Washington, DC–Renowned astrophysicist and National Medal of Science awardee Vera Rubin passed away in Princeton N.J., the evening of December 25, 2016, at the age of 88. Rubin confirmed the existence of dark matter—the invisible material that makes up more than 90% of the mass of the universe. She...
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    “Scientists are my best friends,” wildlife photographer Frans Lanting said during a retrospective program at Carnegie’s Washington, DC, headquarters last week.

    He added that without the ability to learn from researchers and generate ideas for new images with them, his work would not hold the same power. “It’s like sculpting,” he said, speaking of these collaborations and conversations.

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Stanford, CA—New work from Carnegie’s Shouling Xu and Zhiyong Wang reveals that the process of synthesizing many important master proteins in plants involves extensive modification, or “tagging” by sugars after the protein is assembled. Their work uncovers both similarity and distinction between plants and animals in their use of this protein modification. It is published by Proceedings of the National Academy of Sciences.

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Washington, DC— An international team of astronomers released the largest-ever compilation of exoplanet-detecting observations made using a technique called the radial velocity method. They demonstrated how these observations can be used to hunt for planets by detecting more than 100 potential exoplanets, including one orbiting the fourth-closest star to our own Solar System, which is about 8.1 light years away from Earth.

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Although helium is the second most-abundant element (after hydrogen) in the universe, it doesn’t play well with others. It is a member of a family of seven elements called the noble gases, which are called that because of their chemical aloofness—they don’t easily form compounds with other elements. Helium, widely believed to be the most inert element, has no stable compounds under normal conditions. Now, an international team of researchers including several Carnegie scientists has predicted two stable helium compounds.

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Baltimore, MD—A first-of-its-kind study on almost 20,000 K-12 underrepresented public school students shows that Project BioEYES, based at Carnegie’s Department of Embryology, is effective at increasing students’ science knowledge and positive attitudes about science. Younger students had the greatest attitude changes. The study covered five years and tested students before and after the one-week BioEYES program.

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In mammals, most lipids, such as fatty acids and cholesterol, are absorbed into the body via the small intestine. The complexity of the cells and fluids that inhabit this organ make it very difficult to study in a laboratory setting. The goal of the Farber lab is to better understand the cell and...
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Fresh water constitutes less than 1% of the surface water on earth, yet the importance of this simple molecule to all life forms is immeasurable. Water represents the most vital reagent for chemical reactions occurring in a cell. In plants, water provides the structural support necessary for plant...
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Until now, computer models have been the primary tool for estimating photosynthetic productivity on a global scale. They are based on estimating a measure for plant energy called gross primary production (GPP), which is the rate at which plants capture and store a unit of chemical energy as biomass...
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Capital Science Evening Lectures
Tuesday, March 7, 2017 -
6:30pm to 8:00pm

Since releasing its first images of space 5 years ago, the Atacama Large Millimeter/submillimeter Array (ALMA) has produced many exciting and fundamental results, enabling transformational science...

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Astronomy Lecture Series
Monday, April 3, 2017 -
7:30pm to 8:30pm

Supernovae are cosmic explosions where a single star can become as bright as a billion stars combined. Even though supernovae are crucial to the Universe, including producing the elements...

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Capital Science Evening Lectures
Thursday, April 6, 2017 -
6:30pm to 8:00pm

Dr. Ostrander’s team has taken advantage of naturally occurring variations in dog populations in order to reveal the genetic mechanisms underlying both simple and complex traits. She will show how...

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Matthew Evans wants to provide new tools for plant scientists to engineer better seeds for human needs. He focuses on one of the two phases to their life cycle. In the first phase, the sporophyte is the diploid generation—that is with two similar sets of chromosomes--that undergoes meiosis to...
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Roiling cauldrons of liquid-laden material flow within Earth’s rocky interior. Understanding how this matter moves and changes is essential to deciphering Earth’s formation and evolution as well as the processes that create seismic activity, such as earthquakes and volcanoes. Bjørn Mysen probes...
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Anthony Piro is the George Ellery Hale Distinguished Scholar in Theoretical Astrophysics at the Carnegie Observatories. He is a theoretical astrophysicist studying compact objects, astrophysical explosions, accretion flows, and stellar dynamics. His expertise is in nuclear physics, thermodynamics,...
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Carnegie Science, Carnegie Institution, Carnegie Institution for Science
February 13, 2017

Washington, DC— An international team of astronomers released the largest-ever compilation of exoplanet-detecting observations made using a technique called the radial velocity method. They demonstrated how these observations can be used to hunt for planets by detecting more than 100 potential exoplanets, including one orbiting the fourth-closest star to our own Solar System, which is about 8.1 light years away from Earth. The paper is published in The Astronomical Journal.

The radial velocity method is one of the most successful techniques for finding and confirming planets. It takes advantage of the fact that in addition to a planet being influenced by the gravity of the star it

February 6, 2017

Washington, DC— Although helium is the second most-abundant element (after hydrogen) in the universe, it doesn’t play well with others. It is a member of a family of seven elements called the noble gases, which are called that because of their chemical aloofness—they don’t easily form compounds with other elements. Helium, widely believed to be the most inert element, has no stable compounds under normal conditions. 

Now, an international team of researchers led by Skoltech’s Artem R. Oganov (also a professor at Stony Brook University and head of Computational Materials Discovery laboratory at Moscow Institute of Physics and Technology) has predicted two stable helium compounds—

February 2, 2017

Washington, D.C.—In Earth’s interior, water (H2O) plays an important role in rock physics, but geoscientists rarely treat water in its constituent forms, that is as hydrogen plus oxygen. New work from a team led by Carnegie’s Dave Mao has identified that hydrogen can escape from the water under conditions found in Earth’s lower mantle leading to a new paradigm in lower-mantle chemistry. Their results were published in Proceedings of the National Academy of Sciences, U.S.A.          

In the atmosphere, hydrogen is a colorless, transparent gas. It bonds with oxygen to form water, which fuels the biosphere on the Earth’s surface. Deep in the rocky world beneath our feet, so-called

February 1, 2017

Yingwei Fei, a high-pressure experimentalist at the Geophysical Laboratory, and Peter Driscoll, theoretical geophysicist in the Department of Terrestrial Magnetism, have been awarded a Carnegie Science Venture Grant for their project “Direct Shock Compression of Pre-synthesized Mantle Mineral to Super-Earth Interior Conditions.”

The project is an entirely new approach to investigate the properties and dynamics of super-Earths—extrasolar planets with masses between one and 10 times that of Earth. They will use the world’s most powerful magnetic, pulsed-power radiation source, called the Z Machine at Sandia National Laboratory, to generate shock waves that can simulate the intense

March 7, 2017

Since releasing its first images of space 5 years ago, the Atacama Large Millimeter/submillimeter Array (ALMA) has produced many exciting and fundamental results, enabling transformational science in a wide range of astronomy and planetary science subjects, from the Solar System to the early universe. Dr. Cox will present a selection of the most-remarkable ALMA scientific discoveries, compare the array’s original fundamental science with its current results, and outline the future evolution of ALMA. 

Dr. Pierre Cox, Director, ALMA
#CosmicOrigins

The Capital Science Evenings are made possible in part by the generous support of Margaret and Will Hearst.

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April 3, 2017

Supernovae are cosmic explosions where a single star can become as bright as a billion stars combined. Even though supernovae are crucial to the Universe, including producing the elements necessary for life, many mysteries remain. What powers them? Which stars are exploding? How do stars die? Astrophysicists are combining clues from observations with theoretical modeling to finally address these issues. And just like with any good mystery, often the answers lead to even more questions.

Tony Piro, George Ellery Hale Distinguished Scholar in Theoretical Astrophysics, Carnegie Observatories

Registration opens Wednesday, February 15. Registration is required. 

April 6, 2017

Dr. Ostrander’s team has taken advantage of naturally occurring variations in dog populations in order to reveal the genetic mechanisms underlying both simple and complex traits. She will show how findings related to the genetic basis for canine disease, behavior, and morphologic traits frame our thinking of human growth regulation, disease, and population migration.

Dr. Elaine Ostrander, Chief, Cancer Genetics and Comparative Genomics, National Human Genome Research Institute, Nation Institute of Health
#DogGenetics

The Capital Science Evenings are made possible in part by the generous support of Margaret and Will Hearst.

Check back one week prior to the

April 17, 2017

The formation of galaxies like our Milky Way involves gravity, dark matter, gases, star formation, and stellar explosions. Theoretical astrophysics is now revealing this complex process by using the world’s most powerful supercomputers to simulate galaxy formation. Dr. Wetzel will describe dramatic new advances in understanding how galaxies form within the cosmic web of the Universe.

Andrew Wetzel, Caltech-Carnegie Postdoctoral Fellow

Registration opens Wednesday, February 15. Registration is required. 

Fifty years ago, Americans led the world in math and science, claiming some of the most important inventions and technological breakthroughs of the 20th century.  Today, American 15-year-olds rank 25th in math compared to their peers worldwide.  Math ƒor America DC strives to reclaim America’s reputation for scientific greatness by recruiting and supporting the very best secondary education math teachers.

Here in Washington DC, the majority of secondary school students are not math proficient.  Only about two thirds of secondary school math teachers are fully certified.Our goals follow:

Recruit candidates with strong math knowledge and teaching aptitude, which enhances the

High-elevation, low relief surfaces are common on continents. These intercontinental plateaus influence river networks, climate, and the migration of plants and animals. How these plateaus form is not clear. Researchers are studying the geodynamic processes responsible for surface uplift in the Hangay in central Mongolia to better understand the origin of high topography in continental interiors.

This work focuses on characterizing the physical properties and structure of the lithosphere and sublithospheric mantle, and the timing, rate, and pattern of surface uplift in the Hangay. They are carrying out studies in geomorphology, geochronology, thermochronology, paleoaltimetry,

Carnegie researchers are developing new scientific approaches that integrate phylogenetic, chemical and spectral remote sensing perspectives - called Spectranomics - to map canopy function and biological diversity throughout tropical forests of the world.

Mapping the composition and chemistry of species in tropical forests is critical to understanding forest functions related to human use and climate change. However, high-resolution mapping of tropical forest canopies is challenging because traditional field, airborne and satellite measurements cannot easily measure the canopy chemical or taxonomic variation among species over large regions. New technology, such as the Carnegie

The thyroid gland secretes thyroxine (TH), a hormone essential for the growth and development of all vertebrates including humans. To understand TH action, the Donald Brown lab studies one of the most dramatic roles of the hormone, the control of amphibian metamorphosis—the process by which a tadpole turns into a frog. He studies the frog Xenopus laevis, from South Africa, because it is easy to rear. Events as different as the formation of limbs, the remodeling of organs, and the resorption of tadpole tissues such as the tail are all directed by TH. How can a simple molecule control so many different developmental changes? The hormone works by regulating the expression of groups of genes

Viktor Struzhkin develops new techniques for high-pressure experiments to measure transport and magnetic properties of materials to understand aspects of geophysics, planetary science, and condensed-matter physics. Among his goals are to detect the transition of hydrogen into a high-temperature superconductor under pressure—a state predicted by theory, but thus far unattained—to discover new superconductors, and to learn what happens to materials in Earth’s deep interior where pressure and temperature conditions are extreme. 

Recently, a team including Struzhkin was the first to discover the conditions under which nickel oxide can turn into an electricity-conducting metal. Nickel

François Schweizer studies galaxy assembly and evolution by observing nearby galaxies, particularly how collisions and mergers affect their properties. His research has added to the awareness that these events are dominant processes in shaping galaxies and determining their stellar and gaseous contents.

When nearby galaxies collide and merge they yield valuable clues about processes that occurred much more frequently in the younger, distant universe. When two gas-rich galaxies collide, their pervasive interstellar gas gets compressed, clumps into dense clouds, and fuels the sudden birth of billions of new stars and thousands of star clusters.

Some of the newborn clusters

Geochemist and director of Terrestrial Magnetism, Richard Carlson, looks at the diversity of the chemistry of the early solar nebula and the incorporation of that chemistry into the terrestrial planets. He is also interested in questions related to the origin and evolution of Earth’s continental crust.

  Most all of the chemical diversity in the universe comes from the nuclear reactions inside stars, in a process called nucleosynthesis. To answer his questions, Carlson developes novel procedures using instruments called mass spectrometers to make precise measurements of isotopes--atoms of an element with different numbers of neutrons--of Chromium (Cr), strontium (Sr), barium ( Ba

Carnegie Science, Carnegie Institution for Science, Carnegie Institution

Greg Asner is a staff scientist in Carnegie's Department of Global Ecology and also serves as a Professor in the Department of Earth System Science at Stanford University. He is an ecologist recognized for his exploratory and applied research on ecosystems, land use, and climate change at regional to global scales.

Asner graduated with a bachelor’s degree in engineering from the University of Colorado, Boulder, in 1991. He earned master's and doctorate degrees in geography and biology, respectively, from the University of Colorado in 1997. He served as a postdoctoral fellow in the Department of Geological and Environmental Sciences at Stanford University until he joined the