Posts tagged Atlantic Ocean
Climate change early warning system called for
Dec 3rd
Climate change has increased concern over possible large and rapid changes in the physical climate system, including Earth’s atmosphere, land surfaces and oceans, said Professor James White of CU-Boulder’s Institute of Arctic and Alpine Research and the chair of the National Research Council committee. Some abrupt changes and impacts already underway – including the loss of Arctic sea ice and increases in the extinction rates of marine and terrestrial species – and others could occur within a few decades or even years, said the committee.
“Research has helped us begin to distinguish more imminent threats from those that are less likely to happen this century,” said White, also a CU-Boulder professor in geological sciences. “Evaluating climate changes and impacts in terms of their potential magnitude and the likelihood they will occur will help policymakers and communities make informed decisions about how to prepare for or adapt to them.”
Other scenarios, such as the destabilization of the west Antarctic ice sheet, have potentially major consequences, but the probability of these changes occurring within the next century is not well understood, highlighting the need for more research, according to the committee.
In some cases, scientific understanding has progressed enough to determine whether certain high-impact climate changes are likely to happen within the next century. The report notes that a shutdown in the Atlantic Ocean circulation patterns or a rapid release of methane from high-latitude permafrost or undersea ice are now known to be unlikely this century, although these potential abrupt changes are still worrisome over longer time horizons.
But even changes in the physical climate system that happen gradually over many decades or centuries can cause abrupt ecological or socio-economic change once a “tipping point” is reached, the report adds. Relatively slow global sea-level rise could directly affect local infrastructure such as roads, airports, pipelines or subway systems if a sea wall or levee is breached. And slight increases in ocean acidity or surface temperatures could cross thresholds beyond which many species cannot survive, leading to rapid and irreversible changes in ecosystems that contribute to extinction events.
Further scientific research and enhanced monitoring of the climate, ecosystems and social systems may be able to provide information that a tipping point is imminent, allowing time for adaptation or possibly mitigation, or that a tipping point has recently occurred, the report says.
“Right now we don’t know what many of these thresholds are,” White said. “But with better information, we will be able to anticipate some major changes before they occur and help reduce the potential consequences.” The report identifies several research needs, such as identifying keystone species whose population decline due to an abrupt change would have cascading effects on ecosystems and ultimately on human provisions such as food supply.
If society hopes to anticipate tipping points in natural and human systems, an early warning system for abrupt changes needs to be developed, the report says. An effective system would need to include careful and vigilant monitoring, taking advantage of existing land and satellite systems and modifying them if necessary, or designing and implementing new systems when feasible. It would also need to be flexible and adaptive, regularly conducting and alternating between data collection, model testing and model predictions that suggest future data needs.
The study was sponsored by the National Oceanic and Atmospheric Administration, National Science Foundation, U.S. intelligence community, and the National Academies. The National Academy of Sciences, National Academy of Engineering, Institute of Medicine, and National Research Council make up the National Academies. They are private, independent nonprofit institutions that provide science, technology, and health policy advice under a congressional charter granted to NAS in 1863. The National Research Council is the principal operating agency of the National Academy of Sciences and the National Academy of Engineering.
For more information and a copy of the report visit http://national-academies.org. For more information on INSTAAR visithttp://instaar.colorado.edu.
Boulder High, CU grad astronaut Scott Carpenter dies at 88
Oct 11th
Carpenter, a Boulder native, entered CU-Boulder’s astronautical engineering program in 1945, eventually earning a bachelor of science degree. He orbited Earth three times on May 24, 1962, in NASA’s Aurora 7 capsule before splashing down in the Atlantic Ocean.
Carpenter was the first of 18 CU-Boulder astronaut affiliates to have flown in space. As one of the first NASA astronauts, Carpenter and his colleagues were celebrated in the Tom Wolfe book, “The Right Stuff,” which told the story of early military test pilots and the original Mercury 7 astronauts.
Born in Boulder on May 1, 1925, Carpenter and graduated from Boulder High School in 1943. He then entered the Navy’s V12a flight training program at Colorado College in Colorado Springs. He spent the next year training in California and Iowa, returning to Boulder in 1945 to study at CU-Boulder.
“In his two-decades long career as a Naval aviator, astronaut and aquanaut, Scott Carpenter brought honor and distinction to CU-Boulder while embodying the adventurous spirit of our nation,” said CU-Boulder Chancellor Philip P. DiStefano. “Our space program, and all space and ocean researchers everywhere, owe him a debt of gratitude. He will be sorely missed.”
In 1965 Carpenter took a leave of absence from NASA to participate in the Navy’s Man-in-the Sea Project as an aquanaut in the SEALAB II project off the coast of La Jolla, Calif. where he spent 30 days living and working on the ocean floor at a depth of more than 200 feet. Because of his groundbreaking deep-sea diving experiences with the Navy, Carpenter is hailed by many to be the first person to conquer both outer and inner space.
“My colleagues and I are deeply saddened by the passing of Astronaut Scott Carpenter,” said CU-Boulder aerospace engineering sciences Chair Penina Axelrad. “He has long been a member of the CU family and a tremendous inspiration for our aerospace faculty and students.”
In a 2012 interview with CU’s alumni magazine, the Coloradan, Carpenter spoke about his historic space journey. “I still remember what a thrill it was being up there — I liked the feeling of weightlessness, and the view I had of Earth.”
Carpenter and the other Mercury 7 astronauts created the Astronaut Scholarship Foundation in 1984. The foundation now involves more than 80 astronauts, awards 28 $10,000 scholarships annually and has dispersed more than $3 million to promising students in science and engineering since 1986.
As one of the original Mercury 7 astronauts, Carpenter followed Alan Shepard, Gus Grissom and Glenn into space and was followed by Wally Schirra, Gordon Cooper and Deke Slayton.
Carpenter was commissioned in the U.S. Navy in 1949 and flew a variety of missions during the Korean War. He attended Navy Test Pilot School in Maryland in 1954 and was assigned as an Air Intelligence Officer on the USS Hornet aircraft carrier. In April of 1959 he was selected by NASA to be an astronaut.
Although he was one course requirement short of graduating with a bachelor’s degree in aeronautical engineering when he left CU in 1949, the university awarded him his degree in 1962 following the successful Aurora 7 flight. When presenting the degree to Carpenter, then-CU President Quigg Newton noted that “his subsequent training as an astronaut has more than made up for his deficiency in the subject of heat transfer.”
In 1967 he became the Navy’s director of aquanaut operations during the SEALAB III experiment. After retiring from the Navy in 1969, he founded and became CEO of Sea Sciences Inc., a venture capital corporation that developed programs aimed at enhanced use of ocean resources and improved health of the planet. He worked closely with noted diver and scientist Jacques Cousteau and members of his Calypso team, and subsequently dove in most of the world’s oceans, including under Arctic ice.
Carpenter later became a consultant to industry and the private sector and has lectured around the world, narrated TV documentaries and written several books, including the 2002 New York Times best-seller, “For Spacious Skies: The Uncommon Journey of a Mercury Astronaut” co-authored with his daughter, Kris Stoever.
-CU-
CU study hints conditions on Mars may support energy for life forms
May 30th
The findings, published in the journal Nature Geoscience, also hint at the possibility that hydrogen-dependent life could have existed where iron-rich igneous rocks on Mars were once in contact with water.
Scientists have thoroughly investigated how rock-water reactions can produce hydrogen in places where the temperatures are far too hot for living things to survive, such as in the rocks that underlie hydrothermal vent systems on the floor of the Atlantic Ocean. The hydrogen gases produced in those rocks do eventually feed microbial life, but the communities are located only in small, cooler oases where the vent fluids mix with seawater.
The new study, led by CU-Boulder Research Associate Lisa Mayhew, set out to investigate whether hydrogen-producing reactions also could take place in the much more abundant rocks that are infiltrated with water at temperatures cool enough for life to survive.
“Water-rock reactions that produce hydrogen gas are thought to have been one of the earliest sources of energy for life on Earth,” said Mayhew, who worked on the study as a doctoral student in CU-Boulder Associate Professor Alexis Templeton’s lab in the Department of Geological Sciences.
“However, we know very little about the possibility that hydrogen will be produced from these reactions when the temperatures are low enough that life can survive. If these reactions could make enough hydrogen at these low temperatures, then microorganisms might be able to live in the rocks where this reaction occurs, which could potentially be a huge subsurface microbial habitat for hydrogen-utilizing life.”
When igneous rocks, which form when magma slowly cools deep within the Earth, are infiltrated by ocean water, some of the minerals release unstable atoms of iron into the water. At high temperatures — warmer than 392 degrees Fahrenheit — scientists know that the unstable atoms, known as reduced iron, can rapidly split water molecules and produce hydrogen gas, as well as new minerals containing iron in the more stable, oxidized form.
Mayhew and her co-authors, including Templeton, submerged rocks in water in the absence of oxygen to determine if a similar reaction would take place at much lower temperatures, between 122 and 212 degrees Fahrenheit. The researchers found that the rocks did create hydrogen — potentially enough hydrogen to support life.
To understand in more detail the chemical reactions that produced the hydrogen in the lab experiments, the researchers used “synchrotron radiation” — which is created by electrons orbiting in a manmade storage ring — to determine the type and location of iron in the rocks on a microscale.
The researchers expected to find that the reduced iron in minerals like olivine had converted to the more stable oxidized state, just as occurs at higher temperatures. But when they conducted their analyses at the Stanford Synchrotron Radiation Lightsource at Stanford University, they were surprised to find newly formed oxidized iron on “spinel” minerals found in the rocks. Spinels are minerals with a cubic structure that are highly conductive.
Finding oxidized iron on the spinels led the team to hypothesize that, at low temperatures, the conductive spinels were helping facilitate the exchange of electrons between reduced iron and water, a process that is necessary for the iron to split the water molecules and create the hydrogen gas.
“After observing the formation of oxidized iron on spinels, we realized there was a strong correlation between the amount of hydrogen produced and the volume percent of spinel phases in the reaction materials,” Mayhew said. “Generally, the more spinels, the more hydrogen.”
Not only is there a potentially large volume of rock on Earth that may undergo these low temperature reactions, but the same types of rocks also are prevalent on Mars, Mayhew said. Minerals that form as a result of the water-rock reactions on Earth have been detected on Mars as well, which means that the process described in the new study may have implications for potential Martian microbial habitats.
Mayhew and Templeton are already building on this study with their co-authors, including Thomas McCollom at CU-Boulder’s Laboratory for Atmospheric and Space Physics, to see if the hydrogen-producing reactions can actually sustain microbes in the lab.
This study was funded by the David and Lucille Packard Foundation and with a U.S. Department of Energy Early Career grant to Templeton.
-CU-
[includeme src=”http://c1n.tv/boulder/media/bouldersponsors.html” frameborder=”0″ width=”670″ height=”300″]