Earth scientist Robert Hazen has an unusually rich research portfolio. He is trying to understand the carbon cycle from deep inside the Earth; chemical interactions at crystal-water interfaces; the interactions of organic molecules on mineral surfaces as a possible springboard to life; how life arose from the chemical to the biological world; how life emerges in extreme environments; and the origin and distribution of life in the universe  just to name a few topics. In tandem with this expansive Carnegie work, he is also the Clarence Robinson Professor of Earth Science at George Mason University. He has authored more than 350 articles and 20 books on science, history, and music.

 As principal investigator of the Deep Carbon Observatory, Hazen oversees the primary mission of work to promote the transformational understanding of the chemical and biological roles of carbon in Earth's interior—a program in part supported by the Sloan Foundation.

Astrobiology is the search for the origin, distribution, and future of life in the universe. Hazen and the Carnegie team have explored the hypothesis that hydrothermal systems on planets and moons might have contributed to the formation of organic molecules, and thus the origin of life, and they have looked at the cosmochemistry of carbon, the essential element of life.

In work on mineral-molecule interactions, it turns out that the origin of life’s biochemicals have “handedness,” like left and right handiness in people. Hazen and team believe that these so-called chiral mineral surfaces may have played a significant role in the selection and concentration of molecules necessary for life.

Although minerals are necessary for essential tasks, science has assumed that the mineral species found on Earth today are much the same as they were during Earth’s first 550 million years—the Hadean Eon—when life emerged. Hazen found this not to be true. He compiled a list of every plausible mineral species on the Hadean Earth and concludes that no more than 420 different minerals—about 8 percent of the nearly 5,000 species found on Earth today—would have been present at or near Earth’s surface.

 Field observations of microbes recovered from deep drill cores, deep mines, and the ocean floor, coupled with laboratory investigations, reveal that microbial life can exist at conditions of extreme temperatures (to above 110ºC) and pressures (to > 10,000 atmospheres) previous thought impossible. Hazen is interested in research on microbes at such extreme conditions. He also explores the factors that promote the emergence of complex evolving systems.

Hazen received both has B.S. and  S.M in Earth science from MIT and his Ph. D. from Harvard University ,where he was also a research assistant and teaching fellow. He joined the scientific staff at Carnegie in 1978. For more see http://hazen.gl.ciw.edu/

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Illustration of Neptune's interior purchased from Shutterstock
October 14, 2021

Washington, DC—A layer of “hot,” electrically conductive ice could be responsible for generating the magnetic fields of ice giant planets like Uranus and Neptune. New work from Carnegie and the University of Chicago’s Center for Advanced Radiation Sources reveals the conditions under which two such superionic ices form. Their findings are published in Nature Physics. 

As all school children learn, water molecules are made up of two hydrogen atoms and one oxygen atom—H20. As the conditions in which water exists change, the organization and properties of these molecules are affected. We can see this in our everyday lives when liquid water is boiled

Peter van Keken
September 30, 2021

Washington, DC— Carnegie geophysicist and geodynamicist Peter van Keken, whose work reveals Earth’s thermal and chemical evolution, was elected a Fellow of the American Geophysical Union.

The AGU is an international nonprofit scientific association with 60,000 members in 137 countries. Only one out of every thousand members are selected each year. The 2021 cohort was chosen for their “outstanding achievements and contributions by pushing the frontiers of our science forward,” according to AGU, as well as for embodying the organization’s “shared vision of a thriving, sustainable, and equitable future for all powered by discovery, innovation, and

Carnegie Earth and Planets Laboratory isotope geochemist Anat Shahar
September 10, 2021

Washington, DC—Carnegie geochemist Anat Shahar, who probes the formation, evolution, and interior dynamics of Earth and other rocky planets, has been selected to give the Reginald Daly Lecture at the American Geophysical Union’s annual Fall Meeting in December.  

In honor of its namesake’s contributions to understanding the forces that shaped our planet, recipients for this recognition are selected for exemplifying excellence in the geosciences.

Earth and Planets Laboratory Staff Scientist Anat Shahar, also the institution’s Associate Science Deputy, uses a combination of isotope geochemistry and high-pressure, high-temperature experiments to

Diana Roman collecting samples, courtesy of Anna Barth, LDEO.
September 1, 2021

Washington, DC—Our planet provides ample research opportunities for scientists like Diana Roman, who has devoted her career to understanding the geologic forces that shape volcanic eruptions. She just needs to be on standby to seize them when they arrive.

Roman, recently named a Harry Oscar Wood Chair of Seismology at the Carnegie Institution for Science, wasn’t initially planning to travel to Iceland to get a look at the Fagradalsfjall “baby” volcano—in Geldingadalir—which erupted onto the scene in the Reykjanes Peninsula just this past March, mesmerizing the world with images of its cascading lava and “science fair”-style cone.

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Established in June of 2016 with a generous gift of $50,000 from Marilyn Fogel and Christopher Swarth, the Marilyn Fogel Endowed Fund for Internships will provide support for “very young budding scientists” who wish to “spend a summer getting their feet wet in research for the very first time.”  The income from this endowed fund will enable high school students and undergraduates to conduct mentored internships at Carnegie’s Geophysical Laboratory and Department of Terrestrial Magnetism in Washington, DC starting in the summer of 2017.

Marilyn Fogel’s thirty-three year career at Carnegie’s Geophysical Laboratory (1977-2013), followed

CALL FOR PROPOSALS

Following Andrew Carnegie’s founding encouragement of liberal discovery-driven research, the Carnegie Institution for Science offers its scientists a new resource for pursuing bold ideas.

Carnegie Science Venture grants are internal awards of up to $100,000 that are intended to foster entirely new directions of research by teams of scientists that ignore departmental boundaries. Up to six adventurous investigations may be funded each year. The period of the award is two

Andrew Steele joins the Rosetta team as a co-investigator working on the COSAC instrument aboard the Philae lander (Fred Goesmann Max Planck Institute - PI). On 12 November 2014 the Philae system will be deployed to land on the comet and begin operations. Before this, several analyses of the comet environment are scheduled from an approximate orbit of 10 km from the comet. The COSAC instrument is a Gas Chromatograph Mass Spectrometer that will measure the abundance of volatile gases and organic carbon compounds in the coma and solid samples of the comet.

The Anglo-Australian Planet Search (AAPS) is a long-term program being carried out on the 3.9-meter Anglo-Australian Telescope (AAT) to search for giant planets around more than 240 nearby Sun-like stars. The team, including Carnegie scientists,  uses the "Doppler wobble" technique to search for these otherwise invisible extra-solar planets, and achieve the highest long-term precision demonstrated by any Southern Hemisphere planet search.

Ana Bonaca is Staff Member at Carnegie Observatories. Her specialty is stellar dynamics and her research aims to uncover the structure and evolution of our galaxy, the Milky Way, especially the dark matter halo that surrounds it. In her research, she uses space- and ground-based telescopes to measure the motions of stars, and constructs numerical experiments to discover how dark matter affected them.

She arrived in September 2021 from Harvard University where she held a prestigious Institute for Theory and Computation Fellowship. 

Bonaca studies how the uneven pull of our galaxy’s gravity affects objects called globular clusters—spheres made up of a million

Peter Gao's research interests include planetary atmospheres; exoplanet characterization; planet formation and evolution; atmosphere-surface-interior interactions; astrobiology; habitability; biosignatures; numerical modeling.

His arrival in September 2021 continued Carnegie's longstanding tradition excellence in exoplanet discovery and research, which is crucial as the field prepares for an onslaught of new data about exoplanetary atmospheres when the next generation of telescopes come online.

Gao has been a part of several exploratory teams that investigated sulfuric acid clouds on Venus, methane on Mars, and the atmospheric hazes of Pluto. He also

Anne Pommier's research is dedicated to understanding how terrestrial planets work, especially the role of silicate and metallic melts in planetary interiors, from the scale of volcanic magma reservoirs to core-scale and planetary-scale processes.

She joined Carnegie in July 2021 from U.C. San Diego’s Scripps Institution of Oceanography, where she investigated the evolution and structure of planetary interiors, including our own Earth and its Moon, as well as Mars, Mercury, and the moon Ganymede.

Pommier’s experimental petrology and mineral physics work are an excellent addition to Carnegie’s longstanding leadership in lab-based mimicry of the

Johanna Teske became the first new staff member to join Carnegie’s newly named Earth and Planets Laboratory (EPL) in Washington, D.C., on September 1, 2020. She has been a NASA Hubble Fellow at the Carnegie Observatories in Pasadena, CA, since 2018. From 2014 to 2017 she was the Carnegie Origins Postdoctoral Fellow—a joint position between Carnegie’s Department of Terrestrial Magnetism (now part of EPL) and the Carnegie Observatories.

Teske is interested in the diversity in exoplanet compositions and the origins of that diversity. She uses observations to estimate exoplanet interior and atmospheric compositions, and the chemical environments of their formation