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	<title>Astronomy News | Sci.News</title>
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	<link>https://www.sci.news/news/astronomy</link>
	<description>Science news from Sci.News: astronomy, archaeology, paleontology, health, physics, space exploration and other topics.</description>
	<lastBuildDate>Mon, 22 Jun 2026 23:15:35 +0000</lastBuildDate>
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		<title>Interstellar Comet 3I/ATLAS Formed Up To 12 Billion Years Ago, New Observations Suggest</title>
		<link>https://www.sci.news/astronomy/interstellar-comet-3i-atlas-isotopic-ratios-14865.html</link>
					<comments>https://www.sci.news/astronomy/interstellar-comet-3i-atlas-isotopic-ratios-14865.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Mon, 22 Jun 2026 23:11:24 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[3I/ATLAS]]></category>
		<category><![CDATA[Carbon]]></category>
		<category><![CDATA[Carbon-12]]></category>
		<category><![CDATA[Carbon-13]]></category>
		<category><![CDATA[Comet]]></category>
		<category><![CDATA[Cosmic Noon]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[Cyanide]]></category>
		<category><![CDATA[Deuterium]]></category>
		<category><![CDATA[Early Milky Way]]></category>
		<category><![CDATA[Early Universe]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Heavy water]]></category>
		<category><![CDATA[Ice]]></category>
		<category><![CDATA[Interstellar comet]]></category>
		<category><![CDATA[Interstellar object]]></category>
		<category><![CDATA[IR]]></category>
		<category><![CDATA[Isotope]]></category>
		<category><![CDATA[Milky Way]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Nitrogen]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[Universe]]></category>
		<category><![CDATA[UVES]]></category>
		<category><![CDATA[VLT]]></category>
		<category><![CDATA[Water]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110500</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS.jpg" class="attachment-full size-full wp-post-image" alt="Hubble captured this image of 3I/ATLAS on July 21, 2025, when the comet was 446 million km (277 million miles) from Earth. Image credit: NASA / ESA / David Jewitt, UCLA / Joseph DePasquale, STScI." style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS.jpg 710w, https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS-300x169.jpg 300w, https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>The interstellar comet 3I/ATLAS carries a chemical fingerprint unlike anything in our Solar System, and it may have formed 10 to 12 billion years ago, before our Sun even existed, according to two papers published in the journal Nature.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/interstellar-comet-3i-atlas-isotopic-ratios-14865.html">Interstellar Comet 3I/ATLAS Formed Up To 12 Billion Years Ago, New Observations Suggest</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Webb Sees Jupiter-Size Exoplanet Being Roasted by Its Star</title>
		<link>https://www.sci.news/astronomy/webb-roasted-hot-jupiter-14861.html</link>
					<comments>https://www.sci.news/astronomy/webb-roasted-hot-jupiter-14861.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Mon, 22 Jun 2026 15:05:00 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Gas giant]]></category>
		<category><![CDATA[HD 80606]]></category>
		<category><![CDATA[HD 80606b]]></category>
		<category><![CDATA[hot Jupiter]]></category>
		<category><![CDATA[IR]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Orbit]]></category>
		<category><![CDATA[Periastron]]></category>
		<category><![CDATA[Temperature]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110482</guid>

					<description><![CDATA[<div><img width="580" height="326" src="https://cdn.sci.news/images/2026/06/image_14861-HD-80606b.jpg" class="attachment-full size-full wp-post-image" alt="An artist’s impression of the hot-Jupiter exoplanet HD 80606b. Image credit: NASA / ESA / CSA / Joseph Olmsted, STScI." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14861-HD-80606b.jpg 580w, https://cdn.sci.news/images/2026/06/image_14861-HD-80606b-300x169.jpg 300w, https://cdn.sci.news/images/2026/06/image_14861-HD-80606b-195x110.jpg 195w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>HD 80606b has one of the most extreme orbits of any known exoplanet and the NASA/ESA/CSA James Webb Space Telescope just caught it getting flash-fried as it whipped past its star.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/webb-roasted-hot-jupiter-14861.html">Webb Sees Jupiter-Size Exoplanet Being Roasted by Its Star</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Astronomers Find Four Separate Generations of Stars in ‘Globular Cluster’ Terzan 5</title>
		<link>https://www.sci.news/astronomy/terzan-5-stars-14854.html</link>
					<comments>https://www.sci.news/astronomy/terzan-5-stars-14854.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 17 Jun 2026 22:08:15 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Globular cluster]]></category>
		<category><![CDATA[Hubble]]></category>
		<category><![CDATA[Milky Way]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Star cluster]]></category>
		<category><![CDATA[Star formation]]></category>
		<category><![CDATA[Terzan 5]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110436</guid>

					<description><![CDATA[<div><img width="580" height="580" src="https://cdn.sci.news/images/2026/06/image_14854-Terzan-5.jpg" class="attachment-full size-full wp-post-image" alt="This Webb/NIRCam image shows the star cluster Terzan 5. Image credit: NASA / ESA / CSA / Webb." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14854-Terzan-5.jpg 580w, https://cdn.sci.news/images/2026/06/image_14854-Terzan-5-300x300.jpg 300w, https://cdn.sci.news/images/2026/06/image_14854-Terzan-5-150x150.jpg 150w, https://cdn.sci.news/images/2026/06/image_14854-Terzan-5-50x50.jpg 50w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>New Webb and Hubble data not only confirm the existence of two distinct populations of stars in the ancient stellar system Terzan 5, once classified as a globular cluster, but also provides evidence for two more recent rounds of star formation.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/terzan-5-stars-14854.html">Astronomers Find Four Separate Generations of Stars in ‘Globular Cluster’ Terzan 5</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Astronomers Trace Elusive High-Energy Neutrino to Star-Forming Galaxy in Early Universe</title>
		<link>https://www.sci.news/astronomy/high-energy-neutrino-star-forming-galaxy-early-universe-14853.html</link>
					<comments>https://www.sci.news/astronomy/high-energy-neutrino-star-forming-galaxy-early-universe-14853.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 17 Jun 2026 19:48:46 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[ALMA]]></category>
		<category><![CDATA[Cosmic Noon]]></category>
		<category><![CDATA[Early Universe]]></category>
		<category><![CDATA[Gemini North Observatory]]></category>
		<category><![CDATA[GMOS]]></category>
		<category><![CDATA[GNIRS]]></category>
		<category><![CDATA[Gravitational lens]]></category>
		<category><![CDATA[IC 210922A]]></category>
		<category><![CDATA[James Clerk Maxwell Telescope]]></category>
		<category><![CDATA[JCMT0402-0424]]></category>
		<category><![CDATA[Neutrino]]></category>
		<category><![CDATA[Star formation]]></category>
		<category><![CDATA[Starburst galaxy]]></category>
		<category><![CDATA[Submillimeter Array]]></category>
		<category><![CDATA[Universe]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110432</guid>

					<description><![CDATA[<div><img width="580" height="209" src="https://cdn.sci.news/images/2026/06/image_14853-JCMT0402-0424.jpg" class="attachment-full size-full wp-post-image" alt="The origin of high-energy astrophysical neutrinos remains unresolved, and secure electromagnetic counterparts to individual events are rare despite rapid follow-up. Dusty star-forming galaxies at cosmic noon (redshift of z ≈ 1-4) are natural cosmic-ray calorimeters, yet observational links between these galaxies and neutrinos have remained unknown. Urata et al. report a compact-core, dusty star-forming galaxy within an IceCube localization, JCMT0402-0424, a quadruply lensed galaxy at z = 2.988 located inside the 90% containment region of the IceCube event IC 210922A. Image credit: International Gemini Observatory / NOIRLab / NSF / AURA / ALMA / ESO / NAOJ / NRAO / T.A. Rector, University of Alaska Anchorage &amp; NSF’s NOIRLab / D. de Martin &amp; M. Zamani, NSF’s NOIRLab / Yuji Urata. MITOS Science Co., LTD." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14853-JCMT0402-0424.jpg 580w, https://cdn.sci.news/images/2026/06/image_14853-JCMT0402-0424-300x108.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>JCMT0402-0424, a dusty starburst galaxy around 11 billion light-years away, is the strongest candidate yet for the source of the high-energy neutrino event IC 210922A, according to a team of astronomer led by Yuji Urata of MITOS Science Co.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/high-energy-neutrino-star-forming-galaxy-early-universe-14853.html">Astronomers Trace Elusive High-Energy Neutrino to Star-Forming Galaxy in Early Universe</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>New Supernova Study Confirms Universe’s Expansion is Still Accelerating</title>
		<link>https://www.sci.news/astronomy/universes-accelerating-expansion-14851.html</link>
					<comments>https://www.sci.news/astronomy/universes-accelerating-expansion-14851.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 17 Jun 2026 16:04:42 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Acceleration]]></category>
		<category><![CDATA[Dark energy]]></category>
		<category><![CDATA[Hubble constant]]></category>
		<category><![CDATA[Supernova]]></category>
		<category><![CDATA[Type Ia supernova]]></category>
		<category><![CDATA[Universe]]></category>
		<category><![CDATA[Universe’s expansion]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110427</guid>

					<description><![CDATA[<div><img width="580" height="366" src="https://cdn.sci.news/images/2015/06/image_2881_1-Solitary-Supernovae.jpg" class="attachment-full size-full wp-post-image" alt="This is an artist’s concept of a Type Ia supernova exploding in the intergalactic space between galaxies within a galactic cluster. Image credit: Alex Parker / NASA / SDSS." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2015/06/image_2881_1-Solitary-Supernovae.jpg 580w, https://cdn.sci.news/images/2015/06/image_2881_1-Solitary-Supernovae-300x189.jpg 300w, https://cdn.sci.news/images/2015/06/image_2881_1-Solitary-Supernovae-80x50.jpg 80w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>A fresh analysis of Type Ia supernovae overturns a controversial 2025 claim that cosmic expansion is slowing.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/universes-accelerating-expansion-14851.html">New Supernova Study Confirms Universe’s Expansion is Still Accelerating</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Webb Delivers Strongest-Ever Case for ‘Black Hole Stars’ Lurking in Early Universe</title>
		<link>https://www.sci.news/astronomy/webb-black-hole-stars-14843.html</link>
					<comments>https://www.sci.news/astronomy/webb-black-hole-stars-14843.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Mon, 15 Jun 2026 14:00:09 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[Abell S1063]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[Black hole star]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[Early Universe]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Galaxy cluster]]></category>
		<category><![CDATA[GLIMPSE-17775]]></category>
		<category><![CDATA[Gravitational lens]]></category>
		<category><![CDATA[Little red dot]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Spectrum]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[Universe]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110384</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/06/image_14843f-GLIMPSE-17775.jpg" class="attachment-full size-full wp-post-image" alt="This Webb image shows the little red dot GLIMPSE-17775, which is located behind the galaxy cluster Abell S1063. Image credit: NASA / ESA / CSA / Vasily Kokorev, UT Austin / Alyssa Pagan, STScI." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14843f-GLIMPSE-17775.jpg 710w, https://cdn.sci.news/images/2026/06/image_14843f-GLIMPSE-17775-300x169.jpg 300w, https://cdn.sci.news/images/2026/06/image_14843f-GLIMPSE-17775-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Using Webb’s NIRCam and NIRSpec instruments, astronomers have obtained the deepest spectrum ever taken of a little red dot.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/webb-black-hole-stars-14843.html">Webb Delivers Strongest-Ever Case for ‘Black Hole Stars’ Lurking in Early Universe</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Astronomers May Have Found Supernova Remnant near Milky Way’s Central Black Hole</title>
		<link>https://www.sci.news/astronomy/sagittarius-c-supernova-remnant-14841.html</link>
					<comments>https://www.sci.news/astronomy/sagittarius-c-supernova-remnant-14841.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Fri, 12 Jun 2026 15:43:13 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Chandra]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[HII region]]></category>
		<category><![CDATA[Milky Way]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Sagittarius A*]]></category>
		<category><![CDATA[Sagittarius C]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[Supernova]]></category>
		<category><![CDATA[Supernova remnant]]></category>
		<category><![CDATA[X-rays]]></category>
		<category><![CDATA[XMM-Newton]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110375</guid>

					<description><![CDATA[<div><img width="580" height="511" src="https://cdn.sci.news/images/2026/06/image_14841-Sagittarius-C-SNR.jpg" class="attachment-full size-full wp-post-image" alt="This composite image contains X-rays from Chandra and XMM-Newton missions (shown in blue) as well as radio data from the MeerKAT telescope (shown in red) in South Africa. These have been combined with an optical image from the Pan-STARRS telescopes in Hawai’i (red, green, and blue). Image credit: NASA / CXC / UCLA / Zhu et al. / ESA / XMM-Newton / PanSTARRS / MeerKAT / CSA / STScI / SAO / L. Frattare &amp; P. Edmonds." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14841-Sagittarius-C-SNR.jpg 580w, https://cdn.sci.news/images/2026/06/image_14841-Sagittarius-C-SNR-300x264.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Using NASA’s Chandra X-ray Observatory and ESA’s XMM-Newton satellite, astronomers identified a possible remnant of ancient stellar explosion just a few dozen light-years from Sagittarius A*, a supermassive black hole at the center of our Milky Way Galaxy.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/sagittarius-c-supernova-remnant-14841.html">Astronomers May Have Found Supernova Remnant near Milky Way’s Central Black Hole</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals</title>
		<link>https://www.sci.news/astronomy/interstellar-object-3i-atlas-alien-radio-signals-14830.html</link>
					<comments>https://www.sci.news/astronomy/interstellar-object-3i-atlas-alien-radio-signals-14830.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Tue, 09 Jun 2026 16:50:11 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[3I/ATLAS]]></category>
		<category><![CDATA[Allen Telescope Array]]></category>
		<category><![CDATA[Comet]]></category>
		<category><![CDATA[Extraterrestrial civilization]]></category>
		<category><![CDATA[Extraterrestrial intelligence]]></category>
		<category><![CDATA[Extraterrestrial life]]></category>
		<category><![CDATA[Extraterrestrials]]></category>
		<category><![CDATA[Interstellar comet]]></category>
		<category><![CDATA[Interstellar object]]></category>
		<category><![CDATA[Radio signal]]></category>
		<category><![CDATA[SETI]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[Technosignature]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110323</guid>

					<description><![CDATA[<div><img width="580" height="344" src="https://cdn.sci.news/images/2026/04/image_14695-3I-ATLAS.jpg" class="attachment-full size-full wp-post-image" alt="This image from the Subaru Telescope shows the interstellar comet 3I/ATLAS. Image credit: NAOJ." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/04/image_14695-3I-ATLAS.jpg 580w, https://cdn.sci.news/images/2026/04/image_14695-3I-ATLAS-300x178.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Using the SETI Institute’s Allen Telescope Array, a 42-element radio interferometer at Hat Creek Radio Observatory in Hat Creek, California, astronomers probed 3I/ATLAS for artificial radio transmissions but found only human-made interference.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/interstellar-object-3i-atlas-alien-radio-signals-14830.html">Astronomers Scan Interstellar Object 3I/ATLAS for Alien Radio Signals</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Astronomers Finally Find Milky Way’s Missing Black Hole Wind</title>
		<link>https://www.sci.news/astronomy/milky-ways-black-hole-wind-14827.html</link>
					<comments>https://www.sci.news/astronomy/milky-ways-black-hole-wind-14827.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Mon, 08 Jun 2026 17:42:00 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[ALMA]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[Black hole wind]]></category>
		<category><![CDATA[Carbon monoxide]]></category>
		<category><![CDATA[Chandra]]></category>
		<category><![CDATA[Galactic wind]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Gas]]></category>
		<category><![CDATA[Milky Way]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Nuclear wind]]></category>
		<category><![CDATA[Outflow]]></category>
		<category><![CDATA[Sagittarius A*]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[X-rays]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110301</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/06/image_14827f-Sagittarius-A-Wind.jpg" class="attachment-full size-full wp-post-image" alt="This image shows the evidence for the wind blowing away from Sagittarius A*: the white dot in the center of the image shows the supermassive black hole; in orange is data from ALMA, mapping the location of cold gas composed of carbon monoxide in the image; in blue is X-ray data from Chandra; a large cone-shaped cavity, visible as an absence of cold gas in the ALMA data, is filled by hot X-ray-emitting gas in the Chandra data. Image credit: NASA / CXC / UMass / Wang et al. / ALMA / ESO / NAOJ / NRAO / Longmore et al. / Minniti et al." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14827f-Sagittarius-A-Wind.jpg 710w, https://cdn.sci.news/images/2026/06/image_14827f-Sagittarius-A-Wind-300x169.jpg 300w, https://cdn.sci.news/images/2026/06/image_14827f-Sagittarius-A-Wind-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>After a 50-year search, astronomers have uncovered evidence that Sagittarius A* -- the 4.3-million-solar-mass black hole that resides at the center of our Milky Way Galaxy -- is blowing a hot cosmic wind into its surroundings, carving out a giant cavity near the Galaxy’s heart.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/milky-ways-black-hole-wind-14827.html">Astronomers Finally Find Milky Way’s Missing Black Hole Wind</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Two Glowing Nebulae Spark Cosmic Pareidolia in New VST Image</title>
		<link>https://www.sci.news/astronomy/two-glowing-nebulae-pareidolia-vst-image-14825.html</link>
					<comments>https://www.sci.news/astronomy/two-glowing-nebulae-pareidolia-vst-image-14825.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Mon, 08 Jun 2026 13:03:22 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Emission nebula]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Gum 10]]></category>
		<category><![CDATA[Gum 11]]></category>
		<category><![CDATA[Nebula]]></category>
		<category><![CDATA[NGC 2579]]></category>
		<category><![CDATA[Pareidolia]]></category>
		<category><![CDATA[RCW 19]]></category>
		<category><![CDATA[VST]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110292</guid>

					<description><![CDATA[<div><img width="580" height="471" src="https://cdn.sci.news/images/2026/06/image_14825-Gum-10-Gum-11.jpg" class="attachment-full size-full wp-post-image" alt="This VST image shows Gum 10 and Gum 11, two nebulae in the southern constellation of Puppis. Image credit: ESO / VPHAS+ Team." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14825-Gum-10-Gum-11.jpg 580w, https://cdn.sci.news/images/2026/06/image_14825-Gum-10-Gum-11-300x244.jpg 300w, https://cdn.sci.news/images/2026/06/image_14825-Gum-10-Gum-11-60x49.jpg 60w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Astronomers using ESO’s VLT Survey Telescope have captured a spectacular image of two little-known nebulae: Gum 10 and Gum 11.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/two-glowing-nebulae-pareidolia-vst-image-14825.html">Two Glowing Nebulae Spark Cosmic Pareidolia in New VST Image</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Jupiter Accelerates Electrons to Near-Light Speed, Offering Clues to Cosmic Ray Origins</title>
		<link>https://www.sci.news/space/jupiter-bow-shock-electron-acceleration-14822.html</link>
					<comments>https://www.sci.news/space/jupiter-bow-shock-electron-acceleration-14822.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Fri, 05 Jun 2026 20:09:47 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Planetary Science]]></category>
		<category><![CDATA[Space Exploration]]></category>
		<category><![CDATA[Acceleration]]></category>
		<category><![CDATA[Bow shock]]></category>
		<category><![CDATA[Cosmic rays]]></category>
		<category><![CDATA[Electron]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Gas giant]]></category>
		<category><![CDATA[Hillas limit]]></category>
		<category><![CDATA[Juno]]></category>
		<category><![CDATA[Jupiter]]></category>
		<category><![CDATA[Milky Way]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Planet]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[Solar wind]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Stellar wind]]></category>
		<category><![CDATA[Sun]]></category>
		<category><![CDATA[Supernova]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110267</guid>

					<description><![CDATA[<div><img width="580" height="417" src="https://cdn.sci.news/images/2026/06/image_14822-Bow-Shock.jpg" class="attachment-full size-full wp-post-image" alt="As planets and stars travel through the streams of charged particles flowing across space, their magnetic fields act like obstacles; incoming particles are slowed and deflected, forming a boundary called the bow shock; just ahead of this boundary lies the foreshock, a variable region where magnetic conditions can accelerate some particles to nearly the speed of light. Image credit: Ben C. Smith, Johns Hopkins Applied Physics Laboratory." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14822-Bow-Shock.jpg 580w, https://cdn.sci.news/images/2026/06/image_14822-Bow-Shock-300x216.jpg 300w, https://cdn.sci.news/images/2026/06/image_14822-Bow-Shock-104x75.jpg 104w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>The giant planet’s bow shock isn’t just deflecting the solar wind, it’s acting as a powerful particle accelerator, firing electrons to relativistic energies of at least 1 MeV, according to a new analysis of data from NASA’s Juno spacecraft.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/space/jupiter-bow-shock-electron-acceleration-14822.html">Jupiter Accelerates Electrons to Near-Light Speed, Offering Clues to Cosmic Ray Origins</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Webb Weighs Most Distant Inactive Black Hole Ever Found</title>
		<link>https://www.sci.news/astronomy/webb-most-distant-inactive-black-hole-14820.html</link>
					<comments>https://www.sci.news/astronomy/webb-most-distant-inactive-black-hole-14820.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Fri, 05 Jun 2026 15:58:51 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[Early Universe]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Gravitational lens]]></category>
		<category><![CDATA[IR]]></category>
		<category><![CDATA[Mass]]></category>
		<category><![CDATA[MRG-M0138]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Quasar]]></category>
		<category><![CDATA[Quiescent galaxy]]></category>
		<category><![CDATA[Star formation]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[Universe]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110256</guid>

					<description><![CDATA[<div><img width="580" height="580" src="https://cdn.sci.news/images/2026/06/image_14820-MRG-M0138.jpg" class="attachment-full size-full wp-post-image" alt="This Webb image shows the highly distorted red galaxy MRG-M0138 seen through a foreground cluster of galaxies (white sources). Image credit: NASA / ESA / CSA / Webb." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14820-MRG-M0138.jpg 580w, https://cdn.sci.news/images/2026/06/image_14820-MRG-M0138-300x300.jpg 300w, https://cdn.sci.news/images/2026/06/image_14820-MRG-M0138-150x150.jpg 150w, https://cdn.sci.news/images/2026/06/image_14820-MRG-M0138-50x50.jpg 50w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>A supermassive black hole 6 billion times the mass of the Sun lurks in MRG-M0138, a gravitationally lensed quiescent galaxy seen when the Universe was just 3 billion years old, according to an analysis of data collected by the NIRSpec Integral Field Spectrograph onboard the NASA/ESA/CSA James Webb Space Telescope.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/webb-most-distant-inactive-black-hole-14820.html">Webb Weighs Most Distant Inactive Black Hole Ever Found</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Astronomers Detect Clearest Signs Yet of Magnetic Fields on Extrasolar Planets</title>
		<link>https://www.sci.news/astronomy/exoplanet-magnetic-fields-14812.html</link>
					<comments>https://www.sci.news/astronomy/exoplanet-magnetic-fields-14812.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Tue, 02 Jun 2026 18:50:56 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Atmosphere]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[ESPRESSO]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Gas giant]]></category>
		<category><![CDATA[Gemini North Observatory]]></category>
		<category><![CDATA[Gemini Observatory]]></category>
		<category><![CDATA[Magnetic field]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[ultrahot Jupiter]]></category>
		<category><![CDATA[VLT]]></category>
		<category><![CDATA[Wind]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110211</guid>

					<description><![CDATA[<div><img width="580" height="326" src="https://cdn.sci.news/images/2026/06/image_14812-Magnetic-Exoplanet.jpg" class="attachment-full size-full wp-post-image" alt="This illustration shows magnetic activity in an ultra-hot Jupiter. Image credit: ESO / M. Kornmesser / L. Calçada." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14812-Magnetic-Exoplanet.jpg 580w, https://cdn.sci.news/images/2026/06/image_14812-Magnetic-Exoplanet-300x169.jpg 300w, https://cdn.sci.news/images/2026/06/image_14812-Magnetic-Exoplanet-195x110.jpg 195w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>By tracking fierce winds racing through the atmospheres of seven ultra-hot Jupiters, astronomers have uncovered the strongest evidence yet that magnetic fields shape weather on worlds beyond our Solar System.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/exoplanet-magnetic-fields-14812.html">Astronomers Detect Clearest Signs Yet of Magnetic Fields on Extrasolar Planets</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Webb Detects Methane on Interstellar Comet 3I/ATLAS</title>
		<link>https://www.sci.news/astronomy/webb-methane-interstellar-comet-3i-atlas-14810.html</link>
					<comments>https://www.sci.news/astronomy/webb-methane-interstellar-comet-3i-atlas-14810.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Tue, 02 Jun 2026 00:07:28 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[3I/ATLAS]]></category>
		<category><![CDATA[Carbon dioxide]]></category>
		<category><![CDATA[Carbon monoxide]]></category>
		<category><![CDATA[Comet]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Interstellar comet]]></category>
		<category><![CDATA[IR]]></category>
		<category><![CDATA[Methane]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[Spectrum]]></category>
		<category><![CDATA[Water]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110195</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS.jpg" class="attachment-full size-full wp-post-image" alt="Hubble captured this image of 3I/ATLAS on July 21, 2025, when the comet was 446 million km (277 million miles) from Earth. Image credit: NASA / ESA / David Jewitt, UCLA / Joseph DePasquale, STScI." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS.jpg 710w, https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS-300x169.jpg 300w, https://cdn.sci.news/images/2026/06/image_14810f-3I-ATLAS-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Using the spectral data from the Mid-Infrared Instrument (MIRI) onboard the NASA/ESA/CSA James Webb Space Telescope, astronomers have detected methane on 3I/ATLAS.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/webb-methane-interstellar-comet-3i-atlas-14810.html">Webb Detects Methane on Interstellar Comet 3I/ATLAS</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Hubble Captures Active Spiral Galaxy: Messier 88</title>
		<link>https://www.sci.news/astronomy/hubble-active-spiral-galaxy-messier-88-14807.html</link>
					<comments>https://www.sci.news/astronomy/hubble-active-spiral-galaxy-messier-88-14807.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Mon, 01 Jun 2026 14:51:17 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Active galactic nucleus]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Galaxy cluster]]></category>
		<category><![CDATA[Hubble]]></category>
		<category><![CDATA[M88]]></category>
		<category><![CDATA[Messier 88]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[NGC 4501]]></category>
		<category><![CDATA[Ram-pressure stripping]]></category>
		<category><![CDATA[Spiral galaxy]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[Virgo Cluster]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110180</guid>

					<description><![CDATA[<div><img width="580" height="277" src="https://cdn.sci.news/images/2026/06/image_14807-Messier-88.jpg" class="attachment-full size-full wp-post-image" alt="This image, taken with the Wide Field Camera 3 (WFC3) instrument aboard the NASA/ESA Hubble Space Telescope, shows the spiral galaxy Messier 88. Image credit: NASA / ESA / Hubble / D. Thilker / MAUVE-HST Team." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/06/image_14807-Messier-88.jpg 580w, https://cdn.sci.news/images/2026/06/image_14807-Messier-88-300x143.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>A newly-released Hubble image shows Messier 88, a black hole-powered spiral galaxy that is gradually plunging toward the crowded heart of the Virgo Cluster.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/hubble-active-spiral-galaxy-messier-88-14807.html">Hubble Captures Active Spiral Galaxy: Messier 88</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Webb Spots Supermassive Black Hole Older Than Its Home Galaxy</title>
		<link>https://www.sci.news/astronomy/webb-supermassive-black-hole-early-universe-14803.html</link>
					<comments>https://www.sci.news/astronomy/webb-supermassive-black-hole-early-universe-14803.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Fri, 29 May 2026 00:26:39 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[A2744-QSO1]]></category>
		<category><![CDATA[Abell 2744]]></category>
		<category><![CDATA[Abell 2744-QSO1]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[Early Universe]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Galaxy cluster]]></category>
		<category><![CDATA[Gravitational lens]]></category>
		<category><![CDATA[Hydrogen]]></category>
		<category><![CDATA[IR]]></category>
		<category><![CDATA[Keplerian motion]]></category>
		<category><![CDATA[Little red dot]]></category>
		<category><![CDATA[Metallicity]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[Universe]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110141</guid>

					<description><![CDATA[<div><img width="580" height="434" src="https://cdn.sci.news/images/2026/05/image_14803-Abell-2744-QSO1.jpg" class="attachment-full size-full wp-post-image" alt="This Webb/NIRCam image shows the little red dot Abell2744-QSO1, magnified and triply imaged by galaxy cluster Abell 2744. Image credit: NASA / ESA / CSA / Lukas Furtak, Ben-Gurion University / Alyssa Pagan, STScI." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/05/image_14803-Abell-2744-QSO1.jpg 580w, https://cdn.sci.news/images/2026/05/image_14803-Abell-2744-QSO1-300x224.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Astronomers using the NASA/ESA/CSA James Webb Space Telescope have found an enormous black hole in the early Universe that appears to predate its own host galaxy, raising fresh questions about how the cosmos’ first supermassive monsters were born.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/webb-supermassive-black-hole-early-universe-14803.html">Webb Spots Supermassive Black Hole Older Than Its Home Galaxy</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Is Dark Energy Unnecessary? Mathematicians Challenge Standard Cosmological Model of Universe</title>
		<link>https://www.sci.news/astronomy/dark-energy-alternative-14801.html</link>
					<comments>https://www.sci.news/astronomy/dark-energy-alternative-14801.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Thu, 28 May 2026 19:28:06 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Mathematics]]></category>
		<category><![CDATA[Physics]]></category>
		<category><![CDATA[Big Bang]]></category>
		<category><![CDATA[Cold dark matter]]></category>
		<category><![CDATA[Dark energy]]></category>
		<category><![CDATA[Friedmann spacetimes]]></category>
		<category><![CDATA[Hubble constant]]></category>
		<category><![CDATA[Space-Time]]></category>
		<category><![CDATA[Standard Model]]></category>
		<category><![CDATA[Universe]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110135</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2018/06/image_6061f-Electric-Dark-Matter.jpg" class="attachment-full size-full wp-post-image" alt="This artist’s impression shows the evolution of the Universe beginning with the Big Bang on the left followed by the appearance of the Cosmic Microwave Background. The formation of the first stars ends the cosmic dark ages, followed by the formation of galaxies. Image credit: M. Weiss / Harvard-Smithsonian Center for Astrophysics." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2018/06/image_6061f-Electric-Dark-Matter.jpg 710w, https://cdn.sci.news/images/2018/06/image_6061f-Electric-Dark-Matter-300x169.jpg 300w, https://cdn.sci.news/images/2018/06/image_6061f-Electric-Dark-Matter-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Mathematicians from University College London and the University of California, Davis, have published a mathematical proof that the Universe’s accelerating expansion can be explained without dark energy, dealing a serious blow to the Lambda-cold dark matter model.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/dark-energy-alternative-14801.html">Is Dark Energy Unnecessary? Mathematicians Challenge Standard Cosmological Model of Universe</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Webb Detects Methane in Atmosphere of Exo-Saturn TOI-199b</title>
		<link>https://www.sci.news/astronomy/webb-methane-atmosphere-exo-saturn-toi-199b-14791.html</link>
					<comments>https://www.sci.news/astronomy/webb-methane-atmosphere-exo-saturn-toi-199b-14791.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Mon, 25 May 2026 18:16:53 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Ammonia]]></category>
		<category><![CDATA[Atmosphere]]></category>
		<category><![CDATA[Carbon dioxide]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[exo-Saturn]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Gas giant]]></category>
		<category><![CDATA[IR]]></category>
		<category><![CDATA[Methane]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Spectrum]]></category>
		<category><![CDATA[TOI-199]]></category>
		<category><![CDATA[TOI-199b]]></category>
		<category><![CDATA[Transmission spectrum]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110081</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2021/09/image_10113f-TOI-1518b.jpg" class="attachment-full size-full wp-post-image" alt="An artist’s rendition of the ultrahot Jupiter TOI-1518b and its parent star. Image credit: Sci-News.com." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2021/09/image_10113f-TOI-1518b.jpg 710w, https://cdn.sci.news/images/2021/09/image_10113f-TOI-1518b-300x169.jpg 300w, https://cdn.sci.news/images/2021/09/image_10113f-TOI-1518b-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Using spectral data from the Near-Infrared Spectrograph (NIRSpec) onboard the NASA/ESA/CSA James Webb Space Telescope, astronomers analyzed the atmosphere of TOI-199b, a distant Saturn-mass world that is neither frozen nor scorching hot.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/webb-methane-atmosphere-exo-saturn-toi-199b-14791.html">Webb Detects Methane in Atmosphere of Exo-Saturn TOI-199b</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Gemini North Telescope Peers into Crystal Ball Nebula</title>
		<link>https://www.sci.news/astronomy/gemini-north-telescope-crystal-ball-nebula-14788.html</link>
					<comments>https://www.sci.news/astronomy/gemini-north-telescope-crystal-ball-nebula-14788.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Fri, 22 May 2026 20:00:49 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Binary star]]></category>
		<category><![CDATA[Crystal Ball Nebula]]></category>
		<category><![CDATA[Gemini North Observatory]]></category>
		<category><![CDATA[Gemini Observatory]]></category>
		<category><![CDATA[GMOS]]></category>
		<category><![CDATA[Nebula]]></category>
		<category><![CDATA[NGC 1514]]></category>
		<category><![CDATA[NOIRLab]]></category>
		<category><![CDATA[NSF]]></category>
		<category><![CDATA[Planetary nebula]]></category>
		<category><![CDATA[Star]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110065</guid>

					<description><![CDATA[<div><img width="580" height="445" src="https://cdn.sci.news/images/2026/05/image_14788-Crystal-Ball-Nebula.jpg" class="attachment-full size-full wp-post-image" alt="This image of the Crystal Ball Nebula was captured by the 8.1-m Gemini North telescope at the International Gemini Observatory. Image credit: J. Miller &amp; M. Rodriguez, International Gemini Observatory &amp; NSF’s NOIRLab / T.A. Rector, University of Alaska Anchorage &amp; NSF’s NOIRLab / D. de Martin &amp; M. Zamani, NSF’s NOIRLab." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/05/image_14788-Crystal-Ball-Nebula.jpg 580w, https://cdn.sci.news/images/2026/05/image_14788-Crystal-Ball-Nebula-300x230.jpg 300w, https://cdn.sci.news/images/2026/05/image_14788-Crystal-Ball-Nebula-74x58.jpg 74w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>A stunning new image from the 8.1-m Gemini North telescope, located on the summit of Maunakea in Hawai’i, reveals the Crystal Ball Nebula in unprecedented detail: a lumpy, glowing sphere of gas sculpted by a pair of stars.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/gemini-north-telescope-crystal-ball-nebula-14788.html">Gemini North Telescope Peers into Crystal Ball Nebula</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<title>Fermi Identifies Hidden Engine behind Superluminous Supernovae</title>
		<link>https://www.sci.news/astronomy/fermi-superluminous-supernovae-14784.html</link>
					<comments>https://www.sci.news/astronomy/fermi-superluminous-supernovae-14784.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 20 May 2026 20:36:28 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Barred spiral galaxy]]></category>
		<category><![CDATA[Core-collapse supernova]]></category>
		<category><![CDATA[Fermi]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Gamma rays]]></category>
		<category><![CDATA[Magnetar]]></category>
		<category><![CDATA[Magnetar wind nebula]]></category>
		<category><![CDATA[Magnetic field]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Neutron star]]></category>
		<category><![CDATA[NGC 3191]]></category>
		<category><![CDATA[SN 2017egm]]></category>
		<category><![CDATA[Spiral galaxy]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Superluminous supernova]]></category>
		<category><![CDATA[Supernova]]></category>
		<category><![CDATA[Wind nebula]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110047</guid>

					<description><![CDATA[<div><img width="580" height="287" src="https://cdn.sci.news/images/2026/05/image_14784-SN-2017egm.jpg" class="attachment-full size-full wp-post-image" alt="The superluminous supernova SN 2017egm was discovered by ESA’s Gaia mission on May 23, 2017; it exploded in a massive barred spiral galaxy known as NGC 3191, shown on the left before the eruption; the image at right, taken on July 1, 2017, shows the supernova outshining the entire galaxy. Image credit: SDSS / PS1 / NOT+ALFSOC / Bose et al." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/05/image_14784-SN-2017egm.jpg 580w, https://cdn.sci.news/images/2026/05/image_14784-SN-2017egm-300x148.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>New gamma-ray observations from NASA’s Fermi Space Telescope suggest ultra-magnetic neutron stars called magnetars could be fueling superluminous supernovae, a rare class of stellar explosions with peak luminosities 10-100 times greater than those of standard core-collapse supernovae.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/fermi-superluminous-supernovae-14784.html">Fermi Identifies Hidden Engine behind Superluminous Supernovae</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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