Mars courier: Bringing the samples to Earth

The first round-trip to the Red Planet will see a European orbiter bringing martian samples back to Earth. ESA is opening the door to industry to build the spacecraft that will deliver the precious rocks, dust and gas from Mars – the key to understanding whether life ever existed on our closest planetary neighbour.

This ‘take-away’ service is called the Earth Return Orbiter, and will be ESA’s major contribution to the Mars Sample Return campaign. The ESA Orbiter will carry NASA’s Capture and Containment and Return System, which will rely on the ESA-led spacecraft for transit to and from Mars.

Three launches from Earth and one from Mars – the first ever from another planet –, two rovers and an autonomous capture in Mars orbit are all part of an ambitious series of missions that ESA is embarking on together with NASA.

he campaign aims to bring at least 500 grams of samples back from the Jezero crater that once held a lake and contains an ancient preserved river delta. The rocks in the area preserve information about Mars’ diverse geology.

NASA’s Mars 2020 rover that is slated for launch in July 2020 will scientifically select the best samples to store in tubes and deposit them onto the martian surface for later retrieval.

ESA is also studying concepts for a small ‘fetch’ rover to scurry quickly across the martian surface to locate and recover the stored samples. It would then carry them back to a football-sized canister that would be launched with a NASA Mars Ascent System – a small rocket.

The Earth Return Orbiter will capture the canister in orbit and transfer it safely to Earth, a return trip that will take about 13 months… [More at link]

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HiRISE: Layers in Tikhonravov

ESP_054975_1935Layers in Tikhonravov. The objective of this observation is to examine layers outside of a crater within the 344-kilometer diameter Tikhonravov Crater. Tikhonravov is believed to have once held a giant lake and was named after Mikhail Tikhonravov, a Russian rocket scientist.

HiRISE Picture of the Day archive. [More at links]

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THEMIS: Graben in Elysium Fossae

Elysium Fossae (THEMIS_IOTD_20190729)THEMIS Image of the Day, July 29, 2019. Today’s VIS image shows a section of one of the graben that comprise Elysium Fossae. Graben are formed during tectonic activity, where blocks of material slide down between paired faults.

Graben are common around volcanic regions on Mars. The rise of magma to the surface bows up the ground, creating the extensive forces that create graben.

Explore more THEMIS Images of the Day by geological subject.

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Curiosity update: Goin’ up

2477MH0001530000902860R00_DXXX-br2Sols 2478-80, July 27, 2019, update by MSL scientist Abigail Fraeman: Over the last few weeks Curiosity has collected hundreds of spectacular images, like the one above, that document the layers and textures of rocks exposed in the “Visionarium.” (And as we heard in the last blog, we also set a mission record yesterday for having the highest tilt we’ve ever had while conducting contact science — over 25 degrees!) With all of this imaging under our belt, we’re now hoping to delve deeper into studying the composition of the rocks in the Visionarium, so we are beginning to look for our next potential drill target.

In the plan for the weekend, Curiosity will drive ~10 m to the top of the southern escarpment in the Visionarium. The drive will place us in an ideal location to image potential future drill targets. Before the drive, we’ll spend a sol collecting MAHLI and APXS data from targets named “Naver” and “Fetterangus,” along with ChemCam and Mastcam observations of “Malin Sea,” “Loch Katrine,” and “Loch Broom.” We’ll also take several environmental science monitoring observations, and an 80 frame stereo Mastcam mosaic of “Hebrides,” which is the area where we hope to find our next drill target… [More at link]

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Mars 2020 rover does biceps curls

The robotic arm on NASA’s Mars 2020 rover does not have deltoids, triceps or biceps, but it can still curl heavy weights with the best. In this time-lapse video, taken July 19, 2019, in the clean room of the Spacecraft Assembly Facility at the Jet Propulsion Laboratory in Pasadena, California, the rover’s 7-foot-long (2.1-meter-long) arm handily maneuvers 88 pounds’ (40 kilograms’) worth of sensor-laden turret as it moves from a deployed to a stowed configuration.

The rover’s arm includes five electrical motors and five joints (known as the shoulder azimuth joint, shoulder elevation joint, elbow joint, wrist joint and turret joint). The rover’s turret includes HD cameras, the Scanning Habitable Environments with Raman & Luminescence for Organics & Chemicals (SHERLOC) science instrument, the Planetary Instrument for X-ray Lithochemistry (PIXL), and a percussive drill and coring mechanism.

On Mars, the arm and turret will work together, allowing the rover to work as a human geologist would: by reaching out to interesting geologic features, abrading, analyzing and even collecting them for further study via Mars 2020′s Sample Caching System, which will collect samples of Martian rock and soil that will be returned to Earth by a future mission… [More at link]

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Curiosity: Parked on the slope

2476-navcamSol 2476, July 25, 2019. With Curiosity parked on the steep slope of the Southern Outcrop, the Navcam shot a composite that shows the terrain to the south. Click the image to enlarge it.

Sol 2476 raw images (from all cameras).

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HiRISE: Flow, moving

ESP_054974_2165Flow, moving. The objective of this observation is to examine a flow that goes through a crater in Nilosyrtis Mensae. It was probably larger in the past and has since been reduced in volume.

HiRISE Picture of the Day archive. [More at links]

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Curiosity update: Records measured in degrees

NLB_617304466EDR_F0762672NCAM00268M_-br2Sol 2477, July 25, 2019, update by MSL scientist Susanne Schwenzer: Europeans, Californians… and many others on the team watched their thermometers rise to record highs today, reaching 36°C in this blogger’s hometown “Milton Keynes.” Thinking about planning, where we currently think about cold, wintertime temperatures on Mars and tosol’s maximum temperature was -30°C according to REMS, this 66°C difference in temperature is a very practical demonstration of orbital mechanics and other factors, and more generally how different Earth and Mars are!

Temperatures are not today’s most important record, though: Curiosity is currently tilted 25° – more than ever before, during science operations. The image above shows just how much this is…. [More at link]

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THEMIS: Terra Cimmeria channel

Terra Cimmeria channel (THEMIS_IOTD_20190726)THEMIS Image of the Day, July 26, 2019. This VIS image shows an unnamed channel in Terra Cimmeria. The channel is located immediately outside of the rim of Knobel Crater.

Explore more THEMIS Images of the Day by geological subject.

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Curiosity update: The Southern Escarpment almost within reach

NLB_617218055EDR_F0762594NCAM00266M_-br2Sol 2476, July 24, 2019, update by MSL engineer Ashley Stroupe: This morning Curiosity found herself parked at the base of the southern escarpment of the Visionarium. She’s at a significant tilt of 21 degrees; you can see the slope of the horizon in the attached image. We’ve been imaging this ridge from several locations over the past few sols, trying to build up our understanding of the geology in this area. In today’s plan Curiosity will continue taking high resolution images of the outcrop with Mastcam and ChemCam; three specific areas are being targeted on the outcrop to see details of the various layering: “Antonine Wall,” “Tyrebagger Hill,” and “Seaton Cliffs.”

After completing the imaging, Curiosity will be driving just a little bit closer to try to put the layers near Tyrebagger Hill into the arm workspace. This requires backing up a short distance, turning slightly, and then re-approaching the ridge at a slightly different location… [More at link]

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