Dr. Vazquez received his B.S. in Physics from Benemerita Universidad Autónoma de Puebla, his M.S. in Astrophysics from the Instituto Nacional de Astrofísica, Optica y Electrónica, and his Ph.D. in Astrophysics from the Instituto de Astronomía, UNAM. Dr. Vazquez is currently a Senior Lecturer of Physics at Salisbury University.

Abstract:  One of the most successful missions from NASA has been the Hubble Space Telescope (HST).  Since Hubble’s launch in 1990, its scientific achievements and longevity have exceeded expectations with the telescope having made over 1.3 million observations and is still in operation after the last servicing mission in 2009.  The successor of HST, the James Webb Space Telescope (JWST) was to be launched in 2007 and is now expected to be deployed in early 2021.  In this talk, the main characteristics of the JWST are reviewed and compared to the HST.  The main missions of the JWST will be explained, emphasizing why this telescope, with its 6.5-meter beryllium mirror, has been designed to observe mainly in the infrared region of the electromagnetic spectrum.  We will also give a broad overview of the instruments on board the JWST and how they are responsible for the success of the mission.  One of the main instruments, the Near Infrared Camera (NIRCAM), will be explained in detail to help understand how it will detect light from the earliest stars and galaxies in the process of formation.  The JWST will also aide our ongoing research project on active galaxies.  This project will utilize observations of Dusty Star Forming Galaxies (DSFG) by the JWST to characterize DSFG star formation at the early ages of the universe. This work will also inform our understanding of galaxy evolution, including the dynamical process of merging and galaxy collisions that occurred early in the universe.

Details

Date:
June 12
Time:
12:00 pm - 1:00 pm

Organizer

Mario Belloni
Email:
mabelloni@davidson.edu

Venue

Dana 146