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"content": "We continue with atmospheric escape with a talk from Ava Morrisey. Over time, sub Neptunes planets - all formed with their H/He envelope - split into two populations because some planets loose their atmospheres, through atmospheric escape that lasts for hours and hours after the transit. \n\nThere are only a few feasible targets because of ISM (too far from us won’t work). They focussed on the young HIP 94235 b and He I escape with CRIRES+.\nhttps://cdn.masto.host/astrodonsocial/media_attachments/files/112/648/261/229/924/532/original/a0639b78de3a5ec7.png\nhttps://cdn.masto.host/astrodonsocial/media_attachments/files/112/648/266/889/914/379/original/0be2fd380ef0fa39.png\nhttps://cdn.masto.host/astrodonsocial/media_attachments/files/112/648/274/226/977/332/original/7500434781bc46b5.png\nhttps://cdn.masto.host/astrodonsocial/media_attachments/files/112/648/278/067/051/282/original/6d91704f771be907.png\n",
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