for 51 Pegasi b Science Summit expenses

for the 1400 Degrees convenings

to fund the annual 51 Pegasi b Fellowship review process

for scientific convenings and roundtables organized by the Foundation in 2024-2025

to support the 2025 51 Pegasi b Summit

for professional development

for the 1400 Degrees convenings

for general support

for general support

for general support ($150,000) and for the development of the Spotlights multimedia project ($50,000)

for general support

for general support

for general support

for general support

for general support

for general support

to support the Agua Salud Project, an ecosystem-services experiment in the Panama Canal

to support timely ecological field measurements in secondary tropical forests

to provide tutor salaries for Onaketa

to support Science News’ increased coverage of COVID-19

to support the Science News Century of Science physics and astronomy coverage and Century of Science Virtual Conference

to support the expansion of the Science News’ coverage of physics and astronomy

to support the Science News’ coverage of physics and astronomy

to support content for the 1400 Degrees Website

to assess water world habitability using liquid phase ocean chemistry & atmospheric photochemistry

to investigate how volcanic rocks contribute to chemical evolution in a prebiotic environment

for 28 nights of observing time on the Anglo-Australian Telescope to complete the Satellites Around Galactic Analogs survey

for remastering archival radar film of the Greenland ice sheet

for retaining undergraduate women in physics through research and community building

for modeling the atmospheric evolution of planets orbiting flaring M dwarf stars

to fund activities during Phase 1 of the Cosmic Axion Spin Precession Experiment (CASPEr), a search for ultra-light dark matter particles such as axions and dark photons

to support a workshop on precision measurement devices to study high energy physics in laboratory-scale experiments

for the acquisition and installation of an oxygen isotope ratio mass spectrometer system

for the optimization of a single-beam optically-levitated microsphere force-sensor for short-distance gravity experiments

for equipment and initial development of the Dark Matter Radio search for ultra-light axions and hidden photons

for the Physics and Astronomy Leadership Council

for the construction and operation of the Phase I Dark Matter Radio experiment

to support the inaugural Global Energy Forum at Stanford University

for studying how AMO physics can inform the development of gravity theories

for the Physics and Astronomy Leadership Council

to search for and characterize closely-separated binary systems of super massive black holes

for research on the formation and evolution of gas giant planets

to retrieve and analyze microbes from atop Earth’s largest tropical glacier

for #BlackInAstro

for modeling chemistry, heat transfer, and material fluxes at the sea floor of Waterworld oceans.

to support the development of a comprehensive proxy-focused model of how marine sediment cores accumulate and change over millennial time scales to form the observed geological record

to support the development and application of data assimilation techniques in paleoclimate deep time

for a week-long workshop introducing participants to numerical modeling of the Earth’s climate and environmental systems

to support the development of novel algorithms and computational tools for high precision radial velocity measurements in the near-infrared wavelengths

for engineering analysis, instrumentation upgrades, and logistics planning for a network of glacier monitoring sensors in Greenland