{ "title": "Bedrock in a Trough in Asimov Crater", "authors": "HiRISE", "metadata": { "thumbnailURL": "https://static.uahirise.org/anews/2020-12-30/ESP_035777_1320.jpg", "excerpt": "The crater appears to have been completely filled by a thick sequence of materials, perhaps including sediments and lava flows." }, "version": "1.5", "identifier": "ESP_035777_1320", "language": "en", "layout": { "columns": 10, "width": 1024, "margin": 85, "gutter": 20 }, "documentStyle": { "backgroundColor": "#faf7f2" }, "components": [ { "role": "heading1", "layout": "heading1Layout", "text": "HiPOD: 30 December 2020" }, { "role": "divider", "layout": "bigDividerLayout", "stroke": { "width": 3, "color": "#8c2028" } }, { "role": "title", "layout": "halfMarginBelowLayout", "text": "Bedrock in a Trough in Asimov Crater" }, { "role": "photo", "layout": "fullBleedLayout", "caption": ">Many of these steep trough slopes in Asimov crater, where facing the equator, have recurring slope lineae activity in the summer when the sun-facing slopes get warm. Less than 1 km across. (NASA/JPL/UArizona)", "URL": "https://static.uahirise.org/anews/2020-12-30/ESP_035777_1320.jpg" }, { "role": "body", "format": "html", "layout": "hipodMarginLayout", "text": "


This image was acquired in southern winter over part of Asimov Crater, showing the equator-facing slope of a deep trough inside the crater. The crater appears to have been completely filled by a thick sequence of materials, perhaps including sediments and lava flows.

Later, deep troughs formed around the outer edge of the fill material, probably by collapse over void spaces at depth. What made the void space is not known, but one idea is that there were lenses of ice that slowly sublimated into the atmosphere. Another idea is that this is part of a sequence of crater fill and “exhumation”, that includes Gale Crater (home of the Curiosity rover). In other words, continued collapse and erosion of Asimov crater could eventually lead to a central mound like Eolis Mons (popular known as “Mt. Sharp”) in Gale Crater. However, at Asimov crater, the southern trough has destroyed the southern rim of the original crater, which didn’t happen at Gale Crater.

Many of these steep trough slopes in Asimov crater, where facing the equator, have recurring slope lineae (RSL) activity in the summer when the sun-facing slopes get warm. The RSL fade in the winter, so none are seen in this image even if they were present last summer when we acquired this image in 2014.

" }, { "role": "photo", "layout": "fullBleedLayout", "caption": "A fuller view of the crater rim. Less than 5 km across and north is down. (NASA/JPL/UArizona)", "URL": "https://static.uahirise.org/anews/2020-12-30/ESP_035777_1320-2.jpg" }, { "role": "body", "format": "html", "layout": "hipodMarginLayout", "text": "

ID: ESP_035777_1320
date: 15 March 2014
altitude: 254 km (158 mi)

NASA/JPL/UArizona

" }, { "role": "caption", "format": "html", "layout": "halfMarginBothLayout", "text": "Enhanced color image is less than 1 km across; black and white is less than 5 km. For full images with scalebars, see the above ID link to our website.

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