Posted on by Nancy Atkinson

University Returns $3 Million in Savings to NASA

Here’s something you don’t read everyday: The University of Colorado at Boulder returned nearly $3 million in cost savings to NASA for the SORCE mission, the Solar Radiation and Climate Experiment, which studies how the sun’s variation influences Earth’s climate and atmosphere. The university designed, built and controls the mission. Tom Woods, principal investigator of SORCE said the cost savings were the result of a small, efficient management team, thorough pre-launch testing of prototype instruments and tight schedule adherence during the development phase. “We have a long history at LASP (Laboratory for Atmospheric and Space Physics, in Boulder) in mission and instrument development and spaceflight management and operations, and our experience clearly showed here,” said Woods. “We didn’t cut any corners, we made the best use of the available budget, and we are extremely pleased to be able to return this substantial cost savings back to NASA.”

The SORCE mission was launched by NASA in 2003. Its total budget of $100 million from 1999 to 2008 included the design and development of the satellite’s five instruments, as well as five-and-one-half years of operations, and did not include launch costs. A $2,997,000 check for the cost savings from SORCE development and operations was presented to NASA officials on June 17.

According to Woods, the cost savings during flight operations were largely due to the “sharing” of Laboratory for Atmospheric and Space Physics (LASP) personnel who also operate three other NASA satellites — ICEsat, QuikSCAT and AIM — from the CU Research Park in Boulder.
According to NASA, CU-Boulder is the single largest recipient of NASA university research dollars in the nation. In fiscal year 2007, CU-Boulder received $46.9 million from NASA and an additional $3 million in federal funds for space research from the Jet Propulsion Laboratory in Pasadena and the Space Telescope Science Institute in Baltimore.

SORCE is part of NASA’s Earth Observing System and has greatly expanded measurements of the sun’s radiation, covering wavelengths from soft x-ray bands and ultraviolet light through the visible and near-infrared wavelengths, said Woods. Accurate measurements of solar variation are essential for predicting the sun’s influence on climate and the atmosphere and quantifying how humans are changing the environment, he said.

The SORCE mission was recently extended through 2012, providing LASP with an additional $18 million for satellite operations and data analysis. NASA ranked the SORCE mission as excellent across the board for quality, timeliness, cost and leadership, a ranking achieved by only 4 percent of all NASA missions.

Original News Source: PhysOrg

Posted on by Nancy Atkinson

Latest Phoenix Images: Ice or Salt?

The Phoenix lander team revealed the latest images from the mission at a press briefing on Friday. This first image shows an area dug by Phoenix’s scoop, which disclosed a bright surface just a few inches down, which may be ice. “There’s still some debate about the bright material,” said Phoenix Principle Investigator Peter Smith. “Not everyone is sure that this is ice. So there’s been some debate on our team, centering around that perhaps there’s a salt layer just under the soil that also would be bright. Everyone does believe there’s ice under the surface, and whether this is ice or not is the question. The other question is, is this thick ice that goes down deep beneath the surface, or is this a thin layer and we’ll be able to scrape through? So being able to scrape with our scoop is a high priority for us.”


This pair of images taken by the Optical Microscope on NASA’s Phoenix Mars Lander offers a side-by-side comparison of an airfall dust sample collected on a substrate exposed during landing (left) and a soil sample scooped up from the surface of the ground beside the lander. In both cases the sample is collected on a silicone substrate, which provides a sticky surface holding sample particles for observation by the microscope.

Similar fine particles at the resolution limit of the microscope are seen in both samples, indicating that the soil has formed from settling of dust.

The microscope took the image on the left during Phoenix’s Sol 9 (June 3, 2008), or the ninth Martian day after landing. It took the image on the right during Sol 17 (June 11, 2008).

The scale bar is 1 millimeter (0.04 inch).


This is the latest color image of Phoenix, its surroundings and the scoop with soil.


While we can’t look inside the Thermal and Evolved Gas Analyzer (TEGA) oven which will “bake” the Martian soil to test the type of gases that are released, we can see that some of the soil has gone into TEGA. “We were finally successful and some of the material has slid down over the screen” said Smith, “sort of like material going over a cheese grater, and some of the material has slid down and filled the oven. We sent the commands for the first operation of TEGA last night, but we don’t have our data back yet, so we can’t report on any results. That will be coming later next week. So this is a very exciting time for us. We find the soil is very clumpy, it’s sticky, it’s an unusual soil not at all like the types of soils we used in our tests, which worked just fine with all the instruments. So we’ve developed another method of collecting samples, which is to tilt the scoop and vibrate it, and so it shakes down a small amount of material onto the instruments.”


And finally, here’s the latest weather report for Mars, on the 17th sol of Phoenix’s stay on Mars.

Sources: Phoenix News, NASA TV

Posted on by Nancy Atkinson

Ulysses Mission to End After 17 Years

For more than 17 years the Ulysses spacecraft studied the sun, pioneering solar science and defining our knowledge of the sun’s heliosphere. But on July 1, the mission will end. The spacecraft has been slowly “dying” due a dwindling power supply which can no longer keep the spacecraft warm enough. But Ulysses lasted almost four times its expected lifespan and has forever changed the way scientists view the sun and its effect on the surrounding space.

Ulysses ends its career after revealing that the magnetic field emanating from the sun’s poles is much weaker than previously observed. This could mean the upcoming solar maximum period will be less intense than in recent history.

“Over almost two decades of science observations by Ulysses, we have learned a lot more than we expected about our star and the way it interacts with the space surrounding it,” said Richard Marsden, Ulysses project scientist and mission manager for the European Space Agency (ESA). “Solar missions have appeared in recent years, but Ulysses is still unique today. Its special point of view over the sun’s poles never has been covered by any other mission.”

Ulysses is in a six-year orbit around the Sun. Its long orbital path carries it out to Jupiter’s orbit and back again. The further it ventures from the Sun, the colder the spacecraft becomes. Once it drops to 2ºC, the spacecraft’s hydrazine fuel will freeze.

This has not been a problem in the past because Ulysses carries heaters to maintain a workable on-board temperature. The spacecraft is powered by the decay of a radioactive isotope and over the 17-plus years, the power it has been supplying has been steadily dropping. Now, the spacecraft no longer has enough power to run all of its communications, heating and scientific equipment simultaneously.

The spacecraft and its suite of 10 instruments had to be highly sensitive, yet robust enough to withstand some of the most extreme conditions in the solar system, including intense radiation while passing by the giant planet Jupiter’s north pole.

Ulysses was the first mission to survey the environment in space above and below the poles of the sun in the four dimensions of space and time. It showed the sun’s magnetic field is carried into the solar system in a more complicated manner than previously believed. Particles expelled by the sun from low latitudes can climb to high latitudes and vice versa, sometimes unexpectedly finding their way out to the planets. Ulysses also studied dust flowing into our solar system from deep space, and showed it was 30 times more abundant than astronomers suspected. In addition, the spacecraft detected helium atoms from deep space and confirmed the universe does not contain enough matter to eventually halt its expansion.

Ulysses has traveled over 8.6 billion kilometers (5.4 billion miles) during its lifetime.

“Ulysses has been a challenging mission since launch,” said Ed Massey, Ulysses project manager at JPL. “Its success required the cooperation and intellect of engineers and scientists from around the world.”

Ulysses has been a joint mission between NASA and ESA.

“When the last bits of data finally arrive, it surely will be tough to say goodbye,” said Nigel Angold, ESA’s Ulysses mission operations manager. “But any sadness I might feel will pale in comparison to the pride of working on such a magnificent mission. Although operations will be ending, scientific discoveries from Ulysses data will continue for years to come.”

News Source: JPL Press Release

Posted on by Nancy Atkinson

“Shake, Shake, Shake” Gets Soil into Phoenix TEGA

When Bill Boynton announced at a Phoenix lander team meeting earlier today that the troublesome, clumpy Martian soil now sits, finally, within the TEGA “oven” on Phoenix, the room erupted with cheers and a standing ovation. Boynton then launched a rendition of “Shake, Shake, Shake” he had cued-up on his laptop, and started dancing. If that mental image doesn’t make it clear, getting the soil into TEGA is big, and the entire Phoenix team is excited about the accomplishment. Boynton, who leads the investigations with the Thermal and Evolved Gas Analyzer instrument, and his team have been trying various methods for several days to get the stubborn soil through a screen and into TEGA. The instrument will heat the soil and analyze the gases released to check for water vapor and other chemicals in the soil.

Commands to vibrate the screen were sent to Phoenix for three separate days. Boynton said that the oven might have filled because of the cumulative effects of all the vibrating, or because of changes in the soil’s cohesiveness as it sat for days on the top of the screen.

“There’s something very unusual about this soil, from a place on Mars we’ve never been before,” said Phoenix Principal Investigator Peter Smith. “We’re interested in learning what sort of chemical and mineral activity has caused the particles to clump and stick together.”

Between the shaking and the other new technique developed with the robotic arm called “sprinkling,” Smith hopes they won’t encounter future problems with getting the soil where they want it to go. “Delivering the soil is something we’re getting better at everyday,” he added.

Tomorrow, Thursday June 12, commands will be sent for the TEGA to heat the soil. Initial results may be available on Friday.

“We’ll do a low temperature bake that will tell us how much ice is in the soil,” said Boynton. ” We really don’t expect there to be much ice in the soil since it has been sitting out in the sun and vibrated through the screen. It does look like the soil has changed.”

TEGA has eight ovens to “bake” soil samples. Once an oven is used, it can’t be emptied and used again, so Phoenix has just eight chances to analyze the soil.

While there’s been some debate about the characteristics of Martian arctic soil, Smith said most researchers on the Phoenix team believe it’s a matter of when and not if Phoenix will definitely prove there is water ice region the lander sits on. “There are very few people who don’t believe there’s ice under the soil,” he said. “There also could be a crusty layer of salt on top because of evaporation.”

“We all have a lot of confidence we’ll get down to the ice,” Boynton added. “We may have exposed some in the act of landing. The MECA instrument will help the debate on salt. In a week or two we hope to get enough data to address these speculations.”

MECA is the Microscopy, Electrochemistry, and Conductivity Analyzer, which contains four single wet chemistry labs that will dissolve small amounts of soil in water, to determine the pH and what minerals are in the soil. Those tests will be done later in the mission.

Plans for today’s activities for Phoenix include sprinkling Martian soil on the delivery port for the spacecraft’s Optical Microscope and taking additional photos for a high-resolution color panorama of the lander’s surroundings.

Original News Sources: Phoenix press conference, Phoenix press release

Posted on by Nancy Atkinson

Phoenix Will Try New “Sprinkle” Technique

Phoenix “vibrates” to move soil through a screen.

New motto for the Phoenix spacecraft: If at first you don’t succeed, then dust yourself off and try again. Since the Martian soil is proving to be a challenge for the Mars lander, engineers will try a new technique to try delivering the frozen arctic soil into the TEGA, or the Thermal and Evolved-Gas Anaylzer, designed to bake and sniff samples to identify key ingredients in the soil. The soil is clumping together, and won’t pass through a screen that brings it to the ovens on board the spacecraft. Engineers operating the Robotic Arm on Phoenix Lander are testing a revised method they are calling the sprinkle technique.

“We’re a little surprised at how much this material is clumping together when we dig into it,” said Doug Ming a Phoenix science team member from NASA’s Johnson Space Center, Houston.

Engineers commanded the spacecraft to vibrate the screen for 20 minutes on Sunday but detected only a few particles getting through the screen, not enough to fill the tiny oven below.

“We are going to try vibrating it one more time, and if that doesn’t work, it is likely we will use our new, revised delivery method on another thermal analyzer cell,” said William Boynton of the University of Arizona, lead scientist for the instrument.

The arm delivered the first sample to TEGA on Friday by turning the scoop over to release its contents. The revised delivery method, which Phoenix is testing for the first time today, will hold the scoop at an angle above the delivery target and sprinkle out a small amount of the sample by vibrating the scoop. The vibration comes from running a motorized rasp on the bottom of the scoop.

Phoenix used the arm Sunday to collect a soil sample for the spacecraft’s Optical Microscope, so look for images of that procedure soon. Today’s plans include a practice of the sprinkle technique, using a small amount of soil from the sample collected Sunday. If that goes well, the Phoenix team assembled at the University of Arizona plans to sprinkle material from the same scoopful onto the microscope later this week.

The Phoenix team also discussed this picture, showing a spring on the ground near a footpad of the spacecraft. It came from Phoenix itself, when the biobarrier was opened to free the robotic arm back on May 30, the sixth Martian day of the mission.

Phoenix News

Posted on by Nancy Atkinson

Where Is the New Horizons Spacecraft?

Even though New Horizons is the speediest spacecraft ever to travel through our solar system, it still has a long way to go on its voyage to Pluto and the Kuiper Belt. However, New Horizons hit an interplanetary milepost yesterday, June 8, by crossing the orbit of Saturn. At 1.5 billion kilometers or 935 million miles (10.06 astronomical units) distant, that’s a mission’s worth of space for most spacecraft. But for New Horizons, it’s just another interplanetary point on its voyage to the outer reaches of our solar system. As a testament to New Horizons’ speed, the spacecraft set a record for the fastest transit to Saturn by any spacecraft, making the trip in two years and four months. Voyager 1, the previous record holder, made the journey in approximately three years and two months.

Still aiming for its arrival at the Pluto/Charon system in July of 2015, New Horizons’ mission managers tell us the spacecraft is healthy, and in electronic hibernation. After a productive two-week series of system checks, maintenance activities, and software and command uploads, New Horizons is humming through the outer solar system at 65,740 kilometers per hour (40,850 mph). The team expects to keep the spacecraft in hibernation until Sept. 2.

Although the first 13 months of the mission kept the New Horizons team pretty busy, through its encounter with and gravity assist from Jupiter in February 2007, the next few years will probably be fairly quiet for the mission’s scientists and engineers.

In a previous interview, Alan Stern, New Horizons’ Principle Investigator told Universe Today, “The middle years will be long and probably, and hopefully, pretty boring. But it will include yearly spacecraft and instrument checkouts, trajectory corrections, instrument calibrations and rehearsals for the main mission.” During the last three years of the interplanetary cruise mission, Stern said teams will be writing, testing and uploading the highly detailed command script for the Pluto/Charon encounter. The mission begins in earnest approximately a year before the spacecraft arrives at Pluto, as it begins to photograph the region.

As New Horizons crossed Saturn’s orbit yesterday, the ringed planet was nowhere to be seen, as it was more than 2.3 billion kilometers (1.4 billion miles) away from the spacecraft.

And speaking of the Voyager spacecraft (way back in the first paragraph), Voyagers 1 and 2 are at the edge of the Sun’s heliosphere some 100 AU away, and are the only spacecraft operating farther out than New Horizons.

The next big milepost on New Horizons’ journey? Crossing the orbit of Uranus, on March 18, 2011.

Original News Source: New Horizons Press Release

Posted on by Nancy Atkinson

Images From The STS-124 Mission

The crew of the STS-124 mission has been busy installing equipment on the International Space Station, fixing a toilet, and trying out the latest robotic arm that’s part of the shiny new Kibo module. The image above shows some of the new additions to the station, which just keeps growing in size with every mission. The mass of modules shown are: the Japanese Pressurized Module (left), the Japanese Logistics Module (top center), the Harmony node (center), the Destiny laboratory (right) of the ISS, and the forward section of Space Shuttle Discovery that is docked to the station.


Astronauts Mike Fossum (left) and Ron Garan, during the second EVA for the mission. The two astronauts installed television cameras on the Kibo Japanese Pressurized Module (JPM) that will aid in the Kibo robotic arm operations, they also removed thermal covers from the Kibo robotic arm, prepared an upper JPM docking port for flight day seven’s attachment of the Kibo logistics module, readied a spare nitrogen tank assembly for its installation during the third spacewalk, retrieved a failed television camera from the Port 1 truss, and inspected the port Solar Alpha Rotary Joint (SARJ). In looking at the SARJ, Fossum found grease streaks and a small amount of a dust-like material. In the third spacewalk, coming up on Sunday, the astronauts will take samples of the materials for further testing. They’ll also continue outfitting and activating the Kibo module.


Inside Kibo: STS 124 Commander Mark Kelly (right) and pilot Ken Ham add a rack inside the recently installed Kibo Pressurized Module.


This is a great image of Space Shuttle Discovery with Earth’s limb in the background. Also visible are parts of the shuttle: the Remote Manipulator System (RMS), the docking mechanism, vertical stabilizer and orbital maneuvering system (OMS) pods. This was taken on flight day two, before the shuttle docked with the space station.

Image Source: NASA Human Spaceflight Gallery

Posted on by Nancy Atkinson

Closest Images Ever of Mars Dust Grains

“To see a world in a grain of sand…” – English Poet William Blake

The Phoenix science team tested out the lander’s Optical Microscope by imaging grains of sand and dust particles, some as small as one-tenth the diameter of a human hair. These are the highest resolution image ever of small soil particles from another planet. “We have images showing the diversity of mineralogy on Mars at a scale that is unprecedented in planetary exploration,” said Michael Hecht of NASA’s Jet Propulsion Laboratory.

The microscope observed particles that had fallen onto an exposed surface of the lander. “It’s a first quick look,” Hecht said. “This experiment was partly an insurance policy for something to observe with the microscope before getting a soil sample delivered by the arm, and partly a characterization of the Optical Microscope. All the tools are working well.”

However, some of the particles may be “alien” – that is, they might have come from inside the spacecraft when Phoenix dropped to Mars surface at landing. But at first glance, many of these grains match expectations for Martian particles. “We will be using future observations of soil samples delivered by the Robotic Arm to confirm whether the types of particles in this dustfall sample are also seen in samples we can be certain are Martian in origin,” Hecht said.

The particles show a range of shapes and colors.

“You can see the amount of variety there is in what appears otherwise to be just reddish brown soil,” said Tom Pike, Phoenix science team member from Imperial College London. He noted that one translucent particle resembles a grain of salt, but that it is too early to say for sure.

Meanwhile, Phoenix received commands Thursday to collect its first soil sample to be delivered to its science lab instrument on the lander deck. Those commands were originally sent on Wednesday, but the lander didn’t receive them as the relay for the commands, the Mars Odyssey, had gone into safe mode. The orbiter may have been hit by a cosmic ray, and engineers from JPL say nominal operations of the spacecraft should return by the end of the week. This type of event has occurred a couple of times in the Odyssey mission, and engineers don’t appear overly concerned about the situation.

So, the commands were successfully re-sent via the Mars Reconnaissance Orbiter. Look for the first science results from Phoenix within the next day or so.

Original News Source: Phoenix news release

Posted on by Ian O'Neill

Odyssey Possibly Hit by High-Energy Particles; Phoenix Science Run About to Begin

A successful scoop of Martian regolith (NASA/JPL-Caltech/University of Arizona/Max Planck Institute)

NASA’s Mars Odyssey has been switched into “safe-mode” after possibly being hit by energetic particles from the Sun, or by cosmic rays. Acting as one of two relay satellites between Earth and Phoenix, this has hindered commands to be sent to the lander, thereby slowing its progress. Phoenix is just about to start scence digging operations on the surface (Martian regolith is shown in the Phoenix test-run scoop of material, pictured). It seems likely that Odyssey will remain in the protective safe-mode until the weekend whilst operators try to understand what caused the problem. For the time being, the second relay satellite NASA’s Mars Reconnaissance Orbiter (MRO) will try to take up the slack and keep the lander in contact with mission control…

This is the second communications error in the otherwise flawless Phoenix Mars mission. The first occurred two days after touch down when the MRO switched its UHF radio into standby mode. Yesterday’s (Wednesday’s) error with another Mars-orbiting satellite, Odyssey, probably won’t be repaired until Saturday. Mission engineers believe the error may have occurred when energetic space particles interrupted Odyssey’s onboard memory. As a safety precaution, the onboard hardware was switched into a low-energy state to protect it from any damage. This event doesn’t seem to be serious, but it does slow down the progress of Phoenix which is currently excavating Mars material from the surface of the red planet, trying to understand the composition of permafrost layers.

The Mars Reconnaissance Orbiter has stepped in for Odyssey (NASA)

Although frustrating, this setback will not cause too many problems to Phoenix, daily commands can still be sent to the MRO and relayed to Phoenix and the first delayed science excavation run is scheduled for today. Test runs over the past few days have revealed a white substance in the fist-sized samples of regolith, so scientists are very excited to “bake” the permafrost material to see if water ice or salt deposits are present. After the preliminary tests, mission scientists believe that Phoenix’s 8-foot robotic arm is up to the task and appears to be functioning excellently.

The following steps will be carried out in the first science run scheduled to start today:

  1. Right of the test-dig area, scientists have identified three “science rich” zones. Phoenix will dig into areas known playfully as “Baby Bear”, “Mama Bear” and “Papa Bear”, after the “Goldilocks” fairy tale. Presumably they are looking for a dig that will be “just right”.
  2. The first dig will cut 3/10 of an inch into the permafrost at the location of “Baby Bear”, and scoop up the material.
  3. With the material safely in the scoop, Phoenix will swing its arm 90 degrees towards the onboard miniature oven. It will then wait for further commands.
  4. Assuming the MRO delivers the commands from mission control, Phoenix will be instructed to drop the sample into the oven so it can be baked. Instruments will be used to look deep into the vapour given off to look for signs of carbon or hydrogen-containing organic compounds. It is at this point that the lander will evaluate the samples to see whether there is in fact current water ice on the surface.

Over the next few days samples from all the Goldilocks sites will be analysed. These are exciting times, let’s hope there are no further communications problems…

Source: Associated Press (printed at Physorg.com)

Posted on by Nancy Atkinson

Phoenix Digs on Mars

Phoenix’s first dig in the Martian soil. Image credit: NASA/JPL-Caltech/ University of Arizona

The Phoenix lander used its robotic arm scoop to dig up soil on Mars surface for the first time during its activities during its seventh day on the Red Planet. The image above shows the hole dug by Phoenix, and below is a picture of the scoop itself, with the Martian soil inside.

The plan was to do a test dig and then dump the soil. If that works correctly, then Phoenix will dig another scoop and bring it to the TEGA device on board the lander, the Thermal and Evolved Gas Analyzer, a “furnace” and mass spectrometer instrument that scientists will use to analyze Martian ice and soil samples.

During its previous day’s activities on Sol 6, Phoenix reached out and touched Mars with its robotic arm scoop to make an impression on the Martian surface. And please, no conspiracy theories here, but the impression looks like a footprint, and the Phoenix scientists have dubbed the mark “Yeti.” Touching the surface was a preliminary test for the robotic arm and scoop, to make sure everything was working correctly before making the first scoop.

However, the TEGA device has experienced an intermittent short circuit, and the TEGA scientists are developing a procedure to work around the problem. But Phoenix can still deliver the soil sample to TEGA, and the sample can be held there until the device is working.

Original News Source: Phoenix