NCBI ROFL: “Back and forth forever” (or, DIY poop therapy). | Discoblog

3155783018_fdaf220ca1Success of self-administered home fecal transplantation for chronic Clostridium difficile infection.

“Clostridium difficile infection (CDI) can relapse in patients with significant comorbidities. A subset of these patients becomes dependent on oral vancomycin therapy for prolonged periods with only temporary clinical improvement. These patients incur significant morbidity from recurrent diarrhea and financial costs from chronic antibiotic therapy. We sought to investigate whether self- or family-administered fecal transplantation could be used to definitively treat refractory CDI. We report a case series (n=7) where 100% clinical success was achieved in treating these individuals with up to 14 months follow up.”

poop_back_and_forth

Thanks to Caryn for today’s ROFL!
Photo: flickr/?Debs?

And in case you didn’t get our title reference:

Related content:
Discoblog: NCBI ROFL: One rat, one cup.
Discoblog: NCBI ROFL: Rectal impaction following enema with concrete mix.
Discoblog: NCBI ROFL: Rectal oven mitt.


Should Policy Try to Reduce Foreclosures?

In 2006, Benjamin Koellmann bought a condominium in Miami Beach. By his calculation, it will be about the year 2025 before he can sell his modest home for what he paid. Or maybe 2040.

“People like me are beginning to feel like suckers,” Mr. Koellmann said. “Why not let it go in default and rent a better place for less?”

After three years of plunging real estate values, after the bailouts of the bankers and the revival of their million-dollar bonuses, after the Obama administration’s loan modification plan raised the expectations of many but satisfied only a few, a large group of distressed homeowners is wondering the same thing. ...

In a situation without precedent in the modern era, millions of Americans are in this bleak position. Whether, or how, to help them is one of the biggest questions the Obama administration confronts as it seeks a housing policy that would contribute to the economic recovery.

In my mind the crucial question is whether to help distressed homeowners, and the right answer is no:

1. these homeowners assumed the risk of buying houses; they should accept the consequences;

2. homeowners who default will acquire a bad credit rating, but they will be free of their debt burden.  Instead of putting money into an asset they may never actually own, they can start to accumulate savings.

2. foreclosing on these homeowners does not mean homeownerhip will decline; it means the houses will become available at low prices to others with limited income.  What's wrong with that?

ARIZONA: Jesse Kelly for US Congress; inspired by the Boston Tea Party, Scott Brown

SPECIAL GUEST EDITORIAL

The Conservative Revolution of 2010
by Jesse Kelly

“This morning the British army in Boston…disgracefully quitted all their strongholds in Boston and Charlestown, fled from before the army of the United Colonies, and took refuge on board their ships…The joy of our friends in Boston, on seeing the victorious and gallant troops of their country enter the town almost at the heels of their barbarous oppressors, was inexpressibly great.” - - As reported by an American newspaperman after the first Washington-led, American victory in Boston, 1776.

Just think about what conservatives have accomplished in 2010. Not in my wildest dreams could I have thought that a fiscally conservative candidate could be Massachusetts’ newest senator. Like General Washington’s victory at Dorchester Heights, the war for the future of liberty in America won its first great battle in the Bay State.

Like many of you, I saw the storm clouds gathering for over a year. The previous administration began an attack on our constitution and our free market system through big government conservatism. President Obama continued the assault on our liberties by putting big government into overdrive. Obama, Pelosi, Reid and Giffords all supported nationalizing our industries, taking over our healthcare and strangling us with environmental regulation. The free citizens of Southern Arizona and these United States are saying, “NO MORE!”

Pundits on every cable news channel are likening this year to 1994; however, they are missing the fundamental difference between that year and this: 1994 was a Republican revolution, 2010 is a CONSERVATIVE REVOLUTION.

No sitting congressman or senator is safe this year. Not Harry Reid, not my opponent, Gabrielle Giffords, not John Murtha, not John McCain. Both Republican and Democratic voters are shouting, “This is not about political teams, team elephant or team donkey! This is about limited government, fiscal sanity and free market solutions to our nation’s problems!” It is fundamentally important for incumbents and challengers alike to realize the following fact: if Republicans are conservatives, they will win. If Republicans are merely tax cutters, but have a record of out-of-control spending, they will lose. If Democrats are conservative, they will win. If Democrats vote with Pelosi, they will lose.

The greatness of the conservative revolution of 2010 lies in its ability to act as a driving force for America far longer than its Republican counterpart 15 years prior. The Republican revolution of 1994 was successful in its onset, but failed to be a lasting movement because it was not wholly and completely rooted in conservatism. Identity without ideology is empty, and the longer the Republican Party occupied the seats of power in Congress, the easier it was for them to stagnate and whither from the vine.

In the conservative revolution of 2010, candidates like me see the Republican Party as an organized medium for my actual ideology, conservatism. Where some want to label Republicans as “the party of no,” conservatives will always be full of pragmatic, new ideas, rooted in the first principles of the Founders. While Republican values are malleable and ill-defined, conservative values are fixed, well reasoned, and applicable to everything from political theory to everyday living.

As a conservative and as republican, I announced my candidacy in early 2009 because I saw the revolution ahead of us could not only be victorious, but also glorious. In my race, in Arizona’s 8th congressional district, I am battling against a big government Republican in the primary and a big government Democrat in the general. It’s time to open up the western front in the conservative revolution of 2010.

Jesse Kelly is a candidate for Congress in Arizona’s Eighth District. His website is http://www.votejessekelly.com

Electostatic Charges in Gas Turbine Compressor

We have GE frame 9E gas turbine. Gas turbine have a carbon brush at Brg#4 i.e Generator DE. I want to know how the electrostatic charges developed in compressor are grounded. Is there any carbon brush near bearing no#1 or 2. Recently during inspection of the accessory gear box of a GT, half beari

NASA Extends Cassini’s Tour of Saturn, Continuing International Cooperation for World Class Science

Saturn equinox 2009
Of the countless equinoxes Saturn has seen since the birth of the solar system, this one, captured here in a mosaic of light and dark, is the first witnessed up close by an emissary from Earth ... none other than our faithful robotic explorer, Cassini. › Full image and caption
NASA will extend the international Cassini-Huygens mission to explore Saturn and its moons to 2017. The agency's fiscal year 2011 budget provides a $60 million per year extension for continued study of the ringed planet.

"This is a mission that never stops providing us surprising scientific results and showing us eye popping new vistas," said Jim Green, director of NASA's planetary science division at NASA Headquarters in Washington. "The historic traveler's stunning discoveries and images have revolutionized our knowledge of Saturn and its moons."

Cassini launched in October 1997 with the European Space Agency's Huygens probe. The spacecraft arrived at Saturn in 2004. The probe was equipped with six instruments to study Titan, Saturn's largest moon. Cassini's 12 instruments have returned a daily stream of data from Saturn's system for nearly six years. The project was scheduled to end in 2008, but the mission received a 27-month extension to Sept. 2010.

"The extension presents a unique opportunity to follow seasonal changes of an outer planet system all the way from its winter to its summer," said Bob Pappalardo, Cassini project scientist at NASA's Jet Propulsion Laboratory in Pasadena, Calif. "Some of Cassini's most exciting discoveries still lie ahead."

This second extension, called the Cassini Solstice Mission, enables scientists to study seasonal and other long-term weather changes on the planet and its moons. Cassini arrived just after Saturn's northern winter solstice, and this extension continues until a few months past northern summer solstice in May 2017. The northern summer solstice marks the beginning of summer in the northern hemisphere and winter in the southern hemisphere.

A complete seasonal period on Saturn has never been studied at this level of detail. The Solstice mission schedule calls for an additional 155 orbits around the planet, 54 flybys of Titan and 11 flybys of the icy moon Enceladus.

The mission extension also will allow scientists to continue observations of Saturn's rings and the magnetic bubble around the planet known as the magnetosphere. The spacecraft will make repeated dives between Saturn and its rings to obtain in depth knowledge of the gas giant. During these dives, the spacecraft will study the internal structure of Saturn, its magnetic fluctuations and ring mass.

The mission will be evaluated periodically to ensure the spacecraft has the ability to achieve new science objectives for the entire extension.

"The spacecraft is doing remarkably well, even as we endure the expected effects of age after logging 2.6 billion miles on its odometer," said Bob Mitchell, Cassini program manager at JPL. "This extension is important because there is so much still to be learned at Saturn. The planet is full of secrets, and it doesn't give them up easily."

Cassini's travel scrapbook includes more than 210,000 images; information gathered during more than 125 revolutions around Saturn; 67 flybys of Titan and eight close flybys of Enceladus. Cassini has revealed unexpected details in the planet's signature rings, and observations of Titan have given scientists a glimpse of what Earth might have been like before life evolved.

Scientists hope to learn answers to many questions that have developed during the course of the mission, including why Saturn seems to have an inconsistent rotation rate and how a probable subsurface ocean feeds the Enceladus' jets.

The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. JPL manages the project for NASA's Science Mission Directorate in Washington. The Cassini orbiter was designed, developed and assembled at JPL.

More Cassini information is available, at http://www.nasa.gov/cassini and http://saturn.jpl.nasa.gov.

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Liberal Universities in U.S. now training grounds for Islamic Terrorists?

Aafia Siddiqui convicted - Shouts blame it on Israel

From Eric Dondero:

A courtroom trial of a "Female Al Qaeda" Islamic Terrorist has highlighted a frightening new trend on at least some of the more liberal college campuses here in the United States.

From NewsMax:

NEW YORK – A U.S.-trained Pakistani scientist was convicted Wednesday of charges that she tried to kill Americans while detained in Afghanistan in 2008, shouting with raised arm as jurors left the courtroom: "This is a verdict coming from Israel, not America."

A jury deliberated three days in federal court in Manhattan before finding Aafia Siddiqui guilty in the third week of her attempted murder trial, which she often interrupted with rambling courtroom outbursts.

After declaring the verdict came from Israel, she turned toward spectators in the packed courtroom and said: "Your anger should be directed where it belongs. I can testify to this and I have proof."

Siddiqui was convicted of attempted murder, on two counts. At a police station in Afghanistan, she managed to get hold of a rifle and fire at 7 US soldiers, while shouting "Death to America!"

The prosecutors in the case described in detail her connections to Al Qaeda. When she was captured she had in her posession plans to blow up the Statue of Liberty and "other New York landmarks."

Most striking about her case, is that she is a graduate of both MIT and Brandeis University in Massachusetts.

MIT is the same university where American-born Islamic Terrorist Major Nidal Malik Hassan, the infamous Ft. Hood shooter, received his training.

Bill Warner, Private Investigator out of Sarasota, Florida, provides more details at his Blog:

Aafia Siddiqui Indicted for Attempting to Kill United States Nationals in Afghanistan and Six Additional Charges. ..On July 17, 2008, when Aafia Siddiqui was detained by Afghan authorities, a number of items were in her possession, including handwritten notes that referred to a “mass casualty attack” and that listed various locations in the United States, including Plum Island, the Empire State Building, the Statue of Liberty, Wall Street, and the Brooklyn Bridge. Other notes in Siddiqui’s possession referred to the construction of “dirty bombs,” and discussed various ways to attack “enemies,” including by destroying reconnaissance drones, using underwater bombs, and using gliders.

Aafia Siddiqui also possessed a computer thumb drive that contained correspondence referring to specific “cells,” “attacks” by certain “cells,” and “enemies.”

Aafia Siddiqui, a 36-year-old Pakistani woman, resided in the United States from in or about 1991 until June 2002, and obtained degrees from the Massachusetts Institute of Technology and Brandeis University. Siddiqui returned to the United States on December 25, 2002, and departed on January 2, 2003...

Terrorist Majid Khan appears to have met with Aafia Saddiqui who is a MIT grad in microbiology, she had access to Anthrax while working at Brandeis Univ in Boston. Assistant United States Attorney Eric Bruce claimed that MIT graduate Aafia Siddiqui was willing to help with an anthrax attack. Eric Bruce repeatedly referred to a planned chemical attack by Majid Khan but never described the plot or when and where it would occur. He said a woman affiliated with al-Qaida opened a Maryland post office box in the names of herself and Majid Khan so immigration documents could be sent there.

Siddiqui, 37, will now spend 60 years in federal prison.

A Little Telescope Goes a Long Way

NASA's Infrared Telescope Facility
NASA's Infrared Telescope Facility atop Mauna Kea, Hawaii. Copyright Ernie Mastroianni
NASA astronomers have successfully demonstrated that a David of a telescope can tackle Goliath-size questions in the quest to study Earth-like planets around other stars. Their work, reported today in the journal Nature, provides a new tool for ground-based observatories, promising to accelerate by years the search for prebiotic, or life-related, molecules on planets orbiting stars beyond our solar system.

The scientists reported on a new technique used with a relatively small Earth-based telescope to identify an organic molecule in the atmosphere of a Jupiter-size planet nearly 63 light-years away. The measurement revealed details of the exoplanet's atmospheric composition and conditions, an unprecedented achievement from an Earth-based observatory.

The surprising new finding comes from a venerable 30-year-old, 3-meter-diameter (10-foot) telescope that ranks 40th among ground-based telescopes - NASA's Infrared Telescope Facility atop Mauna Kea, Hawaii.

The new technique promises to further speed the work of studying planet atmospheres by enabling studies from the ground that were previously possible only through a few very high-performance space telescopes. "Given favorable observing conditions, this work suggests we may be able to detect organic molecules in the atmospheres of terrestrial planets with existing instruments," said lead author Mark Swain, an astronomer at NASA's Jet Propulsion Laboratory, Pasadena, Calif. This can allow fast and economical advances in focused studies of exoplanet atmospheres, accelerating our understanding of the growing stable of exoplanets.

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"The fact that we have used a relatively small, ground-based telescope is exciting because it implies that the largest telescopes on the ground, using this technique, may be able to characterize terrestrial exoplanet targets," Swain said.

This artist concept shows the planetary system called HD 189733, located 63 light-years away in the constellation Vulpecula

Currently, more than 400 exoplanets are known. Most are gaseous like Jupiter, but some "super-Earths" are thought to be large terrestrial, or rocky, worlds. A true Earth-like planet, with the same size as our planet and distance from its star, has yet to be discovered. NASA's Kepler mission is searching from space now, and is expected to find several of these earthly worlds by the end of its three-and-a-half-year prime mission.

On Aug. 11, 2007, Swain and his team turned the infrared telescope to the hot, Jupiter-size planet HD 189733b in the constellation Vulpecula. Every 2.2 days, the planet orbits a K-type main sequence star slightly cooler and smaller than our sun. HD189733b had already yielded breakthrough advances in exoplanet science, including detections of water vapor, methane and carbon dioxide, using space telescopes. Using the new technique, the astronomers successfully detected carbon dioxide and methane in the atmosphere of HD 189733b with a spectrograph, which splits light into its components to reveal the distinctive spectral signatures of different chemicals. Their key work was development of a novel calibration method to remove systematic observation errors caused by the variability of Earth's atmosphere and instability due to the movement of the telescope system as it tracks its target.

"As a consequence of this work, we now have the exciting prospect that other suitably equipped yet relatively small ground-based telescopes should be capable of characterizing exoplanets," said John Rayner, the NASA Infrared Telescope Facility support scientist who built the SpeX spectrograph used for these measurements. "On some days we can't even see the sun with the telescope, and the fact that on other days we can now obtain a spectrum of an exoplanet 63 light-years away is astonishing."

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This chart explains how astronomers measure the signatures of chemicals in the atmospheres of planets that orbit other stars, called exoplanets

In the course of their observations, the team found unexpected bright infrared emission from methane that stands out on the day side of HD189733b, indicating some kind of activity in the planet's atmosphere. Swain said this puzzling feature could be related to the effect of ultraviolet radiation from the planet's parent star hitting the planet's upper atmosphere, but more detailed study is needed. "This feature indicates the surprises that await us as we study exoplanet atmospheres," he added.

"An immediate goal for using this technique is to more fully characterize the atmosphere of this and other exoplanets, including detection of organic and possibly prebiotic molecules" like those that preceded the evolution of life on Earth, said Swain. "We're ready to undertake that task." Some early targets will be the super-Earths. Used in synergy with observations from NASA's Hubble, Spitzer and the future James Webb Space Telescope, the new technique "will give us an absolutely brilliant way to characterize super-Earths," Swain said.

Other authors are Pieter Deroo, Gautam Vasisht and Pin Chen of JPL; Caitlin A. Griffith of the University of Arizona, Tucson; Giovanna Tinetti of University College London; Ian J. Crossfield of UCLA; Azam Thatte of the Georgia Institute of Technology, Atlanta; Jeroen Bouwman, Cristina Afonso and Thomas Henning of Max-Planck Institute for Astronomy, Heidelberg, Germany; and Daniel Angerhausen of the German SOFIA Institute, Stuttgart, Germany.

The work was carried out with funding from NASA's Office of Space Science in Washington, D.C. The NASA Infrared Telescope Facility is managed by the University of Hawaii's Institute for Astronomy. JPL is managed by the California Institute of Technology for NASA.

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Out-of-This-World Super Bowl Coin Lands in Ohio

This medallion, which was flown in space aboard space shuttle Atlantis, will be used for the official coin toss prior to the kickoff of Super Bowl XLIVAfter traveling more than four million miles, and making 171 orbits around Earth on board space shuttle Atlantis, the Super Bowl XLIV opening-toss coin took a slight detour to the Pro Football Hall of Fame Museum in Canton, Ohio, on Jan. 27, before heading to the Super Bowl.

The coin was flown last November on STS-129 by crew members Commander Charlie Hobaugh, Pilot Barry Wilmore, and Mission Specialists Leland Melvin, Randy Bresnik, Mike Foreman and Bobby Satcher.

The astronauts stopped by the museum to return the silver-minted coin, as well as a few other space-flown memorabilia, including a football inscribed with the name of every member of the Hall of Fame. They also returned flown jerseys from the Detroit Lions and the Dallas Cowboys, the two teams Melvin played for in his short stint in the NFL.

The STS-129 crew presents a specially minted silver medallion to National Football League officials at the Pro Football Hall of Fame in Canton, OhioAfter stopping at the Hall of Fame, the coin will journey to Sun Life Stadium in Miami Gardens, Fla., to be the one of the stars of the Super Bowl XLIV pre-game coin toss on Feb. 7.

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<!-- “... ,” said Leland Melvin, STS-129 mission specialist, who was also drafted as a wide receiver in the NFL prior to becoming an astronaut.

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Mystery of the Fading Star

Using NASA's Spitzer Space Telescope, astronomers have found a likely solution to a centuries-old riddle of the night sky.

Every 27 years, a bright star called Epsilon Aurigae fades over period of two years, then brightens. Although amateur and professional astronomers have observed the system extensively, the nature of both the bright star and the companion object that periodically eclipses it have remained unclear. The companion is known to be surrounded by a dusty disk, as illustrated in this artist's concept.

Data from Spitzer finally seems to have solved the riddle. Spitzer's infrared vision revealed the size of the dusty disk that swirls around the companion object. When astronomers plugged this data into a model of the system, they were able to rule out the theory that the main bright star is a supergiant. Instead, it is a bright star with a lot less mass. The new model also holds that the companion object is a so-called "B star" circled by a dusty disk.

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NASA Extends Safety and Mission Assurance Contract at Marshall Space Flight Center in Alabama

NASA has exercised a second one-year option with Bastion Technologies Inc. of Houston for continued services in support of the Safety and Mission Assurance Directorate at NASA's Marshall Space Flight Center in Huntsville, Ala. The extension runs through Jan. 31, 2011.

The contract is a cost plus award fee with award term arrangements. The current potential value of the contract, including this $36 million contract option, is $136 million. Subsequent unexercised options and award terms extend the total period of performance to 2017, with a total potential value of more than $376 million.

Bastion Technologies Inc. continues to provide services, equipment and supplies associated with industrial safety and system safety, reliability and maintainability engineering associated with the design and development engineering and testing performed by Marshall. The contract also provides safety and mission assurance management information, quality assurance and quality engineering, independent assessment services and documentation, project assurance and risk management.

For information about NASA's Marshall Space Flight Center, visit:

http://www.nasa.gov/marshall

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Glow-in-the-Dark Plants are Highlight of International Space Station Science Briefing

NASA will shed light on plant investigations aboard the International Space Station in a briefing at noon EST, Friday, Feb. 5. The briefing from NASA's Kennedy Space Center in Florida will be broadcast live on NASA Television.

The upcoming shuttle mission, planned to launch Feb. 7, will continue assembling the space station so it can be used for continuous scientific research as a national and multinational laboratory.

Microgravity plant growth experiments conducted aboard the station will help prepare for long-duration spaceflights of the future. The use of miniaturized green fluorescent proteins, that glow in the dark, and associated compact imaging systems, may be used to help monitor crop conditions on Earth.

The briefing participants are:
-- Julie Robinson, International Space Station Program scientist, NASA's Johnson Space Center, Houston
-- Robert Ferl, principal investigator of Transgenic Arabidopsis Gene Expression System at the University of Florida, Gainesville
-- Wagner Vendrame, International Space Station National Laboratory investigator for National Lab Pathfinder-Cells at the University of Florida, Homestead
-- Perry Johnson-Green, senior program scientist, Life and Physical Sciences, Canadian Space Agency

NASA has published a new Web feature that provides examples of space station research dividends such as those related to cancer treatment delivery, food poisoning vaccine development, air purification, remote ultrasound tests and more.

For more information about space station science payoffs, visit:

http://www.nasa.gov/mission_pages/station/science/coolstation.html

For NASA TV streaming video, downlink and schedule information, visit:

http://www.nasa.gov/ntv

For more information about the upcoming shuttle mission, designated STS-130, visit:

http://www.nasa.gov/shuttle

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NASA Administrator Names Braun NASA Chief Technologist

NASA Administrator Charles F. Bolden named Robert D. Braun the agency's Chief Technologist, effective Wednesday, Feb. 3. Braun serves as the principle advisor and advocate on matters concerning agency-wide technology policy and programs.

The appointment comes as NASA launches a bold new initiative that targets technologies that could be transformational in their ability to improve the capability, reduce the cost, and expand the reach of future human and robotic missions.

"Bobby brings expert knowledge of spacecraft, robotic and planetary exploration technology development to this new position," Bolden said. "His experience working at NASA Langley and in the academic community brings an excellent skill mix to this exciting and challenging new job."

Braun will help develop a broadly focused advanced concepts and technology development program leading to new approaches to future NASA missions and solutions to significant national needs.

During the coming decade, NASA will increase its support for research in advanced concepts and critical enabling technologies, including test programs for multiple technology flight demonstrations. New technologies include advanced lightweight structures and materials, advanced propulsion, power generation, energy storage and high bandwidth communications. This program also will generate spin-off technologies and potentially entire new industries.

Braun has more than 20 years experience performing design and analysis of planetary exploration systems as a member of the technical staff at NASA's Langley Research Center in Hampton, Va., and the Georgia Institute of Technology. His research has focused on systems aspects of planetary exploration, where he has contributed to the design, development, test, and operation of several robotic space flight systems.

Braun was a member of the Mars Pathfinder design and landing operations team from 1992 to 1997 and has been part of development teams for the Mars Microprobe, Mars Sample Return and Mars Surveyor 2001 projects.

Braun also provided independent assessment and served on NASA review boards for the Mars Polar Lander, Mars Odyssey, Mars Exploration Rover, Phoenix Mars Scout, Genesis, and Mars Science Laboratory flight projects.

Braun received a B.S. in Aerospace Engineering from Penn State in 1987, M.S. in Astronautics from the George Washington University in 1989, and Ph.D. in Aeronautics and Astronautics from Stanford University in 1996. He has received the 1999 AIAA Lawrence Sperry Award, two NASA Exceptional Achievement Medals, two NASA Inventions and Contributions Team Awards, and seven NASA Group Achievement Awards. He is an AIAA Fellow and the principle author or co-author of over 175 technical publications.

For more information about NASA, please visit:

http://www.nasa.gov

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NASA Administrator Names Woodrow Whitlow Associate Administrator for Mission Support

On Wednesday, NASA Administrator Charles Bolden named Dr. Woodrow Whitlow, Jr., the associate administrator for Mission Support at NASA Headquarters in Washington. Whitlow will continue to serve as the director of NASA's Glenn Research Center in Cleveland until a successor is named.

In this new position, Whitlow will be responsible for most NASA management operations, including human capital, budget and systems support as well as a variety of other vital cross agency business, institutional and contract support functions.

"Woodrow is a dedicated and valued member of my senior leadership team, and I am pleased he agreed to accept this new challenge," Bolden said. "As the agency moves forward, we need to streamline the way we do business with a fresh approach and an eye for strategic management and investments. I know the people of Glenn will miss Woodrow, but the entire agency will again have the opportunity to benefit from his insight and experience."

As the Glenn director since Dec. 25, 2005, Whitlow has led a workforce of more than 3,400 civil service and support service contractors. The center is distinguished by its unique blend of aeronautics and spaceflight research and development experience.

Before being named director of Glenn, Whitlow served as the deputy director of NASA's Kennedy Space Center in Florida. He assisted the director in determining and implementing center policy and managing and implementing the center's missions and agency program responsibilities. Areas of responsibility included processing, launch, and recovery of launch vehicles, processing of spacecraft and acquisition of launch services.

Prior to his appointment as deputy director at Kennedy, Whitlow was the director of Research and Technology at Glenn.

Whitlow began his NASA career in 1979 as a research scientist at the agency's Langley Research Center in Hampton, Va. He assumed various positions of increasing responsibility before moving to Glenn in 1998. In 1994, he served as director of the Critical Technologies Division in the Office of Aeronautics at NASA Headquarters.

Whitlow earned his bachelor's degree, master's degree, and doctorate in aeronautics and astronautics from the Massachusetts Institute of Technology.

For more information about NASA and agency programs, visit:

http://www.nasa.gov

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Moon and Mars Not Out

Most people think that the end of the Constellation program, will impede NASA’s ability to go to the Moon and beyond. I believe that we can use the change in direction to get to the Moon or Mars faster than if we stuck to the Constellation program (at the very least we can get to Mars faster). The Constellation program, was projected to get us to the Moon by 2020. However, the program has been over-budget, and behind schedule. Given the lack of proper funding, I predict that if we choose to go through with the Constellation program we would not get to the moon until after 2020, maybe 2022 or 2025 if at all.

Eventhough, I agree that lack of proper funding is a major source of problems with the Constellation program, I still think that the Constellation program is a bad strategy for NASA. The reason that I think it is a bad strategy is because there are too many unknowns, too many things that need to be developed that can’t be developed until later in the program (or at the very least verified), and too rigid a box to get it done (it doesn’t help that we also don’t have the proper budget to get this done, but when you add physical constraints it makes life very difficult). Further the long development time, requires us to develop and work on technology that will be severely outdated by the time we get to use it.

What the Constellation program has given NASA is the strong and clear realization that we need to leave near earth orbit and go to the Moon, Mars and Beyond; while providing a clear path to doing it. The goal of going to the Moon or Mars has to remain central to any planning that NASA does.

  • What technologies can NASA work on now, so that if we were to fund a program in the future to go to the Moon, Mars, etc it would reduce the amount of time needed to get the project done?
  • What technologies can NASA work on now, that can be used as leverage in international partnerships, and commercial partnerships?

Do not be deceived, NASA has a real customer. The customer is the political market. As Mike Coats pointed out, in a recent All-Hands, around every eight years the political party in power changes, and with it comes new direction. Policy defines the priorities that NASA has to be concerned with, and the budget that we have for those specific priorities. Our objective is to explore, WE define that, independently of any policy direction that Congress and the President gives us. When a new direction is given by the President, we get to determine the method of implementing the direction. What we must be able to do is get a significant victory (several preferably) in the pursuit of going to other planets, every time that a new administration and direction is given to us.

For example, with the Constellation Program, the path to get anywhere took too long. Part of the path to the moon could have been to get to the ISS, as a first step, with the CEV capsule, in a method that would have gotten us there before the President was scheduled to leave office.  Scheduling this way would prohibit the project from being stopped by the next President. If we had a second method of getting to the ISS we could comfortably retire the Shuttle, and more funds would have been able to go to funding the path to the Moon or Mars. Also, it is very difficult to argue with success. If we show that we are making progress, the president has less leverage/reason to change the direction. Also, going to the ISS with a new vehicle would have been a great way of getting the public around our mission. Hindsight is 20/20, but this is a lesson that we must learn: there are real timelines (political ones), we must strategize to these timelines.

With the new budget and direction (Robotic Precursor Missions), we could develop a robotic expedition to go to the Moon and return. This would develop critical intelligence, that we have likely lost, in how to return to earth from another planet. By doing it through a robotic expedition, we can minimize the cost of getting this project done. If we do it in such a way that we could one day take cargo to the moon with the capsule, then we could use this project as a stepping stone for new projects in the future (like sending animal experiments to the Moon or Mars). We wouldn’t have to (or want to) develop new rocket technology, it would be wise to use existing technologies to get this done. If it is possible to do it with a stripped down version of the CEV capsule, then we can leverage the work we have already done for the Constellation Program. I don’t know enough, to say if the weight and size (geometric dimensions) would make using the CEV cost prohibitive.

With the “Heavy Lift and Propulsion R&D” money in the budget we could develop technologies that allow us to launch from on-orbit. Launching in space, reduces the amount of thrust and fuel needed to get to our destination. Launching on earth, requires a huge amount of thrust just to move, which causes the launch to go through extreme accelerations. The accelerations cause increased load, which requires stronger structure, which increases the weight. If we launch in space, we can develop rocket technology that has a more steady thrust release. We don’t have to accelerate as fast as we would from earth (we just accelerate for a longer time).   This would reduce the structural strength required (lowering the mass), while still having the ability to get to velocities that get us there quickly.

I guess I will leave with:

We don’t define policy, but we do get to define the approach of implementing the applicable policy. We have to maximize victories needed to explore space, within the political schedule. By showing progress within the political schedule, the policymakers have less leverage to change our direction, increasing the speed that we get to go to the Moon and Mars (or whatever other destination).   Also, the progress helps us get the public around our mission, which increases our chance of getting our budget increased.

Study shows antidepressants useless for mild to moderate depression? Not exactly.

As Harriet Hall has written (http://www.sciencebasedmedicine.org/?p=353), psychiatry bashing is a popular media sport. There seems to be a bias against treatment of psychiatric disabilities, and a common claim is that antidepressants are no better than placebo. The New York Times illustrated both the perpetuation of the myth that antidepressants are ineffective, and the increasing and disturbing tendency of major media organizations to confuse the wholesale acceptance of medical press releases with medical journalism.

In Popular Drugs May Help Only Severe Depression The New York Times credulously publicized the findings of a recent study that claimed to show that antidepressants are ineffective in treating mild and moderate depression. Yes, that’s what the study showed, but the study itself is so limited, so fraught with problems, and the conclusions are so misleading that the article is a terrible disservice.

Before we consider what the study showed, let’s think about what kind of evidence we’d need to conclude that antidepressants don’t work.

First, although there are different types of antidepressants, the term used colloquially refers to antidepressants of a specific type, SSRI’s or selective serotonin receptor inhibitors. There are other, older types of antidepressants that are rarely used today because of their unpleasant side effects. Hence any study that claims to show that “antidepressants” are ineffective, must look at SSRIs.

Second, there are literally thousands of studies of SSRIs, and it would be helpful to aggregate the results. Aggregating results can be done in a type of paper known as metaanalysis. Metaanlysis adds the results of multiple similar studies to find trends that might not be apparent in individual small studies. But a metaanlysis is subject to several important limitations that must always be considered. The most important limitation is that the authors of the metaanalysis choose the papers to be included. Bias can be introduced by examining only papers that have a desired outcome; that can be accomplished by restricting the inclusion criteria in arbitrary ways.

Let’s look at the study, Antidepressant Drug Effects and Depression Severity. According to the abstract:

Randomized placebo-controlled trials of antidepressants approved by the Food and Drug Administration in the treatment of major or minor depressive disorder were selected. Studies were included if their authors provided the requisite original data, they comprised adult outpatients, they included a medication vs placebo comparison for at least 6 weeks, they did not exclude patients on the basis of a placebo washout period, and they used the Hamilton Depression Rating Scale (HDRS). Data from 6 studies (718 patients) were included…

… The magnitude of benefit of antidepressant medication compared with placebo increases with severity of depression symptoms and may be minimal or nonexistent, on average, in patients with mild or moderate symptoms. For patients with very severe depression, the benefit of medications over placebo is substantial.

According to one of the authors was interviewed for the NYTimes article:

“The message for patients with mild to moderate depression,” Dr. DeRubeis said, “is, ‘Look, medications are always an option, but there’s little evidence that they add to other efforts to shake the depression — whether it’s exercise, seeing the doctor, reading about the disorder or going for psychotherapy.’ ”

Let’s go back and compare the paper to the criteria we identified above. The first criterion was to look at the antidepressants currently used in clinical practice. But out of the 6 studies in the metaanalysis, 3 looked at imipramine, a tricyclic antidrepressant that has not been the standard of care for over a decade because of its unpleasant side effects. The other three studies looked at Paxil (paroxitene). Paxil is an SSRI, but it is only one member of the class of SSRIs. Although all SSRIs share the same mechanism of action, they have different profiles of effectiveness and side effects. Therefore, generalizing from Paxil to all SSRIs cannot be justified.

So in terms of clinically relevant information, the paper included only 3 studies of an SSRI. How did the authors whittle down thousands of papers on SSRI effectiveness to only 3? According to the authors:

The criteria for inclusion required studies to be randomized placebo controlled trials of an FDA-approved antidepressant in the treatment of the full range of patients with major or minor depressive disorder … In addition, the studies had to include an ADM/placebo comparison of at least 6 weeks’ duration and HDRS scores at intake and at the end of treatment. Studies were excluded if they excluded patients on the basis of a placebo washout period. The final inclusion criterion was that individual patient-level data had to be available for analysis.

Are these criteria relevant? Certainly, the inclusion of only RCTs is a reasonable criterion. However, it is not clear why the availability of patient level data is a relevant criterion. Most RCTs, from an enormous range of clinical investigations, do not include patient level data, and using that as a criterion is bound to exclude most studies.

Finally, the decision to remove studies that included a placebo washout period also excludes a vast swath of psychiatric studies. That decision is more defensible, however, since there is disagreement among psychiatric researchers about whether a placebo washout period introduces bias into the study. A placebo washout period involves treating everyone in both arms of the study with placebo for an initial period of time, often 3 weeks. People who respond to placebo are then excluded from the study. The theory is that excluding known placebo responders makes it easier to identify real effects.

Others have argued that excluding known placebo responders up front necessarily makes the drug effects look better than they would have. For example, in a traditional placebo controlled RCT, there might be 30% who respond to placebo and 50% who respond to the medication under study, for a difference of 20%. If some placebo responders are identified during a washout period, let’s say 20% of patients, they will be excluded. The final results may be that 10% responded to placebo and 50% responded to the medication under study, for a difference of 40%, making the medication under study look better.

There is one indisputably arbitrary criterion that is acknowledged by the authors. The initial analysis identified 23 studies, but they could only gain access to the data in 6 studies, so they simply ignored the other 17.

In summary, then, by using questionable exclusion criteria, the authors accessed only 3 clinically relevant studies (the Paxil studies), involving only one SSRI. It is not clear that these studies are representative of existing studies on SSRIs, or even if they can be generalized to other SSRIs. Dr. Rubeis’ assertion that for patients with mild to moderate depression there is little evidence that “medications” add to efforts to treat the depression cannot be justified by the findings in his study. I find his claims to be irresponsible. The paper adds to the literature on antidepressants but is so limited that it cannot tell us whether antidepressants are effective for mild to moderate depression.


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