Curiosity: speaking from Mars

Monday August 27th saw NASA host another news briefing on Curiosity’s progress, which included some amazing new images and well as updates on SAM and recent manoeuvrings with the rover.

The briefing started with a message “from Mars”, in the form of a recording of a greeting by NASA Administrator and former astronaut, Charles Bowden. Carried by Curiosity to Mars and then transmitted back to Earth, the message, lasting just over a minute, represents the first broadcast of a human voice from another planet. While primarily of PR value, the broadcast demonstrated the capabilities available with the rover working with (in particular) the Mars Reconnaissance Orbiter (MRO) when transferring large amounts of data to Earth; the speech represented some 4 megabits of voice data, which was transmitted alongside other information. As it is, in just three weeks, Curiosity has returned more data to Earth than the entire Pathfinder and MER rover missions combined.

SAM takes a Sniff

SAM, the Sample Analysis at Mars, is a suite of instruments designed to analyse organics and gases from both atmospheric and solid samples. On Saturday August 25th SAM was allowed to take its first sample of the Martian air, albeit as an engineering calibration exercise rather than a science experiment. After a slight “blip” in the proceedings when traces of calibration gas which should have been evacuated from the system beforehand were measured rather than Martian air, the tests successfully confirmed SAM’s atmospheric sampling capabilities are ready for action. In the future SAM will not only be able to sniff the air (and “taste” samples of Martian rock and soil delivered to it by the robot arm), it should even be able to tell us what Mars smells like (which, given it is thought Gale Crater has levels of sulphur dioxide present, is liable to be, “Ewww! Rotten eggs!”).

Mastcam Demonstrates its Power

The two Mastcam cameras (M100 (telephoto) and M34 (wide-angle)) have almost completed their characterisation check-outs and the Malin Space Science Systems team is getting ready to turn them over to the MSL science team for the start of science operations. Key to this work has been ensuring the cameras are properly focused, a process that has required using the both camera lenses to take high-resolution images across a range of distances. This has resulted in some amazing mosaics of Gale Crater being produced.

In the above image, Mastcam reveals Gale Crater: the grit-like surface on which the rover sits extends outwards to the South-west for about 125m (406ft), and is followed by a slight dip in the land that extends a further 105m (341ft) from the rover to the lip of a small crater about 20m (65ft) across. Beyond the rim of the crater can be seen what is described as a low-lying “moat” surrounding the flanks of “Mount Sharp”, the middle of which is about 3.7km (2.3 miles) from the rover. Beyond this is a field of sand dunes some 5.5km (3.4 miles) distant, with the base slopes of the mound just beyond them. The regions the science team are particularly interested in extend from about 6.6km (4 miles) from the rover out to about 10.7km (6.7 miles).

The image above shows a zoomed-in view of the region of interest, with the dune field in the immediate foreground. The inset image is of a rock roughly the size of Curiosity (the black dot in the inset image), pictured to hep give a sense of scale to the mesas, and show what the rover might look like if it could be pictured from Bradbury Landing once it starts exploring “Mount Sharp”.

While the area of interest is only 10km (6 miles) from Bradbury Landing, it would take Curiosity 100 days to reach it, were it to drive at full speed – which is obviously not what is going to happen, as there is much to study along the way.

On August 27th, NASA released a panoramic movie of Gale Crater and “Mount Sharp” put together using images from the Mastcam captured on the 8th and 18th August (prior to the focus calibrations being completed). The images have been white-balanced to match sunlight levels on earth, with 640×360 and 1280×720 Quick Time version of the movie available on the JPL website (note the 1280 movie is over 242Mb in size and may take time to download and stream).

Continue reading “Curiosity: speaking from Mars”

In memory of Neil Armstrong

Nine summers ago, I went for a visit,
To see if the moon was green cheese.
When we arrived, people on earth asked: “Is it?”
   We answered: “No cheese, no bees, no trees.”
There were rocks and hills and a remarkable view
   Of the beautiful earth that you know,
It’s a nice place to visit, and I’m certain that you
   will enjoy it when you go.

Neil Armstrong, 1978

Neil Armstrong, 1930-2012
First man to walk on the Moon
Missions flown: Gemini 8, Gemini 11, Apollo 11

Relay for Life of InWorldz kickoff rally

August 25th will see the start of the first ever Relay for Life season held in InWorldz, with a special kick-off rally.

The three-month event will run through until November 17th and has the full support of the American Cancer Society.

Other key dates for the season include:

  • Saturday September 22nd: RFL of InWorldz Half-way Event
  • Friday November 2nd through Sunday November 4th: RFL of InWorldz Relay for Life Weekend
  • Saturday 17th November: RFL of InWorldz Closing Party.

The theme for this inaugural season is Colour of Hope, as featured in the season’s banner, as seen in the video, above.

The kick-off rally will be held on Dreamscapes of Poseidon (IWurl), commencing at midday IW time (PDT). It presents a chance for participants to learn how their involvement benefits the American Cancer Society’s goal to save lives and create more birthdays and the opportunity to meet the Society’s IW representative as well as gain inspiration from DJ KyFire Oakleaf’s library of originals created by all those who have been involved in the fight against cancer, including survivors, caregivers and loved ones of those who sadly succumbed to the disease.

Kick-off Rally Schedule

  • 12:00 pm KyFire Oakleaf – RFL Songs
  • 12:15 pm Hairy Thor Chair
  • 12:22 pm RFL Video
  • 12:30 pm TIGGS Beaumont
  • 12:37 pm KyFire
  • 12:40 pm Sting Raymaker
  • 12:50 pm KyFire Oakleaf- closing.

Following the kick-off rally, the season will comprise a number of events held within InWorldz, culminating in the Relay Weekend itself at the start of November. In it, individuals and teams will camp out, picnic, dance, play games and take turns circling around a track “relay” style to raise funds and fight cancer. The Relay Weekend will open  with cancer survivors leading the way around the track and being honoured in the Survivor Lap. They will be followed throughout the day by groups, teams and individuals participating in the track walk which will continue over 24 hours, and the weekend will include the beautiful, moving and silent luminaira ceremony, in which lights are lit in memory of a loved one who won the fight against cancer or in remembrance of a special someone who lost their battle.

Relay For Life represents hope in that those lost to cancer will not be forgotten, that those who face cancer will be supported, and that one day, cancer will be eliminated.

Related Links

Curiosity: stretch, wriggle and roll!

This week has been perhaps the busiest to date for the MSL team, with a series of milestones for the project being reached one after another which pretty much complete the initial characterisation phase of the mission (phases 1a and 1b). These have included the first firings of the rover’s laser system, an initial stretching of the instrument-laden robot arm and Curiosity’s first drive.

Zap!

On Sol 13 (19th August), the mission team carried out the first test firings of the ChemCam laser at a surface object. The inaugural target was a small rock some 7 centimetres (3 inches) across which scientists christened “Coronation” to mark the event, but which was previously designated N165. It had been selected as it presented a relatively flat surface to the rover.

The test firing lasted some 10 seconds, during which the rock was struck by 30 pulses from the laser system, each pulse delivering more than a million watts of power for about five billionths of a second to a tiny spot on the surface of the rock, vaporising it into plasma. Light from the plasma was captured by ChemCam’s telescope and fed via fibre-optics to the rover’s three spectrometers for analysis.

A composite image of the test firing. The background image is from Curiosity’s Navcam, showing N165. The two inset images are from ChemCam’s Remote Micro Imager (RMI)

The results were far better than anticipated, prompting ChemCam Deputy Project Scientist Sylvestre Maurice of the Institut de Recherche en Astrophysique et Planetologie (IRAP) in Toulouse, France, to comment, “It’s surprising that the data are even better than we ever had during tests on Earth, in signal-to-noise ratio. It’s so rich, we can expect great science from investigating what might be thousands of targets with ChemCam in the next two years.”

This was followed-up with a further series of firings on Sol 16 at some of the rocks exposed by the motors of the Descent Stage as it hovered in “skycrane” mode to lower the rover onto the surface of Gale Crater. Here the laser was fired some 50 times at three targets in the exposed rocks, which were also photographed by ChemCam’s RMI.

Images from ChemCam’s RMI showing a laser “hit” on Sol 16. The main image shows the rocks roughly 6 metres from the rover. The inset is  a composite “before” and “after” image of a laser strike. It shows an area on the rock 2.5 sq cm in size. RMI can resolve details as small as 0.5 to 0.6 millimetres

Stretch

On Sol 14 Curiosity finally got to give her arm a bit of a stretch. The 2.1-metre (7 foot) long arm includes a 60-centimetre (2 ft) diameter “hand” called the Turret, which contains a range of scientific instruments and tools essential to the mission, including a dedicated camera (the Mars Hand Lens Imager, or MAHLI), a drill system, a scoop for collecting Martian soil (“fines”), and an Alpha-particle X-ray Spectrometer (APXS).

In this initial manoeuvre, the arm was raised, extended and rotated to use all five of its joints prior to it being stowed once more in preparation for Curiosity’s first drive. The manoeuvre marks the first step in calibrating the arm’s movements and preparing it for science operations. Further tests of the arm and its equipment load will take place over the next several weeks, but the system is unlikely to be fully commissioned until around mid-October.

Curiosity raises its turret of equipment as the robot arm is tested (image captured by the black-and-white Navcam system)

Continue reading “Curiosity: stretch, wriggle and roll!”

Kitely goes mega

I’m a little late getting to this, as I’ve been swimming through a lot of SL-related stuff and other bits, so apologies to Oren and Ilan. 

On the 17th August, Kitely announced the addition of high performance big worlds and world pictures to their on-demand service.

Public World Page Images

Taking the second of the new additions first, Kitely users can now add an image of their world(s) to the Public Worlds listing. Previously, the Public Worlds list was just that – a text list of all worlds in Kitely available for public access. The use of images makes the list more visually appealing and gives those browsing the list a glimpse of the world prior to clicking on the image to access the region’s World Page.

Adding a Public Worlds image via the Manage World Advanced tab

Pictures can be set in one of two places – the World Page, and in the Advanced tab of the Manage World dialogue box. Submitted pictures are automatically resized to fit the available space on upload.

The Public Worlds page has been redesigned to support the new images,  with world images being displayed 12 to a page, with the world name below the image with the world owner’s name. Those worlds that have not yet had an image uploaded for the page will show the Kitely logo, and will generally be listed after all those that have an uploaded image available.

The updated Public Worlds page layout, with my own region in the list 🙂

Big Worlds

Following-on from the promise in the last update, Kitely have implemented their “big world” feature. This allows large, high-performance worlds to be created which can be up to 16 regions in size (i.e. 4 regions x 4 regions). In addition to the 16-region world, big worlds are also offered in four region (2×2) and nine region (3×3) sizes.

The free worlds offered within the Silver and Gold subscription plans can be used to create  various mixes of big worlds and standard regions, according to the user’s requirements. For example: a Silver plan might be used to create 10 individual regions, or two 2×2 big worlds and two “standard” individual regions or a 3×3 big world and single individual region, etc.

However, the size of a world can only be set when it is created, and cannot be changed afterwards. Therefore, single region worlds already created in Kitely cannot be converted to big worlds, regardless of the remaining quota of free regions in a silver or gold plan (e.g. if a user has 3 regions left in their free quota, they cannot combine them with an existing single-region world to create a 2×2 big world).

Additional worlds beyond a plan’s quota can be purchased using Kitely Credits (KC) at the rate of 10KC per region per day. So a 4-region (2×2) big world would cost 1200KC a month (4 regions x 10KC x 30 days), or as little at $4 a month when purchasing Kitely Credits at the maximum discounted rate. The costs of copying, exporting, and replacing big worlds are also dependent on the number of regions in the world. For example, copying a 4-region world will cost 40 KC (10KC per region).

Additional points of note about big worlds:

  • Big worlds have a “root region”, which is always the region in the South-west corner of the world
  • Big worlds have a “default region”, which is initially the root region (SW corner region) of the world, where incoming visitors arrive
    • This can be altered through the use of a tele hub, which can be placed in any region in the world, making it the default for incoming visitors
    • Deleting the telehub will not alter the updated default region
    • Moving the default region does not change the location of the root region
  • There is a limit of 100,000 prims for a world, regardless of the number of regions it contains.  How the total allocation is distributed among the regions within a big world is up to the world owner, but the total of 100,000 prims cannot be exceeded
  • When running in megaregion mode (see below), region crossings are completely eliminated
  • Vivox works seamlessly across all regions in a big world.

By default, Kitely’s big worlds use the OpenSim megaregion mode, wherein multiple regions have been merged into one contiguous region. This eliminates region crossings within a big world and all the dependent issues around them for building, vehicle movement, etc., and provides a much smoother overall performance.

However, Megaregions are an experimental feature so some OpenSim features don’t work properly (e.g. parcel audio only works in the root region). Kitely therefore allows big worlds to be run as either megaregions or non-megaregions; a check-box is provided in the Advanced Tab of the Manage World dialogue box to switch any inactive world (i.e. a world not currently running on a Kitely server) between the two modes.

Kitely have also added a new world template to help in the creation of big worlds. This is the Universal Campus, a 2×2 region build created by Michael Emory Cerquoni (a.k.a. Nebadon Izumi), and licensed under the Creative Commons Attribution-ShareAlike licence.

To support the safe archiving of big world builds, Kitely have extended to the OpenSim Archive (OAR) file format to support the saving of a multi-region world as a single OAR file. Currently, the file format cannot be used to export builds elsewhere, but the code has been submitted for inclusion in standard OpenSim, and once adopted by OpenSim, will allow the exchange of multi-region OAR files between Kitely and other grids (with limitations to protect 3rd party content), although pre-existing multi-region OAR files may require replacing should the file format change as a result of adoption by OpenSim.

In the meantime, Ilan Tochner, Kitely’s CEO has offered a workaround for people to import their own multi-region builds to Kitely ahead of the new file format being adopted.

Related Links

Curiosity: getting ready to zap around

Mission logo

Work continues on readying Curiosity for surface operations on Mars, with characterisation phase well underway.

The week has seen the rover’s Chemistry and Camera system – ChemCam – undergoing its calibration tests using a target system located towards the back of the rover, while scientists have been looking for candidates for the first full test firing of the system at a suitable surface target.

ChemCam is a complex system split between Curiosity’s mast and body. The mast unit is the large box-like unit at the top of the mast. It contains a laser unit, a remote micro-imager (RMI) and a telescope for focusing both.

The Chemcam mast element

The body unit carries three spectrographs for chemical analysis and has its own power supply and an electronic interface to the rover’s central computer system.

ChemCam has two main functions, split between the laser system (the Laser-induced Breakdown Spectroscopy (LIBS), to give it its proper name) and the Remote Micro-Imager (RMI).

LIBS is designed to fire series of laser pulses at a target spot smaller than 1 millimetre on the surface of rocks and soils, vaporizing it. Light from the resultant plasma is captured by the telescope and sent via fibre-optics to the on-board spectrographs for analysis, which should provide information in unprecedented detail about minerals and micro structures in Martian rocks. Additionally, the laser can be used to remove dust from the surfaces of rocks, allowing the drill on Curiosity’s hand to obtain samples of the rock free from surface contaminants.

The RMI provides black-and-white images at 1024×1024 resolution in a 0.02 radian (1.1 degree) field of view – approximately equivalent to a 1500mm lens on a 35mm camera. RMI has two functions. In the first, it will be used in conjunction with LIBS to identify suitable targets and target locations (targets can be selected autonomously or via Earth-based selection and command). Working independently of LIBS, it will be used to obtain close-up images in support of robot arm-mounted experiments or provide images of very distant objects.

This week, ChemCam was calibrated using a target system mounted on the rear section of the rover, mounted below the UHF antenna. As a result of this, ChemCam was confirmed ready for operations, and is expected to make it first test-firing on an actual Martian rock sample on Saturday August 18th. The sample is provisionally designated N165, and sits a short distance from the rover.

ChemCam’s first Martian target

ChemCam is a joint US / French experiment, with the US Los Alamos National Laboratory providing the body unit, the French national space agency (CNES) proving the mast unit (RMI, laser, etc.) and JPL the fibre-optic link between the two.

Continue reading “Curiosity: getting ready to zap around”