Carnival of Space #49

Wolf Rayet Star

Another new host for the Carnival of Space. This week we’re at the home of science journalist Will Gater. Read about the largest stars, gamma ray bursts, black hole interactions, Hubble science and more.

Click here to read the Carnival of Space #49

And if you’re interested in looking back, here’s an archive to all the past carnivals of space. If you’ve got a space-related blog, you should really join the carnival. Just email an entry to [email protected], and the next host will link to it. It will help get awareness out there about your writing, help you meet others in the space community – and community is what blogging is all about. And if you really want to help out, let me know if you can be a host, and I’ll schedule you into the calendar.

Finally, if you run a space-related blog, please post a link to the Carnival of Space. Help us get the word out.

Evidence of Asteroid Impact For Sodom and Gomorrah?

Cuneiform clay tablet. Image Credit: Bristol University

A Cuneiform clay tablet that has puzzled researchers for over 150 years is now believed to describe an asteroid impact in 3123 BC in Austria. Researchers believe the tablet, which seemingly describes a cataclysmic event, may account for the biblical tale of Sodom and Gomorrah. No mention of pillars of salt however, on the clay tablet.

Geologists discovered evidence of a giant landslide centered at Köfels, Austria back in the 19th century. At 500 meters thick and five kilometers in diameter, this landslide mystified researchers trying to figure out why such an event occurred. Some researchers thought the landslide may have been caused by a meteorite impact, because of the evidence of crushing pressures and explosions. But there was no crater, so it didn’t look as an impact site should, and the impact theory fell out of favor. But researchers knew this wasn’t just an ordinary landslide.

But new research brings the impact theory back into play. It centers on another 19th century mystery, a Cuneiform tablet in the British Museum, known as “the Planisphere”. It was found in the remains of the library in the Royal Place at Nineveh, and was made by an Assyrian scribe around 700 BC. It is an astronomical work with drawings of constellations and the text has known constellation names. The clay tablet has attracted a lot of attention but until now no one has come up with a convincing explanation as to what it is.

Alan Bond and Mark Hempsell from Bristol University used computer programs to simulate trajectories and reconstruct the night sky thousands of years ago to establish what the Planisphere tablet refers to. It is a copy of the night notebook of a Sumerian astronomer as he records the events in the sky before dawn on the 29 June 3123 BC (Julian calendar). Half the tablet records planet positions and cloud cover, but the other half of the tablet records an object large enough for its shape to be noted even though it is still in space. The astronomer made an accurate note of its trajectory relative to the stars, which to an error better than one degree is consistent with an impact at Köfels.

The observation suggests the asteroid is over a kilometer in diameter and the original orbit about the Sun was an Aten type, a class of asteroid that orbits close to the earth, that is resonant with the Earth’s orbit. This trajectory explains why there is no crater at Köfels. The incoming angle was very low (six degrees) and means the asteroid clipped a mountain near the town of Längenfeld, 11 kilometers from Köfels, and this caused the asteroid to explode before it reached its final impact point. As it travelled down the valley it became a fireball, about five kilometers in diameter (the size of the landslide). When it hit Köfels it created enormous pressures that pulverized the rock and caused the landslide but because it was no longer a solid object it did not create a classic impact crater.

Mark Hempsell, hinting at the possible fate of Sodom and Gomorrah, added, “Another conclusion can be made from the trajectory. The back plume from the explosion (the mushroom cloud) would be bent over the Mediterranean Sea re-entering the atmosphere over the Levant, Sinai, and Northern Egypt. The ground heating though very short would be enough to ignite any flammable material – including human hair and clothes. It is probable more people died under the plume than in the Alps due to the impact blast.”

This evidence seems to coincide with the biblical story of the legendary dens of vice (“Then the Lord rained down burning sulfur on Sodom and Gomorrah – from the Lord out of the heavens” – Genesis 19:24) but it’s never been categorically proven that the towns actually existed in their suspected location close to the Dead Sea. And the story of Lot’s wife turning into a pillar of salt for turning around to witness the mayhem is just biblical legend as well.

The full translation of the tablet together with the analysis supporting these conclusions can be found in the book, “A Sumerian Observation of the Kofels’ Impact Event” by Bond and Hempsell.

Original News Sources: Bristol University and The Register

Smallest Exo-planet Found

Ignasi Ribas with simulated picture of the new planet. Image Credit: REUTERS/Sergio Perez

We’re getting closer to finding an Earth-like planet out there in the universe. Spanish astronomers announced the discovery of the smallest exo-planet found to date, located 30 light years from earth. “I think we are very close, just a few years away, from detecting a planet like Earth,” team leader Ignasi Ribas said at a news conference on Wednesday April 9, 2008. The newest planet, “GJ 436T” was discovered by a team led by Ribas through its gravitational pull on other planets already discovered around the same star in the constellation of Leo.

The planet has a mass five times the size of Earth, which makes it the smallest extrasolar planet among the roughly 300 identified so far, Ribas said. The astronomers believe the planet could possibly be a rocky, Earth-like planet because of its size. Most of the planets found so far are gas giants like Jupiter.

But Ribas said the new planet is uninhabitable due to the close distance that it orbits its star, which is far less than that between the earth and the sun. Planet GJ 436 orbits close to its small, relatively cool star once every 5.2 Earth days and rotates every 4.2 Earth days.

This latest planet was found by analyzing distortions in the orbit of another, larger planet around the star GJ 436, a technique similar to that used more than 100 years ago to discover Neptune.

“Planets with a mass similar to Earth situated at a distance from their star which allows liquid water on the surface, in other words, a habitable planet, we’re probably a bit further from (discovering those), but we surely will in a decade,” said Ribas of Spain’s CSIC scientific research institute.

Original News Source: Reuters

What Happens When Three Black Holes Collide?

A computer simulation of two black holes colliding, what happens if three collide? (credit: EU Training Network)

The consequences of two black holes colliding may be huge, the energy produced by such a collision could even be detected by observatories here on Earth. Ripples in space-time will wash over the Universe as gravitational waves and are predicted to be detected as they pass through the Solar System. Taking this idea one step further, what would happen if three black holes collide? Sound like science fiction? Well it’s not, and there is observational evidence that three black holes can cluster together, possibly colliding after some highly complex orbits that can only be calculated by the most powerful computers available to researchers…

Caltech/EPFL)
Back in January 2007, a quasar triplet was observed over 10 billion light years away. Quasars are generated by the supermassive black holes eating away at the core of active galaxies. Using the powerful W. M. Keck Observatory, researchers from Caltech were able to peer back in time (10 billion years) to see a period in the Universe’s life when active galaxies and black hole mergers would have been fairly common events (when compared to the calmer Universe of today). They observed three tightly packed quasars, an unprecedented discovery.

Now, scientists Manuela Campanelli, Carlos Lousto and Yosef Zlochower, all working at Rochester Institute of Technology’s Center for Computational Relativity and Gravitation, have simulated the highly complex mechanisms behind three interacting and merging supermassive black holes, much like the situation observed by Keck in 2007. The same group have worked on calculating the collision of two black holes before and have written a code that is powerful enough to simulate the collision of up to 22 black holes. However, 22 black holes probably wouldn’t collide naturally, this simply demonstrates the stability of the code, “Twenty-two is not going to happen in reality, but three or four can happen,” says Yosef Zlochower, an assistant professor. “We realized that the code itself really didn’t care how many black holes there were. As long as we could specify where they were located – and had enough computer power – we could track them.

These simulations are of paramount importance to the gravitational wave detectors such as the Laser Interferometer Gravitational-Wave Observatory (LIGO). So far there has been no firm evidence to come from these detectors, but more time is needed, the LIGO detector requires several years of “exposure time” to collect enough data and remove observational “noise”. But what do gravitational wave astronomers look for? This is the very reason many different cosmic scenarios are being simulated so the characteristics of events like two or three black holes mergers can be identified from their gravitational wave signature.

Gravitational wave astronomers “need to know what to look for in the data they acquire otherwise it will look like just noise. If you know what to look for you can confirm the existence of gravitational waves. That’s why they need all these theoretical predictions.” – Manuela Campanelli, director of RIT’s Center for Computational Relativity and Gravitation.

Source: RIT University News

Next Eclipse Dates

Wondering when the next eclipse is going to be? Book these dates into your calendar now so you won’t miss them.

Next Lunar Eclipse
The next lunar eclipse is going to be on August 16, 2008, the second eclipse of the year. Unfortunately, this will only be a partial eclipse, with the Moon passing only partly through the Earth’s shadow. The entire eclipse will be visible from Africa and Europe, and partially visible from viewers in South America, Asia and Australia.

There will be another partial eclipse on February 9, 2009. We’ll have to wait until December 21, 2010 for the next total lunar eclipse.

Next Solar Eclipse
The next solar eclipse will be on August 1, 2008. Fortunately, this will be a total solar eclipse, where the Moon passes directly in front of the Sun. Unfortunately, the path of totality passes through very northern regions. It starts in Arctic Canada, sweeps through Greenland into Northern Russia. Only in the end does it dip down into Mongolia and China.

Space Station Sacrifices Progress Module to Dump Trash into Pacific

Goodbye Progress 28 - the Russian supply vehicle begins its re-entry (credit: NASA TV)

After all the excitement about last week’s successful docking of the European ATV “Jules Verne”, it’s time to spare a thought for its Russian predecessor. The Progress 28 module was filled with rubbish and unneeded equipment, quietly severed from its docking bay and steered toward Earth. On Monday at 0850 GMT, the selfless module dropped through the atmosphere, burned and eventually reached the Pacific Ocean, sinking into the satellite graveyard 3000 km east of the New Zealand coast…

On February 5th, a Russian Soyuz rocket launched the Progress 28 cargo ship to the International Space Station (ISS) to ferry supplies to the astronauts in orbit. This mission started a very busy period for space traffic controllers. Soon after Progress 28 was sent on its way, Space Shuttle Atlantis blasted off to take the Columbus module to be installed on the station. Then at the start of this month, ESA’s Automated Transfer Vehicle (ATV) sat patiently in an orbital holding pattern until the shuttle undocked and flew back to Earth. Then on April 3rd, the ATV carried out a flawless approach and docking procedure with the ISS.

Watching over all this action on the station was the Progress 28 module attached patiently to the Russian-built Pirs docking compartment. After astronauts had salvaged reusable parts from the Progress module and filled it full of trash, the time came on April 7th to say Spokojnoj Nochi (Russian for “Good Night”) to the ill-fated supply ship to make room for the two Russians and one South Korean to arrive after the Soyuz launch yesterday.

Dropping supply modules into the Pacific may sound unsavoury, but it remains the only viable option to dispose of rubbish and unwanted material when in space. Simply jettisoning it into space cannot be done, there must be a controlled disposal, dumping trash into a used module and blasting it into a re-entry trajectory. Littering Earth orbit is a critical problem, so space agencies are doing the best they can to send potential debris to Earth where most of it can burn up in the atmosphere. Anything left over falls into a predetermined “satellite graveyard” in the worlds largest ocean.

NASA)

Some interesting objects have been dropped from the station into the atmosphere. To mention the most humorous, in 2006 the Russian crew on board the station stuffed an old spacesuit with rubbish and launched “Ivan Ivanovich” into orbit. Ivan lasted for 216 days and set a lifetime record for ISS space debris. The suit eventually succumbed to gravity and burned up in the atmosphere.

The drop zone for spaceship fragments, which did not burn in dense layers of the atmosphere, was located away from navigation routes, about 3,000 kilometers east of the New Zealand capital city of Wellington.” – Russia’s Federal Space Agency spokesperson Valery Lyndin.

Don’t think the sparkling new ATV is being let off either, in six months this hi-tech vehicle will be stuffed with garbage and thrown to a fiery death above the Pacific. Sad really…

Source: Space.com, New Scientist

Amazing Image of the Martian Moon Phobos

Martian moon Phobos

I think this will easily capture the prize for the best space photo of the month. Check out this amazing picture of Mars’ moon Phobos, captured in colour (and 3D) by NASA’s Mars Reconnaissance Orbiter.

The spacecraft snapped the picture on March 23, 2008 during a flyby. It took two separate images of the moon within 10 minutes of each other, which scientists later merged together into a stereo view.

“Phobos is of great interest because it may be rich in water ice and carbon-rich materials,” said Alfred McEwen, HiRISE principal investigator at the Lunar and Planetary Laboratory at the University of Arizona, Tucson.

Previous spacecraft, like Mars Global Surveyor, have actually flown closer to Phobos, and taken higher resolution images, but according to the researchers, “the HiRISE images are higher quality, making the new data some of the best ever for Phobos.”

When MRO took the first picture, Phobos was 6,800 km (4,200 miles) away, and it was able to resolve features as small as 20 metres (65 feet) across. For the second image, the spacecraft was 5,800 km (3,600 miles) away, and could resolve features down to 15 metres (50 feet) across.

Phobos itself is only 22 km (13.5 miles) in diameter. Since it’s so small, it doesn’t have the gravity to pull itself into a sphere, so it has an oblong shape.

Planetary scientists are hoping to understand if there are reserves of water on the surface of the Martian moon, and to get more clues about its history. Did Phobos form with Mars, or was it captured later on?

If you have a pair of red-blue glasses, you can take a look at the 3D view of Phobos on the HiRISE site. Here’s a link.

Original Source: NASA/JPL/HiRISE News Release

Help Move An Asteroid and Other Space-Related Opportunities

Asteroid Deflection Techniques. Image Credit: British National Space Center

If you’ve got some ideas about how to deflect an asteroid or comet heading towards Earth, there’s an opportunity out there to have your concept reviewed by some of the world’s top astronomers and physicists. The only restriction is that you must be a student or a young professional under the age of 33. This announcement comes on the heels of notices of other opportunities for young people to get involved with space missions. The space sector must be listening to recent complaints that the younger generation feels a disconnect to space-related activities. At any rate, these are great opportunities.

Here’s more on the asteroid competition, as well as more ways for students to get involved with space missions:

The “Move An Asteroid 2008” competition is sponsored by the Space Generation Advisory Council. It’s an international technical paper competition looking for unique and innovative concepts for how to deflect an asteroid or comet that may impact the Earth. The competition is open to individuals or teams, and they must write and submit a 3-10 page original technical paper on their innovative concept. The 1st place award is a trip to present the winning paper at this year’s Space Generation Congress (SGC) and International Astronautical Congress (IAC) which take place in Glasgow, Scotland from late September until early October 2008. The 2nd place award is a trip to present at the SGC. Entries are due on June 9, 2008 and winners will be announced on June 30, 2008, the 100th anniversary of the Tunguska Event, the largest asteroid/comet impact event in Earth’s recent history.

Another opportunity is the Cassini Scientist for a Day contest. The contest is open to all students in the U.S. between grades 5 and 12, working alone or in groups of up to four students. This is a competition for the privilege of deciding where to point the cameras onboard the Cassini spacecraft on June 10, 2008. There will be 55 minutes of time where the winners will control of spacecraft, plenty of time to turn it as needed and point the cameras at pretty much any target you’d like. In case you’re not sure what targets would be best, the Cassini team has narrowed the field of possible targets. Deadline for submission is Noon, Pacific Daylight Time on May 8, 2008 (3:00 p.m. Eastern time).

Next, there’s the NASA Quest LIMA Challenge for Students in Grades 4-8. In this challenge, students become scientists and propose Antarctic research. The Landsat Image Mosaic of Antarctica is the first true-color high-resolution satellite view of the Antarctic continent. Using this view of Antarctica, students must develop a research question and debate the value of studying the chosen feature. Registration is currently open and educational resources are available online. This is going on right now, with the deadline for preliminary proposals due on April 20, 2008, so check this one out soon.

Also, there’s a chance for U.S. students to involved working with the mission operations associated with the Mars Reconnaissance Orbiter and specificially the CRISM (Compact Reconnaissance Imaging Spectrometer for Mars) on board MRO, currently orbiting Mars. The project is called Mars Exploration Student Data Teams. This is an ongoing program for high school students, and one adult facilitator is required. This program is facilitated through a cooperative effort by NASA and Arizona State University. Another similar program is the Mars Student Imaging Project that works with the Mars Odyssey orbiter. You can find more info on that program here.

Also ongoing is the ISS EarthKAM (Earth Knowledge Acquired by Middle school students)program, a NASA education program which gives students teachers the chance to choose targets on Earth for pictures to be taken from the International Space Station. Learn more about that program here.

Original News Source: Space Generation Advisory Council

Intel to Protect Microchips from Cosmic Rays

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

As computers become more advanced, the microprocessors inside them shrink in size and use less electrical current. These new, energy efficient chips can be crammed closer together, increasing the number of calculations that can be done per second, therefore making the computer more powerful. But even the mighty supercomputer has its Achilles heel: an increased sensitivity to interference from charged particles originating beyond your office. These highly energetic particles come from space and may cause critical hardware to miscalculate, possibly putting lives at risk.

Foreseeing this problem, microchip manufacturer Intel has begun devising ways to detect when a shower of charged particles may hit their chips, so when they do, calculations can be re-run to iron out any errors…

Cosmic rays originate from our Sun, supernovae and other unknown cosmic sources. Typically, they are very energetic protons that zip through space close to the speed of light. They could be so powerful that on impact with the upper atmosphere of the Earth it has been postulated that they may create micro black holes. Naturally these energetic particles can cause some damage. In fact, they may be a huge barrier to travelling beyond the safety of Earth’s magnetic field (the magnetosphere deflects most cosmic radiation, even astronauts in Earth orbit are well shielded), the health of astronauts will be severely damaged during prolonged interplanetary flight.

But what about on Earth, where we are protected from the full force of cosmic rays? Although a small portion of our annual radiation dose comes from cosmic rays (roughly 13%), they can have extensive effects over large volumes of the atmosphere. As cosmic rays collide with atmospheric molecules, a cascade of light particles is produced. This is known as an “air shower”. The billions of particles within the air shower from a single impact are often highly charged themselves (but of lesser energy than the parent cosmic ray), but the physics behind the air shower is beginning to grow in importance, especially in the realms of computing.

It seems computer microprocessor manufacturer Intel has been pondering the same question. They have just released a patent detailing their plans should a cosmic ray penetrate the atmosphere and hit one of their delicate microchips. The problem will come when computing becomes so advanced that the tiny chips may “misfire” when a comic ray impact event occurs. Should the unlucky chip be hit by a cosmic ray, a spike of electrical current may be exerted across the circuitry, causing a miscalculation.

This may sound pretty benign; after all, what’s one miscalculation in billions? Intel’s senior scientist Eric Hannah explains:

All our logic is based on charge, so it gets interference. […] You could be going down the autobahn [German freeway] at 200 miles an hour and suddenly discover your anti-lock braking system doesn’t work because it had a cosmic ray event.” – Eric Hannah.

After all, computers are getting smaller and cheaper, they are being used everywhere including critical systems like the braking system described by Hannah above. As they are so small, many more chips can occupy computers, increasing the risk. Where a basic, one processor computer may only experience one cosmic ray event in several years (producing an unnoticed calculation error), supercomputers with tens of thousands of processors may suffer 10-20 cosmic ray events per week. What’s more, in the near future even humble personal laptops may have the computing power of today’s supercomputer; 10-20 calculation errors per week would be unworkable, there would be too high a risk of data loss, software corruption or hardware failure.

Orbital space stations, satellites and interplanetary spacecraft also come to mind. Space technology embraces advanced computing as you get far more processing power in a smaller package, reducing weight, size and cost. What happens when a calculation error occurs when a cosmic ray hits a satellite’s circuitry? A single miscalculation could spell the satellite’s fate. I’d dread to think what could happen to future manned missions to the Moon, Mars and beyond.

It is hoped that Intel’s plan may be the answer to this ominous problem. They want to manufacture a cosmic ray event tracker that would detect a cosmic ray impact, and then instruct the processor to recalculate the previous calculations from the point before the cosmic ray struck. This way the error can be purged from the system before it becomes a problem.

There will of course be many technical difficulties to overcome before a fast detector is developed; in fact Eric Hannah admits that it will be hard to say when such a device may become a practical reality. Regardless, the problem has been identified and scientists are working on a solution, at least it’s a start…

Source: BBC