Through school visits, public events, an inflatable planetarium, hands-on demonstrations, and Carnegie Observatories’ annual Open House, Outreach Coordinator Jeff Rich is connecting people—especially ...
An interdisciplinary research team from Carnegie, USC, and UC Riverside will work to solve some of cosmology's biggest puzzles thanks to a new $4 million grant from the Templeton Foundation. Pasadena, ...
The 2026 CASSI (Carnegie Astrophysics Summer Student Internship) cohort has arrived! This summer, 16 undergraduate students are joining Carnegie Science's Observatories in Pasadena for 10 weeks of ...
How do diatoms thrive in a wide variety of light conditions? New research reveals a gene, STROBE1, that may contribute to their abililty to succeed across a range of marine environments, including ...
Resources Sequencing Illumina HiSeq 2000 and NextSeq 500 Illumina Adapter Sequences Illumina TruSeq Nano DNA Illumina Nextera XT DNA Illumina TruSeq RNA v2 using Invitrogen SuperScript II RT Illumina ...
Ana Martinez Garcia Carnegie Postdoctoral Fellow Lélia Libon Carnegie Postdoctoral Fellow ...
Debris dust in the habitable zones of stars-otherwise known as exozodiacal dust-comes from extrasolar asteroids and comets and is thus an expected part of a planetary system. Background flux from the ...
Each summer, we invite undergrad students to join our multifaceted internship programs. Interns will contribute to real-life projects in these programs, working alongside our highly accomplished staff ...
Meteoritical Bulletin 109 contains the 2790 meteorites approved by the Nomenclature Committee of the Meteoritical Society in 2020. It includes 17 falls (Al Farciya, Auckland, Cavezzo, Flensburg, ...
Two new polyhydrides of calcium have been synthesized at high pressures and high temperatures and characterized by Raman spectroscopy, infrared spectroscopy, and synchrotron X-ray diffraction. Above ...
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.
The distribution, accumulation and circulation of oxygen and hydrogen in Earth's interior dictate the geochemical evolution of the hydrosphere, atmosphere and biosphere(1). The oxygen-rich atmosphere ...
Results that may be inaccessible to you are currently showing.
Hide inaccessible results