How Far Down is the Center of the Earth?

Cut away of planet Earth

Everyone has wanted to dig a hole down to the center of the Earth at some time in their lives. I think I was in the 3rd grade, and my friends and I tried to dig down as far as we could go. I never told them my goal, but in my heart, we were going all the way through. In the end we actually got down about 2 meters, but the bottom kept filling in with water.

Of course, digging down to the centre of the Earth was always out of reach.

In order to be able to dig down to the center of the Earth, my friends and I would have needed to dig our way through 6,378 km of rock, mantle, and iron. Most of this journey would be through temperatures hot enough to melt rock, getting as high as 7,000 Kelvin at the center.

The first 35 km or so of digging would be through the outer crust of the Earth. Assuming we could actually get through the solid rock, and keep water from filling back into our super deep hole, we might actually be able to make some progress through this.

Temperatures rise as you get deeper, though. One of the deepest mines in the world is the TauTona gold mine in South Africa, a mere 3.6 kilometers deep. Even though this just scratches the surface of the Earth, temperatures at the bottom of TauTona already get as high as 55°C.

Once you break through the crust, you’re into the Earth’s mantle. At this point, you’re looking at about 3,000 km of rock heated to such a high temperature that it’s a liquid. Volcanoes are points on the Earth when magma from the mantle breaks through to the surface.

How we’d dig through that… I have no idea. But let’s say we could.

Then we’d break through into the core of Earth. This region extends for another 3,500 km or so, and its comprised almost entirely of iron, with a little nickel, and some other trace metals. And it’s even hotter than the mantle above it. This is where temperatures get to 7,000 Kelvin. Assuming we could bore through the iron, and could withstand the heat, we could get down to the center of the Earth.

At this point, we would have traveled 6,378 km to complete our journey. And then another 6,378 km to get through the other side and visit the folks in China.

Sources:
http://en.wikipedia.org/wiki/Earth_radius
http://en.wikipedia.org/wiki/TauTona_Mine
http://en.wikipedia.org/wiki/Mantle_%28geology%29

The Latest in Space Fashion from NASA

NASA unveiled a new design of spacesuits for the Constellation program today. Astronauts will be donning the new suits on the first flights of the Orion spaceship, scheduled for 2015, on trips to the International Space Station, with additional EVA suits ready for the first missions to the moon, scheduled for 2020. The spacesuits feature rear entry, enhanced shoulder mobility and modular, interchangeable parts. The spacesuits will be designed and produced by Oceaneering International Inc. of Houston, Texas, which received a contract worth $183.8 million for 2008-2014.

NASA required two spacesuit system configurations for the Constellation program. The first type of spacesuit (Configuration One) will be used for launch and landing operations, as well as inside the spacecraft during an emergency like loss of pressurization of the Orion crew compartment.


Configuration Two will build upon Configuration One and will support lunar surface operations. While preparing to walk on the moon, the astronauts will be able to build their own personal Configuration Two spacesuits by replacing elements of Configuration One with elements specialized for surface operations.

Suits and support systems will be needed for as many as four astronauts on moon voyages and as many as six space station travelers. For short trips to the moon, the suit design will support a week’s worth of moon walks. The system also must be designed to support a significant number of moon walks during potential six-month lunar outpost expeditions. In addition, the spacesuit and support systems will provide contingency spacewalk capability and protection against the launch and landing environment, such as spacecraft cabin leaks.

Video of the new Constellation spacesuits.

Video of spacesuit tests.

Pdf. file for more info on the new spacesuits and the contract award.
Original News Source: NASA Press Release

Alien Mineral From Comet Dust Found in Earth’s Atmosphere

Astoundingly, about 40,000 tons of dust particles fall to Earth each year which originates from space “leftovers,” mostly from disintegrating comets and asteroid collisions. Scientists are very interested in this dust because of its pristine nature –it is made of the original building blocks of the solar system. Some of that dust also resides in Earth’s atmosphere, and for years, NASA has routinely collected cosmic and interplanetary dust from Earth’s stratosphere with high-altitude research aircraft. NASA announced today that a new mineral has been found from this atmospheric research, in material that likely came from a comet.


Usually, any unique dust particles found in the atmosphere are difficult to trace as far as their origin, and whether it came from a comet or other space debris. But this new mineral, a manganese silicide which has been named “Brownleeite,” was discovered within an interplanetary dust particle, or IDP, that appears to have originated from comet 26P/Grigg-Skjellerup. The comet was discovered in 1902 and reappears every 5 years. A new method of collecting IDPs was suggested by space scientist Scott Messenger, from Johnson Space Center. He predicted comet 26P/Grigg-Skjellerup was a source of dust grains that could be captured in Earth’s stratosphere at a specific time of the year.

In response to his prediction, NASA performed stratospheric dust collections, using an ER-2 high-altitude aircraft flown from NASA’s Dryden Flight Research Center at Edwards Air Force Base, Calif. The aircraft collected IDPs from this particular comet stream in April 2003. The new mineral was found in one of the particles. To determine the mineral’s origin and examine other dust materials, a powerful new transmission electron microscope was installed in 2005 at Johnson.

“When I saw this mineral for the first time, I immediately knew this was something no one had seen before,” said Keiko Nakamura-Messenger, also from Johnson Space Center. “But it took several more months to obtain conclusive data because these mineral grains were only 1/10,000 of an inch in size.”

“Because of their exceedingly tiny size, we had to use state-of-the-art nano-analysis techniques in the microscope to measure the chemical composition and crystal structure of Keiko’s new mineral,” said Lindsay Keller, Johnson space scientist and a co-discoverer of the new mineral. “This is a highly unusual material that has not been predicted either to be a cometary component or to have formed by condensation in the solar nebula.”

The mineral was surrounded by multiple layers of other minerals that also have been reported only in extraterrestrial rocks. There have been 4,324 minerals identified by the International Mineralogical Association, or IMA. This find adds one more mineral to that list.

Brownleeite, is named after Donald E. Brownlee, professor of astronomy at the University of Washington, Seattle. Brownlee founded the field of IDP research. The understanding of the early solar system established from IDP studies would not exist without his efforts. Brownlee also is the principal investigator of NASA’s Stardust mission.

Brownlee says he’s always been intrigued by minerals and now “it’s great to be one.”

Original News Source: PhysOrg, AP

Where are the Sunspots? Are we in for a Quiet Solar Cycle?

The Suns photosphere is looking particulary boring (NASA/SOHO)
The Suns photosphere is looking particulary boring (NASA/SOHO)

So what’s up with our Sun? Is it going through a depression? It seems as if our closest star is experiencing a surprisingly uneventful couple of years. Solar minimum has supposedly passed and we should be seeing a lot more magnetic activity, and we certainly should be observing lots more sunspots. Space weather forecasts have been putting Solar Cycle 24 as a historically active cycle… but so far, nothing. So what’s the problem? Is it a ticking bomb, waiting to shock us with a huge jump in solar activity, flares and CMEs over a few months? Or could this lack of activity a prelude to a very boring few years, possibly leading the Earth toward another Ice Age?

It’s funny. Just as we begin to get worried that the next solar maximum is going to unleash all sorts of havoc on Earth (i.e. NASA’s 2006 solar storm warning), scientists begin to get concerned as to whether there is going to be a solar maximum at all. In a conference last week at Montana State University, solar physicists discussed the possibility that the Sun could be facing a long period of calm, leading to the concern that there could be another Maunder Minimum. The Maunder Minimum (named after the late 19th Century solar astronomer Edward W. Maunder, who discovered the phenomenon) was a 17th Century, 30-year period when very few sunspots were observed on the disk of the Sun. It is thought by many scientists that this period contributed to what became known as the “Little Ice Age” here on Earth. As the Sun provides Earth with all its energy, during extended periods when the solar output is lower than average, it seems possible a lack of sunspots on the Sun (i.e. low activity) may be linked with periods of cold down here.

It continues to be dead. That’s a small concern, a very small concern.” – Saku Tsuneta, National Astronomical Observatory of Japan and program manager for the Hinode solar mission.

However, solar physicists are not too worried about this possibility, after all, it’s only been two years since solar minimum. Although activity has been low for the beginning of Cycle 24, sunspots have not been non-existent. In January of this year, a newborn spot was observed, as expected, in high latitude regions. More spots were seen in April. In March, sunspots from the previous solar cycle even made an appearance, putting on an unexpected show of flares and coronal mass ejections (CMEs).

As pointed out by David Hathaway, a solar physicist at NASA’s Marshall Space Flight Center, the fact that sunspots have already been observed in this new cycle means that it is highly unlikely we face anything as extreme as another Maunder Minimum. Hathaway says there is nothing unusual about having a relatively understated solar cycle after several particularly active cycles. Solar Cycle 23 was a very active period for the Sun with a greater than average number of sunspots observed on the solar surface.

It appears there are two different predictions for the activity level of the next solar cycle. On the one hand we have scientists that think this cycle might be below average, and on the other hand we have scientists who believe the next cycle will be the biggest yet. We certainly have a long way to go before we can begin making any accurate solar forecasts…

Source: Space.com

Weekend SkyWatcher’s Forecast – June 13-16, 2008

Fra Mauro by Wes Higgins

Greetings, fellow SkyWatchers! It’s big… It’s bright… It’s the Moon! The greatest night sky light polluter is back on the scene, but that doesn’t mean we can’t have a great time as we use telescopes or binoculars to explore the Apollo 14 mission landing site. We’ll continue to visit the lunar surface this weekend, as well as take a look at double stars and two arriving meteor showers. Sky to bright to see meteors? Then let’s try something new….

Friday, June 13 – Today in 1983, Pioneer 10 became the first man made object to leave the solar system. What wonders would it see? Are there other galaxies out there like our own? Will there be life like ours? While we can’t see through Pioneer’s “eyes,” tonight let’s take an historic journey to the Moon, as we look at the northeast shore of Mare Cognitum and the Apollo 14 mission landing site – Fra Mauro.

As craters go, 3.9 billion year old Fra Mauro is on the shallow side and spans 95 kilometers. At some 730 meters deep, standing at the foot of one of its walls would be like standing at the bottom of the Grand Canyon… Yet, time has so eroded this crater that its west wall is completely missing and its floor is covered with fissures.

NASAEven though ruined Fra Mauro seems like a forbidding place to land a manned mission, it remained high on the priority list because it is geologically rich. Ill-fated Apollo 13 was to land in a formation north of the crater which was formed by ejecta belonging to the Imbrium Basin – material which had already been mapped telescopically. By returning samples of this material from deep within the Moon’s crust, scientists would have been able to determine the exact time these changes came about.

As you view Fra Mauro tonight, picture yourself in a lunar rover traversing this barren landscape and viewing the rocks thrown out from a long-ago impact. How willing would you be to take on the vision of others and travel to another world?

Saturday, June 14 – As the day begins and you wait on dawn, keep watch for the peak of the Ophiuchid meteor shower with its radiant near Scorpius. The fall rate is poor with only three per hour, but fast moving bolides are common. Today is about the midpoint – and the activity peak – of this 25 day long stream.

Too moony to see anything? Then try an experiment both Ian and I have been working on. When a meteoroid enters our atmosphere, it has an impact on the ionosphere. Take a few moments and download Google Ionosphere and watch what happens as the meteor shower progresses! And don’t forget the “radio” either… Simply tune any FM radio to the lowest frequency that doesn’t receive a clear signal and listen. These ionospheric disturbances will sound like snatches of radio signal, hisses, pops and more. It’s a great way to catch a meteor shower with more than just your eyes!

Wes HigginsTonight let’s venture toward the south shore of Palus Epidemiarum to have a high power look at crater Capuanus. Named for Italian astronomer Francesco Capuano di Manfredonia, this 60 kilometer wide crater boasts a still-tall southwest wall, but the northeast one was destroyed by lava flow. At its highest, it reaches around 1900 meters above the lunar surface, yet drops to no more than 300 meters at the lowest. Look for several strikes along the crater walls as well as more evidence of a strong geological history. To its north is the Hesiodus Rima…a huge fault line extending 300 kilometers across the surface!

To the east, Jupiter is now rising… But give it some time to clear the atmospheric distortion! By far brighter than neighboring stars to the unaided eye, giant Jupiter will move slowly along the ecliptic plane over the course of the evening. To smaller binoculars it is easily observed as an orb with two grey bands across the middle. To larger binoculars, the equatorial belts become much clearer and the four Galilean moons are easily seen with steady hands. To the small telescope, no planet offers greater details. Even at very low magnifying power, the north, south and central equatorial zones are easily observable and all four moons are clear and steady.

Wes HigginsFor most observers, tonight will show Callisto, Ganymede, Europa and Io grouped to the east of the Mighty Jove, but as time progresses, so do their positions! Try observing over a period of several hours and watch just how quickly these four bright moons shuttle around… You might even catch a possible transit of Io!

To the mid-sized telescope, far greater details begin to appear – such as temperate belts on the planet’s surface and the soft appearance of the Great Red Spot. Finer details are visible during steady seeing, and small things like being able to see which satellite is closer to – or further away from – our vantage point become very easy. Simple things, like watching a moon transit the surface and the resulting shadow on the planet are much easier. With a large telescope, seeing details on Jupiter depends more on seeing conditions. While more aperture allows finer views – conditions are everything when it comes to the Mighty Jove!

Wes HigginsSunday, June 15 – As we wait on the sky to darken tonight, let’s start our adventures by taking a close look at crater Kepler. Situated just north of central along tonight’s terminator, this great crater named for Johannes Kepler only spans 32 kilometers, but drops to a deep 2750 meters below the surface. This class I crater is a geological hotspot!

As the very first to be mapped by the U.S. Geological Survey, the area around Kepler contains many smooth lava domes reaching no more than 30 meters above the plains. According to records, in 1963 a glowing red area was spotted near Kepler and extensively photographed. Normally one of the brightest regions of the Moon, the brightness value at the time nearly doubled! Although it was rather exciting, scientists later determined the phenomenon was caused by high energy particles from a solar flare reflecting from Kepler’s high albedo surface. In the days ahead all details around Kepler will be lost, so take this opportunity to have a good look at one awesome small crater!

Palomar Observatory, courtesy of Cal TechWhen skies are dark, it’s time to have a look at the 250 light-year distant silicon star Iota Librae (RA 15 12 13 Dec 19 47 28). This is a real challenge for binoculars – but not because the components are so close. In Iota’s case, the near 5th magnitude primary simply overshadows its 9th magnitude companion! In 1782, Sir William Herschel measured them and determined them to be a true physical pair. Yet, in 1940 Librae A was determined to have an equal magnitude companion only 0.2 arcseconds away… And the secondary was proved to have a companion of its own which echoes the primary. A four star system!

No matter if you stayed up late chasing deep sky, or got up early, right now is the time to catch the peak of the June Lyrids meteor shower. Although the Moon will make observing difficult, it’s still an opportunity for those wishing to log their meteor observations. Look for the radiant near bright Vega – you may see up to 15 faint blue meteors per hour from this branch of the May Lyrid meteor stream. Try the ionosphere and radio observing!!

Wishing you clear skies and a great weekend…

This week’s image credits: Detail view of Fra Mauro, Capuanus, Kepler and Jupiter – Credit: Wes Higgins, Shepard at Frau Mauro – Credit: NASA, Iota Librae – Credit: Palomar Observatory, courtesy of Caltech.

Comet Boattini Sails Towards the Sun

Boattini C/2007 W1 by Dr. Joseph Brimacombe

Serious comet chasers have been watching Comet C/2007 W1 (Boattini) for some time. For awhile, it exceeded its predicted brightness but is back to cruising at normal. During the time this photograph was taken, Boattini was a southern hemisphere object… But not for long. Now its about to round the Sun and head north!

On November 20, 2007 the comet was spotted by Andrea Boattini during the course of the Mt. Lemmon survey in Arizona. Italian Boattini’s interest is in near-Earth asteroids and he during his research has discovered and co-discovered no less than 170 mostly main-belt asteroids. Since that time, Andrea has become involved with the Catalina and Mt. Lemmon program and has made several additional asteroid discoveries. Of these, object 2007 WD5, made headlines during its extremely close approach to Mars at the end of January 2008. Comet C/2007 W1 is Andrea Boattini’s first comet discovery and we hope not the last!

Comet Boattini is sailing through our solar system in a long-period orbit with an oddly small inclination of 10 degrees. In the southern hemisphere, comet observers had a grand chance to watch as it passed 0.21 AU from Earth on June 12, and heads for inferior conjunction by June 15. Right now Comet Boattini is near fifth magnitude and easily seen without aid by experienced southern observers and it’s heading our way…

Comet C/2007 W1 will make its appearance in the northern hemisphere morning sky on July 15th in Cetus as a 7-8th magnitude observing target – easily within reach of small binoculars and telescopes. It will continue to sail north and fade as it heads away from the Sun (and Earth) and will return to a challenging 12th magnitude object. Spectacular? No. Interesting? You betcha’.

What makes Comet C/2007 W1 Boattini a little more special than the rest? Probably because the most recent orbital calculations show that this is W1 Boattini’s first visit into the inner solar system from the Oort Cloud and it won’t be back for about another 63,000 years. While there’s very little chance that it will become another great “first visit” comet like Kohoutek, it’s a great opportunity for you to catch another traveler from the farthest reaches of our solar system.

Good luck!

Comet C/2007 W1 Boattini video and still photography provided by Dr. Joseph Brimacombe from Macedon Ranges Observatory.

New Transistor Could Side-Step Space Radiation Problem

A simulation of the impact a cosmic ray has on entering the atmosphere (credit: AIRES package/Chicago University)

Space is a very dangerous place to be, whether you’re a human or a transistor. Highly energetic particles may hit astronauts, causing damage to their DNA, but as computers become more and more powerful (yet more and more sensitive); the hazards to unprotected circuitry are increasing. There are many examples of satellites and robotic space missions getting hit by energetic particles, sometimes with crippling results. Not only are millions of dollars at stake, lives are put at risk too. Now, using a new technique and material, Northwestern University scientists have developed a new type of transistor with a twist and it is currently being tested on the International Space Station…

Only a few days ago, the spectre of space radiation reared its ugly head. On June 4th, NASA reported that the Mars orbiter Odyssey had been switched to “safe mode” after the spacecraft’s onboard circuitry was hit by energetic particles from the Sun or from deep space. Fortunately, to avoid system errors, the satellite switched itself into “safe-mode” to await an investigation by mission control to assess any damage. It is not thought this event has caused any lasting harm to Odyssey, but it did cause delays in communications between Earth and Phoenix.

Other spacecraft have not been so lucky. One of the earliest examples of satellite failure through space radiation was the world’s first communications satellite, Telstar. In 1962, this historic satellite was launched to provide trans-Atlantic communications for the first time. Unfortunately, it was launched too soon after a high-altitude US nuclear weapon test codenamed “Star Fish Prime” (see the archival footage of the test) which resulted in manmade energization of the Earth’s Van Allen Belts, causing artificial aurorae in equatorial locations such as Hawaii. Little was known at this time about the response of electrical equipment inside a high-energy environment and Telstar was soon severely damaged as its transistors succumbed to the high energy particles a few months later.

As we now have a huge armada of satellites in orbit around the Earth, and an increasing number of exploratory craft throughout the solar system, there are many vulnerabilities to energetic particles ejected by the Sun.

To address this problem, scientists from Northwestern University sent their new design of transistor to the ISS in March on board Space Shuttle Endeavour. Since then these microscopic components have been rigorously tested and exposed to a space environment to see how the new material reacts.

Arrays of printed transistors on flexible plastic (Northwestern University)

Traditionally, computer transistors are manufactured from the semi-conducting material silicon dioxide. Your home computer uses them, deep space missions such as the New Horizons Pluto mission use them; silicon-based electronics have revolutionized the computing world. However, silicon dioxide transistors are susceptible to radiation. Should a high energy particle impact one of the microscopic transistors of millions that can be built in a microchip, silicon-based material captures the particle, causing a loss of charge or a build-up of charge. Either way, this is bad for computing as it can result in calculation errors.

The new transistors developed by Northwestern use a new type of gate dielectric material called self-assembled nanodielectric (SAND). SAND has an added benefit – they can be printed and they are flexible. This has obvious applications for flat-screen technology and condensing vastly complex circuitry into a very small space. As this is a departure from silicon dioxide, these transistors appear to be very robust when faced with a high-radiation environment here on Earth.

The ISS experiments are expected to take a year to complete, so the space computing world will be waiting to see if this new technology can revolutionize space-based instrumentation, protecting valuable spacecraft from the ravages of energetic particles…

For more information:

Source: EurikAlert

Where In The Universe Challenge #8

Its time for another “Where in the Universe” challenge. I’ll admit, this one is a little unusual. And I’ll also admit, the picture here is just part of of a larger image. But, showing the entire image might give it away. Can you guess what this is? This challenge requires high energy for our readers to undertake, I know, and I appreciate everyone who has written to say how much they enjoy “Where in the Universe.” We search across the sky, across the galaxy, and across the universe to find unique images, and hopefully this challenge provides a welcome diversion to your day. Have you made a guess, formulated a speculation, or deduced a deduction? Or do you just know what this is? No peeking below until your guesses are in….

In honor of the successful launch of GLAST today, this image is in memory of the last orbiting gamma ray telescope, the Compton Gamma Ray Observatory. This is the all-sky map produced by the EGRET instrument, or the Energetic Gamma Ray Experiment Telescope. Here’s the full image:

This image shows the emissions from interactions between cosmic rays and the interstellar gas along the plane of our Galaxy, the Milky Way. Some point sources in this map are pulsars along the plane. For example, the Crab and Geminga pulsars are found near the extreme right side of the EGRET all-sky map. One of the major discoveries made by EGRET is the class of objects known as blazars – these are quasars that emit the majority of their electromagnetic energy in the 30 MeV to 30 GeV portion of the spectrum.

The Compton Gamma Ray Observatory was the second of NASA’s Great Observatories. Compton was launched on April 5, 1991 aboard the space shuttle Atlantis, and was safely deorbited and re-entered the Earth’s atmosphere on June 4, 2000.

How’d you do?

Image source: Compton Gamma Ray Observatory site

XMM-Newton Discovers Strange-Shaped Supernova Remnant

X-ray emission from supernova remnant (to the left) and neutron star (to the right). (ESA/XMM-Newton/EPIC)

XMM-Newton has just released this beautiful image of a supernova remnant and its companion neutron star. To be more accurate, it didn’t “discover” the object, remnant G350.1-0.3 had previously been mistaken to be a distant galaxy. The X-ray observatory has reclassified the object as a Milky Way binary system with one neutron star and the remnant of a young supernova. A wonderful tale about mistaken identity and re-opening a cosmic cold-case, a thousand years after the event…

G350.1-0.3 is special in so many ways. Many astronomers have dubbed this object a “celestial gem” because it is a strikingly beautiful X-ray observation. Apart from its looks, this re-classification by XMM-Newton is very significant to astrophysicists studying the chemical composition, formation and cause of a supernova event. This said, G350.1-0.3 isn’t any normal supernova remnant.

Supernova remnants are usually observed as symmetrical, expanding “bubbles” of hot stellar plasma. Generally, as a massive star finally dies, the explosion should send material out equally in all directions, it is for this reason they are usually easy to distinguish from background galaxies. G350.1-0.3 doesn’t obey this rule; some outside influence had given the remnant a rather odd shape. In the 1980’s, this celestial object was observed in high-resolution images and the knotted gases in the image gave astronomers the impression that the object was “just another distant galaxy” and then forgotten about. That was until NASA’s X-ray observatory XMM-Newton re-examined the object. It quickly became apparent that it was a supernova remnant in the Milky Way, not a far-flung galaxy.

Radio and X-ray emissions from the supernova remnant (ESA/XMM-Newton/EPIC)

This is also a very young supernova remnant. According to Bryan Gaensler and Anant Tanna, from the University of Sydney, who used XMM-Newton to not only prove appearances can be deceptive, but also that the remnant is only 1000 years old. Finding such a young remnant is extremely valuable. “We’re seeing these heavy elements fresh out of the oven,” said Gaensler when referring to G350.1-0.3. Generally, any supernova remnant over 20,000 years old is pretty much the same as another remnant of that age. Finding one so young, so bright and so close gives astrophysicists a prime opportunity to understand the dynamics of a supernova only a short period of time after it blew.

But why the strange shape? It turns out the supernova detonated right next to a dense cloud of gas about 15,000 light-years from Earth. The cloud strongly influenced the expanding gas, preventing the hot matter from expanding uniformly in all directions. This is rare, misshapen supernova remnants aren’t seen very often.

The supernova may have occurred around the time when William the Conqueror invaded England in 1066; perhaps the Battle of Hastings was being waged when the explosion happened overhead. Unfortunately, it may not have been witnessed:

The X-ray data tell us that there’s a lot of dust lying between it and Earth. Even if you’d been looking straight at it when it exploded, it would’ve been invisible to the naked eye.” – Bryan Gaensler

This is some tremendous detective work by the Australian team and the XMM-Newton telescope, ensuring G350.1-0.3 will never be forgotten again. I just hope they give it a better name soon!

Source: ESA

“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