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            <title>
									Astrovéga Club Forum - Posts Récents				            </title>
            <link>https://www.astrovega.be/astrovega-forum/</link>
            <description>Astrovéga Club Forum de discussion</description>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-382</link>
                        <pubDate>Wed, 13 May 2026 14:53:29 +0000</pubDate>
                        <description><![CDATA[GW190728Le signal gravitationnel GW190728 montrait peut-être l&#039;empreinte de la matière noire2029Des observations réalisées par Chandra montrent que l&#039;amas de galaxie Abell 2029 est encore en...]]></description>
                        <content:encoded><![CDATA[<p><span>GW190728</span><br /><br /><span>Le signal gravitationnel GW190728 montrait peut-être l'empreinte de la matière noire.</span><br /><br /><a href="https://news.mit.edu/2026/new-way-spot-signs-dark-matter-0512" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://news.mit.edu/2026/new-way-spot-signs-dark-matter-0512&amp;source=gmail&amp;ust=1778770165125000&amp;usg=AOvVaw0BUyaUSa9klImFHOTHjj_r">https://news.mit.edu/2026/new-<wbr />way-spot-signs-dark-matter-051<wbr />2</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Abell 2029</span><br /><br /><span>Des observations réalisées par Chandra montrent que l'amas de galaxie Abell 2029 est encore en train de se stabiliser après une violente collision avec un amas plus petit, il y a 4 milliards d'années.</span><br /><br /><a href="https://chandra.harvard.edu/photo/2026/a2029/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://chandra.harvard.edu/photo/2026/a2029/&amp;source=gmail&amp;ust=1778770165125000&amp;usg=AOvVaw3_i7bVOaBcl6RBXx3p_4B2">https://chandra.harvard.edu/ph<wbr />oto/2026/a2029/</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Soleil</span><br /><br /><span>Une nouvelle approche fondée sur l'intelligence artificielle permet de mieux « écouter » l'intérieur du Soleil.</span><br /><br /><a href="https://sheffield.ac.uk/mps/news/scientists-use-ai-interpret-suns-acoustic-heartbeat" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://sheffield.ac.uk/mps/news/scientists-use-ai-interpret-suns-acoustic-heartbeat&amp;source=gmail&amp;ust=1778770165125000&amp;usg=AOvVaw1vba3SA9SWJutbh3AoRICG">https://sheffield.ac.uk/mps/ne<wbr />ws/scientists-use-ai-interpret<wbr />-suns-acoustic-heartbeat</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-382</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-381</link>
                        <pubDate>Tue, 12 May 2026 09:47:48 +0000</pubDate>
                        <description><![CDATA[Toile cosmiqueLe JWST a permis d&#039;étabir la carte la plus détaillée d&#039;une partie de la toile cosmiquétudiant sa capacité à conserver une atmosphère, les chercheurs ont déterminé qu&#039;une planèt...]]></description>
                        <content:encoded><![CDATA[<p><span>Toile cosmique</span><br /><br /><span>Le JWST a permis d'étabir la carte la plus détaillée d'une partie de la toile cosmique</span><br /><br /><a href="https://news.ucr.edu/articles/2026/05/11/astronomers-produce-most-detailed-map-cosmic-web" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://news.ucr.edu/articles/2026/05/11/astronomers-produce-most-detailed-map-cosmic-web&amp;source=gmail&amp;ust=1778664252076000&amp;usg=AOvVaw35tXDS2JGwoP8MJm2hx4Li">https://news.ucr.edu/articles/<wbr />2026/05/11/astronomers-produce<wbr />-most-detailed-map-cosmic-web</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Habitabilité</span><br /><br /><span>En étudiant sa capacité à conserver une atmosphère, les chercheurs ont déterminé qu'une planète légèrement plus petite que la Terre ne permet probablement pas le développement de la vie.</span><br /><br /><a href="https://phys.org/news/2026-05-size-limit-habitable-exoplanets.html" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://phys.org/news/2026-05-size-limit-habitable-exoplanets.html&amp;source=gmail&amp;ust=1778664252076000&amp;usg=AOvVaw2WYQLgxU3fdMGicInCAUA-">https://phys.org/news/2026-05-<wbr />size-limit-habitable-exoplanet<wbr />s.html</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Effet papillon</span><br /><br /><span>Les modélisations de galaxies ne donnent pas toujours les mêmes résultats, même en  partant de conditions identiques. Une nouvelle étude de l'université de Leyde montre qu'il ne s'agit pas d'une faille, mais d'une conséquence du comportement des galaxies qui devient imprédictable après un million d'années.</span><br /><br /><a href="https://www.universiteitleiden.nl/en/news/2026/05/new-study-shows-how-a-single-star-can-reshape-an-entire-galaxy" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.universiteitleiden.nl/en/news/2026/05/new-study-shows-how-a-single-star-can-reshape-an-entire-galaxy&amp;source=gmail&amp;ust=1778664252076000&amp;usg=AOvVaw3-geQ7EFw2JeUsio4PlF3W">https://www.universiteitleiden<wbr />.nl/en/news/2026/05/new-study-<wbr />shows-how-a-single-star-can-<wbr />reshape-an-entire-galaxy</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-381</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-380</link>
                        <pubDate>Mon, 11 May 2026 13:47:33 +0000</pubDate>
                        <description><![CDATA[GanymèdeDe potentiels cryovolcans ont été identifiés sur Ganymède, en prévision de l&#039;arrivée de la sonde JUICEla poussière cosmique récoltée dans des glaces Antarctiques montre le passage de...]]></description>
                        <content:encoded><![CDATA[<p><span>Ganymède</span><br /><br /><span>De potentiels cryovolcans ont été identifiés sur Ganymède, en prévision de l'arrivée de la sonde JUICE.</span><br /><br /><a href="https://hsc.gov.gr/en/study-identifies-candidate-cryovolcanic-regions-on-ganymede-for-esas-juice-mission/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://hsc.gov.gr/en/study-identifies-candidate-cryovolcanic-regions-on-ganymede-for-esas-juice-mission/&amp;source=gmail&amp;ust=1778593134293000&amp;usg=AOvVaw0flxqXPTfAmcrac_ydHgBy">https://hsc.gov.gr/en/study-id<wbr />entifies-candidate-cryovolcani<wbr />c-regions-on-ganymede-for-<wbr />esas-juice-mission/</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Poussière</span><br /><br /><span>De la poussière cosmique récoltée dans des glaces Antarctiques montre le passage de notre système solaire dans un nuage contaminé par les supernovae.</span><br /><br /><a href="https://www.sciencealert.com/stardust-trapped-in-antarctic-ice-reveals-earths-journey-through-the-cosmos" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.sciencealert.com/stardust-trapped-in-antarctic-ice-reveals-earths-journey-through-the-cosmos&amp;source=gmail&amp;ust=1778593134293000&amp;usg=AOvVaw3QsGU-YZCUhZWS2Z5FeBIO">https://www.sciencealert.com/s<wbr />tardust-trapped-in-antarctic-i<wbr />ce-reveals-earths-journey-thro<wbr />ugh-the-cosmos</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Folklore spatial</span><br /><br /><span>Trump a fait publier divers rapports d'OVNIs et voilà que certains tentent de les lier aux anges (ou aux démons) plutôt qu'aux ETs - un peu d'originalité pour mettre du piment dans le débat...</span><br /><br /><a href="https://www.dailymail.com/sciencetech/article-15802807/ufo-files-eight-pointed-craft-angel-theory.html" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.dailymail.com/sciencetech/article-15802807/ufo-files-eight-pointed-craft-angel-theory.html&amp;source=gmail&amp;ust=1778593134293000&amp;usg=AOvVaw13QAPNPnizMuKC1JtyG9wc">https://www.dailymail.com/scie<wbr />ncetech/article-15802807/ufo-<wbr />files-eight-pointed-craft-ange<wbr />l-theory.html</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-380</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-379</link>
                        <pubDate>Sun, 10 May 2026 07:48:46 +0000</pubDate>
                        <description><![CDATA[CompositionL&#039;analyse des météorites suggère que la Terre s&#039;est formée presque exclusivement à partir de matériaux croisant dans le système solaire interne. De plus, la terre, Mars et Vesta p...]]></description>
                        <content:encoded><![CDATA[<p><span>Composition</span><br /><br /><span>L'analyse des météorites suggère que la Terre s'est formée presque exclusivement à partir de matériaux croisant dans le système solaire interne. De plus, la terre, Mars et Vesta partageraient des compositions similaires, mais pas Vénus ou Mercure.</span><br /><br /><a href="https://www.skyatnightmagazine.com/news/earth-formed-from-same-material-as-mars" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.skyatnightmagazine.com/news/earth-formed-from-same-material-as-mars&amp;source=gmail&amp;ust=1778485211890000&amp;usg=AOvVaw2tSssX8d4E664maMdAI9ch">https://www.skyatnightmagazine<wbr />.com/news/earth-formed-from-<wbr />same-material-as-mars</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>XMM-VID1-2075</span><br /><br /><span>Le JWST révèle que XMM-VID1-2075, l'une des plus grosses galaxies de l'univers jeune ne tourne pas, sans doute formée par la collision de deux galaxies tournant en sens opposés.</span><br /><br /><a href="https://www.ucdavis.edu/news/non-rotating-early-galaxy-surprise-astronomers" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.ucdavis.edu/news/non-rotating-early-galaxy-surprise-astronomers&amp;source=gmail&amp;ust=1778485211890000&amp;usg=AOvVaw092G7FF3veLFdWPzXmsfOj">https://www.ucdavis.edu/news/n<wbr />on-rotating-early-galaxy-surpr<wbr />ise-astronomers</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-379</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-378</link>
                        <pubDate>Fri, 08 May 2026 14:00:11 +0000</pubDate>
                        <description><![CDATA[Amas stellairesL&#039;observation avec Hubble et Webb de nombreux amas stellaires dans plusieurs galaxies, montre que les amas massifs émergent plus rapidement que les autres de leurs nuages nata...]]></description>
                        <content:encoded><![CDATA[<p><span>Amas stellaires</span><br /><br /><span>L'observation avec Hubble et Webb de nombreux amas stellaires dans plusieurs galaxies, montre que les amas massifs émergent plus rapidement que les autres de leurs nuages natals.</span><br /><br /><a href="https://www.esa.int/Science_Exploration/Space_Science/Webb/Webb_Hubble_find_massive_star_clusters_emerge_faster" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.esa.int/Science_Exploration/Space_Science/Webb/Webb_Hubble_find_massive_star_clusters_emerge_faster&amp;source=gmail&amp;ust=1778334984528000&amp;usg=AOvVaw1RyoD9lvwmLmdXuRnUcqmc">https://www.esa.int/Science_Ex<wbr />ploration/Space_Science/Webb/<wbr />Webb_Hubble_find_massive_star_<wbr />clusters_emerge_faster</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Premières galaxies</span><br /><br /><span>De nouvelles observations par le JWST montrent que les vents extrêmes à l'échelle des galaxies étaient courants parmi les premiers quasars, entravant la formation stellaire plus tôt qu'on ne l'imaginait.</span><br /><br /><a href="https://www.ncl.ac.uk/press/articles/latest/2026/05/quasaroutflows/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.ncl.ac.uk/press/articles/latest/2026/05/quasaroutflows/&amp;source=gmail&amp;ust=1778334984528000&amp;usg=AOvVaw3Fk7jBWdFJoFY4cWoTHdAx">https://www.ncl.ac.uk/press/ar<wbr />ticles/latest/2026/05/quasarou<wbr />tflows/</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Rayons cosmiques</span><br /><br /><span>Certains des rayons cosmiques les plus énergétiques pourraient être constitués de noyaux atomiques plus lourds que le fer.</span><br /><br /><a href="https://www.psu.edu/news/eberly-college-science/story/ultrahigh-energy-cosmic-messengers-may-carry-ultraheavy-secrets" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.psu.edu/news/eberly-college-science/story/ultrahigh-energy-cosmic-messengers-may-carry-ultraheavy-secrets&amp;source=gmail&amp;ust=1778334984528000&amp;usg=AOvVaw0lBVHxgddFOXsP5fV7eKmX">https://www.psu.edu/news/eberl<wbr />y-college-science/story/ultrah<wbr />igh-energy-cosmic-messengers-<wbr />may-carry-ultraheavy-secrets</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Ganymède</span><br /><br /><span>Le coeur métallique de Ganymède est toujours en cours de formation, ce qui expliquerait son champ magnétique.</span><br /><br /><a href="https://www.science.org/content/article/core-solar-system-s-largest-moon-may-still-be-forming" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.science.org/content/article/core-solar-system-s-largest-moon-may-still-be-forming&amp;source=gmail&amp;ust=1778334984528000&amp;usg=AOvVaw0n3rgWlZGoxMEKSo2XPO-Q">https://www.science.org/conten<wbr />t/article/core-solar-system-s-<wbr />largest-moon-may-still-be-<wbr />forming</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>neutrinos</span><br /><br /><span>La distribution en énergie des neutrinos cosmiques aurait un tournant vers 30TeV. Reste à comprendre pourquoi.</span><br /><br /><a href="https://physicsworld.com/a/gap-in-neutrino-energy-spectrum-raises-questions-about-cosmic-environments/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://physicsworld.com/a/gap-in-neutrino-energy-spectrum-raises-questions-about-cosmic-environments/&amp;source=gmail&amp;ust=1778334984528000&amp;usg=AOvVaw2JAX43zr8-QB2gwSqwOw5V">https://physicsworld.com/a/gap<wbr />-in-neutrino-energy-spectrum-<wbr />raises-questions-about-cosmic-<wbr />environments/</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/19/#post-378</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-377</link>
                        <pubDate>Wed, 06 May 2026 11:14:32 +0000</pubDate>
                        <description><![CDATA[OI-1130Les observations par le JWST de TOI-1130 b et c, une Jupiter chaude et une mini-Neptune, suggèrent que ces deux planètes se sont formées étonnamment loin de leur étoile hôtebrunesAvec...]]></description>
                        <content:encoded><![CDATA[<p><span>OI-1130</span><br /><br /><span>Les observations par le JWST de TOI-1130 b et c, une Jupiter chaude et une mini-Neptune, suggèrent que ces deux planètes se sont formées étonnamment loin de leur étoile hôte.</span><br /><br /><a href="https://news.mit.edu/2026/astronomers-pin-down-origins-planetary-odd-couple-0505" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://news.mit.edu/2026/astronomers-pin-down-origins-planetary-odd-couple-0505&amp;source=gmail&amp;ust=1778152397720000&amp;usg=AOvVaw0gifnWHid8a0Mjbly1Pq30">https://news.mit.edu/2026/astr<wbr />onomers-pin-down-origins-plane<wbr />tary-odd-couple-0505</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Naines brunes</span><br /><br /><span>Avec 3000 découvertes au cours de la dernière décennie, le projet citoyen/participatif "Backyard Worlds: Planet 9" a doublé le nombre de naines brunes connues.</span><br /><br /><a href="https://science.nasa.gov/get-involved/citizen-science/nasa-volunteers-double-known-population-of-brown-dwarfs/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://science.nasa.gov/get-involved/citizen-science/nasa-volunteers-double-known-population-of-brown-dwarfs/&amp;source=gmail&amp;ust=1778152397720000&amp;usg=AOvVaw02fMEUecJ8bmY5RHcc668b">https://science.nasa.gov/get-i<wbr />nvolved/citizen-science/nasa-v<wbr />olunteers-double-known-populat<wbr />ion-of-brown-dwarfs/</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Simulation cosmologique</span><br /><br /><span>La simulation ColdSIM montre comment se forment les premières étoiles et confirment le taux élevé de formation: le changement de température de l'univers rend les conditions fort différentes de ce qui se produit après ces premières étapes.</span><br /><br /><a href="https://www.space.com/astronomy/galaxies/why-were-galaxies-so-active-in-the-early-universe-we-may-be-getting-close-to-the-answer" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.space.com/astronomy/galaxies/why-were-galaxies-so-active-in-the-early-universe-we-may-be-getting-close-to-the-answer&amp;source=gmail&amp;ust=1778152397720000&amp;usg=AOvVaw0PuR-9sE580EVXH8zX8l2q">https://www.space.com/astronom<wbr />y/galaxies/why-were-galaxies-<wbr />so-active-in-the-early-<wbr />universe-we-may-be-getting-<wbr />close-to-the-answer</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Tourne pas</span><br /><br /><span>La galaxie XMM-VID1-2075 a été observée par le JWST. Elle n'a pas de rotation globale, alors qu'elle est encore jeune, ce qui n'est pas attendu.</span><br /><br /><a href="https://www.ucdavis.edu/news/non-rotating-early-galaxy-surprise-astronomers" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.ucdavis.edu/news/non-rotating-early-galaxy-surprise-astronomers&amp;source=gmail&amp;ust=1778152397720000&amp;usg=AOvVaw1Vhj4WCLCVp_xLhTwtALdI">https://www.ucdavis.edu/news/n<wbr />on-rotating-early-galaxy-surpr<wbr />ise-astronomers</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-376</link>
                        <pubDate>Tue, 05 May 2026 08:24:59 +0000</pubDate>
                        <description><![CDATA[LHS 3844 bLes observations par le JWST ont permis de conclure que la surface de la super-Terre LHS 3844 b ressemble à celle de la Lune ou de MercureXV93L&#039;objet trans-neptunien (612533) 2002 ...]]></description>
                        <content:encoded><![CDATA[<p><span>LHS 3844 b</span><br /><br /><span>Les observations par le JWST ont permis de conclure que la surface de la super-Terre LHS 3844 b ressemble à celle de la Lune ou de Mercure.</span><br /><br /><a href="https://www.mpg.de/26189037/astronomers-explore-the-surface-composition-of-a-nearby-super-earth" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.mpg.de/26189037/astronomers-explore-the-surface-composition-of-a-nearby-super-earth&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw352KBL_3MR2ZQAF8VI4asR">https://www.mpg.de/26189037/as<wbr />tronomers-explore-the-surface-<wbr />composition-of-a-nearby-super-<wbr />earth</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>2002 XV93</span><br /><br /><span>L'objet trans-neptunien (612533) 2002 XV93 - un "plutino" - possède une atmosphère très ténue.</span><br /><br /><a href="https://www.cbsnews.com/news/mysterious-world-beyond-pluto-atmosphere-study/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.cbsnews.com/news/mysterious-world-beyond-pluto-atmosphere-study/&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw3ktPeqF56gFDq9JjXGcfCn">https://www.cbsnews.com/news/m<wbr />ysterious-world-beyond-pluto-a<wbr />tmosphere-study/</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Particule</span><br /><br /><span>Des mesures au LHCb viennent confirmer des mesures précédentes au CMS: il y aurait une petite différence entre les mesures et le modèle standard - à confirmer et expliquer...</span><br /><br /><a href="https://theconversation.com/une-anomalie-au-lhc-laisse-entrevoir-une-percee-majeure-en-physique-des-particules-281164" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://theconversation.com/une-anomalie-au-lhc-laisse-entrevoir-une-percee-majeure-en-physique-des-particules-281164&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw1lTOm-wMKXv2KbnRvS0A32">https://theconversation.com/un<wbr />e-anomalie-au-lhc-laisse-entre<wbr />voir-une-percee-majeure-en-<wbr />physique-des-particules-281164</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Exoplanètes</span><br /><br /><span>On connaît 18 cas de planètes circumbinaires, en voilà 27 de plus, trouvées grâce à TESS. L'annonce ne s'est pas faite par hasard - des planètes genre Tatooine pour le "jour de la force" (May 4th)...</span><br /><br /><a href="https://science.nasa.gov/missions/tess/for-nasas-tess-stellar-eclipses-shed-light-on-possible-new-worlds/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://science.nasa.gov/missions/tess/for-nasas-tess-stellar-eclipses-shed-light-on-possible-new-worlds/&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw1Pyf6y3RGjNVGC-LAwe8os">https://science.nasa.gov/missi<wbr />ons/tess/for-nasas-tess-stella<wbr />r-eclipses-shed-light-on-<wbr />possible-new-worlds/</a><br /><a href="https://www.smithsonianmag.com/smart-news/astronomers-discover-27-potential-planets-each-orbiting-two-stars-just-like-the-fictional-tatooine-in-star-wars-180988667/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.smithsonianmag.com/smart-news/astronomers-discover-27-potential-planets-each-orbiting-two-stars-just-like-the-fictional-tatooine-in-star-wars-180988667/&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw26vHMnRSleS75jtOqo1hl9">https://www.smithsonianmag.com<wbr />/smart-news/astronomers-discov<wbr />er-27-potential-planets-each-<wbr />orbiting-two-stars-just-like-<wbr />the-fictional-tatooine-in-<wbr />star-wars-180988667/</a><br /><a href="https://news.unsw.edu.au/en/almost-30-real-life-tatooine-planet-candidates-discovered" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://news.unsw.edu.au/en/almost-30-real-life-tatooine-planet-candidates-discovered&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw2GHmlcqRuvyWcSXVsUHnwj">https://news.unsw.edu.au/en/al<wbr />most-30-real-life-tatooine-pla<wbr />net-candidates-discovered</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Vieil observatoire</span><br /><br /><span>Le village d'Aspéro, dans la zone archéologique de Caral, possède une série de plates-formes désormais considérées comme des observatoires primitifs.</span><br /><br /><a href="https://www.theartnewspaper.com/2026/04/30/ancient-astronomical-observatory-peru" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.theartnewspaper.com/2026/04/30/ancient-astronomical-observatory-peru&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw2zAxtlTgEUNTJaV50mJmVH">https://www.theartnewspaper.co<wbr />m/2026/04/30/ancient-astronomi<wbr />cal-observatory-peru</a><br /><a href="https://www.gob.pe/institucion/cultura/noticias/1381248-civilizacion-caral-descubren-en-aspero-estructura-vinculada-a-la-observacion-astronomica" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.gob.pe/institucion/cultura/noticias/1381248-civilizacion-caral-descubren-en-aspero-estructura-vinculada-a-la-observacion-astronomica&amp;source=gmail&amp;ust=1778055523914000&amp;usg=AOvVaw3g9qWusHq9Gj7yUixmPgu_">https://www.gob.pe/institucion<wbr />/cultura/noticias/1381248-<wbr />civilizacion-caral-descubren-<wbr />en-aspero-estructura-<wbr />vinculada-a-la-observacion-<wbr />astronomica</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-376</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-375</link>
                        <pubDate>Mon, 04 May 2026 14:39:42 +0000</pubDate>
                        <description><![CDATA[Matériau utileUn nouveau matériau a été trouvé pour bloquer les radiations et il est fin, un atout non négligeable pour les sondes et vaisseaux spatiauxmieux comprendre les éruptions solaire...]]></description>
                        <content:encoded><![CDATA[<p><span>Matériau utile</span><br /><br /><span>Un nouveau matériau a été trouvé pour bloquer les radiations et il est fin, un atout non négligeable pour les sondes et vaisseaux spatiaux.</span><br /><br /><a href="https://www.eurekalert.org/news-releases/1125238" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.eurekalert.org/news-releases/1125238&amp;source=gmail&amp;ust=1777991220905000&amp;usg=AOvVaw37mE20W4nAKYkOjkVx27cn">https://www.eurekalert.org/new<wbr />s-releases/1125238</a><br /><a href="https://www.space.com/technology/thinner-than-a-hair-and-stretchy-like-rubber-new-material-could-shield-against-radiation-in-next-gen-space-tech" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.space.com/technology/thinner-than-a-hair-and-stretchy-like-rubber-new-material-could-shield-against-radiation-in-next-gen-space-tech&amp;source=gmail&amp;ust=1777991220905000&amp;usg=AOvVaw0h93aBsJzGQf2se6nQw1O8">https://www.space.com/technolo<wbr />gy/thinner-than-a-hair-and-<wbr />stretchy-like-rubber-new-<wbr />material-could-shield-against-<wbr />radiation-in-next-gen-space-<wbr />tech</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Soleil</span><br /><br /><span>Pour mieux comprendre les éruptions solaires, des astronomes se sont concentrés sur le comportement des rubans de plasma (et notamment leurs bords).</span><br /><br /><a href="https://nso.edu/blog/reading-the-suns-fireworks-how-flare-ribbons-reveal-hidden-solar-explosions/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://nso.edu/blog/reading-the-suns-fireworks-how-flare-ribbons-reveal-hidden-solar-explosions/&amp;source=gmail&amp;ust=1777991220905000&amp;usg=AOvVaw0HnjAhg9tp9N_1wXVQtQS3">https://nso.edu/blog/reading-t<wbr />he-suns-fireworks-how-flare-ri<wbr />bbons-reveal-hidden-solar-expl<wbr />osions/</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-375</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-374</link>
                        <pubDate>Fri, 01 May 2026 07:01:00 +0000</pubDate>
                        <description><![CDATA[Rayons cosmiquesLe satellite DAMPE a permis de préciser les caractéristiques spectrales des cinq noyaux principaux de rayons cosmiques primaires, confirmant le modèle d&#039;accélération dépendan...]]></description>
                        <content:encoded><![CDATA[<p><span>Rayons cosmiques</span><br /><br /><span>Le satellite DAMPE a permis de préciser les caractéristiques spectrales des cinq noyaux principaux de rayons cosmiques primaires, confirmant le modèle d'accélération dépendant de la charge proposé dès les années 1960, et offrant un indice essentiel pour résoudre le mystère de leur origine.</span><br /><br /><a href="https://english.cas.cn/newsroom/research-news/202604/t20260430_1158281.shtml" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://english.cas.cn/newsroom/research-news/202604/t20260430_1158281.shtml&amp;source=gmail&amp;ust=1777704180869000&amp;usg=AOvVaw3VDzMxl_ecNtZI5aLJbdZe">https://english.cas.cn/newsroo<wbr />m/research-news/202604/t202604<wbr />30_1158281.shtml</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Pétaétron</span><br /><br /><span>L'observatoire LHAASO (Large High Altitude Air Shower Observatory) a détecté un rayonnement gamma de l'ordre du pétaélectronvolt provenant de la nébuleuse "à vent de pulsar"  PSR J1849-0001. Ce nouveau pétaétron remet en question la théorie classique de l'accélération des particules dans ces nébuleuses.</span><br /><br /><a href="https://english.cas.cn/research/platforms/large-research-infrastructures/particle-and-nuclear-physics/lhaaso/202604/t20260422_1157829.shtml" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://english.cas.cn/research/platforms/large-research-infrastructures/particle-and-nuclear-physics/lhaaso/202604/t20260422_1157829.shtml&amp;source=gmail&amp;ust=1777704180869000&amp;usg=AOvVaw3oq3zysWQxlqsCrG3NGfy2">https://english.cas.cn/researc<wbr />h/platforms/large-research-<wbr />infrastructures/particle-and-<wbr />nuclear-physics/lhaaso/202604/<wbr />t20260422_1157829.shtml</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-374</guid>
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                        <title>RE: Astro Océano Géo ELG Newsletter</title>
                        <link>https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-373</link>
                        <pubDate>Thu, 30 Apr 2026 07:33:10 +0000</pubDate>
                        <description><![CDATA[Amas stellairesLa masse d&#039;un amas stellaire est corrélée à la masse de ses étoiles les plus brillantesd&#039;OrionDes mesures radio ont permis d&#039;estimer la masse d&#039;étoiles jeunes de la région de ...]]></description>
                        <content:encoded><![CDATA[<p><span>Amas stellaires</span><br /><br /><span>La masse d'un amas stellaire est corrélée à la masse de ses étoiles les plus brillantes.</span><br /><br /><a href="https://www.uni-bonn.de/en/news/cosmic-order-inside-star-clusters" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.uni-bonn.de/en/news/cosmic-order-inside-star-clusters&amp;source=gmail&amp;ust=1777620024155000&amp;usg=AOvVaw2Pa8kuE8SRGpuu6CvuUe5N">https://www.uni-bonn.de/en/new<wbr />s/cosmic-order-inside-star-clu<wbr />sters</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Complexe d'Orion</span><br /><br /><span>Des mesures radio ont permis d'estimer la masse d'étoiles jeunes de la région de formation stellaire d'Orion.</span><br /><br /><a href="https://public.nrao.edu/news/unraveling-the-mass-mystery/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://public.nrao.edu/news/unraveling-the-mass-mystery/&amp;source=gmail&amp;ust=1777620024155000&amp;usg=AOvVaw0fj-R8wa8N6u9wk1BBVerT">https://public.nrao.edu/news/u<wbr />nraveling-the-mass-mystery/</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Galaxies naines</span><br /><br /><span>Des simulations montrent comment les galaxies naines ultra-faibles peuvent refléter les conditions de l'univers primitif et expliquer pourquoi certaines galaxies se sont développées, et d'autres pas.</span><br /><br /><a href="https://www.ras.ac.uk/news-and-press/news/milky-ways-little-cousins-may-hold-clues-about-infant-universe" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.ras.ac.uk/news-and-press/news/milky-ways-little-cousins-may-hold-clues-about-infant-universe&amp;source=gmail&amp;ust=1777620024155000&amp;usg=AOvVaw31oQ0nETQmABg0hp2zIq9_">https://www.ras.ac.uk/news-and<wbr />-press/news/milky-ways-little-<wbr />cousins-may-hold-clues-about-<wbr />infant-universe</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Formation planétaire</span><br /><br /><span>Les planètes se formeraient plus facilement autour d'étoiles doubles que d'étoiles simples, mais assez loin et ce seraient des géantes gazeuses.</span><br /><br /><a href="https://www.lancashire.ac.uk/news/two-suns-are-better-than-one" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.lancashire.ac.uk/news/two-suns-are-better-than-one&amp;source=gmail&amp;ust=1777620024155000&amp;usg=AOvVaw0vyB5ZYbNk6OG-Z1DzhW5e">https://www.lancashire.ac.uk/n<wbr />ews/two-suns-are-better-than-o<wbr />ne</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>X-ray dot</span><br /><br /><span>3DHST-AEGIS-12014, distant de 11,8 milliards d'années-lumière, serait un maillon essentiel entre trous noirs stellaires et trous noirs supermassifs en phase de croissance. Il présente la plupart des caractéristiques des LRD (Little Red Dot) mais émet des rayons X.</span><br /><br /><a href="https://chandra.si.edu/press/26_releases/press_042826.html" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://chandra.si.edu/press/26_releases/press_042826.html&amp;source=gmail&amp;ust=1777620024155000&amp;usg=AOvVaw2s_HE6gz9eFlzHbgfmsDp4">https://chandra.si.edu/press/2<wbr />6_releases/press_042826.html</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Cosmologie</span><br /><br /><span>Le projet FLAMINGO a publié l'un des plus vastes ensembles de simulations cosmologiques visant à modéliser l'évolution de la matière dans l'univers.</span><br /><br /><a href="https://www.astronomie.nl/nieuws/en/astronomers-release-massive-set-of-virtual-universes-for-global-research-4815" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.astronomie.nl/nieuws/en/astronomers-release-massive-set-of-virtual-universes-for-global-research-4815&amp;source=gmail&amp;ust=1777620024156000&amp;usg=AOvVaw0-dhNNm9F0jgL3TDU78PVu">https://www.astronomie.nl/nieu<wbr />ws/en/astronomers-release-mass<wbr />ive-set-of-virtual-universes-<wbr />for-global-research-4815</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Rotation</span><br /><br /><span>Des simulations montrent comment les champs magnétiques dans la zone de convection déterminent l'évolution de la rotation des étoiles massives.</span><br /><br /><a href="https://www.kyoto-u.ac.jp/en/research-news/2026-04-28-0" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.kyoto-u.ac.jp/en/research-news/2026-04-28-0&amp;source=gmail&amp;ust=1777620024156000&amp;usg=AOvVaw0c5KNQLH6ula99yvi38qAH">https://www.kyoto-u.ac.jp/en/r<wbr />esearch-news/2026-04-28-0</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Flares</span><br /><br /><span>Les observations par NICER et Hisaki de UX Arietis lors d'un superflare permettent d'attribuer l'origine de la raie X du fer, dite  "K-alpha", à la photoionisation.</span><br /><br /><a href="https://www.kyoto-u.ac.jp/en/research-news/2026-04-28" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://www.kyoto-u.ac.jp/en/research-news/2026-04-28&amp;source=gmail&amp;ust=1777620024156000&amp;usg=AOvVaw1Nu0wa_iGGFgAaqjNdzWI_">https://www.kyoto-u.ac.jp/en/r<wbr />esearch-news/2026-04-28</a><br /><br /><span>------------------------------</span><wbr /><span>------------------------------</span><wbr /><span>--------------</span><br /><br /><span>Formation planétaire</span><br /><br /><span>Les données de TESS révèlent que les naines M de stade intermédiaire à avancé abritent de nombreuses super-Terres, mais pratiquement aucune sous-Neptune, une découverte qui remet en question les théories actuelles sur la formation des planètes.</span><br /><br /><a href="https://news.mcmaster.ca/new-findings-about-exoplanets-challenge-theories-of-planet-formation/" target="_blank" rel="noopener noreferrer" data-saferedirecturl="https://www.google.com/url?q=https://news.mcmaster.ca/new-findings-about-exoplanets-challenge-theories-of-planet-formation/&amp;source=gmail&amp;ust=1777620024156000&amp;usg=AOvVaw1Ep4czZjphYzvX47udxiTX">https://news.mcmaster.ca/new-f<wbr />indings-about-exoplanets-chall<wbr />enge-theories-of-planet-format<wbr />ion/</a></p>]]></content:encoded>
						                            <category domain="https://www.astrovega.be/astrovega-forum/"></category>                        <dc:creator>Raoul Lannoy</dc:creator>
                        <guid isPermaLink="true">https://www.astrovega.be/astrovega-forum/astronomie/astro-oceano-geo-elg-newsletter/paged/18/#post-373</guid>
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