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<channel>
	<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>Fri, 07 Aug 2026 16:13:10 +0000</lastBuildDate>
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		<title>Inouye Solar Telescope Discovers Hidden Plasma Vortices on Sun</title>
		<link>https://www.sci.news/astronomy/inouye-solar-telescope-plasma-vortices-sun-14974.html</link>
					<comments>https://www.sci.news/astronomy/inouye-solar-telescope-plasma-vortices-sun-14974.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Fri, 07 Aug 2026 16:13:10 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[Corona]]></category>
		<category><![CDATA[Inouye Solar Telescope]]></category>
		<category><![CDATA[Kelvin-Helmholtz instability]]></category>
		<category><![CDATA[Photosphere]]></category>
		<category><![CDATA[Plasma]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Sun]]></category>
		<category><![CDATA[Vortex]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=111149</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/08/image_14974f-Sun-Photosphere.jpg" class="attachment-full size-full wp-post-image" alt="The highest-resolution image of the Sun’s surface (photosphere) ever captured, taken at 416 nm by the Inouye Solar Telescope; it reveals deformed boundaries of magnetic elements and ultra-fine scale stripes, both associated with Kelvin-Helmholtz instability. Image credit: NSF / NSO / AURA / MPS." style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/08/image_14974f-Sun-Photosphere.jpg 710w, https://cdn.sci.news/images/2026/08/image_14974f-Sun-Photosphere-300x169.jpg 300w, https://cdn.sci.news/images/2026/08/image_14974f-Sun-Photosphere-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Astronomers using the 4-m Daniel K. Inouye Solar Telescope in Hawaii have detected tiny plasma vortices on the Sun’s surface (photosphere) for the first time, revealing a long-suspected process that could transport energy into the million-degree corona.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/inouye-solar-telescope-plasma-vortices-sun-14974.html">Inouye Solar Telescope Discovers Hidden Plasma Vortices on Sun</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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			</item>
		<item>
		<title>Astronomers Discover First-Ever Three-Lobed Asteroid</title>
		<link>https://www.sci.news/astronomy/three-lobed-asteroid-nysa-14965.html</link>
					<comments>https://www.sci.news/astronomy/three-lobed-asteroid-nysa-14965.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Tue, 04 Aug 2026 21:17:17 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Asteroid]]></category>
		<category><![CDATA[Asteroid belt]]></category>
		<category><![CDATA[E-type asteroid]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Large Binocular Telescope]]></category>
		<category><![CDATA[Nysa]]></category>
		<category><![CDATA[SHARK-VIS]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[SPHERE]]></category>
		<category><![CDATA[VLT]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=111101</guid>

					<description><![CDATA[<div><img width="580" height="580" src="https://cdn.sci.news/images/2026/08/image_14965-Nysa.jpg" class="attachment-full size-full wp-post-image" alt="This image of the Nysa system was captured on February 15, 2026. Image credit: Minker et al., arXiv: 2607.25786." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/08/image_14965-Nysa.jpg 580w, https://cdn.sci.news/images/2026/08/image_14965-Nysa-300x300.jpg 300w, https://cdn.sci.news/images/2026/08/image_14965-Nysa-150x150.jpg 150w, https://cdn.sci.news/images/2026/08/image_14965-Nysa-50x50.jpg 50w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>High-resolution images from ESO’s Very Large Telescope and the Large Binocular Telescope reveal that the E-type asteroid (44) Nysa may be unlike any other world in the Solar System, with three connected lobes and a newly discovered satellite that could help explain how the bizarre object formed.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/three-lobed-asteroid-nysa-14965.html">Astronomers Discover First-Ever Three-Lobed Asteroid</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<item>
		<title>Pluto’s Thin Atmosphere May Be Starting to Shrink</title>
		<link>https://www.sci.news/astronomy/plutos-atmosphere-14963.html</link>
					<comments>https://www.sci.news/astronomy/plutos-atmosphere-14963.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Tue, 04 Aug 2026 15:53:24 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Planetary Science]]></category>
		<category><![CDATA[Space Exploration]]></category>
		<category><![CDATA[Atmosphere]]></category>
		<category><![CDATA[Dwarf planet]]></category>
		<category><![CDATA[Planet]]></category>
		<category><![CDATA[Pluto]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Stellar occultation]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=111091</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2015/10/image_3323f-Plutos-Blue-Skies.jpg" class="attachment-full size-full wp-post-image" alt="According to NASA scientists, complex chemical compounds called tholins give Pluto a distinctive blue haze. Image credit: NASA / Johns Hopkins University Applied Physics Laboratory / Southwest Research Institute." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2015/10/image_3323f-Plutos-Blue-Skies.jpg 710w, https://cdn.sci.news/images/2015/10/image_3323f-Plutos-Blue-Skies-300x169.jpg 300w, https://cdn.sci.news/images/2015/10/image_3323f-Plutos-Blue-Skies-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Pluto’s tenuous atmosphere appears to have begun contracting after years of holding steady, according to a new study published in the Planetary Science Journal.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/plutos-atmosphere-14963.html">Pluto’s Thin Atmosphere May Be Starting to Shrink</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 Spot Wandering Supermassive Black Hole Far From Its Galaxy’s Heart</title>
		<link>https://www.sci.news/astronomy/wandering-supermassive-black-hole-14953.html</link>
					<comments>https://www.sci.news/astronomy/wandering-supermassive-black-hole-14953.html#comments</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 29 Jul 2026 13:36:38 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[TDE 2025abcr]]></category>
		<category><![CDATA[Tidal disruption]]></category>
		<category><![CDATA[Wandering black hole]]></category>
		<category><![CDATA[WISEA J014656.04-152214.7]]></category>
		<category><![CDATA[Zwicky Transient Facility]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=111047</guid>

					<description><![CDATA[<div><img width="580" height="580" src="https://cdn.sci.news/images/2026/07/image_14953-TDE-2025abcr.jpg" class="attachment-full size-full wp-post-image" alt="TDE 2025abcr. Image credit: Stein et al., doi: 10.3847/2041-8213/ae77f3." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14953-TDE-2025abcr.jpg 580w, https://cdn.sci.news/images/2026/07/image_14953-TDE-2025abcr-300x300.jpg 300w, https://cdn.sci.news/images/2026/07/image_14953-TDE-2025abcr-150x150.jpg 150w, https://cdn.sci.news/images/2026/07/image_14953-TDE-2025abcr-50x50.jpg 50w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Astronomers have discovered a dormant supermassive black hole 30,000 light-years from the center of WISEA J014656.04-152214.7 -- a massive galaxy located about 750 million light-years away in the constellation of Cetus -- after it briefly lit up by tearing apart a star.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/wandering-supermassive-black-hole-14953.html">Astronomers Spot Wandering Supermassive Black Hole Far From Its Galaxy’s Heart</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 Directly Image Betelgeuse’s Long-Suspected Stellar Companion</title>
		<link>https://www.sci.news/astronomy/direct-image-betelgeuse-b-14951.html</link>
					<comments>https://www.sci.news/astronomy/direct-image-betelgeuse-b-14951.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Tue, 28 Jul 2026 20:43:12 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[Betelgeuse]]></category>
		<category><![CDATA[Betelgeuse B]]></category>
		<category><![CDATA[Binary star]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Red supergiant]]></category>
		<category><![CDATA[SPHERE]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Supergiant star]]></category>
		<category><![CDATA[VLT]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=111031</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/07/image_14951f-Betelgeuse-B.jpg" class="attachment-full size-full wp-post-image" alt="This VLT/SPHERE image shows the clearest image ever of what likely is Betelgeuse B. Image credit: ESO / Montargès et al." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14951f-Betelgeuse-B.jpg 710w, https://cdn.sci.news/images/2026/07/image_14951f-Betelgeuse-B-300x169.jpg 300w, https://cdn.sci.news/images/2026/07/image_14951f-Betelgeuse-B-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>After a century of speculation, astronomers using ESO’s Very Large Telescope (VLT) have captured the clearest evidence yet that the red supergiant Betelgeuse is orbited by a faint companion star.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/direct-image-betelgeuse-b-14951.html">Astronomers Directly Image Betelgeuse’s Long-Suspected Stellar Companion</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<item>
		<title>Hubble Spots Spiral Galaxy Warped by Cosmic Forces</title>
		<link>https://www.sci.news/astronomy/hubble-warped-intermediate-spiral-galaxy-14947.html</link>
					<comments>https://www.sci.news/astronomy/hubble-warped-intermediate-spiral-galaxy-14947.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Mon, 27 Jul 2026 16:05:31 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Galaxy cluster]]></category>
		<category><![CDATA[Hubble]]></category>
		<category><![CDATA[Intermediate spiral galaxy]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[NGC 4639]]></category>
		<category><![CDATA[NGC 4654]]></category>
		<category><![CDATA[Ram-pressure stripping]]></category>
		<category><![CDATA[Spiral galaxy]]></category>
		<category><![CDATA[Virgo Cluster]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=111008</guid>

					<description><![CDATA[<div><img width="580" height="557" src="https://cdn.sci.news/images/2026/07/image_14947-NGC-4654.jpg" class="attachment-full size-full wp-post-image" alt="This Hubble image shows NGC 4654, an intermediate spiral galaxy some 55 million light-years away in the constellation of Virgo. Image credit: NASA / ESA / Hubble / D. Thilker / J. Lee / PHANGS-HST Team." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14947-NGC-4654.jpg 580w, https://cdn.sci.news/images/2026/07/image_14947-NGC-4654-300x288.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>A stunning new image captured by the NASA/ESA Hubble Space Telescope shows the lopsided intermediate spiral galaxy NGC 4654, whose unusual shape was sculpted by both a close encounter with another galaxy and a headlong plunge through the hot gas of the Virgo Cluster.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/hubble-warped-intermediate-spiral-galaxy-14947.html">Hubble Spots Spiral Galaxy Warped by Cosmic Forces</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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		<item>
		<title>Planetary-Mass Exomoon Found Circling Brown Dwarf</title>
		<link>https://www.sci.news/astronomy/brown-dwarf-exomoon-14945.html</link>
					<comments>https://www.sci.news/astronomy/brown-dwarf-exomoon-14945.html#respond</comments>
		
		<dc:creator><![CDATA[Natali Anderson]]></dc:creator>
		<pubDate>Sun, 26 Jul 2026 23:35:45 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[Brown dwarf]]></category>
		<category><![CDATA[Brown dwarf moon]]></category>
		<category><![CDATA[CD-35 2722]]></category>
		<category><![CDATA[CRIRES+]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Exomoon]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Gas giant]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[VLT]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=111002</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/07/image_14945f-CD-35-2722.jpg" class="attachment-full size-full wp-post-image" alt="This illustration shows the stellar system CD-35 2722, with the newly found exomoon at the center; the star has about half the mass of our Sun, and it is orbited by a brown dwarf, the reddish-brown object seen here in the foreground (right). Image credit: ESO / M. Kornmesser." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14945f-CD-35-2722.jpg 710w, https://cdn.sci.news/images/2026/07/image_14945f-CD-35-2722-300x169.jpg 300w, https://cdn.sci.news/images/2026/07/image_14945f-CD-35-2722-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Astronomers using ESO’s Very Large Telescope (VLT) have discovered a gas giant around a brown dwarf in the stellar system CD-35 2722.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/brown-dwarf-exomoon-14945.html">Planetary-Mass Exomoon Found Circling Brown Dwarf</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>Our Milky Way Galaxy Likely Underwent Disk Flip after Ancient Galactic Collision: Study</title>
		<link>https://www.sci.news/astronomy/milky-way-galaxy-disk-flip-14935.html</link>
					<comments>https://www.sci.news/astronomy/milky-way-galaxy-disk-flip-14935.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 22 Jul 2026 15:57:12 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Dark matter]]></category>
		<category><![CDATA[Dark matter halo]]></category>
		<category><![CDATA[Early Milky Way]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Gaia satellite]]></category>
		<category><![CDATA[Gaia-Sausage-Enceladus]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Galaxy disk]]></category>
		<category><![CDATA[Halo]]></category>
		<category><![CDATA[Merger]]></category>
		<category><![CDATA[Milky Way]]></category>
		<category><![CDATA[Rotation]]></category>
		<category><![CDATA[Spiral galaxy]]></category>
		<category><![CDATA[Star]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110939</guid>

					<description><![CDATA[<div><img width="580" height="486" src="https://cdn.sci.news/images/2026/07/image_14935-Milky-Way-Disk-Flip.jpg" class="attachment-full size-full wp-post-image" alt="Using supercomputer simulations of galaxies like the Milky Way, Batrakov et al. found that galaxies with slowly rotating stellar haloes are more likely to have experienced a major ‘disk flip,’ where our Galaxy’s disk changed its orientation by more than 90 degrees. Image credit: Batrakov et al." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14935-Milky-Way-Disk-Flip.jpg 580w, https://cdn.sci.news/images/2026/07/image_14935-Milky-Way-Disk-Flip-300x251.jpg 300w, https://cdn.sci.news/images/2026/07/image_14935-Milky-Way-Disk-Flip-60x49.jpg 60w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>A head-on collision with another galaxy billions of years ago may have dramatically reoriented the Milky Way’s disk, according to new supercomputer simulations that reveal how violent mergers can leave spiral galaxies looking surprisingly normal today.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/milky-way-galaxy-disk-flip-14935.html">Our Milky Way Galaxy Likely Underwent Disk Flip after Ancient Galactic Collision: Study</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>Puzzling Near-Earth Asteroid Turns Out to Be Comet with Weak Tail</title>
		<link>https://www.sci.news/astronomy/p-1998-sh2-comet-14933.html</link>
					<comments>https://www.sci.news/astronomy/p-1998-sh2-comet-14933.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Tue, 21 Jul 2026 19:21:38 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[1998 SH2]]></category>
		<category><![CDATA[Acceleration]]></category>
		<category><![CDATA[CFHT]]></category>
		<category><![CDATA[Comet]]></category>
		<category><![CDATA[Danish Telescope]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Near-Earth asteroid]]></category>
		<category><![CDATA[Near-Earth comet]]></category>
		<category><![CDATA[Near-Earth object]]></category>
		<category><![CDATA[Non-gravitational acceleration]]></category>
		<category><![CDATA[P/1998 SH2]]></category>
		<category><![CDATA[Solar System]]></category>
		<category><![CDATA[VLT]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110920</guid>

					<description><![CDATA[<div><img width="580" height="363" src="https://cdn.sci.news/images/2026/07/image_14933_1-1998-SH2.jpg" class="attachment-full size-full wp-post-image" alt="This artist’s concept depicts a near-Earth asteroid with an elongated orbit; a few objects such as these can exhibit significant perturbations in their motion around the Sun and, like 1998 SH2, could turn out to be regular comets with a weak tail and coma. Image credit: NASA / JPL-Caltech." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14933_1-1998-SH2.jpg 580w, https://cdn.sci.news/images/2026/07/image_14933_1-1998-SH2-300x188.jpg 300w, https://cdn.sci.news/images/2026/07/image_14933_1-1998-SH2-80x50.jpg 80w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>The near-Earth object (875163) 1998 SH2, which is currently classified as an asteroid, has revealed a hidden identity: it’s actually a comet in disguise, according to a new study published in the journal Nature Astronomy.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/p-1998-sh2-comet-14933.html">Puzzling Near-Earth Asteroid Turns Out to Be Comet with Weak Tail</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 Omega Centauri’s First Stellar-Mass Black Hole</title>
		<link>https://www.sci.news/astronomy/omega-centauris-first-stellar-mass-black-hole-14928.html</link>
					<comments>https://www.sci.news/astronomy/omega-centauris-first-stellar-mass-black-hole-14928.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Mon, 20 Jul 2026 15:56:16 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Binary star]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Globular cluster]]></category>
		<category><![CDATA[Hubble]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Omega Centauri]]></category>
		<category><![CDATA[oMEGACat BH-2]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Star cluster]]></category>
		<category><![CDATA[Stellar-mass black hole]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110895</guid>

					<description><![CDATA[<div><img width="580" height="580" src="https://cdn.sci.news/images/2026/07/image_14928-oMEGACat-BH-2.jpg" class="attachment-full size-full wp-post-image" alt="Whitaker et al. found Omega Centauri’s first stellar-mass black hole, which has a visible star companion that is shown in greater detail. Image credit: ESA / NASA / Maximilian Häberle, MPIA / Joseph DePasquale, STScI." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14928-oMEGACat-BH-2.jpg 580w, https://cdn.sci.news/images/2026/07/image_14928-oMEGACat-BH-2-300x300.jpg 300w, https://cdn.sci.news/images/2026/07/image_14928-oMEGACat-BH-2-150x150.jpg 150w, https://cdn.sci.news/images/2026/07/image_14928-oMEGACat-BH-2-50x50.jpg 50w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>After decades of searching, astronomers have pinpointed the first of an estimated 10,000 stellar-mass black holes thought to lurk in Omega Centauri, the most massive stellar system in the Milky Way found so far, with a stellar mass of 3.6 million solar masses.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/omega-centauris-first-stellar-mass-black-hole-14928.html">Astronomers Find Omega Centauri’s First Stellar-Mass 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>Potential Atmosphere Detected on Habitable-Zone Exoplanet LHS 1140b</title>
		<link>https://www.sci.news/astronomy/atmosphere-habitable-zone-exoplanet-lhs-1140b-14925.html</link>
					<comments>https://www.sci.news/astronomy/atmosphere-habitable-zone-exoplanet-lhs-1140b-14925.html#comments</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Thu, 16 Jul 2026 23:37:45 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Atmosphere]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Habitable zone]]></category>
		<category><![CDATA[Helium]]></category>
		<category><![CDATA[Las Campanas Observatory]]></category>
		<category><![CDATA[LHS 1140]]></category>
		<category><![CDATA[LHS 1140b]]></category>
		<category><![CDATA[M-dwarf star]]></category>
		<category><![CDATA[Magellan Clay telescope]]></category>
		<category><![CDATA[Red dwarf]]></category>
		<category><![CDATA[Spectrum]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[super-Earth]]></category>
		<category><![CDATA[WINERED]]></category>
		<category><![CDATA[X-rays]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110868</guid>

					<description><![CDATA[<div><img width="580" height="326" src="https://cdn.sci.news/images/2026/07/image_14925-LHS-1140.jpg" class="attachment-full size-full wp-post-image" alt="An artist’s concept of rocky planets LHS 1140b and LHS 1140c. Image credit: Melissa Weiss / Harvard &amp; Smithsonian’s Center for Astrophysics." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14925-LHS-1140.jpg 580w, https://cdn.sci.news/images/2026/07/image_14925-LHS-1140-300x169.jpg 300w, https://cdn.sci.news/images/2026/07/image_14925-LHS-1140-195x110.jpg 195w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Using spectral data from the Magellan Clay telescope at Las Campanas Observatory, astronomers detected helium escaping from LHS 1140b, a rocky exoplanet that orbits in the habitable zone of the nearby low-mass star LHS 1140.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/atmosphere-habitable-zone-exoplanet-lhs-1140b-14925.html">Potential Atmosphere Detected on Habitable-Zone Exoplanet LHS 1140b</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>Barnard’s Star Planetary System May Be Filled with Water-Poor Rocky Worlds</title>
		<link>https://www.sci.news/astronomy/barnards-star-planets-14924.html</link>
					<comments>https://www.sci.news/astronomy/barnards-star-planets-14924.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Thu, 16 Jul 2026 21:28:45 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Atmosphere]]></category>
		<category><![CDATA[Barnard’s star]]></category>
		<category><![CDATA[Barnard’s star b]]></category>
		<category><![CDATA[Barnard’s star c]]></category>
		<category><![CDATA[Barnard’s star d]]></category>
		<category><![CDATA[Barnard’s star e]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Habitability]]></category>
		<category><![CDATA[Magnesium]]></category>
		<category><![CDATA[Periclase]]></category>
		<category><![CDATA[Planetary system]]></category>
		<category><![CDATA[Red dwarf]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[sub-Earth]]></category>
		<category><![CDATA[Water]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110866</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2025/03/image_13740f-Barnards-Star.jpg" class="attachment-full size-full wp-post-image" alt="An artist’s illustration of exoplanets orbiting Barnard’s star. Image credit: International Gemini Observatory / NOIRLab / NSF / AURA / P. Marenfeld." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2025/03/image_13740f-Barnards-Star.jpg 710w, https://cdn.sci.news/images/2025/03/image_13740f-Barnards-Star-300x169.jpg 300w, https://cdn.sci.news/images/2025/03/image_13740f-Barnards-Star-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>A new analysis suggests the four sub-Earth exoplanets orbiting Barnard’s star -- the Sun’s nearest single-star neighbor -- are likely packed with the deep-Earth mineral periclase, stripped of their atmospheres and far too hostile to support life.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/barnards-star-planets-14924.html">Barnard’s Star Planetary System May Be Filled with Water-Poor Rocky Worlds</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 Gamma-Ray Burst’s Magnetic Fingerprint</title>
		<link>https://www.sci.news/astronomy/gamma-ray-bursts-magnetic-fingerprint-14921.html</link>
					<comments>https://www.sci.news/astronomy/gamma-ray-bursts-magnetic-fingerprint-14921.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 15 Jul 2026 22:42:14 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Faraday rotation]]></category>
		<category><![CDATA[Gamma-Ray Burst]]></category>
		<category><![CDATA[GRB 260310A]]></category>
		<category><![CDATA[Magnetic field]]></category>
		<category><![CDATA[NSF]]></category>
		<category><![CDATA[Polarization]]></category>
		<category><![CDATA[Polarized light]]></category>
		<category><![CDATA[Radio signal]]></category>
		<category><![CDATA[VLA]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110843</guid>

					<description><![CDATA[<div><img width="580" height="387" src="https://cdn.sci.news/images/2026/07/image_14921-GRB-260310A.jpg" class="attachment-full size-full wp-post-image" alt="This illustration depicts Faraday rotation in the afterglow of a gamma-ray burst. A powerful jet (upper left) sends polarized radio waves outward through the thin wall of a surrounding bubble of magnetized gas called an HII region. As the light passes through this material, its polarization angle is twisted by the magnetic field. Because the effect is stronger at longer wavelengths, the red and blue waves, which represent different radio wavelengths, exit the bubble oscillating in different directions. By measuring this difference, astronomers were able to map the magnetic environment surrounding GRB 260310A for the first time. Image credit: NSF / AUI / NRAO / M. Weiss" loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14921-GRB-260310A.jpg 580w, https://cdn.sci.news/images/2026/07/image_14921-GRB-260310A-300x200.jpg 300w, https://cdn.sci.news/images/2026/07/image_14921-GRB-260310A-84x55.jpg 84w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Using NSF’s Very Large Array (VLA), astronomers made the first radio detection of polarized light and Faraday rotation from a gamma-ray burst afterglow, offering an unprecedented glimpse of the magnetic fields surrounding one of the Universe’s most powerful explosions.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/gamma-ray-bursts-magnetic-fingerprint-14921.html">Astronomers Detect Gamma-Ray Burst’s Magnetic Fingerprint</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 Discover and Directly Image Third Planet in Beta Pictoris System</title>
		<link>https://www.sci.news/astronomy/third-planet-beta-pictoris-system-14920.html</link>
					<comments>https://www.sci.news/astronomy/third-planet-beta-pictoris-system-14920.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 15 Jul 2026 21:33:11 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[Beta Pictoris]]></category>
		<category><![CDATA[Beta Pictoris d]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Gas giant]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[VLT]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110837</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/07/image_14920f-Beta-Pictoris-.jpg" class="attachment-full size-full wp-post-image" alt="This artist’s concept shows the Beta Pictoris system with the discovered giant exoplanet Beta Pictoris d at the right. Image credit: NASA / ESA / CSA / STScI / Ralf Crawford, STScI." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14920f-Beta-Pictoris-.jpg 710w, https://cdn.sci.news/images/2026/07/image_14920f-Beta-Pictoris--300x169.jpg 300w, https://cdn.sci.news/images/2026/07/image_14920f-Beta-Pictoris--195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Named Beta Pictoris d, the newly-discovered world is 100 times fainter than Beta Pictoris b -- the first planet discovered around the A5-type star Beta Pictoris -- and is among the lightest exoplanets ever to be imaged from the ground.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/third-planet-beta-pictoris-system-14920.html">Astronomers Discover and Directly Image Third Planet in Beta Pictoris System</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 Catches Supermassive Black Hole Feeding from Cosmic Gas Streams</title>
		<link>https://www.sci.news/astronomy/webb-supermassive-black-hole-feeding-14916.html</link>
					<comments>https://www.sci.news/astronomy/webb-supermassive-black-hole-feeding-14916.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Tue, 14 Jul 2026 20:54:21 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Active galactic nucleus]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[Centaurus Cluster]]></category>
		<category><![CDATA[Circumnuclear disk]]></category>
		<category><![CDATA[CSA]]></category>
		<category><![CDATA[Elliptical galaxy]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[Filament]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Gas]]></category>
		<category><![CDATA[IR]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[NGC 4696]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[Webb]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110818</guid>

					<description><![CDATA[<div><img width="580" height="435" src="https://cdn.sci.news/images/2016/12/image_4416-NGC-4696.jpg" class="attachment-full size-full wp-post-image" alt="This Hubble image shows the elliptical galaxy NGC 4696. Image credit: NASA / ESA / Hubble / A. Fabian." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2016/12/image_4416-NGC-4696.jpg 580w, https://cdn.sci.news/images/2016/12/image_4416-NGC-4696-300x225.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>New images of the giant elliptical galaxy NGC 4696 from the NASA/ESA/CSA James Webb Space Telescope reveal gas filaments funneling material into a spinning disk around a supermassive black hole 800 light-years across.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/webb-supermassive-black-hole-feeding-14916.html">Webb Catches Supermassive Black Hole Feeding from Cosmic Gas Streams</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 Discover Four New White Dwarfs in Solar Neighborhood</title>
		<link>https://www.sci.news/astronomy/four-white-dwarfs-solar-neighborhood-14915.html</link>
					<comments>https://www.sci.news/astronomy/four-white-dwarfs-solar-neighborhood-14915.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Tue, 14 Jul 2026 15:45:17 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Binary star]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[G 203-47]]></category>
		<category><![CDATA[GJ 207.1]]></category>
		<category><![CDATA[Hubble]]></category>
		<category><![CDATA[LHS 1817]]></category>
		<category><![CDATA[NASA]]></category>
		<category><![CDATA[Red dwarf]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[STIS]]></category>
		<category><![CDATA[UV]]></category>
		<category><![CDATA[White dwarf]]></category>
		<category><![CDATA[Wolf 1130]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110815</guid>

					<description><![CDATA[<div><img width="580" height="394" src="https://cdn.sci.news/images/2026/07/image_14915-White-Dwarf.jpg" class="attachment-full size-full wp-post-image" alt="An artist’s impression of a red dwarf with a white dwarf binary companion peeking out from behind. Image credit: Mark A. Garlick / University of Warwick." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14915-White-Dwarf.jpg 580w, https://cdn.sci.news/images/2026/07/image_14915-White-Dwarf-300x204.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Using near-UV spectroscopic data from the Space Telescope Imaging Spectrograph (STIS) on the NASA/ESA Hubble Space Telescope, astronomers discovered four white dwarfs orbiting nearby red dwarf stars.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/four-white-dwarfs-solar-neighborhood-14915.html">Astronomers Discover Four New White Dwarfs in Solar Neighborhood</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 Sugar in Interstellar Space for First Time</title>
		<link>https://www.sci.news/astronomy/sugar-interstellar-space-14913.html</link>
					<comments>https://www.sci.news/astronomy/sugar-interstellar-space-14913.html#respond</comments>
		
		<dc:creator><![CDATA[Natali Anderson]]></dc:creator>
		<pubDate>Mon, 13 Jul 2026 19:54:35 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Featured]]></category>
		<category><![CDATA[Chiral molecule]]></category>
		<category><![CDATA[Chirality]]></category>
		<category><![CDATA[Erythrulose]]></category>
		<category><![CDATA[G+0.693-0.027]]></category>
		<category><![CDATA[Interstellar medium]]></category>
		<category><![CDATA[Interstellar space]]></category>
		<category><![CDATA[IRAM]]></category>
		<category><![CDATA[Milky Way]]></category>
		<category><![CDATA[Molecular cloud]]></category>
		<category><![CDATA[Radio signal]]></category>
		<category><![CDATA[Sugar]]></category>
		<category><![CDATA[Yebes Observatory]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110798</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2026/07/image_14913f-Erythrulose.jpg" class="attachment-full size-full wp-post-image" alt="This composite image of the Milky Way’s central region shows the location of the molecular cloud G+0.693-0.027. Image credit: Ashley Barnes / Izaskun Jiménez-Serra / Juan García de la Concepción." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14913f-Erythrulose.jpg 710w, https://cdn.sci.news/images/2026/07/image_14913f-Erythrulose-300x169.jpg 300w, https://cdn.sci.news/images/2026/07/image_14913f-Erythrulose-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Using the Yebes 40-m and IRAM 30-m radio telescopes, astronomers have discovered erythrulose, a four-carbon sugar commonly found in raspberries and sunless tanning cosmetics, in the molecular cloud G+0.693-0.027.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/sugar-interstellar-space-14913.html">Astronomers Detect Sugar in Interstellar Space for First Time</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 Uncover Hidden Structures Surrounding Orion Nebula</title>
		<link>https://www.sci.news/astronomy/hidden-structures-orion-nebula-14907.html</link>
					<comments>https://www.sci.news/astronomy/hidden-structures-orion-nebula-14907.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Fri, 10 Jul 2026 15:46:59 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Diffuse nebula]]></category>
		<category><![CDATA[FAST]]></category>
		<category><![CDATA[Filament]]></category>
		<category><![CDATA[Hydrogen]]></category>
		<category><![CDATA[M42]]></category>
		<category><![CDATA[Map]]></category>
		<category><![CDATA[Messier 42]]></category>
		<category><![CDATA[Nebula]]></category>
		<category><![CDATA[Neutral hydrogen]]></category>
		<category><![CDATA[NGC 1976]]></category>
		<category><![CDATA[Orion Nebula]]></category>
		<category><![CDATA[Radio signal]]></category>
		<category><![CDATA[Shell]]></category>
		<category><![CDATA[Star]]></category>
		<category><![CDATA[Star formation]]></category>
		<category><![CDATA[VLA]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110767</guid>

					<description><![CDATA[<div><img width="580" height="580" src="https://cdn.sci.news/images/2026/07/image_14907-Orion-Nebula.jpg" class="attachment-full size-full wp-post-image" alt="Extended Orion nebula shell sampled by HI emission from the combined VLA and FAST observations (shown in red), Hα emission from the European Southern Observatory Digitized Sky Survey (shown in green), and 3.4-μm emission registered by the Wide-field Infrared Survey Explorer (WISE) satellite (shown in blue). Image credit: Juan D. Soler, University of Vienna / NRAO / VLA / NASA / WISE." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14907-Orion-Nebula.jpg 580w, https://cdn.sci.news/images/2026/07/image_14907-Orion-Nebula-300x300.jpg 300w, https://cdn.sci.news/images/2026/07/image_14907-Orion-Nebula-150x150.jpg 150w, https://cdn.sci.news/images/2026/07/image_14907-Orion-Nebula-50x50.jpg 50w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Using the Karl G. Jansky Very Large Array (VLA) s and the Five-hundred-meter Aperture Spherical Radio Telescope (FAST), astronomers have created the sharpest-ever radio maps of neutral hydrogen around the Orion Nebula.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/hidden-structures-orion-nebula-14907.html">Astronomers Uncover Hidden Structures Surrounding Orion 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>Astronomers Probe Chemistry of Giant Exoplanet Beta Pictoris b</title>
		<link>https://www.sci.news/astronomy/beta-pictoris-b-chemistry-14905.html</link>
					<comments>https://www.sci.news/astronomy/beta-pictoris-b-chemistry-14905.html#respond</comments>
		
		<dc:creator><![CDATA[Enrico de Lazaro]]></dc:creator>
		<pubDate>Thu, 09 Jul 2026 15:02:27 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Atmosphere]]></category>
		<category><![CDATA[Beta Pictoris]]></category>
		<category><![CDATA[Beta Pictoris b]]></category>
		<category><![CDATA[Carbon]]></category>
		<category><![CDATA[Carbon monoxide]]></category>
		<category><![CDATA[Carbon-12]]></category>
		<category><![CDATA[Carbon-13]]></category>
		<category><![CDATA[ESO]]></category>
		<category><![CDATA[Exoplanet]]></category>
		<category><![CDATA[Gas giant]]></category>
		<category><![CDATA[Planet formation]]></category>
		<category><![CDATA[VLTI]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110749</guid>

					<description><![CDATA[<div><img width="710" height="401" src="https://cdn.sci.news/images/2018/08/image_6336f-Beta-Pictoris-b.jpg" class="attachment-full size-full wp-post-image" alt="This artist’s impression shows how the gas giant exoplanet inside the disc of Beta Pictoris may look. Image credit: L. Calçada / ESO." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2018/08/image_6336f-Beta-Pictoris-b.jpg 710w, https://cdn.sci.news/images/2018/08/image_6336f-Beta-Pictoris-b-300x169.jpg 300w, https://cdn.sci.news/images/2018/08/image_6336f-Beta-Pictoris-b-195x110.jpg 195w" sizes="(max-width: 710px) 100vw, 710px" /></div>
<p>Using the upgraded GRAVITY+ instrument on ESO’s Very Large Telescope Interferometer (VLTI), astronomers have measured the ratio of carbon isotopes in the atmosphere of the young exoplanet Beta Pictoris, offering new insights into how giant planets form.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/beta-pictoris-b-chemistry-14905.html">Astronomers Probe Chemistry of Giant Exoplanet Beta Pictoris b</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>Euclid Discovers Earliest Quasars Ever Seen</title>
		<link>https://www.sci.news/astronomy/euclid-earliest-quasars-14903.html</link>
					<comments>https://www.sci.news/astronomy/euclid-earliest-quasars-14903.html#respond</comments>
		
		<dc:creator><![CDATA[News Staff]]></dc:creator>
		<pubDate>Wed, 08 Jul 2026 21:56:24 +0000</pubDate>
				<category><![CDATA[Astronomy]]></category>
		<category><![CDATA[Active galactic nucleus]]></category>
		<category><![CDATA[Black hole]]></category>
		<category><![CDATA[Early Universe]]></category>
		<category><![CDATA[ESA]]></category>
		<category><![CDATA[EUCL J1253]]></category>
		<category><![CDATA[EUCL J1729]]></category>
		<category><![CDATA[Euclid]]></category>
		<category><![CDATA[Galaxy]]></category>
		<category><![CDATA[Quasar]]></category>
		<category><![CDATA[Supermassive black hole]]></category>
		<category><![CDATA[Universe]]></category>
		<guid isPermaLink="false">https://www.sci.news/?p=110737</guid>

					<description><![CDATA[<div><img width="580" height="346" src="https://cdn.sci.news/images/2026/07/image_14903-Euclid-Quasars.jpg" class="attachment-full size-full wp-post-image" alt="This collage shows 15 of the 31 newly discovered quasars by ESA’s Euclid space telescope. EUCL J172902.75+641018.1 and EUCL J125308.55+705432.3 are visible on the first row, the first and second from the left, respectively. Image credit: ESA / Euclid / Euclid Consortium / NASA / Euclid Science Ground Segment / Antoine Basset, CNES." loading="lazy" style="margin-bottom: 15px;" srcset="https://cdn.sci.news/images/2026/07/image_14903-Euclid-Quasars.jpg 580w, https://cdn.sci.news/images/2026/07/image_14903-Euclid-Quasars-300x179.jpg 300w" sizes="(max-width: 580px) 100vw, 580px" /></div>
<p>Astronomers using ESA’s Euclid space telescope have discovered 31 ancient quasars from a time when the Universe was just 670 to 800 million years old. One of these objects, dubbed EUCL J172902.75+641018.1, sets the new record for the most distant quasar ever reported.</p>
<p>The post <a rel="nofollow" href="https://www.sci.news/astronomy/euclid-earliest-quasars-14903.html">Euclid Discovers Earliest Quasars Ever Seen</a> appeared first on <a rel="nofollow" href="https://www.sci.news">Sci.News: Breaking Science News</a>.</p>
]]></description>
		
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