Martian winds probably won't cause serious problems for NASA's upcoming Phoenix Mars Lander mission but could complicate efforts to collect soil and ice at the landing site, according to University of Michigan atmospheric scientist Nilton Renno.
New results from U-M wind tunnel tests suggest that winds could blow away some of the laboriously collected soil and ice, but probably not enough to affect onboard laboratory experiments, said Renno, a member of the Phoenix science team.
"Basically, my conclusion is that if you do the delivery properly and plan it well, you can guarantee that a large fraction of the sample is going to fall inside the instrument intake," said Renno, an associate professor in the U-M College of Engineering's Department of Atmospheric, Oceanic and Space Sciences.
Set for launch from Florida as early as Aug. 3, the Phoenix spacecraft will land on the planet's northern arctic plains, analyzing soil and ice to see if it could support microbial life. An 8-foot robotic arm will scoop up the soil and dump it into onboard science instruments.
With funding from NASA, Renno and his graduate students have been studying the possibility that Martian winds could blow away bits of falling soil and ice as the samples are dropped.
Winds of up to 11 mph are expected much of the time at the Phoenix landing site during the three-month main mission, which begins with arrival on May 25, 2008. Renno calculated that if the soil samples were dropped from a height of 10 centimeters (4 inches)—as called for in the original mission plan—the vast majority of the particles wouldn't make it into the instrument intakes under windy conditions.
Based in part on Renno's work, the Phoenix team decided to move the Phoenix scoop closer to the science-instrument intakes before dropping the soil, he said.
Robert Bonitz, lead engineer on the robotic arm team at NASA's Jet Propulsion Laboratory in Pasadena, Calif., said the new plan is to dump the samples from 2 cm (0.8 inches). And Washington University in St. Louis researcher Raymond Arvidson, lead scientist on the robotic arm team, said the goal is to deliver samples to the instruments during calm periods.
"With Nilton's tests and Bob's ability to deliver at 2 cm., we should be OK," Arvidson said. "I am not particularly concerned about wind dispersal of our samples. Just another issue to keep in mind."
To test his wind-dispersal calculations, Renno and his graduate students completed about a dozen wind-tunnel experiments at his Ann Arbor laboratory in recent weeks. They placed a model of the Phoenix robotic-arm scoop inside the cylindrical, 10-foot-long test chamber.
The scoop contained wood grains of various densities to represent bits of martian dust, soil and ice. The grains were released from a height of 5 centimeters into simulated cross winds ranging from 1 to 10 meters per second (2.25 to 22.5 mph), and their trajectories were photographed with a high-speed camera.
Based on the wind-tunnel results, Renno concluded that only about one-third of the Phoenix samples would make it into the science-instrument intakes when dropped from 5 centimeters into winds of a few meters per second.
But losing two-thirds of a hard-won sample during a $420 million mission isn't as calamitous as it might sound, Renno said. The Phoenix instruments need about 1 gram per test, and the scoop will deliver several grams during each dump. So even if two-thirds of the sample blows away, there would be enough soil and ice to complete the test, he said.
And the recent decision to dump from a height of 2 centimeters, along with the plan to deliver samples during calm weather, should further reduce sample losses.
"We will deliver more volume than needed, in case of lateral transport," Arvidson said. "And we will deliver in calm conditions, based on examination of the meteorology data we collect."
Renno leads the Phoenix science team's atmospheric sciences theme group. His main research goal during the mission is to better understand the water cycle at the landing site. Mars is a frigid desert, and liquid water can't survive at the surface.
But subsurface ice exists in the Martian arctic. Some scientists suspect that near-surface ice periodically melts, during warmer parts of long-term climate cycles.
Since liquid water is required by all known forms of life, the melted ice could provide a home for hardy, opportunistic microorganisms. The Phoenix spacecraft is not equipped to detect current or past life, but it can determine if the prerequisites for life are present.
"The main goal of the mission is to see if there are conditions that could allow life to evolve on Mars, Renno said."Understanding the water cycle will help us answer that question."
Additional U-M tests concerning the dust cloud likely to be kicked up by the Phoenix landing engines have been delayed until September.
NASA's Phoenix mission is led by Peter Smith of the University of Arizona, with project management at the Jet Propulsion Laboratory and development partnership at Lockheed Martin, Denver. International contributions are provided by the Canadian Space Agency; the University of Neuchatel, Switzerland; the University of Copenhagen, Denmark; the Max Planck Institute, Germany; and the Finnish Meteorological Institute.
Jim Erickson | EurekAlert!
Astronomers find unexpected, dust-obscured star formation in distant galaxy
24.03.2017 | University of Massachusetts at Amherst
Gravitational wave kicks monster black hole out of galactic core
24.03.2017 | NASA/Goddard Space Flight Center
Astronomers from Bonn and Tautenburg in Thuringia (Germany) used the 100-m radio telescope at Effelsberg to observe several galaxy clusters. At the edges of these large accumulations of dark matter, stellar systems (galaxies), hot gas, and charged particles, they found magnetic fields that are exceptionally ordered over distances of many million light years. This makes them the most extended magnetic fields in the universe known so far.
The results will be published on March 22 in the journal „Astronomy & Astrophysics“.
Galaxy clusters are the largest gravitationally bound structures in the universe. With a typical extent of about 10 million light years, i.e. 100 times the...
Researchers at the Goethe University Frankfurt, together with partners from the University of Tübingen in Germany and Queen Mary University as well as Francis Crick Institute from London (UK) have developed a novel technology to decipher the secret ubiquitin code.
Ubiquitin is a small protein that can be linked to other cellular proteins, thereby controlling and modulating their functions. The attachment occurs in many...
In the eternal search for next generation high-efficiency solar cells and LEDs, scientists at Los Alamos National Laboratory and their partners are creating...
Silicon nanosheets are thin, two-dimensional layers with exceptional optoelectronic properties very similar to those of graphene. Albeit, the nanosheets are less stable. Now researchers at the Technical University of Munich (TUM) have, for the first time ever, produced a composite material combining silicon nanosheets and a polymer that is both UV-resistant and easy to process. This brings the scientists a significant step closer to industrial applications like flexible displays and photosensors.
Silicon nanosheets are thin, two-dimensional layers with exceptional optoelectronic properties very similar to those of graphene. Albeit, the nanosheets are...
Enzymes behave differently in a test tube compared with the molecular scrum of a living cell. Chemists from the University of Basel have now been able to simulate these confined natural conditions in artificial vesicles for the first time. As reported in the academic journal Small, the results are offering better insight into the development of nanoreactors and artificial organelles.
Enzymes behave differently in a test tube compared with the molecular scrum of a living cell. Chemists from the University of Basel have now been able to...
20.03.2017 | Event News
14.03.2017 | Event News
07.03.2017 | Event News
27.03.2017 | Earth Sciences
27.03.2017 | Life Sciences
27.03.2017 | Life Sciences