In 1903, Carnegie Science established the Desert Botanical Laboratory in Tucson, Arizona—a boundary-pushing interdisciplinary facility that was the precursor to the Department of Plant Biology, now ...

Last week, Carnegie Science brought exoplanetary research to D.C.’s favorite comic convention with a stellar panel titled “Exploring the Science of Sci-Fi Planets.” The session drew an enthusiastic ...

The nature of the first stars (or “popIII” stars), including their IMF, supernovae, and nucleosynthetic yields, remains a key astrophysical mystery. Although JWST has opened up new windows into the ...

There are no planets intermediate in size between Earth and Neptune in our Solar System, yet these objects are found around a substantial fraction of other stars1. Population statistics show that ...

Ten takeaways from "The New Golden Age of Astronomy: Hubble’s Universe Today" celebrating the 100th anniversary of Edwin Hubble’s groundbreaking discovery that our galaxy isn’t alone in the universe.

The Drosophila Gateway™ Vector collection is a set of 68 Gateway-based vectors designed to express epitope-tagged proteins in Drosophila culture cells or flies. At its core is Invitrogen's Gateway™ ...

Carnegie Science empowers our investigators to pursue the biggest questions of our time, advancing discoveries that transform our understanding of life, planets, and the broader universe. Our research ...

Minerals are information-rich materials that offer researchers a glimpse into the evolution of planetary bodies. Thus, it is important to extract, analyze, and interpret this abundance of information ...

How to achieve net zero emissions goals. Over the past few years, a wave of actors–governments at all levels, electric utilities, companies, and educational institutions–have set targets to reach net ...

Responses of the terrestrial biosphere to rapidly changing environmental conditions are a major source of uncertainty in climate projections. In an effort to reduce this uncertainty, a wide range of ...

Feiite (Fe3TiO5) is a high-pressure Fe-Ti oxide mineral recently discovered in martian meteorite Shergotty. Feiite is isostructural with Fe4O5, a high-pressure iron oxide stable at pressures >10 GPa.