Tag: Spaceflight

Between the comets

Posted on by Inara Pey
Siding Spring (circled) passing Mars (the glowing object, bottom left) as seen via the SLOOH telescope at the Pontificia Universidad Católica De Chile (PUC) Chile (images via SLOOH live feed, October 19th, 2014)
Siding Spring (circled) passing Mars (the glowing object, bottom left) as seen via the SLOOH telescope at the Pontificia Universidad Católica De Chile (PUC) – image via SLOOH live feed, October 19th, 2014

It’s now a week since Siding Spring passed by Mars as it hurtled through the inner solar system for what might be the very first time. As I reported on the day of the comet’s flyby, C/2013 A1 – to give the comet its official designation – passed by Mars at a distance of around 136,000km (85,000 miles) and at a speed of some 56 kilometres (35 miles) per second. Since then, the comet reached perihelion – the point of its closest approach to the Sun (Saturday, October 25th, 2014), and it is now on its way back out of the solar system, travelling “up” and out of the plane of the ecliptic as it does so.

It will not be back this way for at least a million years.

Despite some getting their knickers in something of a knot over video footage apparently showing an “explosion”/ “electromagnetic pulse” in the Martian atmosphere around the time of the comet’s closest approach to Mars. In particular, the video footage – some 75 images captured by amateur astronomer Fritz Helmut Hemmerich M.D., captured between 21:00 and 22:00 UT on October 19th, from an altitude of some 1200 metres in Tenerife, have had proponents of the “electric universe” theory (aka Plasma Cosmology) in something of a tizzy.

Quite what caused the artefact in Dr. Hemmerich’s images is unclear – but lens flare cannot be entirely ruled-out. Given that within hours of the comment’s passage the various orbital vehicles around Mars started popping-up and reporting their status, it would appear highly unlikely that the artefact was anything to do with some kind of massive electrical discharge within the Martian atmosphere, simply because it is not unreasonable to suppose had this been the case, it would have adversely affected at least some of the craft.

Siding Spring passing Mars, October 19th, 2014 (image: Scott Ferguson, Florida, USA)
Siding Spring passing Mars, October 19th, 2014 (image: Scott Ferguson, Florida, USA)

As it is, all of NASA’s vehicles reported absolutely no ill effects from the comet’s passage or as a result of the period of “peak dust flux” when they were expected to be at the greatest risk from the passage of very high velocity dust particles (travelling at tens of kilometres per second), and all were back in full operation within hours of the comet’s passage past Mars, as were both India’s MOM and Europe’s Mars Express. NASA’s Mars Reconnaissance Orbiter (MRO) in particular remained in contact with Earth throughout the time the comet passed by Mars and reported nothing to suggest the Tenerife images were showing anything of major significance occurring around Mars at the time of the flyby.

Currently, all of NASA’s orbital assets are continuing to study the comet and how dust and debris ejected from it has affected the Martian atmosphere, although it is expected to be several more days before the data being returned has been analysed and assessed.

In the meantime, on Friday, October 24th, and in a timely move, the European Space Agency reminded the world of another cometary encounter that is taking place. This was via the public premier of Ambition, a short film by Tomek Bagiński, starring Aidan Gillen (“Petyr Baelish” in Game of Thrones) and Aisling Franciosi (“Katie” in The Fall).

The film takes a unique look at the decade-long Rosetta mission, which is only now commencing its primary mission to observe a comet at very close quarters, including landing a robot vehicle on the surface of the comet on November 12th, 2014.

Rosetta and Philae (image: European Space Agency)
Rosetta and Philae (image: European Space Agency)

Continue reading “Between the comets” →

Duck and Cover

Posted on by Inara Pey

Sunday October 19th marked the culmination of what is regarded as one of the most unique astronomical events to take place in human history – so unique, some commentators believe it may only happen once every million years or so: the opportunity to study something which may have existed before the Earth was created.

For the last several months, comet Siding Spring has been under observation as it hurtles through the solar system at an acute angle relative to the plane of the ecliptic – the imaginary line along which the planets orbit, and on Sunday October 19th, it made its closest approach to Mars, passing just in front of the planet relative to the Sun.

Siding Spring was first identified by Australian astronomer Rob McNaught, and bears the name of his observatory as a result, although officially it is catalogued as C/2013 A1. Since then, it has been under observation from a veritable armada of international space craft, and its passage past Mars presents further unique opportunities for observation and data-gathering.

Siding spring is a comet originating in the Oort cloud, and beleived to be making perhaps its first foray into the inner solar system, passing inside the orbit of Jupiter
Siding spring is a comet originating in the Oort cloud, and believed to be making perhaps its first foray into the inner solar system, passing inside the orbit of Jupiter

The comet has been identified as coming from the Oort cloud (or the Öpik–Oort cloud, to give proper recognition both astronomers who initially and independently postulated its existence). This is a spherical cloud of debris left-over from the creation of the solar system, occupying a huge area starting some 2,000-5,000 AU (2,000 to 5,000 times the distance from the Earth to the Sun) and extending out to around 50-100,000 AU – or about one light year away. Thus, Siding Spring represents some of the material “left-over” from the formation of the solar system 4.6 billion years ago – older than the Earth itself. In fact, such is the distance of the Oort cloud from the Sun, that some postulate the much of the material within it may actually come from stars which shared the same “stellar nursery” as the Sun.

There is nothing unique per se about comets coming from the Oort cloud – it is one of two places from which all comets originate, the other being the Kuiper belt (or Edgeworth–Kuiper belt, as it is also known in recognition of the two astronomers to postulate its existence in the form we now know it has). A disk of material also from the early history of the solar system, the Kuiper belt orbits the Sun at a distance of around 30-50 AU, and gives rise to “periodic” comets. These are comets which circle the Sun in periods of up to 200 years. Two of the most famous Kuiper belt comets are comet Halley, with it 76-year orbit, and comet Shoemaker-Levy 9, which broke-up during a close approach to Jupiter in 1992 prior to colliding with the gas giant in 1994.

Siding Springs passage through the solar system
Siding Springs passage through the solar system

What makes Siding Spring of interest to astronomers is that this is probably the first time in its long, cold history it has ever come inside the orbit of Jupiter since it was first nudged out of the Oort cloud. This led Dr Michael Brown, an astronomer at Monash University, to describe the comet as “essentially a refrigerator of pristine parts of the creation of the solar system. The particles it gives off are effectively opening up the door of the fridge so we can see what the solar system was like 4.6 billion years ago.”

John Grunsfeld, former astronaut and associate administrator for NASA’s Science Mission Directorate in Washington was equally enthused by the comet’s passage, referring to it as “a cosmic science gift that could potentially keep on giving.” Speaking at a press conference held earlier in the year to discuss NASA’s plans to observe Siding Spring, he continued, “The agency’s diverse science missions will be in full receive mode.” He went on, “This particular comet has never before entered the inner solar system, so it will provide a fresh source of clues to our solar system’s earliest days.”

The chance for scientific discovery notwithstanding, the comet’s path was initially a cause for concern, at least in terms of Mars’ future. Early attempts to track the comet’s likely route  “up” through the solar system suggested that rather than passing the Red Planet, Siding Spring would in fact smash into it.

Had the comet struck, estimates suggest it would have created a crater between 10 and 15km in diameter, depending on the actual size of the comet’s nucleus, thought to be between 700m and 1km across.  While that is certainly enough to result in quite an extraordinary bang and some severe changes in the Martian atmosphere (not to mention the sizable dent it would make in the planet’s surface), Mars has actually withstood much larger impacts in its time.

Take Hellas Basin, for example. It is the largest visible crater in the solar system, some 2,300km (1,440 miles) across, and with an ejecta ring some 7,000km (4,375 miles) across. It is believed to have been created by the impact of an asteroid some 400km (250 miles) in diameter.

The Hellas Basin, shown in purple in the image of the right, above. Deeper than Mount Everest is tall, the depression was likely caused by the impact of an asteroid some 400km across. The impact also resulted in the Tharsis Bulge on the opposite side of the planet, and shown in red in the image on the left, topped by the three massive Tharsis volcanoes, and split by the 5,000km length of the Vallis Marineris
The Hellas Basin, shown in purple in the image of the right, above. Deeper than Mount Everest is tall, the depression was likely caused by the impact of an asteroid some 400km across. The impact also resulted in the Tharsis Bulge on the opposite side of the planet, and shown in red in the image on the left, topped by the three massive Tharsis volcanoes, and split by the 5,000km length of the Vallis Marineris

As Grunsfeld noted, such is the scientific opportunity presented by the comet, that NASA has put a significant number of assets in the front line of tracking and observing Siding Spring. These include the Hubble Space Telescope, the Spitzer infra-red space telescope, the WISE infra-red space telescope, the Chandra X-ray observatory, the Kepler orbital observatory (used in the search for Earth-sized extra-solar planets) and more, as well a host of ground-based observatories.

Foremost in the front line, by dint of the comet’s close passage past Mars, are NASA’s orbital and surface vehicles there. Curiosity, Opportunity, the Mars Reconnaissance Orbiter (MRO), Mars Odyssey and MAVEN, together with Europe’s Mars Express and India’s MOM, are all watching the comet, although for the orbiting spacecraft, this comes with a degree of risk.

Siding Spring has been, and is, under observation by an armada of science probes and also from observatories on Earth
Siding Spring has been, and is, under observation by an armada of science probes and also from observatories on Earth – including these from NASA

Continue reading “Duck and Cover” →

Martian technology comes down to Earth; NASA asks students to help

Posted on by Inara Pey

CuriosityThere’s some interesting news coming from the Mars Science Laboratory, with NASA revealing that Curiosity is contributing to matters of safety here on Earth.

Over the decades, NASA has established a strong track record for space-focused technologies having spin-off applications here on Earth. The Apollo programme, for example, lead to some 1,400 patents and technical developments which impacted all of our lives. These have included:

  • Physical therapy and athletic development machine used by football teams, sports clinics, and medical rehabilitation centres
  • Water purification systems used in community water supply systems and cooling towers to kill bacteria, viruses and algae
  • Freeze-drying technology to preserve nutritional value and taste in foods; improvements in kidney dialysis arising from the need to recycle fluids in space
  • The widespread use of flame-resistant textiles used by fire fighters, service personnel, etc.
  • Sensor system to detect the presence of hazardous gases in oil fields, refineries, offshore platforms, chemical plants, waste storage sites, and other locations where gases could be released into the environment.
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Lance Christensen of NASA’s Jet Propulsion Laboratory, demonstrates the gas leak detection device developed using his tunable laser spectrometer develop for the Mars Science Laboratory

It is in reference to this last aspect of spin-off technologies that Curiosity is contributing to safety on Earth.

On Wednesday October 2nd, NASA’s JPL announced that technology developed for the Curiosity rover is now being tested by the Pacific Gas and Electric Company (PG&E) which should enable their personnel to identify possible leak locations, fast-tracking their ability to repair gas leaks.

The new system utilises laser-based technology developed for MSL to aid detection of Methane on Mars. It is a spin-off of the tunable laser spectrometer, developed by JPL science engineer Lance Christensen, and one of the principal science instruments carried within the body of the Mars rover. The PG&E application utilities elements of the laser system together with a tablet computer in a hand-held device. This allows field engineers to detect trace elements of gas coming from a leak by passing the detector over the ground above the line of the pipe. Testing is currently underway, and it is hoped that if successful, it will see the system introduced for general use in the US utility industry in 2015. It is particularly relevant to PG&E, after one of their gas pipes ruptured in 2010 and the resultant explosion killed eight people.

Curiosity’s compact spectrometer systems have already given rise to the testing of a new generation of compact, portable, multi-purpose spectrometers for use by geologists and researchers working in the field, and the development of this system with PG&E marks another significant step in NASA’s tradition of contributing back to technology, engineering, safety, etc., here on Earth.

NASA 3D Printing Contest for Students

3D printing has the potential to revolutionise many areas of life and business – both on Earth and in space. Earlier in 2014, for example, British Aerospace has received European Aviation Safety Agency (EASA) Form 1 certification approval to use a 3D printed part in one of their aeroplanes, and the European Space Agency (ESA) is investigating the use of 3D printing methods for space applications.

NASA, in partnership with the American Society of Mechanical Engineers Foundation has now opted to launch a competition for US school and college students, to design and submit a digital 3-D model of a tool that they think astronauts will need in space.

Introducing the competition in a video (below), NASA astronaut Doug Wheelock says, “As you know, we don’t have overnight shipping up in space, so when we really need something, we have to wait. To be able to make parts on demand will forever change that for us.”

The competition, launched in late September, has a closing date of December 15th, 2014. Two grand prizes are on offer: the winner of the 5-12 year age group will get a 3-D printer for his or her school, while the winner in the 13-19 age range will receive a trip to NASA’s Payload Operations in Huntsville, Alabama, where the student will watch his or her object manufactured on the International Space Station.The winners will be announced in January 2015, and full details for entry can be found on the Future Engineers website.

Continue reading “Martian technology comes down to Earth; NASA asks students to help” →

A Mars Namaste and taxis to the space station

Posted on by Inara Pey

CuriosityIt’s been a busy couple of weeks on and around Mars and with space exploration in general. This being the case, I’m going to be tagging some of the other items of potential interest to the end of this Curiosity update.

On September 24th, Curiosity obtained its first sample of rock gathered from the foothills of “Mount Sharp”, or Aeolis Mons as it is more correctly named. The sample was taken from a rock in the area dubbed “Pahrump Hills”, an uprising within the initial transitional zone between what is regarded as the floor of Gale Crater and the material making up the huge mound of “Mount Sharp” located at the centre of the crater.

The rover officially arrived within the area of interest on September 19th, and conducted surveys of its surroundings and a potential candidate area was selected for sample gathering. On September 22nd, an initial “mini drill” test operation was carried out on a rock surface in the target area, dubbed “Confidence Hills”, to assess its suitability for sample gathering.

A mosaic of images captured by Curiosity's Mastcam showing the Pahrump Hills area the rover is currently investigating (foreground) and the Murrary formation, a near-term destination, beyond
A mosaic of images captured by Curiosity’s Mastcam showing the Pahrump Hills area the rover is currently investigating (foreground) and the Murray formation, a near-term destination, beyond – click any image for full size

As noted in a previous update, “mini drilling” operations are used to test a potential target for a range of factors prior to actually committing the rover’s drill to a sample-gathering exercise, the intention being to ensure as far as possible that nothing untoward may happen which may damage the drill mechanism or adversely impact future sample gathering work.

The September 22nd mini drilling was important for two reasons; not only was it intended to assess the suitability of the target rock for sample gathering, it also marked the first time the drill cut into what is essentially “new” and “softer” material compared to previous drilling activities, and it was doubly unclear as to how the drill or the rock might react.

The bore hole image from the September 24th sample-gathering at “Parump Hills”. A “merged-focused product” combining a set of images captured by the Mars Hand Lens Imager (MAHLI) from just 2 centimetres above the hole, it show the bore cut by the rover’s drill and surrounding tailings which, interestingly, don’t share the same distinctive light gray colouring seen with samples gathered on the crater floor. The hole is 1.6cm across and about 6 cm deep. The images were taken on September 24th, 2014, during the 759th Sol, of Curiosity’s work on Mars

The sample-gathering drilling took place on September 24th, PDT (Sol 759 for Curiosity on Mars) and resulted in cutting a hole some 6 centimetres (2.6 inches) deep into the target rock and the successful gathering of tailings. “This drilling target is at the lowest part of the base layer of the mountain, and from here we plan to examine the higher, younger layers exposed in the nearby hills,” said Curiosity Deputy Project Scientist Ashwin Vasavada following the operation. “This first look at rocks we believe to underlie Mount Sharp is exciting because it will begin to form a picture of the environment at the time the mountain formed, and what led to its growth.”

Curiosity is liable to stay within the “Pahrump Hills” area for a while prior to moving up onto the Murray Formation above it, which is regarded as the formal boundary area between “Mount Sharp” and the crater floor, and as such is designated a target of particular interest. As a part of its studies of “Pahrump Hills”, and as well as gathering an initial rock sample, the rover has been surveying the rocks in its immediate surroundings with other instruments including the ChemCam laser system and the high-magnification Mars Hand Lens Imager camera, also mounted on the robot arm.

Of particular interest to the science team have been a series geometrically distinctive features on the rock surface. These are thought to be common to the Murray formation mudstones, and are believed to be the accumulations of erosion-resistant materials. They occur both as discrete clusters and as dendrites with formations arranged in tree-like branching. By investigating the shapes and chemical ingredients in these features, the team hopes to gain information about the possible composition of fluids at this Martian location long ago.

Another merged-focused image from MAHLI, showing accumulations of erosion-resistant materials in the “Pahrump Hills” area on the slopes of “Mount Sharp”. Similar features on Earth form when shallow bodies of water begin to evaporate and minerals precipitate from the concentrated brines. The width of the image covers about 2.2 centimetres, and it combines a series of images captured on September 23rd, 2014, during Curiosity’s 758th Sol

Currently, the sample gathered from the “Confidence Hills” are held within CHIMRA, the Collection and Handling for In-Situ Martian Rock Analysis system, in the rover’s robot arm. This is a mechanism that allows sample material to be graded by the size of the tailings by passing them through a series of sieves as the robot arm is vibrated at high rates, producing multiple samples which can then be delivered in turn to the rover’s onboard science instruments for detailed analysis.

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You can’t always get what you want …

Posted on by Inara Pey

CuriosityAugust 5th marked the 2nd anniversary on Curiosity’s landing on Mars. The “landiversary”, as NASA dubbed the occasion, passed in something of a subdued manner in many respects, featuring a re-run of the August 2012 video reviewing the MSL’s arrival on Mars. Reviews of the mission from the perspective of two years on from that remarkable lading didn’t start-up until the days after the anniversary, with videos and lectures from members of the mission team.

One of the films which did appear, directly out of Caltech, rather than NASA’s Jet Propulsion Laboratory (which is located on Caltech’s Pasadena, California, campus), is Our Curiosity, a 6-minute celebration of Curiosity’s mission, and humanity’s drive to explore, to seek, to learn, and to understand, narrated by Felicia Day and the superb Neil DeGrasse Tyson.

August 5th also marked my last MSL report, when Curiosity was some 3 kilometres from the lower slopes of “Mount Sharp”, the huge mound at the centre of Gale Crater, and the rover’s primary target for exploration. At that time, the rover had started to cross a region of chaotic terrain, marked by a rocky plateau cut by a series of sandy-bottomed valleys. The plateau itself proved to be littered with sharp-edges rocks and stones which had already caused some increase in the wear and tear being suffered by the rover’s wheels – albeit not as much as mission engineers had feared – by the time Curiosity had reached the edge of the nearest of the shallow valleys, which had been dubbed “Hidden Valley”.

The plan had been to use the valleys, where the sand would be less wearing on the rover’s aluminium wheels, to reach an exposed area of bedrook designated the “Pahrump Hills”, where Curiosity would engage in further rock sampling work prior to it continuing on to the “Murray Buttes”, the entry point for its ascent up the lower slopes of “Mount Sharp”.

However, rather than drive the one-tonne rover straight through the middle of the valley, where there are numerous dunes of potentially soft, wind-blown sand which might cause some difficulty traversing, the idea had been for Curiosity to skirt along the edge of the valley, where it was hoped the sand would be firmer and make for a better driving surface. Unfortunately, this proved not to be the case; as the rover proceeded along “Hidden Valley” it exhibited far more signs of wheel slippage than had been anticipated, giving rise to fears that it might get bogged-down in the sand were it to continue.

The sands of Mars: an image from Curiosity’s black and white Navcam system captured on August 4th, showing the loose sands the rover was traversing as it continued into “Hidden Valley” (click for full size)

As a result, the rover reversed course, driving back out of the valley. In doing so, it crossed the rocky “ramp” it had used to originally enter the valley, and one of its wheels cracked the slab-like rock’s surface, revealing bright material within, possibly from mineral veins. The rock, dubbed “Bonanza King” showed similar signs of origin as “Pahrump Hills”, so a decision was made to examine it as a possible substitute drilling site.

“Geologically speaking, we can tie the Bonanza King rocks to those at “Pahrump Hills”. Studying them here will give us a head start in understanding how they fit into the bigger picture of Gale Crater and Mount Sharp,” said Curiosity Deputy Project Scientist Ashwin Vasavada, before continuing, “This rock has an appearance quite different from the sandstones we’ve been driving through for several months. The landscape is changing, and that’s worth checking out.”

Continue reading “You can’t always get what you want …” →

Why we’ll take VR and virtual worlds to other planets

Posted on by Inara Pey
The first touchdown: human missions to the surface of Mars have long been dreamed about and planned for. Sometime in the next 30 years or less, they’ll become a reality. And VR, AR and virtual worlds are likely to play a role (image: SpaceX)

Sometime in the next thirty years, it is likely that humans will set foot on the surface of Mars. The mission that takes them there might be an international government-sponsored mission, or it might be the result of private endeavour. However it comes about, it will be the culmination of decades of planning, hopes and dreams stretching back beyond the birth of the space age.

There is much that a crew on such a mission will be taking with them in terms of hardware, equipment and technology. And it is very likely that when looking down the list of technologies they’ll take with them, one will be able to find virtual reality, virtual worlds and augmented reality – an in a variety of roles and uses.

Take the crew’s psychological health and well-being for example. A round-trip mission to Mars will take between two and 2.5 years to complete, depending upon the “class” of mission undertaken.

The two classes of Mars mission: opposition (l), which are launched when Earth and Mars are on the same side of the Sun, and conjunction class (r) are launched when the Earth and Mars are on opposite sides of the Sun both amount to a mission duration of 2- 2.5 years
The two classes of Mars mission: opposition (l), which are launched when Earth and Mars are on the same side of the Sun, and conjunction class (r) are launched when the Earth and Mars are on opposite sides of the Sun both amount to a mission duration of 2 – 2.5 years

Throughout that entire time, they’ll be completely isolated from everything we take for granted here on Earth – the freedom to wander outdoors, the sight of a blue sky, green hills, rivers, the sea, cities, lakes, people; they’ll be confined to enclosed spaces which really don’t offer too much in the way of privacy. They’ll even be confined to meals from a menu set months in advance, with no real option to give into a whim for a particular delicacy if it isn’t on their vessel.

For the majority of the mission time, the only people they’ll be able to directly converse with are their fellow crew members – with a minimum round-trip time delay in communications between Earth and Mars of 8 minutes (and potentially as much as 40 minutes through parts of the mission), having real-time conversations with loved ones on Earth simply isn’t going to be possible; they’ll have to rely on pre-recorded messages and video and e-mail.

In these circumstances, stresses are bound to develop, both for the individual members of the crew and, potentially, between team members, no matter how carefully selected for compatibility ahead of the mission or how well-trained. One way of potentially dealing with them is through the use of VR and virtual environments, as NASA and other organisations have been investigating for much of the last decade.

It’s not hard to imagine, for example, a crew going to Mars with a library of pre-filmed environments and events  which they can then explore and enjoy individually or together through the use of personal headsets – or for such a library to be updated with new items beamed via  something like OPALS to their craft. Such environments and activities could provide psychological relief from the confines of the space vehicle.

In June 2014, NASA’s OPALS system beamed the high-definition, 36-second movie “Hello, World” from the International Space Station (travelling at 28,000 kilometres an hour (17,500 mph) to a receiver on Earth in just 3.5 seconds (compared to the 10-12 minutes radio communications would have required. Systems like OPAL offer the key to providing very high bandwidth communications capabilities between Earth and Mars, allowing much more data to be passed back and forth (image: NASA)

Similarly, high fidelity virtual world environments which support direct interaction, such as through haptic feedback mechanisms, might provide the means by which crew members can “remove” themselves from the confines of their vehicle and enjoy a variety of activities, including something we take for granted in VWs today – the ability to create and build.

ANSIBLE (A Network of Social Interactions for Bilateral Life Enhancement) was an initial attempt by NASA, working with SIFT and All These Worlds, to explore how virtual worlds might be leveraged to provide astronauts with environments which could be shared or used individually, and which might offer a range of AI interactions as well.

A screen capture of the main ANSIBLE environment. While openSim probably won't be the VW of choice for a Mission to Mars, the ANSIBLE environment has been used as a means of assessing virtual world environments could each the psychological pressures face by a a confined crew on a long duration space mission
A screen capture of the main ANSIBLE environment. While OpenSim likely won’t be the VW of choice for a Mission to Mars, the ANSIBLE environment is perhaps the first step towards assessing how virtual world environments could ease the psychological pressures face by a confined crew on a long duration space mission (image: SIFT / All These Worlds)

An intriguing element with ANSIBLE was the exploration of the idea that virtual world environments could be asynchronously “shared” between crew members and their friends and family on Earth, allowing them to engage in shared content creation activities, for example, through the swapping back and forth of OAR files, the ability to engage in “shared” immersive games and so on. ANSIBLE researchers even suggested that used in this way, a personal virtual world space could enable an astronaut and their family “share” special occasions more personally than could be done via e-mail, radio or video.

Commenting on the used of immersive environments and haptic technologies in Moving to Mars: There and Back Again (Journal of Cosmology, 2010, Vol 12), Sheryl L. Bishop, Ph.D, noted, “Telepresence and full fidelity audio/video/3-D communication replay capability will provide for more effective psychological support and interaction for crew members and to families and friends back on Earth.”

In terms of crew welfare, virtual reality has another potential use: assisting in matters of fitness. Most current mission scenarios involve the crew travelling to and / or from Mars in a “weightless” environment. Such an environment can be detrimental to many aspects of human physiology – muscles, bones, heart, lungs, etc. It is therefore essential long exposure to weightlessness is countered by routine exercise of up to two hours every day.

Exercise is an essential part of life in micro-gravity, where muscles can easily atrophy, bones suffer calcium loss, the cardiovascular system weaken, etc., away from the pull of Earths gravity. VR could help make such exercise more interesting and help space crews “escape” to more Earth-like environments (image: NASA)

In the confines of a space vehicle, the opportunities for exercise tend to be limited and potentially boring. How much more pleasant it might be for an astronaut who, after lugubriously strapping themselves into a treadmill harness and making all the required tension adjustments ready for 30 or so minutes of going nowhere while staring at a bulkhead, could slip on a VR headset, and go for a run through a woodland park or along a beach, the sounds of nature or the waves in their ears?

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