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 ...

This winter, a delegation from Dallas’ Perot Museum of Nature and Science visited Carnegie Science’s Las Campanas Observatory, deepening a programmatic partnership that shared the wonders of the Great ...

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.

Join us Thursday mornings throughout October for seminars on the theme of redox controls on planetary processes. Continuing the series Vincenzo Stagno of Università di Roma will present, "Redox and ...

In the first Neighborhood Lecture of 2025, Carnegie Science welcomed its 12th President, John Mulchaey, to its Broad Branch Road campus for a journey through 100 years of astrophysical breakthroughs.

10 Things We Learned About the Universe from John Mulchaey’s Neighborhood Lecture Postdoctoral alumna Jo Ann Eder is committed to making the world a better place by supporting organizations, like ...

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 ...

Colloquium: Hydrogen Gas in Galaxies Over One-Third the Age of the Universe (z = 0 to 0.5) With CHILES ...