Poor Weather Might Take out Opportunity

2007-0801rover.thumbnail.jpg

Okay, this is starting to get worrysome. As I reported twice in the past few weeks, there’s a series of dust storms currently raging across the surface of Mars. And the plucky Mars rovers, Spirit and Opportunity are right in the middle of it. NASA put out a news release today, that was a little grim.

They’re worried about Opportunity.

As you know, the Mars Exploration Rovers are solar powered. Every activity they take: driving around, using their instruments, and communicating with Earth requires electricity generated through solar power. The power isn’t an option, it’s a necessity. That’s because they use the energy to run a heater that keeps their most fragile equipment warmed during the frigid Martian nights.

The latest communications received from Opportunity on July 30, 2007 told a grim tale. Dust from the atmosphere is settling out onto the rovers’ solar panels, blocking the amount of light they receive. The rover is already in a low-power regimen, using the absolutely bare minimum to survive. And the light it’s receiving is steadily going down.

Even though the weather has gotten a little warmer since the dust storm started, the temperature of Opportunity’s electronic modules has gone down at night. Right now, it’s getting down to -37 degrees C (-35 degrees F). This is just within a couple of degrees from the point that the rover will need to turn on its electronics heaters. At that point, the heaters will deplete the rover’s batteries more quickly than it can refill them with sunlight.

NASA engineers have a plan, but it’s a little bit risky. They’re having the rover use its electronics for a longer period each day. If the skies don’t clear up, it might go overboard and switch into a low-power fault mode. This would take the batteries off-line, and put the rover to sleep to wait for sunlight to return. The rover might go to sleep for days, weeks or even months, waiting for enough sunlight to get moving again.

“We will continue to watch the situation on Mars and do all we can to assist our rovers in this ongoing battle against the environmental elements on the Red Planet,” said John Callas, rover project manager at NASA’s Jet Propulsion Laboratory, Pasadena, Calif.

Original Source: NASA/JPL News Release

Mars Phoenix Lander Launch Delayed

2007-0731phoenix.thumbnail.jpg

NASA announced today that they’re going to be postponing the launch of the Phoenix Mars Lander for 24 hours. It has two launch windows on Saturday, August 4th: 5:26 am EDT and 6:02 am EDT.

Mission planners decided on the delay because of a severe weather forecast around the Kennedy Space Center on Tuesday afternoon. This storm will delay the fueling of the Delta II rocket’s second stage, and so it pushed back the schedule for all the following activities.

Here’s more that I’ve written about the mission.

Original Source: NASA News Release

Will Mars Look as Big as the Moon on August 27? Nope

2007-0724mars.thumbnail.jpg

Every year around this time, an email circulates across the Internet speculating that on August 27th, Mars will look as big as the Moon in the sky. And every year, I go ahead and debunk it. Here’s a link to last year’s version. Once again, I’d like to inoculate all my Universe Today readers, to make sure you understand what’s going on, and you’re prepared to explain to your eager friends why this non-event isn’t going to happen.

Say it with me. Mars won’t look as big as the Moon on August 27th.


This strange hoax first surfaced on the Internet back in 2003. An email made the rounds with the following text:

The Red Planet is about to be spectacular! This month and next, Earth is catching up with Mars in an encounter that will culminate in the closest approach between the two planets in recorded history. The next time Mars may come this close is in 2287. Due to the way Jupiter’s gravity tugs on Mars and perturbs its orbit, astronomers can only be certain that Mars has not come this close to Earth in the Last 5,000 years, but it may be as long as 60,000 years before it happens again.

The encounter will culminate on August 27th when Mars comes to within 34,649,589 miles of Earth and will be (next to the moon) the brightest object in the night sky. It will attain a magnitude of -2.9 and will appear 25.11 arc seconds wide. At a modest 75-power magnification

Mars will look as large as the full moon to the naked eye. By the end of August when the two planets are closest, Mars will rise at nightfall and reach its highest point in the sky at 12:30 a.m. That’s pretty convenient to see something that no human being has seen in recorded history. So, mark your calendar at the beginning of August to see Mars grow progressively brighter and brighter throughout the month. Share this with your children and grandchildren. NO ONE ALIVE TODAY WILL EVER SEE THIS AGAIN

There are a few problems with this. The first problem is that the email doesn’t actually mention the date; it just says August 27th. This means it can live on for years and years, going around and around the Internet, forwarded by gullible people to their friends.

The second problem is that it’s wrong. Mars isn’t going to be making a close approach on August 27. The close approach this email is discussing happened back in 2003. It did indeed get closer than it had in at least 50,000 years, but this was a very small amount. On August 27th, 2003, Mars closed to a distance of only 55,758,006 kilometers (34,646,418 miles). The Moon, by comparison, orbits the Earth at a distance of only 385,000 km (240,000 miles). Mars was close, but it was still 144 times further away than the Moon.

Instead of appearing as a huge red orb in the sky, Mars looked like a bright red star. Observers around the world set up their telescopes, and took advantage of this close encounter. But you still needed a telescope. And if you read the email carefully again, you’ll see that it’s trying to explain that.

There’s an extra paragraph break. The last sentence of second paragraph is hanging. It says, “At a modest 75-power magnification “, but there’s no period. The next paragraph starts up with the text, “Mars will look as large as the full moon to the naked eye.” In other words, if you put one eye into the telescope and looked at Mars, and kept your other eye looking at the Moon (which isn’t actually humanly possible), the two orbs would look roughly the same size.

Mars and Earth do come together every two years, reaching the closest point on their orbits – astronomers call this “opposition”. And we’re in one of those years. But it’s not going to happen on August 27th. Instead, we’ll make our opposition on December 18th, 2007. At this point, Mars will be 88.42 million km (55 million miles) – further away than its 2003 opposition.

NASA is taking advantage of the upcoming opposition, and will launch the Phoenix Mars Lander in August. The spacecraft will make its shortest possible journey to reach Mars, arriving early next year.

And by next July, it’ll be time to write this article all over again.

Martian Dust Devil Seen from Above

2007-0720devil.thumbnail.jpg

Here’s a cool picture of a Martian dust devil, captured by the HiRISE camera on the Mars Reconnaissance Orbiter. This little dust devil has nothing to do with the dust storm that’s currently ravaging the Red Planet. The image was captured about a month ago in the southern hemisphere, near Hellas Planitia during the Martian mid-afternoon.

Dust devils like this form when the temperature on the ground is much warmer than the air above. The hot air rises, and then in the right conditions, starts to twist into a vortex that sucks in more warm air. If the vortex can get strong enough, it’ll suck dust off the ground, and create a dust devil.

From this vantage point, the dust devil appears to be about 200 metres (660 feet) across, but it’s probably much smaller where it touches the surface of Mars. Seen from the ground, it would look like a dusty tornado reaching about 500 metres (1,600 feet) high.

Original Source: UA News Release

Dust Storm Threatens the Martian Rovers

2007-0720marsrovers.thumbnail.jpg

That Martian dust storm I reported on a week ago has intensified, engulfing most of the planet. The Martian rovers currently crawling around the surface of the Red Planet will learn first hand what impact these kinds of storms can have on their operations.

The dust is now blocking 99% of the direct sunlight falling on Opportunity’s solar panels. And here’s the problem. With limited electricity for an extended period of time, the roves won’t be able to generate enough electricity to keep their heaters going. These heaters keep their core electronics from becoming too cold in the frigid Martian landscape.

Before the dust storm, Opportunity was generating about 700 watt hours of electricity per day. With this dust, the power output has been reduced to 400 watt hours. Mission operators have been forced to cut back the rovers’ operations, including driving, use of its robotic arm, and cameras and other scientific instruments. On Wednesday, July 18, the power output dropped to just 128 watt hours.

If the storm is too intense or long-lasting, one or both rovers could be damaged permanently or even disabled. And storms like this can last days, weeks, or even longer.

Hang in there little rovers.

Original Source: NASA/JPL News Release

The Mars Landing Approach: Getting Large Payloads to the Surface of the Red Planet

The first true-colour image of Mars from ESA’s Rosetta generated using the OSIRIS orange (red), green and blue colour filters. The image was acquired on 24 February 2007 at 19:28 CET from a distance of about 240 000 km. Credit: MPS for OSIRIS Team MPS/UPD/LAM/ IAA/ RSSD/ INTA/ UPM/ DASP/ IDA

Some proponents of human missions to Mars say we have the technology today to send people to the Red Planet. But do we? Rob Manning of the Jet Propulsion Laboratory discusses the intricacies of entry, descent and landing and what needs to be done to make humans on Mars a reality.

There’s no comfort in the statistics for missions to Mars. To date over 60% of the missions have failed. The scientists and engineers of these undertakings use phrases like “Six Minutes of Terror,” and “The Great Galactic Ghoul” to illustrate their experiences, evidence of the anxiety that’s evoked by sending a robotic spacecraft to Mars — even among those who have devoted their careers to the task. But mention sending a human mission to land on the Red Planet, with payloads several factors larger than an unmanned spacecraft and the trepidation among that same group grows even larger. Why?

Nobody knows how to do it.

Surprised? Most people are, says Rob Manning the Chief Engineer for the Mars Exploration Directorate and presently the only person who has led teams to land three robotic spacecraft successfully on the surface of Mars.

“It turns out that most people aren’t aware of this problem and very few have worried about the details of how you get something very heavy safely to the surface of Mars,” said Manning.

He believes many people immediately come to the conclusion that landing humans on Mars should be easy. After all, humans have landed successfully on the Moon and we can land our human-carrying vehicles from space to Earth. And since Mars falls between the Earth and the Moon in size, and also in the amount of atmosphere it has then the middle ground of Mars should be easy. “There’s the mindset that we should just be able to connect the dots in between,” said Manning.

But as of now, the dots will need to connect across a large abyss.

“We know what the problems are. I like to blame the god of war,” quipped Manning. “This planet is not friendly or conducive for landing.”

The real problem is the combination of Mars’ atmosphere and the size of spacecraft needed for human missions. So far, our robotic spacecraft have been small enough to enable at least some success in reaching the surface safely. But while the Apollo lunar lander weighed approximately 10 metric tons, a human mission to Mars will require three to six times that mass, given the restraints of staying on the planet for a year. Landing a payload that heavy on Mars is currently impossible, using our existing capabilities. “There’s too much atmosphere on Mars to land heavy vehicles like we do on the moon, using propulsive technology completely,” said Manning, “and there’s too little atmosphere to land like we do on Earth. So, it’s in this ugly, grey zone.”

But what about airbags, parachutes, or thrusters that have been used on the previous successful robotic Mars missions, or a lifting body vehicle similar to the space shuttle?

None of those will work, either on their own or in combination, to land payloads of one metric ton and beyond on Mars. This problem affects not only human missions to the Red Planet, but also larger robotic missions such as a sample return. “Unfortunately, that’s where we are,” said Manning. “Until we come up with a whole new trick, a whole new system, landing humans on Mars will be an ugly and scary proposition.”

Road Mapping
In 2004 NASA organized a Road Mapping session to discuss the current capabilities and future problems of landing humans on Mars. Manning co-chaired this event along with Apollo 17 astronaut Harrison Schmitt and Claude Graves, who has since passed away, from the Johnson Space Center. Approximately 50 other people from across NASA, academia and industry attended the session. “At that time the ability to explain these problems in a coherent way was not as good,” said Manning. “The entry, descent and landing process is actually made up of people from many different disciplines. Very few people really understood, especially for large scale systems, what all of the issues were. At the Road Mapping session we were able to put them all down and talk about them.”

The major conclusion that came from the session was that no one has yet figured out how to safely get large masses from speeds of entry and orbit down to the surface of Mars. “We call it the Supersonic Transition Problem,” said Manning. “Unique to Mars, there is a velocity-altitude gap below Mach 5. The gap is between the delivery capability of large entry systems at Mars and the capability of super-and sub-sonic decelerator technologies to get below the speed of sound.”

Plainly put, with our current capabilities, a large, heavy vehicle, streaking through Mars’ thin, volatile atmosphere only has about ninety seconds to slow from Mach 5 to under Mach 1, change and re-orient itself from a being a spacecraft to a lander, deploy parachutes to slow down further, then use thrusters to translate to the landing site and finally, gently touch down.

No Airbags
When this problem is first presented to people, the most offered solution, Manning says, is to use airbags, since they have been so successful for the missions that he has been involved with; the Pathfinder rover, Sojourner and the two Mars Exploration Rovers (MER), Spirit and Opportunity.

But engineers feel they have reached the capacity of airbags with MER. “It’s not just the mass or the volume of the airbags, or the size of the airbags themselves, but it’s the mass of the beast inside the airbags,” Manning said. “This is about as big as we can take that particular design.”

In addition, an airbag landing subjects the payload to forces between 10-20 G’s. While robots can withstand such force, humans can’t. This doesn’t mean airbags will never be used again, only that airbag landings can’t be used for something human or heavy.

Even the 2009 Mars Science Laboratory (MSL) rover, weighing 775 kilograms (versus MER at 175.4 kilograms each) requires an entirely new landing architecture. Too massive for airbags, the small-car sized rover will use a landing system dubbed the Sky Crane. “Even though some people laugh when they first see it, my personal view is that the Sky Crane is actually the most elegant system we’ve come up with yet, and the simplest,” said Manning. MSL will use a combination of a rocket-guided entry with a heat shield, a parachute, then thrusters to slow the vehicle even more, followed by a crane-like system that lowers the rover on a cable for a soft landing directly on its wheels. Depending on the success of the Sky Crane with MSL, it’s likely that this system can be scaled for larger payloads, but probably not the size needed to land humans on Mars.

Atmospheric Anxiety and Parachute Problems
“The great thing about Earth,” said Manning “is the atmosphere.” Returning to Earth and entering the atmosphere at speeds between 7-10 kilometers per second, the space shuttle, Apollo and Soyuz capsules and the proposed Crew Exploration Vehicle (CEV) will all decelerate to less than Mach 1 at about twenty kilometers above the ground just by skimming through Earth’s luxuriously thick atmosphere and using a heat shield. To reach slower speeds needed for landing, either a parachute is deployed, or in the case of the space shuttle, drag and lift allow the remainder of the speed to bleed away.

But Mars’ atmosphere is only one per cent as dense as Earth’s. For comparison, Mars atmosphere at its thickest is equivalent to Earth’s atmosphere at about 35 kilometers above the surface The air is so thin that a heavy vehicle like a CEV will basically plummet to the surface; there’s not enough air resistance to slow it down sufficiently. Parachutes can only be opened at speeds less than Mach 2, and a heavy spacecraft on Mars would never go that slow by using just a heat shield. “And there are no parachutes that you could use to slow this vehicle down,” said Manning. “That’s it. You can’t land a CEV on Mars unless you don’t mind it being a crater on the surface.”

That’s not good news for the Vision for Space Exploration. Would a higher lift vehicle like the space shuttle save the day? “Well, on Mars, when you use a very high lift to weight to drag ratio like the shuttle,” said Manning, “in order to get good deceleration and use the lift properly, you’d need to cut low into the atmosphere. You’d still be going at Mach 2 or 3 fairly close to the ground. If you had a good control system you could spread out your deceleration to lengthen the time you are in the air. You’d eventually slow down to under Mach 2 to open a parachute, but you’d be too close to the ground and even an ultra large supersonic parachute would not save you.”

Supersonic parachute experts have concluded that to sufficiently slow a large shuttle-type vehicle on Mars and reach the ground at reasonable speeds would require a parachute one hundred meters in diameter.

“That’s a good fraction of the Rose Bowl. That’s huge,” said Manning. “We believe there’s no way to make a 100-meter parachute that can be opened safely supersonically, not to mention the time it takes to inflate something that large. You’d be on the ground before it was fully inflated. It would not be a good outcome.”

Heat Shields and Thrusters

It’s not that Mars’ atmosphere is useless. Manning explained that with robotic spacecraft, 99% of the kinetic energy of an incoming vehicle is taken away using a heat shield in the atmosphere. “It’s not inconceivable that we can design larger, lighter heat shields,” he said, “but the problem is that right now the heat shield diameter for a human-capable spacecraft overwhelms any possibility of launching that vehicle from Earth.” Manning added that it would almost be better if Mars were like the moon, with no atmosphere at all.

If that were the case, an Apollo-type lunar lander with thrusters could be used. “But that would cause another problem,” said Manning, “in that for every kilogram of stuff in orbit, it takes twice as much fuel to get to the surface of Mars as the moon. Everything is twice as bad since Mars is about twice as big as the moon.” That would entail a large amount of fuel, perhaps over 6 times the payload mass in fuel, to get human-sized payloads to the surface, all of which would have to be brought along from Earth. Even on a fictitious air-less Mars that is not an option.

But using current thruster technology in Mars’ real, existing atmosphere poses aerodynamic problems. “Rocket plumes are notoriously unstable, dynamic, chaotic systems,” said Manning. “Basically flying into the plume at supersonics speeds, the rocket plume is acting like a nose cone; a nose cone that’s moving around in front of you against very high dynamic pressure. Even though the atmospheric density is very low, because the velocity is so high, the forces are really huge.”

Manning likened theses forces to a Category Five hurricane. This would cause extreme stress, with shaking and twisting that would likely destroy the vehicle. Therefore using propulsive technology alone is not an option.

Using thrusters in combination with a heat shield and parachute also poses challenges. Assuming the vehicle has used some technique to slow to under Mach 1, using propulsion just in last stages of descent to gradually adjust the lander’s trajectory would enable the vehicle to arrive very precisely at the desired landing site. “We’re looking at firing thrusters less than 1 kilometer above the ground. Your parachute has been discarded, and you see that you are perhaps 5 kilometers south of where you want to land,” said Manning. “So now you need the ability to turn the vehicle over sideways to try to get to your landing spot. But this may be an expensive option, adding a large tax in fuel to get to the desired landing rendezvous point.”

Additionally, on the moon, with no atmosphere or weather, there is nothing pushing against the vehicle, taking it off target, and a la Neil Armstrong on Apollo 11, the pilot can “fly out the uncertainties” as Manning called it, to reach a suitable or desired landing site. On Mars, however, the large variations in the density of the atmosphere coupled with high and unpredictable winds conspire to push vehicles off course. “We need to have ways to fight those forces or ways to make up for any mis-targeting using the propulsion system,” said Manning. “Right now, we don’t have that ability and we’re a long way from making it happen.”

Supersonic Decelerators

The best hope on the horizon for making the human enterprise on Mars possible is a new type of supersonic decelerator that’s only on the drawing board. A few companies are developing a new inflatable supersonic decelerator called a Hypercone.

Imagine a huge donut with a skin across its surface that girdles the vehicle and inflates very quickly with gas rockets (like air bags) to create a conical shape. This would inflate about 10 kilometers above the ground while the vehicle is traveling at Mach 4 or 5, after peak heating. The Hypercone would act as an aerodynamic anchor to slow the vehicle to Mach 1.

Glen Brown, Chief Engineer at Vertigo, Inc. in Lake Elsinore, California was also a participant in the Mars Road Mapping session. Brown says Vertigo has been doing extensive analysis of the Hypercone, including sizing and mass estimates for landers from four to sixty metric tons. “A high pressure inflatable structure in the form a of a torus is a logical way to support a membrane in a conical shape, which is stable and has high drag at high Mach numbers,” Brown said, adding that the structure would likely be made of a coated fabric such as silicon-Vectran matrix materials. Vertigo is currently competing for funding from NASA for further research, as the next step, deployment in a supersonic wind tunnel, is quite expensive.

The structure would need to be about thirty to forty meters in diameter. The problem here is that large, flexible structures are notoriously difficult to control. At this point in time there are also several other unknowns of developing and using a Hypercone.

One train of thought is that if the Hypercone can get the vehicle under Mach 1, then subsonic parachutes could be used, much like the ones employed by Apollo, or that the CEV is projected to use to land on Earth. However, it takes time for the parachutes to inflate, and subsequently there would only be a matter of seconds of use, allowing time to shed the parachutes before converting to a propulsive system.

“You’d also need to use thrusters,” said Manning. “You’re falling 10 times faster because the density of Mars’ atmosphere is 100 times less than Earth’s. That means that you can’t just land with parachutes and touch the ground. You’d break people’s bones, if not the hardware. So you need to transition from a parachute system to an Apollo-like lunar legged lander sometime before you get to the ground.”

Manning believes that those who are immersed in these matters, like himself, see the various problems fighting each other. “It’s hard to get your brain around all these problems because all the pieces connect in complex ways,” he said. “It’s very hard to see the right answer in your mind’s eye.”

The additional issues of creating new lightweight but strong shapes and structures, with the ability to come apart and transform from one stage to another at just the right time means developing a rapid-fire Rube Goldberg-like contraption.

“The honest truth of the matter,” said Manning, “is that we don’t have a standard canonical form, a standard configuration of systems that allows us to get to the ground, with the right size that balances the forces, the loads, the people, and allows us to do all the transformation that needs to be done in the very small amount of time that we have to land.”

Other Options and Issues

Another alternative discussed at the 2004 Mars Road Mapping session was the space elevator.

“Mars is really begging for a space elevator,” said Manning. “I think it has great potential. That would solve a lot of problems, and Mars would be an excellent platform to try it.” But Manning admitted that the technology needed to suspend a space elevator has not yet been invented. The issues with space elevator technology may be vast, even compared with the challenges of landing.

Despite these known obstacles, there are few at NASA currently spending any quality time working on any of the issues of landing humans on Mars.

Manning explained, “NASA does not yet have the resources to solve this problem and also develop the CEV, complete the International Space Station and do the lunar landing systems development at the same time. But NASA knows that this is on its plate of things to do in the future and is just beginning to get a handle on the needed technology developments. I try to go out of my way to tell this story because I’m encouraging young aeronautical engineering students, particularly graduate students, to start working on this problem on their own. There is no doubt in my mind that with their help, we can figure out how to make reliable human-scale landing systems work on Mars.”

While there is much interest throughout NASA and the space sector to try to tackle these issues in the ensuing years, technology also needs a few more years to catch up to our dreams of landing humans on Mars.

And this story, like all good engineering stories, will inevitably read like a good detective novel with technical twist and turns, scientific intrigue, and high adventure on another world.

NASA is Sending a Phoenix to Mars

2007-0717lander.thumbnail.jpg

Since the launch of the Mars Phoenix Lander is just around the corner, I thought I’d give you a quick explainer on the mission.

So, let’s get into it. Meet NASA’s Mars Phoenix Lander. Scheduled for launch on August 3rd, this mission will blast off from Cape Canaveral atop a Delta II rocket. It’ll take almost 10 months to reach Mars, entering the atmosphere in May, 2008.

The spacecraft is equipped with a pulsed thrust system to slow its descent through the atmosphere. Its landing system is pared down to the bare essentials to maximize the amount of scientific equipment it can land with. It doesn’t have an airbag system like the rovers, and instead will use parachutes and thrusters to land gently on the surface on its three landing legs.

Unlike the Mars rovers currently crawling around the surface of the Red Planet, Mars Phoenix Lander will be stationary. Once it touches down in the Martian polar regions, it’ll live out the rest of its days searching from that position.

Its purpose is to determine if life ever arose on the surface of Mars, or even there’s life there today. Although the surface of Mars is cold, dry, scoured by wind and dust, and blasted by radiation from the Sun and space, just underneath the topsoil, there could water ice and even life, protected from the harsh elements.

The Phoenix Lander will use its 2.3 metre (7.7 feet) folding arm to dig down into the Martian soil around its landing site. NASA’s Mars Odyssey spacecraft revealed that there are large deposits of water ice just a few centimetres beneath the surface of Mars. The Phoenix Lander should be able to break through into this crust, and see if there’s anything alive down there.

The robotic arm will lift the soil samples up onto the main spacecraft deck so that a suite of scientific instruments can examine it for evidence of life. One will heat the samples, and measure the kinds of gases given off. Another will analyze the chemistry of the soil itself.

In addition to its search for evidence of past and present life, Mars Phoenix Lander will serve as a Martian weather station, following changes in the polar regions to help scientists predict weather patterns on the Red Planet.

Good luck Mars Phoenix Lander.

Original Source: NASA/JPL News Release

Scientists are Keeping an Eye on a Martian Dust Storm

2007-0712storm.thumbnail.jpg

From time to time, dust storms get going on Mars that can severely limit our view of the Red Planet, and the ability of the Mars Rovers to generate power. There’s a storm on Mars right now that NASA scientists are watching carefully to see how it affects the fleet of spacecraft on and around the Red Planet.

This latest storm got rolling during the last week in June in the planet’s cratered southern highlands. Over the course of a week, it grew large enough to encircle the entire planet. And now dust is drifting up into the northern hemisphere as well. As the winds sweep dust into the atmosphere, it gets warmer, adding to the storm’s power and helping it to pick up more dust.

When the dust gets thick enough, it reflects sunlight away from the surface. This cools the storm and causes it to settle down.

For the NASA spacecraft currently at Mars, this current storm is stealing some of their power. Fortunately, it’s currently summer for the Mars rovers, so they’re experiencing this dimming during the peak of their energy generation.

The storm will likely last a few months more, and then the atmosphere will clear up again.

Original Source:ASU News Release

Opportunity is Ready Descend Into Victoria Crater

2007-0628rover.thumbnail.jpg

NASA’s Opportunity rover has been tentatively checking out the rim of Victoria Crater, gathering as much science as it can before going down inside. Mission controllers announced today that they’ve got all the data they need, and they’re ready to push the rover over the edge, and send it on a potentially one-way journey down into the crater.

A meteor impact created Victoria Crater millions of years ago, blasting though layers of rock, and gouging out a hole on Mars 800 metres across (.5 miles). As Opportunity crawls down the steep slope, it’ll be traveling back in time, observing older and older layers of rock on the exposed walls of the crater. As before, it’s looking for evidence of ancient, wet environments.

They’re not planning on a one-way journey. Even though the rover has lasted 12 times longer than mission planners were expecting (90 days), and its capabilities are reduced, it should be able to crawl back out. The slope shouldn’t get any steeper than 15-20 degrees, and it’s on exposed bedrock for good traction.

Here’s a quote from the principal investigator, Steve Squyres:

“We don’t want this to be a one-way trip. We still have some excellent science targets out on the plains that we would like to visit after Victoria. But if Opportunity becomes trapped there, it will be worth the knowledge gained.”

Good luck Opportunity, and hang on tight. It’s going to be a wild ride.

Original Source: NASA News Release

Strange Features on Mars at Aeolis Mensae

2007-0628mars.thumbnail.jpg

This is a cool photograph taken by ESA’s Mars Express spacecraft. It shows the Aeolis Mensae region on Mars, an area known to be on a tectonic transition zone. This might be an explanation for the long linear features and carved valleys.

The area is nearby the volcanic region of Elysium, which separates the southern highlands and the northern lowlands. Aeolis Mensae is right at the transition zone between these two regions, and there’s a 3 km (1.8 mile) elevation difference between the two regions. Why there’s such a steep drop is still a matter of discussion between planetary scientists.

The three-dimensional view was created on computer based on Mars Express’ stereo view, which was captured on March 26th and 29th, 2007.

Original Source: ESA News Release