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    <title>Astrobiology</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/" />
    <link rel="self" type="application/atom+xml" href="http://astrobiology.com/atom.xml" />
    <id>tag:astrobiology.com,2010-05-17:/13</id>
    <updated>2013-05-23T23:50:55Z</updated>
    <subtitle>Astrobiology Web is an online guide to the origin, evolution, and distribution of life in the Universe as well as all other aspects of space exploration.</subtitle>
    <generator uri="http://www.sixapart.com/movabletype/">Movable Type Pro 4.38</generator>

<entry>
    <title>Smartphone Becomes a Tricorder</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/smartphone-becomes-a-tricorder.html" />
    <id>tag:astrobiology.com,2013://13.71108</id>

    <published>2013-05-23T23:48:34Z</published>
    <updated>2013-05-23T23:50:55Z</updated>

    <summary>Researchers and physicians in the field could soon run on-the-spot tests for environmental toxins, medical diagnostics, food safety and more with their smartphones. University of Illinois at Urbana-Champaign researchers have developed a cradle and app for the iPhone that uses...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Astrobiology (general)" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Tricorder" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="iphone" label="iPhone" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="tricorder" label="tricorder" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Researchers and physicians in the field could soon run on-the-spot tests for environmental toxins, medical diagnostics, food safety and more with their smartphones. University of Illinois at Urbana-Champaign researchers have developed a cradle and app for the iPhone that uses the phone's built-in camera and processing power as a biosensor to detect toxins, proteins, bacteria, viruses and other molecules.</p>]]>
        <![CDATA[<p>Having such sensitive biosensing capabilities in the field could enable on-the-spot tracking of groundwater contamination, combine the phone's GPS data with biosensing data to map the spread of pathogens, or provide immediate and inexpensive medical diagnostic tests in field clinics or contaminant checks in the food processing and distribution chain.</p>

<p>"We're interested in biodetection that needs to be performed outside of the laboratory," said team leader Brian Cunningham, a professor of electrical and computer engineering and of bioengineering at the U. of I. "Smartphones are making a big impact on our society - the way we get our information, the way we communicate. And they have really powerful computing capability and imaging. A lot of medical conditions might be monitored very inexpensively and non-invasively using mobile platforms like phones. They can detect molecular things, like pathogens, disease biomarkers or DNA, things that are currently only done in big diagnostic labs with lots of expense and large volumes of blood."</p>

<p>The wedge-shaped cradle contains a series of optical components - lenses and filters - found in much larger and more expensive laboratory devices. The cradle holds the phone's camera in alignment with the optical components.</p>

<p>At the heart of the biosensor is a photonic crystal. A photonic crystal is like a mirror that only reflects one wavelength of light while the rest of the spectrum passes through.  When anything biological attaches to the photonic crystal - such as protein, cells, pathogens or DNA - the reflected color will shift from a shorter wavelength to a longer wavelength.</p>

<p>For the handheld iPhone biosensor, a normal microscope slide is coated with the photonic material. The slide is primed to react to a specific target molecule. The photonic crystal slide is inserted into a slot on the cradle and the spectrum measured. Its reflecting wavelength shows up as a black gap in the spectrum. After exposure to the test sample, the spectrum is re-measured. The degree of shift in the reflected wavelength tells the app how much of the target molecule is in the sample. See a video of the app in action at http://www.youtube.com/watch?v=Kh7MUjIYuyw.</p>

<p>The entire test takes only a few minutes; the app walks the user through the process step by step. Although the cradle holds only about $200 of optical components, it performs as accurately as a large $50,000 spectrophotometer in the laboratory. So now, the device is not only portable, but also affordable for fieldwork in developing nations.</p>

<p>In a paper published in the journal Lab on a Chip, the team demonstrated sensing of an immune system protein, but the slide could be primed for any type of biological molecule or cell type. The researchers are working to improve the manufacturing process for the iPhone cradle and are working on a cradle for Android phones as well. They hope to begin making the cradles available next year.</p>

<p>Cunningham's group is now collaborating with other groups across campus at the U. of I. to explore applications for the iPhone biosensor. The group recently received a grant from the National Science Foundation to expand the range of biological experiments that can be performed with the phone, in collaboration with Steven Lumetta, a professor of electrical and computer engineering and of computer science at the U. of I. They are also are also working with food science and human nutrition professor Juan Andrade to develop a fast biosensor test for iron deficiency and vitamin A deficiency in expectant mothers and children.</p>

<p>In addition, Cunningham's team is working on biosensing tests that could be performed in the field to detect toxins in harvested corn and soybeans, and to detect pathogens in food and water.</p>

<p>"It's our goal to expand the range of biological experiments that can be performed with a phone and its camera being used as a spectrometer," Cunningham said. "In our first paper, we showed the ability to use a photonic crystal biosensor, but in our NSF grant, we're creating a multi-mode biosensor. We'll use the phone and one cradle to perform four of the most widely used biosensing assays that are available."</p>

<p>Cunningham also is affiliated with the Institute for Genomic Biology, the Beckman Institute for Advanced Science and Technology, and the Micro and Nanotechnology Laboratory, all at the U. of I. </p>]]>
    </content>
</entry>

<entry>
    <title>Wild Weather Could Be Ahead on Titan</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/wild-weather-could-be-ahead-on-titan.html" />
    <id>tag:astrobiology.com,2013://13.71107</id>

    <published>2013-05-23T23:28:57Z</published>
    <updated>2013-05-23T23:30:58Z</updated>

    <summary>Saturn&apos;s moon Titan might be in for some wild weather as it heads into its spring and summer, if two new models are correct. Scientists think that as the seasons change in Titan&apos;s northern hemisphere, waves could ripple across the...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Europa and Icy Moons" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Global Climate &amp; Habitability" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="cassini" label="Cassini" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="saturn" label="Saturn" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="titan" label="Titan" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Saturn's moon Titan might be in for some wild weather as it heads into its spring and summer, if two new models are correct. Scientists think that as the seasons change in Titan's northern hemisphere, waves could ripple across the moon's hydrocarbon seas, and hurricanes could begin to swirl over these areas, too. </p>]]>
        <![CDATA[<p>The model predicting waves tries to explain data from the moon obtained so far by NASA's Cassini spacecraft. Both models help mission team members plan when and where to look for unusual atmospheric disturbances as Titan summer approaches.</p>

<p>"If you think being a weather forecaster on Earth is difficult, it can be even more challenging at Titan," said Scott Edgington, Cassini's deputy project scientist at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "We know there are weather processes similar to Earth's at work on this strange world, but differences arise due to the presence of unfamiliar liquids like methane. We can't wait for Cassini to tell us whether our forecasts are right as it continues its tour through Titan spring into the start of northern summer."</p>

<p>Titan's north polar region, which is bejeweled with sprawling hydrocarbon seas and lakes, was dark when Cassini first arrived at the Saturn system in 2004. But sunlight has been creeping up Titan's northern hemisphere since August 2009, when the Sun's light crossed the equatorial plane at equinox. Titan's seasons take about seven Earth years to change. By 2017, the end of Cassini's mission, Titan will be approaching northern solstice, the height of summer.</p>

<p>Given the wind-sculpted dunes Cassini has seen on Titan, scientists were baffled about why they hadn't yet seen wind-driven waves on the lakes and seas. A team led by Alex Hayes, a member of Cassini's radar team who is based at Cornell University, Ithaca, N.Y., set out to look for how much wind would be required to generate waves. Their new model, just published in the journal Icarus [http://www.sciencedirect.com/science/article/pii/S0019103513001644], improves upon previous ones by simultaneously accounting for Titan's gravity; the viscosity and surface tension of the hydrocarbon liquid in the lakes; and the air-to-liquid density ratio.</p>

<p>"We now know that the wind speeds predicted during the times Cassini has observed Titan have been below the threshold necessary to generate waves," Hayes said. "What is exciting, however, is that the wind speeds predicted during northern spring and summer approach those necessary to generate wind waves in liquid ethane and/or methane. It may soon be possible to catch a wave in one of the solar system's most exotic locations."</p>

<p>The new model found that winds of 1 to 2 mph (2 to 3 kilometers per hour) are needed to generate waves on Titan lakes, a speed that has not yet been reached during Titan's currently calm period. But as Titan's northern hemisphere approaches spring and summer, other models predict the winds may increase to 2 mph (3 kilometers per hour) or faster. Depending on the composition of the lakes, winds of that speed could be enough to produce waves 0.5 foot (0.15 meter) high.</p>

<p>The other model about hurricanes, recently published in Icarus [<a href="http://www.sciencedirect.com/science/article/pii/S0019103513000389">http://www.sciencedirect.com/science/article/pii/S0019103513000389</a>], predicts that the warming of the northern hemisphere could also bring hurricanes, also known as tropical cyclones. Tropical cyclones on Earth gain their energy from the build-up of heat from seawater evaporation and miniature versions have been seen over big lakes such as Lake Huron. The new modeling work, led by Tetsuya Tokano of the University of Cologne, Germany, shows that the same processes could be at work on Titan as well, except that it is methane rather than water that evaporates from the seas. The most likely season for these hurricanes would be Titan's northern summer solstice, when the sea surface gets warmer and the flow of the air near the surface becomes more turbulent. The humid air would swirl in a counterclockwise direction over the surface of one of the northern seas and increase the surface wind over the seas to possibly 45 mph (about 70 kilometers per hour).</p>

<p>"For these hurricanes to develop at Titan, there needs to be the right mix of hydrocarbons in these seas, and we still don't know their exact composition," Tokano said. "If we see hurricanes, that would be one good indicator that there is enough methane in these lakes to support this kind of activity. So far, scientists haven't yet been able to detect methane directly."</p>

<p>Contact:<br />
Jia-Rui C. Cook<br />
Jet Propulsion Laboratory, Pasadena, Calif.<br />
+1 818-354-0850<br />
jccook@jpl.nasa.gov</p>

<p>The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency, and the Italian Space Agency. The mission is managed by JPL for NASA's Science Mission Directorate, Washington. JPL is a division of the California Institute of Technology in Pasadena, Calif.</p>

<p>More information about Cassini and its mission:<br />
<a href="http://www.nasa.gov/cassini">http://www.nasa.gov/cassini</a><br />
<a href="http://saturn.jpl.nasa.gov">http://saturn.jpl.nasa.gov</a><br />
</p>]]>
    </content>
</entry>

<entry>
    <title>Bacterium from Canadian High Arctic and life on Mars</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/bacterium-from-canadian-high-arctic-and-life-on-mars.html" />
    <id>tag:astrobiology.com,2013://13.71106</id>

    <published>2013-05-23T23:24:16Z</published>
    <updated>2013-05-23T23:27:45Z</updated>

    <summary>The temperature in the permafrost on Ellesmere Island in the Canadian high Arctic is nearly as cold as that of the surface of Mars. So the recent discovery by a McGill University led team of scientists of a bacterium that...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Astrobiology (general)" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Mars" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Polar Research" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="astrobiology" label="Astrobiology" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="ellesmereisland" label="Ellesmere Island" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="mars" label="Mars" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="permafrost" label="permafrost" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>The temperature in the permafrost on Ellesmere Island in the Canadian high Arctic is nearly as cold as that of the surface of Mars. So the recent discovery by a McGill University led team of scientists of a bacterium that is able to thrive at -15oC, the coldest temperature ever reported for bacterial growth, is exciting.</p>]]>
        <![CDATA[<p>The bacterium offers clues about some of the necessary preconditions for microbial life on both the Saturn moon Enceladus and Mars, where similar briny subzero conditions are thought to exist.</p>

<p>The team of researchers, led by Prof. Lyle Whyte and postdoctoral fellow Nadia Mykytczuk, both from the Dept. of Natural Resource Sciences at McGill University, discovered Planococcus halocryophilus OR1 after screening about 200 separate High Arctic microbes looking for the microorganism best adapted to the harsh conditions of the Arctic permafrost. "We believe that this bacterium lives in very thin veins of very salty water found within the frozen permafrost on Ellesmere Island," explains Whyte. "The salt in the permafrost brine veins keeps the water from freezing at the ambient permafrost temperature (~-16oC), creating a habitable but very harsh environment. It's not the easiest place to survive but this organism is capable of remaining active (i.e. breathing) to at least -25oC in permafrost."</p>

<p>In order to understand what it takes to be able to do so, Mykytczuk, Whyte and their colleagues studied the genomic sequence and other molecular traits of P. halocryophilus OR1. The researchers found that the bacterium adapts to the extremely cold, salty conditions in which it is found thanks to significant modifications in its cell structure and function and increased amounts of cold-adapted proteins. These include changes to the membranes that envelop the bacterium and protect it from the hostile environment in which it lives.</p>

<p>The genome sequence also revealed that this permafrost microbe is unusual in other ways. It appears to maintain high levels of compounds inside the bacterial cell that act as a sort of molecular antifreeze, keeping the microbe from freezing solid, while at the same time protecting the cell from the very salty exterior environment.</p>

<p>The researchers believe however, that such microbes may potentially play a harmful role in extremely cold environments such as the High Arctic by increasing carbon dioxide emissions from the melting permafrost, one of the results of global warming.</p>

<p>Whyte is delighted with the discovery and says with a laugh, "I'm kind of proud of this bug. It comes from the Canadian High Arctic and is our cold temperature champion, but what we can learn from this microbe may tell us a lot about how similar microbial life may exist elsewhere in the solar system."</p>

<p>This research was funded by: Natural Sciences and Engineering Research Council of Canada CREATE Canadian Astrobiology Training Program, Canadian Space Agency, the Polar Continental Shelf Program, Canada Research Chairs Program, and the Canada Foundation for Innovation.</p>

<p>Contact Information<br />
Contact: Katherine Gombay<br />
Organization: Media Relations Office<br />
Email: katherine.gombay@mcgill.ca<br />
Office Phone: 514-398-2189</p>]]>
    </content>
</entry>

<entry>
    <title>Kepler&apos;s Dozen&quot; 13 Stories About Distant Worlds That Really Exist</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/keplers-dozen-13-stories-about-distant-worlds-that-really-exist.html" />
    <id>tag:astrobiology.com,2013://13.71080</id>

    <published>2013-05-22T17:01:43Z</published>
    <updated>2013-05-22T17:03:38Z</updated>

    <summary>For centuries, humans have pondered what life on other planets beyond our solar system might be like. With the launch of the Kepler spacecraft in 2009 we now have evidence for the widespread existence of such planets....</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Astrobiology (general)" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Extrasolar Planets" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="exoplanet" label="exoplanet" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="extrasolar" label="extrasolar" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="kepler" label="Kepler" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>For centuries, humans have pondered what life on other planets beyond our solar system might be like. With the launch of the Kepler spacecraft in 2009 we now have evidence for the widespread existence of such planets.</p>]]>
        <![CDATA[<p>Kepler's discovery of hundreds of planet candidates around other stars has inspired a new book that combines both science and science fiction: "A Kepler's Dozen: Thirteen Stories about Distant Worlds that Really Exist." This anthology is co-edited by David Lee Summers (author of "The Pirates of Sufiro" and editor of "Space Pirates") and Dr. Steve Howell, Kepler Project Scientist. (Figure 1)</p>

<p>Each individual story in this book is prefaced by actual scientific data for a particular planet and its host star, based on Kepler discoveries and follow-up. This gives the reader a feel for the type of sun and planets that exist in these alien solar systems. For example, a story titled "A Mango and Two Peanuts" deals with Kepler 37, a star just slightly cooler and less massive than our own Sun, now identified as having three planets in orbit around it, all smaller than Earth.</p>

<p>The Kepler satellite, in orbit around the Sun, stares at a region of the northern hemisphere sky sandwiched between the bright stars Vega and Deneb. Attached to the telescope is the largest imaging camera ever flown into space -- 16 million pixels -- the only instrument on the telescope and the one used to monitor all the stars in its search for planets. Planets are detected if they pass in front of their parent sun, causing a very slight dip in the star's brightness. When this dip repeats periodically, it reveals the presence of a possible planet, the length of the plant's "year", and other information.</p>

<p>The location of the 13 stars featured in this book are marked in the Kepler field, shown over Kitt Peak National Observatory (KPNO) in Figure 2, and numbered using astronomical convention. The planets themselves are named after their host star followed by a lower case letter. For example, the first planet orbiting the star named Kepler 17 would be called Kepler 17b. The next would normally be Kepler 17c and so on. Kepler 17a is the star itself, and the "a" is simply not used.</p>

<p>To date, the Kepler satellite has identified a remarkable 2,500 candidate planets around other stars: however, confirmation of their existence requires further observations from ground-based telescopes. All 13 extrasolar planets featured in this book have been observed from KPNO at either the Mayall 4-meter telescope (seen in Fig. 2) or the WIYN 3.5-meter. Such follow-up observations include gathering spectra of these stars, which tell astronomers far more about the system. (The star field shown in Fig. 2 was taken with a diffraction grating which shows the spectra, or rainbow, of the brighter stars.)</p>

<p><a href="http://www.hadrosaur.com/kepler.html"><img src="http://images/spaceref.com/news/2013/KeplersDozen.jpg" alt="" align="right"></a>Media Contact:</p>

<p>Dr. Katy Garmany, Deputy Press Officer<br />
National Optical Astronomy Observatory<br />
+1 520-318-8526<br />
kgarmany@noao.edu</p>

<p>Science Contact:</p>

<p>Dr. Steve Howell<br />
Project Scientist, Kepler Mission<br />
NASA Ames Research Center<br />
+1 650-604-4238<br />
steve.b.howell@nasa.gov</p>

<p>"A Kepler's Dozen: Thirteen Stories about Distant Worlds that Really Exist":<br />
<a href="http://www.hadrosaur.com/kepler.html">http://www.hadrosaur.com/kepler.html</a><br />
<a href="http://www.amazon.com/Keplers-Dozen-Thirteen-Stories-Distant/dp/1885093683/">http://www.amazon.com/Keplers-Dozen-Thirteen-Stories-Distant/dp/1885093683/</a></p>

<p>Note to Editors: Review copies are available from the publisher, David Lee Summers, Hadrosaur Press, P.O. Box 2194, Mesilla Park, NM 88047-2194; hadrosaur@zianet.com.</p>

<p>Kitt Peak National Observatory is a division of the National Optical Astronomy Observatory (NOAO), which is operated by Association of Universities for Research in Astronomy Inc. (AURA) under a cooperative agreement with the National Science Foundation.</p>]]>
    </content>
</entry>

<entry>
    <title>Kepler Mission Manager Update</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/kepler-mission-manager-update.html" />
    <id>tag:astrobiology.com,2013://13.71074</id>

    <published>2013-05-22T16:08:54Z</published>
    <updated>2013-05-22T16:10:31Z</updated>

    <summary>Following the apparent failure of reaction wheel 4 on May 11, 2013, engineers were successful at transitioning the spacecraft from a Thruster-Controlled Safe Mode to Point Rest State at approximately 3:30 p.m. PDT on Wednesday, May 15, 2013. The spacecraft...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Extrasolar Planets" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="exoplanet" label="exoplanet" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="extrasolar" label="extrasolar" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="kepler" label="Kepler" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Following the apparent failure of reaction wheel 4 on May 11, 2013, engineers were successful at transitioning the spacecraft from a Thruster-Controlled Safe Mode to Point Rest State at approximately 3:30 p.m. PDT on Wednesday, May 15, 2013. The spacecraft has remained safe and stable in this attitude and is no longer considered to be in a critical situation.</p>]]>
        <![CDATA[<p>As part of a normal spacecraft response to a pointing error, redundant electronics were automatically powered off to isolate them as a possible cause. However, once the team recovered the spacecraft to Point Rest State (PRS) and exonerated those systems, they were turned back on, providing full redundancy to the spacecraft. The reaction wheels remain offline. The photometer, which was turned off to reduce the power load, will be turned back on in the near future to keep thermal conditions of the spacecraft within nominal operating parameters. Kepler is not in science data collection.</p>

<p>PRS was developed in order to preserve fuel for an eventual recovery effort once a second wheel failed. This state uses thrusters to control the pointing of the spacecraft, tipping it towards the sun and letting the solar pressure tip it back away, resembling the motion of a pendulum. This is a very fuel-efficient mode, and it also provides an on-demand telemetry link to allow engineers to monitor and command the spacecraft. With nearly a week of PRS operations, the fuel usage appears to be on the low end of our estimates, allowing time for recovery planning. </p>

<p>The operations staff at Ball Aerospace did a wonderful job at developing and implementing PRS. As a result, the spacecraft is not in an emergency condition, and work can be conducted at a more deliberate pace. For the next week or so, we will contact the spacecraft on a daily basis to ensure PRS continues to operate as expected.</p>

<p>Over the coming weeks, an anomaly response team (ART) will evaluate wheel recovery options. The ART includes members from NASA Ames, Ball Aerospace, the Jet Propulsion Laboratory and UTC, the wheel manufacturer. This team has access to a broader reach of experts throughout NASA and industry, and will manage the wheel recovery efforts. </p>

<p>The team will continue to analyze recent telemetry received from the spacecraft. This analysis, and any planned recovery actions, will take time, and will likely be on the order of weeks, possibly months. Any planned commanding will first be vetted on the spacecraft test bed to validate command operability. </p>

<p>For now, PRS is working very well and keeping Kepler safe. We will provide updates on significant changes as the plan develops.</p>

<p>We are grateful to all our followers for their well wishes and support!</p>

<p>Regards,<br />
Roger<br />
</p>]]>
    </content>
</entry>

<entry>
    <title>The Antiquity of Metalloenzymes</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/the-antiquity-of-metalloenzymes.html" />
    <id>tag:astrobiology.com,2013://13.71035</id>

    <published>2013-05-18T19:18:55Z</published>
    <updated>2013-05-18T19:20:00Z</updated>

    <summary>Astrobiologists funded in part by the NASA Astrobiology Institute have uncovered new information about the role of metalloenzymes in the origins of life. Metalloenzymes are enzymes where metals act as a co-factor or are incorporated as part of the molecule....</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Genomics and Cell Biology" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="metalloenzymes" label="Metalloenzymes" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Astrobiologists funded in part by the NASA Astrobiology Institute have uncovered new information about the role of metalloenzymes in the origins of life. Metalloenzymes are enzymes where metals act as a co-factor or are incorporated as part of the molecule. Phylogenetic analysis of metalloenzymes involved in chemiosmosis suggests that they may have been present in the Last Universal Common Ancestor (LUCA) of life on Earth.</p>]]>
        <![CDATA[<p>The paper was published as part of a Special Issue of the journal<a href="http://www.sciencedirect.com/science/article/pii/S0005272813000340"> Biochimica et Biophysica Acta</a> entitled: Metals in Bioenergetics and Biomimetics Systems.</p>]]>
    </content>
</entry>

<entry>
    <title>Mars Icebreaker Life Mission</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/mars-icebreaker-life-mission.html" />
    <id>tag:astrobiology.com,2013://13.71034</id>

    <published>2013-05-18T19:14:43Z</published>
    <updated>2013-05-18T19:16:20Z</updated>

    <summary>Missions to Mars have only scratched its surface. To go deeper, scientists are proposing a spacecraft that can drill into the Red Planet to potentially find signs of life....</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Mars" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="antartica" label="antartica" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="astrobiology" label="astrobiology" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="mars" label="Mars" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Missions to Mars have only scratched its surface. To go deeper, scientists are proposing a spacecraft that can drill into the Red Planet to potentially find signs of life. </p>]]>
        <![CDATA[<p>The driving goal for exploring Mars is finding signs of life, said planetary scientist Christopher McKay at NASA's Ames Research Center. There are mountains of evidence that Mars was once home to liquid water on its surface, and virtually wherever there is water on Earth, there is life. Some researchers have even suggested that life on Earth may have originally come from Mars, stemming from microbes in rocks blasted off the Red Planet by cosmic impacts -- some 220 pounds (100 kilograms) or so of meteorites from Mars are known to have landed on Earth. </p>

<p>Although the cold, thin atmosphere Mars has now means that liquid water cannot last on its surface long, orbital images from NASA's Mariner 9 mission and many other findings since then suggest Mars was once covered in rivers and seas, and that water may have even flowed there recently. Mars also has an atmosphere possessing carbon and nitrogen, essential elements for life as we know it, and organic molecules -- the carbon-based compounds that building blocks of life such as proteins and DNA are made from -- are expected to rain down in meteorites onto Mars, potentially once serving as the raw material for life. </p>

<p>NASA's Viking landers failed to find organic compounds or active microbes on Mars in the 1970s. However, in the last five years, NASA's Phoenix lander unexpectedly discovered that perchlorates seemed common in Martian dirt. Perchlorates are thermally reactive compounds that would destroy organic compounds when heated with them, which the Viking probes did when they analyzed dirt they'd scooped up. As such, the fact Viking did not find organics is no longer conclusive evidence that organics are absent on Mars. </p>

<p>One of the best places to potentially find signs of life or "biomarkers" on Mars is within its near-surface ice, which the Mars Odyssey orbiter revealed is widespread. Such ground ice on Earth is good at preserving organic compounds and biological material -- indeed, experiments have suggested it can preserve living cells for up to millions of years. Ice can also protect organic biomarkers from destruction from radiation from space and harsh chemicals on Mars. </p>

<p>"Why search for a second genesis of life?" McKay asked. "The implication is that life is common in the universe." </p>

<p>As such, McKay and his colleagues have spent about a decade developing the Icebreaker Life mission to Mars. The spacecraft would drill up to about 3 feet (1 meter) down and scan ice shavings for organic biomarkers -- molecules that would be conclusive evidence of life, ones too complex to be produced non-biologically. Discovering any organic biomarkers such as enzymes would not only be evidence of life, but also shed light on the biology of any putative organisms, potentially yielding hints to their genetics and metabolism. </p>

<p>An ideal region for the Icebreaker Life mission to drill would actually be the area where Phoenix landed in 2008. The ice-cemented ground in the northern plains of Mars are the most recently habitable places currently known on Mars -- the atmospheric pressure there is high enough to keep water from automatically boiling away. And as recently as 5 million years ago, Mars was tilted in relation to the Sun enough for its polar regions to receive roughly the same level of summer sunlight as Earth's polar regions do nowadays, so ice might have melted. </p>

<p>"This mission focuses on a far more recent time period of Mars than almost any other mission has. And that is wonderful," said planetary scientist Norbert Schorghofer at the University of Hawaii at Manoa, who did not take part in this research. </p>

<p>The Icebreaker Life drill is rotary-percussive, meaning it both spins and hammers. The drill bit has a heat sensor to detect if the ice is close to melting; the drill will slow or stop to prevent melting, since the water could refreeze and lock the drill. Using a separate robotic arm, the lander could pack samples into a capsule that a future mission could return to Earth. </p>

<p>After every 2 inches (5 centimeters) the drill goes into the ground, a brush collects samples off the drill. A battery of instruments can then analyze this material. For instance, the Signs of Life Detector (SOLID) can detect whole cells, complex organic molecules, and simple compounds of potential biological origin with the aid of a digital camera and the latest generation of lab-on-a-chip technology that essentially shrinks a lab's worth of beakers, flasks and other equipment to fit onto microchips for chemistry experiments. </p>

<p>Other potential instruments can measure acidity, alkalinity, dissolved salts and elemental composition, or use lasers to vaporize samples and scan the gas for organic molecules at low enough temperatures for them not to react with perchlorates. The way compounds soluble in water are spread out in the dirt could shed light on how liquid water might once have flowed on Mars. </p>

<p>Analyses of perchlorates could be especially useful. A number of microbes on Earth are known to live off perchlorates in combination with iron found in volcanic rock, so any microbes on Mars could have done the same thing, the researchers noted. Moreover, perchlorates are toxic to humans, so even if no life is found on Mars, learning more about the chemistry and distribution of perchlorates there might be important for any human missions to the Red Planet. </p>

<p>McKay and his colleagues tested the drill up to 3 feet (1 m) depth at Mars atmospheric pressure and against a wide range of materials, including ice, icy soils, icy soils with rocks, and rocks. They also tested it in the Arctic and the Antarctic, where the ice-cemented ground mimics Mars. In all cases, the drill reached 3 feet (1 m) in depth after about an hour. </p>

<p>The Icebreaker Life mission currently uses the same design as the NASA's solar-powered Phoenix spacecraft with only minor adjustments, and would land near the Phoenix site, operating only during polar summers, the researchers said. Their scenario involves a launch in December 2018 and landing in August 2019. </p>

<p>The scientists also noted the Icebreaker Life payload could accompany other Mars landing systems. For instance, while the SpaceX Dragon capsule is aimed primarily at delivering crew and cargo to the International Space Station, it was also designed to land on Mars, and could deliver the Icebreaker Life mission there. The mission does not have to land at the poles, and does not even have to drill into ice -- for instance, if any massive salt deposits are found on Mars, salt could be nearly as good a preservative for life as ice. </p>

<p>McKay cautioned Mars might neither have life now nor ever had it in the past. In addition, critics might say "we are advocating the search for organic biomarkers and we do not yet have direct evidence for organics. This is a valid criticism," McKay said. </p>

<p>Nevertheless, in the hope a future Icebreaker mission could discover signs of life on Mars, "we continue to develop the drill, the sample handling tools and the biomarker detection instrument," McKay said. The researchers would like to improve how deep Icebreaker can drill -- "right now we're only 1 meter deep. I would like to be deeper," McKay said. </p>

<p>"A question that needs be asked for every life detection mission is: What will we learn if no life is detected?" Schorghofer asked. "For the Icebreaker mission, the answer is delightfully clear -- we will learn a tremendous amount about Mars' recent climate history." </p>

<p>However, the current government financial crisis might doom the Icebreaker Life mission more than any threats on Mars. </p>

<p>"From a technical point of view, it is perfectly possible," Schorghofer added. "From a budgetary and programmatic point of view, it is unlikely to launch as soon as 2018." </p>

<p>The scientists detailed their findings online April 5 in the journal <a href="http://online.liebertpub.com/doi/abs/10.1089/ast.2012.0878">Astrobiology</a>.</p>

<p>Charles Q. Choi, <a href="http://www.astrobio.net/exclusive/5476/mars-icebreaker-life-mission">Astrobiology Magazine</a><br />
</p>]]>
    </content>
</entry>

<entry>
    <title>Astrobiology Daily News 18 May 2013</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/astrobiology-daily-news-18-may-2013.html" />
    <id>tag:astrobiology.com,2013://13.71036</id>

    <published>2013-05-17T19:22:09Z</published>
    <updated>2013-05-18T19:22:57Z</updated>

    <summary>- KOI-127b: a very low-albedo, Saturn-mass transiting planet around a metal rich solar-like star, astro-ph - The effect of rotation and tidal heating on the thermal lightcurves of Super Mercuries, astro-ph - Lucky Imaging of transiting planet host stars with...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Daily Science News" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>- <a href="http://xxx.lanl.gov/abs/1305.3891">KOI-127b: a very low-albedo, Saturn-mass transiting planet around a metal rich solar-like star</a>, astro-ph<br />
- <a href="http://xxx.lanl.gov/abs/1305.3858">The effect of rotation and tidal heating on the thermal lightcurves of Super Mercuries</a>, astro-ph<br />
- <a href="http://xxx.lanl.gov/abs/1305.3795">Lucky Imaging of transiting planet host stars with LuckyCam</a>, astro-ph<br />
- <a href="http://xxx.lanl.gov/abs/1305.3652">The future of the Sun: an evolved solar twin revealed by CoRoT</a>, astro-ph<br />
</p>]]>
        <![CDATA[<p>- <a href="http://astrobiology.com/2013/05/the-antiquity-of-metalloenzymes.html">The Antiquity of Metalloenzymes</a>, NASA<br />
- <a href="http://astrobiology.com/2013/05/mars-icebreaker-life-mission.html">Mars Icebreaker Life Mission</a>, Astrobiology Magazine</p>]]>
    </content>
</entry>

<entry>
    <title>Astrobiology Daily News 15 May 2013</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/astrobiology-daily-news-15-may-2013.html" />
    <id>tag:astrobiology.com,2013://13.71006</id>

    <published>2013-05-16T17:46:13Z</published>
    <updated>2013-05-16T17:46:46Z</updated>

    <summary>- Deep fracture fluids isolated in the crust since the Precambrian era, Nature - An Understanding of the Shoulder of Giants: Jovian Planets around Late K Dwarf Stars and the Trend with Stellar Mass, astro-ph - Evidence for Microbial Carbon...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Daily Science News" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>- <a href="http://www.nature.com/nature/journal/v497/n7449/full/nature12127.html">Deep fracture fluids isolated in the crust since the Precambrian era</a>, Nature<br />
- <a href="http://xxx.lanl.gov/abs/1305.3228">An Understanding of the Shoulder of Giants: Jovian Planets around Late K Dwarf Stars and the Trend with Stellar Mass</a>, astro-ph<br />
- <a href="http://www.sciencemag.org/content/339/6125/1305.full">Evidence for Microbial Carbon and Sulfur Cycling in Deeply Buried Ridge Flank Basalt</a>, Science</p>]]>
        
    </content>
</entry>

<entry>
    <title>Untangling The Tree of Life on Earth</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/untangling-the-tree-of-life-on-earth.html" />
    <id>tag:astrobiology.com,2013://13.70984</id>

    <published>2013-05-15T16:14:10Z</published>
    <updated>2013-05-15T16:16:14Z</updated>

    <summary>Two recent high-profile phylogenetic studies reached conflicting conclusions about whether snail&apos;s closest relatives are bivalves or an enigmatic group called tusk shells. Vanderbilt phylogeneticists suggest that the cause of this conflict is that the three groups diverged rapidly a long...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Genomics and Cell Biology" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Origin &amp; Evolution of Life" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="evolution" label="evolution" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="phylogeny" label="phylogeny" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Two recent high-profile phylogenetic studies reached conflicting conclusions about whether snail's closest relatives are bivalves or an enigmatic group called tusk shells. Vanderbilt phylogeneticists suggest that the cause of this conflict is that the three groups diverged rapidly a long time ago. Credit: Antonis Rokas, Vanderbilt University</p>]]>
        <![CDATA[<p>These days, phylogeneticists - experts who painstakingly map the complex branches of the tree of life - suffer from an embarrassment of riches. The genomics revolution has given them mountains of DNA data that they can sift through to reconstruct the evolutionary history that connects all living beings. But the unprecedented quantity has also caused a serious problem: The trees produced by a number of well-supported studies have come to contradictory conclusions.</p>

<p>"It has become common for top-notch studies to report genealogies that strongly contradict each other in where certain organisms sprang from, such as the place of sponges on the animal tree or of snails on the tree of mollusks," said Antonis Rokas, Cornelius Vanderbilt Chair in Biological Sciences at Vanderbilt University.</p>

<p>In a study published online May 8 by the journal Nature, Rokas and graduate student Leonidas Salichos analyze the reasons for these differences and propose a suite of novel techniques that can resolve the contradictions and provide greater accuracy in deciphering the deep branches of life's tree.</p>

<p>"The study by Salichos and Rokas comes at a critical time when scientists are grappling with how best to detect the signature of evolutionary history from a deluge of genetic data. These authors provide intriguing insights into our standard analytical toolbox, and suggest it may be time to abandon some of our most trusted tools when it comes to the analysis of big data sets.</p>

<p>This significant work will certainly challenge the community of evolutionary biologists to rethink how best to reconstruct phylogeny," said Michael F. Whiting, program director of systematics and biodiversity science at the National Science Foundation, which funded the study.</p>

<p>To gain insight into this paradox, Salichos assembled and analyzed more than 1,000 genes - approximately 20 percent of the entire yeast genome - from each of 23 yeast species. He quickly realized that the histories of the 1,000-plus genes were all slightly different from each other as well as different from the genealogy constructed from a simultaneous analysis of all the genes.</p>

<p>"I was quite surprised by this result," Salichos pointed out.</p>

<p>By adapting an algorithm from information theory, the researchers found that they could use these distinct gene genealogies to quantify the conflict and focus on those parts of the tree that are problematic.</p>

<p>In broad terms, Rokas and Salichos found that genetic data is less reliable during periods of rapid radiation, when new species were formed rapidly. A case in point is the Cambrian explosion, the sudden appearance about 540 million years ago of a remarkable diversity of animal species, without apparent predecessors. Before about 580 million years ago, most organisms were very simple, consisting of single cells occasionally organized into colonies.</p>

<p>"A lot of the debate on the differences in the trees has been between studies concerning the 'bushy' branches that took place in these 'radiations'," Rokas said.</p>

<p>The researchers also found that the further back in time they went the less reliable the genetic data becomes. "Radioactive dating methods are only accurate over a certain time span," said Rokas. "We think that the value of DNA data might have a similar limit, posing considerable challenges to existing algorithms to resolve radiations that took place in deep time."</p>

<p>###</p>

<p>The research was supported by National Science Foundation CAREER award DEB-0844968.</p>

<p>Visit Research News @ Vanderbilt for more research news from Vanderbilt. [Media Note: Vanderbilt has a 24/7 TV and radio studio with a dedicated fiber optic line and ISDN line. Use of the TV studio with Vanderbilt experts is free, except for reserving fiber time.] </p>]]>
    </content>
</entry>

<entry>
    <title>Astrobiology Daily News 14 May 2013</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/astrobiology-daily-news-14-may-2013.html" />
    <id>tag:astrobiology.com,2013://13.70979</id>

    <published>2013-05-15T02:37:37Z</published>
    <updated>2013-05-15T02:38:27Z</updated>

    <summary>- Characterizing Exoplanets in the Visible and Infrared: A Spectrometer Concept for the EChO Space Mission, astro-ph - Seed particle formation for silicate dust condensation by SiO nucleation, astro-ph - TAU: A 1D radiative transfer code for transmission spectroscopy of...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Daily Science News" scheme="http://www.sixapart.com/ns/types#category" />
    
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>- <a href="http://xxx.lanl.gov/abs/1305.3089">Characterizing Exoplanets in the Visible and Infrared: A Spectrometer Concept for the EChO Space Mission</a>, astro-ph<br />
- <a href="http://xxx.lanl.gov/abs/1305.2879">Seed particle formation for silicate dust condensation by SiO nucleation</a>, astro-ph<br />
- <a href="http://xxx.lanl.gov/abs/1305.2787">TAU: A 1D radiative transfer code for transmission spectroscopy of extrasolar planet atmospheres</a>, astro-ph</p>]]>
        <![CDATA[<p>- <a href="http://astrobiology.com/2013/05/celebrate-one-year-of-virtual-discovery-and-exploration-with-sagan.html">Celebrate One Year of Virtual Discovery and Exploration with S.A.G.A.N.</a><br />
- <a href="http://astrobiology.com/2013/05/key-to-cosmic-carbons-molecular-evolution.html">Key to Cosmic Carbon's Molecular Evolution</a>, NASA<br />
- <a href="http://astrobiology.com/2013/05/instrument-concepts-for-europa-exploration-1.html">Instrument Concepts for Europa Exploration</a>, NASA</p>]]>
    </content>
</entry>

<entry>
    <title>Celebrate One Year of Virtual Discovery and Exploration with S.A.G.A.N.</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/celebrate-one-year-of-virtual-discovery-and-exploration-with-sagan.html" />
    <id>tag:astrobiology.com,2013://13.70966</id>

    <published>2013-05-14T22:26:10Z</published>
    <updated>2013-05-14T22:27:04Z</updated>

    <summary>Are we alone in the universe? How did life begin? Will the human civilization expand out into the solar system and beyond? How can we act as curators of our home planet to achieve long-term sustainability? As astrobiologists we recognize...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Education and Outreach" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="astrobiology" label="astrobiology" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="carlsagan" label="Carl Sagan" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Are we alone in the universe? How did life begin? Will the human civilization expand out into the solar system and beyond? How can we act as curators of our home planet to achieve long-term sustainability? As astrobiologists we recognize these scientific and societal questions as some of the greatest of our time. </p>]]>
        <![CDATA[<p>These questions are powerful not only because they engage scientists but also inspire the wider public. Motivated by a vision of providing an easily accessible, inclusive online environment for scientists and the public to engage these big questions, the Social Action for a Grassroots Astrobiology Network (S.A.G.A.N.) was launched in April of 2012 at the Astrobiology Science Conference in Atlanta, GA. S.A.G.A.N. is a social network and collaborative web platform anyone can access by visiting www.saganet.org. </p>

<p>Celebrating our first year anniversary, S.A.G.A.N. has grown to a community of over 650 members from across the world, with backgrounds ranging from professional scientists, to science enthusiasts, students, educators, and journalists. </p>

<p>What is in it for you?</p>

<p>For professional scientists, S.A.G.A.N. provides an easily accessible platform for communication and collaboration, with freely available built-in video conferencing tools (found in our Breakout Rooms), document sharing, live text chat, and resources to start your own private or public groups. S.A.G.A.N. also provides a social platform for sharing Education and Public Outreach efforts and activities via blogs, lectures, or status updates, or even running outreach through the site! </p>

<p>For science enthusiasts and students, S.A.G.A.N. offers a fun and rich platform to ask questions, join special interest-groups, read about interesting and relevant astrobiology news, listen to podcasts, view seminars, interact with scientists, find like-minded individuals in regional settings, and find mentors. </p>

<p>For educators, S.A.G.A.N. offers opportunities to directly connect your classroom and students with "real life" scientists and stay up-to-date with the latest science news.</p>

<p>For administrators, S.A.G.A.N. offers a targeted audience to communicate science relevant opportunities, such as conferences, summer-schools, graduate student/post-doc/faculty opportunities, and other programs relevant to space exploration and astrobiology.</p>

<p>Events and Activities on S.A.G.A.N. are as follows (but not limited to!):</p>

<p>* Monthly "Talk to an Astrobiologist" live chat with a renowned astrobiologist (1st Tues of every month). Our upcoming guests include Dr. Chris McKay and Dr. David DesMarais! <br />
* Weekly seminars including live broadcasts of the Arizona State University Astrobiology Coffee Hour seminars and SETI Institute Public Lectures!<br />
* Book club, currently reading "Cosmos and Culture"<br />
* Weekly discussions on engaging questions in space exploration and astrobiology.<br />
* Opportunities to learn about international astrobiology activities and interact with astrobiology enthusiasts from all over the world! <br />
* Celebrate each month with a different theme: Mars enthusiasts out there, May is for you and filled with a variety of Mars themed events!</p>

<p>If you haven't logged in, and are interested in astrobiology, space exploration and related disciplines, or in the public communication of science check out S.A.G.A.N. and join in on the conversation at <a href="http://www.saganet.org">www.saganet.org</a>. </p>

<p>We look forward to your involvement!</p>

<p>Your S.A.G.A.N. Team <br />
Contact: admins@saganet.org<br />
Join us on Facebook: <a href="https://www.facebook.com/SaganCommunity">https://www.facebook.com/SaganCommunity</a> <br />
Follow us on Twitter: @saganorg</p>]]>
    </content>
</entry>

<entry>
    <title>Key to Cosmic Carbon&apos;s Molecular Evolution</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/key-to-cosmic-carbons-molecular-evolution.html" />
    <id>tag:astrobiology.com,2013://13.70965</id>

    <published>2013-05-14T22:14:07Z</published>
    <updated>2013-05-14T22:16:55Z</updated>

    <summary>Scientists at NASA&apos;s Ames Research Center now have the capability to systematically investigate the molecular evolution of cosmic carbon. For the first time, these scientists are able to automatically interpret previously unknown infrared emissions from space that come from surprisingly...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Astrochemistry" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="astrobiology" label="astrobiology" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="astrochemistry" label="astrochemistry" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="astronomy" label="astronomy" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="nasa" label="NASA" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Scientists at NASA's Ames Research Center now have the capability to systematically investigate the molecular evolution of cosmic carbon. For the first time, these scientists are able to automatically interpret previously unknown infrared emissions from space that come from surprisingly complex organic molecules, called polycyclic aromatic hydrocarbons (PAHs), which are abundant and important across the universe.</p>]]>
        <![CDATA[<p>Between 2003 and 2005, thanks to its unprecedented sensitivity, NASA's Spitzer Space Telescope, managed and operated by NASA's Jet Propulsion Laboratory, Pasadena, Calif., created maps of the tell-tale PAH signature across large regions of space, from hot regions of harsh ultraviolet (UV) radiation close to stars, to cold, dark clouds where stars and planets form. </p>

<p>By exclusively using their unique collection of authentic PAH spectra, coupled with algorithm-driven, blind-computational analyses, scientists at Ames were able to interpret the cosmic infrared maps with complex organic molecules. They found that PAHs changed significantly in size, electrical charge and structure, to adjust to the different environment at each spot in the map. Carbon is one of the most abundant atoms in space and scientists believe that the spectral changes across these maps trace the molecular evolution of carbon across the universe. </p>

<p>"At the time of our discovery, the 'signature,' or identifying spectrum, of this unexpected, but common infrared (IR) radiation from space hinted that PAHs might be responsible, but we were limited to a handful of small PAHs and very few were available to study," said Louis Allamandola, an astrophysics researcher at Ames. "To test the idea that PAHs were responsible, we measured and computed PAH spectra under astronomical conditions, creating the world's largest collection of PAH spectra. Today, our collection contains more than 700 PAH spectra."</p>

<p>Results will be published May 14 in "Properties of PAHs in the Northwest PDR of NGC 7023 1: PAH size, charge, composition and structure distribution," Astrophysical Journal, vol. 769 (2) article 117, 2013.</p>

<p>To determine the spectral changes across these maps, these astrophysicists used the PAH spectra collected in the PAH IR Spectroscopic Database (<a href="http://www.astrochem.org/pahdb/">http://www.astrochem.org/pahdb/</a>) at Ames. They analyzed the Spitzer infrared map of the Iris Nebula (NGC 7023) that hosts both the extreme environment of a region close to a star, as well as the more shielded, benign environment of a cold molecular cloud.</p>

<p>The new maps showed that small, electrically neutral, irregularly shaped PAHs are most common near the cold molecular cloud that is far from the star that excites PAH emission. However, when PAHs move closer to the exciting star and away from the cold cloud, they become large, symmetric and are electrically charged. "The large PAHs take over because they are more robust than the smaller, irregularly-shaped PAHs, which are destroyed by the unshielded star light," said Christiaan Boersma, an astrophysicist at Ames.</p>

<p>Finally, these large PAHs are themselves broken down, as they are stripped of hydrogen and become small fragments. At this point, the emission from the dehydrogenated PAHs takes over in the observed region. There were two findings that are especially important: the first is that positively-charged, nitrogen-containing PAHs are needed to complete the match between the correct spectral signature and the observed emission, and the second is that dehydrogenation and fragmentation occur close to the exciting star.</p>

<p>"The indication of nitrogen-containing PAHs (PANHs) is significant, as these have not been seriously considered previously. They represent an important class of prebiotic molecules, which are precursors to life," said Jesse Bregman, also an astrophysicist at Ames. "If borne out, this indicates complex, nitrogen-containing, aromatic molecules are present across the universe."</p>

<p>This approach of analyzing the aromatic infrared bands using the spectra of individual PAHs provides new, fundamental information about the UV-driven, spatial evolution of PAH subpopulations. It also ties these variations to changes in local conditions, such as those due to the physical shape and history of the region, radiation field, etc.</p>

<p>"Spitzer detected the PAH signature across the universe and showed PAHs were already forming only a couple of billion years after the Big Bang. Since PAHs are so sensitive to local conditions, analyzing the PAH bands, as we did here, represents a powerful new astronomical tool to trace the evolution of cosmic carbon and, at the same time, probe conditions across the universe," concluded Allamandola.</p>

<p>This work was supported by NASA's Carbon in the Galaxy Consortium under the auspices of the Astrophysics Research and Analysis Program (APRA).</p>

<p>For more information about the PAH IR Spectroscopic Database and available graphics, visit: <a href="http://www.astrochem.org/pahdb/">http://www.astrochem.org/pahdb/</a> </p>

<p>For more information about NASA, visit: <a href="http://www.nasa.gov">http://www.nasa.gov</a><br />
</p>]]>
    </content>
</entry>

<entry>
    <title>Instrument Concepts for Europa Exploration </title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/instrument-concepts-for-europa-exploration-1.html" />
    <id>tag:astrobiology.com,2013://13.70961</id>

    <published>2013-05-14T16:17:13Z</published>
    <updated>2013-05-14T16:19:33Z</updated>

    <summary>The Instrument Concepts for Europa Exploration (ICEE) Program supports the advanced development of spacecraft-based instruments for Europa exploration. The goal of the program is to mature and reduce the technical risk of instruments for a potential future Europa mission to...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Europa and Icy Moons" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Missions, Hardware, Software, &amp; Sensors" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="astrobiology" label="astrobiology" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="europa" label="Europa" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="nasa" label="NASA" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>The Instrument Concepts for Europa Exploration (ICEE) Program supports the advanced development of spacecraft-based instruments for Europa exploration. The goal of the program is to mature and reduce the technical risk of instruments for a potential future Europa mission to the point where they may be proposed in response to a future flight announcement of opportunity (AO) without additional extensive technology development. </p>]]>
        <![CDATA[<p>Note that the ICEE Program itself does not solicit instruments for a flight opportunity. This opportunity is open to any instrument addressing the six overarching goals for Europa exploration provided in the most recent Decadal Survey "Vision and Voyages for Planetary Science in the Decade 2013-2022." However, instruments must be compatible with a Europa flyby mission architecture. It is a priority for NASA to invest in development of all instruments in the strawman science payload, but selections may not be limited to those instruments.</p>

<p>This Amendment creates Appendix C.22. Notices of Intent are requested by May 13, 2013, and proposals are due June 10, 2013.</p>

<p>On April 19, 2013, this Amendment to the NASA Research Announcement "Research Opportunities in Space and Earth Sciences (ROSES) 2013" (NNH13ZDA001N) was posted on the NASA research opportunity homepage at <a href="http://nspires.nasaprs.com/">http://nspires.nasaprs.com/</a> and appeared on the RSS feed at: <a href="http://nasascience.nasa.gov/researchers/sara/grant-solicitations/roses-2013">http://nasascience.nasa.gov/researchers/sara/grant-solicitations/roses-2013</a></p>

<p>Questions concerning Appendix C.22, Instrument Concepts for Europa Exploration, may be directed to Curt S. Niebur, Planetary Science Division, Science Mission Directorate, NASA Headquarters, Washington, DC 20546-0001. Telephone: (202) 358-0390; E-mail: curt.niebur@nasa.gov.</p>]]>
    </content>
</entry>

<entry>
    <title>The Hadean Earth-Moon System - Workshop Without Walls</title>
    <link rel="alternate" type="text/html" href="http://astrobiology.com/2013/05/the-hadean-earth-moon-system---workshop-without-walls.html" />
    <id>tag:astrobiology.com,2013://13.70958</id>

    <published>2013-05-14T04:11:22Z</published>
    <updated>2013-05-14T04:12:44Z</updated>

    <summary>Please join us for the NAI Early Earth Focus Group Workshop Without Walls on &quot;The Hadean Earth-Moon System&quot;. The workshop is aimed at providing the most up-to-date science on the first billion years&apos; history of the Earth-Moon system, from solar...</summary>
    <author>
        <name>Keith Cowing</name>
        <uri>https://mt.spaceref.net/mt4/mt/mt-cp.cgi?__mode=view&amp;blog_id=13&amp;id=2</uri>
    </author>
    
        <category term="Geobiology" scheme="http://www.sixapart.com/ns/types#category" />
    
        <category term="Global Climate &amp; Habitability" scheme="http://www.sixapart.com/ns/types#category" />
    
    <category term="astrobiology" label="astrobiology" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="earth" label="Earth" scheme="http://www.sixapart.com/ns/types#tag" />
    <category term="moon" label="Moon" scheme="http://www.sixapart.com/ns/types#tag" />
    
    <content type="html" xml:lang="en" xml:base="http://astrobiology.com/">
        <![CDATA[<p>Please join us for the NAI Early Earth Focus Group Workshop Without Walls on "The Hadean Earth-Moon System". The workshop is aimed at providing the most up-to-date science on the first billion years' history of the Earth-Moon system, from solar system formation at 4.567 Ga to the widespread preservation of crustal rocks at 3.5 Ga to evidence for life preserved within those rocks. </p>]]>
        <![CDATA[<p>Themes to be presented/discussed include:</p>

<p>* Solar system accretion<br />
* Moon-forming giant impact<br />
* Late heavy bombardment<br />
* Formation and preservation of early crust: A cool early Earth?<br />
* Formation and capture of the hydrosphere<br />
* A reducing/anoxic/oxic atmosphere?<br />
* Habitats of Earth's earliest life<br />
* Early microbial metabolisms, including photosynthesis</p>

<p>This virtual workshop will consist of presentations and discussion periods held over a period of 4 hours each day for two consecutive days, facilitated through an online multi-user video-conferencing system using Adobe Connect to be hosted by the technical facilities of the NAI. The meeting will start at 19:00 UTC on both May 20 and May 21.</p>

<p>To view the agenda and for information on how to join online visit this <a href="https://astrobiology.nasa.gov/seminars/featured-seminar-channels/conferences-and-workshops/2013/05/20/nai-workshop-without-walls-on-hadean-earth-moon-system/">link</a></p>]]>
    </content>
</entry>

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