Opportunity Grinds Away

Image credit: NASA/JPL
On sol 31, which ended at 3:36 a.m. Wednesday, February 25, Opportunity awoke to “Rock Around the Clock” by Bill Haley and his Comets. At 1:00 a.m. Local Solar Time, Opportunity sent data to Earth via the Mars Global Surveyor orbiter and then sent another whopping 145.6 megabits of data at 3:30 a.m. Local Solar Time via the Mars Odyssey orbiter.

During the morning hours, Opportunity collected data with the alpha particle X-ray spectrometer for five hours and took measurements with its miniature thermal emission spectrometer from inside its newly formed hole that was created on sol 30 by the rock abrasion tool. Later, Opportunity retracted and closed the door of the alpha particle X-ray spectrometer and swapped the Moessbauer spectrometer into the hole made by the abrasion tool for a leisurely 24-hour observation.

Opportunity also updated its “attitude knowledge,” which fine-tunes the rover’s information about its exact location and position on Mars. Updating the attitude knowledge allows the rover to more accurately point the high gain antenna toward Earth, which increases the communications capabilities. The attitude adjustment also enables scientists and engineers to point instruments onboard Opportunity more precisely at targets of interest, such as particular rocks and patches of soil. To adjust the attitude knowledge, engineers have the rover turn the panoramic camera to the Sun and watch the Sun travel across the sky for 15 minutes. The rover is then smart enough to take the Sun movement data collected from the panoramic camera to calculate its own location in the universe?..on Mars. The rover gathers attitude knowledge errors over time as it drives and uses the robotic arm extensively, but it only needs an attitude adjustment about once a week or after driving long distances.

Around 12:15 pm Local Solar Time, Opportunity went to sleep to recharge its batteries from its strenuous rock abrasion tool activities on sol 30, but reawakened briefly at 4 p.m. Local Solar Time and again in the evening to send data to Earth via additional overflights by the Mars Global Surveyor and Odyssey orbiters.

The plan for sol 32, which ends at 4:15 a.m. Thursday, February 26, is to take another unique set of Moessbauer measurements to look at the rover-created hole in a different spectrum. The goal is to then crawl slightly forward on sol 33 to position Opportunity to use the rock abrasion tool on the upper target of the El Capitan/McKittrick area.

Original Source: NASA/JPL News Release

Watch the Rosetta Launch Live

The European Space Agency’s Rosetta mission is now on the launch pad, and it should be heading up into space early tomorrow. If you’ve got some free time and a connection to the Internet, why not watch the launch live on your computer? I really enjoy watching the launches live, since there’s still a quite a bit of suspense. You also get a sense of the various tasks that need to be performed to get a spacecraft off the ground. The launch is scheduled for early Thursday, February 26 at 0736 UTC (2:36 am EST). I know, that’s the middle of the night for a lot of you, but if you’re a night owl, tune it in.

Click here to access the live feed.

Enjoy!

Fraser Cain
Publisher
Universe Today

Getting a Greenhouse to Work on Mars

Image credit: NASA
Confused? Then you’re just like plants in a greenhouse on Mars.

No greenhouses exist there yet, of course. But long-term explorers, on Mars, or the moon, will need to grow plants: for food, for recycling, for replenishing the air. And plants aren’t going to understand that off-earth environment at all. It’s not what they evolved for, and it’s not what they’re expecting.

But in some ways, it turns out, they’re probably going to like it better! Some parts of it, anyway.

“When you get to the idea of growing plants on the moon, or on Mars,” explains molecular biologist Rob Ferl, director of Space Agriculture Biotechnology Research and Education at the University of Florida, “then you have to consider the idea of growing plants in as reduced an atmospheric pressure as possible.”

There are two reasons. First, it’ll help reduce the weight of the supplies that need to be lifted off the earth. Even air has mass.

Second, Martian and lunar greenhouses must hold up in places where the atmospheric pressures are, at best, less than one percent of Earth-normal. Those greenhouses will be easier to construct and operate if their interior pressure is also very low — perhaps only one-sixteenth of Earth normal.

The problem is, in such extreme low pressures, plants have to work hard to survive. “Remember, plants have no evolutionary preadaption to hypobaria,” says Ferl. There’s no reason for them to have learned to interpret the biochemical signals induced by low pressure. And, in fact, they don’t. They misinterpret them.

Low pressure makes plants act as if they’re drying out.

In recent experiments, supported by NASA’s Office of Biological and Physical research, Ferl’s group exposed young growing plants to pressures of one-tenth Earth normal for about twenty-four hours. In such a low-pressure environment, water is pulled out through the leaves very quickly, and so extra water is needed to replenish it.

But, says Ferl, the plants were given all the water they needed. Even the relative humidity was kept at nearly 100 percent. Nevertheless, the plants’ genes that sensed drought were still being activated. Apparently, says Ferl, the plants interpreted the accelerated water movement as drought stress, even though there was no drought at all.

That’s bad. Plants are wasting their resources if they expend them trying to deal with a problem that isn’t even there. For example, they might close up their stomata — the tiny holes in their leaves from which water escapes. Or they might drop their leaves altogether. But, those responses aren’t necessarily appropriate.

Fortunately, once the plants’ responses are understood, researchers can adjust them. “We can make biochemical alterations that change the level of hormones,” says Ferl. “We can increase or decrease them to affect the plants’ response to its environment.”

And, intriguingly, studies have found benefits to a low pressure environment. The mechanism is essentially the same as the one that causes the problems, explains Ferl. In low pressure, not only water, but also plant hormones are flushed from the plant more quickly. So a hormone, for example, that causes plants to die of old age might move through the organism before it takes effect.

Astronauts aren’t the only ones who will benefit from this research. By controlling air pressure, in, say, an Earth greenhouse or a storage bin, it may be possible to influence certain plant behaviors. For example, if you store fruit at low pressure, it lasts much longer. That’s because of the swift elimination of the hormone ethylene, which causes fruit to ripen, and then rot. Farm produce trucked from one coast to the other in low pressure containers might arrive at supermarkets as fresh as if it had been picked that day.

Much work remains to be done. Ferl’s team looked at the way plants react to a short period of low pressure. Still to be determined is how plants react to spending longer amounts of time — like their entire life — in hypobaric conditions. Ferl also hopes to examine plants at a wider variety of pressures. There are whole suites of genes that are activated at different pressures, he says, and this suggests a surprisingly complex response to low pressure environments.

To learn more about this genetic response, Ferl’s group are bioengineering plants whose genes glow green when activated. In addition they are using DNA microchip technology to examine as many as twenty-thousand genes at a time in plants exposed to low pressures.

Plants will play an extraordinarily important role in allowing humans to explore destinations like Mars and the Moon. They’ll will provide food, oxygen and even good cheer to astronauts far from home. To make the best use of plants off-Earth, “we have to understand the limits for growing them at low pressure,” says Ferl. “And then we have to understand why those limits exist.”

Ferl’s group is making progress. “The exciting part of this is, we’re beginning to understand what it will take to really use plants in our life support systems.” When the time comes to visit Mars, plants in the greenhouse might not be so confused after all.

Original Source: NASA Science News

Your Pictures of Venus and the Moon

I asked for pictures, and you sent them in? thanks! In fact, I received dozens of photos of Venus and the Moon last night from around the world. I’ve published just a sample of the pictures sent in. I hope you had a chance to see the beautiful sight last night – we sure didn’t here in Vancouver (clouds and rain).

If you missed it last night, head outside tonight. They won’t be side by side, but both Venus and the Moon will be bright in the sky, and well worth the trip outside. No telescope necessary.

Fraser Cain
Publisher
Universe Today

Spirit Could Have Found Salty Brine

Image credit: NASA/JPL
Opportunity has been getting the lion’s share of the attention in recent weeks, because its twin sister Spirit has been engaged mostly in long-distance driving. But it may be about to steal the spotlight. For several sols, Spirit has been working its way towards nearby Bonneville crater. But even before it gets there, the mobile robot may make a critical discovery. It may find evidence of liquid water on Mars.

Well, not exactly liquid water. Liquid brine, actually. Brine is water that contains dissolved salts. The salts lower the melting temperature of the mixture so that it remains liquid well below the freezing point of pure water. (That’s why road crews “salt” roadways to melt ice in the winter.) Scientists have long speculated that brines, or super brines – a super brine contains high concentrations of dissolved salts – may exist in the martian subsurface.

Spirit’s discovery of patterns in the surface soil at Gusev Crater is what led scientists to believe that there may be subsurface brines there. As of sol 45 (Tuesday, February 17), Spirit had traveled to Laguna Hollow, a small depression located about halfway between Spirit’s landing site and Bonneville crater. In the fine-grained surface material inside the hollow, scientists can see irregular patterns of lines and polygons.

The science team is anxious to learn more about this material, which is unlike anything seen before on Mars. They saw that the topmost layer appeared to be made of different material than what lay just beneath it, and that the surface material stuck to the rover’s wheels.

Dave Des Marais, a science team member from NASA Ames Research Center, explained the possibilities this way: “It could be that it’s a very fine grained dust; fine dust can be coherent when it’s compressed. But it could also have salt in it, or for that matter, a brine or a little bit of water to give it moisture.” On Earth, he said, “you can get that with freeze-thaw type activity, at higher latitudes, such as in tundra. You can also get that in a salt flat, where the salt, by warming, or by wetting and drying, expands and contracts, and forms a very characteristic polygon pattern. You can do it with mud flats, with mud cracks.”

Next on the agenda for Spirit is to dig a deeper trench into the Laguna Hollow material. That, said Des Marais, will enable the MER science team to determine why the material is sticky. “If we’re looking at salt that’s moving up and down, with the assistance of water, we might expect to see a concentration of salt near the surface and as we go deeper perhaps less of a concentration.”

Because the patterns are visible at the surface, Des Marais speculates that they could be due to an active, ongoing process on Mars. Even if the process is currently active, though, that doesn’t necessarily mean there’s a sub-surface body of water present. “I wouldn’t expect to see a pool of water when we dig. You don’t need to have that much [water] to explain these properties that we see. It could be just enough to cause a moistening and a very dense concentrated brine,” he said.

If there is brine beneath the surface at Laguna Hollow, the implications for the possibility of life on Mars could be tremendous. On Earth, some microbes have adapted to thrive in water containing concentrations of salts many times that of sea water. Microbes have also been found eking out a meager existence in tiny brine pockets scattered throughout Arctic sea ice. Scientists know for certain that these microbes can survive at temperatures as low as minus 20 degrees Celsius (minus 4 degrees Fahrenheit). It’s possible that they can live at even lower temperatures.

Meanwhile, Opportunity has completed its first trenching operation into the soil at the floor of the crater where it landed. It will now move on to conduct a more detailed exploration of “El Capitan,” the name that has been given to a portion of the nearby bedrock outcrop. El Capitan offers the most extensive stratigraphic section (the tallest continuous stack of exposed layers, or strata) in the outcrop. The topmost layers appear to be composed of different material than the lower layers. By examining both regions in detail, scientists hope to gain a better understanding of the origin of both the rock matrix (the material the layers are composed of) and the tiny spherules that are embedded within the matrix.

One particularly intriguing discovery at Meridiani is the presence of sulfur on the surface of the bedrock. How the sulfur got there is still unknown. Scientists want to find out whether it is present merely within a surface coating, or deeper within the rock. “If we see it only at the surface and not below the surface,” said Steve Squyres, principle investigator for the MER mission, “then it’s some kind of coating.” That, he said, would “tell us something interesting about recent processes, but it doesn’t tell us about the formation of the outcrop itself.”

If, on the other hand, Opportunity ground into the rock with its RAT and detected sulfur deeper within the rock, it would indicate that the sulfur was around long ago, when the bedrock formed. Scientists would then want to know which sulfate (sulfur-containing) minerals were present within the rock. There are many different types of sulfate minterals. Some form in volcanic environments; many others, such as gypsum, form in the presence of water.

According to Squyres, if the M?ssbauer spectrometer detects “evidence for a sulfate that is the kind that forms only in the presence of liquid water, that would be an extraordinarily exciting finding. That would be probably the most interesting thing that we’d found yet” at Meridiani.

Original Source: Astrobiology Magazine

Venus and the Moon

I just wanted to give you all another quick reminder that Venus and the Moon will be right beside each other tonight in the Western Sky. If you’re outside and it’s clear, you really can’t miss them. Use this as an opportunity to give some non-space nut a chance to see a beautiful sight, and maybe hook them on the rewarding hobby of astronomy. 🙂

Take some pictures, and send them in – I may publish a few.

Thanks!

Fraser Cain
Publisher
Universe Today

Scientists Watch an Explosion on a Neutron Star

Image credit: NASA
Scientists at the Canadian Institute for Theoretical Astrophysics (CITA) and NASA have captured unprecedented details of the swirling flow of gas hovering just a few miles from the surface of a neutron star, itself a sphere only about ten miles across.

A massive and rare explosion on the surface of this neutron star – pouring out more energy in three hours than the Sun does in 100 years – illuminated the area and allowed the scientists to spy on details of the region never before revealed. They could see details as fine as the ring of gas swirling around and flowing onto the neutron star as this ring buckled from the explosion and then slowly recovered its original form after approximately 1,000 seconds.

All of this was occurring 25,000 light years from Earth, captured second-by-second in movie-like fashion through a process called spectroscopy with NASA’s Rossi X-ray Timing Explorer.

Dr. David Ballantyne of CITA at the University of Toronto and Dr. Tod Strohmayer of NASA’s Goddard Space Flight Center in Greenbelt, Md., present this result in an upcoming issue of Astrophysical Journal Letters. The observation provides new insight into the flow of a neutron star’s (and perhaps a black hole’s) “accretion disk,” usually far too minute to resolve with even the most powerful telescopes.

“This is the first time we have been able to watch the inner regions of an accretion disk, in this case literally a few miles from the neutron star’s surface, change its structure in real-time,” said Ballantyne. “Accretion disks are known to flow around many objects in the Universe, from newly forming stars to the giant black holes in distant quasars. Details of how such a disk flows could only be inferred up to now.”

A neutron star is the dense, core remains of an exploded star at least eight times more massive than the Sun. The neutron star contains about a sun’s worth of mass packed in a sphere no larger than Toronto. An accretion disk refers to the flow of hot gas (plasma) swirling around neutron stars and black holes, attracted by the strong gravity of the region. This gas is often supplied by a neighboring star.

As matter crashes down on the neutron star it builds up a 10- to 100-meter layer of material comprised mostly of helium. The fusion of the helium into carbon and other heavier elements releases enormous energy and powers a strong burst of X-ray light, far more energetic than visible light. (Nuclear fusion is the same process that powers the Sun.) Such bursts can occur several times a day on a neutron star and last for about 10 seconds.

What Ballantyne and Strohmayer observed on this neutron star, named 4U 1820-30, was a “superburst”. These are much more rare than ordinary, helium-powered bursts and release a thousand times more energy. Scientists say these superbursts are caused by a buildup of nuclear ash in the form of carbon from the helium fusion. Current thinking suggests that is takes several years for the carbon ash to buildup to such an extent that it begins to fuse.

The superburst was so bright and long that it acted like a spotlight beamed from the neutron star surface and onto the innermost region of the accretion disk. The X-ray light from the burst illuminated iron atoms in the accretion disk, a process called fluorescence. The Rossi Explorer captured the characteristic signature of the iron fluorescence — that is, its spectrum. This, in turn, provided information about the iron’s temperature, velocity and location around the neutron star.

“The Rossi Explorer can get a good measurement of the fluorescence spectrum of the iron atoms every few seconds,” Strohmayer said. “Adding up all this information, we get a picture of how this accretion disk is being deformed by the thermonuclear blast. This is the best look we can hope to get, because the resolution needed to actually see this action as an image, instead of spectra, would be a billion times greater than what the Hubble Space Telescope offers.”

The scientists said the bursting neutron stars serve as a laboratory to study accretion disks, which are seen (but in less detail) through the Universe around nearby stellar black holes and exceedingly distant quasar galaxies. Stellar black holes with accretion disks do not produce X-ray bursts.

The Rossi Explorer was launched in December 1995 to observe fast-changing, energetic and rapidly spinning objects, such as supermassive black holes, active galactic nuclei, neutron stars and millisecond pulsars.

Original Source: NASA News Release

NASA Awards Research Grants to Support Space Flight

NASA’s Office of Biological and Physical Research recently selected 22 researchers to receive grants of up to four years to conduct research and development in advanced human support technologies. These technologies are expected to have a significant impact on the ability of humans to conduct long-duration space flight missions safely. Benefits to the quality of life on Earth from improved environmental technologies may also result from this research.

The proposals were selected for one-to-four-year efforts, and are potentially worth $16.5 million over four years. Work under these grants will enhance safe human space flight in both low earth orbit, where the International Space Station operates, and in exploration of the solar system beyond low earth orbit.

Five of the grants are for new technologies in advanced environmental monitoring of space habitats. Three grants address strategies for advanced control systems or systems analysis. Two projects are for biomass production. Four projects focus on space human-factors engineering. Eight others address novel approaches to waste processing, including air revitalization, water recycling and treatment of solid wastes.

NASA received 122 proposals in response to a NASA Research Announcement, which was released in March 2003. The proposals were peer-reviewed by scientific and technical experts from academia, government and industry before selections were made. In addition to technical and scientific merit, selection criteria also included cost, relevance to NASA programs and feasibility of utilization by NASA.

For a listing of the selected researchers, listed by state, along with their institutions and their research titles, visit:

http://research.hq.nasa.gov/code_u/nra/current/NRA-03-OBPR-01/winners.html
For more information on space research, visit:

http://spaceresearch.nasa.gov/

Original Source: NASA News Release

Deadly Fire at a Rocket Plant in India

An explosion at a solid fuel booster plant caused a large fire at the main Indian space complex; reports about the number of dead and injured are still coming in. ISRO Chairman G Madhavan Nair rushed to the Satish Dhawan Space Centre at Sriharikota to survey the damage and assist the recovery. Not more than seven people were known to be in the building. Three were sent to hospital with burns, and rescuers are searching for 3 more who were in the booster plant when the explosion occurred.

Europe’s Plan to Search for Life on Mars

Image credit: ESA
Before humans can leave their boot prints on the dusty surface of Mars, many questions have to be answered and many problems solved. One of the most fundamental questions ? one that has intrigued humankind for centuries ? is whether life has ever existed on Mars, the most Earthlike of all the planets.

Through its long-term Aurora Programme of solar system exploration, ESA is already preparing a series of robotic missions that will reveal the Red Planet?s secrets and pave the way for a human expedition in decades to come.

A major step towards the realisation of this ambitious robotic programme was completed this week with the selection of two industrial teams to carry out the detailed design of the ExoMars rover and its Pasteur payload of scientific instruments.

The parallel Phase A studies for ExoMars, the first Flagship mission in the Aurora Programme, will be carried out by companies from ESA Member States and Canada.

The teams are:
* Prime contractor Astrium UK, with subcontractors Galileo Avionica (Italy), Von Hoerner & Sulger (Germany) and SciSys (UK)
* Prime contractor MD Robotics (Canada), with subcontractors Kayser Threde (Germany), Laben (Italy), Carlo Gavazzi (Italy) and Alcatel Space (France)

?The industrial groups will be responsible for producing a detailed design concept for the rover, the first vehicle of its kind to be built by ESA,? said Bruno Gardini, Aurora Project Manager.

?In addition to defining the optimum conceptual design for the rover, they will also be expected to consider the unique operational environment on Mars. The studies will also take into account the design of the Pasteur payload and how the scientific instrument package can best be integrated with such a highly mobile vehicle.?

This week?s announcement follows the September 2003 selection of two industrial teams to carry out a full, end-to-end mission design for ExoMars. Those contracts cover all phases of the mission, from launch, through the long interplanetary voyage to the landing of the rover on the planet.

ESA has also issued an open announcement or ?Call for Ideas?, requesting the participation of the scientific community in the ExoMars mission by proposing a well-defined set of instruments for the Pasteur payload.

After receiving some 50 proposals from more than 600 scientists in 30 countries, ESA intends to appoint three scientific Investigator Working Groups to advise on the final composition of the payload and its utilisation on Mars.

?ExoMars will be ESA?s first mission to carry an exobiology payload, a set of instruments specifically designed to search for life,? said Jorge Vago, ExoMars Study Scientist. ?Over the next few months we shall zero in on the final instrument composition and then pass this information on to the industrial contractors,? he said. ?Our intention is to define a multi-instrument package that will be able to fulfil a number of key tasks.?

?It should be able to drill into the surface, retrieve and analyse samples, study the physical environment and look for evidence of biomarkers ? clear signs that life has existed on Mars in the past, or even survives to the present day,? he added.

ExoMars, which is scheduled for launch in 2009, includes an orbiter and a descent module that will land a large (200 kg), high-mobility rover on the surface of Mars. After delivery of the lander/rover, the ExoMars orbiter will operate as a data relay satellite between the Earth and the vehicle on the Martian surface.

The primary objective of the rover and its state-of-the-art Pasteur payload will be to search for signs of life, past or present, on the Red Planet. Additional measurements will be taken to identify potential surface hazards for future human missions, to determine the distribution of water on Mars and to measure the chemical composition of the surface rocks.

Pasteur will be the most comprehensive scientific package ever to land on Mars, with tools that can extract, handle and analyse samples of Martian soil. The instrument mass of this payload is anticipated to be around 40 kg.

Its unique capability to obtain underground samples at depths of up to two metres will provide an excellent opportunity to gain access to ice-rich soil layers – and possibly the first definitive evidence of primitive Martian life.

Original Source: ESA News Release