Posted on by Nancy Atkinson

Reminder: Help Uwingu Begin a New Way to Fund Space Exploration

A couple of weeks ago we wrote about Uwingu, a creative, out-of-the-box concept to help solve what appears to be a growing problem for researchers, scientists, educators and students: how to get funding for research and other ground-breaking space exploration and astronomy projects. Why are a group of individuals from the space and astronomy community taking matters into their own hands to do this?

Alan Stern one of the founders of Uwingu, and the Principal Investigator for the New Horizons mission to Pluto, explained it quite well in today’s episode of the 365 Days of Astronomy.

“Well, it seems almost every year we have budget problems,” he said. “This year the planetary budget got cut 20%. Just last week a report came out cutting the National Science Foundation astronomy facilities, recommending those cuts. And every year it’s the economy or it’s an overrun with NASA, or it’s the President’s budget, or it’s something that happens in Congress. And in space research, in space education, unlike, for example, medical research or if you’re a weather researcher or many other fields, there really aren’t very many places to turn when NASA’s budget is cut or the NSF budget’s cut. That’s about it in terms of the funding portfolio. We like to say, you know, if you only own one stock, you probably deserve what you get when it goes down. We’re out to try and diversify that portfolio a little bit.”

UPDATE: Uwingu now has their own website!

The Uwingu team — and by the way, Uwingu means ‘sky’ in Swahili — has put out a new video about their project, and in doing so, reveal a little more about how they plan to create a new funding method. For two years, they’ve been designing and building software products that will be sold, and the proceeds will create the Uwingu Fund for space research, exploration and education.

Pamela Gay described their ideas as “so elegant that I can’t believe they haven’t already been done.”

Uwingu needs to raise about $75,000 to get their concept off the ground, and after that should be self-supporting, as well as supporting an impressive amount of other researchers every year.

So if you haven’t yet checked out Uwingu, here’s a little reminder to do so. Just head to their Indiegogo page and see what you think.

Posted on by Ken Kremer

Curiosity Takes Aim at Martian Destination – Mount Sharp

Image Caption: Curiosity Points to Mount Sharp. Curiosity unstowed the robotic arm on Aug. 20 and aimed it directly at her Martian drive destination – Mount Sharp. This mosaic of the robotic arm was assembled from navigation camera images from Sols 2, 12 and 14 and shows 18,000 foot high Mount Sharp in the background and the shadow of the martian robot’s head at center. Curiosity will search for hydrated minerals using the robotic arm and a neutron detector on the body. Image stitching and processing by Ken Kremer and Marco Di Lorenzo. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

Curiosity flexed her mighty robotic arm for the first time on Monday (Aug. 20) and aimed the hand-like tool turret squarely at Mount Sharp, her ultimate driving destination.

If you want to see exactly where Curiosity is headed and why she was sent to Gale Crater, just take a look at the new mosaic assembled by Ken Kremer and Marco Di Lorenzo.

Curiosity is pointing with her robotic arm right at Mount Sharp, the huge 18,000 foot tall (5.5 kilometer) mysterious mound that covers the center of the 96 mile (154 km) wide crater. Our mosaic was prominently featured on the front page of NBC News and in a new article by Alan Boyle – here

The layered sediments in Mount Sharp could unveil the geologic history of Mars stretching back billions of years and reveal why the planet transitioned from an ancient, wet period of flowing liquid water on the surface to the dry, desiccated era of today.

As Curiosity unstowed and raised the 7 foot long (2.1 m) arm and reached towards Mount Sharp, the mast mounted navigation cameras on her head snapped a series of black and white images that included the shadow of NASA’s newest Martian robot. The 6 wheeled, car-sized rover made a harrowing pinpoint touchdown barely 2 weeks ago.

The arm is critical to the success of the mission because it will be used to maneuver a sophisticated turret, mounted at the arms terminus and laden with scientific instruments. It weighs a hefty 66 pounds (30 kg) and is about 2 feet in diameter. The turret includes a high resolution focusable color camera, a drill, an X-Ray spectrometer, a scoop and mechanisms for sieving and portioning samples of powdered rock and soil.

“We continue to hit home runs. We unstowed the robotic arm and took a look at the tools on the end of the arm,” said Curiosity Mission Manager Michael Watkins of NASA’s Jet Propulsion Lab (JPL) at a news briefing on Tuesday, Aug. 21. “It’s kind of a Swiss army knife there where we have a lot of instruments. We wanted to make sure all of that was working by doing these first motor checks. All of that went successfully.”

Watkins said the team was thrilled to finally see images of the arm deployed on Mars after seeing thousands of engineering test images.

“We have looked at images thousands of times in our test environment and I always see the walls of the test lab there.Now to see the arm out there deployed with Mars out there in the background is just a great feeling.”

The next step is more tests to confirm the arms utility and movements and calibrate the instruments . “We will fully check out the arm, drill and processing unit,” said Louise Jandura of JPL, sample system chief engineer for Curiosity, at the briefing. “The arm has already performed all these motions on Earth, but in a different gravity condition and that gravity does matter. Our turret at the end of the arm weighs as much as a small child and the differences in gravity change the amount of sag at the end of the arm. We want to be able to fine tune these end-point positions. So it will take some time to put the arm through all its paces.”

What’s more is that Curiosity is wiggling her wheels and is all set to make her first martian test drive on Wednesday.

“Late tonight, we plan to send Curiosity the commands for doing our first drive tomorrow,” said Watkins. “Curiosity will drive about 10 feet, turn right and then back up so her rear wheels will wind up about where her front wheels are now. The cameras will photograph the tracks and evaluate the performance of Curiosity driving ability and the softness of the surface soil.”

The 1 ton mega robot is also equipped with the DAN (Dynamic Albedo of Neutrons) instrument provided by Russia to check for water bound into minerals as hydrates in the top three feet (one meter) of soil beneath the rover.

“Curiosity has begun shooting neutrons into the ground,” said Igor Mitrofanov of Space Research Institute, Moscow, principal investigator for DAN. “We measure the amount of hydrogen in the soil by observing how the neutrons are scattered, and hydrogen on Mars is an indicator of water.”

The mission goal is to ascertain whether the Red Planet was ever capable of supporting microbial life, past or present and to search for the signs of life in the form of organic molecules during the 2 year primary mission phase.

Ken Kremer

Image Caption: Panoramic Vista of Mount Sharp (at right) and Gale Crater from NASA’s Curiosity rover on Mars. Curiosity will eventually climb 3.4 mile high Mount Sharp in search of hydrated minerals. This colorized panoramic mosaic shows was assembled from new navigation camera (Navcam) images snapped by Curiosity on Sol 2 and Sol 12 and colorized based on Mastcam imagery from Curiosity. Image stitching and processing by Ken Kremer and Marco Di Lorenzo. See black and white version below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo Lorenzo – www.kenkremer.com

Posted on by Jenny Winder

Desert RATS Begin Simulated Asteroid Mission Today

Caption: Artist’s Concept, Space Exploration Vehicle Use Comparison. Credit: NASA

Conspiracy theories abound that the Apollo landings all took place on a film set in California, but today NASA’s Desert RATS team begins a mission to asteroid Itokawa. They will land, rove and even undertake spacewalks, without ever stepping foot out of their home base at Johnson Space Center in Texas. This is no hoax however, but a simulated mission to test out NASA’s audacious plan to send astronauts to an asteroid by 2025.

The Desert RATS have been testing robots and other tools that could be used on future exploration missions since 1997, (this is their 15th mission) usually doing analog missions out in the field. “Desert” refers to the Arizona desert, where a lot of the team’s activities take place and “RATS” stands for “Research and Technology Studies.”

However, since they are now testing out a zero-G visit to an asteroid, the team will use mockups inside JSC’s Space Vehicle Mockup Facility, which offers a medley of tools and simulators that would be difficult to transport to a field test location.

For example, the Multi-Mission Space Exploration Vehicle (MMSEV) is designed to both rove across a planetary surface on a wheeled chassis or fly in space using advanced propulsion systems. Four crew members will take it in turns to live in and operate the simulator to explore the asteroid.

The MMSEV can be put on a sled on an air-bearing floor to simulate the moves that the crew might feel during a real mission. There will also be a 50-second delay in voice transmission, going each way to simulate the light-speed travel time between Earth and the asteroid.

The crew can also undertake spacewalks using ARGOS (Active Response Gravity Offload System) an overhead gantry crane system that simulates the reduced gravity environment. In reality nothing would stop astronauts from just floating off the surface but NASA is thinking about using jetpacks, tethers, bungees, nets or spiderwebs to allow them to float just above the surface attached to a smaller mini-spaceship.

A team of scientists from the Astromaterials Research and Exploration Science Directorate will ensure proper scientific methods are applied to asteroid sample collection techniques throughout the 10 day mission.

The mission is slated to run until August 30th or 31st. Find out more here or follow the NASA Desert RATS team on Twitter

Second image caption: ARGOS can be used to make spacewalkers feel as though they weigh 1/6 of their weight, as they would on the moon, or 1/3, as on Mars. Photo credit: NASA

Posted on by Ken Kremer

Sweeping Panoramic Vista of Mount Sharp and Gale Crater from Curiosity

Image Caption: Panoramic Vista of Mount Sharp (at right) and Gale Crater from NASA’s Curiosity rover on Mars. Curiosity will eventually climb 3.4 mile high Mount Sharp in search of hydrated minerals. This colorized panoramic mosaic shows more than half of the landing site surrounding Curiosity in the distance to the visible peak of Mount Sharp and a portion of the stowed robotic arm (at left) and the shadow of the camera mast (center) in the foreground. The mosaic was assembled from new navigation camera (Navcam) images snapped by Curiosity on Sol 2 and Sol 12 and colorized based on Mastcam imagery from Curiosity. Image stitching and processing by Ken Kremer and Marco Di Lorenzo. See black and white version below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

At last the Curiosity mega rover is beaming back the first higher resolution panoramic images that many of us have longed to see – a complete view to the visible summit of towering Mount Sharp, the mountain she will scale, surrounded by the sweeping vistas of the tall eroded rim of Gale Crater, her touchdown site barely 2 weeks ago.

See our panoramic mosaics above and below incorporating the best available raw images to date. Curiosity’s stowed robotic arm and the shadow cast by the camera mast are visible in the foreground.

The new images from Curiosity’s mast mounted navigation cameras (Navcam) show the huge mountains peak to as far up as the rover can see from her vantage point some 7 kilometers (4 miles) from the base of the 18,000 foot (5.5 km) high Mount Sharp which is taller than Mount Rainier, the tallest peak in the contiguous United States.

By stitching together the newly received full resolution Navcam images from Sols 2 and 12, we (Ken Kremer and Marco Di Lorenzo) have created a panoramic mosaic showing the breathtaking expanse to the top of Mount Sharp combined with the perspective of Gale Crater from the rover’s eye view on the crater’s gravelly surface.

Image Caption: Panoramic Vista of Mount Sharp (at right) and Gale Crater from NASA’s Curiosity rover on Mars. Curiosity will eventually climb 3.4 mile high Mount Sharp in search of hydrated minerals. This panoramic mosaic shows more than half of the landing site surrounding Curiosity in the distance to the peak of Mount Sharp and a portion of the stowed robotic arm (at left) and the shadow of the camera mast (center) in the foreground. The mosaic was assembled from new navigation camera (Navcam) images snapped by Curiosity on Sol 2 and Sol 12. Image stitching and processing by Ken Kremer and Marco Di Lorenzo. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo – www.kenkremer.com

In coming weeks, Curiosity will take aim at Mount Sharp with the pair of high resolution Mastcam cameras (34 mm and 100) mounted on the rover’s mast and eventually provide much clearer images to the peak resulting in the most spectacular pictures imaginable of the mysterious mountain that holds the mother lode of hydrated mineral deposits that the robot was sent to investigate by NASA. So far the Mastcam cameras have only imaged the lower reaches of Mount Sharp.

The nuclear powered, car sized Curiosity rover was specifically engineered to accomplish a pinpoint landing inside the 96 mile (154 km) wide Gale Crater beside Mount Sharp so she could scale the mountain and take soil and rock samples of the clays and hydrated sulfated minerals that scientists believe formed in liquid water that flowed billions of years ago.

Mount Sharp is a gigantic mound that covers the entire central portion of Gale Crater and learning how it formed is one of the many mysteries researchers seek to unveil with the highly sophisticated 1 ton robot.

John Grotzinger, the project scientist for NASA’s Curiosity Mars Science Lab (MSL) rover, says that the hydrated minerals are all located in about the first 400 meters or so of Mount Sharp’s vertical elevation, based on spectral data collected by NASA and ESA spacecraft orbiting Mars. He says Curiosity will spend about a year traversing and investigating targets on the crater floor before reaching the foothills of Mount Sharp.

Curiosity will eventually spend years climbing Mount Sharp in the valleys between the 1 to 3 story tall mesas and buttes at the giant mountain’s base and lower elevations in search of sedimentary layers of the clay and hydrated sulfate mineral deposits.

The powerful ChemCam laser that Curiosity successfully test fired today will be absolutely key to finding the best targets for detailed analysis by her 10 state of the art science instruments.

The mission goal is to ascertain whether the Red Planet was ever capable of supporting microbial life, past or present and to search for the signs of life in the form of organic molecules during the 2 year primary mission phase.

Ken Kremer

Image Caption: Gale Crater and Mount Sharp from orbit with Curiosity landing site ellipse

Posted on by Ken Kremer

Curiosity Blasts 1st Mars Rock with Powerful Laser Zapper

Image Caption: PewPew !! – First Laser Zapped rock on Mars. This composite image, with magnified insets, depicts the first laser test by the Chemistry and Camera, or ChemCam, instrument aboard NASA’s Curiosity Mars rover. The composite incorporates a Navigation Camera image taken prior to the test, with insets taken by the camera in ChemCam. The circular insert highlights the rock before the laser test. The square inset is further magnified and processed to show the difference between images taken before and after the laser interrogation of the fist-sized rock, called “Coronation.” It is the first rock on any extraterrestrial planet to be investigated with such a laser test. ChemCam inaugurated use of its laser when it used the beam to investigate Coronation during Curiosity’s 13th day after landing. Credit: NASA/JPL-Caltech/LANL/CNES/IRAP

NASA’s Curiosity rover successfully blasted a Mars rock with a powerful laser beam, for the first time in history, today Aug. 19, inaugurating a revolutionary new era in planetary science with a new type of instrument that will deliver bountiful discoveries. The fist sized Martian rock zapped during the maiden laser target practice shots was appropriately dubbed “Coronation”.

The ChemCam instrument mounted at the top of Curiosity’s mast fired a total of 30 one-million watt pulses over a 10 second period at the 3 inch wide rock that vaporized a pinhead sized spot into an ionized, glowing plasma.

Each pulse lasted about five one-billionths of a second and was sufficient in energy to generate a spark of plasma to be observed with the ChemCam telescope and trio of spectrometers below deck in order to identify the elemental composition.

“Yes, I’ve got a laser beam attached to my head. I’m not ill tempered; I zapped a rock for science. PewPew,” tweeted Curiosity.

The NASA composite image above shows Coronation before and after the laser shots – watch out little Martians !

“We got a great spectrum of Coronation — lots of signal,” said ChemCam Principal Investigator Roger Wiens of Los Alamos National Laboratory, N.M. “Our team is both thrilled and working hard, looking at the results. After eight years building the instrument, it’s payoff time!”

Image caption: This mosaic shows the first target Curiosity zapped with the ChemCam laser, before being blasted on Aug. 19. The 3 inch wide rock was provisionally named N165 and is now called “Coronation”. Credit: NASA/JPL-Caltech/MSSS/LANL

ChemCam recorded spectra from the laser-induced spark during all 30 pulses at 6,144 different wavelengths of ultraviolet, visible and infrared light. The purpose of this test was target practice to make sure the laser could be precisely aimed and to characterize the instrument.

Ultimately the goal is use the laser to penetrate below the dusty surface and reveal the interior composition of the targeted rocks using the telescopic camera and spectrometers.

ChemCam, which stands for Chemistry and Camera, is a joint project between the US and France said Wiens at a news briefing on Aug. 17. “The science team is half French and half US.”

“It’s surprising that the data are even better than we ever had during tests on Earth, in signal-to-noise ratio,” said ChemCam Deputy Project Scientist Sylvestre Maurice of the Institut de Recherche en Astrophysique et Planetologie (IRAP) in Toulouse, France. “It’s so rich, we can expect great science from investigating what might be thousands of targets with ChemCam in the next two years.”

ChemCam is a remote sensing instrument and will get the most use of any of Curiosity’s instruments. It will be analyzing about 14,000 samples and help winnow down the targets and guide Curiosity to the most interesting samples for more detailed analysis, Wiens explained.

ChemCam uses a technique called laser-induced breakdown spectroscopy that has precedent in determining the composition of targets in other extreme environments such as inside nuclear reactors and on the sea floor, but is unprecedented in interplanetary exploration.

NASA’s 1 ton mega rover Curiosity is the biggest and most complex robot ever sent to the surface of another planet, sporting a payload of 10 state of the art science instruments weighing 15 times more than any prior roving vehicle. Curiosity’s goal is to determine if Mars was ever capable of supporting microbial life, past or present and to search for the signs of life in the form of organic molecules during the 2 year primary mission phase.

Ken Kremer

Posted on by Ken Kremer

1st Laser Firing and 1st Motion Imminent for Curiosity

Image Caption: This self-portrait shows the deck of NASA’s Curiosity rover from the rover’s Navigation camera. The image is distorted because of the wide field of view. The back of the rover can be seen at the top left of the image, and two of the rover’s right side wheels can be seen on the left. The undulating rim of Gale Crater forms the lighter color strip in the background. Bits of gravel, about 0.4 inches (1 centimeter) in size, are visible on the deck of the rover. Credit: NASA/JPL-Caltech

The 1st firing of Curiosity’s rock zapping laser and 1st motion of her six wheels is imminent and likely to take place within the next 24 to 72 hours said mission scientists at Friday’s (Aug 17) media briefing at NASA’s Jet Propulsion Lab (JPL) in Pasadena, Calif., home to mission control for the nuclear-powered, car-sized robot.

Furthermore the team has decided on the target of her 1st Martian Trek, a science hot spot dubbed Glenelg because it lies at the natural intersection of three different types of geologic formations (see graphic below), including layered bedrock and an alluvial fan through which liquid water flowed eons ago. Glenelg is about 400 meters (1300 feet) east of the rover’s landing site.

With each passing Sol, or Martian day, NASA biggest, best and most daring mobile lab becomes ever more capable, like a growing child, as engineers energize and successfully test more and more of her highly advanced systems to accomplish feats of exploration and discovery never before possible.

“Everything is going really well,” said John Grotzinger, project scientist for NASA’s Curiosity Mars Science Lab (MSL) rover. “The excitement from the point of view of the science team is all the instruments continue to check out.”

Image Caption: Martian Treasure Map -This image shows the landing site of NASA’s Curiosity rover and destinations scientists want to investigate. Curiosity landed inside Gale Crater on Mars on Aug. 5 PDT (Aug. 6 EDT) at the green dot, within the Yellowknife quadrangle. The team has chosen for it to move toward the region marked by a blue dot that is nicknamed Glenelg. That area marks the intersection of three kinds of terrain. The science team thought the name Glenelg was appropriate because, if Curiosity traveled there, it would visit it twice — both coming and going — and the word Glenelg is a palindrome. Then, the rover will aim to drive to the blue spot marked “Base of Mt. Sharp”, which is a natural break in the dunes that will allow Curiosity to begin scaling the lower reaches of Mount Sharp. At the base of Mt. Sharp are layered buttes and mesas that scientists hope will reveal the area’s geological history. The image was acquired by the High Resolution Imaging Science Experiment (HiRISE) camera on NASA’s Mars Reconnaissance Orbiter. Credit: NASA/JPL-Caltech/Univ. of Arizona

Curiosity will blast her first rock, dubbed N165, in the history of planetary science as early as Saturday night, Aug. 18, with the powerful mast-mounted laser and telescope on the Chemistry and Camera instrument, or ChemCam that includes spectrometers inside the rover.

ChemCam is a remote sensing instrument. It will get the most use by analyzing about 14,000 samples and help winnow down the targets and guide Curiosity to the most interesting samples for detailed analysis, Wiens explained.

“Rock N165 looks like your typical Mars rock, about three inches wide. It’s about 10 feet away,” said Roger Wiens, principal investigator of the ChemCam instrument from the Los Alamos National Laboratory in New Mexico. “We are going to hit it with 14 millijoules of energy 30 times in 10 seconds. It is not only going to be an excellent test of our system, it should be pretty cool too.”

ChemCam has a range of about 23 feet (7 meters). It fires with a million watts of power for 5 billionths of a second, sufficient energy to excite a pinhead sized spot to a glowing plasma that the instrument observes with the spectrometer below deck to identify the chemical composition.

Image caption: This mosaic image shows the first target NASA’s Curiosity rover aims to zap with a laser on its Chemistry and Camera (ChemCam) instrument, a rock provisionally named N165. Credit: NASA/JPL-Caltech/MSSS/LANL

“We are very excited. Our team has waited eight long years to get to this date and we’re happy that everything is looking good so far,” said Wiens. “Hopefully we’ll be back early next week and be able to talk about how Curiosity’s first laser shots went.”

We will take images of Rock N165 before and after the laser firing. The camera has the same resolution as the Mastcam and can take images that resolve to the width of a human hair from 7 feet away.

Engineers plan to turn the rover’s wheels over the next few days and execute a short test drive and turns of about 10 feet (3 meters).

Grotzinger indicated the drive to Glenelg could take a month or more.

“We will drive efficiently to Glenelg and it will take about 3 to 4 weeks. Along the way we may do scooping to take some soil samples if we find fine grained materials”

Glenelg, a palindrome, is also the 1st location where Curiosity will actually drill into rocks. Then it will deliver sifted samples into the two analytical chemistry instruments, SAM (Sample Analysis at Mars) and CheMin (Chemistry and Minerology), which will determine the chemical and mineralogical composition and search for signs of organic molecules – the carbon based molecules that are the building blocks of life.

“We’ll stay and do about a month or more of science at Glenelg”

“With such a great landing spot in Gale Crater, we literally had every degree of the compass to choose from for our first drive,” Grotzinger said. “We had a bunch of strong contenders. It is the kind of dilemma planetary scientists dream of, but you can only go one place for the first drilling for a rock sample on Mars. That first drilling will be a huge moment in the history of Mars exploration.”

After thoroughly investigating Glenelg until around the end of this calendar year, then it’s off to Mount Sharp, an 18,000 foot tall mound (5.5 km) that’s the missions ultimate destination because it preserves millions to billions of years of Martian history, stretching from the wet water era of billions of years ago to the more recent desiccated era. It could take a year or so to reach the base.
Mount Sharp is about 7 kilometers (4.4 miles) distant from the current location of Curiosity.

“What’s really cool about this topography is that the crater rim kind of looks like the Mojave Desert and now what you see here kind of looks like the Four Corners area of the western U.S., or maybe around Sedona, Ariz., where you’ve got these buttes and mesas made out of these layered, kind of light-toned reddish-colored outcrops. There’s just a rich diversity over there,” Grotzinger said at the briefing.

Curiosity will spend years climbing Mount Sharp in search of sedimentary layers of clays and sulfates, the hydrated minerals that form in flowing liquid water and could hold the ingredients of life.

New high resolution images of the foothills of Mount Sharp from Curiosity show the giant mountain’s base is littered with mesas and buttes ranging in height from 1 to 3 story tall buildings, with valleys in between.

Curiosity’s goal is to search for signs of Martian microbial habitats, past or present, with the most sophisticated suite of 10 state of the art science instruments ever sent to the surface of another planet.

Ken Kremer

Image Caption: Curiosity’s Wheels on Mars set to Rove soon inside Gale Crater. This colorized mosaic shows Curiosity wheels, UHF antenna, nuclear power source and pointy low gain antenna (LGA) in the foreground looking to the eroded northern rim of Gale Crater in the background. The mosaic was assembled from full resolution Navcam images snapped by Curiosity on Sol 2 on Aug. 8. Image stitching and processing by Ken Kremer and Marco Di Lorenzo. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

Posted on by Ken Kremer

Curiosity Wheels Initial Rove in a Week on Heels of Science and Surgery Success

Image Caption: Curiosity’s Wheels Set to Rove soon Mars inside Gale Crater after ‘brain transplant’. This colorized mosaic shows Curiosity wheels, nuclear power source and pointy low gain antennea (LGA) in the foreground looking to the eroded northern rim of Gale Crater in the background. The mosaic was assembled from full resolution Navcam images snapped by Curiosity on Sol 2 on Aug. 8. Image stitching and processing by Ken Kremer and Marco Di Lorenzo. see black & white version below. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

Curiosity’s weekend “Brain transplant” proceeded perfectly and she’ll be ready to drive across the floor of Gale Crater in about a week, said the projects mission managers at a NASA news briefing on Tuesday, Aug. 14. And the team can’t wait to get Curiosity’s 6 wheels mobile on the heels of a plethora of science successes after just a week on Mars.

Over the past 4 sols, or Martian days, engineers at NASA’s Jet Propulsion Lab (JPL) successfully uploaded the new “R10” flight software that is required to carry out science operations on the Red Planet’s surface and transform the car-sized Curiosity from a landing vehicle into a fully fledged rover.

The step by step flight software transition onto both the primary and backup computers “went off without a hitch”, said mission manager Mike Watkins of JPL at the news briefing. “We are ‘Go’ to continue our checkout activities on Sol 9 (today).”
Watkins added that the electronic checkouts of all the additional science instruments tested so far, including the APXS, DAN and Chemin, has gone well. Actual use tests are still upcoming.

“With the new flight software, we’re now going to test the steering actuators on Sol 13, and then we are going to take it out for a test drive here probably around Sol 15,” said Watkins . “We’re going to do a short drive of a couple of meters and then maybe turn and back up.”

See our rover wheel mosaic above, backdropped by the rim of Gale Crater some 15 miles away.

Image Caption: Curiosity landed within Gale Crater near the center of the landing ellipse. The crater is approximately the size of Connecticut and Rhode Island combined. This oblique view of Gale, and Mount Sharp in the center, is derived from a combination of elevation and imaging data from three Mars orbiters. The view is looking toward the southeast. Mount Sharp rises about 3.4 miles (5.5 kilometers) above the floor of Gale Crater. Credit: NASA/JPL-Caltech/ESA/DLR/FU Berlin/MSSS

Curiosity made an unprecedented pinpoint landing inside Gale Crater using the rocket powered “Sky Crane” descent stage just a week ago on Aug. 5/6 and the team is now eager to get the huge rover rolling across the Martian plains towards the foothills of Mount Sharp, about 6 miles (10 km) away as the Martian crow flies.

“We have a fully healthy rover and payload,” said Ashwin Vasavada, Mars Science Laboratory (MSL) deputy project scientist. “We couldn’t be happier with the success of the mission so far. We’ve never had a vista like this on another planet before.”

“In just a week we’ve done a lot. We’ve taken our 1st stunning panorama of Gale crater with focusable cameras, 1st ever high energy radiation measurement from the surface, the 1st ever movie of a spacecraft landing on another planet and the 1st ground images of an ancient Martian river channel.”

A high priority is to snap high resolution images of all of Mount Sharp, beyond just the base of the 3.4 mile (5.5 km) tall mountain photographed so far and to decide on the best traverse route to get there.

“We will target Mount Sharp directly with the mastcam cameras in the next few days,” said Watkins.

Climbing the layered mountain and exploring the embedded water related clays and sulfate minerals is the ultimate goal of Curiosity’s mission. Scientists are searching for evidence of habitats that could have supported microbial life.

Curiosity will search for the signs of life in the form of organic molecules by scooping up soil and rock samples and sifting them into analytical chemistry labs on the mobile rovers’ deck.

Vasavada said the team is exhaustively discussing which terrain to visit and analyze along the way that will deliver key science results. He expects it will take about a year or so before Curiosity arrives at the base of Mount Sharp and begins the ascent in between the breathtaking mesas and buttes lining the path upwards to the sedimentary materials.

Watkins and Vasavada told me they are confident they will find a safe path though the dunes and multistory tall buttes and mesas that line the approach to and base of Mount Sharp.

“Curiosity can traverse slopes of 20 degrees and drive over 1 meter sized rocks. The team has already mapped out 6 potential paths uphill from orbital imagery.”

“The science team and our rover drivers and really everybody are kind of itching to move at this point,” said Vasavada. “The science and operations teams are working together to evaluate a few different routes that will take us eventually to Mount Sharp, maybe with a few waypoints in between to look at some of this diversity that we see in these images. We’ll take 2 or 3 samples along the way. That’s a few weeks work each time.”

Caption: Destination Mount Sharp. This image from NASA’s Curiosity rover looks south of the rover’s landing site on Mars towards Mount Sharp. Colors have been modified as if the scene were transported to Earth and illuminated by terrestrial sunlight. This processing, called “white balancing,” is useful for scientists to be able to recognize and distinguish rocks by color in more familiar lighting. Credit: NASA/JPL-Caltech/MSSS

“We estimate we can drive something like a football field a day once we get going and test out all our driving capabilities. And if we’re talking about a hundred football fields away, in terms of 10 kilometers or so, to those lower slopes of Mount Sharp, that already is a hundred days plus.”

“It’s going to take a good part of a year to finally make it to these sediments on Mount Sharp and do science along the way,” Vasavada estimated.

The 1 ton mega rover Curiosity is the biggest and most complex robot ever dispatched to the surface of another planet and is outfitted with a payload of 10 state of the art science instruments weighing 15 times more than any prior roving vehicle.

Ken Kremer

Image Caption: Curiosity’s Wheels Set to Rove soon Mars inside Gale Crater. This mosaic shows Curiosity wheels, nuclear power source and pointy low gain antennea (LGA) in the foreground looking to the eroded northern rim of Gale Crater in the background. The mosaic was assembled from full resolution Navcam images snapped by Curiosity on Sol 2 on Aug. 8. Image stitching and processing by Ken Kremer and Marco Di Lorenzo. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo – www.kenkremer.com

Image Caption: Mosaic of Mount Sharp inside Curiosity’s Gale Crater landing site. Gravelly rocks are strewn in the foreground, dark dune field lies beyond and then the first detailed view of the layered buttes and mesas of the sedimentary rock of Mount Sharp. Topsoil at right was excavated by the ‘sky crane’ landing thrusters. Gale Crater in the hazy distance. This mosaic was stitched from three full resolution Navcam images returned by Curiosity on Sol 2 (Aug 8) and colorized based on Mastcam images from the 34 millimeter camera. Processing by Ken Kremer and Marco Di Lorenzo. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

Posted on by Ken Kremer

Curiosity sees Mount Sharp Up Close and gets ‘Brain Transplant’

Image Caption: Mosaic of Mount Sharp inside Curiosity’s Gale Crater landing site. Gravelly rocks are strewn in the foreground, dark dune field lies beyond and then the first detailed view of the layered buttes and mesas of the sedimentary rock of Mount Sharp. Topsoil at right was excavated by the ‘sky crane’ landing thrusters. Gale Crater in the hazy distance. This mosaic was stitched from three full resolution Navcam images returned by Curiosity on Sol 2 (Aug 8) and colorized based on Mastcam images from the 34 millimeter camera. Processing by Ken Kremer and Marco Di Lorenzo. Credit: NASA/JPL-Caltech/Ken Kremer/Marco Di Lorenzo

The Curiosity rover has beamed back the first detailed images of Mount Sharp, offering a stupendous initial view of her ultimate driving goal, and is now in the midst of a crucial “brain transplant” this weekend that will transform her into a fully operational rover.

The science team will direct the six-wheeled Curiosity to begin climbing Mount Sharp at some later date during the rovers’ two year primary mission after traversing and extensively investigating the floor of her landing site inside Gale Crater.

See our mosaic focusing on the base of Mount Sharp using three full resolution images snapped by the Navcam navigation camera located on the newly erected camera and instrument mast with colorization based on the 34 millimeter Mastcam color camera.

Curiosity came to rest almost flat on the martian surface, but with a slight 3 degree tilt down in the front and the images thus far are taken from that preprogrammed viewpoint, roughly some six miles or so from the base of Mount Sharp.

The terrain is strewn with small pebbles that may stem from a nearby alluvial fan through which liquid water flowed long ago, scientist think. Observations from orbit with NASA’s Mars Reconnaissance Orbiter have identified clay and sulfate minerals in the lower layers of Mount Sharp, indicating a wet history. At higher elevations, scientists hope to discover a boundary layer and indications of what led to the “Great Dessication Event” and loss of liquid water on the ancient Martian surface.

This weekend Curiosity has also begun transmitting spectacular hi res Mastcam images that will far exceed anything else thus far. Here is the Mastcam 360 pano as assembled by NASA so far:

Image Caption: First Hi-Res Color Mosaic of Curiosity’s Mastcam Images. NASA/JPL-Caltech/MSSS

But before the car-sized robot can actually rove around, reach out with her 7 foot (2 meter) long instrument loaded arm and scoop up samples for analysis by the on board chemistry labs she needs the software smarts to accomplish the science tasks.

With all the initial post landing objectives accomplished, engineers at NASA’s Jet Propulsion Lab in Pasadena, Calif., are spending 4 Sols, or Martian days, bracketing this weekend to upload a new software package named “R10” that is optimized for surface operations and will replace the current “R9” package.

“We designed the mission from the start to be able to upgrade the software as needed for different phases of the mission,” said Ben Cichy of NASA’s Jet Propulsion Laboratory in Pasadena, Calif., chief software engineer for the Mars Science Laboratory mission. “The flight software version Curiosity currently is using [R9] was really focused on landing the vehicle. It includes many capabilities we just don’t need any more. It gives us basic capabilities for operating the rover on the surface, but we have planned all along to switch over after landing to a version of flight software that is really optimized for surface operations.”

Software on both the primary and backup computers is being carefully upgraded in step by step stages. He said an initial “toe dip” on Friday to test the upgrade was the first step.

“R10 is optimized for surface operations and has what the science team wants. It’s being downloaded over the next four Sols to enable this fantastic mission,” Cichy said at a JPL news briefing on August 10. They will stand down on science for the next four Sols during the installation.

“Right now, we have the capability in our basic surface software to check out the health of the instruments, but we don’t really have the capability to go and make the full use of all this great hardware we shipped to Mars.”

“So the R10 software gives us the capability to use the robotic arm fully, to use the drill, to use the dust removal tool, to use the whole sampling chain and injest the samples and analyze them, all this exciting stuff this mission will do.”

“Curiosity is a Martian mega rover and born to drive ! R10 gives us the ability to drive autonomously and use images to detect hazards and drive safely.”

So far, the software upgrade is going as planned this weekend.

Curiosity made an unprecedented pinpoint landing inside Gale Crater on Aug. 5/6 using the rocket powered “Sky Crane” descent stage that lowered Curiosity by cables onto the Red Planet’s surface exactly as planned on the plains astride Mount Sharp just a few miles from the base of the gigantic mountain.

Mount Sharp covers much of the interior of the 96 mile wide (154 km) Gale Crater. The peak of the 3.4 mile (5.5 km) high layered mountain is taller than Mount Whitney in California.

For comparison, see Curiosity’s initial wider field post-landing shots of Mount Sharp in 2 D and 3 D from the lower resolution fish-eye Hazcam cameras, here

NASA’s 1 ton mega rover Curiosity is the biggest and most complex robot ever sent to the surface of another planet, sporting a payload of 10 state of the art science instruments weighing 15 times more than any prior roving vehicle. Curiosity’s goal is to determine if Mars was ever capable of supporting microbial life, past or present and to search for the signs of life in the form of organic molecules.

Ken Kremer

Posted on by Jason Major

Mystery Blur in Mars Image Explained

When Curiosity executed a perfect six-wheel landing on Mars on the morning of August 6 to the excitement of millions worldwide — not to mention quite a few engineers and scientists at JPL — it immediately began relaying images back to Earth. Although the initial views were low-resolution and taken through dusty lens covers, features of the local landscape around the rover could be discerned… distant hills, a pebbly surface, the rise of Gale Crater’s central peak — and a curious dark blur on the horizon that wasn’t visible in later images.

What could it have been? Another bit of lens dust? An image artifact? A piece of ancient Martian architecture that NASA demanded be erased from the image? As it turns out, it was most likely something even cooler (or at least real): the result of Curiosity’s descent stage crash-landing into the Martian surface.

Seen in an image from NASA’s Mars Reconnaissance Orbiter’s HiRISE camera, the remnants of Curiosity’s descent to Mars are scattered around the landing site. The heat shield, parachute, back shell — and undeniably the star player of Curiosity’s EDL sequence, the descent stage and sky crane — all landed in relatively close proximity to where the rover touched down. As it turned out, Curiosity’s’s rear Hazcam happened to be aimed right where the sky crane landed after it severed Curiosity’s bridles and rocketed safely away — just as it had been shown in the landing animation.

See an infographic on Curiosity’s EDL timeline here.

Seen in the first images captured by Curiosity’s rear Hazcams just minutes after touchdown — but not in higher-resolution images acquired later — the dark blur is now thought to be a plume of dust and soil kicked up by the sky crane’s impact.

“We know that the cloud was real because we saw it in both the left and right rear Hazcams, so it wasn’t just a smudge on the lens cover or anything like that… and then 45 minutes later it was gone,” said Steven Sell, Deputy Operations for Entry, Descent and Landing at JPL, during an interview with Universe Today on Friday.

“When we were putting together the sequence of images of what would happen after touchdown, we specifically put in the Hazcam shots as soon as we could on the off chance that we would see something,” Sell said. “It was just one of those things where we had some choices we could make, and we said if we put these really close to landing maybe we’ll actually see part of the descent stage.”

Although capturing the sky crane or other part of the descent stage on camera was an intriguing idea, it wasn’t any particular goal of the mission.

“We know that the cloud was real because we saw it in both the left and right rear Hazcams, so it wasn’t just a smudge on the lens cover or anything like that.”

– Steven Sell, Deputy Operations for Entry, Descent and Landing at JPL in Pasadena, CA

“We literally weren’t even thinking about it,” Sell said. “It’s a total bonus that we were able to capture that.”

Unfortunately, the plume only appears in the initial Hazcam shots, which were taken through lens covers coated with dust from landing. It wasn’t until nearly an hour later that the covers were removed and clearer images were captured, and by then the plume was gone. Plus the Hazcams themselves are low-resolution by design — they’re more for navigation than landscape photography.

“Those cameras are not intended for doing that kind of science, or even any science at all,” said Sell. “They’re strictly engineering cameras.”

It’s been said that the best camera is the one you have with you, and in this case Curiosity’s best camera happened to be aimed in the right place at the right time. Plus the sky crane just so happened to land in view of the cameras that got turned on first, which wasn’t a guarantee.

“The descent stage had two possible directions to go: it could have gone forward or backward,” Sell explained. “The way it decides which way to go is whichever direction would take it more north. We knew that the science target is toward the south — the scientists want to study the mountain — and so we didn’t want to throw the descent stage toward the mountain.

Read: Curiosity’s First 360-Degree Color Panorama

“The good news is that the forward Hazcams were at a lower temperature upon landing, we knew they were going to be colder,” Sell said. “The cameras have to reach a certain temperature before they can take a picture, so we knew the rear Hazcams were going to get the picture first, and so the fact that the thing flew to the rear was another coincidence.”

About the same mass as the rover itself, the sky crane weighed about 800 kg (1700 lbs) at the time of impact  — including 100 kg of fuel — and hit going 100 mph. That’s going to kick up a good-sized plume (although exactly how large has yet to be determined.)

“It was one hell of an impact,” Sell said.

You can watch Steve Sell describe this and other data from the first few days of the MSL mission in the press conference held at JPL on Friday, August 10 below, and follow Sell on his Twitter feed here.


Images: NASA/JPL-Caltech. HiRISE image NASA/JPL/University of Arizona.

Posted on by Elizabeth Howell

Chasing The Little Prince in New York City

“One sees clearly only with the heart. Anything essential is invisible to the eyes.” – Antoine de Saint-Exupéry

 

I didn’t expect to find a story about a stranded aviator and a cosmos-travelling boy in the United Nations bookstore in New York City.

Yet there The Little Prince was, prominently displayed on a table near the door – an easy find in a bookstore dominated by tales of war, genocide and oppression of minorities.

Is there a special reason why Antoine de Saint-Exupéry’s message – of hope, of learning to judge yourself before others, and of keeping a childlike wonder about the world – is embedded in such a place, I wondered?

Purchased book in hand, I turned to the Internet for answers. Turns out the famed author and aviator lived in New York City for a time after escaping from occupied France in 1940. While there, he worked on three books, among them The Little Prince.

As a long-time fan of the book, I decided to go on a self-guided walking tour of his haunts. I only had about a day of tour time available and focused on two places: a restaurant and one of his homes.

 

La Vie Parisienne (3 East 52nd St.)

On the exterior of the second floor of a Midtown building rests a plaque commemorating Saint-Exupéry. In French and English, the plaque says several chapters of The Little Prince were written in a studio at 3 East 52nd St.

The studio actually was being used by Bernard Lamotte, a Parisian painter. It is said that his circle of artistic friends included luminaries such as actor-sketch writer Charlie Chaplin, actor-singer Marlene Dietrich, and of course, Saint-Exupéry.

Accounts say Saint-Exupéry was a writer who took to the skies to support his talents at the pen. Additionally, he drew on his experiences as an aviator in many of his writings, such as Southern Mail, Wind, Sand and Stars and Flight to Arras.

On the ground floor of the building was La Vie Parisienne (The Parisian Life), a French restaurant. Today, patrons can take in fine French dining at the same location courtesy of the restaurant La Grenouille (The Frog). The plaque is reportedly below where Lamotte’s table sat.

 

Saint-Exupéry’s residence (240 Central Park South)

Saint-Exupéry actually lived in three locations in the New York City area, but this one was the most accessible to me given time constraints.

Less than 20 minutes’ walk from La Vie Parisienne, Saint-Exupéry would have found the location an easy stroll from where he gathered with his friends. Just across the road from the six-decade-old building is Columbus Circle and Central Park itself, providing a respite from New York City’s busy streets if Saint-Exupéry desired it.

When Saint-Exupéry moved into the building in 1941, it was only a year old and considered to be very modern. Today, the two-tower building still looks very fresh courtesy of a renovation to its exterior a decade ago that among other things, restored the yellow-orange bricks to their former glory.

The Souvenir Français society (which honours members of the French military) initially wanted to place the plaque at this location. The owner denied them because he feared it would bring in tourists.

 

Saint-Exupéry yearned to defend his country and left for North Africa in 1943. He disappeared forever over the Mediterranean in 1944.

Still, New York City remembers him. As late as last year, a staged production of The Little Prince played at the New Victory Theatre, with the prince himself portrayed by a puppet.

 

All photos in those post taken by Elizabeth Howell. Historical information in this article, unless otherwise indicated, came from a 2001 article in The New York Times written by Christopher Gray.

Read Universe Today’s recent article on the B612 Foundation — named after the asteroid in “The Little Prince” — and plans to fund a private asteroid mapping mission.