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  • 12
    May
    2013
    6:38pm, EDT

    Project aims to track big city carbon footprints

    AP Photo / Jae C. Hong

    Riley Duren, the chief systems engineer for the Earth Science and Technology Directorate at NASA's Jet Propulsion Laboratory (JPL) demonstrates on the laser radar designed to measure carbon dioxide in the air at Caltech's Linde + Robinson Laboratory in Pasadena, Calif., Friday, April 12, 2013. A mile above this city, sensors gaze down on the basin from atop Mount Wilson the way a satellite fixates on Earth, collecting pieces of information about Los Angeles' carbon footprint.

     

    By Alicia Chang, AP

    LOS ANGELES (AP) - Every time Los Angeles exhales, odd-looking gadgets anchored in the mountains above the city trace the invisible puffs of carbon dioxide, methane and other greenhouse gases that waft skyward.

    Halfway around the globe, similar contraptions atop the Eiffel Tower and elsewhere around Paris keep a pulse on emissions from smokestacks and automobile tailpipes. And there is talk of outfitting Sao Paulo, Brazil, with sensors that sniff the byproducts of burning fossil fuels.

    It's part of a budding effort to track the carbon footprints of megacities, urban hubs with over 10 million people that are increasingly responsible for human-caused global warming.

    For years, carbon dioxide and other greenhouse pollutants have been closely monitored around the planet by stations on the ground and in space. Now, scientists are eyeing large cities — with LA and Paris as guinea pigs — and aiming to observe emissions in the atmosphere as a first step toward independently verifying whether local — and often lofty — climate goals are being met.

    For the past year, a high-tech sensor poking out from a converted shipping container has stared at the Los Angeles basin from its mile-high perch on Mount Wilson, a peak in the San Gabriel Mountains that's home to a famous observatory and communication towers.

    Like a satellite gazing down on Earth, it scans more than two dozen points from the inland desert to the coast. Every few minutes, it rumbles to life as it automatically sweeps the horizon, measuring sunlight bouncing off the surface for the unique fingerprint of carbon dioxide and other heat-trapping gases.

    In a storage room next door, commercially available instruments that typically monitor air quality double as climate sniffers. And in nearby Pasadena, a refurbished vintage solar telescope on the roof of a laboratory on the California Institute of Technology campus captures sunlight and sends it down a shaft 60 feet below where a prism-like instrument separates out carbon dioxide molecules. 

    On a recent April afternoon atop Mount Wilson, a brown haze hung over the city, the accumulation of dust and smoke particles in the atmosphere. 

    "There are some days where we can see 150 miles way out to the Channel Islands and there are some days where we have trouble even seeing what's down here in the foreground," said Stanley Sander, a senior research scientist at the NASA Jet Propulsion Laboratory. 

    What Sander and others are after are the pretty much invisible greenhouse gases spewing from factories and freeways below. 

    There are plans to expand the network. This summer, technicians will install commercial gas analyzers at a dozen more rooftops around the greater LA region. Scientists also plan to drive around the city in a Prius outfitted with a portable emission-measuring device and fly a research aircraft to pinpoint methane hotspots from the sky. (A well-known natural source is the La Brea Tar Pits in the heart of LA where underground bacteria burp bubbles of methane gas to the surface.) 

    Six years ago, elected officials vowed to reduce emissions to 35 percent below 1990 levels by 2030 by shifting to renewable energy and weaning the city's dependence on out-of-state coal-fired plants, greening the twin port complex and airports and retrofitting city buildings.

    It's impractical to blanket the city with instruments so scientists rely on a handful of sensors and use computer models to work backward to determine the sources of the emissions and whether they're increasing. They won't be able to zero in on an offending street or a landfill, but they hope to be able to tell whether switching buses from diesel to alternative fuel has made a dent. 

    Project manager Riley Duren of JPL said it'll take several years of monitoring to know whether LA is on track to reach its goal.

    Scientists not involved with the project say it makes sense to dissect emissions on a city level to confirm whether certain strategies to curb greenhouse gases are working. But they're divided about the focus. 

    Allen Robinson, an air quality expert at Carnegie Mellon University, said he prefers more attention paid to measuring a city's methane emissions since scientists know less about them than carbon dioxide release. 

    Nearly 58 percent of California's carbon dioxide emissions in 2010 came from gasoline-powered vehicles, according to the U.S. Energy Department's latest figures. 

    In much of the country, coal —usually as fuel for electric power — is a major source of carbon dioxide pollution. But in California, it's responsible for a tad more than 1 percent of the state's carbon dioxide emissions. Natural gas, considered a cleaner fuel, spews one third of the state's carbon dioxide. 

    Overall, California in 2010 released about 408 million tons of carbon dioxide into the air. The state's carbon dioxide pollution is greater than all but 20 countries and is just ahead of Spain's emissions. In 2010, California put nearly 11 tons of carbon dioxide into the air for every person, which is lower than the national average of 20 tons per person. 

    Gregg Marland, an Appalachian State University professor who has tracked worldwide emissions for the Energy Department, said there's value in learning about a city's emissions and testing techniques.

    "I don't think we need to try this in many places, but we have to try some to see what works and what we can do," he said. 

    Launching the monitoring project came with the usual growing pains. In Paris, a carbon sniffer originally tucked away in the Eiffel Tower's observation deck had to be moved to a higher floor that's off-limits to the public after tourists' exhaling interfered with the data. 

    So far, $3 million have been spent on the U.S. effort with funding from federal, state and private groups. The French, backed by different sponsors, have spent roughly the same. 

    Scientists hope to strengthen their ground measurements with upcoming launches of Earth satellites designed to track carbon dioxide from orbit. The field experiment does not yet extend to China, by far the world's biggest carbon dioxide polluter. But it's a start, experts say. 

    With the focus on megacities, others have worked to decipher the carbon footprint of smaller places like Indianapolis, Boston and Oakland, where University of California, Berkeley, researchers have taken a different tack and blanketed school rooftops with relatively inexpensive sensors. 

    "We are at a very early stage of knowing the best strategy, and need to learn the pros and cons of different approaches," said Inez Fung, a professor of atmospheric science at Berkeley who has no role in the various projects. 

    Follow Alicia Chang on Twitter at @SciWriAlicia.

    10 comments

    I appreciate that there is at least some concerted effort to measure our impact on our environment, even if it's just in the beginning stages now. The ClimateChange troll above is good example of how public relations money is spent by large CO2 producing industries to discredit common sense science  …

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  • Updated
    20
    Feb
    2013
    12:08am, EST

    Out-of-control spaceship? Nope: It's asteroid 2012 DA14, seen on radar

    Low-resolution imagery from NASA's Goldstone radar dish shows asteroid 2012 DA14 flying away on Feb. 15-16.

    By Alan Boyle, Science Editor, NBC News

    Follow @b0yle


    A pixelated profile from NASA's Goldstone radar dish makes the passing asteroid 2012 DA14 look a bit like an out-of-control Viper space fighter from "Battlestar Galactica." But the real-life asteroid is almost five times as big, and might well pack a bigger wallop if it ever hit our planet.

    NASA's Jet Propulsion Laboratory on Tuesday released a movie combining 73 radar images of 2012 DA14, captured over the course of eight hours on the night of Feb. 15-16. The image resolution is 13 feet (4 meters) per pixel.

    In a news release, NASA said the images show the roughly 130-foot-long (40-meter-long) asteroid moving away from us, at a distance ranging from 74,000 miles to 195,000 miles (120,000 to 314,000 kilometers). These readings were made just hours after the time of closest approach, when the asteroid came within 17,200 miles (27,680 kilometers) of our planet.


    2012 DA14's close encounter on Feb. 15 was eclipsed by the nuclear-scale impact of a meteor over the Russian city of Chelyabinsk earlier in the day — a widely witnessed event that caused more than 1,200 injuries and did an estimated $33 million in damage. NASA said the asteroid behind Russia's meteoric display was about a third the size of 2012 DA14.

    If 2012 DA14 had hit instead, the damage would have been much, much worse. Experts have compared the bigger space rock to the object that blew up over a Siberian forest in 1908, knocking down millions of trees over an 820-square-mile area. As it is, the Russian meteor rates as the biggest observed cosmic impact since Siberia's Tunguska event.

    JPL's radar observations, which continue through Wednesday, are aimed at fine-tuning the calculations of 2012 DA14's future orbit by getting a better fix on its size, shape, rotation, surface features and surface roughness. For what it's worth, the asteroid's estimated length of 40 meters along its long axis is between four and five times the length of the Colonial Viper spacecraft that buzzed the Cylons in the "Battlestar Galactica" TV series.

    The asteroid's path was perturbed by Earth's gravitational field in such a way that it won't come as close in the foreseeable future. However, a better understanding of its orbit and its composition could help scientists prepare for encounters with other asteroids — and figure out the best way to divert potentially threatening near-Earth objects.

    The radar observation campaign is led by JPL's Lance Benner and Marina Brozovic.

    Here are a more views of 2012 DA14 from other observers:

    An international team led by MIT's Nicholas Moskovitz observed asteroid 2012 DA14 with a number of telescopes, including the 2.1-meter telescope at Kitt Peak National Observatory. This animated image shows the asteroid as it was leaving Earth's vicinity. Check out the National Optical Astronomy Observatory's news release for more information. If you missed seeing the animation, click here for a refreshed view.

    2012 DA14 - 2013 Feb. 15 from 20h01 to 20h16 UTC from Francois Colas on Vimeo. The asteroid can be seen moving from lower right to upper left.

    2012 DA14 from Alessandro Della Bella on Vimeo. Go full-screen HD for best results.

    Asteroid 2012 DA 14 from Daniel Lopez on Vimeo.

    Night Wanderers from Colin Legg on Vimeo. Asteroid 2012 DA14 is a bright speck on the left side of the frame, moving from top to bottom. But the video also shows a bright meteor blazing across the sky and leaving a debris train. Watch this video at full-screen HD. (Hat tip to Bad Astronomy's Phil Plait.)

    Follow @CosmicLog

    More about the asteroid:

    • Watch a passing asteroid fade out
    • How it rates among asteroid hits and misses
    • Earth kicks asteroid into safer orbit
    • NBCNews.com's asteroid archive

    Alan Boyle is NBCNews.com's science editor. Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter and adding the Cosmic Log page to your Google+ presence. To keep up with Cosmic Log as well as NBCNews.com's other stories about science and space, sign up for the Tech & Science newsletter, delivered to your email in-box every weekday. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

    This story was originally published on Tue Feb 19, 2013 5:24 PM EST

    36 comments

    The videos are awesome

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  • 26
    Jan
    2013
    4:16pm, EST

    Watch how thawing carbon dioxide sculpts the sand dunes of Mars

    Mars Reconnaissance Orbiter captures the springtime thaw of seasonal carbon dioxide ice on Mars.

    Watch on YouTube
    By Mike Wall, Space.com

    The seasonal thawing of carbon dioxide ice near Mars' north pole carves grooves in the region's sand dunes, three new studies reveal.

    The discovery, made using observations from NASA's Mars Reconnaissance Orbiter spacecraft, or MRO, reinforces that the Red Planet's surface continues to be transformed today, even though Mars' volcanoes have died out and its liquid surface water apparently dried up long ago. 

    "It's an amazingly dynamic process," Candice Hansen of the Planetary Science Institute in Tucson, Ariz., lead author of one of the studies, said in a statement. "We had this old paradigm that all the action on Mars was billions of years ago. Thanks to the ability to monitor changes with the Mars Reconnaissance Orbiter, one of the new paradigms is that Mars has many active processes today."


    MRO photographed dunes in Mars' far northern latitudes using its High Resolution Imaging Science Experiment camera, or HiRISE. The images revealed a number of grooves appearing in the dunes as the northern spring took hold and progressed. [Dry Ice 'Smoke' Moves Mars Sand (Video)]

    The phenomenon is driven by the springtime thawing of a surface layer of frozen carbon dioxide, also known as dry ice.

    This thawing occurs first on the ice layer's underside, which is in contact with the warming ground, researchers said. The dry ice sublimes from a solid state to a gaseous one, and pressure builds as more and more gas is produced and trapped. 

    Eventually, cracks form in the ice, and some of the carbon dioxide gas breaks free, forming temporary grooves in the dune as it hisses out.

    The escaping gas also carries sand, which forms dark streaks as it spills across the dry ice covering the dune. These dark fans disappear as the seasonal ice evaporates, and Martian winds erase most of the newly formed grooves before the next winter and springtime roll around.

    The grooves are smaller versions of the "gullies" MRO has spotted on other, steeper Martian dunes, which were apparently formed in a similar way, researchers said. And similar processes have been observed near the Red Planet's south pole.

    "It is a challenge to catch when and how those changes happen, they are so fast," Ganna Portyankina of the University of Bern in Switzerland, lead author of another one of the studies, said in a statement. "That's why only now we start to see the bigger picture that both hemispheres actually tell us similar stories."

    The three new studies, which appear in the journal Icarus, were based on observations made by MRO over three Martian years, or about six Earth years. The papers document a variety of seasonal changes on Mars, including the dune grooves and the distribution of water frost, which is blown around by springtime winds.

    Follow Space.com senior writer Mike Wall on Twitter @michaeldwall or Space.com @Spacedotcom. We're also on Facebook and Google+.

    • Martian Dry Ice 'Smoke' Moves Dark Sand | Video
    • Photos From NASA's Mars Reconnaissance Orbiter
    • 7 Biggest Mysteries of Mars
    • Mars Myths & Misconceptions: Quiz

    © 2013 Space.com. All rights reserved. More from Space.com.

    12 comments

    Head north Rover Curiosity . Check out and analyze some samples from around those freezing sand dunes . Drilling there should be allot easier also .

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  • 11
    Jan
    2013
    8:13pm, EST

    Flight director's family gets back down to Earth after life on Mars time

    Since its historic landing on Mars, the Curiosity rover's mission has been followed by the whole world. One of the mission's team members took a creative approach to balancing work and family by living on "Mars time."

    By Alan Boyle, Science Editor, NBC News

    Follow @b0yle


    A California family's journey on Mars time had its ups and downs, but NASA flight director David Oh says he's glad he took his wife and kids on the ride.

    "My kids loved it, I loved it, and I think it served to bring the family together," Oh told NBC News on Friday.

    Oh is one of the flight directors for NASA's $2.5 billion Mars Science Laboratory mission, which sent the Curiosity rover on a two-year quest to determine whether the Red Planet ever had the chemical ingredients required for life as we know it. Each Martian day, or sol, is 39 minutes and 35 seconds longer than an Earth day. So, to stay in sync with the mission's initial phase, the team at NASA's Jet Propulsion Laboratory in Pasadena, Calif., was put on a Martian schedule for the first 90 sols.


    That meant that Oh's workday quickly fell out of sync with Earth time. To make it easier on himself, and on his wife and three children, the Oh family decided to spend 30 sols on Mars time.

    "The kids weren't going to get to see Daddy for long periods of time," Oh's wife, Bryn, said. "It just seemed like the right thing to do," 

    The time warp meant that the family dinner could take place at 4 p.m. PT, or 4 a.m., depending on how the Martian day meshed with their earthly schedule. But it also meant the Oh children — 13-year-old Braden, 10-year-old Ashlyn and 8-year-old Devyn — had lots of quality time to learn about what Dad is doing.

    "Curiosity's mission is to go try and find life on another planet, which is totally cool," Ashlyn Oh said.

    Follow @CosmicLog

    David Oh said the rest of the family switched back to Earth time in September, a month after Curiosity's landing, to get into sync with the school schedule. "It really felt like we all had gone off on a journey, and we came back," he recalled. But the tough part of Oh's journey was just beginning: He had to stay on Mars time for an additional 60 sols, and during that period he struggled to juggle his work duties and family time. He remembered some days when he got just four hours of sleep at a time.

    "I was in a state of continual jet lag for the last couple of months," he said.

    Finally, in November, Curiosity's mission team shifted back en masse to an Earth-day schedule. It took Oh a couple of days to adjust, but now he's firmly back on an earthly schedule. The kids are clamoring to live on Mars time again — but that's one trip Oh doesn't plan to repeat anytime soon.

    "It's a once-in-a-lifetime experience," he said.


    Alan Boyle is NBCNews.com's science editor. Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter and adding the Cosmic Log page to your Google+ presence. To keep up with Cosmic Log as well as NBCNews.com's other stories about science and space, sign up for the Tech & Science newsletter, delivered to your email in-box every weekday. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

    11 comments

    What a great way to remember and teach the difference from Mars time to ours . Nice job Oh family . Thanks .

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  • 10
    Jan
    2013
    4:59pm, EST

    Another doomsday threat dies out: Asteroid Apophis won't hit us in 2036

    Apophis, nicknamed the "Doomsday Asteroid," was once considered a potential threat, but now scientists realize the chance of the asteroid colliding with Earth is negligible. NBC's Brian Williams reports.

    By Alan Boyle, Science Editor, NBC News

    Follow @b0yle


    Radar observations made during this week's close encounter with the asteroid Apophis have ruled out the risk of a catastrophic cosmic collision in 2036, NASA says. Experts say it'll be much farther away at that time than it is right now.

    The crucial readings came on Wednesday when the space rock, which is thought to measure at least 885 feet (270 meters wide), approached within 9 million miles (14.5 million kilometers) of Earth. NASA is monitoring Apophis with its 230-foot (70-meter) Goldstone radio dish in California. Optical readings also have come in from the Magdalena Ridge Observatory in New Mexico and the Pan-STARRS observatory in Hawaii.

    The bottom line? "We have effectively ruled out the possibility of an Earth impact by Apophis in 2036," Don Yeomans, manager of NASA's Near-Earth Object Program Office at the Jet Propulsion Laboratory, said today in the all-clear news release. "The impact odds as they stand now are less than one in a million, which makes us comfortable saying we can effectively rule out an Earth impact in 2036. Our interest in asteroid Apophis will essentially be for its scientific interest for the foreseeable future."


    Jon Giorgini, who developed JPL's online Horizons database to keep track of solar system objects, would go even further. He says that according to calculations based on the Goldstone data, Apophis will probably pass by Earth at a distance of 36 million miles (58 million kilometers, or 0.39 AU), and absolutely no closer than 14 million miles (22 million kilometers, or 0.15 AU). "That is a very extreme minimum," he told NBC News. "Nothing else plausible can get you closer."

    Apophis, a.k.a. 2004 MN4, created a huge splash when it was discovered in 2004 because the initial assessment of its orbit gave a 1-in-40 chance of Earth impact in 2029. That would be catastrophic: The space rock is big enough to wipe out a city if it struck land, or create killer tsunami waves if it splashed into the ocean.

    Additional orbital data quickly eliminated the risk for 2029, but showed that it would pass within 20,000 miles (32,000 kilometers) of our planet at that time. That's so close that Earth's gravitational field will perturb Apophis' orbit. The experts worried that if the asteroid passed through a particular half-mile-wide zone in space, known as a "keyhole," its orbit would be perturbed just enough to set up a smash-up during the 2036 encounter. Fortunately, the latest observations indicate that Apophis will miss the keyhole by a long shot.

    Did I just hear a cosmic sigh of relief?

    UH / IA

    The asteroid Apophis, highlighted here by a white circle, was discovered in June 2004.

    Follow @CosmicLog

    There are still a few uncertainties surrounding Apophis: Astronomers don't yet have enough data to determine how the asteroid is spinning or how solar radiation is affecting its orbital path — a phenomenon known as the Yarkovsky effect. Giorgini said that even under the worst-case scenario, the effect won't push Apophis into a collision in 2036. But there could conceivably be other risky encounters in the decades or centuries ahead.

    "There's a non-linear amplification that can really move it around more," Giorgini said.

    Also, there are questions about Apophis' exact size. Just this week, readings from the European Space Agency's Herschel space telescope suggested that the asteroid may be nearly 20 percent bigger than previously thought. But that larger size estimate is based on the assumption that Apophis is a spheroid, and astronomers already know that it's elongated.

    "We're not seeing that larger size in the radar data," Giorgini said.

    By the end of next month, continued radar observations from Goldstone as well as the Arecibo Observatory in Puerto Rico should give astronomers a much better fix on Apophis' spin and its size. When those factors are fully accounted for, the Jet Propulsion Observatory will update its official risk assessment for Apophis — and could take this bad boy off the hit list for good.

    Update for 6:30 p.m. ET: Clark Chapman, senior scientist at the Southwest Research Institute, weighed in on the current state of the asteroid hunt in an email:

    "One thing you should be aware of, and might mention, is that the next Planetary Defense Conference, an every-two-year international meeting, will be held April 15-19 in Flagstaff, Arizona. ... Some presentations are already listed in the program, which should be finalized a week from now, which is the due date for abstracts.

    "An interesting tie-in with the new observations of Apophis is that a similar thing happened with 2011 AG5 a few weeks ago, when observations with the huge Gemini telescope in Hawaii showed that it would, in 2023, miss the roughly 350-km-wide 'keyhole' and, therefore, not strike the Earth in 2040.  Prior to these critical observations, the chance of a 2040 impact was unusually high (though still low in everyday terms) at 1 in 500.

    "A point to be realized is that while the chances of impact in these cases are very low by ordinary standards, they aren't zero, and the consequences of an impact could be very terrible, so it is important to plan and prepare for the possibility of impact until it is ruled out.

    "It was important to get these observations of AG5 in the autumn of 2012, because if it had turned out that AG5 was actually on an impact trajectory, it would have given us an additional year to mount a deflection mission and succeed in deflecting it from the 2023 keyhole. Without making a major observational effort with a very large telescope this autumn, the next routine observational opportunity wasn't until this coming autumn."

    Update for 8:30 p.m. ET: One of NASA's experts on the asteroid threat and two former NASA astronauts have weighed in on the report about Apophis. David Morrison of NASA's Ames Research Center sent these comments via email:

    "One possible angle is the recent proposal from [NASA Administrator] Charlie Bolden, based on a Keck study, that we retrieve a 7-meter carbonaceous near-Earth asteroid and bring it into lunar orbit. There are many questions about this idea, but the one I have in mind is our assumed ability, without Sentinel, to find 7-meter C-type asteroids in Earthlike orbits. If you can't find them, you can’t protect against them, or do anything with them as potential resources." 

    Now here's an email from Ed Lu, a veteran of two space shuttle missions and an extended stay on the International Space Station. Lu now serves as chairman and CEO of the B612 Foundation, which is planning to launch the Sentinel space telescope to track half a million near-Earth asteroids:

    "While it is great that Apophis is much better understood, and we know it won't hit us in 2036, the greatest danger from an asteroid strike is from the ones we haven't yet found.  Of asteroids larger than the one that struck Tunguska in 1908, we know of less than 1 percent of them.  And as David Morrison points out, we can't protect ourselves from the unknown asteroids (or make use of them either). The B612 Foundation Sentinel Space Telescope is going to work on finding and tracking these asteroids."

    And here are some comments from Apollo 9 astronaut Rusty Schweickart, who has played a key role in raising awareness about the threats and opportunities presented by near-Earth objects. It was Schweickart who warned in the wake of Hurricane Katrina that asteroids like Apophis could spark a much more devastating "cosmic Katrina":    

    "I'm hoping that you don’t follow the bad (surprisingly wide) precedent of stating that [the risk from] Apophis has been eliminated.  Please look on the JPL risk page  and especially the more detailed info and note that 1) The 2036 impact possibility is, while significantly reduced, still possible, and 2) that the 2068 impact possibility is now elevated ... to a level that exceeds what the 2036 impact was prior to this apparition.

    "There’s certainly good news re the 2036 impact decreasing in probability ... but frankly it was 1 in 234,000 prior to the new observations ... not exactly an impact probability to worry one. (There are many NEOs with higher impact probability ... but no one pays attention to them ... they aren't the 'poster child' that Apophis is.) My personal reaction was one of surprise that the new 2036 impact was not zero!

    "But/And ... there are more radar observations to integrate in ... as well as optical tracking both now and for the next several years.  Apophis isn't going away ... the impact possibilities are simply shifting around a bit with refinement of the tracking data. 2036 is now less probable; 2068 is now more probable (but still very low).

    "Until JPL and the other guys get more data (enough to really define the Yarkovsky effect), we really won’t be able to get definitive data for longer time scales that we can rely on."

    JPL's Giorgini said the risk assessment that Schweickart mentioned won't be full updated until after Goldstone and Arecibo finish their observational campaign in mid-February — so there may still be a non-zero risk listed until then. But Giorgini is confident that the 2036 risk will disappear when all the observations are factored in. (As of this writing, the estimated risk of collision is listed at 1 chance out of 10,989,000.) But you're right, Rusty: In order to eliminate the risk completely, astronomers will have to get more data about Apophis' physical characteristics. And then there are all those other unknown killer asteroids that might be out to get us...

    More doomsday worries addressed:

    • Asteroid 2012 DA14 won't hit Earth next month
    • Asteroid 2011 AG5 won't hit Earth in 2040
    • This year's big comets won't pose a threat
    • Asteroid-hunting telescope to be launched in 2017

    Alan Boyle is NBCNews.com's science editor. Connect with the Cosmic Log community by "liking" the log's Facebook page, following @b0yle on Twitter and adding the Cosmic Log page to your Google+ presence. To keep up with Cosmic Log as well as NBCNews.com's other stories about science and space, sign up for the Tech & Science newsletter, delivered to your email in-box every weekday. You can also check out "The Case for Pluto," my book about the controversial dwarf planet and the search for new worlds.

    64 comments

    I'm not disappointed . Try not to worry and be happy . Thanks for the article .

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The Case for Pluto
Alan Boyle's first book tells the story of Pluto's ups and downs as well as the discoveries of other dwarf planets in our own solar system and even more alien worlds beyond. Buy "The Case for Pluto" ...

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