{ "title": "HiPOD", "metadata": { "thumbnailURL": "bundle://header.jpg", "excerpt": "Tartarus Colles are a group of knobby hills in the northern plains of Mars." }, "version": "1.5", "identifier": "testArticle", "language": "en", "layout": { "columns": 10, "width": 1024, "margin": 85, "gutter": 20 }, "documentStyle": { "backgroundColor": "#F5F9FB" }, "components": [ { "role": "heading1", "layout": "heading1Layout", "text": "HiPOD: THURSDAY, 10 OCTOBER 2019" }, { "role": "divider", "layout": "bigDividerLayout", "stroke": { "width": 3, "color": "#8c2028" } }, { "role": "title", "layout": "halfMarginBelowLayout", "text": "A Mesa in the Tartarus Colles Region" }, { "role": "photo", "layout": "fullBleedLayout", "caption": "A mesa in the Tartarus Colles region of Mars. (NASA/JPL/University of Arizona)", "URL": "bundle://ESP_055234_1910-main.jpg" }, { "role": "caption", "layout": "halfMarginBothLayout", "text": "Less than 5 km across, 278 km above the surface. (NASA/JPL/University of Arizona)" }, { "role": "body", "format": "html", "layout": "hipodMarginLayout", "text": "
The objective of this observation is to examine layers around a mesa. Some layers are thin; others much thicker.
Tartarus Colles are a group of knobby hills in the northern plains of Mars. Their formation might be the result of interactions between lava and water to form what are often called “rootless cones.”
NASA/JPL/University of Arizona
ID: ESP_055234_1910