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                    <title>University of Texas McDonald Observatory in the news</title>
            <link>https://phys.org/</link>
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            <description>Latest news from University of Texas McDonald Observatory</description>

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                    <title>Chemical cartography reveals the Milky Way&#039;s spiral arms</title>
                    <description>Keith Hawkins, assistant professor of astronomy at The University of Texas at Austin, has used chemical cartography—also known as chemical mapping—to identify regions of the Milky Way&#039;s spiral arms that have previously gone undetected. His research, published in the Monthly Notices of the Royal Astronomical Society, demonstrates the value of this pioneering technique in understanding the shape, structure, and evolution of our home Galaxy.</description>
                    <link>https://phys.org/news/2023-07-chemical-cartography-reveals-milky-spiral.html</link>
                    <category>Astronomy</category>                    <pubDate>Wed, 19 Jul 2023 17:17:04 EDT</pubDate>
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                    <title>Astronomers observe giant tails of helium escaping Jupiter-like planet</title>
                    <description>A team of astronomers has used observations from the Hobby-Eberly Telescope (HET) at The University of Texas at Austin&#039;s McDonald Observatory to discover some of the longest tails of gas yet observed escaping a planet.</description>
                    <link>https://phys.org/news/2023-06-astronomers-giant-tails-helium-jupiter-like.html</link>
                    <category>Astronomy</category>                    <pubDate>Wed, 07 Jun 2023 17:29:03 EDT</pubDate>
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                    <title>Texas astronomers revive idea for &#039;Ultimately Large Telescope&#039; on the moon</title>
                    <description>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.</description>
                    <link>https://phys.org/news/2020-11-texas-astronomers-revive-idea-ultimately.html</link>
                    <category>Astronomy</category>                    <pubDate>Mon, 16 Nov 2020 15:42:44 EST</pubDate>
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                    <title>New tricks from old data: Astronomer uses 25-year-old Hubble data to confirm planet Proxima Centauri c</title>
                    <description>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&#039;s nearest neighbor, Proxima Centauri, and to pin down the planet&#039;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.</description>
                    <link>https://phys.org/news/2020-06-astronomer-year-old-hubble-planet-proxima.html</link>
                    <category>Astronomy</category>                    <pubDate>Tue, 02 Jun 2020 16:28:54 EDT</pubDate>
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                    <title>Magnetic waves create chaos in star-forming clouds</title>
                    <description>New research by Stella Offner, assistant professor of astronomy at The University of Texas at Austin, finds that magnetic waves are an important factor driving the process of star formation within the enormous clouds that birth stars. Her research sheds light on the processes that are responsible for setting the properties of stars, which in turn affects the formation of planets orbiting them, and, ultimately, life on those planets. The research is published in the current issue of the journal Nature Astronomy.</description>
                    <link>https://phys.org/news/2018-09-magnetic-chaos-star-forming-clouds.html</link>
                    <category>Astronomy</category>                    <pubDate>Thu, 13 Sep 2018 08:34:29 EDT</pubDate>
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                    <title>Discovery of new planet reveals distant solar system to rival our own</title>
                    <description>The discovery of an eighth planet circling the distant star Kepler-90 by University of Texas at Austin astronomer Andrew Vanderburg and Google&#039;s Christopher Shallue overturns our solar system&#039;s status as having the highest number of known planets. We&#039;re now in a tie.</description>
                    <link>https://phys.org/news/2017-12-discovery-planet-reveals-distant-solar.html</link>
                    <category>Astronomy</category>                    <pubDate>Thu, 14 Dec 2017 13:35:07 EST</pubDate>
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                    <title>High school student helps discover new planet, calculates frequency of Jupiter-like planets</title>
                    <description>High school senior Dominick Rowan of Armonk, New York, is making discoveries about other worlds. Working with University of Texas at Austin astronomer Stefano Meschiari, Rowan has helped to find a Jupiter-like planet and has calculated that this type of planet is relatively rare, occurring in three percent of stars overall. Their research is has been accepted for publication in the Astrophysical Journal.</description>
                    <link>https://phys.org/news/2015-12-high-school-student-planet-frequency.html</link>
                    <category>Astronomy</category>                    <pubDate>Thu, 10 Dec 2015 06:26:05 EST</pubDate>
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                    <title>Astronomers solve mystery of &#039;born again&#039; stars with Hubble Space Telescope</title>
                    <description>University of Texas astronomer Natalie Gosnell has used Hubble Space Telescope to better understand why some stars aren&#039;t evolving as predicted. These so-called &quot;blue stragglers&quot; look hotter and bluer than they should for their advanced age. It&#039;s almost as it they were somehow reinvigorated to look much younger than they really are.</description>
                    <link>https://phys.org/news/2015-12-astronomers-mystery-born-stars-hubble.html</link>
                    <category>Astronomy</category>                    <pubDate>Tue, 08 Dec 2015 05:26:50 EST</pubDate>
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                    <title>Upgraded Hobby-Eberly Telescope sees first light</title>
                    <description>After several years and a massive team effort, one of the world&#039;s largest telescopes has opened its giant eye again. The Hobby-Eberly Telescope (HET) at The University of Texas at Austin&#039;s McDonald Observatory has completed a $25 million upgrade and, now using more of its primary mirror, has achieved &quot;first light&quot; as the world&#039;s third-largest optical telescope.</description>
                    <link>https://phys.org/news/2015-11-hobby-eberly-telescope.html</link>
                    <category>Space Exploration</category>                    <pubDate>Wed, 04 Nov 2015 06:02:42 EST</pubDate>
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                    <title>Globular clusters rotate at heart</title>
                    <description>(Phys.org) —Astronomers from the University of Texas at Austin and Germany&#039;s Max Planck Institute for Extraterrestrial Physics (MPE) recently found a surprise when studying some of the oldest star clusters in our galaxy. The stars at the centers of these clusters are rotating around a common axis. It was previously thought any central rotation would have been long erased, leaving the central stars to random orbits. The work has been accepted for publication in the Astrophysical Journal Letters.</description>
                    <link>https://phys.org/news/2014-05-globular-clusters-rotate-heart.html</link>
                    <category>Astronomy</category>                    <pubDate>Fri, 09 May 2014 13:11:28 EDT</pubDate>
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                    <title>Astronomers discover pulsations in crystalized, dying star</title>
                    <description>(Phys.org) —Astronomers from The University of Texas at Austin and colleagues have used the 2.1-meter Otto Struve Telescope at the university&#039;s McDonald Observatory to discover pulsations from the crystalized remnant of a burnt-out star. The finding will allow astronomers to see below the star&#039;s atmosphere and into its interior, much like earthquakes allow geologists to study compositions below Earth&#039;s surface. The findings appear in the current issue of The Astrophysical Journal Letters.</description>
                    <link>https://phys.org/news/2013-06-astronomers-pulsations-crystalized-dying-star.html</link>
                    <category>Astronomy</category>                    <pubDate>Thu, 20 Jun 2013 10:18:01 EDT</pubDate>
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                    <title>Orionid meteor shower peaks Oct. 20-21, 2012</title>
                    <description>As it does each year, early fall brings crisper air, turning leaves, and the Orionid meteor shower. This year&#039;s best viewing will be in the several hours around midnight October 20 and before dawn on October 21, according to the editors of StarDate magazine.</description>
                    <link>https://phys.org/news/2012-10-orionid-meteor-shower-peaks-oct.html</link>
                    <category>Space Exploration</category>                    <pubDate>Thu, 18 Oct 2012 11:48:15 EDT</pubDate>
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                    <title>Astronomers measure largest-ever magnetic field around massive star</title>
                    <description>(Phys.org)—A group of astronomers led by Gregg Wade of the Royal Military College of Canada have used the Hobby-Eberly Telescope (HET) at The University of Texas at Austin&#039;s McDonald Observatory and the Canada-France Hawaii Telescope (CFHT) on Hawaii&#039;s Mauna Kea to measure the most magnetic massive star yet. Their work is published in today&#039;s issue of the research journal Monthly Notices of the Royal Astronomical Society. </description>
                    <link>https://phys.org/news/2012-09-astronomers-largest-ever-magnetic-field-massive.html</link>
                    <category>Astronomy</category>                    <pubDate>Tue, 11 Sep 2012 15:07:09 EDT</pubDate>
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