About: Shari


Recent Posts by Shari

Jul 2

George Blumenthal

University of California, Santa Cruz George Blumenthal is Chancellor Emeritus and Professor Emeritus of Astronomy and Astrophysics at the University of California, Santa Cruz. His Ph.D. degree is from UC San Diego, and his research interests include theoretical cosmology, the theory of cold dark matter, and active galactic nuclei. He was the chair of the […]

Jun 26

Raja GuhaThakurta

University of California Santa Cruz Raja GuhaThakurta is a Distinguished Professor of Astronomy and Astrophysics at the University of California Santa Cruz, He received his Ph.D. from Princeton University, completed postdoctoral stints at the Institute for Advanced Study and Princeton University, and was an Assistant Astronomer at Space Telescope Science Institute, before joining the UCSC […]

Jun 26

Kathie Olsen

KLO International Dr. Olsen earned her Ph.D. in Neuroscience at UC-Irvine and did Postdoctoral research at Harvard-Children’s Hospital before becoming an Asst. Professor at SUNY-Stony Brook. She served over 20 years in the federal government in variety scientific leadership positions beginning as program officer at NSF, and then moved to a Senator’s Office who was a member of the […]

Jun 26

 Timothy M. Heckman 

Johns Hopkins University Timothy M. Heckman is the Dr. A. Hermann Pfund Professor in the William H. Miller III Department of Physics & Astronomy at Johns Hopkins University. He was the department Chair from 2015 to 2022. Heckman has served as a member of the NAS Committee on Astronomy & Astrophysics and the Board on […]

Jun 23

Ever-changing Universe Revealed in First Imagery From NSF–DOE Vera C. Rubin Observatory

The NSF-DOE Vera C. Rubin Observatory, a major new scientific facility jointly funded by the U.S. National Science Foundation and the U.S. Department of Energy’s Office of Science, released its first imagery today at an event in Washington, D.C. The imagery shows cosmic phenomena captured at an unprecedented scale. In just over 10 hours of test observations, NSF-DOE Rubin Observatory has already captured millions of galaxies and Milky Way stars and thousands of asteroids. The imagery is a small preview of Rubin Observatory’s upcoming 10-year scientific mission to explore and understand some of the universe’s biggest mysteries. 

Jun 13

Mark Your Calendars! NSF–DOE Vera C. Rubin Observatory Will Unveil First Look Images on 23 June 2025

We invite you to attend the live stream of NSF–DOE Vera C. Rubin Observatory’s First Look event, taking place on 23 June 2025 at 11:00 a.m. EDT. At this international celebration the Rubin Observatory team will unveil the observatory’s first spectacular images. The event will be live streamed via YouTube in English and Spanish. Links to the live streams will be made available on rubinobservatory.org.

Apr 24

Largest Imaging Spectro-Polarimeter Achieves First Light at the NSF Daniel K. Inouye Solar Telescope

The U.S. National Science Foundation Daniel K. Inouye Solar Telescope, the world’s most powerful solar telescope, operated by the NSF National Solar Observatory (NSO) near the summit of Maui’s Haleakalā, reached a major milestone: achieving first light with its most advanced instrument, the new Visible Tunable Filter (VTF). The solar image it produced shows early promise to the instrument’s scientific capabilities. Designed and built by the Institut für Sonnenphysik (KIS) in Freiburg, Germany, the VTF is the world’s largest imaging spectro-polarimeter, emerging as a centerpiece to the Inouye’s instrument suite.

Apr 16

NSF NOIRLab Astronomer Discovers Oldest Known Spiral Galaxy in the Universe

An international team led by NSF NOIRLab astronomer Christina Williams has discovered the most distant spiral galaxy known to date. Named Zhúlóng, meaning ‘Torch Dragon’ in Chinese mythology, this ultra-massive system existed just one billion years after the Big Bang, and yet it shows a surprisingly mature structure. Zhúlóng was discovered as part of the PANORAMIC Survey conducted on the James Webb Space Telescope.

Apr 14

With NASA’s Webb, Dying Star’s Energetic Display Comes Into Full Focus

Gas and dust ejected by a dying star at the heart of NGC 1514 came into complete focus thanks to mid-infrared data from NASA’s James Webb Space Telescope. Its rings, which are only detected in infrared light, now look like “fuzzy” clumps arranged in tangled patterns, and a network of clearer holes close to the central stars shows where faster material punched through.

Apr 8

Gemini South Observes Shape and Origin of Near-Earth Asteroid 2024 YR4

Using observations from the Gemini South telescope in Chile, one half of the International Gemini Observatory, partly funded by the U.S. National Science Foundation and operated by NSF NOIRLab, astronomers have constructed a 3D representation of the newly discovered near-Earth asteroid 2024 YR4. The team determined that the unusually-shaped rock is one of the largest objects in recent history that could impact the Moon, and that it likely originated from the main asteroid belt.

Mar 31

20-Year Hubble Study of Uranus Yields New Atmospheric Insights

The ice-giant planet Uranus, which travels around the Sun tipped on its side, is a weird and mysterious world. Now, in an unprecedented study spanning two decades, researchers using NASA’s Hubble Space Telescope have uncovered new insights into the planet’s atmospheric composition and dynamics. This was possible only because of Hubble’s sharp resolution, spectral capabilities, and longevity. 

Mar 26

NASA’s Webb Captures Neptune’s Auroras For First Time

For the first time, NASA’s James Webb Space Telescope has captured bright auroral activity on Neptune. Auroras occur when energetic particles, often originating from the Sun, become trapped in a planet’s magnetic field and eventually strike the upper atmosphere. The energy released during these collisions creates the signature glow. 

Mar 19

Tantalizing Hints That Dark Energy is Evolving — New Results and Data Released by the DESI Project

The DESI collaboration has published a new analysis of dark energy using their first three years of collected data, which spans nearly 15 million galaxies and quasars. Combined with studies of the cosmic microwave background, supernovae, and weak lensing, the analysis hints that dark energy changes over time. Data Release 1, containing data from DESI’s survey validation and first year of observations, has now been made available for scientists and the public to explore.


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