Mostrando entradas con la etiqueta Vida. Mostrar todas las entradas
Mostrando entradas con la etiqueta Vida. Mostrar todas las entradas

domingo, 2 de noviembre de 2014

Bolivia passes "Law of Mother Earth" which gives rights to our planet as a living system



The Law of Mother Earth ("Ley de Derechos de La Madre Tierra") holds the land as sacred and holds it as a living system with rights to be protected from exploitation, and creates 11 distinguished rights for the environment. It was passed by Bolivia's Plurinational Legislative Assembly. This 10 article law is derived from the first part of a longer draft bill, drafted and released by the Pact of Unity by November 2010. Can we please spread this law? There has to be a way for the free market to interoperate with reverence for this planet. Period.

In accordance with the philosophy of Pachamama, it states, "She is sacred, fertile and the source of life that feeds and cares for all living beings in her womb. She is in permanent balance, harmony and communication with the cosmos. She is comprised of all ecosystems and living beings, and their self-organisation."

"It makes world history. Earth is the mother of all," said Vice-President Alvaro García Linera. "It establishes a new relationship between man and nature, the harmony of which must be preserved as a guarantee of its regeneration."

The law enumerates seven specific rights to which Mother Earth and her constituent life systems, including human communities, are entitled to:

  1. To life: It is the right to the maintenance of the integrity of life systems and natural processes which sustain them, as well as the capacities and conditions for their renewal
  2. To the Diversity of Life: It is the right to the preservation of the differentiation and variety of the beings that comprise Mother Earth, without being genetically altered, nor artificially modified in their structure, in such a manner that threatens their existence, functioning and future potential
  3. To water: It is the right of the preservation of the quality and composition of water to sustain life systems and their protection with regards to contamination, for renewal of the life of Mother Earth and all its components
  4. To clean air: It is the right of the preservation of the quality and composition of air to sustain life systems and their protection with regards to contamination, for renewal of the life of Mother Earth and all its components
  5. To equilibrium: It is the right to maintenance or restoration of the inter-relation, interdependence, ability to complement and functionality of the components of Mother Earth, in a balanced manner for the continuation of its cycles and the renewal of its vital processes
  6. To restoration: It is the right to the effective and opportune restoration of life systems affected by direct or indirect human activities
  7. To live free of contamination: It is the right for preservation of Mother Earth and any of its components with regards to toxic and radioactive waste generated by human activities

Sources:

ORIGINAL: Minds
October 19, 2014

sábado, 15 de marzo de 2014

RNA World 2.0

Most scientists believe that ribonucleic acid played a key role in the origin of life on Earth, but the versatile molecule isn’t the whole story.

© KEVIN HAND
The ubiquity and diverse functionality of ribonucleic acid (RNA) in today’s world suggest that the information polymer could well have been the leading player early on in the establishment of life on Earth, and, in theory, it’s a logical basis for primitive life. One can readily imagine that RNA, as a catalytic molecule capable of serving as a template for its own replication, might have reproduced itself and grown exponentially in the primordial environment. Perhaps such an RNA-based proto–life-form even replicated with an appropriate level of fidelity to allow natural selection to begin directing its evolution.

But there’s a snag: “The odds of suddenly having a self-replicating RNA pop out of a prebiotic soup are vanishingly low,” says evolutionary biochemist Niles Lehman of Portland State University in Oregon.

For decades, researchers from diverse fields have theorized—and argued—about how early life might have begun, and about what sparked the 3.5 billion years of evolution that led to the plethora of cell-based life that occupies almost every nook and cranny of modern Earth. Different camps emerged. So-called “metabolism first” researchers focus on understanding chemical cycles that may have materialized in a prebiotic environment and could have led to the synthesis of nucleotides and other organic molecules. Those subscribing to the theory of “genetics first” want to identify the first information molecule and understand how it arose, replicated, and evolved.

The RNA world, first posited by Francis Crick1 and others in the late 1960s, remains an attractive hypothesis. Many of the chemical hurdles that once challenged the laboratory synthesis of the molecule under presumed primordial conditions are being overcome, and in vitro evolution experiments are yielding RNA molecules that perform numerous functions, including copying themselves or other RNAs. “I don’t think there can be much doubt that RNA was a major central player as both a catalyst and an early replicator,” says Nick Lane, a biochemist at the University College London whose research falls under the “metabolism first” label. “So the RNA world is absolutely correct, as far as I’m concerned, in that.”

But the notion that RNA, on its own, spontaneously assembled and evolved on early Earth has fallen out of favor. More likely, whatever conditions spawned compounds as complex as nucleotides also generated other organics, perhaps early forms of modern amino acids and fatty acids, the constituent parts of proteins and membranes. “I’m not sure how many people anymore believe in a pure RNA world. I certainly don’t,” says Lane. “I think the field has drifted away from that, and there’s now an acknowledgment it had to be ‘dirty.’ ”

“I think most people would argue that there’s . . . more than just RNA,” agrees Matthew Powner, a “genetics first” origins-of-life researcher, also at University College London. (See “Matthew Powner: Origin Solver,” The Scientist, March 2014) “People have relaxed their opinions of the RNA world . . . from its original inception where RNA was fundamental to all parts of biology in the earliest form of life.”

martes, 25 de febrero de 2014

Celebrate this week for Life’s Birthday!

Life has an incredible amount to teach us about living sustainably, in no small part due to the fact that organisms have been surviving and thriving on Earth for 3.85 billion years. But, how long is that really? If we take the age of Earth (4.5 billion years) and compress it into one year, we can better grasp the time-tested wisdom our fellow planet-mates can bring to the design table. And referencing this compressed calendar (see below), February 25, is life’s birthday!

To celebrate, for this week only we are offering a 38% discount on the following biomimicry resources:

Biomimicry Resource Handbook: A Seed Bank of Best Practices
Reg. $69.00 now for only $42.00. Promo code: BookBDay2014

Introduction to Biomimicry Online Foundational Course
Reg. $99.00, now for only $62.00. Promo code: CourseBDay2014

In addition, 38% of the proceeds will go directly to the Biomimicry 3.8 Institute to provide biomimicry education tools to students, educators, and practitioners around the world.

This birthday party ends on Friday, February 28 at 11:59 p.m. MST, so take advantage of the special now. To get your 38% discount, please follow these steps:

Click “Enroll” to sign up for a new account or log in



In the shopping cart enter the promo code(s)
Click “Checkout” to complete the process


Earth’s Calendar




ORIGINAL: Biomimicry.net

domingo, 9 de junio de 2013

Life & The Universe Most Astounding Fact - Neil deGrasse Tyson

ORIGINAL: YouTube
Jan 8, 2013

Astrophysicist Dr. Neil DeGrasse Tyson was asked by a reader of TIME magazine, "What is the most astounding fact you can share with us about the Universe?" This is his answer.

www.facebook.com/EducateInspireChange

Special thanks to:
Reid Gower http://saganseries.com/
Carl Sagan http://www.hulu.com/cosmos
Neil deGrasse Tyson http://www.facebook.com/neiltyson
NASA http://www.nasa.gov/
...for their inspiration.

CREDITS
Narration: TIME Magazine's "10 Questions for Neil Degrasse Tyson"
http://www.youtube.com/watch?v=wiOwqD...
Music: "To Build a Home" by the Cinematic Orchestra feat. Patrick Watson
http://www.cinematicorchestra.com/

Video (in order of appearance):
IMAX: Hubble 3D (Orion)
http://www.imax.com/hubble/
Yellowstone: Battle for Life (Tree & Waterfall)
http://www.bbc.co.uk/programmes/b00jcdml
Supernova to Crab Nebula
http://www.spacetelescope.org/videos/...
BBC: Wonders of the Solar System (formation of the solar system)
http://www.bbc.co.uk/programmes/b00qyxfb
Accretion and First Eukaryotes from the 2011 film "Tree of Life" directed by Terrence Malick
http://en.wikipedia.org/wiki/Accretio...)
http://en.wikipedia.org/wiki/Origin_o...
http://en.wikipedia.org/wiki/Timeline...
http://www.wired.com/wiredscience/200...
http://www.twowaysthroughlife.com/
BBC: Charles Darwin and the Tree of Life
http://www.wellcometreeoflife.org/
"Salar de Uyuni, Bolivia" by Ayrton Orio (Model: Xharon Kendelker)
http://vimeo.com/9505354
"Afghanistan - touch down in flight" by Augustin Pictures
http://vimeo.com/31426899
http://lukasugustin.de
"mongolia!" by wiissa
http://vimeo.com/27876709
http://wiissa.com

Excerpt from "Outside In", Copyright Stephen van Vuuren/SV2 Studios (Saturn's moon Mimas)
http://www.outsideinthemovie.com
IMAX: Hubble 3D (Inside Orion Nebula)
http://en.wikipedia.org/wiki/Orion_Ne...
Shuttle Launch from 1985 IMAX film "The Dream is Alive"
http://en.wikipedia.org/wiki/The_Drea...
"Earth -- Time Lapse View from Space, Fly Over -- NASA, ISS" by Michael Konig
http://www.youtube.com/watch?v=ls9yJT...
http://koenigm.com
Excerpt from "The Island" - La Palma Time Lapse Video by Christoph Malin
http://vimeo.com/27539860
http://christophmalin.com
Galaxy Map and Galaxy Formation by NCSA's Advanced Visualization Lab
http://avl.ncsa.illinois.edu/
"Mars sunset" captured by NASA's Mars Exploration Rover Spirit http://www.nasa.gov/multimedia/imageg...

Edited by Max Schlickenmeyer

Neil goes on to say "For me, that is the most profound revelation of 20th century astrophysics and I look forward to what the 21st century will bring us, given the frontiers that are now unfolding."

Copyright Disclaimer Under Section 107 of the Copyright Act 1976, allowance is made for "fair use" for purposes such as criticism, comment, news reporting, teaching, scholarship, and research. Fair use is a use permitted by copyright statute that might otherwise be infringing. Non-profit, educational or personal use tips the balance in favor of fair use. All copyrighted materials contained herein belong to their respective copyright holders, I do not claim ownership over any of these materials. I realize no profit, monetary or otherwise, from the exhibition of these videos.

sábado, 20 de abril de 2013

3 new planets could host life

ORIGINAL: CNN
By Elizabeth Landau, CNN
April 18, 2013 -- Updated 2000 GMT (0400 HKT) 

This diagram lines up planets recently discovered by Kepler in terms of their sizes, compared to Earth. Kepler-22b was announced in December 2011; the three Super-Earths were announced April 18, 2013. All of them could potentially host life, but we do not yet know anything definitive about their compositions or atmosphere

Where life might live beyond Earth 

STORY HIGHLIGHTS

Scientists discovered 3 planets in the "habitable zone" of their host stars 

They are all more than 1,000 light-years away 

The Kepler satellite is looking at more than 150,000 stars for possible planets orbiting them 

(CNN) -- In the midst of chaos here on Earth, scientists are finding hope for life on other planets. 

Scientists announced Thursday the discovery of three planets that are some of the best candidates so far for habitable worlds outside our own solar system -- and they're very far away. 

NASA's Kepler satellite, which is keeping an eye on more than 150,000 stars in hopes of identifying Earth-like planets, found the trio. 

Two of the planets -- Kepler-62e and Kepler-62f -- are described in a study released Thursday in the journal, Science. They are part of a five-planet system in which the candidates for life are the farthest from the host star. 

The host star -- the equivalent of Earth's sun -- takes the name Kepler-62, where the individual planets are designated by letters thereafter. 

The third planet that's potentially habitable, but not included in the Science study, is called Kepler-69c. Liquid water could theoretically exist on the surfaces of any of them, researchers said. They are the smallest planets ever found in the "habitable zone," the area near a star in which a planet can theoretically hold liquid water. 

"With all of these discoveries we're finding, Earth is looking less and less like a special place and more like there's Earth-like things everywhere," said Tom Barclay, Kepler scientist at the Bay Area Environmental Research Institute in Sonoma, California. 

You won't be swimming on the planets anytime soon, though. The Kepler-62 star is 1,200 light-years away; Kepler-69 is 2,700 light-years away. A light-year, the distance that light travels in a vacuum in one year, is nearly 6 trillion miles. 

What are these planets like? 
The smaller a planet is, the more likely it's rocky and the less likely it's made of gas, said William Borucki, Kepler science principal investigator at NASA Ames Research Center

That makes Kepler-62f, thought to be 40% larger than Earth, potentially the most like our planet out of the new discoveries. It could be rocky, Borucki said, with polar caps, land mass and water as well. It goes around its star once every 267.3 days (Earth days, that is). 

If you were standing on Kepler-62f, the star in the sky would look bigger than our sun does, but "the illumination level would be like walking around on Earth on a cloudy day," Borucki said at a press briefing. "It drops by a factor of five." 

Kepler-62e appears to be 60% larger than our planet and a little closer to its host star; this one could be a "water world" of mostly deep oceans, he said. It circles its star in 122.4 days. 

"All these planets that we're finding are quite different than planets in our own solar system," Borucki said. 

Kepler-69c appears to orbit a star similar to Earth's sun, Barclay said. As it's estimated to be about 70% larger than Earth, it may also be a water world, with oceans thousands of kilometers deep. This planet is also exciting because it is the smallest scientists have found that orbits a sun-like star in the habitable zone. 

It's not likely to have a rocky surface, Barclay said. According to what little we know about it, Kepler-69c is probably significantly warmer than Earth and could be more like Venus. 

"Probably, if there is life, it would be very unlike what we see on our own world," Barclay said. 

If scientists' notions of a "habitable zone" were applied to our own solar system, both Earth and Mars would fit the bill. But Mars doesn't have enough gravity to hold onto an atmosphere that could heat it sufficiently, said Lisa Kaltenegger, research group leader at the Max Planck Institute for Astronomy in Heidelberg, Germany, in a press conference. 

Other worlds that may have life 
Borucki said the new planets are "by far" better candidates for life than any others we know about, but a handful of others also have been identified as potentially capable of hosting life. 

You may recall planet Kepler-22b, which was announced in December 2011 and also was hailed as a potential candidate for hosting life. That planet had a radius 2.4 times that of Earth and is 600 light-years away. 

Kepler-22b was thought to have a temperature similar to that of Earth, according to modeling by Borucki and colleagues. The planet's host star is dimmer and cooler than our sun, but the planet is also 15% closer than we are to the sun. 

There is also a planet called Gliese-581g, discovered in September 2010, which is thought to be even more like Earth than Kepler-22b in terms of its suitability for plants and animals. It's only 20 light-years from Earth -- a lot closer than the newly discovered planets, though there has been some controversy about its existence. 

In its solar system there is another planet, Gliese-581d, that is also of interest in the search for life, according to the Planetary Habitability Laboratory at the University of Puerto Rico at Arecibo. The group's catalog lists a few other candidates

However, just like the other planets, we haven't seen or tested the atmospheres of any of these planets, so whether they're habitable remains theoretical. 

Often, when you find an example of a kind of planet, you start seeing a lot of them, said Sara Seager, professor of planetary science at Massachusetts Institute of Technology. She used to be part of the Kepler team but is now independent. 

"Planets in the habitable zones of stars must be everywhere," she said. 

Seager called the discovery of the three planets "a huge milestone," but her excitement is tempered because potentially habitable planets have been announced in the past and there's currently no way to get more details, given how far away they are. 

"We'll possibly never know if these particular ones do have water oceans or signs of life," she said. 


Identifying planets, not atmospheres 
The goal of the Kepler mission wasn't to find alien lifeforms, however. The satellite is supposed to investigate Earth-sized planets around stars that resemble our sun. 

The Kepler telescope, launched in 2009, allows scientists to measure changes in brightness of individual stars over time; these dimming events signal that a planet is nearby. Scientists undertake sophisticated calculations to verify that such signals are planets and not passing rocks. 

The satellite finds planets that are very far away because it's surveying so many stars. Imagine, said Seager, that you are in Times Square and you want to see 150,000 people at once. You wouldn't be able to do it in such a way that you could see any details of the people; you'd have to get far enough away that that many people would fit into your field of view. 

In total, Kepler has found 122 confirmed planets and more than 2,700 planet candidates. A total of seven confirmed planets were announced Thursday -- the three in the habitable zone, and four others that are not. 

This isn't the only planet-finding technique. The Gliese-581 system was found with the Keck I Telescope in Hawaii, using what is called the radial velocity method. The telescope's spectrometer allows scientists to look for wobbles in the motion of a star, which happens in response to the gravity of nearby planets. 

It would take a different kind of mission to investigate the atmosphere of one of these distance planets to find out answers to the most-pressing questions. Is there carbon dioxide and water? Is there oxygen? 

"Future NASA missions are going to focus on more nearby stars that we can look at in much more detail," Barclay said. 

You can read more about the Kepler discoveries at the mission website.

miércoles, 13 de marzo de 2013

NASA Rover Finds Conditions Once Suited for Ancient Life on Mars

ORIGINAL: NASA
March 12, 2013

PASADENA, Calif. -- An analysis of a rock sample collected by NASA's Curiosity rover shows ancient Mars could have supported living microbes

Scientists identified sulfur, nitrogen, hydrogen, oxygen, phosphorus and carbon -- some of the key chemical ingredients for life -- in the powder Curiosity drilled out of a sedimentary rock near an ancient stream bed in Gale Crater on the Red Planet last month. 

"A fundamental question for this mission is whether Mars could have supported a habitable environment," said Michael Meyer, lead scientist for NASA's Mars Exploration Program at the agency's headquarters in Washington. "From what we know now, the answer is yes.

Clues to this habitable environment come from data returned by the rover's Sample Analysis at Mars (SAM) and Chemistry and Mineralogy (CheMin) instruments. The data indicate the Yellowknife Bay area the rover is exploring was the end of an ancient river system or an intermittently wet lake bed that could have provided chemical energy and other favorable conditions for microbes. The rock is made up of a fine-grained mudstone containing clay minerals, sulfate minerals and other chemicals. This ancient wet environment, unlike some others on Mars, was not harshly oxidizing, acidic or extremely salty. 

The patch of bedrock where Curiosity drilled for its first sample lies in an ancient network of stream channels descending from the rim of Gale Crater. The bedrock also is fine-grained mudstone and shows evidence of multiple periods of wet conditions, including nodules and veins. 

Curiosity's drill collected the sample at a site just a few hundred yards away from where the rover earlier found an ancient streambed in September 2012. 

"Clay minerals make up at least 20 percent of the composition of this sample," said David Blake, principal investigator for the CheMin instrument at NASA's Ames Research Center in Moffett Field, Calif. 

These clay minerals are a product of the reaction of relatively fresh water with igneous minerals, such as olivine, also present in the sediment. The reaction could have taken place within the sedimentary deposit, during transport of the sediment, or in the source region of the sediment. The presence of calcium sulfate along with the clay suggests the soil is neutral or mildly alkaline

Scientists were surprised to find a mixture of oxidized, less-oxidized, and even non-oxidized chemicals, providing an energy gradient of the sort many microbes on Earth exploit to live. This partial oxidation was first hinted at when the drill cuttings were revealed to be gray rather than red. 

"The range of chemical ingredients we have identified in the sample is impressive, and it suggests pairings such as sulfates and sulfides that indicate a possible chemical energy source for micro-organisms," said Paul Mahaffy, principal investigator of the SAM suite of instruments at NASA's Goddard Space Flight Center in Greenbelt, Md. 

An additional drilled sample will be used to help confirm these results for several of the trace gases analyzed by the SAM instrument. 

"We have characterized a very ancient, but strangely new 'gray Mars' where conditions once were favorable for life," said John Grotzinger, Mars Science Laboratory project scientist at the California Institute of Technology in Pasadena, Calif. "Curiosity is on a mission of discovery and exploration, and as a team we feel there are many more exciting discoveries ahead of us in the months and years to come.

Scientists plan to work with Curiosity in the "Yellowknife Bay" area for many more weeks before beginning a long drive to Gale Crater's central mound, Mount Sharp. Investigating the stack of layers exposed on Mount Sharp, where clay minerals and sulfate minerals have been identified from orbit, may add information about the duration and diversity of habitable conditions. 

NASA's Mars Science Laboratory Project has been using Curiosity to investigate whether an area within Mars' Gale Crater ever has offered an environment favorable for microbial life. Curiosity, carrying 10 science instruments, landed seven months ago to begin its two-year prime mission. NASA's Jet Propulsion Laboratory in Pasadena, Calif., manages the project for NASA's Science Mission Directorate in Washington. 

For more about the mission, visit: http://www.jpl.nasa.gov/msl , http://mars.jpl.nasa.gov/msl/ and http://www.nasa.gov/msl . You can follow the mission on Facebook and Twitter at: http://www.facebook.com/marscuriosity and http://www.twitter.com/marscuriosity

DC Agle 818-393-9011
Jet Propulsion Laboratory, Pasadena, Calif.
agle@jpl.nasa.gov 

Dwayne Brown 202-358-1726
NASA Headquarters, Washington
Dwayne.c.brown@nasa.gov




Two Different Aqueous Environments
This set of images compares rocks seen by NASA's Opportunity rover and Curiosity rover at two different parts of Mars. On the left is " Wopmay" rock, in Endurance Crater, Meridiani Planum, as studied by the Opportunity rover. 

First Curiosity Drilling Sample in the Scoop. This image from NASA's Curiosity rover shows the first sample of powdered rock extracted by the rover's drill. Image credit: NASA/JPL-Caltech/MSSS 

Minerals at 'Rocknest' and 'John Klein' 
This side-by-side comparison shows the X-ray diffraction patterns of two different samples collected from the Martian surface by NASA's Curiosity rover. These images, made from data obtained by Curiosity's Chemistry and Mineralogy instrument (CheMin), show the patterns obtained from a drift of windblown dust and sand called "Rocknest" and from a powdered rock sample drilled from the "John Klein" bedrock.

The presence of abundant clay minerals in the John Klein drill powder and the lack of abundant salt suggest a fresh water environment. The presence of calcium sulfates rather than magnesium or iron sulfates (as found at Meridiani Planum by NASA's Mars Exploration Rover Opportunity) suggests a neutral to mildly alkaline pH environment. The Rocknest sand shadow mineralogy suggests a dry, aeolian (wind-shaped) environment with low water activity. The John Klein mineralogy suggests a lacustrine (lakebed) environment with high water activity.

As seen on the left, the Rocknest data reveal abundant plagioclase feldspar, pyroxene and olivine minerals. The data also indicate reveal small amounts of magnetite and anhydrite. In addition, the Rocknest sample contains 25 to 35 percent amorphous, or non-crystalline, material.

X-ray diffraction analysis of the John Klein drill powder reveals abundant phyllosilicate (a class of clay minerals called smectites that form by the action of relatively pure and neutral pH water on source minerals), plagioclase feldspar, pyroxene, magnetite and olivine. Alternatively, the clay minerals could have been transported by water from sources higher up the sediment fan to form the John Klein mineral assemblage. The region of the pattern indicating the phyllosilicates is labeled in the annotated version of this image. The data also show minor amounts of anhydrite and bassanite. The John Klein sample also contains about 20 percent amorphous material.

NASA's Jet Propulsion Laboratory, a division of Caltech in Pasadena, manages the project for NASA's Science Mission Directorate, Washington, and built Curiosity and CheMin.



An Earth Analog to Mars' Yellowknife Bay. This set of images shows a modern terrestrial analog to the "Yellowknife Bay" area that NASA's Curiosity rover is exploring. At left is a sampling pit exposing clay-bearing lake sediments, deposited in a basaltic basin in southern Australia. Image Credit: NASA/JPL-Caltech/Ames 


Location of John Klein Drill Site 

Studying Habitability in Ancient Martian Environments
This set of images shows the results from the rock abrasion tool from NASA's Mars Exploration Rover Opportunity (left) and the drill from NASA's Curiosity rover (right). Note how the rock grindings from Opportunity are brownish red, indicating the presence of hematite, a strongly oxidized iron-bearing mineral. Such minerals are less supportive of habitability and also may degrade organic compounds. The diameter of the abraded circle is 1.8 inches (4.5 centimeters). The image was cropped from an image
taken on Sol 35 (the 35th Martian day of Opportunity's operations, or Feb. 28, 2004, on Earth) by Opportunity's panoramic camera at a target called "Guadalupe" inside Eagle Crater.

On the right is the hole produced by Curiosity during the first drilling into a rock on Mars to collect a sample from inside the rock. In this case, the rock produced gray tailings -- not red -- suggesting the presence of iron that is less oxidized. One possibility is magnetite, which was determined to be present by Curiosity's Chemistry and Mineralogy instrument. Magnetite has less oxygen than hematite and would be more compatible with habitability and the preservation of organics, all other factors being equal. These other factors would include the primary concentration of organics in the sedimentary environment, in addition to later exposure of rock to surface radiation. The diameter of the hole is 0.63 inch (1.6 centimeters), which is approximately 1/3 of that on the left-hand image. The image was cropped fromPIA16726. It was taken on Sol 182 (the 182d Martian day of Curiosity's operations, or Feb. 8, 2013, on Earth) by the Mars Hand Lens Imager on Curiosity's arm after that day's drilling at a target rock called "John Klein."

JPL manages the Mars Science Laboratory/Curiosity for NASA's Science Mission Directorate in Washington. The rover was designed, developed and assembled at JPL, a division of the California Institute of Technology in Pasadena.

For more about NASA's Curiosity mission, visit: http://www.jpl.nasa.gov/msl, http://www.nasa.gov/mars, andhttp://mars.jpl.nasa.gov/msl.

Major Gases Released from Drilled Samples of the 'John Klein' Rock
An analysis of a drilled rock sample from NASA's Curiosity rover shows the presence of water, carbon dioxide, oxygen, sulfur dioxide, and hydrogen sulfide released on heating. The results analyzing the high temperature water release are consistent with smectite clay minerals.

Curiosity's Sample Analysis at Mars (SAM) instrument suite conducted the analysis. The first step in the analysis of a portion of this drilled sample was to heat the sample in a quartz oven to 1,535 degrees Farenheit (835 degrees Celsius) and analyze the gases as they were released using SAM's quadrupole mass spectrometer (QMS). The signatures of more than five hundred mass values were sampled during the heating of this drilled sample and analyzed by the QMS. Five are shown in the graph. These traces are diagnostic of water, carbon dioxide, oxygen, and two forms of sulfur (sulfur dioxide, the oxidized form, and hydrogen sulfide, the reduced form) measured by the QMS.

The second step in the analysis was to send a portion of the gas released from the sample to the tunable laser spectrometer (TLS) to measure isotopes of carbon, oxygen and hydrogen, in both water and carbon dioxide. The ratio of deuterium (a heavy form of hydrogen) to the lighter, more abundant form of hydrogen was lower than the deuterium-to-hydrogen ratio measured by SAM in more loosely bound water in the sample from the "Rocknest" drift. The high deuterium-to-hydrogen ratio in water in the Mars atmosphere is a signature of the lighter hydrogen more rapidly escaping to space over geological time. Therefore, measuring the deuterium-to-hydrogen in water released from rocks is one tool that can be used to explore ancient reservoirs of water on Mars.

The third step in the analysis was to inject gas trapped during the heating process into SAM's third instrument, the gas chromatograph. Individual compounds separate out in time in a long capillary column in this instrument and are then introduced into the QMS. The gas chromatograph mass spectrometer is a prime tool in the SAM search for organic compounds.

The ratio of reduced species to oxidized species released by the SAM ovens is significantly higher in this drilled bedrock than in the previously scooped dust samples. These results indicate a significant amount of available chemical energy because oxidized and less oxidized versions of molecules are present. This result, combined with suitable aqueous conditions at this site in the distant past, made this a potentially habitable environment.

The SAM analysis was conducted on Sol 200 (the 200th Martian day of Curosity's operations, which was Feb. 27, 2013, on Earth).

JPL manages the Mars Science Laboratory/Curiosity for NASA's Science Mission Directorate in Washington. The rover was designed, developed and assembled at JPL, a division of the California Institute of Technology in Pasadena.

For more about NASA's Curiosity mission, visit: http://www.jpl.nasa.gov/msl, http://www.nasa.gov/mars, andhttp://mars.jpl.nasa.gov/msl.




Chlorinated Forms of Methane at 'John Klein' Site
NASA's Curiosity rover has detected the simple carbon-containing compounds chloro- and dichloromethane from the powdered rock sample extracted from the "John Klein" rock on Mars. These species were detected by the gas chromatograph mass spectrometer (GCMS) on Curiosity's Sample Analysis at Mars instrument (SAM).

The blue peak on the left shows the presence of chloromethane and the two red peaks on the right show the presence of dichloromethane. The powdered rock sample from John Klein was heated and some of the gas released was injected into the capillary column of the GCMS. The time at which different compounds exited the gas chromatograph column and entered the mass spectrometer, and the patterns produced in the mass spectrometer indicated molecular identity.

This chart also indicates "blank runs," which were conducted on Mars prior to delivery of this drilled sample to SAM. The runs helped to insure that signals from the gases released from the John Klein sample were above background levels. Curiosity began drilling at John Klein in February 2013. The SAM analysis was conducted on Sol 200 (the 200th Martian day of Curosity's operations, which was Feb. 27, 2013, on Earth).

Both chloro- and dichloromethane were also detected earlier by SAM at the "Rocknest" drift. It is possible that these simple carbon-containing compounds were produced by the reaction between Martian carbon and chlorine released when this sample was heated in the SAM oven. However, analysis of an additional drilled sample is required to help scientists understand if instead any residual terrestrial carbon from the drill, or perhaps chlorine left over from the Rocknest sample, is responsible for the generation of some or all of these compounds. In any case, these detections demonstrate clearly that the SAM GCMS is performing as designed and ready to continue the search for organic compounds in Gale Crater.

JPL manages the Mars Science Laboratory/Curiosity for NASA's Science Mission Directorate in Washington. The rover was designed, developed and assembled at JPL, a division of the California Institute of Technology in Pasadena.

For more about NASA's Curiosity mission, visit: http://www.jpl.nasa.gov/msl, http://www.nasa.gov/mars, andhttp://mars.jpl.nasa.gov/msl.

miércoles, 20 de febrero de 2013

‘Bioconcrete’ Uses Bacteria to Heal Itself

ORIGINAL: This Big City
20 February 2013


No product evokes a sense of solidity and sturdiness the way concrete does. However, the tiniest of cracks in an otherwise colossal slab will inevitably lead to structural degradation, leakages and costly repairs.

It is precisely this problem that two Dutch researchers from Delft Technical University have been working on. Beginning in 2006, Henk Jonkers, a microbiologist, and Eric Schlangen, a specialist in concrete development, sought to develop a self-healing cement [pictured] that would stop cracks from forming in the concrete, thereby extending the life of constructions.

Microcracks have a width of just 0.2-0.4mm, but that’s enough for water to leak in, degrading the concrete and the steel reinforcements embedded within it. Using the potentially damaging water to their advantage, Jonkers and Schlangen added a healing agent into the concrete, composed of bacterial spores and a feed.

Jonkers explains that the incoming water activates the bacterial spores, causing them to convert the feed into limestone, which seals the crack. Tunnels, basements and highway infrastructure are ideal ‘wet environments’ which will benefit from this innovation.

Rachel Armstrong, senior lecturer in the School of Architecture and Construction at the University of Greenwich, calls the project “a landmark in developing ‘living’ materials”.

However, “the production of calcite does not appear to me to actually increase the structural integrity of the concrete: [it] just stops the progression of the faults”, Armstrong added.

While this bacteria-infused cement is not alone in the world of self-healing concrete, Jonkers and Schlangen’s concrete has succeeded in healing cracks 10 times longer than other methods.

At present, the biggest challenge is producing large-scale quantities of the healing agent at affordable costs.

With the hope of long-term savings from the increased life expectancy of constructions, several companies and stakeholders have expressed interest in the product, including the Dutch ministry of road affairs.

The two researchers expect their concrete to enter the market in about four years.

You can watch Jonkers talk about bioconcrete in the video below:


This article originally appeared in Green Futures, the magazine of independent sustainability experts Forum for the Future. Image via astounde



miércoles, 13 de febrero de 2013

TEDxSF - Louie Schwartzberg - Gratitude

ORIGINAL: TEDxSF





Louie Schwartzberg is an award-winning cinematographer, director, and producer whose notable career spans more than three decades providing breathtaking imagery for feature films, television shows, documentaries and commercials.

This piece includes his short film on Gratitude and Happiness. Brother David Steindl-Rast's spoken words, Gary Malkin's musical compositions and Louie's cinematography make this a stunningly beautiful piece, reminding us of the precious gift of life, and the beauty all around us.

As a visual artist, Louie has created some of the most iconic and memorable film moments of our time. He is an innovator in the world of time-lapse, nature, aerial and "slice-of-life" photography - the only cinematographer in the world who has literally been shooting 24 hours a day, 7 days a week continuously for more than 30 years.

Louie was recognized as one of the top 70 Cinematographers for the On Film Kodak Salute Series. He is a member of the Directors Guild of America and the Academy of Motion Pictures Arts and Sciences.

Louie is credited by many with pioneering the contemporary stock footage industry by founding Energy Film Library, a global company with a network of 12 foreign offices, which was acquired by Getty Images in 1997. Motion picture clients of his cinematic artistry include Sex in the City, The Bourne Ultimatum, Die Hard 4, Syriana, Crash, Men in Black and classics such as American Beauty, Koyaanisqatsi and E.T. among others. 

Louie went on to found BlackLight Films, a creative production company specializing in producing original theatrical feature, large format films, HD and TV programming.

In 2004, BlackLight Films completed production of the theatrical feature film, America's Heart & Soul, distributed theatrically by Walt Disney Pictures. In 2006, BlackLight Films completed a series of HD shorts, Louie Films, for the launch of Buena Vista Home Entertainment's Blu-Ray DVD releases. In 2007, the company produced a 1-hour special, Chasing the Light, which aired nationally on PBS.

Past projects include the 35mm film Seasons of the Vine for Disney's California Adventure Theme Park and a 26-half hour series, America!, for The Hallmark Channel.

Louie has won two Clio Awards for Best Environmental Broadcast Spot, an Emmy nomination for Best Cinematography for the Discovery Channel Special, Oceans of Air, and the Heartland Film Festival's Truly Moving Picture Award for Walt Disney Pictures' feature film release America's Heart & Soul. 

Louie completed production on a feature length nature documentary, Wings of Life, to be theatrically released worldwide, under Walt Disney Pictures' new production banner, Disneynature. The film was released in France (March 2011) under the title Pollen and won the Roscar Award for Best Cinematography at the 2011 Wild Talk Africa Film Festival. 

Louie spoke at the TED 2011 conference in Long Beach, CA and has been a regular presenter at the annual Bioneers Conference in San Francisco. Currently, Louie is in production with National Geographic to produce Hidden Worlds, a 3D Imax film.

sábado, 2 de febrero de 2013

Life, the Universe, and Everything: An Interview with David Haussler

ORIGINAL: PLOS GENETICS
Jane Gitschier
January 31, 2013

David Haussler. Photograph by Ron Jones, courtesy of the Center for Biomolecular Science and Engineering, University of California Santa Cruz.doi:10.1371/journal.pgen.1003282.g001
Citation: Gitschier J (2013) Life, the Universe, and Everything: An Interview with David Haussler. PLoS Genet 9(1): e1003282. doi:10.1371/journal.pgen.1003282

Copyright: © 2013 Jane Gitschier. This is an open-access article distributed under the terms of the Creative Commons Attribution License, which permits unrestricted use, distribution, and reproduction in any medium, provided the original author and source are credited.


Among the pantheon of computer scientists who have framed our capacity to interpret DNA sequences stands David Haussler of the University of California, Santa Cruz (UCSC). Applying his prowess in computer learning theory to the problems of protein modeling and gene structure prediction, Haussler emerged in the mid-1990s as a trail-blazer in the field of computational biology. He came to wider prominence in 2000 during the frenetic race to produce a draft sequence of the human genome by nucleating an impassioned team of coders and engineers who assembled the sequence data and launched the UCSC Genome Browser. Fittingly, his team's contribution made manifest the vision of Robert Sinsheimer, who as Chancellor of UCSC in 1985 convened a pivotal workshop to explore sequencing the human genome.

Haussler (Image 1) now plays, by my count, at least half-a-dozen leadership roles, including co-director of the Genome 10 K project, coordinating committee member of The Cancer Genome Atlas project, and director of the Center for Biomolecular Science and Engineering at UCSC. He is easily spotted by his predilection for Hawaiian shirts, whose informality, he suggests, fosters inter-disciplinary collaboration. Indeed, Haussler's ken for machine learning and his quest for the meaning of life are so expansive that I was tempted to title this piece “Deep Thought”, a nod to the fictional computer in Douglas Adams' The Hitchhiker's Guide to the Galaxy, but chose a more subdued allusion instead.

I located Haussler on the upper reaches of the stunning UCSC campus in the engineering building, a sleek structure of glass and aluminum, tucked into a redwood grove that was still dripping and fragrant from the morning's rain. The anteroom to his modest office was decorated with handsome prints from UCSC's scientific illustration program as well as books on the genome project, and a box labeled “for the intron lounge” was piled high with journals. Haussler swept in via bicycle, swiftly signed a few documents, and downed a cold drink as we began with a discussion of his growing up in the town of North Hills in the San Fernando Valley.

Haussler: My dad went to Caltech and because of the economic pressures of having a young family, decided not to pursue pure science, but to pursue a professional position in structural engineering. He worked on mathematical problems as a hobbyist and had a love of pure science. Both my brother and I ended up living out his dream to be a scientist. My brother is a highly accomplished biochemist.

Gitschier: I saw that your first paper in the early '70s was with a Haussler and had assumed it was your father, but then, looking at his picture, I realized he must be your sibling.

Haussler: My only sibling is my brother. He was professor of biochemistry in University of Arizona and taught me how to do science. And he is really one of the leading scientists in the world on vitamin D, which was the subject of that first paper.

Gitschier: How much older is he?

Haussler: Twelve years.

Gitschier: So he was established when you were just a kid.

Haussler: Right. The summer after my freshman year [in college], I spent time in his lab. Every third week, I would sacrifice a chick that was raised without vitamin D. I would take out its intestines for receptors for the hormonal form of vitamin D, and we used those receptors in a radio-receptor competitive binding assay to first measure the level of the hormonal form of vitamin D in the human bloodstream, in both normal and diseased humans. By the end of the summer, we had a paper in Science! You know, big breakthrough.

Then I went back the next summer, and nothing worked. I remember my brother saying to me, “Now, this is how science really is.” But I was undaunted.

Gitschier: Let's talk about your transition to science, because I know your first college experience was in art.

Haussler: I did visual art mostly. Acrylic painting and metal sculpture were probably my favorites, although I did stone lithography and all kinds of fabulous things in the San Francisco Academy of Art. Then, I switched schools and into psychology.

Gitschier: And that was where?

Haussler: That was actually at a crazy little experimental college. You have to understand that this was the early '70s…

Gitschier: I do understand! [Haussler and I were born the same year.]

Haussler: My mother was hoping I'd go to UCLA, but I was a rebel and said “No, I want to go to a crazy place,Immaculate Heart College [IHC] in Hollywood.

Gitschier: Immaculate Heart doesn't sound so “crazy” on the surface.

Haussler: It doesn't, not at all, but the thought leader there was Sister Corita Kent, and you remember from the '60s, those love posters? A lot of the art movement and the philosophy that was expressed in art and posters in that era actually came out of Sister Corita Kent and a number of other rebels. The sisters at IHC were essentially kicked out of the Catholic Church for being radicals, and they had an extremely experimental college. So I, being the contrarian I was, applied there. It was strong in art and music and psychology. We studied Fritz Perls and Carl Rogers and all of these self-realization psychology thinkers at the time. And I was extremely into that. We had intensive encounter groups and dug very deeply into personal interactions.

Gitschier: But you didn't stick with Immaculate Heart.

Haussler: I got interested in science by working with my brother. I then transferred to Connecticut College back east. Again, I liked very intimate, individual learning. This was part of my whole psychology background. I view essential human progress being made, including learning, within a very intensive, one-on-one or small group interaction.

Gitschier: When you went there, you knew you wanted to do math?

Haussler: Yes. During those two summers with my brother, the one thing that mattered most was not the wet lab experiments that I had done, but when it came to analyzing the data. Someone in the lab was showing concentration in relation to a radioactive response curve and trying to fit that data with a linear function. And I said, “Well you can't use linear regression on this until you transform the variables.” And they looked at me and said, “Can you do that?”

And then I realized, hey wait a minute, I can contribute on the math side and it's a lot more fun than grinding up chicken guts! I like the quote that “mathematics is the queen of sciences” [attributed to Gauss]. Mathematics is the beautiful unity in the universe, and that's what totally captivated me.

Gitschier: Then, you find yourself at the University of Colorado doing PhD work in computer science. That seems like a logical transition to me.

Haussler: Logical is the correct word. After studying pure mathematics as an undergrad, I decided that the foundation for everything was logic. And I read extensively before I went to graduate school, but even after getting my undergraduate degree in mathematics and a minor in physics, I still hadn't decided to pursue a life of science.

Gitschier: What were you thinking of—art, philosophy, psychology?

Haussler: I wanted to get at the heart of the meaning of life.

Gitschier: Wow. [I had to swallow the answer, “42”.]

Haussler: Still this rebel spirit, I guess. I wasn't convinced that I would find that at traditional institutions. I spent about nine months wandering around Europe and then settled in San Luis Obispo on the family farm, kind of between generations. My grandfather was aging and my father was active as an engineer, so there was no one to take care of it.

While I was there, I wanted to keep touch with my intellectual side, so my friends and I—it was almost like a commune—believed in working hard on the ranch during the day and then reading and discussing philosophy, history, literature, and psychology at night.

Gitschier: Who were these people that you recruited to the farm?

Haussler: Well, important people that I met in my life and in my travels. We read books and had wonderful discussions. I remember my favorite title was The Origin of Consciousness in the Breakdown of the Bicameral Mind. We were trying to build a non-traditional intellectual environment.

But size is a factor there. What was missing at that time was the Internet. There was no way to get in touch with other people who had very specific interests except through the library and through post. So it became a 19th century gentleman-scholar kind of activity, which has very limited impact.

Gitschier: What happened to the farm after you left?

Haussler: My father did retire there. He and my mother had a spectacular retirement, raising organic fruit and selling it at the farmers market. So I played an important role in the family; I was the bridge to that retirement and it allowed me close friendship and think time.

Gitschier: And what firm had your father worked for?

Haussler: Oh, in my family, we never worked for anybody else! Robert Haussler Structural Engineering!

Gitschier: I see. It was a tradition!

Haussler: My great grandfather, my grandfather, my father always ran their own businesses. Never had a boss. It was a crazy, fierce, independent kind of tradition.

Gitschier: So this was instilled in you very early. I'm now seeing the fuller context!

Haussler: Right. I wasn't going to play along with any institutional programs! Those were the days when you could be anti every institution and get away with it.

Well, I look back at my writings from that time and there was some very creative stuff but isolated from the bulk of the intellectual mainstream, it's very hard to make progress. So I was thrilled to get re-engaged, just by taking advanced math classes at Cal Poly [San Luis Obispo].

Applied mathematics was my major, but I took computer science classes as well. I seized on the question of what is computable. What can be formalized by mathematics? And the answer, according to Alan Turing, was that this is the same as what can be computed on a very simple kind of machine. I was tremendously taken by that and by the fact that Turing and Kurt Gödel had established that there were things that were fundamentally uncomputable; true but unprovable. It appealed to my mystical side. I was always interested in the unity of the universe and the mystery of it.

Gitschier: Are you still?

Haussler: I still am in many ways. The mystery of “why life” and “is there a mathematical inevitability that there will be life” are questions that I spend quite a bit of time thinking about. I don't write much about them because I'm engaged in areas that are more immediately applied and have urgent impact, but I think a lot about them.

And there's a theme in my thinking and in my life that has been constant since those days as a young adult searching for answers. I turned away from thinking about that as a humanistic quest—to understand my psychology and our interactions—into an absolute quest for knowledge about the universe. In a sense that is the one thread that unites my entire adult life because I've been in so many different scientific areas.

But life itself has always been something that fascinated me, life in the broadest sense, that spans everything from the actual biological life that we observe on this planet, to the abstract notion of life. Like in Conway's Game of Life where you have a disarmingly simple mathematical system that nevertheless is sufficiently complex that it is naturally an incubator of self-reproducing patterns; you start with a random pattern, and you will have emergent forms that will be self-replicating entities that interact, as in living systems.