The American Association for the Advancement of Science—the organization that publishes the journal Science and holds the world's largest multidisciplinary scientific conference—is coming to Austin. The 2018 AAAS Annual Meeting offers many ways for the Texas Science community to get involved.
With the discovery of an eighth planet, the Kepler-90 system is the first to tie with our solar system in number of planets. (Click to expand) Credit: NASA/Ames Research Center/Wendy Stenzel.
The discovery of an eighth planet circling the distant star Kepler-90 by University of Texas at Austin astronomer Andrew Vanderburg and Google's Christopher Shallue overturns our solar system's status as having the highest number of known planets. We're now in a tie.
A new tool uses artificial intelligence to recognize objects from City of Austin raw traffic camera footage and characterize how those objects move and interact. Image by Texas Advanced Computing Center/Center for Transportation Research
Look above the traffic light at a busy intersection in your city and you will probably see a camera. These devices may have been installed to monitor traffic conditions and provide visuals in the case of a collision. But can they do more? Can they help planners optimize traffic flow or identify sites that are most likely to have accidents? And can they do so without requiring individuals to slog through hours of footage?
Social group membership is the most important factor influencing the composition of a lemur's gut microbiome, according to research at The University of Texas at Austin.
A full-sized model of the James Webb Space Telescope is seen in Austin during the South by Southwest festival in 2013.
NASA's James Webb Space Telescope, the powerful successor to the Hubble Space Telescope, is expected to launch in 2019 after decades of development. Now the agency has announced the scientists who will use the $8 billion telescope first, testing its instruments to prove it's in good working order. Steven Finkelstein, an associate professor of astronomy at The University of Texas at Austin, leads one of the chosen Early Release Science projects as principal investigator.
Students from the Division of Textiles and Apparel head to New York City as part of an experiential learning program that takes discovery from the classroom to the Big Apple.
UT in NYC, a program designed to bring students together for an integrated look at the fashion industry with an entrepreneurial focus, is unparalleled, partnering with world-renowned fashion icon, entrepreneur and visiting professor Iris Apfel.
Alumna Lynne Chantranupong was named as one of the inaugural Howard Hughes Medical Institute (HHMI) 2017 Hanna H. Gray Fellows.
UT Austin alumna Lynne Chantranupong —currently a postdoctoral research fellow in neurobiology at Harvard Medical School—was named as one of the inaugural Howard Hughes Medical Institute (HHMI) 2017 Hanna H. Gray Fellows. HHMI is an early-career science award providing up to $1.4 million in financial support, mentoring, and active involvement within the HHMI community during early postdoctoral training through several years of a tenure-track faculty position.
The GMT mirror 5 mold filled with 17,500 kg of low expansion glass, ready for the lid of the furnace to be placed. (Credit: University of Arizona)
Today, The University of Texas at Austin and its partners in the Giant Magellan Telescope Organization (GMTO) are beginning to cast the fifth of seven mirrors that will form the heart of the Giant Magellan Telescope (GMT). The mirror is being cast at The University of Arizona's Richard F. Caris Mirror Laboratory, a facility known for creating the world's largest mirrors for astronomy. The 25-meter diameter GMT will be located in the Chilean Andes and will study planets around other stars and to look back to the time when the first galaxies formed.
Rylee Ross, second from left, poses with other members of the White Dwarf Stars research stream in front of the 2.1m Otto Struve Telescope at the McDonald Observatory. Students used the telescope to make time series measurements of pulsating white dwarf stars.
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