{ "title": "Aligned Mounds and Broad Pits", "authors": "HiRISE", "metadata": { "thumbnailURL": "https://static.uahirise.org/anews/2020-04-06/ESP_063414_2070.jpg", "excerpt": "Our goal with this observation is to also include a look at nearby buttes and depressions." }, "version": "1.5", "identifier": "ESP_063414_2070", "language": "en", "layout": { "columns": 10, "width": 1024, "margin": 85, "gutter": 20 }, "documentStyle": { "backgroundColor": "#faf7f2" }, "components": [ { "role": "heading1", "layout": "heading1Layout", "text": "HiPOD: 6 APRIL 2020" }, { "role": "divider", "layout": "bigDividerLayout", "stroke": { "width": 3, "color": "#8c2028" } }, { "role": "title", "layout": "halfMarginBelowLayout", "text": "Aligned Mounds and Broad Pits" }, { "role": "photo", "layout": "fullBleedLayout", "caption": ". Less than 5 km across. (NASA/JPL/UArizona)", "URL": "https://static.uahirise.org/anews/2020-04-06/ESP_063414_2070.jpg" }, { "role": "body", "format": "html", "layout": "hipodMarginLayout", "text": "
Is it possible that the aligned features are some sort of igneous landform (rootless cones, cinder cones, spatter cones) or are they the remains of secondary impact craters, or something else altogether? Our goal is to also include nearby buttes and depressions, as well, so as to make comparisons.
This observation is located north of Antoniadi Crater in the Northern Hemisphere of Mars.
ID: ESP_063414_2070
date: 21 May 2019
altitude: 294 km
NASA/JPL/UArizona