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        <title><![CDATA[Universe Today]]></title>
        <description><![CDATA[Space and Astronomy News from Universe Today]]></description>
        <link>https://www.universetoday.com</link>
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        <lastBuildDate>Fri, 26 Jun 2026 07:33:27 +0000</lastBuildDate>
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        <item>
            <title><![CDATA[Euclid's New Portrait of the Milky Way's Crowded Bulge]]></title>
            <link>https://www.universetoday.com/articles/euclids-new-portrait-of-the-milky-ways-crowded-bulge</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/euclids-new-portrait-of-the-milky-ways-crowded-bulge</guid>
            <pubDate>Thu, 25 Jun 2026 23:41:24 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/Euclid_s_view_of_our_galaxy_s_bulge_20260625_190524.jpg" alt="The ESA has released a new image of the Milky Way's central bulge from the Euclid Space Telescope. It's the largest optical light, high-resolution image of the bulge ever taken. There are more than 60 million individual stars in this image, which will be used to help find exoplanets. Image Credit: ESA/Euclid/Euclid Consortium/NASA, CFHT, image processing by J.-C. Cuillandre and E. Bertin (CEA Paris-Saclay)
Licence: CC BY-SA 3.0 IGO or ESA Standard Licence" width="1280" height="720" /></p><p>The ESA's Euclid space telescope took 26 hours to capture this portrait of the Milky Way's central bulge. This isn't part of its primary mission; instead it's kind of like bonus science. It'll be used in the Roman Space Telescope's gravitational microlensing search for exoplanets. Regardless of the science, it's an impressive image.</p>]]></description>
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            <title><![CDATA[The Galaxy That Cleared the Fog]]></title>
            <link>https://www.universetoday.com/articles/hubble-details-early-galaxy-transforming-neighborhood</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/hubble-details-early-galaxy-transforming-neighborhood</guid>
            <pubDate>Thu, 25 Jun 2026 22:51:31 +0000</pubDate>
            <dc:creator><![CDATA[Mark Thompson]]></dc:creator>
            <author>Mark Thompson (https://www.universetoday.com/authors/mark)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/STScI-01KV6GC312KY26Z9KGR2YQH042_20260625_225127.png" alt="MXDFz4.4 has helped a team of astronomers to understand a little more about the evolution of the universe (Credit : NASA)" width="1280" height="720" /></p><p>For its first billion years the universe was lost in fog, a thick haze of hydrogen that swallowed light whole. Something burned it away, and astronomers have long wondered what. Now Hubble has caught a tiny, furious galaxy in the very act of clearing the murk, glimpsed as it was just 1.4 billion years after the big bang. It may be the smoking gun for how the universe first became clear.</p>]]></description>
        </item>
        <item>
            <title><![CDATA[Beyond Fermi's Paradox XVIII: What if We Make Contact?]]></title>
            <link>https://www.universetoday.com/articles/beyond-fermis-paradox-xviii-what-if-we-make-contact</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/beyond-fermis-paradox-xviii-what-if-we-make-contact</guid>
            <pubDate>Thu, 25 Jun 2026 20:01:00 +0000</pubDate>
            <dc:creator><![CDATA[Matthew Williams]]></dc:creator>
            <author>Matthew Williams (https://www.universetoday.com/authors/houseofwilliams)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/potw1217a_20260625_191109.jpg" alt="The Karl G. Jansky Very Large Array (VLA) listening for radio waves from space. Credit: NRAO" width="1280" height="720" /></p><p>Welcome to the final installment in the Fermi series, where we look at the impact that making contact with extraterrestrials could have and the rules governing how such an event should be treated.</p>]]></description>
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        <item>
            <title><![CDATA[Crystalline Clocks Confirm Earth's Oldest Crater]]></title>
            <link>https://www.universetoday.com/articles/crystalline-clocks-confirm-earths-oldest-crater</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/crystalline-clocks-confirm-earths-oldest-crater</guid>
            <pubDate>Thu, 25 Jun 2026 19:35:00 +0000</pubDate>
            <dc:creator><![CDATA[Carolyn Collins Petersen]]></dc:creator>
            <author>Carolyn Collins Petersen (https://www.universetoday.com/authors/cc-petersen)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/NorthPoleDome_feature-image-2_20260625_210003.jpg" alt="Large conical shatter cones within the Pilbara Craton, Western Australia, provide visible proof of a meteorite impact some 3 billion years ago. Credit: Chris Kirkland, Curtin University" width="1280" height="720" /></p><p>A chip of zircon found in Western Australian rocks at a place called North Pole Dome revealed the age of Earth's oldest known impact crater. The team that found it was working on age-dating the crater, which is located in a region called the Pilbara Craton. They used mineral dating to pinpoint the exact time it was dug out by an impactor. Team lead Chris Kirkland from the Timescales of Minerals Systems Group within Curtin University's School of Earth and Planetary Sciences, said the findings help resolve a longstanding question about the timing of the impact. The results of the team's analysis of several minerals at the site, along with zircon, indicated that the North Pole Dome impact occurred at 3.024 billion years ago (plus or minus a few million years).</p>]]></description>
        </item>
        <item>
            <title><![CDATA[Magnetic Fields Channel Gas Through Filaments into Star Formation Sites]]></title>
            <link>https://www.universetoday.com/articles/magnetic-fields-channel-gas-through-filaments-into-star-formation-sites</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/magnetic-fields-channel-gas-through-filaments-into-star-formation-sites</guid>
            <pubDate>Thu, 25 Jun 2026 18:44:39 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/dr21-magnetic-field-lines-00_20260625_154610.jpg" alt="This Spitzer Space Telescope image shows the DR21 star-forming region, a large molecular hydrogen cloud about 6,000 light years away. DR21 forms stars rapidly, and new research shows how magnetic fields funnel gas into the region. The magnetic field lines in this image are from the now-ended SOFIA mission. Image Credit: T. Pillai/SOFIA/NASA and J. Kauffmann/JPL-Caltech/NASA" width="1280" height="720" /></p><p>Stars form inside molecular clouds where cold gas collapses gravitationally on itself. But there's more to this process than gravity. New research shows how magnetic field lines funnel gas through sub-filaments into star formation sites.</p>]]></description>
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        <item>
            <title><![CDATA[The Universe's First Stars Were Shaped By Turbulence and Were Not As Massive as Thought]]></title>
            <link>https://www.universetoday.com/articles/the-universes-first-stars-were-shaped-by-turbulence-and-were-not-as-massive-as-thought</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-universes-first-stars-were-shaped-by-turbulence-and-were-not-as-massive-as-thought</guid>
            <pubDate>Thu, 25 Jun 2026 15:41:28 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/turbulent_minhalos_1_20260624_201938.jpg" alt="These three panels show simulated primordial mini haloes, dense pockets of dark matter where the first stars formed. The new simulations show that turbulence was a greater factor in the formation of the Universe's stars than thought. While these Population III stars were long thought to be uniformly massive, the turbulence in these simulations shows that may not be true. Image Credit: Meng-Yuan Ho et al 2026 ApJ" width="1280" height="720" /></p><p>For a long time, astrophysicists thought that the Universe's first stars, called Population III stars, were uniformly massive. It seemed like the conditions they formed in were calm and serene, which favoured massive stars. But new research based on high-resolution simulations show that conditions were more chaotic than thought, and gas cloud turbulence means that Population III stars were not all massive. This affected the metallicity of the next stars to form.</p>]]></description>
        </item>
        <item>
            <title><![CDATA[A Star Dying by the Wrong Rules]]></title>
            <link>https://www.universetoday.com/articles/a-star-dying-by-the-wrong-rules</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/a-star-dying-by-the-wrong-rules</guid>
            <pubDate>Thu, 25 Jun 2026 06:14:00 +0000</pubDate>
            <dc:creator><![CDATA[Mark Thompson]]></dc:creator>
            <author>Mark Thompson (https://www.universetoday.com/authors/mark)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/Screenshot_2026-06-25_at_07.03.43_20260625_061340.png" alt="Image of KSP-OT-202104a in a quiescent phase image made by stacking 549 x 60s exposures (Credit : Sang Chul Kim et al)" width="1280" height="720" /></p><p>Half the stars in the universe live in pairs and when one of them dies it can feed hungrily off the other in a slow, violent dance. Now a Korean team has caught a couple of stars breaking the rules, locked in an orbit so impossibly fast that our best theories of how stars grow old cannot account for it. So what is this dying star trying to tell us?</p>]]></description>
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            <title><![CDATA[The Galaxy Living Too Fast]]></title>
            <link>https://www.universetoday.com/articles/the-galaxy-living-too-fast</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-galaxy-living-too-fast</guid>
            <pubDate>Thu, 25 Jun 2026 06:00:33 +0000</pubDate>
            <dc:creator><![CDATA[Mark Thompson]]></dc:creator>
            <author>Mark Thompson (https://www.universetoday.com/authors/mark)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/weic2612a_20260625_060015.jpg" alt="The Cigar Galaxy seen here with data from both Hubble and James Webb (Credit : NASA/ESA/CSA)" width="1280" height="720" /></p><p>Twelve million light years away, a galaxy is living fast and burning bright, forging new stars ten times quicker than our own Milky Way in a frenzy that cannot possibly last. Now the James Webb Space Telescope has cut clean through its veil of dust to count an astonishing 16.5 million of its stars, one by one. So what is driving the Cigar Galaxy to burn so furiously?</p>]]></description>
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        <item>
            <title><![CDATA[Astronomers Find Stellar Evidence of an Engulfed Planet]]></title>
            <link>https://www.universetoday.com/articles/astronomers-find-stellar-evidence-of-an-engulfed-planet</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/astronomers-find-stellar-evidence-of-an-engulfed-planet</guid>
            <pubDate>Thu, 25 Jun 2026 00:47:44 +0000</pubDate>
            <dc:creator><![CDATA[Carolyn Collins Petersen]]></dc:creator>
            <author>Carolyn Collins Petersen (https://www.universetoday.com/authors/cc-petersen)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/you-just-ate-that-planet-didnt-you-engulfment_illustration_20260625_004425.png" alt="The path of a planet as it spirals into its star. The result is that the event tears the planet apart and sucks its elements into the star. Image credit: NASA, ESA, CSA, Ralf Crawford (STScI)" width="1280" height="720" /></p><p>A team of 14 researchers from the United States and Chile have found evidence of a subgiant star eating one of its planets. The star, called TOI-5882, was already known to astronomers because of its massive companion, a brown dwarf called TOI-5882 b. The companion may well have helped kick a planet onto a spiraling journey into the star.</p>]]></description>
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        <item>
            <title><![CDATA[That "Pink Planet" Astronomers Found Turns Out to be a Salty Customer!]]></title>
            <link>https://www.universetoday.com/articles/that-pink-planet-astronomers-found-turns-out-to-be-a-salty-customer</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/that-pink-planet-astronomers-found-turns-out-to-be-a-salty-customer</guid>
            <pubDate>Thu, 25 Jun 2026 00:20:43 +0000</pubDate>
            <dc:creator><![CDATA[Matthew Williams]]></dc:creator>
            <author>Matthew Williams (https://www.universetoday.com/authors/houseofwilliams)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/pink-planet1940__FitMaxWzk3MCw2NTBd_20260623_184217.jpg" alt="Discovered in 2013, the Pink Planet orbits a sun-like star located 57 light-years from Earth. Credit: NASA/Goddard Space Flight Center" width="1280" height="720" /></p><p>Found in 2013, Pink Planet was too faint to study with ground-based telescopes. In new study, scientists used JWST and advanced processing methods to obtain its spectrum for the first time. Observations provided some of the first direct evidence for salt clouds in a cold object atmosphere. Pink Planet could be a giant planet or brown dwarf, so astronomers refer to it as a ‘planetary-mass companion’.</p>]]></description>
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            <title><![CDATA[The JWST Spies Six Galaxies Becoming One]]></title>
            <link>https://www.universetoday.com/articles/the-jwst-spies-six-galaxies-becoming-one</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-jwst-spies-six-galaxies-becoming-one</guid>
            <pubDate>Wed, 24 Jun 2026 18:59:28 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/d1180x428_20260624_172018.jpg" alt="These JWST images show the six galaxies in the protocluster, and the SMBH in the dotted orange ellipse. The image on the right also shows fast-moving gas in blue. Image Credit: NASA/ESA/CSA" width="1280" height="720" /></p><p>The JWST looked back in time and saw 6 galaxies merging into one. At the heart of the assembly, a supermassive black hole is lurking. It all happened when the Universe was only about 1.5 billion years old, and the red-shifted light is just reaching us now.</p>]]></description>
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            <title><![CDATA[Finding Organics on Mars Isn't Enough. ExoMars Will Look for Their "Handedness."]]></title>
            <link>https://www.universetoday.com/articles/finding-organics-on-mars-isnt-enough-exomars-will-look-for-their-handedness</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/finding-organics-on-mars-isnt-enough-exomars-will-look-for-their-handedness</guid>
            <pubDate>Wed, 24 Jun 2026 14:05:59 +0000</pubDate>
            <dc:creator><![CDATA[Andy Tomaswick]]></dc:creator>
            <author>Andy Tomaswick (https://www.universetoday.com/authors/andy-tomaswick)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/ExoMars_Rosalind_Franklin_rover_20260623_140305.jpg" alt="Artist's depiction of the Rosalind Franklin rover on Mars. Credit - ESA/ATG medialab" width="1280" height="720" /></p><p>We’ve known for a long time that there are organic molecules on Mars. Rovers and landers keep turning them up wherever they look. But, “organic” simply means a molecule is made up of carbon and hydrogen atoms, not that it was created by life - there are plenty of non-biological processes that can create organic molecules. But there is one feature of organic molecules that can point very strongly in the direction of life or not - its chirality, and a new instrument on the Rosalind Franklin rover, planned for launch to Mars in the 2030s, just proved it can successfully look for it.</p>]]></description>
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            <title><![CDATA[Hot Jupiter Endures Star-Powered Barbecue]]></title>
            <link>https://www.universetoday.com/articles/hot-jupiter-endures-star-powered-barbecue</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/hot-jupiter-endures-star-powered-barbecue</guid>
            <pubDate>Wed, 24 Jun 2026 03:21:00 +0000</pubDate>
            <dc:creator><![CDATA[Laurence Tognetti, MSc]]></dc:creator>
            <author>Laurence Tognetti, MSc (https://www.universetoday.com/authors/laurencetognetti)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/STScI-01KTQRQV4XDP5XZRVJT8KB2MFA_750_20260624_032052.jpg" alt="Artist's illustration of HD 80606 b. (Credit: NASA, ESA, CSA, Joseph Olmsted (STScI))" width="1280" height="720" /></p><p>You’re the grillmaster at the annual family 4th of July BBQ and you’re sweating bullets standing over the grill in the sweltering summer heat. You’re trying to stay cool by pressing a cold beer can on your forehead, but to no avail. You can’t go inside because, once again, you’re the grillmaster and need to watch the food simmering on your freshly cleaned grill. Your brother-in-law is a university astronomy professor and walks over asking how you’re doing. You say, “This heat is killing me. I feel hotter than the barbeque!” Your science teacher brother-in-law slyly says, “Try being an exoplanet.” You roll your eyes.</p>]]></description>
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            <title><![CDATA[The Long-Lived Chicxulub Hydrothermal System Lasted 8 Million Years]]></title>
            <link>https://www.universetoday.com/articles/the-long-lived-chicxulub-hydrothermal-system-lasted-8-million-years</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/the-long-lived-chicxulub-hydrothermal-system-lasted-8-million-years</guid>
            <pubDate>Tue, 23 Jun 2026 22:20:30 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/hydrothermal-system-chicxulub-lpi-usra-hero_20260623_210556.jpg" alt="Scientists have known about the hydrothermal system created by the Chicxulub impact. These types of systems could be where prebiotic chemistry got a boost, leading to the appearance of the first simple life. But for that to happen, the system needed to last for a long time. New research says it lasted 8 million years, much longer than previous estimates. Image Credit: Victor O. Leshyk" width="1280" height="720" /></p><p>The asteroid that caused the extinction of the dinosaurs also created an underground environment suited to supporting new life, and new research suggests it lasted for millions of years longer than previously suspected. While previous research showed the buried hydrothermal system of porous rock, hot water, and chemical nutrients may have lasted 2 million years, new research says it lasted for 8 million years.</p>]]></description>
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            <title><![CDATA[Did Gravitational Tides Cause Earth's Extinctions?]]></title>
            <link>https://www.universetoday.com/articles/did-gravitational-tides-cause-earths-extinctions</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/did-gravitational-tides-cause-earths-extinctions</guid>
            <pubDate>Tue, 23 Jun 2026 19:24:52 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/flyby_tidal_wave_20260623_175654.jpg" alt="This illustration shows a massive tidal wave created by the flyby of a planetary mass object. New research says Earth may have experienced multiple dangerous flybys that contributed to or caused extinctions in the last 600 million years. Image Credit: Fargion 2026. PoS." width="1280" height="720" /></p><p>Many of Earth's mass extinctions await clear explanations. We know an impact wiped out the dinosaurs, but what about the planet's other extinction events? New research says flybys of planetary mass objects could've been responsible.</p>]]></description>
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            <title><![CDATA[Radio Observations Reveal the Secret of Early Galaxy Growth]]></title>
            <link>https://www.universetoday.com/articles/cosmic-dawn-fuel-discovery-unlocks-early-galaxy-growth-secrets-vla-fuel-discovery</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/cosmic-dawn-fuel-discovery-unlocks-early-galaxy-growth-secrets-vla-fuel-discovery</guid>
            <pubDate>Tue, 23 Jun 2026 18:39:19 +0000</pubDate>
            <dc:creator><![CDATA[Matthew Williams]]></dc:creator>
            <author>Matthew Williams (https://www.universetoday.com/authors/houseofwilliams)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/PIG259-cosmic_timeline5F_lrg_20260623_183147.jpg" alt="This illustration traces the universe’s evolution from the Big Bang to the present day, highlighting REBELS-25, a very distant galaxy seen during the Epoch of Reionization 13 billion years ago. Credit: NSF/AUI/NSF NRAO/M.Weiss" width="1280" height="720" /></p><p>Astronomers have discovered a huge reservoir of cold molecular gas, the direct fuel for star formation, in REBELS-25, a massive, star-forming galaxy.The team, led from ​​Leiden University, focused on REBELS-25, seen when the universe was only about 700 million years old, around 5% of its current age. Astronomers use “redshift” to describe this distance, which measures how much the universe’s expansion has stretched a galaxy’s light to redder wavelengths.</p>]]></description>
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            <title><![CDATA[Ariane 6 Sets New Record for Europe with More Powerful Boosters]]></title>
            <link>https://www.universetoday.com/articles/ariane-6-sets-new-record-for-europe-with-more-powerful-boosters</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/ariane-6-sets-new-record-for-europe-with-more-powerful-boosters</guid>
            <pubDate>Tue, 23 Jun 2026 17:49:31 +0000</pubDate>
            <dc:creator><![CDATA[Matthew Williams]]></dc:creator>
            <author>Matthew Williams (https://www.universetoday.com/authors/houseofwilliams)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/First_Ariane_6_liftoff_with_P160C-based_boosters_20260623_174132.jpg" alt="The inaugural launch of the Ariane 6 with the more powerful P160C-derived boosters. Credit: ESA–S. Corvaja" width="1280" height="720" /></p><p>On 17 June at 09:21 local time (13:21 BST, 14:21 CEST) Ariane 6 flight VA269 soared to orbit from Europe’s Spaceport in French Guiana. 36 satellites for Amazon’s Leo constellation were placed into their orbit just over an hour after liftoff – the eighth successful mission insertion in a row for Europe’s newest rocket.</p>]]></description>
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            <title><![CDATA[This is the First Pair of Sibling Supernova Remnants]]></title>
            <link>https://www.universetoday.com/articles/this-is-the-first-pair-of-sibling-supernova-remnants</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/this-is-the-first-pair-of-sibling-supernova-remnants</guid>
            <pubDate>Tue, 23 Jun 2026 17:18:33 +0000</pubDate>
            <dc:creator><![CDATA[Evan Gough]]></dc:creator>
            <author>Evan Gough (https://www.universetoday.com/authors/ion23drive)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/IC443_IR_opt_UV_narrow_sml_20260622_210606.jpg" alt="This is a multiwavelength image of the Jellyfish Nebula, a supernova remnant about 5,000 light years away. It's made from optical, infrared, and UV observations. The Jellyfish Nebula is the large structure on the right, but the image also shows an arching filament of gas in purple. That filament is actually part of another supernova remnant about the same distance away. New research shows that the pair of remnants may be siblings. Image Credit: NASA Goddard Space Flight Center and M. Michailidis et al. 2026; optical: DSS; infrared: NASA/WISE/JPL-Caltech/UCLA; ultraviolet: NASA/Swift" width="1280" height="720" /></p><p>Astrophysicists have found what is likely the very first pair of sibling supernova remnants. One is the well-known Jellyfish Nebula, and the other was long thought to be hidden in the bright glare from the Jellyfish. The pair are connected by a bright filament of gas.</p>]]></description>
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            <title><![CDATA[The Solar Gravitational Lens Could Map White Dwarfs and Black Holes]]></title>
            <link>https://www.universetoday.com/articles/the-solar-gravitational-lens-could-map-white-dwarfs-and-black-holes</link>
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            <pubDate>Tue, 23 Jun 2026 13:11:07 +0000</pubDate>
            <dc:creator><![CDATA[Andy Tomaswick]]></dc:creator>
            <author>Andy Tomaswick (https://www.universetoday.com/authors/andy-tomaswick)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/eso1907a_20260622_170512.jpg" alt="First ever image of a black hole, taken by the Event Horizon Telescope. Credit - EHT Collaboration" width="1280" height="720" /></p><p>It feels like every few months we get to report on another academic paper coming out singing the praises of the Solar Gravitational SGL (SGL). Partly, this is due to Dr. Slava Turyshev’s astounding productivity in terms of pumping out academic articles, but partly because such a ground-breaking mission has lots of positive aspects, but also challenges that need to be addressed. A new paper, available in pre-print on arXiv from Dr. Turyshev, stresses an often overlooked feature of the SGL - how useful it can be at imaging things other than far away exoplanets.</p>]]></description>
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            <title><![CDATA[Happy Asteroid Day! Prize-Winning Plan Focuses on Space Infrastructure]]></title>
            <link>https://www.universetoday.com/articles/asteroid-day-schweickart-prize-protect-space-infrastructure</link>
            <guid isPermaLink="true">https://www.universetoday.com/articles/asteroid-day-schweickart-prize-protect-space-infrastructure</guid>
            <pubDate>Tue, 23 Jun 2026 04:01:00 +0000</pubDate>
            <dc:creator><![CDATA[Alan Boyle]]></dc:creator>
            <author>Alan Boyle (https://www.universetoday.com/authors/cosmiclog)</author>
            <description><![CDATA[<p><img src="https://www.universetoday.com/article_images/260618-satellites2_20260623_033214.jpg" alt="Scientists say Earth's growing web of satellites is vulnerable to meteor storms. (OneWeb Illustration)" width="1280" height="720" /></p><p>A proposal to create a new network for monitoring cosmic threats to off-world infrastructure has won this year's Schweickart Prize, which recognizes bright ideas for planetary defense.</p>]]></description>
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