Mars Express: Shaping the surface with water, wind, and ice

Perspective_view_of_Nili_FossaeESA’s Mars Express has imaged an intriguing part of the Red Planet’s surface: a rocky, fragmented, furrowed escarpment lying at the boundary of the northern and southern hemisphere.

This region is an impressive example of past activity on the planet and shows signs of where flowing wind, water and ice once moved material from place to place, carving out distinctive patterns and landforms as it did so. (…)

Northern Mars also displays large areas of smooth land, whereas the planet’s southern regions are heavily pockmarked and scattered with craters. This is thought to be the result of past volcanic activity, which has resurfaced parts of Mars to create smooth plains in the north – and left other regions ancient and untouched.

The star of this Mars Express image, a furrowed, rock-filled escarpment known as Nili Fossae, sits at the boundary of this north-south divide. This region is filled with rocky valleys, small hills, and clusters of flat-topped landforms (known as mesas in geological terms), with some chunks of crustal rock appearing to be depressed down into the surface creating a number of ditch-like features known as graben… [More at link]

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THEMIS: Dunes in Kaiser Crater

Kaiser Crater dunes (THEMIS_IOTD_20181123)THEMIS Image of the Day, November 23, 2018. This VIS image shows part of the floor of Kaiser Crater, including several sand dunes. Kaiser Crater is located in Noachis Terra.

The dunes’ dark tone indicates they are free of dust, so it is likely that the sand is loose and being moved by winds today.

See more THEMIS Images of the Day by geological subject.

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HiRISE: Pitted cones in Chryse Planitia

tumblr_pii1f8JtJZ1rlz4gso2_1280Pitted cones in Chryse Planitia. Beautiful Mars series. [More at links]

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InSight: Science and engineering of a Mars lander

Prior to landing on the Red Planet, NASA discusses the engineering that went into the InSight lander. Launched on May 5, InSight marks NASA’s first Mars landing since the Curiosity rover in 2012. The landing will kick off a two-year mission in which InSight will become the first spacecraft to study Mars’ deep interior. Its data also will help scientists understand the formation of all rocky worlds, including our own.

InSight is being followed to Mars by two miniature NASA spacecraft, jointly called Mars Cube One (MarCO), the first deep-space mission for CubeSats. If MarCO makes its planned Mars flyby, it will attempt to relay data from InSight as it enters the planet’s atmosphere and lands.

InSight and MarCO flight controllers will monitor the spacecraft’s entry, descent and landing from Mission Control at JPL.

Speakers include:

  • Thomas Zurbuchen, Associate Administrator
  • Tom Hoffman, InSight project manager at JPL
  • Stu Spath, InSight Program Manager, Lockheed Martin Science
  • Rob Grover, Entry, Descent and Landing (EDL) Phase Lead for InSight, NASA-JPL
  • Anne Marinan, MarCO-B Mission Manager, NASA-JPL

[More at link]

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THEMIS: Swiss-cheese weathering in old volcanic region

Circular erosion in lava flows (THEMIS_IOTD_20181122)THEMIS Image of the Day, November 22, 2018. Amphitrites Patera is an old volcanic complex located south of Hellas Planitia.

The surface in this VIS image has a unusual “Swiss-cheese” texture, one seen more commonly on the nearby south polar ice. The surface appears to be eroding in a fashion that creates small circular features which grow and coalesce into larger circles.

See more THEMIS Images of the Day by geological subject.

 

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MARCI weather report, November 12-18, 2018

MARCI-November-18-2018For the past week on Mars, dust storm activity was largely inactive — apart from some areas in the northern hemisphere. The low-lying plains of Acidalia, Amazonis, and Chryse each had a couple of transient local-scale dust storms over the course of the week. Looking to the southern highlands, dust lifting continued to be diminished across many regions. Only a few hazes associated with the defrosting seasonal south polar ice cap were observed. Among the low-latitudes, water ice clouds endured over the southernmost volcano of the Tharsis Montes, known as Arsia Mons. Both rover sites… [More at link, including video]

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Mantle plumes still active under Tharsis, Elysium?

figure-2[Editor’s note: From a paper by A.-C. Plesa and eight co-authors recently published in Geophysical Research Letters.]

The thermal state and interior structure of Mars

We constrain the thermal state and interior structure of Mars by combining a large number of observations with thermal evolution models. Models that match the available observations require a core radius larger that half the planetary radius and a crust thicker than 48.8 km but thinner than 87.1 km on average.

All best‐fit models suggest that more than half of the planet’s bulk abundance of heat producing elements is located in the crust. Mantle plumes may still be active today in the interior of Mars and produce partial melt underneath the Tharsis volcanic province.

Our results have important implications for the thermal evolution of Mars. Future data from the InSight (Interior exploration using Seismic Investigations, Geodesy and Heat Transport) mission can be used to validate our models and further improve our understanding of the thermal evolution of Mars. [More at link]

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InSight: On course toward landing

PIA22100_hiresNASA’s Mars Interior Exploration using Seismic Investigations, Geodesy and Heat Transport (InSight) spacecraft is on track for a soft touchdown on the surface of the Red Planet on Nov. 26, the Monday after Thanksgiving.

But it’s not going to be a relaxing weekend of turkey leftovers, football, and shopping for the InSight mission team. Engineers will be keeping a close eye on the stream of data indicating InSight’s health and trajectory, and monitoring Martian weather reports to figure out if the team needs to make any final adjustments in preparation for landing, only five days away.

“Landing on Mars is hard. It takes skill, focus and years of preparation,” said Thomas Zurbuchen, associate administrator for the Science Mission Directorate at NASA Headquarters in Washington. “Keeping in mind our ambitious goal to eventually send humans to the surface of the Moon and then Mars, I know that our incredible science and engineering team – the only in the world to have successfully landed spacecraft on the Martian surface – will do everything they can to successfully land InSight on the Red Planet.” [More at link]

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HiRISE: Mysterious features on crater floor

tumblr_pib2zzFvtR1rlz4gso2_1280Mysterious! These interesting-looking features are on the floor of crater near Amazonis Mensa. They might be wind-driven erosional features.

Beautiful Mars series. [More at links]

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We’re going to Jezero!

jezero_delta_perspective_20k_doran_f840[From Emily Lakdawalla’s blog at the Planetary Society]

NASA announced [November 19] the selection of Jezero crater for the landing site of the Mars 2020 mission. Mars 2020’s launch period opens 19 July 2019, and landing will happen on 18 February 2021 regardless of the launch date. (“It’s a Thursday!” landing team lead Allen Chen said during today’s press briefing.)

Jezero — which is named after a town in Bosnia and Herzegovina is a 45-kilometer-wide crater that once held a lake. It is correctly pronounced something like “YEH-zuh-doh,” though mission team members typically pronounce it “DZEH-zuh-row.” (Many thanks to Katherine Sredl for recording the correct pronunciation for me.) Jezero contains a spectacular preserved river delta, which will be the focus of the rover’s primary mission. At Jezero, Mars 2020’s goal will be “to explore the history of water and chemistry in an ancient crater lake basin and associated river-delta environments to probe early Martian climates and search for life,” according to a mission overview for Jezero (PDF) by team members Sanjeev Gupta and Briony Horgan… [More at link]

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