BEGIN:VCALENDAR
VERSION:2.0
PRODID:-//TYPO3/NONSGML News system (news)//EN
BEGIN:VEVENT
UID:news-34235@phys.au.dk
DTSTAMP:20210928T103045Z
DTSTART:20170112T151500Z
DTEND:20170112T160000Z
END:VEVENT
END:VCALENDAR




<div class="news news-single">
	<div class="article" itemscope="itemscope" itemtype="http://schema.org/Article">
		
	
			<script type="text/javascript">
				const showAllContentLangToken = "Show all content ";
			</script>

			
			

			<article class="typo3-delphinus delphinus-gutters">

				<!-- News PID: 83035 - used for finding folder/page which contains the news / event -->
				<!-- News UID: 34235 - the ID of the current news / event-->

				<div class="news-event">
					<div class="news-event__header">
						<!-- Categories -->
						
							<span class="text--stamp">
<!-- categories -->
<span class="news-list-category">
	
		
	
		
	
		
	
		
	
</span>

</span>
						

						<!-- Title -->
						<h1 itemprop="headline">SAC Seminar - Matthew Kenworthy: Observing Hill Sphere-filling Exoring Systems around the exoplanets J1407b and beta Pictoris b</h1>
						
					</div>

					

					<div class="news-event__content">

						<!-- Events info box -->
						
								

								<div class="news-event__info theme--dark" id="event-info">
									<h2 class="screenreader-only">Info about event</h2>

									
											<!--- Same date -->
											<div class="news-event__info__item news-event__info__item--time">
												<h3 class="news-event__info__item__header text--label-header">Time</h3>
												<div class="news-event__info__item__content">
													<span class="u-avoid-wrap">
														Thursday 12  January 2017,
													</span>
													<span class="u-avoid-wrap">
														&nbsp;at 16:15 -  17:00
													</span>
													<p class="news-event__info__item__ical-link"><a href="/en/news/item?tx_news_pi1%5Baction%5D=detail&amp;tx_news_pi1%5Bcontroller%5D=News&amp;tx_news_pi1%5Bformat%5D=ical&amp;tx_news_pi1%5Bnews%5D=34235&amp;type=9819&amp;cHash=224234539e92b831dcc6fdfbb9a92fbd">Add to calendar</a></p>
												</div>
											</div>
										

									<!-- Location detailed -->
									
											<!-- Location Simple -->
											
												<div class="news-event__info__item">
													<h3 class="news-event__info__item__header text--label-header">Location</h3>
													<div class="news-event__info__item__content">
														<p>1520-732</p>
													</div>
												</div>
											
										

									<!-- Organizer detailed -->
									
											<!-- Organizer Simple -->
											
										

									<!-- Price -->
									

									<!-- Event link -->
									

									<!-- Registration -->
									
								</div>
							

						
							<!-- Media -->
							
								



							
						

						
							<div class="news-event__content__text">
								<span class="text--byline" id="byline">
									

									<!-- Author -->
									
										<span itemprop="author" itemscope="itemscope" itemtype="http://schema.org/Person">
											
													By
												

											
													<a href="mailto:louise@phys.au.dk">
														<span itemprop="name">Louise Børsen-Koch</span>
													</a>
												
										</span>
									
								</span>

								

									<!-- Body text -->
									<p>In 2007, the 20 million year old pre-main sequence star J1407 underwent a complex series of eclipses lasting two months, showing temporal structure down to a timescale of 20 minutes. We interpret this as a giant ring system surrounding an unseen secondary companion, J1407b, that is being sculpted by forming exomoons. This ring system fills most of the Hill sphere and is 200 times larger than Saturn's rings.<br><br>In mid-2017, the Hill sphere of the young exoplanet orbiting the bright southern hemisphere star beta Pictoris will transit, presenting a unique opportunity to search for Hill sphere filling rings and to perform transmission spectroscopy of the circumplanetary material.<br><br>I will present our latest observations on J1407 and our observing campaign for beta Pictoris in 2017, including our bRing cameras that will carry out continuous monitoring of this star throughout the next 14 months.</p>
								
							</div>
						
					</div>

					
						<!-- Content elements -->
						
					
				</div>
			</article>

			
				
				
			

			<!-- related things -->
			
		

	</div>
</div>
