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						<h1 itemprop="headline">Ole Rømer Colloquium</h1>
						
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							<p class="text--intro" itemprop="description">Join us for the next Ole Rømer Colloquium where Prof. Jes Kristian Jørgensen from NBI will visit us.</p>
						
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									<h2 class="screenreader-only">Oplysninger om arrangementet</h2>

									
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												<h3 class="news-event__info__item__header text--label-header">Tidspunkt</h3>
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														Onsdag 27. november 2024,
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														&nbsp;kl. 14:00 -  15:15
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													<p class="news-event__info__item__ical-link"><a href="/aktuelt/nyhed/artikel/ole-roemer-colloquium-1?tx_news_pi1%5Bformat%5D=ical&amp;type=9819&amp;cHash=c4b0a2df6740e9b7d2bcaab59a5befd1">Tilføj til kalender</a></p>
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														<p>1523-318</p>
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													Af
												

											
													<a href="mailto:annakatrine@phys.au.dk">
														<span itemprop="name">Anna Katrine Mathiassen</span>
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									<p>His talk is titled:&nbsp;<em>Setting the Stage for Solar System Formation</em></p>
<p>Abstract: Over the last years significant advances have been made in our understanding of how and where stars and planets form and how they&nbsp;evolve during their earliest stages, both from a physical and chemical point of view. Deep observations of the gas and ice in the&nbsp;environments in which young stars form demonstrate that these regions are characterised by rich and varied chemistry with high&nbsp;abundances of complex organic molecules – some perhaps even of prebiotic relevance. At the same time, a picture has emerged where the&nbsp;first seeds for planets are planted in protoplanetary disks already during the first few 100,000 years after stars form. But what is the link&nbsp;between this complex chemistry and the structure of the newly formed protoplanetary disks – and does it have any implications for the&nbsp;origin and composition of planets outside of our own Solar System? In the colloquium I will discuss how our understanding of the earliest&nbsp;stages of star and planet formation has evolved over recent years. In particular, I will focus on how ALMA and JWST are helping to shed new&nbsp;light on how the properties of emerging protoplanetary disks reflect the evolution of protostars and conditions in their natal environments.</p>
								
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