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2 min read<\/p>\n
Written by Margaret Deahn, Ph.D. Student at Purdue University<\/p>\n
Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called \u2018Port Anson\u2019. In addition to this contact, the rover has encountered a variety of neat rocks that may have originated from elsewhere and transported to their current location, also known as float.<\/p>\n
Pictured above is an observation named \u2018Skull Hill\u2019 taken by the rover\u2019s Mastcam-Z instrument. This float rock uniquely contrasts the surrounding light-toned outcrop with its dark tone and angular surface, and it features a few pits in the rock. If you look closely, you might even spot spherules within the surrounding regolith! See Alex Jones\u2019 recent blog post for more information on these neat features: https:\/\/science.nasa.gov\/blog\/shocking-spherules\/<\/a>. The pits on Skull Hill may have formed via the erosion of clasts from the rock or scouring by wind. We\u2019ve found a few of these dark-toned floats in the Port Anson region, and the team is working to better understand where these rocks came from and how they got here.<\/p>\nSkull Hill\u2019s dark color is reminiscent of meteorites found in Gale crater by the Curiosity rover: https:\/\/www.jpl.nasa.gov\/news\/curiosity-mars-rover-checks-odd-looking-iron-meteorite\/<\/a>. Chemical composition is an important factor in identifying a meteorite, and Gale\u2019s meteorites contain significant amounts of iron and nickel. However, recent analysis of SuperCam data from nearby similar rocks suggests a composition inconsistent with a meteorite origin.\u00a0<\/p>\nAlternatively, \u2018Skull Hill\u2019 could be an igneous rock eroded from a nearby outcrop or ejected from an impact crater. On Earth and Mars, iron and magnesium are some of the main contributors to igneous rocks, which form from the cooling of magma or lava. These rocks can include dark-colored minerals such as olivine, pyroxene, amphibole, and biotite. Luckily for us, the rover has instruments that can measure the chemical composition of rocks on Mars. Understanding the composition of these darker-toned floats will help the team to interpret the origin of this unique rock!<\/p>\n\n\n\n\nExplore More<\/h2>\n<\/div>\n<\/div>\n\n\n\t\t\t\t\t\t<\/p>\n\n\n<\/figure>\n<\/div>\n<\/div>\n\n2 min read<\/div>\n\nSols 4511-4512: Low energy after a big weekend?<\/h3>\n<\/div>\n\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t<\/path><\/path><\/g><\/g><\/svg>\n\t\t\t\t\t\t\t\t\t\tArticle<\/span>\n\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t2 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/div>\n\n\t\t\t\t\t\t<\/p>\n\n\n<\/figure>\n<\/div>\n<\/div>\n\n3 min read<\/div>\n\nSols 4509-4510: A weekend of long drives<\/h3>\n<\/div>\n\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t<\/path><\/path><\/g><\/g><\/svg>\n\t\t\t\t\t\t\t\t\t\tArticle<\/span>\n\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t2 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/div>\n\n\t\t\t\t\t\t<\/p>\n\n\n<\/figure>\n<\/div>\n<\/div>\n\n2 min read<\/div>\n\nSols 4507-4508: \u201cJust Keep Driving\u201d<\/h3>\n<\/div>\n\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t<\/path><\/path><\/g><\/g><\/svg>\n\t\t\t\t\t\t\t\t\t\tArticle<\/span>\n\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t6 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/div>\n<\/div>\n<\/section>\n<\/div>\n\n\n\n\nKeep Exploring<\/div>\nDiscover More Topics From NASA<\/h2>\n<\/div>\n<\/div>\n\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Resources<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nExplore this page for a curated collection of Mars resources.<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tRover Basics<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nEach robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Exploration: Science Goals<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nThe key to understanding the past, present or future potential for life on Mars can be found in NASA\u2019s four\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
Skull Hill\u2019s dark color is reminiscent of meteorites found in Gale crater by the Curiosity rover: https:\/\/www.jpl.nasa.gov\/news\/curiosity-mars-rover-checks-odd-looking-iron-meteorite\/<\/a>. Chemical composition is an important factor in identifying a meteorite, and Gale\u2019s meteorites contain significant amounts of iron and nickel. However, recent analysis of SuperCam data from nearby similar rocks suggests a composition inconsistent with a meteorite origin.\u00a0<\/p>\nAlternatively, \u2018Skull Hill\u2019 could be an igneous rock eroded from a nearby outcrop or ejected from an impact crater. On Earth and Mars, iron and magnesium are some of the main contributors to igneous rocks, which form from the cooling of magma or lava. These rocks can include dark-colored minerals such as olivine, pyroxene, amphibole, and biotite. Luckily for us, the rover has instruments that can measure the chemical composition of rocks on Mars. Understanding the composition of these darker-toned floats will help the team to interpret the origin of this unique rock!<\/p>\n\n\n\n\nExplore More<\/h2>\n<\/div>\n<\/div>\n\n\n\t\t\t\t\t\t<\/p>\n\n\n<\/figure>\n<\/div>\n<\/div>\n\n2 min read<\/div>\n\nSols 4511-4512: Low energy after a big weekend?<\/h3>\n<\/div>\n\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t<\/path><\/path><\/g><\/g><\/svg>\n\t\t\t\t\t\t\t\t\t\tArticle<\/span>\n\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t2 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/div>\n\n\t\t\t\t\t\t<\/p>\n\n\n<\/figure>\n<\/div>\n<\/div>\n\n3 min read<\/div>\n\nSols 4509-4510: A weekend of long drives<\/h3>\n<\/div>\n\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t<\/path><\/path><\/g><\/g><\/svg>\n\t\t\t\t\t\t\t\t\t\tArticle<\/span>\n\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t2 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/div>\n\n\t\t\t\t\t\t<\/p>\n\n\n<\/figure>\n<\/div>\n<\/div>\n\n2 min read<\/div>\n\nSols 4507-4508: \u201cJust Keep Driving\u201d<\/h3>\n<\/div>\n\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t<\/path><\/path><\/g><\/g><\/svg>\n\t\t\t\t\t\t\t\t\t\tArticle<\/span>\n\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t\t\n\t\t\t\t\t\t\t\t\t\t6 days ago\t\t\t\t\t\t\t\t\t<\/span>\n\t\t\t\t\t\t\t\t<\/div>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/div>\n<\/div>\n<\/section>\n<\/div>\n\n\n\n\nKeep Exploring<\/div>\nDiscover More Topics From NASA<\/h2>\n<\/div>\n<\/div>\n\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Resources<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nExplore this page for a curated collection of Mars resources.<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tRover Basics<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nEach robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Exploration: Science Goals<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nThe key to understanding the past, present or future potential for life on Mars can be found in NASA\u2019s four\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
Alternatively, \u2018Skull Hill\u2019 could be an igneous rock eroded from a nearby outcrop or ejected from an impact crater. On Earth and Mars, iron and magnesium are some of the main contributors to igneous rocks, which form from the cooling of magma or lava. These rocks can include dark-colored minerals such as olivine, pyroxene, amphibole, and biotite. Luckily for us, the rover has instruments that can measure the chemical composition of rocks on Mars. Understanding the composition of these darker-toned floats will help the team to interpret the origin of this unique rock!<\/p>\n
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Explore this page for a curated collection of Mars resources.<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tRover Basics<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nEach robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Exploration: Science Goals<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nThe key to understanding the past, present or future potential for life on Mars can be found in NASA\u2019s four\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tRover Basics<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nEach robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Exploration: Science Goals<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nThe key to understanding the past, present or future potential for life on Mars can be found in NASA\u2019s four\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
Each robotic explorer sent to the Red Planet has its own unique capabilities driven by science. Many attributes of a\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Exploration: Science Goals<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nThe key to understanding the past, present or future potential for life on Mars can be found in NASA\u2019s four\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars Exploration: Science Goals<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/h3>\nThe key to understanding the past, present or future potential for life on Mars can be found in NASA\u2019s four\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
The key to understanding the past, present or future potential for life on Mars can be found in NASA\u2019s four\u2026<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
<\/a>\n\t\t\t\t\t<\/p>\n\n\n\n\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
\n\t\t\t\t\t\t\t\tMars 2020 Perseverance Rover<\/span>\n\t\t\t\t\t\t\t\t<\/circle><\/path><\/svg>\n\t\t\t\t\t\t\t<\/p>\n<\/div>\n<\/div>\n<\/figure>\n<\/div>\n<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\nPowered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
<\/a>\n\t\t\t\t<\/div>\n<\/div>\n<\/div>\n
Powered by WPeMatico<\/a><\/small><\/p>\nGet The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
Get The Details…<\/a><\/p>\n","protected":false},"excerpt":{"rendered":"Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>
Written by Margaret Deahn, Ph.D. Student at Purdue University Last week, NASA\u2019s Mars 2020 rover continued its journey down lower \u2018Witch Hazel Hill\u2019 on the Jezero crater rim. The rover stopped along a boundary visible from orbit dividing light and dark rock outcrop (also known as a contact) at a site the team has called [\u2026] Continue reading → <\/span><\/a><\/p>\n<\/div>Spread the love<\/div><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a><\/path><\/svg><\/span><\/a>