Posted on by Ken Kremer

Curiosity Completes Crucial Course Correction – 1 Week from Mars !

Image Caption: Course correcting thruster firings on July 29 successfully placed Curiosity on target to touchdown beside Mount Sharp inside Gale Crater on Mars on Aug 6 in search of signs of a habitable environment. Credit: NASA

Now just 1 week out from landing beside a 3 mile high (5 km) layered Martian mountain in search of life’s ingredients, aiming thrusters aboard the cruise stage of NASA’s car sized Curiosity Mars Science Lab successfully fired to set the rover precisely on course for a touchdown on Mars at about 1:31 a.m. EDT (531 GMT) early on Aug. 6 (10:31 p.m. PDT on Aug. 5).

Two precise and brief thruster bursts lasting about 7 seconds were successfully carried out just hours ago earlier today at 1 a.m. on July 29, EDT (10 p.m. PDT on July 28). The effect was to change the spacecraft’s velocity by about 1/40 MPH or 1 cm/sec as it smashes into Mars at about 13,200 mph (5,900 meters per second).

This was the fourth and possibly last of 6 interplanetary Trajectory Correction Manuevers (TCM’s) planned by mission engineers to steer Curiosity since departing Earth for the Red Planet.

If necessary, 2 additional TCM’s could be implemented in the final 48 hours next Saturday and Sunday before Curiosity begins plunging into the Martian atmosphere late Sunday night on a do or die mission to land inside the 100 mile wide Gale Crater with a huge mountain in the middle. All 6 TCM maneuvers were preplanned long before the Nov 26, 2011 liftoff from Cape Canaveral, Florida.

Without this course correction firing, MSL would have hit a point at the top of the Martian atmosphere about 13 miles (21 kilometers) east of the target entry point. During the preprogrammed Entry, Descent and Landing (EDL) sequence the vehicle can steer itself in the upper atmosphere to correct for an error amounting to a few miles.

On landing day, MSL can steer enough during its flight through the upper atmosphere to correct for missing the target entry aim point by a few miles and still land on the intended patch of Mars real estate. The mission’s engineers and managers rated the projected 13-mile miss big enough to warrant a correction maneuver.

“The purpose of this maneuver is to move the point at which Curiosity enters the atmosphere by about 13 miles,” said Tomas Martin-Mur of NASA’s Jet Propulsion Laboratory, Pasadena, Calif., chief of the mission’s navigation team. “The first look at telemetry and tracking data afterwards indicates the maneuver succeeded as planned.”


Image Cation: Curiosity Mars Science Laboratory Rover – inside the Cleanroom at KSC, with robotic arm extended prior to encapsulation and Nov. 26, 2011 liftoff. Credit: Ken Kremer/kenkremer.com

As of today (July 30), Curiosity has traveled about 97% of the overall journey to Mars or about 343 million miles (555 million kilometers) of its 352-million-mile (567-million-kilometer) total flight distance.

“I will not be surprised if this was our last trajectory correction maneuver,” Martin Mur said of the TCM-4 firing. “We will be monitoring the trajectory using the antennas of the Deep Space Network to be sure Curiosity is staying on the right path for a successful entry, descent and landing.”

Curiosity will use an unprecedented rocket powered descent stage and a helicopter like sky crane to set down astride the sedimentary layers of Mount Sharp.

She will then conduct a minimum 2 year prime mission with the most sophisticated science instrument package ever dispatched to Mars to determine if a habitable zone ever existed on this region of Mars.

Curiosity will search for the ingredients of life in the form of organic molecules – the carbon based molecules which are the building blocks of life as we know it. The one-ton behemoth is packed to the gills with 10 state of the art science instruments including a 7 foot long robotic arm, scoop, drill and laser rock zapper.

As Curiosity dives down to Mars surface on Aug. 6, 3 spacecraft from NASA and ESA are now positioned in orbit around the Red Planet and are ready to relay and record signals from the “7 Minutes of Terror” – Read the details in my article – here

Watch NASA TV online for live coverage of the Curiosity landing on Aug 5/6:
mars.jpl.nasa.gov or www.nasa.gov

Ken Kremer

Posted on by Ken Kremer

T Minus 9 Days – Mars Orbiters Now in Place to Relay Critical Curiosity Landing Signals

Image Caption: NASA’s Mars Odyssey will relay near real time signals of this artist’s concept depicting the moment that NASA’s Curiosity rover touches down onto the Martian surface. NASA’s Mars Reconnaissance Orbiter (MRO) and ESA’s Mars Express (MEX) orbiter will also record signals from Curiosity for later playback, not in real time. Credit: NASA

It’s now just T minus 9 Days to the most difficult and complex Planetary science mission NASA has ever attempted ! The potential payoff is huge – Curiosity will search for signs of Martian life

The key NASA orbiter at Mars required to transmit radio signals of a near real-time confirmation of the August 5/6 Sunday night landing of NASA’s car sized Curiosity Mars Science Lab (MSL) rover is now successfully in place, and just in the nick of time, following a successful thruster firing on July 24.

Odyssey will transmit the key signals from Curiosity as she plunges into the Martian atmosphere at over 13,000 MPH (21,000 KPH) to begin the harrowing “7 Minutes of Terror” known as “Entry, Descent and Landing” or EDL – all of which is preprogrammed !

Engines aboard NASA’s long lived Mars Odyssey spacecraft fired for about 6 seconds to adjust the orbiters location about 6 minutes ahead in its orbit. This will allow Odyssey to provide a prompt confirmation of Curiosity’s landing inside Gale crater at about 1:31 a.m. EDT (531 GMT) early on Aug. 6 (10:31 p.m. PDT on Aug. 5) – as NASA had originally planned.

Without the orbital nudge, Odyssey would have arrived over the landing site about 2 minutes after Curiosity landed and the signals from Curiosity would have been delayed.

A monkey wrench was recently thrown into NASA relay signal plans when Odyssey unexpectedly went into safe mode on July 11 and engineers weren’t certain how long recovery operations would take.

“Information we are receiving indicates the maneuver has completed as planned,” said Mars Odyssey Project Manager Gaylon McSmith of NASA’s Jet Propulsion Laboratory, Pasadena, Calif. “Odyssey has been working at Mars longer than any other spacecraft, so it is appropriate that it has a special role in supporting the newest arrival.”

Odyssey has been in orbit at Mars since 2001 conducting orbital science investigations.

Read my review article on Odyssey’s science discoveries – here

Odyssey serves as the primary communications relay for NASA’s other recent surface explorers – Opportunity, Spirit and Phoenix. Opportunity recently passed 3000 Sols of continuous operations.

Two other Mars orbiters, NASA’s Mars Reconnaissance Orbiter and the European Space Agency’s Mars Express, also will be in position to receive radio transmissions from the Mars Science Laboratory during its descent. However, they will be recording information for later playback, not relaying it immediately, as only Odyssey can.

“We began optimising our orbit several months ago, so that Mars Express will have an orbit that is properly “phased” and provides good visibility of MSL’s planned trajectory,” says Michel Denis, Mars Express Spacecraft Operations Manager.

Mars Express has been orbiting the planet since December 2003.


Image Caption: Mars Express supports Curiosity MSL. Credit: ESA

“NASA supported the arrival of Mars Express at Mars in 2003, and, in the past few years, we have relayed data from the rovers Spirit and Opportunity,” says ESA’s Manfred Warhaut, Head of Mission Operations.

“Mars Express also tracked the descent of NASA’s Phoenix lander in 2008 and we routinely share our deep space networks.

“Technical and scientific cooperation at Mars between ESA and NASA is a long-standing and mutually beneficial activity that helps us both to reduce risk and increase the return of scientific results.”

Watch NASA TV online for live coverage of Curiosity landing: mars.jpl.nasa.gov or www.nasa.gov

Ken Kremer

Posted on by Jason Major

Will Curiosity Look for Life on Mars? Not Exactly…

“Curiosity is not a life detection mission. We’re not actually looking for life and we don’t have the ability to detect life if it was there. What we are looking for is the ingredients of life.”
– John Grotzinger, MSL Project Scientist

And with these words this latest video from NASA’s Jet Propulsion Laboratory begins, explaining what Curiosity’s goal will be once it arrives on Mars on August 5. There will be a lot of media coverage of the event and many news stories as the date approaches, and some of these will undoubtedly refer to Mars Science Laboratory as a “search for life on Mars” mission… but in reality the focus of MSL is a bit subtler than that (if no less exciting.)

But hey, one can always dream…

Video: NASA/JPL

Posted on by Jason Major

Flashback: 1978 NASA Film Shows Viking Discoveries

In what’s a sort of foreshadowing of the upcoming August 5 MSL landing, which is being called “seven minutes of terror”, here’s a flashback film from 1978 called “19 Minutes to Earth” which looks at the discoveries made by the Viking orbiter and lander, which made its historic arrival on Mars 36 years ago, on July 20, 1976.

In true late ’70s style the video is full of funky music and (what was then) state-of-the-art video graphics. Awesome.


Even more than the music, though, what’s interesting about the 1978 film is how the subject of microbial life is discussed. Both Viking 1 and 2 were designed to search for evidence of biological activity on Mars, which they did by digging into the Martian soil and looking for signs of resulting respiration.

Although the results were initially deemed inconclusive, further research into the Viking data has prompted some scientists to claim that the landers did, in fact, find evidence of life on Mars.

It’s still a much-debated topic, one that scientists hope to help settle with the upcoming research performed by Curiosity and the Mars Science Laboratory mission.

Funky music and all, the Viking programs paved the way for all future missions to Mars. Lessons learned from Viking technology have blazed the trail for Mars research, from Pathfinder’s Sojourner rover to Spirit and Opportunity, the Mars Reconnaissance Orbiter and ESA’s Mars Express. Very soon Curiosity will continue on with the legacy of robotic exploration of the Red Planet, and someday I’m sure our children and grandchildren will look back at the “funky videos” of our time.

Let’s hope that by then they’ve made their own great strides in space exploration and have found answers to the questions that inspire us today.

Video: NASA. Image: artist’s concept of the Viking lander (NASA).

Posted on by Nancy Atkinson

Latest from Mars: Massive Polar Ice Cliffs, Northern Dunes, Gullied Craters

Several gorgeous images are in this week’s update from the HiRISE camera on board the Mars Reconnaissance Orbiter. This lovely image shows the cliffs at the edges of huge ice sheet at the North Pole of Mars. These cliffs are about 800 meters (2,600 feet) high, and the ice sheet is several kilometers thick at its center. This is a great spot to look for ice avalanches that HiRISE has captured previously. The HiRISE team said that the slopes of these cliffs are almost vertical, plus dense networks of cracks cover the icy cliff faces making it easier for material to break free. The team regularly monitors sites like this to check for new blocks that have fallen. You can look for yourself to see if any avalanches have occurred since the last image was taken of this area, almost exactly one Martian year ago.

The HiRISE scientists monitor these regions to help in understand the climatic record stored in the ice sheet itself.

What else did HiRISE see this week?

These cool-looking dunes look reminiscent of Pac-Man, and they might even be moving across the surface of Mars! They are approximately 100 meters across and are traversing a bumpy, hard terrain, pushed across the surface by the winds on Mars. The HiRISE team will take more images of this dune field in subsequent passes to determine whether these dunes are really moving.

This image shows a gullied crater in the Southern mid-latitudes with light-toned deposits near the center of its floor, and two areas of collapsed terrain at the northern and southern edges of the crater floor.

For more information on each of these images, click on them to see the original page on the HiRISE website, or go to the HiRISE website to see all the wonderful images from Mars.

Posted on by Nancy Atkinson

Latest Panoramic View from Mars Rover

What’s a Mars rover to do when there’s not enough power to rove? Take pictures. LOTS of pictures! This wonderful new panoramic view of the Opportunity rover’s stopping place this past Mars winter, Greeley Haven, is composed of 817 images taken between Dec. 21, 2011, and May 8, 2012. It shows fresh rover tracks and the rim of an ancient impact crater, Endeavour, which awaits more explorations from Opportunity. You’ll want to click and see a bigger version of it here.

But to get the full effect, check out this great interactive sphere of the panorama put together by John O’Connor of the NASATech website!

The images were taken with the color camera mounted on the mast of Oppy, providing a sense of sitting on top of the rover and taking in the view. This is actually a false color image, which emphasizes the difference between the materials.

“The view provides rich geologic context for the detailed chemical and mineral work that the team did at Greeley Haven over the rover’s fifth Martian winter, as well as a spectacularly detailed view of the largest impact crater that we’ve driven to yet with either rover over the course of the mission,” said Jim Bell of Arizona State University, Tempe, Pancam lead scientist.

Opportunity has recently reached a milestone: On July 2, Opportunity reached its 3,000th Martian day, or Sol. You can read a great write-up of the accomplishment at the Road to Endeavour blog by Stu Atkinson, which includes interviews of rover drivers Scott Maxwell and Paolo Bellutta.

Stu also compiled this mosaic close-up of a RAT (Rock Abrasion Tool) hole drilled by Oppy into a rock called “Grasburg.”

Opportunity has recently started to take short drives coming off the long Martian winter, and the team notes in the latest update that the rover has been benefiting from solar array dust cleaning events, which increase the daily energy production: as of Sol 3001 (July 3, 2012), the solar array energy production was 577 watt-hours. That’s great news for future drives and the longevity of the long-lived rover, which has been on Mars since 2004. Truly, Oppy is the Energizer Bunny of rovers!

Lead image caption: This full-circle scene combines 817 images taken by the panoramic camera (Pancam) on NASA’s Mars Exploration Rover Opportunity. It shows the terrain that surrounded the rover while it was stationary for four months of work during its most recent Martian winter. Image Credit: NASA/JPL-Caltech/Cornell/Arizona State Univ.

Second image caption: A close-up look at a hole drilled by Opportunity’s RAT (Rock Abrasion Tool). Mosaic of 4 microscopic imager photos by Stu Atkinson.

Source: JPL

Posted on by Nancy Atkinson

Integrating New Concepts for Entry, Descent and Landing for Future Human Missions to Mars

Editor’s note: This guest post was written by Andy Tomaswick, an electrical engineer who follows space science and technology.

One of the most technically difficult tasks of any future manned missions to Mars is to get the astronauts safely on the ground. The combination of the high speed needed for a short trip in space and the much lighter Martian atmosphere creates an aerodynamics problem that has been solved only for robotic spacecraft so far. If people will one day walk Mars’ dusty surface, we will need to develop better Entry Descent and Landing (EDL) technologies first.

Those technologies are part of a recent meeting of the Lunar Planetary Institute (LPI), The Concepts and Approaches for Mars Exploration conference, held June 12-14 in Houston, which concentrated on the latest advances in technologies that might solve the EDL problem.

Of the multitude of technologies that were presented at the meeting, most seemed to involve a multi-tiered system comprising several different strategies. The different technologies that will fill those tiers are partly mission-dependent and all still need more testing. Three of the most widely discussed were Hypersonic Inflatable Aerodynamic Decelerators (HIADs), Supersonic Retro Propulsion (SRP), and various forms of aerobraking.

HIADs are essentially large heat shields, commonly found many types of manned reentry capsule used in the last 50 years of spaceflight. They work by using a large surface area to create enough drag through the atmosphere of a planet to slow the traveling craft to a reasonable speed. Since this strategy has worked so well on Earth for years, it is natural to translate the technology to Mars. There is a problem with the translation though.

HIADs rely on air resistance for its ability to decelerate the craft. Since Mars has a much thinner atmosphere than Earth, that resistance is not nearly as effective at slowing reentry. Because of this drop in effectiveness, HIADs are only considered for use with other technologies. Since it is also used as a heat shield, it must be attached to the ship at the beginning of reentry, when the air friction causes massive heating on some surfaces. Once the vehicle has slowed to a speed where heating is no longer an issue, the HIAD is released in order to allow other technologies to take over the rest of the braking process.

One of those other technologies is SRP. In many schemes, after the HIAD is released, SRP becomes primarily responsible for slowing the craft down. SRP is the type of landing technology commonly found in science fiction. The general idea is very simple. The same types of engines that accelerate the spacecraft to escape velocity on Earth can be turned around and used to stop that velocity upon reaching a destination. To slow the ship down, either flip the original rocket boosters around upon reentry or design forward-facing rockets that will only be used during landing. The chemical rocket technology needed for this strategy is already well understood, but rocket engines work differently when they are traveling at supersonic speeds. More testing must be done to design engines that can deal with the stresses of such velocities. SRPs also use fuel, which the craft will be required to carry the entire distance to Mars, making its journey more costly. The SRPs of most strategies are also jettisoned at some point during the descent. The weight shed and the difficulty of a controlled descent while following a pillar of flame to a landing site help lead to that decision.

Once the SRP boosters fall away, in most designs an aerobraking technology would take over. A commonly discussed technology at the conference was the ballute, a combination balloon and parachute. The idea behind this technology is to capture the air that is rushing past the landing craft and use it to fill a ballute that is tethered to the craft. The compression of the air rushing into the ballute would cause the gas to heat up, in effect creating a hot air balloon that would have similar lifting properties to those used on Earth. Assuming enough air is rushed into the ballute, it could provide the final deceleration needed to gently drop the landing craft off on the Martian surface, with minimal stress on the payload. However, the total amount this technology would slow the craft down is dependent on the amount of air it could inject into its structure. With more air come larger ballute, and more stresses on the material the ballute is made out of. With those considerations, it is not being considered as a stand-alone EDL technology.

These strategies barely scratch the surface of proposed EDL methods that could be used by a human mission to Mars. Curiosity, the newest rover soon set to land on Mars, is using several, including a unique form of SRP known as the Sky Crane. The results of its systems will help scientists like those at the LPI conference determine what suite of EDL technologies will be the most effective for any future human missions to Mars.

Read our previous article about the difficulties of landing large payloads on Mars, an interview with JPL’s Rob Manning.


Lead image caption: Artist’s concept of Hypersonic Inflatable Aerodynamic Decelerator slowing the atmospheric entry of a spacecraft. Credit: NASA

Second image caption: Supersonic jets are fired forward of a spacecraft in order to decelerate the vehicle during entry into the Martian atmosphere prior to parachute deployment. The image is of the Mars Science Lab at Mach 12 with 4 supersonic retropropulsion jets. Credit: NASA

Source: LPI Concept and Approaches for Mars Exploration

Posted on by Jason Major

New “Flying Tea Kettle” Could Get Us To Mars in Weeks, Not Months

At 54.6 million km away at its closest, the fastest travel to Mars from Earth using current technology (and no small bit of math) takes around 214 days — that’s about 30 weeks, or 7 months. A robotic explorer like Curiosity may not have any issues with that, but it’d be a tough journey for a human crew. Developing a quicker, more efficient method of propulsion for interplanetary voyages is essential for future human exploration missions… and right now a research team at the University of Alabama in Huntsville is doing just that.

This summer, UAHuntsville researchers, partnered with NASA’s Marshall Space Flight Center and Boeing, are laying the groundwork for a propulsion system that uses powerful pulses of nuclear fusion created within hollow 2-inch-wide “pucks” of lithium deuteride. And like hockey pucks, the plan is to “slapshot” them with plasma energy, fusing the lithium and hydrogen atoms inside and releasing enough force to ultimately propel a spacecraft — an effect known as “Z-pinch”.

“If this works,” said Dr. Jason Cassibry, an associate professor of engineering at UAH, “we could reach Mars in six to eight weeks instead of six to eight months.”

Read: How Long Does It Take To Get To Mars?

The key component to the UAH research is the Decade Module 2 — a massive device used by the Department of Defense for weapons testing in the 90s. Delivered last month to UAH (some assembly required) the DM2 will allow the team to test Z-pinch creation and confinement methods, and then utilize the data to hopefully get to the next step: fusion of lithium-deuterium pellets to create propulsion controlled via an electromagnetic field “nozzle”.

Although a rocket powered by Z-pinch fusion wouldn’t be used to actually leave Earth’s surface — it would run out of fuel within minutes — once in space it could be fired up to efficiently spiral out of orbit, coast at high speed and then slow down at the desired location, just like conventional rockets except… better.

“It’s equivalent to 20 percent of the world’s power output in a tiny bolt of lightning no bigger than your finger. It’s a tremendous amount of energy in a tiny period of time, just a hundred billionths of a second.”

– Dr. Jason Cassibry on the Z-pinch effect

In fact, according to a UAHuntsville news release, a pulsed fusion engine is pretty much the same thing as a regular rocket engine: a “flying tea kettle.” Cold material goes in, gets energized and hot gas pushes out. The difference is how much and what kind of cold material is used, and how forceful the push out is.

Everything else is just rocket science.

Read more on the University of Huntsville news site here and on al.com. Also, Paul Gilster at Centauri Dreams has a nice write-up about the research as well as a little history of Z-pinch fusion technology… check it out. Top image: Mars imaged with Hubble’s Wide-Field Planetary Camera 2 in March 1995.

Posted on by Nancy Atkinson

NASA Holding Big Events for Curiosity Rover Landing; Register for Chance to Attend

It’s a big rover, so nothing but a big event is appropriate. NASA is going to hold the first-ever multi-center “Social” (formerly known as Tweetups) in conjunction with the landing of the Mars Science Laboratory’s Curiosity rover on Aug. 6 EDT (Aug. 5 PDT). In case you’re not familiar, NASA Socials are in-person meetings with people who engage with the agency through Twitter, Facebook, Google+ and other social networks.

You can register to attend events at one of six NASA centers: Ames Research Center in Moffett Field, Calif.; Glenn Research Center in Cleveland; Goddard Space Flight Center in Greenbelt, Md.; Johnson Space Center in Houston; Langley Research Center in Hampton, Va.; and Jet Propulsion Laboratory (JPL) in Pasadena, Calif. JPL will be having the main event, and each of the other centers will be connected via a multi-center NASA Television simulcast with JPL, home of the Curiosity rover.

If you live close to any of these centers or are willing to travel, and are at all even remotely interested in space exploration, you should register for the chance to attend. Tweetups NASA Socials are incredible events (some attendees have called them life-altering) where you get behind-the-scenes looks at the centers, tours that aren’t normally given to the public, and presentations by scientists, engineers and managers. The events also will provide guests the opportunity to interact with fellow social media users, space enthusiasts and members of NASA’s social media team. Participants will learn about the Mars Science Laboratory mission and their respective NASA field center. They are encouraged to share their experience with others through their favorite social networks.

Registration for the five new NASA Socials opens at noon EDT, Friday, June 29, and closes at noon Tuesday, July 3. NASA randomly will select participants from online registrations. People may register for NASA Socials to be held at multiple locations, but selectees will be chosen for one event only. Each field center’s social and number of guests allowed varies. For more information on each center’s activities and rules pertaining to NASA Social registration, visit:
http://www.nasa.gov/social

Curiosity is currently scheduled to land at Mars’ Gale crater at approximately 1:31 a.m. EDT Aug. 6 (10:31 p.m. PDT Aug. 5), so be prepared to stay up late! But it should be worth it.

During the two-year prime mission, the rover will investigate whether the selected area of Mars offered environmental conditions favorable for microbial life or if evidence of it existed. Find out more about MSL at this website: http://www.nasa.gov/msl