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We will be explaining a little of the science behind the MDRS |
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experiments below, as our intrepid |
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crews brave the wilds of the martian atmosphere, sample the alien geology and take in the sights of a truly dark sky.
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KiwiSpace Mars Analog missions will simulate a manned expedition on the surface of planet Mars.The research conducted by the MDRS expeditions is very useful for the future exploration of Mars – such missions were performed by NASA prior to the Apollo trips to the Moon. The missions take place at the Mars Desert Research Station in Utah.
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Introducing Mars
Welcome to Mars!
Whilst the martian environment is considered 'most similar to Earth's' when compared to other planets in our Solar System, it really doesn't do justice to the weird and wonderful nature of the martian environment! Both Mars and Earth are 'terrestrial' planets, so called because you're able to wander around on them, like the Apollo astronauts did on the lunar surface 30 years ago. You would feel a little lighter on Mars than you're used to here on Earth though - because it's much smaller than the earth about half as wide and only about 1/8th of the Earth's mass. The red planet's characteristic hue comes from huge amounts of rusty (iron oxide) dust strewn across its surface, which is mostly composed of silicate rocks and other metals. However the dry, dusty Mars that our minds conjure pictures of when we imagine it, is a relatively new phase in Mars' life (compared to its current age of around 4 and a half billion years!). We believe, because of strange, wavelike patters on the Martian surface that is was once much hotter and wetter than it is now. Currently, Mars' surface temperatures sit between about -90 and -10 degrees Celsius, far to cold for anything to be 'wet' as any water would instantly freeze at those temperatures. This begs the obvious question: What happened to Mars that so drastically changed its atmosphere? (and importantly, could the same thing happen to Earth?)
The answer to this lies deep within the Mars core, where Mars once again reminds us of just how different it is from our home here on Earth. Mars has much weaker magnetic field than the Earth's, in fact the only field it has comes from magnetic elements in the dust that covers its surface. Compare that to Earth which has a strong magnetic field due to the movement of iron deep within our planet. Why is this important? Our magnetic field is what protects us from much of the violent debris that are constantly being fired out towards us by solar storms on the surface of our Sun. Without this protection, this so called 'Solar Wind' slowly stripped Mars of much of its atmospheric gasses, leaving it cold and with a much thinner atmosphere (and thus lower atmospheric pressure) than Earth. What's left of the martian atmosphere is mostly made up of carbon dioxide, much of which freezes as 'dry ice' at Mars' polar regions during its winters. All in all, when you look out at Mars tonight (it's the bright orange-red object mid-way up in NZ's northern skies during early currently), think fondly of our brave Kiwi-naughts huddled in their heated, pressurised space suits as they brave the wilds of Utah. And all in the name of science! Image Credit: NASA/JPL/Texas A&M/Cornell
Water, water everywhere but not a drop to drink!
Like Earth, mars has two polar ice caps that shrink and grow depending on the seasons. This is where the majority of ice on mars is found, but also there are small amounts in frosts, glaciers and snow storms, all of which have been witnessed on the martian surface. Stream beds, eroded craters and minerals directly connected to the existence of liquid water have also been observed that strongly suggest the existence of liquid water on mars, yet the question remains: is there liquid water on the surface there now? NASA's next mars mission, the Curiosity Mars Rover, that is due to land in August 2012 is set to answer this question as well as to detect the chemical signatures of microbial life on mars.
Martin weather - dusty with a chance of storms
!http://ph.cdn.photos.upi.com/sv/ph/UPI-19701331239878/6c0358ec733df21106a91f9586b40fce/Orbiter-captures-image-of-Mars-dust-devil.jpg|align=right,border=1,width=388,height=247!Again, bear in mind the infancy of our knowledge of the martian surface. Recent expeditions have shown martian weather to not only be active, but in many cases to be far more violent and strange than anything we experience on Earth. Some of the most curious is the presence of dust devils, huge pillars of dust that stretch over 10km in height (that's 1/10 of the way to the edge of space on Earth) and whirl across the surface. These are caused, as they are on Earth, by convection currents (the mixing of hot and cold air) creating whirlwinds that then spin themselves upright carrying vast plumes of the reddish surface dust with them.
They are responsible for some of the most spectacular patterns we have seen on the martian surface as their shadows wriggle across the dust plains creating serpentine trails overlaid on the desolate surface. Dust features prominently in martian weather systems, due in large part to the lower martian gravity and the sheer amount of dust that abounds on mars' surface. Dust devils aren't the only method for spreading this around though - occasionally mars experiences planet-wide dust storms like those shown on the left. In 2001, a dust storm erupted that covered the entire planet in thick clouds of dust and debris in one of the most extreme displays of weathers power observed in our entire solar system. Imagine of something like that happened here on Earth? It would probably be similar to the aftermath of an impact like the one that is thought to have killed of most of the dinosaurs!
Mars' past - volcanism and canyons
Could any Earth life survive on Mars? 
Martian astronomy
Solar clock
Navigation using the stars
Dark-sky requirements
Hab Science
The hab design
Power sources
Greenhouse experiments
Antipodes
The AoudaX Spacesuit
The Dachstein Giant Ice Caves
Antipodes 0 - Communications and the AoudaX
Antipodes 1 - Rover command
Antipodes 2 - Biological sampling at MDRS
Exploration & ResearchFollowing an initial training and induction period, the crew will perform a range of experiments and exercises, related to their areas of expertise or interest. Schools and other groups within New Zealand will be able to propose and contribute additional experiments. We will also be encouraging schools to run ‘control’ versions of experiments back in New Zealand for comparison, and to increase engagement.
Mission ProgressAlso see Education and Outreach section. Students and the public will be able to get regularly updated information from our website. This will include:
Following the expedition completion, a formal report will also be produced and distributed to schools and via the website. |
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