Astrosphere for January 31, 2008

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Enough of this cold, wet January. Let’s have some cold wet February. Your space photo for the day is this astonishing image of the International Space Station captured by Mike Salway. And here’s a bonus. If you follow this link, you’ll see two more images.

Today is the 50th anniversary of the launch of Explorer 1. Nancy looked back here on Universe Today, but we’re not the only ones to mark the day. Here are a selection of articles from Cosmic Log, Astroprof and Space Politics.

Spirit says, it’s a rock. And now you can get the T-shirt.

From Astronomy Picture of the Day comes the Young Cluster Westerlund 2.

Astroblog has Comet Holmes in thrilling stereo.

Daily Galaxy reports on a new strategy to search for wormholes and signs of extraterrestrial intelligence.

If you’ve got some time on your hands, why not go searching for craters on Mars.

And finally, Visual Astronomy has a video of asteroid 2007 TU24’s close approach to the Earth.

Carnival of Space #39

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We’ve got another first-time host for the Carnival of Space this week: Sean Welton and his website, Visual Astronomy. So please take a moment, visit his site, and enjoy the space articles prepared for your education and entertainment. Thanks Sean!

Click here to read the Carnival of Space #39

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.

50 Years Ago: Explorer 1

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The launch of Sputnik in October 1957 changed the world overnight. And with the Soviet Union’s second successful launch of Sputnik 2 the following month, Americans were feeling a little left behind in the dust, especially after the US’s first satellite launch attempt with the Vanguard rocket exploded on the launchpad. But space pioneer Werner Von Braun, shown in this picture with JPL Director William Pickering and scientist James Van Allen, came through with his Jupiter C rocket that launched the US’s first satellite, Explorer 1, into space on January 31, 1958.

Explorer 1 was not all that big, with a length of 203 centimeters (80 inches), a diameter of 15.9 centimeters (6.25 inches), and a weight of 14 kilograms (30.8 pounds). But it did its job, which was, first and foremost, to reach orbit, and then return scientific information.

The Jet Propulsion Laboratory got the assignment of designing and building a scientific payload for the launch, which they accomplished in three months.

The primary science instrument on Explorer 1 was a cosmic ray detector designed to measure the radiation above the atmosphere. Dr. James Van Allen designed the experiment, which revealed a much lower cosmic ray count than expected. Van Allen theorized that the instrument may have been saturated by very strong radiation from a belt of charged particles trapped in space by Earth’s magnetic field. A subsequent launch by Explorer 3 two months later confirmed the existence of these radiation belts, which became known as the Van Allen Belts, in honor of their discoverer.

There were other scientific findings from Explorer 1 as well. Because of its symmetrical shape, Explorer 1 was used to help determine the upper atmospheric densities.

Two other instruments on board looked for micrometeorites in orbit: a micrometeorite detector and an acoustic microphone to detect the sound of an micrometeorite impact. The micrometeorite detector was made of a grid of electrical wires. A micrometeorite of about 10 microns would fracture a wire upon impact, destroy the electrical connection, and record the event. One or two of the wires were destroyed during launch. The equipment worked for about 60 days, but showed only one possible meteorite impact. Data from the acoustical sensor microphone were obtained only when an impact occurred while the satellite was over a ground recording station. However, over an 11-day period (February 1, 1958, to February 12, 1958), 145 impacts were recorded. The high impact rates on one portion of the orbit and the subsequent failures in the satellite’s electronic system were attributed to a meteor shower.

The batteries ran out on Explorer 1 on May 23, 1958 when the last signal was recorded. The US’s first satellite burned up in re-entry of the atmosphere in March of 1970.

Original News Source: Explorer 1

“Suits and Ties” Collaborate on Successful Space Station Repair

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At the end of Wednesday’s successful spacewalk to change out a faulty motor on one of the International Space Station’s solar array positioning devices, the astronauts outside the ISS and flight controllers in Houston were congratulating each other on the group effort it took to pull off this particularly tricky and potentially dangerous repair job.

“You guys looked really good to us. Thanks for making it look so easy,” Mission Control in Houston radioed up to the spacewalkers after their seven-hour and 10 minutes EVA.

“Yeah,” said ISS astronaut Dan Tani. “And we did’t even have to put on a tie.”

This spacewalk really was a collaboration between the “suits and ties” at NASA. The suits — spacesuits, that is — were worn by astronauts Tani and Peggy Whitson. The ties were sported by the engineers and astronauts in Mission Control who planned the repair and guided the spacewalkers during the entire EVA.

Tani and Whitson were thanking one tie-wearing astronaut in particular. Tom Marshburn had practiced the choreography of the spacewalk in the Neutral Buoyancy Lab in Houston, and shared his insights with the spacewalkers. Usually astronauts get to practice their own EVA’s in the enormous pool that contains a mock-up of the ISS. But the Bearing Motor Roll Ring Module on the starboard solar array quit working in December when Whitson and Tani were already on board the station. So the plan and nuances of the EVA were tested in the pool by Marshburn and former ISS resident Suni Williams and relayed up to Tani and Whitson.

The spacewalk was especially hazardous because of the risk of electrical shock from 160 volts of electricity that flows through the arrays. For safety, Whitson and Tani waited until the International Space Station was on the dark side of Earth, giving them only 33 minute increments to complete their tasks. Whitson had to squeeze inside the station’s truss girder to swap out the 250 pound (113 kilograms) garbage can-sized motor.

The new motor successfully performed a 360-degree test spin during the spacewalk. It’s power-generating capabilities were tested successfully as well.

“Yay, it works!” exclaimed Whitson as she and Tani watched the solar wing turn. “Excellent, outstanding…isn’t that cool?”

The successful repair means the station should be able to generate enough power to support the new modules that will be brought on the next shuttle missions, the European Columbus science lab, and the Japanese Kibo labratory.

“Given the complexity of this spacewalk and the risks that we had to manage … we are exceptionally pleased with how things went,” flight director Kwatsi Alibaruho said after the EVA.

In addition to the motor repair, Whitson and Tani also performed another inspection of the station’s starboard Solar Alpha Rotary Joint, a 10-ft wide gear that keeps the solar wings pointing toward the sun The SARJ is not working and is contaminated with metal shavings. The spacewalkers evaluated damage from the debris and collected samples from areas previously unseen.

Alibaruho said the new debris samples will help determine what repairs will be done, perhaps later this year. NASA hopes to launch up to five shuttle flights to the ISS this year.

Wednesday’s EVA was the final planned spacewalk of the Expedition 16 mission and the 101st dedicated to space station assembly and maintenance. The spacewalk also marked the sixth career EVA’s for both Whitson and Tani.

So, there’s just one question for Dan Tani: Which is harder — donning a 280 lb spacesuit or tying a Windsor Knot?

Original News Source: NASA TV

Mercury is Less Like the Moon than Previously Believed

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With Mercury fading in MESSENGER’s rear view mirror, scientists are just starting to pore through the torrent of images sent back. And as you can probably guess, the new mysteries are piling up fast and furious. The planet is much less like the Moon than scientists previously thought.

MESSENGER made its closest approach to Mercury on January 14, passing just a few hundred kilometres above its surface. During the flyby it captured a total of 1,213 images.

One of the most unique features discovered by MESSENGER has been dubbed “The Spider” by scientists. And that’s what it looks like. The feature has a central crater surrounded by more than a hundred narrow, flat-floored troughs (called graben) radiating away.

Unlike the Moon, Mercury has huge cliffs or scarps, which can snake hundreds of kilometres across the planet’s surface. They trace the lines of old volcanic faults, from when the planet was still geologically active.

Because of its small size and high density, Mercury has a surprisingly large pull of gravity. Astronauts walking around its surface would experience 38% of the Earth’s gravity. This higher gravity means that the impact craters look different. Material doesn’t splash out from the impact craters so far, and there are many more secondary crater chains.

“We have seen new craters along the terminator on the side of the planet viewed by Mariner 10 where the illumination of the MESSENGER images revealed very subtle features. Technological advances that have been incorporated in MESSENGER are effectively revealing an entirely new planet from what we saw over 30 years ago,� said Science Team Co-Investigator Robert Strom, professor emeritus at the University of Arizona and the only member of both the MESSENGER and Mariner 10 science teams.

MESSENGER wasn’t just taking pictures. It also had a suite of scientific instruments measuring many features of the planet. Perhaps the most puzzling of these is its magnetic field. Even though Mercury cooled down and solidified eons ago, it still has an magnetic field. This was first detected by Mariner 10, and MESSENGER confirmed it.

This is just the beginning. MESSENGER will return to Mercury on October 6, 2008 to make a second flyby, and then a third on September 29, 2009. The spacecraft make its final return to the planet on March 18, 2011 when it’ll begin a year-long orbital mission.

Original Source: MESSENGER News Release

NASA Announces the Next Shuttle Launch Attempt: February 7, 2008

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After more than a month’s delays, the space shuttle Atlantis is finally ready to head back into space. NASA managers announced that they’ve targeted the shuttle for launch on February 7th, 2008 at 2:45 p.m. EST.

There’s one last little problem, though. Engineers inspecting the shuttle on Tuesday noticed a bent hose in its radiator cooling system. The hose runs from the shuttle body to the radiator panels on the cargo bay doors. It carries Freon to keep the shuttle’s systems cool in space.

So the question is: will the bend be a problem?

“Right now, that hose is perfectly functional,” Space Shuttle Program Manager Wayne Hale said. “Since the hose is not leaking now and the sister hose on Discovery didn’t leak on a number of flights, I’m feeling very positive we’ll come to a good conclusion. But we have to do our work here, the engineers have to do their work and we want to make sure we know what we’re doing before we go fly this vehicle.”

Even though it’s got this bent hose, the shuttle managers feel confident enough to launch Atlantis anyway. But they’re planning to meet again on Saturday to evaluate their testing, and think of any other problems that could happen.

Original Source: NASA Shuttle Status Report

Recovering from a Mass Extinction is Slow Going

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With the diversity of life on Earth, and its ability to exploit every niche, you would think planet could bounce back from a devastating extinction event. Or maybe not. According to researchers from the University of Bristol, life took a full 30 million years to recover from the Permian extinction.

The poor animals alive during the Permian extinctions were struck by three waves of disaster. The largest of these happened at the boundary between the Permian and Triassic periods around 251 million years ago. Geologists think it was caused by large-scale volcanism in Russia which produced the ‘Siberian Traps’ – vast regions of lava 200,000 square km (77,000 square miles) in area. In a geologic heartbeat, 90% of all life on Earth was completely wiped out: insects, planets, marine animals, amphibians, and reptiles… everything. Life never got so close to being completely wiped off the face of the Earth.

Life did bounce back quickly, but diversity didn’t. Instead of the rich ecosystems we see today, very opportunistic creatures filled the empty spaces left behind by the extinction. One example is Lystrosaurus, a hardy herbivore the size of a pig.

Sarda Sahney and Professor Michael Benton at the University of Bristol looked at the recovery of animals like amphibians and reptiles. Although these creatures did make a recovery quickly, it took 30 million years for the number of animals and their diversity to match the pre-extinction levels.

Sahney said: “Our research shows that after a major ecological crisis, recovery takes a very long time. So although we have not yet witnessed anything like the level of the extinction that occurred at the end of the Permian, we should nevertheless bear in mind that ecosystems take a very long time to fully recover.�

This is an important thought to consider now that we’re in one of the most rapid periods of species loss in history.

Original Source: University of Bristol

Innovative Laser Trap Captures Most Neutron-Rich Substance Made On Earth: Helium-8

Configuration of helium isotopes (credit: Physorg.com)
Configuration of helium isotopes (credit: Physorg.com)

US researchers have used a new and innovative method to create, trap and study the elusive helium-8 isotope. Helium-8, containing six neutrons and only two protons, is the most neutron rich substance we can create on Earth and until now, we have been unable to accurately characterize it. Through the use of a “laser trap”, physicists in the U.S. Department of Energy’s Argonne National Laboratory have accurately mapped the distribution of the atom and could help us understand the science behind exotic neutron stars.

So, how do you “trap” a helium-8 isotope? The answer is far from simple, but Argonne physicist Peter Mueller has found a solution. Using the GANIL cyclotron facility in northern France, helium-4, 6, and occasionally helium-8 isotopes can be generated. This is one of the only cyclotrons is the world with enough energy to generate the helium-8 isotope. It is all very well creating the particle, but to separate helium-8 from its other helium isotope siblings requires a clever and highly accurate laser “prison” for the heavier helium isotope to fall in to, whilst allowing the other, lighter, isotopes to fly straight through.

Acting as the “bars” of prison gates, six lasers are accurately aligned at such spacing that only isotopes with the dimensions of helium-8 are trapped. When aligned, helium-8 will fall between them, and should the isotope try to escape, repulsion forces keep the isotope still. Once enough time is allowed to pass (about one helium-8 atom is generated every two minutes) the team fire another two lasers into the middle at the same frequency as the resonant frequency of helium-8. Should the laser prison glow, helium-8 has been captured.

The most common, stable form of helium has two protons and two neutrons. Helium can also have two unstable isotopes, helium-6 (four neutrons) and helium-8 (six neutrons). In the unstable isotopes, the additional neutrons form a “halo” around the compact central core (pictured above). Helium-6 has a halo containing two neutrons and helium-8 has a halo of four neutrons. In the halo containing two neutrons, helium-6 has a distinctive “wobble” as the halo neutrons arrange themselves asymmetrically around the core (i.e. they bunch together). This lopsidedness moves the center of balance away from the core and more toward the halo pair of neutrons. Helium-8 on the other hand wobbles less as the four halo neutrons arrange themselves more symmetrically around the core. The laser trap is the only method known to trap a helium-8 atom, and because of this, the structure of its halo can finally be analyzed to such a high degree of accuracy.

To measure the characteristics of helium-8 is complicated by its radioactivity. Helium-8 has a half-life of only a tenth of a second, so all measurements of the atom must be taken instantly as the “prison glow” is detected. Measurements are therefore taken “on-line”, which is a difficult task in itself.

Detection of the rare helium-8 isotope is a major step to particle physicists and astrophysicists alike. It is important to understand how helium configures itself after production from a particle accelerator, but it is also of use when understanding the properties of cosmic bodies such as neutron stars. The implications of the Argonne experiment will be useful as better spectroscopic observations become available so the signature of the helium-8 structure might be detected other than on Earth.

Source: Physorg.com

Astrosphere for January 30, 2008

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Your space photo for today is Saturn, captured by Mike Salway.

In his Cosmic Log, Alan Boyle talks about the state of science in the US after the recent State of the Union speech.

Phil debunks another Moon hoax claim.

Astronomy Picture of the Day has the closest photos of Asteroid 2007 TU24 during its recent flyby.

Ars Technica reports on a new video game based on Orson Scott Card’s Ender’s Game.

SPACE.com has the news of John Benac’s attempts to get space exploration policies at the forefront of the new election campaign.

For you southern hemispheroids, the February edition of the Southern Skywatch is up. Thanks to Ian Musgrave for the link.

Future astronauts are going to need to drink, so Colony Worlds has the solution.

New Technique for Finding Intermediate Mass Black Holes

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It’s one of the big mysteries in astronomy. There are stellar mass black holes and the supermassive variety, but nothing in between. Where are all the intermediate mass black holes? Astronomers theorize that they could be located in globular star clusters, but nothing definitive has turned up yet. A team of researchers think they’ve come up with a new way to detect intermediate black holes – a way to see them for billions of light-years.

First a little background. When white dwarf stars are in a close binary system with another star, they pull off material, piling it up on their surface. When the white dwarf reaches 1.4 times the mass of our Sun, it reignites in a reaction that happens so quickly the star detonates. This is a Type 1a supernova, and astronomers use them as standard candles to determine distance since they always explode with the same amount of energy.

But researchers from UC Santa Cruz think there’s another situation where you might get a supernova explosion from a white dwarf: when it’s orbiting an intermediate mass black hole.

If a black hole has just the right amount of mass – 500 to 1000 times the mass of the Sun – a white dwarf might get torn apart in a particularly spectacular way. As the dwarf passes the whole, it would get compressed and heated. Its formerly dead material would now have the pressure and temperature to reignite in a powerful explosion similar to a Type 1a supernova.

The explosion would eject more than half of the debris into space, but the rest would fall back into the black hole and form an accretion disk around it. This disk would then emit X-ray radiation detectable by space telescopes like the Chandra X-Ray Observatory.

“This is a new mechanism for ignition of a white dwarf that results in a very different type of supernova than the standard type Ia, and it is followed by an x-ray source,” said Enrico Ramirez-Ruiz, assistant professor of astronomy and astrophysics at the University of California, Santa Cruz.

According to Ramirez-Ruiz, events like this would happen in about 1% of Type 1a supernova explosions. Future surveys, such as the Large Synoptic Survey Telescope, due for completion in 2013, is expected to discover hundreds of thousands of Type 1a supernovae each there. With those kinds of numbers, there should be many of these intermediate black hole interactions detected.

The mass of the white dwarf doesn’t really matter. They ran various sized stars through their simulation and found that you would still get the same outcome; the white dwarf would be tidally disrupted and then it would detonate.

Original Source: UC Santa Cruz News Release