John Mulchaey and Yixian Zheng named interim co-presidents

Carnegie Observatories Director John Mulchaey and Carnegie Embryology Director Yixian Zheng jointly will serve in the Office of the President on an interim basis starting January 1, 2018. Their selection as interim co-presidents was a unanimous decision of the Carnegie Board of Trustees. 

Explore this Story

Give to Carnegie

You Can Support Scientific Discovery.

Learn More

WASHINGTON, D.C. – US2020, a  nationwide network of more than 350 organizations to advance the STEM (Science, Technology, Engineering and Math) fields, chose the DC STEM Network as one of 15 finalists for the STEM Coalition Challenge.  Ninety-two partner networks, working to advance STEM mentoring and learning to underrepresented students, competed.

Explore this Story

Without eyes, ears, or a central nervous system, plants can perceive the direction of environmental cues and respond to ensure their survival. For example, roots need to extend through the maze of nooks and crannies in the soil toward sources of water and nutrients. The various ways that plants guide this branching to take advantage of their environment is of great interest to scientists and of potential use by farmers in need of crops that produce more food with fewer resources.

Explore this Story

How far away is that galaxy? 

Our entire understanding of the Universe is based on knowing the distances to other galaxies, yet this seemingly-simple question turns out to be fiendishly difficult to answer. The best answer came more than 100 years ago from an astronomer who was mostly unrecognized in her time—and last year a Carnegie Observatories summer student made those distance measurements more precise than ever. 

Explore this Story

Stay Connected

Sign Up to Receive Carnegie Communications. 

If you are interested in receiving any of our materials, learn more

Astronomers with the Sloan Digital Sky Survey (SDSS), including Carnegie's Johanna Teske, have learned that the chemical composition of a star can exert unexpected influence on its planetary system.

Explore this Story
Carnegie researchers recently constructed genetically encoded FRET sensors for a variety of important molecules such as glucose and glutamate. The centerpiece of these sensors is a recognition element derived from the superfamily of bacterial binding protiens called periplasmic binding protein (...
Explore this Project
The NASA Astrobiology Institute (NAI) Carnegie Team focuses on life’s chemical and physical evolution, from the interstellar medium, through planetary systems, to the emergence and detection of life by studying extrasolar planets, Solar System formation, organic rich primitive planetary bodies,...
Explore this Project
The Fan laboratory studies the molecular mechanisms that govern mammalian development, using the mouse as a model. They use a combination of biochemical, molecular and genetic approaches to identify and characterize signaling molecules and pathways that control the development and maintenance of...
Explore this Project
Capital Science Evening Lectures
Carnegie Science, Carnegie Institution, Carnegie Institution for Science, Julia Clarke, University of Texas
Thursday, March 29, 2018 - 6:30pm to 8:00pm

How do we go beyond the bones to bring dinosaurs to life? Dr. Clarke will explain the new toolkits she uses to  study what dinosaurs might have sounded or looked like when they roamed the Earth....

Explore this Event
Capital Science Evening Lectures
Carnegie Science, Carnegie Institution, Carnegie Institution for Science, Oregon State University, Joy Leighton
Wednesday, April 25, 2018 - 6:30pm to 8:00pm

Can we use the ocean without using it up? The task is daunting given current trajectories in fisheries, plastics, and other pollutants, and the impacts of climate change and ocean acidification. ...

Explore this Event
Capital Science Evening Lectures
Carnegie Science, Carnegie Institution, Carnegie Institution for Science, University of Bristol
Wednesday, May 9, 2018 - 6:30pm to 8:00pm

Looking upward, the vastness of the heavens are accessible through giant telescopes that collect light from the beginning of time. Turn a telescope downward and the opaqueness of our planet...

Explore this Event
John Mulchaey, director of the Observatories, serves as co-interim president of Carnegie as of January 1, 2018. He investigates groups and clusters of galaxies, elliptical galaxies, dark matter—the invisible material that makes up most of the universe—active galaxies and black holes. He is also a...
Meet this Scientist
Peter Driscoll studies the evolution of Earth’s core and magnetic field including magnetic pole reversal. Over the last 20 million or so years, the north and south magnetic poles on Earth have reversed about every 200,000, to 300,000 years and is now long overdue. He also investigates the Earth’s...
Meet this Scientist
Andrew Newman works in several areas in extragalactic astronomy, including the distribution of dark matter--the mysterious, invisible  matter that makes up most of the universe--on galaxies, the evolution of the structure and dynamics of massive early galaxies including dwarf galaxies, ellipticals...
Meet this Scientist

Explore Carnegie Science

January 18, 2018

Washington, DC— Dust is everywhere—not just in your attic or under your bed, but also in outer space. To astronomers, dust can be a nuisance by blocking the light of distant stars, or it can be a tool to study the history of our universe, galaxy, and Solar System.

For example, astronomers have been trying to explain why some recently discovered distant, but young, galaxies contain massive amounts of dust. These observations indicate that type II supernovae—explosions of stars more than ten times as massive as the Sun—produce copious amounts of dust, but how and when they do so is not well understood.

New work from a team of Carnegie cosmochemists published by Science

January 16, 2018

WASHINGTON, D.C. – US2020, a  nationwide network of more than 350 organizations to advance the STEM (Science, Technology, Engineering and Math) fields, chose the DC STEM Network as one of 15 finalists for the STEM Coalition Challenge.  Ninety-two partner networks, working to advance STEM mentoring and learning to underrepresented students, competed. The finalists will compete for $1-million in resources to implement their innovative approaches to STEM teaching and learning.  

The DC STEM Network is a collaboration between the Carnegie Science’s education arm, Carnegie Academy for Science Education (CASE) and the DC Office of the State Superintendent of Education (OSSE). The

Carnegie Science, Carnegie Institution, Carnegie Institution for Science, Stanford University
January 9, 2018

Washington, DC— Without eyes, ears, or a central nervous system, plants can perceive the direction of environmental cues and respond to ensure their survival.

For example, roots need to extend through the maze of nooks and crannies in the soil toward sources of water and nutrients. The various ways that plants guide this branching to take advantage of their environment is of great interest to scientists and of potential use by farmers in need of crops that produce more food with fewer resources.

Carnegie and Stanford University biologist José Dinneny has spent years studying how root growth responds to water, particularly through a phenomenon called hydropatterning, which

January 9, 2018

National Harbor, MD—How far away is that galaxy? 

Our entire understanding of the Universe is based on knowing the distances to other galaxies, yet this seemingly-simple question turns out to be fiendishly difficult to answer. The best answer came more than 100 years ago from an astronomer who was mostly unrecognized in her time—and today, another astronomer has used Sloan Digital Sky Survey (SDSS) data to make those distance measurements more precise than ever. 

"It's been fascinating to work with such historically significant stars," says Kate Hartman, an undergraduate from Pomona College who announced the results at today’s American Astronomical Society (AAS) meeting in

Carnegie Science, Carnegie Institution, Carnegie Institution for Science, Julia Clarke, University of Texas
March 29, 2018

How do we go beyond the bones to bring dinosaurs to life? Dr. Clarke will explain the new toolkits she uses to  study what dinosaurs might have sounded or looked like when they roamed the Earth.

Dr. Julia Clarke: Wilson Professor of Vertebrate Paleontology & HHMI Professor, Jackson School of Geosciences, The University of Texas at Austin

#DinosaurBones

Carnegie Science, Carnegie Institution, Carnegie Institution for Science, Oregon State University, Joy Leighton
April 25, 2018

Can we use the ocean without using it up? The task is daunting given current trajectories in fisheries, plastics, and other pollutants, and the impacts of climate change and ocean acidification.  However, new scientific insights, tools, and partnerships are providing hope that it’s not too late to transition to more-sustainable practices and policies.  Dr. Lubchenco wuill draw on her four years as the Under Secretary of Commerce for Oceans and Atmosphere and the Administrator of the U.S. National Oceanic and Atmospheric Administration (NOAA), her two years as the first U.S. Science Envoy for the Ocean, and her decades of research around the world to summarize the importance to people of

Carnegie Science, Carnegie Institution, Carnegie Institution for Science, University of Bristol
May 9, 2018

Looking upward, the vastness of the heavens are accessible through giant telescopes that collect light from the beginning of time. Turn a telescope downward and the opaqueness of our planet conceals the secrets of its origin and evolution. Diamonds, those translucent rarities, illuminate the depths of our planet and reveal connections between the deep earth and the surface of our planet through both time and space.

Dr. Michael Walter: Incoming Director, Carnegie Geophysical Laboratory

#DiamondScience

Carnegie Science, Carnegie Institution, Carnegie Institution for Science, MIT
June 12, 2018

The direct measurement of gravitational waves predicted by Albert Einstein 100 years ago has open a new field of science – gravitational wave astrophysics and astronomy. The recent discoveries and the prospects for the new field will be presented.

Dr. Rainer Weiss: Emeritus Professor of Physics, MIT, on behalf of the LIGO Scientific Collaboration

#GravitationalWaves

The NASA Astrobiology Institute (NAI) Carnegie Team focuses on life’s chemical and physical evolution, from the interstellar medium, through planetary systems, to the emergence and detection of life by studying extrasolar planets, Solar System formation, organic rich primitive planetary bodies, prebiotic molecular synthesis through catalyzing with minerals, and the connection between planetary evolution to the emergence, and sustenance of biology. This program attempts to integrate the sweeping narrative of life’s history through a combination of bottom-up and top-down studies. On the one hand, this team studies processes related to chemical and physical evolution in plausible prebiotic

The Energy Frontier Research in Extreme Environments Center (EFree) was established to accelerate the discovery and synthesis of kinetically stabilized, energy-related materials using extreme conditions. Partners in this Carnegie-led center include world-leading groups in five universities—Caltech, Cornell, Penn State, Lehigh, and Colorado School of Mines—and will use facilities built and managed by the Geophysical Laboratory at Argonne, Brookhaven, and Oak Ridge National Laboratories. Nine Geophysical Laboratory scientists will participate in the effort, along with Russell Hemley as director and Tim Strobel as associate director.

To achieve their goal, EFree personnel synthesize

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 years,

Anna Michalak’s team combined sampling and satellite-based observations of Lake Erie with computer simulations and determined that the 2011 record-breaking algal bloom in the lake was triggered by long-term agricultural practices coupled with extreme precipitation, followed by weak lake circulation and warm temperatures. The bloom began in the western region in mid-July and covered an area of 230 square miles (600 km2). At its peak in October, the bloom had expanded to over 1930 square miles (5000 km2). Its peak intensity was over 3 times greater than any other bloom on record. The scientists predicted that, unless agricultural policies change, the lake will continue to experience

Peter Driscoll studies the evolution of Earth’s core and magnetic field including magnetic pole reversal. Over the last 20 million or so years, the north and south magnetic poles on Earth have reversed about every 200,000, to 300,000 years and is now long overdue. He also investigates the Earth’s inner core structure; core-mantle coupling; tectonic-volatile cycling; orbital migration—how Earth’s orbit moves—and tidal dissipation—the dissipation of tidal forces between two closely orbiting bodies. He is also interested in planetary interiors, dynamos, upper planetary atmospheres and exoplanets—planets orbiting other stars. He uses large-scale numerical simulations in much of his research

Alan Boss is a theorist and an observational astronomer. His theoretical work focuses on the formation of binary and multiple stars, triggered collapse of the presolar cloud that eventually made  the Solar System, mixing and transport processes in protoplanetary disks, and the formation of gas giant and ice giant protoplanets. His observational works centers on the Carnegie Astrometric Planet Search project, which has been underway for the last decade at Carnegie's Las Campanas Observatory in Chile.

While fragmentation is universally recognized as the dominant formation mechanism for binary and multiple stars, there are still major questions. The most important of these is the

Guillermo Blanc wants to understand the processes by which galaxies form and evolve over the course of the history of the universe. He studies local galaxies in the “present day” universe as well as very distant and therefore older galaxies to observe the early epochs of galaxy evolution. Blanc conducts a series of research projects on the properties of young and distant galaxies, the large-scale structure of the universe, the nature of Dark Energy—the mysterious repulsive force, the process of star formation at galactic scales, and the measurement of chemical abundances in galaxies.

To conduct this work, he takes a multi-wavelength approach including observations in the UV,

Andrew Newman works in several areas in extragalactic astronomy, including the distribution of dark matter--the mysterious, invisible  matter that makes up most of the universe--on galaxies, the evolution of the structure and dynamics of massive early galaxies including dwarf galaxies, ellipticals and cluster. He uses tools such as gravitational lensing, stellar dynamics, and stellar population synthesis from data gathered from the Magellan, Keck, Palomar, and Hubble telescopes.

Newman received his AB in physics and mathematics from the Washington University in St. Louis, and his MS and Ph D in astrophysics from Caltech. Before becomming a staff astronomer in 2015, he was a