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

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