News / Updates

Odyssey Space Joins Landolt Astrophysics Calibration Mission

Apr 18, 2025 | Mission Support

Landolt mission calibration concept

Odyssey Space joins the Landolt astrophysics calibration mission led by GMU with NASA partners.

Support includes mission architecture, instrumentation analysis, and coordination across technical teams.

Odyssey Space is supporting technical milestones associated with the Landolt astrophysics calibration mission led by George Mason University in collaboration with partners at NASA Goddard Space Flight Center and the broader astrophysics community. The mission is designed to advance high-precision photometric calibration capabilities that will support the next generation of space observatories and astronomical surveys.

Odyssey Space is contributing mission architecture support, instrumentation analysis, and coordination across technical teams developing key elements of the mission concept. The work includes early system trade studies, instrument performance modeling, and integration considerations necessary to ensure calibration systems achieve the accuracy required by modern astrophysics missions.

The Landolt mission aims to establish a new generation of calibration references in space, improving the precision with which telescopes measure the brightness and spectral properties of stars and galaxies. These calibration capabilities are critical for future observatories studying dark energy, galaxy evolution, and the large-scale structure of the universe.

About the Landolt Mission

The Landolt mission is being developed to create a space-based photometric calibration standard that can support multiple astronomical observatories across the astrophysics community. By providing stable reference measurements from orbit, the mission will help ensure consistent calibration between instruments and surveys operating across different wavelengths and observing platforms.

Odyssey Space supports the mission by contributing mission architecture analysis, instrument integration planning, and technical coordination across partner institutions. The goal is to ensure that calibration systems are engineered from the outset to meet the precision requirements needed for next-generation astrophysics research while maintaining compatibility with future observatory platforms.