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A group of astronomers from The University of Texas at Austin has found that a telescope idea shelved by NASA a decade ago can solve a problem that no other telescope can: It would be able to study the first stars in the universe. The team, led by NASA Hubble Fellow Anna Schauer, will publish their results in an upcoming issue of The Astrophysical Journal.

​The GMTO Corporation has received a $17.5 million grant from the National Science Foundation (NSF) to accelerate the prototyping and testing of some of the most powerful optical and infrared technologies ever engineered. These crucial advancements for the Giant Magellan Telescope (GMT), of which The University of Texas at Austin is a founding partner, will allow astronomers to see farther into space with more detail than any other optical telescope before.

An international team of astronomers has used NASA's Transiting Exoplanet Survey Satellite (TESS) and retired Spitzer Space Telescope to discover what may be the first intact planet found closely orbiting a white dwarf, the dense leftover of a sun-like star only 40% larger than Earth. The work, led by Andrew Vanderburg of The University of Texas at Austin, included follow-up observations with the 10-meter Hobby-Eberly Telescope at the university's McDonald Observatory.

The University of Texas at Austin's McDonald Observatory is planning to reopen to the public, in a limited fashion, on Friday, Aug. 28. Beginning with a star party that night, the observatory's Frank N. Bash Visitors Center will begin holding public programs again.

A team of astronomers including McDonald Observatory's Bill Cochran have made a detailed study of a young planet slightly smaller than Neptune with the Habitable-zone Planet Finder at The University of Texas at Austin's McDonald Observatory. They characterized the planet's mass, radius, and the tilt of its orbit. This work provides insight into how such planets form and evolve, and has been accepted for publication in the Astronomical Journal.

An international team of astronomers including Stella Offner of The University of Texas at Austin has proposed a new method for the formation of aluminum-26 in star systems that are forming planets. Because its radioactive decay is thought to provide a heat source for the building blocks of planets, called planetesimals, it's important for astronomers to know where aluminum-26 comes from. Their research is published in the current issue of The Astrophysical Journal.

Jupiter-size planets orbiting close to their stars have upended ideas about how giant planets form. Finding young members of this planet class could help answer key questions. For most of human history our understanding of how planets form and evolve was based on the eight (or nine) planets in our solar system. But over the last 25 years, the discovery of more than 4,000 exoplanets, or planets outside our solar system, changed all that.

Fritz Benedict has used data he took over two decades ago with Hubble Space Telescope to confirm the existence of another planet around the Sun's nearest neighbor, Proxima Centauri, and to pin down the planet's orbit and mass. Benedict, an emeritus Senior Research Scientist with McDonald Observatory at The University of Texas at Austin, will present his findings today in a scientific session and then in a press conference at a meeting of the American Astronomical Society.

​Scientists from across The University of Texas at Austin are joining forces in the hunt for life on other planets. Astronomers, geoscientists, chemists, biologists and aerospace engineers have pooled resources to form the UT Center for Planetary Systems Habitability, a cross-campus, interdisciplinary research unit.

A team of transatlantic scientists led by The University of Texas at Austin's Andrew Vanderburg has used reanalyzed data from NASA's Kepler space telescope to discover an Earth-size exoplanet orbiting in its star's habitable zone, the area around a star where a rocky planet could support liquid water.