Category: Space Sunday

Things are starting to pick-up on Mars once more as Curiosity starts into a new round of science studies in the region dubbed “The Kimberley”. Having been surveying the region since its arrival there at the beginning of April, the rover was commanded to move to a sandstone slab scientists dubbed “Windjana” after a gorge in Western Australia, and is in keeping with giving notable landmarks in the area unofficial names lifted from that part of Australia.

The slab lay a short distance roughly southwards from the rover’s position where the Mars Reconnaissance Orbiter (MRO) imaged it on April 11th, 2014. Following the initial selection of the slab as an area for further study, the rover was commanded to drive closer to it to enable further visual inspection. The slab is around 60 centimetres (2 feet) across, and was selected because it offered a good surface for drilling, and lay within what scientists call the “middle unit” because its location is intermediate between rocks that form buttes in the area and lower-lying rocks that show a pattern of striations.

The sandstone rock in the area is of particular interest to mission scientists because it represents a somewhat different environment to that studied extensively by Curiosity during the time it spent in the “Yellowknife Bay” area, drilling and sampling mudstone rocks.

“We want to learn more about the wet process that turned sand deposits into sandstone here,” Curiosity’s lead Project Scientist, John Grotzinger, explained. “What was the composition of the fluids that bound the grains together? That aqueous chemistry is part of the habitability story we’re investigating.”

Understanding why some sandstones in the area are harder than others also could help explain major shapes of the landscape where Curiosity is working inside Gale Crater. Erosion-resistant sandstone forms a capping layer of mesas and buttes. It could even hold hints about why Gale Crater has a large layered mountain, dubbed “Mount Sharp” (officially called Aeolis Mons), at its centre.

Once the rover had positioned itself close to the rock, initial inspection operations were carried out, which included using the turret-mounted spectrometer on Curiosity’s robot arm as well as the mast-mounted ChemCham laser so that the rock could be properly analysed ahead of any drilling operation. These operations also included deploying the rover’s “wire brush” to clean an area of the rock’s surface, removing dust and debris to expose the rock itself, allowing for further examination and analysis.

Before any sample drilling could occur, however, the rover would need to carry out a “mini-drilling” operation, much as it did at “Yellowknife Bay”. Such operations both confirm the drill’s readiness for sample gathering and confirm that the subject rock is a suitable target for drilling and gathering sample material.

This “mini-drilling” operation took place on Tuesday, April 29th, cutting a hole around 2 centimetres (0.8 inch) deep into the rock. This allowed the science team to evaluate the interaction between the drill and this particular rock – an important factor given issues enountered due to vibration during the rover’s previous operations – and also for the tailings of powder rock created by the drilling operation to be examined for their suitability for collection by the drilling mechanism.

When collecting sample material, the rover’s hammering drill bores as deep as 6.4 centimetres (2.5 inches) into a target rock. As it does so, some of the tailings from the drilling operation are forced up into the drill bit itself, and delivered to one of two holding chambers (Chambers A and B in the diagram below) located in the head of the drill bit mechanism.

Once drilling is complete, the gathered samples are transferred to CHIMRA – the Collection and Handling for In-Situ Martian Rock Analysis system, also within the rover’s turret system, where the tailings are sifted and sorted ready for eventual transfer to the Curiosity’s on-board chemical laboratory systems, comprising the Chemical and Mineralogy (CheMin) and Sample Analysis at Mars (SAM) suites of instruments.

At the present time, the outcome of the analysis of the mini-drilling operation, and the suitable of “Windjana” as a sample-gathering point is unclear; however, it would appear likely that sample drilling operations will go ahead nearby as a result of this test.

 First Asteroid Image from the Surface of Mars

Curiosity racked-up another first on Sol 606 (April 20th), when the Mastcam captured the first image of  asteroids taken from the surface of Mars. The image was combined with pictures captured the same night of the Martian Moons Phobos and Deimos, and the planets Jupiter and Saturn. Deimos, the outermost on the Martian moons, and which may have itself been an asteroid prior to wandering in Mars’ gravitational influence, appears at its correct location in the sky at the time the image of Ceres and Vista was captured. Phobos, Jupiter and Saturn, which were all imaged at different times, are shown as inset images on the left. All of the images form a part of ongoing astronomical work the rover has been performing periodically.

Ceres, with a diameter of about 950 kilometres (550 miles), is the largest object in the asteroid belt, large enough to be classified as a dwarf planet. Vesta is the third-largest object in the asteroid belt, about 563 kilometres (350 miles) wide. These two bodies are the destinations of NASA’s Dawn mission, which orbited Vesta in 2011 and 2012 and which is now on its way to begin orbiting Ceres in 2015.

The main image appears grainy, with Ceres, Vista and three stars appearing as streaks because it was captured over a 1-2 second exposure period. The graining on the image is the result of cosmic rays striking the camera detector is the image was captured. The images of Deimos, Phobos, Jupiter and Saturn were all captured over a much shorter 0.25-second exposure, thus rendering them as bright objects against a “clean” black background. Sunlight reflected by Deimos makes it appear overly large.

The interesting point (for those into astronomy) with the main image is that Vesta and Ceres would be naked-eye visible to anyone with average eyesight were they to be standing on the surface of Mars.

• MSL coverage in this blog

All images courtesy of NASA JPL.

On Wednesday April 16th, NASA JPL released a remarkable image captured using the High Resolution Imaging Science Experiment (HiRISE) camera on the Mars Reconnaissance Orbiter (MRO).

The image reveals the the Mars Science Laboratory, Curiosity parked alongside the multi-layered rock formation dubbed “The Kimberley”, as it prepares to undertake a range of science studies in the area.

The image was captured by MRO on April 11th during an overflight of the rover’s position as it sits at the foot of a rocky butte mission scientists have dubbed “Mount Remarkable”, and which forms a part of a multi-layered rocky location which has been dubbed “the Kimberley” due to its resemblance to a similar confluence of rock types found in Western Australia.

“The Kimberley” is an area of four distinguishable rock types exposed close together in a decipherable geological relationship to each other.  As such, they should provide further clues about ancient environments that may have been favourable for life. It is of particular interest to Scientists because like “Yellowknife Bay”, where the rover spent several months analysing and drilling rocks, “the Kimberley” demonstrates features which suggest that some of the rocks have only been exposed for a short time, geologically speaking.

This matters because Mars doesn’t have a magnetosphere and thick atmosphere like Earth’s, which protect us from energetic particles from space that break down organic material. So, rocks that have been exposed or close to the surface for a very long time are less likely to contain complex organic material, which might either be the remnants of past life, or help inform scientists about past habitability, the potential to support life in an area – as was the case with “Yellowknife Bay”.

Continue reading “Small blue dot on a red planet” →

Curiosity officially reached its next planned waypoint – dubbed “the Kimberley” on Wednesday April 2nd, 2014, with a final drive of some 30 metres (98 feet), after detouring from its planned drive route to reduce the amount of wear and tear being suffered by the rover’s aluminium wheels, the result of traversing some particularly rough terrain for several months.

“The Kimberley” was identified from orbit in 2013 as a possible location of interest during the rover’s drive down towards the point at which it will start its explorations of the lower slopes of “Mount Sharp”. It is an area of four distinguishable rock types exposed close together in a decipherable geological relationship to each other.  As such, they should provide further clues about ancient environments that may have been favourable for life.

As a major waypoint, “the Kimberley” will form an extended stopover for Curiosity which, while unlikely to be as long as the 6 months the rover spent exploring and examining “Glenelg” and “Yellowknife Bay”, will still be in the order of several weeks. The first part of this work is study the area in more detail, and the location occupied by the rover and the end of its April 2nd drive  – Sol 589 for the mission – is ideal for this. A slight rise compared to the surrounding terrain, it provides an excellent vantage point from which the rover can survey its surroundings, allowing mission scientists to comprehensively review the area and plan the coming science programme in finer detail than can be achieved when using orbital images alone. The science work is expected to involve observation of the surrounding region, sample-gathering from the rock formations, and onboard analysis of the samples gathered.

As I’ve previously reported, a cause of concern for mission personnel of late has been the amount of wear and tear the rover’s six aluminium wheels have suffered during the drive south from “Yellowknife Bay”. While the matter is far from serious in terms of impeding the rover’s manoeuvring or driving capabilities, with Curiosity’s nuclear battery offering the chance for a mission as much as 20 years in duration barring unforeseen circumstances, and what might provide to be a punishing climb up into the slopes of “Mount Sharp” still to come, the rover was directed onto less harsh terrain – comparatively speaking – in February 2014. Since then the mission team have been periodically checking on the wheels for further signs of damage and, as I noted last time around, the wear on the wheels is now around a tenth of that which had been experienced prior to the diversion. Nevertheless checks are still being carried out – including during the period in which this report was being written, as demonstrated by the raw image below, taken directly from the NASA image archive for Curiosity.

Continue reading “Sitting on the Kimberley and seeing spots” →

It’s been a quiet time for the last three weeks as far as news from NASA’s Mars Science Laboratory is concerned. There have been a couple of reasons for this.

The primary reason is that the rover is on a slow but steady drive towards its next intended science waypoint while en route to the lower slopes of “Mount Sharp”. At the start of February, that waypoint had been around half a kilometre from the rover. However, concerns over the amount of wear and tear being suffered by the rover’s wheels as a result of traversing very rough terrain meant that Curiosity took a diversion.

While this put the rover on much smoother – comparatively speaking – terrain, it also meant the route to the waypoint had become more circuitous, requiring Curiosity cover around a kilometre in order to reach its intended stopover. In addition, engineers have been periodically checking the amount of damage to the wheel which may be accruing, further slowing daily progress, as well as continuing to test alternative driving methods to further ease the load on the wheels – such as letting the rover drive backwards towards its destination. However, the good news is that in the month since crossing Dingo Gap on February 18th, wear on Curiosity’s wheels has been around one-tenth what had been experienced per month during the months traversing the rougher terrain.

Additional tests using Curiosity’s test bed “twin” on Earth have revealed that the rover could sustain substantially more damage than incurred so far, including breaks in the wheel treads themselves, and still remain operational. However, given the potential duration of the mission – Curiosity’s nuclear “battery” could provide it with an operational life measured in a couple of decades barring other failures – means caution is key at this stage of the mission.

“The wheel damage rate appears to have levelled off, thanks to a combination of route selection and careful driving,” said JPL’s Richard Rainen, mechanical engineering team leader for Curiosity. “We’re optimistic that we’re doing OK now, though we know there will be challenging terrain to cross in the future.”

MRO Computer Glitch

The other break in news, although brief in nature, was caused by an unexpected issue with Curiosity’s primary communications relay between itself and Earth – the Mars Reconnaissance Orbiter (MRO) unexpectedly switched itself into a “safe” operating mode on Sunday March 9th. This immediately brought a cessation in the orbiter’s communications relay function for both Curiosity and Opportunity on the surface of the planet, although it did not put either rover entirely out of communications with Earth.

While MRO forms the primary means of communications between the surface of Mars and mission control at NASA’s Jet Propulsion Laboratory facility at the California Institute of Technology, the rovers on Mars can also use NASA’s Mars Odyssey as a relay – and, should it be required, Europe’s Mars Express. However, Mars Odyssey, which has been operating around Mars for almost twelve and a half years, has much lower bandwidth and data transmission rates compared to MRO, which reduces the amount of information which can be relayed to Earth at any given time.

MRO’s issue first became apparent on March 9th, when the orbiter performed an unplanned swap between its duplicate computer systems. This is the prescribed response by a spacecraft when it detects conditions outside the range of normal expectations; the safe mode is initiated to reduce the risk of whatever caused the out-of-range event from being repeated by the second computer and potentially permanently harming the vehicle while matters are investigated. MRO has experienced unplanned computer swaps triggering safe-mode entry four times previously, most recently in November 2011, the root cause of which still hasn’t been clearly determined.

The March 9th safe mode entry also included a swap to a redundant radio transponder on the orbiter, marking the first time this has happened during the vehicle’s eight years in orbit around Mars. Whether or not the transponder issue triggered the computer swap-out is unclear. However, after carrying out a series of diagnostics on MRO from Earth, the mission team began bringing the orbiter back-up to full operational capabilities on March 11th, leaving it operating on the computer the swap-out switched to, together with the previously redundant radio transponder.

“The spacecraft is healthy, in communication and fully powered,” Mars Reconnaissance Orbiter Project Manager Dan Johnston said on March 11th. “We have stepped up the communication data rate, and we plan to have the spacecraft back to full operations within a few days.”

Charting a New Frost Channel

Since that event, MRO mission scientists have released a photo comparison showing the active nature of the Martian environment. The image shows two pictures of the same slope in the wall of crater Terra Sirenum, located in the southern highlands of Mars. There were captured some two and a half years apart (roughly equivalent to 1.2 Martian years), in November 2010 and May 2013 respectively.

The right-hand (May 2013) clearly shows the creation of a new gully down the inner wall of the crater, created when material flowing down the older channel broke out to form a new channel and corresponding fantail deposit. While the material responsible for the new gully was liquid in nature, as the event occurred in the Martian winter period in the southern hemisphere, it is believed that carbon dioxide ice, and not water, played the major role in forming the new channel.

NASA had previously experimented with dry ice to see if it could be responsible for such gullies, with interesting results.

 

Continue reading “On reaching Kimberley, managing communications and solving mysteries” →