Monitoring ice-calving at the Astrolabe glacier (Antarctica) with seismological and optical satellite

<p><span>Better understanding the behaviour of tidewater outlet glaciers fringing marine ice sheets is of paramount importance to simulate Antarctica&#8216;s future response to global warming. Addressing the processes underlying these glaciers dynamics (ice motion, crack propagation, basal melting, sea ice interaction, calving events, etc) is a mean of constraining their ice discharge to the sea and hence the ice sheet global mass balance. </span><span>We here focus on the Astrolable glacier located in Terre Ad</span><span>&#233;</span>lie (140<span>&#176;</span>E, 67<span>&#176;</span><span>S) near the Dumont d'Urville French research station. </span><span>In January 2019,</span><span> a large crack of around 3km length was observed in the western shore of the glacier potentially leading to a calving of ca. 28 km</span>²<span>.The fissure has progressively grown until November 2021 when an iceberg of 20km</span>^{<span>2</span>}<span> was eventually released.&#160;</span></p><p><span>The location of the glacier outlet at the proximity of the Dumont D</span><span>&#8217;</span><span>Urville French research station is an asset to collect in-situ observations such as GNSS surveys and seismic monitoring. Satellite optical imagery also provides numerous acquisitions from the early nineties till the end of 2021 thanks to the Landsat and Sentinel-2 missions. </span><span>We used two monitoring techniques: optical remote sensing and seismology to analyze changes in the activity of the glacier</span><span> outlet</span><span>. We computed the </span><span>displacement of the ice </span><span>surface</span><span> with MPIC-OPT-ICE service available on the ESA Geohazards Exploitation Platform (GEP) and derived the</span><span> velocity and strain rates from </span><span>the archive</span><span> of multispectral Sentinel-2 imagery</span><span> from 2017 to the end of 2021</span>. <span>The images of the Landsat mission are used to map the limit of the ice front in order to retrieve the calving cycle of the Astrolabe. We observe that the ice front had significantly advanced toward the sea (4 km) since September 2016 and such an extension has not been observed in the previous years (since 2006) despite minor calving episodes. </span></p><p><span>The joint analysis of the seismological data and the velocity and strain maps are discussed with the recent evolution of the </span><span>glacier outlet</span><span>. The strain maps show complex patterns of extension and compression areas. The number of calving events</span><span> detected in the seismological dataset</span><span> significantly increased during 2016-2021 in comparison with the period 2012-2016.</span>&#160;<span>Since the beginning of 2021, both datasets show an acceleration. The number of calving events increased exponentially from June 2021 until the rupture in November 2021 and the velocity of the ice surface accelerated from 1 m.day</span>^{<span>-1</span>}<span> to 4 m.day</span>^{<span>-1</span>}<span> in the part of the glacier that detached afterward. This calving event is the first one of this magnitude ever documented over the Astrolabe glacier.</span></p>