A small image of a galaxy distorted by gravitational lensing into a dim ring. At the top of the ring are three very bright spots with diffraction spikes coming off them, right next to each other: these are copies of a single quasar in the lensed galaxy, duplicated by the gravitational lens. In the centre of the ring, the elliptical galaxy doing the lensing appears as a small blue dot. The background is black and empty.

The gravitational lensing of the quasar known as RX J1131-1231 is considered one of the best lensed quasars discovered to date. The foreground galaxy smears the image of the background quasar into a bright arc and creates four images of the object. Credit: ESA/Webb, NASA & CSA, A. Nierenberg

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Public: $15
Members, youth, and seniors: $12

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Revealing Dark Matter with Strong Gravitational Lensing
Monday, June 2, 7:30 pm
Morrison Planetarium

Featuring Dr. Anna Nierenberg, UC Merced

The overwhelming majority of matter in our Universe is believed to be an unknown new ‘dark’ particle that exists outside the standard model of physics and does not interact with light. An important goal of modern physics is to understand what this particle is. Dr. Nierenberg will provide an overview of the observational evidence for the existence of dark matter, introduce strong gravitational lensing- where space-time is bent by massive objects- and conclude by explaining how we are using this phenomenon to gain new insights into the nature of dark matter with the James Webb Space Telescope, Hubble Space Telescope, and Keck Observatories.

Headshot of Anna Nierenberg

Anna Nierenberg was born in Sacramento and raised in the Bay Area and San Diego. She received her B.S. in Physics from UCLA and her Ph.D. in Physics from UCSB. After a three-year stint at the University of Ohio as a Postdoctoral Fellow, Dr. Nierenberg was grateful to return to California and is currently a professor in the Physics Department at the University of California, Merced, researching dark matter.

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