IXV paves the way for PRIDE and more

An artist's impression of ESA's IXV lifting body attached to its upper sage booster during its first sub-orbital flight
An artist’s impression of ESA’s IXV lifting body attached to its upper sage booster during its first sub-orbital flight

On Wednesday, February 11th, the European Space Agency (ESA) launched a Vega rocket from their Guiana Space Centre in French Guiana, South America. The rocket has been Europe’s launch system for lightweight payloads since 2012, and in this capacity it has generally been used to lift Earth observation mission payloads into polar orbits, where they can see as much of the Earth’s surface as the planet rotates beneath them.

The February 11th mission was different, however. This was launched due west, out over the Atlantic and directly towards Africa. And, rather than carrying a satellite, the rocket carried a new, experimental spaceplane, very unglamorously called IXV,  for Intermediate eXperimental Vehicle.

Dubbed a “mini-shuttle” by some in the media, IXV is more correctly a lifting body design. That is, it has no wings of any description. Instead, it uses its own aerodynamic shape to generate lift and stability during re-entry into the Earth’s atmosphere. This particular principle of flight isn’t new. Lifting body designs have been used for a number of experimental purposes over the years, including in the 1960s and 1970s as NASA investigated potential designs for a reusable space vehicle (although the evolving mission requirements for the space shuttle meant that a lifting body design was eventually rejected in favour of a delta wing configuration).

The IXV mission
The IXV mission

In popular culture, and for those old enough to remember, footage of the crash and disintegration of a lifting body piloted by Bruce Peterson, was used in the opening titles of the TV series The Six Million Dollar Man. Unlike the fictional Steve Austin, however, Peterson survived his crash without the aid of bionics, although he did lose his sight in one eye … courtesy of an infection which occurred while he was in hospital after the crash. More recently, the use of a lifting body approach has been been demonstrated by Sierra Nevada’s Dream Chaser vehicle, which had been intended to fly crews to and from the International Space Station.

Europe’s IXV is an uncrewed vehicle, weighing just under 2 tonnes. It’s primary objective is to research the re-entry and flight characteristics of such a vehicle shape and to test the re-entry shielding technologies that ESA are developing. All of this is with a view to developing a new generation of reusable space vehicles that could be employed for both crewed and uncrewed missions. The first of these is likely to be PRIDE – the Programme for Reusable In-orbit Demonstrator in Europe – a genuine spaceplane using a combination lifting body / winged design.

ESA's PRIDE aims to demonstrate the use of a reusable spaceplane in satellite launch operations
ESA’s PRIDE aims to demonstrate the use of a reusable spaceplane in satellite launch operations

PRIDE is designed to be launched atop a rocket and, once in orbit, deploy satellite payloads prior to returning to Earth for a conventional runway landing, refurbishment and reuse. In this, it would be somewhat similar to the US Air Force’s uncrewed and classified X-37B spaceplane, which is capable of long duration orbital flights, notching-up some 1,367 days in space in just 3 missions between 2010 and 2014. However, unlike the X-37 programme, which is believed to be both an advanced technologies test vehicle and potentially capable of undertaking reconnaissance activities when in orbit, PRIDE would be a purely civilian operation.

Another potential use for the technologies seen in IXV is in providing the means to operate reusable boosters as a part of Europe’s next generation of launch vehicles, which would be capable of flying themselves back to a safe landing after use. Lifting body technologies and the re-entry systems used on IXV might also be used in missions to returns samples from Mars and the asteroids to Earth, and spaceplane technologies in general might one day form a part of ESA’s strategy for ferrying crews to / from orbital space facilities in the future.

The technologies being tested by IXV may one day be used in reusable boosters forming a part of ESA's next generation of launchers
The technologies being tested by IXV may one day be used in reusable boosters forming a part of ESA’s next generation of launchers

IXV’s maiden flight was relatively short – just under 2 hours in duration – and sub-orbital in nature. Boosted to an altitude of around 450 kilometres (281 miles), the vehicle cruised over Africa prior to initiating re-entry through the Earth’s atmosphere at a speed of some 7.5 kilometres per second (just under 16,800 miles per hour), using its shape to generate lift and stability, and two tail-mounted “paddles” for steering. Once through the heat of re-entry and slowed to hypersonic speeds, a special parachute deployed to slow the vehicle to subsonic speeds. This allowed the main parachute system could be deployed, which brought the car-sized vehicle to a relatively “soft” splashdown at just 7 metres a second (12.5 mph), so it could be recovered by the vessel Nos Aries.

The entire mission, from launch to splashdown, occurred almost precisely on schedule. Only a slight delay prior to lift-off causing the schedule to be adjusted. Ironically, recovery of the vehicle following splashdown took almost as along as the mission itself, and an overcast sky in the recovery zone presented images being captured of the vehicle’s descent by parachute.

Nevertheless, the mission was a great success. Now begins a long trawl through the data gathered by some 300 instruments and sensors spread throughout and over the little spaceplane.

All images and video, courtesy of the European Space Agency

LG morph Cardboard into plastic to rival Samsung in the mobile VR world

LG's VR for G3 uses Google Cardboard to bring VR to users of their G3 'phones
LG’s VR for G3 uses Google Cardboard to bring VR to users of their G3 ‘phones

In June 2014, Google informed the world that, in order to enjoy a VR experience on your mobile ‘phone, all you need is … Cardboard. Then, as I reported at the end of 2014, Samsung announced the availability of its Gear VR headset, which utilises their Galaxy Note 4 phablet and technology from Oculus VR, while Zeiss released VR One for the Samsung Galaxy S5 and iPhone 6.

Now, not to be outdone, Samsung’s home-grown rival in the world of mobile devices and consumer electronics, LG, is also getting in on the act.

On Monday, February 9th, LG announced the availability of VR for their G3 handsets. Like Google’s DIY cardboard kit (made available in full kit form by Dodocase, to save you having to source the parts yourself), VR for G3 is a hand-held unit providing a set of optics into which LG’s new range of G3 ‘phones can sit. In fact, not only does it look like Google Cardboard’s grown-up cousin, it is actually based on the cardboard headset design and is intended to be used with the Google Cardboard development environment for mobile VR experiences, and any apps built using that environment.

What’s more, it’s free. Well, free for those buying a new LG G3 handset, and then possibly only for a limited time period. Currently, no details have been released on pricing once the promotional period has ended. It is also currently unclear if VR for G3 will be made available as a separate accessory for the G3 ‘phone.

The hand-held headset is modelled on Google's original Cardboard DIY headset, and utilises the Cardboard development environment and applications
The hand-held headset is modelled on Google’s original Cardboard DIY headset, and utilises the Cardboard development environment and applications

“This is just the beginning of the virtual reality movement, which until recently was expensive and inaccessible to everyday consumers,” Chris Yie, vice president and head of marketing communications at the LG Electronics Mobile Communications, was quoted as saying in a press release from the company announcing the move. “By leveraging Google Cardboard, not only are regular consumers able to participate in the VR experience, we’ll be able to introduce this technology to future developers who may one day show us how VR can be used to improve our lives.”

VR for G3 will be rolled-out across LG’s global markets over the coming month, and the promotion will include a code allowing purchasers of the handset and headset to download the VR game Robobliteration.

With a screen resolution of  2560 x 1440, and packing a whooping 538 pixels-per-inch, the G3 handset is seen by LG as an ideal candidate for running immersive VR applications, and the hand-held headset includes optics specifically designed to leverage the screen’s capabilities.  As with Google’s original Cardboard design, a ring mounted on the left side of the headset, together with a small magnet within the unit work with the gyroscope sensor in the G3 to select applications and scroll through menus without the user needing to touch the display.

The G3 'phone sits within the snap-one cover of the headset, but the unique design of the 'phone, with it's back-mounted sleep button meanes that it doesn't have to be removed in order to place the phone into, or bring it out of, sleep mode
The G3 ‘phone sits within the snap-one cover of the headset, but the unique design of the ‘phone, with it’s back-mounted sleep button means that it doesn’t have to be removed in order to place the phone into, or bring it out of, sleep mode

Google are also keen to emphasise their involvement in LG’s entry in to the VR marketplace. “With Google Cardboard, we wanted to create more immersive and delightful experiences for anyone on their mobile devices,” Andrew Nartker, Product Manager for Google Cardboard is also quoted as saying in the LG press release. “We are excited about VR for G3, and the rich ecosystem of developers and manufacturers who are innovating with Google Cardboard and making VR more easily accessible.”

How much of an actual market exists for mobile VR has yet to be seen (by necessity, VR-on-the-go is more suited to sitting down rather than wandering the streets, so many might perfer to await the arrival of Oculus Rift CV-1 and similar headsets). However, it would appear that manufacturers like LG might see it as a way of reinvigorating ‘phone sales in the face of an saturated market.

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All images courtesy of LG Electronics Mobile Communications Company.

 

“I spy with my big eye…” and landing a rocket on Earth

CuriosityNASA’s Curiosity rover has been a busy bunny on Mars. Currently still parked in the “Pahrump Hills” terrain on the lower slopes of “Mount Sharp”, the Mars Science Laboratory (MSL) rover has now completed its latest drilling activity, collecting samples from a rock dubbed “Mojave 2”.

This isn’t actually the rock from which the science team had originally hoped to gather samples. That rock, dubbed “Mojave” broke apart as a result of the percussive action of the rover’s drill during a “mini-drill” test. As a result, the rock was ruled out as a sample gathering target. “Mojave” was of particularly interest to scientists as Curiosity had images tiny, rice-grain sized crystalline minerals that might have resulted from evaporation of a drying lake, thus presenting the science team with a further insight into environmental conditions within Gale Crater.

To counter this loss, the team relocated Curiosity to  “Mojave 2”, another rock within the same outcrop as “Mojave”, and which exhibits similar crystalline features. In doing so, the team were able to bring into play software improvements only recently uploaded to the rover as a part of an overall systems upgrade, which was deployed to one of the rover’s two computer systems at the end of January.

The software improvements for the drill are the result of investigations into the fracturing of a rock during a previous attempt to obtain samples prior to the rover arriving on “Mount Sharp”. Like an Earth-based hammer drill, the rover’s drill uses a percussive action, so that as well as drilling into a rock, the drill bit effectively hammers its way into the rock. In all, there are six settings governing the amount of percussive energy used during drilling, which range from a gentle tapping (level 1) through to hammering at the rate of 30 times a second with a 20-fold increase in energy imparted (level 6).

During early drilling operations the software monitoring these percussion settings “learned” that defaulting to the “level 4” setting best met the needs of gathering samples in the harder rock types the rover initially encountered. However, this was proving too forceful for the softer rocks closer to, and on, “Mount Sharp”, but the software was unable to switch down to a lower setting.

The drill hopes on "Mojave 2" captured by Curiosity's Mastcam. Towards the top is the small, "mini drilling" test bore, just a couple of centimetres deep, created on Sol 881 (January 28th, 2015, PDT) and some 10 centimetres below it, the sample-gathering bore hole, some 6.5 centimetres deep, cut on Sol 882 (January 29th, 2015, PDT).
The drill holes on “Mojave 2” captured by Curiosity’s Mastcam. Towards the top is the small, “mini drilling” test bore, just a couple of centimetres deep, created on Sol 881 (January 28th, 2015, PDT) and some 10 centimetres below it, the sample-gathering bore hole, some 6.5 centimetres deep, cut on Sol 882 (January 29th, 2015, PDT).

The new update causes the drill software to reset to “level 1” after each drilling operation, and then step through the levels incrementally until the ideal is found. As a result, a sample was gathered from “Mojave 2” without the drill needing to step beyond the “level 2” percussion action.

Drilling operations on “Mojave 2” took place on Sol 881 and Sol 882 (January 28th and 29th, PDT, respectively). As per standard operating procedure, the first drilling operation was a test “mini drilling” to see how the rock responded to encroachment and cutting. The second, which took the dill to a depth of around 6.5 centimetres (2.6 inches). The gathered samples were then sifted and sorted through the CHIMRA system in the rover’s turret, prior to being transferred via the surface scoop to Curiosity’s primary laboratory systems, ChemMin and SAM.

At the same time as Curiosity was carrying out its initial analysis of the “Mojave 2” rock, NASA released an image captured by the HiRise (High Resolution Imaging Science Experiment) carried aboard the orbiting Mars Reconnaissance Orbiter (MRO), which forms the mainstay of the rover’s communications with Earth. The image, which was taken on December 13th, 2014, reveals Curiosity mid-way through its “walkabouts” in “Pahrump Hills”, when it was seeking potential targets of interest for further study.

While not the first time the rover has been imaged from orbit, this is one of the clearest pictures from the rover yet capture from an altitude of around 280 kilometres (175 miles) above the surface of Mars.

"I see you!" - MRO's HiRise image of the curiosity rover, obtained on December 13th, 2014, as the rover explores the "Pahrump Hills" region on a basal slopes of "Mount Sharp"
“I see you!” – MRO’s HiRise image of the curiosity rover, obtained on December 13th, 2014, as the rover explores the “Pahrump Hills” region on a basal slopes of “Mount Sharp”

Initial results from ChemMin (the Chemical and Mineralogy) instrumental has shown that the rock was likely effected by water that was much more acidic in nature than evidenced through the analysis of other rock samples obtained by the rover. The still-partial analysis shows a significant amount of jarosite, an oxidized mineral containing iron and sulphur that forms in acidic environments. This raises the question of whether the more acidic water was part of environmental conditions when sediments were being deposited to form “Mount Sharp”, or the result of fluids soaking the rocks at a later time.

ChemMin was also unable to identify a clear candidate mineral for the crystalline deposits which first attracted the science team to the outcrop; this presents the possibility that the minerals responsible for originally forming the crystals may have been leached away over time and replaced by other minerals during later periods of wet environmental conditions.

It is hoped that SAM – the Sample Analysis at Mars – suite of instruments may be able to reveal more about the nature and composition of the samples once they have completed their round of analysis. Depending on the outcome of this work, Curiosity may be ordered to gather a further rock sample from “Pahrump Hills”, or may be ordered to continue upwards and into new territory on “Mount Sharp”.

Continue reading ““I spy with my big eye…” and landing a rocket on Earth”

Of mansions and motifs

Explore the Great Gatsby - the Buchanan's mansion and pier with its green light from Gatsby's estate: "“I thought of Gatsby's wonder when he first picked out the green light at the end of Daisy's dock. He had come a long way to this lawn and his dream must have seemed so close that he could hardly fail to grasp it. He did not know that it was already behind him."
Explore the Great Gatsby – the Buchanan’s mansion and pier with its green light from Gatsby’s estate: ““I thought of Gatsby’s wonder when he first picked out the green light at the end of Daisy’s dock. He had come a long way to this lawn and his dream must have seemed so close that he could hardly fail to grasp it. He did not know that it was already behind him.”

At 09:00 SLT,  the Seanchai Library’s retelling of  F. Scott Fitzgerald’s tragic tale, The Great Gatsby draws to a close as Corwyn Allen reads the final part of the story. The reading will take place at Explore the Great Gatsby Online, the interactive venue conceived and developed by Caledonia Skytower as a part of Seanchai Library’s presence in Kitely, and operating in support of a production of Simon Levy’s stage adaptation of The Great Gatsby, which also ends it run at the Tacoma Little Theatre (TLT) on February 8th.

I’ve covered Explore the Great Gatsby twice  so far in this blog. The first time as a result of an invitation extended to me by Caledonia and TLT’s Managing Artistic Director Chris Serface ahead of the official opening of the installation and the play. This gave me the opportunity to preview the unique collaborative, cross-functional and educational nature of the partnership between Seanchai Library and TLT. My second, more recent visit, was to explore the initial sets visitors to the installation would be able to explore, and the opportunities within them to discover more about the story, F. Scott Fitzgerald’s writings, and the man himself.

As indicated in both of those articles, the Explore the Great Gatsby installation was intended to grow over time, thus encouraging visitors – particularly those who attended TLT’s performances of the play –  to make return visits. Given the significance of Sunday, February 8th as noted above, I also decided to take a further trip to Explore the Great Gatsby and see the latest additions and updates.

Explore the Great Gatsby - Gatsby's mansion: "The one on my right was a colossal affair by any standard—it was a factual imitation of some Hôtel de Ville in Normandy, with a tower on one side, spanking new under a thin beard of raw ivy, and a marble swimming pool, and more than forty acres of lawn and garden."
Explore the Great Gatsby – Gatsby’s mansion: “The one on my right was a colossal affair by any standard—it was a factual imitation of some Hôtel de Ville in Normandy, with a tower on one side, spanking new under a thin beard of raw ivy, and a marble swimming pool, and more than forty acres of lawn and garden.”

New since my last visit is the Gothic opulence of Jay Gatsby’s “new money” mansion, its great towers and spires rising high above the trees, fairly shouting news of the wealth of their owner to the world at large. The scene of lavish parties – all intended to lure Daisy Buchanan to his door – the mansion’s ground floor can be explored by visitors, and several iconic elements have been reproduced, including the location of the final scene of tragedy, the swimming pool. There are a number of interactive elements to the mansion, which provide gateways to further information on the novel, so careful examination of the rooms is encouraged!

Tom and Daisy Buchanan’s mansion (which serves as a façade for a model of the Tacoma Little Theatre), has undergone further exterior work, allowing it to stand in strong contrast to Gatsby’s ostentatiousness, exactly as F. Scott Fitzgerald intended.  Thus it – and the bay which sits between it and Gatsby’s edifice – serves to underline Fitzgerald’s observation of the divide that existed between those of established wealth and those newly-rich.

Explore the Great Gatsby - The buchanan's mansion: "Their house was even more elaborate than I expected, a cheerful red-and-white Georgian Colonial mansion, overlooking the bay ... The lawn started at the beach and ran toward the front door for a quarter of a mile, jumping over sun-dials and brick walks and burning gardens."
Explore the Great Gatsby – The buchanan’s mansion: “Their house was even more elaborate than I expected, a cheerful red-and-white Georgian Colonial mansion, overlooking the bay … The lawn started at the beach and ran toward the front door for a quarter of a mile, jumping over sun-dials and brick walks and burning gardens.”

With a wealth of interactive elements throughout, including links to the Tacoma Little Theatre, resources that explore the story of the Great Gatsby in more detail, and the opportunity to really immerse yourself a a piece of truly great American literature, Explore the Great Gatsby is very much worth taking the time to visit – and if you haven’t already done so, I’d urge you to so – it will remain open and available to visitors through until March 1st, 2015.

Signing-up to Kitely (if you need to) is easy, and the Seanchai Library team provide the necessary guidance for those who might need it. What’s more, once you are signed-up, you have the freedom to explore the rest of Seanchai Library’s extensive projects and offerings in both the Seanchai Homeworld, and through their satellite worlds.

Explore the Great Gatsby - you can also explore other locations within the installation, such as the Fitzgerald Gallery, the Welcome Centre and that other iconic landmark from the the story, the Valley of Ashes: "But above the grey land and the spasms of bleak dust which drift endlessly over it, you perceive, after a moment, the eyes of Doctor T. J. Eckleburg."
Explore the Great Gatsby – you can also explore other locations within the installation, such as the Fitzgerald Gallery, the Welcome Centre and that other iconic landmark from the the story, the Valley of Ashes: “But above the grey land and the spasms of bleak dust which drift endlessly over it, you perceive, after a moment, the eyes of Doctor T. J. Eckleburg.”

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All change, getting virtual on Mars and watching the asteroid go by

CuriosityThe start of the year has brought – and is bringing – some changes to the Mars Science Laboratory mission. The first change has occurred here on Earth. On January 5th, 2015, John Grotzinger from the California Institute of Technology stepped down as the mission’s principal Project Scientist in overall charge of a team of some 500 people from across the globe who are operating the rover and its suite of scientific instruments.

Recently promoted to chair Caltech’s Division of Geological and Planetary Sciences, Grotzinger will still be involved in the mission, but his new responsibilities mean he cannot reasonably continue in such a lead role within the project. Stepping into his shoes, therefore, is Ashwin Vasavada of NASA’s Jet Propulsion Laboratory. He has been serving in the role of Deputy Project Scientist since the mission’s inception 2004, and has been intimately involved in both the development of the mission’s science packages and the rover itself. As such, he is ideally placed to take over from Grotzinger.

“John Grotzinger put his heart and soul into Curiosity for seven years, leaving a legacy of success and scientific achievement,” he said on taking over the role. “Now I look forward to continuing our expedition to Mars’ ancient past, with a healthy rover and a dedicated and passionate international team. And yes, this is all just incredibly cool.”

Ashwin Vasavada of NASA’s Jet Propulsion Laboratory, Pasadena, California, took over has the MSL’s Project Scientist from John Grotzinger at the start of January, 2015

Meanwhile, on Mars, Curiosity is engaged in further studies of rocks within the “Pahrump Hills” area on the lower slopes of “Mount Sharp”. These studies will involve drilling for rock samples from at least one more target of interest,  prior to the rover continuing its climb up the flank of the mountain.

The initial target for sample gathering has been dubbed “Mojave”, which appears to be rich in crystalline minerals. Slightly smaller than grains of rice, the structures first appeared on early images of the rock captured by the rover, and have caused intense – no pun intended – curiosity among mission scientists.

“We don’t know what they represent,” Vasavada said of the mineral forms and the decision to target “Mojave” for drilling. “We’re hoping that mineral identifications we get from the rover’s laboratory will shed more light than we got from just the images and bulk chemistry.”

Prior to drilling for actual samples, Curiosity was first ordered to carry out a “mini drilling” operation. This is a routine test to ascertain a number of things prior to committing to a full-on sample gathering exercise. These include making sure the rock is stable enough for a full drilling operation, gathering data of the reaction of the drill to penetrating the rock surface, ensuring any drilling operation will not cause undue vibration within the rover’s mechanisms, and so on.

A unique view of the "mini drilling" operation on "Mojave". Captured by Curiosity's Hazcam navigation cameras, the image shows the rover's "hand" oriented such that the dril (visible with its two steadying arms) is placed against the rock
A unique view of the “mini drilling” operation on “Mojave”. Captured by Curiosity’s Hazcam navigation cameras, the image shows the rover’s “hand” oriented such that the drill (visible with its two steadying arms) is placed against the rock, with the peak of “Mount Sharp” forming a backdrop.

The initial mini-drilling operation took place on January 13th 2015, during the 867th Martian day, or Sol, of Curiosity’s work on Mars. It marks the third phase of science operations in the “Pahrump Hills” area, having been preceded by a “walkabout” of the area in which potential target sites for detail investigation were noted prior to follow-up examinations of several of them using some of the rover’s on-board systems, such as the Alpha Particle X-Ray Spectrometer and the Mars Hand Lens Imager (MAHLI), both of which are also mounted on the “hand” or turret at the end of the rover’s robot arm.

Once samples from “Mojave” have been collected, they’ll be passed through the CHIMRA system inside the turret, which will prepare them for delivery to the rover’s main on-board science suits, SAM and ChemMin. The latter (standing for Chemistry and Mineralogy instrument), will hopefully reveal a lot more about the chemical composition of the crystals. Additionally the drilling operation itself should reveal whether the crystals are only at the surface, like a salty crust, or are also deeper in the rock, which itself might lead to clues about their origins

“There could be a fairly involved story here,” Vasavada said. “Are they salt crystals left from a drying lake? Or are they more pervasive through the rock, formed by fluids moving through the rock? In either case, a later fluid may have removed or replaced the original minerals with something else.”

Two other potential targets for drilling operations are also under consideration before the rover moves out of the “Pahrump Hills” area.

The view is a mosaic of four focus-merge images created by Curiosity from 40 images acquired using MAHLI on Sol 809 (November 15th, 2014 PDT). It shows an area of the “Mojave” rock which has been cleaned by the rover’s dust removal tool in order to reveal the tiny rice-like crystalline deposits. The penny in the lower left is to scale with the mosaic

Continue reading “All change, getting virtual on Mars and watching the asteroid go by”

The Beagle had landed

An artist's impression of Beagle 2 on Mars (credit: European Space Agency)
An artist’s impression of Beagle 2 on Mars (credit: European Space Agency)

In June 2003 the European Space Agency launched a pair of vehicles to Mars. The larger of the two, an orbiter vehicle called Mars Express, is still in operation today, albeit often overlooked by the media in favour of its American cousins also in orbit around the Red Planet.  The other vehicle, piggybacking on Mars Express, was a tiny lander (quite literally, being just 39 inches across) called Beagle 2.

Designed to search for signs of life, past or present on Mars, Beagle 2 was the Mission That Almost Never Was, because at the time it was proposed, no-one outside of those wanting to build it, wanted it. And yet, even today, the science package it did eventually take to Mars is one of the most remarkable feats of science engineering put together, with capabilities that will not be repeated until NASA flies their one tonne Mars 2020 mission at the start of the next decade.

Sadly, for all its innovation and despite overcoming the odds to actually fly to Mars, Beagle 2 never achieved its goals; all contact was lost on the very day it was due to land on the Red Planet, December 25th, 2003. What happened to it remained a mystery for twelve years, but on Friday, January 16th, members of the Beagle 2 team were able to reveal that the fate of the plucky little lander was now known.

The Beagle 2 story begins in April 1997, when the European Space Agency held a meeting to discuss the possibility of flying an orbiter mission to Mars in 2003, following the failure of an earlier mission. This new mission would be called “Mars Express”, both in recognition of the exceptionally short lead-time to develop and fly it, even using instruments and systems developed for the failed mission, and for the fact that in 2003, Earth and Mars would be the closest they’ve been for some 60,000 years, allowing anything launched around the middle of that year to reach Mars in a comparatively short time.

Colin Pillinger, the man very much at the centre of Beagle 2, and who brought the mission to the public eye
Colin Pillinger, the man very much at the centre of Beagle 2, and who brought the mission to the public eye

Professor Colin Pillinger, a planetary scientist and a founder of the Open University’s prestigious Planetary Science Research Institute (since merged with the OU’s Department of Physics and Astronomy), attended the meeting together with his wife Judith, also a planetary scientist. At the time, Professor Pillinger was one of a number of scientists involved in investigating whether or not biogenic features had been discovered in a meteorite found in Antarctica, but which had originated on Mars.

This particular debate was focused on a piece of rock called ALH84001, regarded as one of the oldest pieces of the Solar System, being just over 4 billion years old, and which formed at a time when Mars was likely a warm wet planet. It had been raging for a year with no sign of abating, and Professor Pillinger had already come to the conclusion that one way to settled it would be to put a life sciences package actually on Mars.  He realised the proposed Mars Express mission presented the perfect opportunity for doing so, as did his wife. So much so, that by the time they got back to the UK, she had the perfect name for a mission designed to seek out evidence of life on Mars: Beagle 2, named for the vessel commanded by Captain Robert FitzRoy that carried Charles Darwin on his seminal voyage of discovery.

The microscopic structures revealed by a scanning electron microscope deep within a fragment of ALH84001 that suggested biogenic origins
One of the microscopic structures revealed by a scanning electron microscope deep within a fragment of ALH84001 that suggested biogenic origins

Given all of the controversy surrounding ALH84001 and the question of possible microbial life on Mars that dated back to the Viking Lander experiments of the 1990s, you’d think the ESA would jump at the opportunity to put a life sciences mission on Mars. Not so; for one thing, others also saw Mars Express as an opportunity to fly their projects to Mars and were busy lobbying. More to the point, it was held that the 6-year time frame for developing a lander mission from scratch was too short.

However, Colin Pillinger was not one to be deterred. In the UK he brought together a team from academia and industry, including Doctor Mark Sims, who was to prove pivotal in the  engineering design of the lander. With many of those involved in the nascent project initially working on it entirely in their own time, Beagle 2 rapidly developed from a series of rough designs “on the backs of beer mats”, to a proposal which, when presented to ESA managers, so impressed them, they provisionally agreed to the idea of flying a lander to Mars – but only if the UK was able to fund it. No money would be forthcoming from ESA.

Dr. Mark Sims of the University of Leiceter, who lead the engineering team responsible for Beagle 2, seen with another model of the lander (image: University of Leicester)
Dr. Mark Sims of the University of Leicester, who lead the engineering team responsible for Beagle 2, seen with another model of the lander (image: University of Leicester)

Thus began one of the most remarkable public relations exercises in annals of space history, with Beagle 2 becoming a household name in the UK, as Colin Pillinger sought to promote in on television, the radio, through newspaper and magazines, and giving public presentations. Space advocacy groups were rallied to the cause, celebrities were brought in to add their weight to things, Parliament and industry were lobbied and won over. In the end, the entire £44 million (US $70 million) was raised, with 50% coming from the UK government and the rest from the private sector.

Continue reading “The Beagle had landed”