Tag: Mars

[/caption]
Need to get away from it all? If you have a background in medicine, computers or engineering and can speak a little Russian and English, this might be just what you are looking for. The European Space Agency and the Russian Institute of Medical and Biological Problems are still looking for volunteers to participate in a 520-day simulation of an expedition to Mars. The institute announced last week the opening of registration, but haven’t yet gotten enough applicants. The nearly two-year experiment will simulate all aspects of a journey to the Red Planet, with a 250-day outward trip, a 30-day stay on its surface, and a 240-day return flight.

Basic requirements: age 25-50, higher education, knowledge of the Russian and English languages ensuring professional and household communication, and a citizen of Russia or ESA member countries.

This full-up simulation follows an earlier 14-day experiment in November 2007, and a 105-day simulation of a mission to Mars this year that ended in July. That mission involved four Russians and two members of the European Space Agency, who spent over three months hunkered down together in a lab that simulated life on board a spaceship.

But now comes the real test. The mission is slated to begin mid-2010 and the participants will live and work in a sealed facility in Moscow, Russia, to investigate the psychological and medical aspects of a long-duration space mission, focusing on the effect that isolation has on the human subjects. Similar to reality TV, the six participants will be filmed throughout their stay.

Scientists will also test various life-support, communications and scientific equipment.

The crew will grow their own vegetables in a special lab, sleep in capsule-sized rooms and will only leave the facility during their 30-day trip to Mars “surface.” They will stick to a rigid daily regime of work, rest and exercise, and follow the same diet as crews aboard the International Space Station.

The participants will be paid, although the amount isn’t specified. For the 105-day mission, each participant was paid 15,500 Euros ($20,000).

For more information or to sign up go to this website from ESA.

Sources: RiaNovosti, ESA, Russian Institute of Biological and Medical Problems

If you enjoyed the zoomable poster of 50 year of space exploration, you’ll probably also like this new poster of Mars missions. It’s basically a bar graph, with missions to Mars as listed chronologically, and the mission result is coded by how close the corresponding bar reaches to Mars. The poster also lists a few of the upcoming missions as well. Cool!

Via Fast Company

[/caption]
Images of recent impact craters taken by the HiRISE Camera on the Mars Reconnaissance Orbiter have revealed sub-surface water ice halfway between the north pole and the equator on Mars. While the Phoenix lander imaged subsurface ice where the top layer of soil had been disturbed at the landing site near the north pole, these new images – taken in quick succession, detecting how the ice sublimated away — are the first to show evidence of water ice at much lower latitudes. Surprisingly, the white ice may be made from 99 percent pure water.

“We knew there was ice below the surface at high latitudes of Mars, but we find that it extends far closer to the equator than you would think, based on Mars’ climate today,” said Shane Byrne of the University of Arizona, a member of the High Resolution Imaging Science Experiment, or HiRISE camera.

“The other surprising discovery is that ice exposed at the bottom of these meteorite impact craters is so pure,” Byrne said. “The thinking before was that ice accumulates below the surface between soil grains, so there would be a 50-50 mix of dirt and ice. We were able to figure out, given how long it took that ice to fade from view, that the mixture is about one percent dirt and 99 percent ice.”

Scientists used several instruments on MRO to take a series of images, detecting and confirming highly pure, bright ice exposed in new craters, ranging from 1.5 feet to 8 feet deep, at five different Martian sites.

The images here were taken of the Arcadia Planitia region, located northwest of the Tharsis region in the northern lowlands, at 40-60° North and 150-180° West. The before and after HiRISE images show a fresh meteorite crater 12 meters, or 40 feet, and reveal how water ice excavated at the crater faded with time. The images, each 35 meters, or 115 feet across, were taken in November 2008 and January 2009.

The discovery of these “white” impact craters began in August 2008, the orbiter’s Context camera team examined their images for any dark spots or other changes that weren’t visible in earlier images of the same area. Meteorites usually leave dark marks when they crash into dust-covered Mars terrain.
The HiRISE team followed up in September 2008 by taking high-resolution images of the dark spots.

“We saw something very unusual when we followed up on the first of these impact craters,” Byrne said, “and that was this bright blue material poking up from the bottom of the crater. It looked a lot like water ice. And sure enough, when we started monitoring this material, it faded away like you’d expect water ice to fade, because water ice is unstable on Mars’ surface and turns directly into water vapor in the atmosphere.”

A few days later in September 2008, the orbiter’s “CRISM” team used their Compact Reconnaissance Imaging Spectrometer for Mars and got the spectral signature of water ice exposed in one of the impact craters, further clinching the discovery.

“All of this had to happen very quickly because 200 days after we first saw the ice, it was gone, it was the color of dirt,” Byrne said. “If we had taken HiRISE images just a few months later, we wouldn’t have noticed anything unusual. This discovery would have just passed us by.”

How far water ice extends toward the equator depends largely on how much water has been available in the Martian atmosphere in the recent past, Byrne said: “The ice is a relic of a more humid climate not very long ago, perhaps just several thousand years ago.”

While Phoenix’s discovery of sub-surface ice was not totally unexpected, finding highly pure ice far closer to the equator because of random meteor impacts was unexpected, he said.

There are several theories about how a layer of such pure ice could have formed beneath Mars surface. Byrne said he thinks that one of the most promising ideas is that this ice on Mars formed in the same way that pure ice lenses form beneath the surface of the Earth.

“That’s where you have very thin films of liquid water around ice grains and soil grains and they migrate around to form clear ice lenses on top of the ice table, even at temperatures well below zero. This process is called ‘frost heave’ on Earth, and it’s considered a nuisance in most places because it cracks up roads and tilts walls and destroys foundations of houses.

“But on Mars it would be of great interest if we could discover a process that involved liquid water in today’s climate, and not just in some of the warmest areas of the planet but in some of the coldest areas of the planet in the high latitude regions,” Byrne said.

Source: EurekAlert

[/caption]
Is Mars red due to rocks being rusted by the water that once flooded the red planet? And is the only explanation for the hematite found by Mars orbiters and studied by the Mars Exploration rovers is that water once was present in volumes on Mars? Not necessarily, says a new study. Research done by Dr. Jonathan Merrison at the Aarhus Mars Simulation Laboratory in Denmark shows that the red dust that covers Mars may be formed by ongoing grinding of surface rocks. Liquid water need not have played any significant role in the red dust formation process.

“Mars should really look black, between its white polar caps, because most of the rocks at mid-latitudes are basalt,” said Merrison. “For decades we assumed that the reddish regions on Mars are related to the water-rich early history of the planet and that, at least in some areas, water-bearing heavily oxidized iron minerals are present.”

Fine red dust covers Mars’s surface and is even present in Mars’s atmosphere, dominating the weather and sometimes becoming so thick that it plunges the planet into darkness. Even though dust is ubiquitous, we do not fully understand its physical, chemical and geological properties.

Merrison and his team have been working on getting accurate measurements of the composition and mineralogy of Mars in order to understand the structure and evolution of the near-surface environment and its interaction with the atmosphere, as well as in searching for potential habitats on Mars.

In their recent laboratory study, the scientists at the Mars Simulation Laboratory have pioneered a novel technique to simulate the sand transport on Mars. They hermetically sealed sand (quartz) t samples in glass flasks and mechanically “tumbled” them for several months, turning each flask ten million times. After gently tumbling pure quartz sand for seven months, almost 10% of the sand had been reduced to dust. When scientists added powdered magnetite, an iron oxide present in Martian basalt, to the flasks they were surprised to see it getting redder as the flasks were tumbled.

“Reddish-orange material deposits, which resemble mineral mantles known as desert varnish, started appearing on the tumbled flasks. Subsequent analysis of the flask material and dust has shown that the magnetite was transformed into the red mineral hematite, through a completely mechanical process without the presence of water at any stage of this process,” said Dr. Merrison.

The scientists suspect that, as the quartz sand grains are tumbled around they get quickly eroded and an alteration of minerals through contact ensues. How exactly this happens need to be further investigated through more experimental and analytical work. What is clear though is that the first experiments show that this process occurs not only in air but also in a dried carbon dioxide atmosphere, that is, in conditions that perfectly resemble those occurring on Mars. It may also imply that the reddish Martian dust is geologically recent.

Scientists worldwide, aided by new missions and improved instrumentation reaching the planet, will continue developing new improved computer models and Earth-bound simulators to try to pierce through the red planet’s mysteries.

“By simulating the conditions and developing accurate analogues of the Martian environment, we will certainly gain a deeper understanding of its dusty nature. In particular, developing better analogues of the Martian surface and atmosphere is vital in interpreting observations made on Mars by landers as well as pioneering the next generation of experiments to be flown,” said Dr Merrison.

Merrison presented his findings at the European Planetary Science Congress last week.

Source: Europlanet