HiRISE: Light-toned mounds in Gorgonum Basin

ESP_050948_1430Gorgonum Basin is one of several large basins within the Terra Sirenum region of Mars. Each basin has light-toned mounds, many of which contain clays.

Scientists think that Terra Sirenum once had a large lake during an epoch called the Late Noachian/Early Hesperian, and each basin filled with sediments. The water within the lake may have altered these sediments to form the clays we now observe from orbit. Ma’adim Vallis, which drains into Gusev Crater where the Spirit rover landed, drained the water from this ancient lake… [More at link]

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THEMIS: Southern ice cap layers

Southern ice cap layers THEMIS Art #137 (THEMIS_IOTD_20170630)THEMIS Image of the Day, June 30, 2017. Do you see what I see? Looks like a plank of wood, with a beautiful grain to it. (THEMIS Art #137)

More THEMIS Images of the Day by geological topic.

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Algorithm helps protect Curiosity’s wheels

traction_control_sensor_vid-6secThere are no mechanics on Mars, so the next best thing for NASA’s Curiosity rover is careful driving.

A new algorithm is helping the rover do just that. The software, referred to as traction control, adjusts the speed of Curiosity’s wheels depending on the rocks it’s climbing. After 18 months of testing at NASA’s Jet Propulsion Laboratory in Pasadena, California, the software was uploaded to the rover on Mars in March. Mars Science Laboratory’s mission management approved it for use on June 8, after extensive testing at JPL and multiple tests on Mars.

Even before 2013, when the wheels began to show signs of wear, JPL engineers had been studying how to reduce the effects of the rugged Martian surface. On level ground, all of the rover’s wheels turn at the same speed. But when a wheel goes over uneven terrain, the incline causes the wheels behind or in front of it to start slipping.

This change in traction is especially problematic when going over pointed, embedded rocks. When this happens, the wheels in front pull the trailing wheels into rocks; the wheels behind push the leading wheels into rocks.

In either case, the climbing wheel can end up experiencing higher forces, leading to cracks and punctures. The treads on each of Curiosity’s six wheels, called grousers, are designed for climbing rocks. But the spaces between them are more at risk.

“If it’s a pointed rock, it’s more likely to penetrate the skin between the wheel grousers,” said Art Rankin of JPL, the test team lead for the traction control software. “The wheel wear has been cause for concern, and although we estimate they have years of life still in them, we do want to reduce that wear whenever possible to extend the life of the wheels.” [More at link]

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Curiosity update: Cat Sized Island

NRB_551884866EDR_F0641470NCAM00297M_-br2Sol 1741-43, June 28, 2017, update by MSL scientist Mark Salvatore: Last evening (June 27) between 8pm and 9pm PDT, Curiosity drove approximately 34 meters to the east to position herself just north of a large field of ripples on her way closer to ascending the iron oxide-bearing Vera Rubin Ridge. As Curiosity progresses towards the east, scientists back on Earth continue to look for opportunities to both gaze ahead towards interesting locations on the ridge itself, in addition to looking at the local rocks and sediment surrounding the rover. As we approach the lower units of Vera Rubin Ridge, our measurements of the “typical” rock that surrounds the rover will be vital to helping scientists understand how and why the ridge is different than the other units that have been investigated thus far in Gale Crater. Are we going to observe a very sharp transition in the composition and textures of rocks as we cross the threshold between the underlying mudstones of the Murray formation and the lowermost units of Vera Rubin Ridge? Or, alternatively, are we going to see a very subtle transition that might have gone unnoticed if not for the methodical measurements made upon approaching the ridge? Only time will tell, but we are making sure that we have the information necessary to definitively understand the nature of this transition.

Our science plan for the next two days begins with firing the ChemCam laser at a bedrock target right in front of Curiosity known as “Cat Sized Island”. The rock is almost a meter in length (more of a bobcat size than a standard house cat) and shows some interesting nodular textures that the science team wants to… [More at link]

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THEMIS: Northern ice cap’s edge in false color

Northern ice cap edge in false color THEMIS Art #136 (THEMIS_IOTD_20170629)THEMIS Image of the Day, June 19, 2017. Do you see what I see? I’d hang this piece of abstract art on my wall. (THEMIS Art #136)

More THEMIS Images of the Day by geological topic.

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HiRISE: Crater floor deposits in Terra Sabaea

tumblr_oqc3vvcn0H1rlz4gso1_1280Deposits on the floor of a crater in Terra Sabaea. Beautiful Mars series.

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Curiosity: Rocks and sand rise toward the ridge

1739-navcamSol 1739, June 28, 2017. Curiosity’s Navcam has captured the ground leading up to Vera Rubin Ridge and also Mt. Sharp rising in the distance behind. The rover is driving eastward, perhaps to go around the sand patch seen at left. Mission controllers are maneuvering the rover toward a place where it can easily drive up onto the ridge. (Click image to enlarge it.)

Sol 1739 raw images (from all cameras), and Curiosity’s latest location.

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HiRISE: ‘Elementary, my dear deposit…’

ESP_050250_1435Just like Earth, Mars experiences seasons that change as the planet orbits the Sun. Seasonal changes are most apparent at the higher latitudes. As these regions in each hemisphere enter their respective summer seasons, the sun rises higher in the Martian sky causing frost and ice to sublimate, and illuminate more features across the landscape. As the high latitudes of each hemisphere move toward their respective winters, the days (called “sols”) grow shorter and the sun hangs low on the horizon, giving rise to prolonged periods of cold, darkness, and frost accumulation… [More at link]

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Trace Gas Orbiter: Aerobraking suspended

ExoMars_Trace_Gas_Orbiter-640On 25 June, the Trace Gas Orbiter (TGO) will suspend its aerobraking campaign until the end of August due to Mars’ conjunction with the Sun.

With Mars behind the Sun, TGO’s communication with Earth will be difficult, and so the spacecraft orbit will be raised safely out of the atmosphere. The orbiter is now on an aerobraking campaign, exploiting the resistance of the Martian atmosphere on the spacecraft to slow itself down and lower its orbit with minimal fuel consumption.

(…) The Martian atmosphere is highly variable and this variability makes it impossible to plan ahead for more than a handful of orbits; so, during the conjunction period, the spacecraft is being taken out of aerobraking and placed into a safe orbit where the atmosphere won’t disturb it. TGO’s descent will resume after the end of conjunction…. [More at link]

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MARCI weather report, June 19-25, 2017

MARCI-June-22-2017Dust-raising activity persevered along the edge of the seasonal north polar ice cap this past week. While the majority of the storms were small in scale, more extensive storm fronts were spotted over Utopia Planitia towards the end of the week. Meanwhile, on the other side of the red planet, dust storms continued over the southern highlands near the developing south polar hood. During the middle of the week, active… [More at link, including video]

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