Keeping Astronauts Safe from Meteoroids

Astronauts Steve Bowen and Alvin drew work in tandem on one of the truss sections of the ISS during the first spacewalk of the STS-133 mission. Credit: NAS

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About 100 tons of meteoroids bombard the Earth’s atmosphere every day. For spacecraft in Earth orbit, a collision with these particles could cause serious damage or catastrophic failure, and a hit on an astronaut or cosmonaut conducting extra-vehicular activities in space would be life-threatening, if not fatal. But before anyone steps outside the space shuttle or the International Space Station, NASA checks with data from Canadian Meteor Orbit Radar to determine if it’s safe.

The CMOR system consists of three identical radar systems slaved together to transmit and receive simultaneously. Credit: University of Western Ontario

Using a series of ‘smart cameras’, a one-of-a-kind triple-frequency radar system and computer modeling, CMOR provides real-time data, tracking a representative sample of the meteoroids around and approaching Earth, which are traveling at hypervelocity speeds averaging 10 km/s (22,000 mph).

The system is based at based at The University of Western Ontario.

“When it’s in orbit, the largest danger posed to the space shuttle is impact from orbital debris and meteoroids,” said Peter Brown, Western physics and astronomy professor. By knowing when meteoroid activity is high, NASA can make operational changes such as shielding vulnerable areas of the shuttle or deferring space walks so astronauts remain protected.

Brown told Universe Today that the meteoroids tracked by the system are from 0.1mm and larger, and it detects the ionization trails left by these meteoroids and not the solid particles themselves.

CMOR records about 2,500 meteoroid orbits per day by using a multi-frequency HF/VHF radar. The radar produces data on the range, angle of arrival, and velocity/orbit in some instances. In operation since 1999, the system has measured 4 million individual orbits, as of 2009.

NASA makes daily decisions based on the data from this system. Radio waves are bounced off the ionization trails of meteors by the radar, allowing the system to provide the data necessary to understand meteoric activity on a given day. “From this information we can figure out how many meteoroids are hitting the atmosphere, as well as the direction they’re coming from and their velocity,” Brown said.

NASA says the greatest challenge is medium size particles (objects with a diameter between 1 cm to 10 cm), because of how difficult they are to track, and they are large enough to cause catastrophic damage to spacecraft and satellites. Small particles less than 1 cm pose less of a catastrophic threat, but they do cause surface abrasions and microscopic holes to spacecraft and satellites.

STS-35 Space Shuttle window pit from orbital debris impact. Credit: NASA

But the radar information from the Canadian system can also be combined with optical data to provide broader information about the space environment and produce models useful during the construction of satellites. Scientists are better able to shield or protect the satellites to minimize the effect of meteoroid impacts before sending them into space.

The ISS is the most heavily shielded spacecraft ever flown, and uses “multishock” shielding, which uses several layers of lightweight ceramic fabric to act as “bumpers,” which shocks a projectile to such high energy levels that it melts or vaporizes and absorbs debris before it can penetrate a spacecraft’s walls. This shielding protects critical components such as habitable compartments and high-pressure tanks from the nominal threat of particles approximately 1 cm in diameter. The ISS also has the capability of maneuvering to avoid larger tracked objects.

The original radar system was developed for measuring winds in the Earth’s upper atmosphere, and has since been modified by Brown and his fellow researchers to be optimized for the kinds of astronomical measurements currently being used by NASA.

When the radar detects meteors, the software analyzes the data, summarizes it and sends it to NASA electronically. Brown’s role is to keep the process running and continue to develop the techniques used to obtain the information over time.

Western has been working co-operatively with NASA for 15 years, and has been involved with its Meteor Environment Office (MEO) since it was created in 2004. The role of the MEO is predominantly to evaluate risk. “Everyone knows that rocks fly through space,” says MEO head Bill Cooke. “Our job is to help NASA programs, like the space station, figure out the risk to their equipment, educate them on the environment and give them models to evaluate the risks posed to spacecrafts and astronauts.”

More information on CMOR.

Source: University of Western Ontario, NASA

MESSENGER’s First Image from Orbit of Mercury

MESSENGER's first image from Mercury orbit, with the bright Debussy crater visible at upper right. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington
MESSENGER's first image from Mercury orbit, with the bright Debussy crater visible at upper right. Credit: NASA/Johns Hopkins University Applied Physics Laboratory/Carnegie Institution of Washington

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Here it is, the first image taken by the MESSENGER spacecraft since entering orbit around Mercury on March 17, and it includes portions of the planet not yet previously seen by spacecraft. The image was taken on today, March 29, 2011 at 5:20 am EDT by the Mercury Dual Imaging System as the spacecraft sailed high above Mercury’s south pole. The dominant rayed crater in the upper portion of the image is Debussy, and the smaller crater Matabei with unusual dark rays is visible to the west of Debussy. The bottom portion of this image near Mercury’s south pole is new territory, with MESSENGER being the first spacecraft to image this region of Mercury.


After capturing its first image, MESSENGER acquired an additional 363 images during six hours before downlinking some of the data to Earth. The MESSENGER team is currently looking over the newly returned data, which are still continuing to come down.

The image was acquired as part of the orbital commissioning phase of the MESSENGER mission. Over the next three days, the spacecraft will acquire 1,185 additional images in support of MDIS commissioning-phase activities. Continuous global mapping of Mercury will begin on April 4.

“The entire MESSENGER team is thrilled that spacecraft and instrument checkout has been proceeding according to plan,” says MESSENGER Principal Investigator Sean Solomon, of the Carnegie Institution of Washington. “The first images from orbit and the first measurements from MESSENGER’s other payload instruments are only the opening trickle of the flood of new information that we can expect over the coming year. The orbital exploration of the Solar System’s innermost planet has begun.”

Several other images will be released tomorrow, March 30, in conjunction with a media teleconference. We’ll get them posted as quickly as possible!

Source: MESSENGER website

Cosmology 101: The End

A1689-zD1, one of the brightest and most distant galaxies, is 12.8 billion light years away - an extremely far distance in our expanding universe. Image credit: NASA/ESA/JPL-Caltech/STScI

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Welcome back to the third, and last, installment of Cosmology 101. So far, we’ve covered the history of the universe up to the present moment. But what happens next? How will our universe end? And how can we be so sure that this is how the story unfolded?

Robert Frost once wrote, “Some say the world will end in fire; some say in ice.” Likewise, some scientists have postulated that the universe could die either a dramatic, cataclysmic death – either a “Big Rip” or a “Big Crunch” – or a slower, more gradual “Big Freeze.” The ultimate fate of our cosmos has a lot to do with its shape. If the universe were open, like a saddle, and the energy density of dark energy increased without bound, the expansion rate of the cosmos would eventually become so great that even atoms would be torn apart – a Big Rip. Conversely, if the universe were closed, like a sphere, and gravity’s strength trumped the influence of dark energy, the outward expansion of the cosmos would eventually come to a halt and reverse, collapsing on itself in a Big Crunch.

Despite the poetic beauty of fire, however, current observations favor an icy end to our universe – a Big Freeze. Scientists believe that we live in a spatially flat universe whose expansion is accelerating due to the presence of dark energy; however, the total energy density of the cosmos is most likely less than or equal to the so-called “critical density,” so there will be no Big Rip. Instead, the contents of the universe will eventually drift prohibitively far away from each other and heat and energy exchange will cease. The cosmos will have reached a state of maximum entropy, and no life will be able to survive. Depressing and a bit anti-climactic? Perhaps. But it probably won’t be perceptible until the universe is at least twice its current age.

At this point you might be screaming, “How do we know all this? Isn’t it all just rampant speculation?” Well, first of all, we know without a doubt that the universe is expanding. Astronomical observations consistently demonstrate that light from distant stars is always redshifted relative to us; that is, its wavelength has been stretched due to the expansion of the cosmos. This leads to two possibilities when you wind back the clock: either the expanding universe has always existed and is infinite in age, or it began expanding from a smaller version of itself at a specific time in the past and thus has a fixed age. For a long time, proponents of the Steady State Theory endorsed the former explanation. It wasn’t until Arno Penzias and Robert Wilson discovered the cosmic microwave background in 1965 that the big bang theory became the most accepted explanation for the origin of the universe.

Why? Something as large as our cosmos takes quite a while to cool completely. If the universe did, in fact, began with the kind of blistering energies that the big bang theory predicts, astronomers should still see some leftover heat today. And they do: a uniform 3K glow evenly dispersed at every point in the sky. Not only that – but WMAP and other satellites have observed tiny inhomogeneities in the CMB that precisely match the initial spectrum of quantum fluctuations predicted by the big bang theory.

What else? Take a look at the relative abundances of light elements in the universe. Remember that during the first few minutes of the cosmos’ young life, the ambient temperature was high enough for nuclear fusion to occur. The laws of thermodynamics and the relative density of baryons (i.e. protons and neutrons) together determine exactly how much deuterium (heavy hydrogen), helium and lithium could be formed at this time. As it turns out, there is far more helium (25%!) in our current universe than could be created by nucleosynthesis in the center of stars. Meanwhile, a hot early universe – like the one postulated by the big bang theory – gives rise to the exact proportions of light elements that scientists observe in the universe today.

But wait, there’s more. The distribution of large-scale structure in the universe can be mapped extremely well based solely on observed anisotropies in the CMB. Moreover, today’s large-scale structure looks very different from that at high redshift, implying a dynamic and evolving universe. Additionally, the age of the oldest stars appears to be consistent with the age of the cosmos given by the big bang theory. Like any theory, it has its weaknesses – for instance, the horizon problem or the flatness problem or the problems of dark energy and dark matter; but overall, astronomical observations match the predictions of the big bang theory far more closely than any rival idea. Until that changes, it seems as though the big bang theory is here to stay.

Japan’s Trash-laden HTV-2 Undocks from ISS

Japan's Kounotori 2 –or ‘White Stork’ – cargo carrier as it arrived at the ISS in January. Credit: Paolo Nespol/NASA

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Japan’s HTV-2 Kounotori resupply ship undocked from the International Space Station at 15.45 GMT on March 28, and will burn up in Earth’s atmosphere sometime early Wednesday March 31. Back in January, the craft brought five metric tons of equipment and supplies to the station, but now it is loaded with trash and unneeded equipment and packing materials. Most of the HTV will likely disintegrate as it passes through the atmosphere, but any pieces left over will find a watery grave in a remote area in the Central Pacific. But sensors on board the HTV-2 will provide data on how the craft behaves during its fiery demise.

The Re-entry Breakup Recorder (REBR) will record temperature, acceleration, rotational rate and other data.

The second HTV from Japan arrived at the ISS on January 27 carrying its cargo of food, water supplies, and equipment. Japan expects to send another seven cargo ships to the station by 2015, with the next one scheduled to arrive in January 2012.

The ISS crew grappled HTV-2 with the Canadarm 2, undocked it from the station and then maneuvered the HTV into a release position about 30 feet below the station. The Space Station Integration and Promotion Center in Tsukuba, Japan was able to handle the commands to activate and check out the freighter’s guidance, navigation and control systems. Because of the March 11 earthquake in Japan, controls of the HTV and Japan’s Kibo laboratory was temporarily handed over to NASA in Houston, but the center is now fully restored for full commanding, telemetry and voice capabilities for the ISS.

The cargo ship will enter the atmosphere on Wednesday at 03.09 GMT, and any remaining fragments will fall into the Pacific Ocean 31 minutes later.

So long Konotori, and we thank you.

Amazing Image: Kepler’s Transiting Exoplanets

Visualization of Kepler's planet candidates shown in transit with their parent stars. Credit: Jason Rowe/Kepler Mission/NASA

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Wow. This remarkable visualization shows every Kepler planetary candidate host star with its transiting companion in silhouette. Jason Rowe from the Kepler science team created the image, and the sizes of the stars and transiting companions are properly scaled. For reference, Rowe has included the Sun with a transiting Earth and Jupiter (below the top row on the right by itself.) The largest star is 6.1 times larger that the Sun and the smallest stars are estimated to be only 0.3 times the radius of the Sun. On his Flickr page, Rowe says the colors of the stars represent how the eye would see the star outside of the Earths atmosphere. “Stars have been properly limb darkened and the companions have been offset relative to one another to match the modeled impact parameter. Some stars will even show more than one planet!” he writes.

For more information and high resolution versions of the image, see Jason Rowe’s Flickr page. This image is featured on today’s (March 29, 2011) Astronomy Picture of the Day.

How to Wake Up an Astronaut: Vote Now

From folk to boogey-woogey to cute kids singing, you’ve got 10 original choices for which song should be the winner of NASA’s Space Rock contest in the Original Songs category. While I’m personally bummed that my song didn’t get chosen as a finalist, the ten choices are creative, fun and really awesome. It’s great to know that there are other songwriters out there who are passionate about space exploration, too! NASA said 1,350 original songs were submitted, including 693 from 47 states in the US, 105 from Canada, and 552 from 61 other countries. The two songs with the most votes will be the first original songs chosen by the public to be played as wakeup music for a shuttle crew, and will be played during the STS-134 mission, sending a ‘rise and shine’ to space shuttle Commander Mark Kelly and his five crewmates during their mission to the International Space Station. Voting runs from Tuesday, March 29 through launch day, which currently is targeted for April 19.

Listen to the songs and vote at the Space Rock webpage.

And you can still participate in the “Face in Space” project, which allows you to send a picture to space via an electronic transfer. During Discovery’s mission, more than 194,000 images flew in space. So far, almost 117,000 images have been submitted to fly aboard shuttle Endeavour’s STS-134 flight. To send your face to space aboard Endeavour, or Atlantis on the STS-135 mission targeted for June, visit the Face in Space Website.

Fancy doing a Messier Marathon this Weekend?

The Messier Catalog
The Messier Catalog Credit: SEDS

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If you are new to astronomy, you may ask “what is a Messier Marathon and how do I do one?”

Basically a Messier Marathon is an all night (Dusk til Dawn) observing session held around mid March/ early April every year, where an observer attempts to see all, or as many of the 110 Messier objects as listed by Charles Messier.

The Messier list includes: Nebulae, Galaxies, Star clusters, Supernovae and many other deep sky objects. All of the objects in the Messier list are observable with small amateur telescopes and many of the objects are observable with binoculars.

The reason why Messier marathons take place from mid March to early April is because this is when all of the objects are visible in one evening. Other times of the year aren’t suitable as some of the objects will be in daylight or below the horizon etc.

You don’t have to be an astronomy ace or a seasoned astronomer to do a Messier marathon, but you will need a good telescope to see all of the objects. You don’t even need to do a full Messier marathon as many people do half marathons and depending on your location, or when you observe, you may not be able to see all 110 objects as there is a very tight window of opportunity and higher latitude observers do lose a couple of objects below the horizon.

Timing is key to enable you to see as many of 110 messier objects as possible. Many astronomers put tables and even star charts on the internet to help observers see as many objects as possible.

Observing starts at dusk and ends after dawn and on average each object gets about 5 minutes of observing time before you have to move onto the next one. There can be a short respite half way through the observing session for food and rest, but this depends on the order and success of the objects you are viewing?

Before starting your night of viewing Charles Messier’s wonders, make sure you have all your equipment ready, are dressed warm as it will get cold, have all your charts and viewing tables ready. It also helps to have a hot drink and something nice to eat.

The best dates this year for doing a Messier Marathon have passed and the sky was drenched with the glow of the full moon, but we still have early April. Good luck.

Charles Messier (26 June 1730 – 12 April 1817) was a French astronomer most notable for publishing an astronomical catalogue consisting of deep sky objects such as nebulae and star clusters that came to be known as the 110 “Messier objects”. The purpose of the catalogue was to help astronomical observers, in particular comet hunters such as himself, distinguish between permanent and transient objects in the sky.

Israel and Russia Sign Space Cooperation Agreement

Officials from Israel and Russia sign a space cooperation agreement. Credit: Israeli governmental news office.

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The Israeli government has signed an agreement with Roscosmos, the Russian space agency, for cooperation in space for peaceful purposes. Areas where the two countries may work together are exploration and research, remote sensing of Earth from space, materials science, space biology and medicine, satellite navigation technology, and launch services. Israel also has similar agreements with NASA and the ESA.

The two countries have already been cooperating extensively in development of high-tech hardware, and Russia has purchased Israeli-made unmanned drones for its security services.

One of the goals of the Israeli Space Agency is to promote innovative scientific projects based on international collaboration.

“The trend of international cooperation and unification of forces for action in space is more and more dominant and there are now several major multinational projects like the space station, handling problems and global warming climate research, spacecraft operation… physics and solar system exploration,” said Dr. Zvi Kaplan, head of the Israeli Space Agency. “We thank all of the organizations that were active in achieving the agreement, including the Foreign Ministry and the Ministry of Justice.”

Those present at the signing included Kaplan, Anatoly Perminov, head of Roscosmos, Israeli Prime Minister Benjamin Netanyahu and Minister of Science and Technology Professor Daniel Hershkowitz, Russian Ambassador to Israel, Peter Stganye, and experts from both countries in space.

According to the Israeli science news website Hayadan, Netanyahu said that the combination of Russia’s most developed industrial and Israel’s sophisticated technology will provide for improvements and changes for both countries in space.

“The road was indeed was short, but the desire to work together existed, and last year the two sides accelerated the pace, because of the desire to get started,” said Menachem Grinblum, Director General, Ministry of Science and Technology. “We expect the agreement will be translated into joint action research institutions and industries in both countries.”

Source: Hayadan, with special thanks to editor Avi Blizovsky.

Everyday Astronauts

Astronaut Fill'er Up! Image credit and copyright: Hunter Freeman. Used by permission.

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What do astronauts do when they aren’t in space? Commercial photographer Hunter Freeman’s images all seem to have a bit of whimsy included, and his series of suited astronauts doing everyday things us regular humans may find humdrum will bring a smile to your face, guaranteed. Make sure you look for the small, very relevant details! Check out the entire series at this link, and learn more about his work at his website.

Astrophoto: A Mexican Orion

The Orion Nebula from Paredón, Coah, Mexico. Credit: César Cantú

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This stunning new image of the Orion Nebula has a bit of salsa to it! César Cantú of the Chiledog Observatory in Monterrey, Mexico took this image earlier this month. But he had to travel to Paredón, Coah in Mexico to escape the fog to get this great image. Here are the specs: Orion Atlas mount, 90mm Astrotech APO telescope camera; LRGB QSI540, 3 hours with 600 seconds subs. But the fog tried to follow, César told us. “The intention was 4 hours, but the fog did not allow it,” he said. See more of his great images at this website, Astronomía Y Astrofotografía.