“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

IAU Throws Pluto a Bone: “Plutoid”

Almost two years after the International Astronomical Union (IAU) General Assembly demoted Pluto from a “real” planet to the new category of dwarf planets, the IAU, as promised, has decided on a name for trans-Neptunian dwarf planets similar to Pluto. The name “Plutoid” was proposed and accepted by the IAU at its recent meeting in Oslo, Norway. Here’s the definition of a Plutoid: “Celestial bodies in orbit around the Sun at a distance greater than that of Neptune that have sufficient mass for their self-gravity to overcome rigid body forces so that they assume a hydrostatic equilibrium (near-spherical) shape, and that have not cleared the neighborhood around their orbit.” The two known and named Plutoids are Pluto and Eris. It is expected that more Plutoids will be named as science progresses and new discoveries are made, for example, when the New Horizons mission arrives at the Kuiper Belt region in 2015.

Ceres, however, although a dwarf planet, is not a Plutoid, as it is located in the asteroid belt between Mars and Jupiter. Astronomers believe that Ceres is the only object of its kind. Therefore, a separate category of Ceres-like dwarf planets may be defined and named at a later date.

The IAU has been responsible for naming planetary bodies and their satellites since the early 1900s, and oversees the assignment of names to surface features on bodies in the Solar System.

The IAU confirmed that in French plutoid is “plutoïde,” and in Spanish “plutoide.”

Sources: PhysOrg, International Astronomical Union

GLAST Blasts Off

A powerful new space observatory called GLAST launched successfully today, and will provide a huge leap in our capabilities to study gamma rays, the highest-energy form of light. The Gamma Ray Large Area Space Telescope will enable scientists to answer persistent questions about a broad range of topics, including supermassive black-holes, pulsars, cosmic rays, and searches for signals of new physics in the stars of our galaxy. GLAST blasted off at 12:05 pm EDT, after a brief delay regarding weather and concerns on the water suppression system at the launchpad. But the problems were cleared and the launch proceeded with no complications. Now, the big question is, what will be GLAST’s new name?

As per tradition, GLAST will be renamed with a more user friendly, non-acronym name following it’s successful launch and deployment. The vehicle will go into a parking orbit for about 55 minutes following launch, then the second stage will restart, burn for two minutes, coast for about 5 minutes, then the spacecraft will separate and deploy the solar arrays. That’s when the mission is officially underway.

In its first year of operations, GLAST will concentrate on using its high sensitivity to create a new map of the skies, which is expected to reveal between 5,000 and 10,000 new sources of gamma-rays, which are invisible to human eyes.

The GLAST spacecraft is about 9-feet high by 8-feet in diameter when stowed in the fairing section of the rocket. GLAST will become a little bit taller and much wider after it is launched into space, when the Ku-band antenna deploys and the solar arrays are extended.

With high sensitivity GLAST is the first imaging gamma-ray observatory to survey the entire sky every day. It will give scientists a unique opportunity to learn about the ever-changing universe at extreme energies. GLAST will detect thousands of gamma-ray sources, most of which will be supermassive black holes in the cores of distant galaxies.

The observatory will be a significant upgrade to the previous orbiting gamma-ray telescope, the Compton Gamma Ray Observatory. GLAST should make observations in days that took the Compton years to make.

“GLAST is about to open up the Universe to us in new and exciting ways,” said Steven Ritz, of Nasa’s Goddard Space Science Center, and the project’s chief scientist. “GLAST enables scientists to look under the hood and see how the universe works.”

The mission is an astrophysics and particle physics partnership, developed by NASA in collaboration with the U.S. Department of Energy, along with important contributions from academic institutions and partners in France, Germany, Italy, Japan, Sweden, and the U.S.

Sources: NASA TV, GLAST website

Phoenix Sprinkles Successfully

Successful Sprinkle

The Phoenix Mars Lander used its Robotic Arm during the mission’s 15th Martian sol to test the “sprinkling” method for delivering small samples of soil to instruments on the lander deck. The “movie” shown here is a sequence of four images from the spacecraft’s Surface Stereo Imager, and demonstrates the actions of Phoenix for a 20 minute period. The sprinkling was tested because a couple of days ago, the first attempt at bringing soil samples to the scientific instruments was unsuccessful. The soil, when just dumped as a whole onto Phoenix’s deck, clumped together and wouldn’t go through a screen that brings the materials to the TEGA instrument to analyze the soil. The sprinkling technique, by contrast, holds the scoop at a steady angle and vibrates the scoop by running the motorized rasp located beneath the scoop. This gently jostles some material out of the scoop to the target below.

This method seems to distribute the material better, and “unclumps” the frozen clods of soil. For this test, the target was near the upper end the cover of the Microscopy, Electrochemistry and Conductivity Analyzer instrument suite, or MECA. The cover is 20 centimeters (7.9 inches) across. The scoop is about 8.5 centimeters (3.3 inches) across.

Based on the test’s success in delivering a small quantity and fine-size particles, the Phoenix team plans to use the sprinkle method for delivering more samples to MECA and then to the Thermal and Evolved-Gas Analyzer, or TEGA. The delivery to MECA’s Optical Microscope, will be via the port in the MECA cover, visible at the bottom of the image.

Meanwhile, Phoenix will continue a set of atmospheric observation begun during the Martian evening on Tuesday in coordination with overhead passes of NASA’s Mars Reconnaissance Orbiter. These take advantage of opportunities for instruments on Phoenix and on the orbiter to examine the same column of atmosphere simultaneously from above and below.

“It allows us to put the Phoenix measurements into global perspective and gives a ground level calibration for the orbiter’s measurements,” said Phoenix Project Scientist Leslie Tamppari of the Jet Propulsion Laboratory.

Source: Phoenix News

Launchpad Damage Threatens Future Missions

The damage to Launchpad 39 A is apparently worse than first thought. According to a report from WESH TV in Orlando, not only were bricks blasted from launchpad walls during the launch of Discovery on May 31, 2008, but damage also extended hundreds of square feet under the pad. NASA Officials said engineers inspected the walls and found more areas ready to fail, making the pad dangerous to use. Repairs will begin as soon as possible, as there are only two launchpads for the shuttle. Complicating matters is that both pads, 39 A and 39 B must be available for the next space shuttle mission, a flight to the Hubble Space Telescope, and preliminary work has begun to switch 39 B from a shuttle launch pad to the site where the first Ares rockets will be tested next year for the new Constellation program.

STS-125’s mission to Hubble, scheduled for October 2008, will require a shuttle ready on each launchpad, as post-Columbia flight guidelines require a backup shuttle to serve as a recue ship for any mission not going to the International Space Station, where the crew could take refuge if any damage occurred that would prohibit the shuttle from landing.

So, just closing down the damaged Pad 39A is not an option, said shuttle program manager Leroy Cain. “We need both launch pads, so that’s not a negotiable term at this point.”

But switching to pad 39B as the primary launch pad would also present issues, as this site is currently being readied for launches for the Constellation program.

Last week’s launch tore huge gouges into the pad’s walls. Bricks were blasted and thrown on a roadway a quarter of a mile away, and into the waterway behind the pad. NASA is concerned about bricks being thrust up and damaging the space shuttle during future launches.

“We have lots of things that are susceptible to breaking away, or peeling away and hitting the launch vehicle,”said Leroy Cain. “Will there be impacts to the shuttle program, potentially the station, and no doubt the Constellation program? I’m sure there would be.”

Both launchpads were initially built to launch the Saturn rockets for the Apollo program, back in the 1960’s.

But as it stands now, Launchpad 39 A can’t be used again until NASA determines how and why the damage occurred, and how to prevent it from happening again.

Sources: WESH TV, NASA TV

New Details on Venus’ Clouds from Venus Express

Mysterious clouds blanket Venus, obscuring our sister planet from view. These clouds billow up between 45 and 70 km above the surface, and in the upper part of the atmosphere, clouds swirl by at a rate of 300 km/h, driven by fierce winds. Composed mainly of sulfuric acid along with chlorine and fluorine, these clouds wouldn’t be friendly to life as we know it, but still, their mysteries beckon us. The science team from the European Space Agency’s Venus Express has been imaging the planet’s enigmatic atmosphere, and has released new images in several different wavelengths that provide new details on the clouds of Venus.
Continue reading “New Details on Venus’ Clouds from Venus Express”

Double Spaceship Sighting Alert

Looking for the International Space Station flying overhead is one of my favorite space-related pastimes. But for a couple of evenings (or early mornings, depending where you are) starting on Wednesday, June 11 you can see two spacecraft for the price of one. Space shuttle Discovery is scheduled to undock from the International Space Station on Wednesday morning, June 11th, at 7:42 am EDT. This means some sky watchers will be able to see both spaceships flying in tandem. They’ll be seen as separate but closely-spaced points of light. Double flybys will continue on Thursday the 12th and to a lesser extent on Friday the 13th, with Discovery scheduled to land on Saturday. Southeastern parts of the United States (e.g., Miami and Atlanta) are favored with some especially good viewing, depending, of course, on cloud cover.

To find out if you’ll be able to see spaceships in your area, there are a few different sites to check out:

Spaceweather.com, has a Satellite Tracker Tool. Just put in your zip code (good for the US and Canada) to find out what satellites will be flying over your house.

NASA has a Skywatch page where you can find your specific city to look for satellite sighting info.

Heaven’s Above also has a city search, but also you can input your exact latitude and longitude for exact sighting information, helpful if you live out in the country.

Seeing the two spacecraft flying closely in tandem is a very unique and thrilling sight. Good luck!

And if you like the image above, it is from the current STS-124 mission: Astronaut Mike Fossum used a digital camera to create this self-portrait during one of the EVAs of the mission, with both himself and the International Space Station visible in his helmet visor.

Original News Source: Spaceweather.com

Hubble Zooms In On Coma Galaxy Cluster

The Coma Cluster is one of the densest known clusters of galaxies, containing thousands of elliptical and spherical star systems. The entire cluster is huge, more than 20 million light-years in diameter. It’s also very far away, over 300 million light years distant. But no telescope brings the Coma Cluster closer than the Hubble Space Telescope, and a new Hubble image has captured the magnificent starry population in one area of the Coma Cluster with the Advanced Camera for Surveys.

The above Hubble image focuses on an area that is roughly one-third of the way out from the center of the whole cluster. One bright spiral galaxy is visible in the upper left of the image (see below for a close-up of this galaxy). It is distinctly brighter and bluer than the galaxies surrounding it. A series of dusty spiral arms appears reddish brown against the whiter disc of the galaxy, and suggests that this galaxy has been disturbed at some point in the past. The other galaxies in the image are either elliptical galaxies, S0 (s-zero) galaxies or background galaxies that are far beyond the Coma Cluster sphere.

Ellipticals are featureless “fuzz-balls,” pale golden brown in color and contain populations of old stars. Both dwarf and giant ellipticals are found in abundance in the Coma Cluster.

Farther out from the centre of the cluster there are several spiral galaxies. These galaxies contain clouds of cold gas that are giving birth to new stars. Spiral arms and dust lanes “accessorise” these bright bluish-white galaxies, which have a distinctive disc structure.

S0 (S-zero) galaxies form a morphological class of objects between the better known elliptical and spiral galaxies. They consist of older stars and show little evidence of recent star formation, but they do show some structure — perhaps a bar or a ring that may eventually give rise to more disc-like features.


This image zooms in on one area of the new Hubble image, the stunning Lenticular galaxy (in the lower left of the first image) with numerous background galaxies visible as well.

The cluster’s position in space – near the Milky Way’s north pole— places it in an area not obscured by dust and gas, making it easily visible from Earth.

Original News Source: Hubble Site

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

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