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Petition for Cosmic Pathfinders Chapter

26 November 2024

Members of the program who are at the same university or institution may self-organize into chapters upon completion of NASA Cosmic Pathfinders (NASA CPP) chapter petition form and required materials. Such groups further galvanize the engagement of students with NASA astrophysics. Chapters are modeled after similar campus organizations (e.g., Society of Physics Students, NSBE, SACNAS, etc). Chapters may host regular meetings to discuss relevant prevailing academic and professional issues and focus on developing essential scientific, mathematical, and interdisciplinary skills. They present a unique opportunity for students to connect with a national network of astronomers, astrophysicists, and space scientists, and foster a sense of belonging within the larger scientific community.

Students and early-careers interested in a NASA CPP chapter must fill out the NASA Cosmic Pathfinders Program Statement of Interest Form BEFORE chapter approval.

Interested students, early-careers in STEM, and professionals can interface and join the dedicated LinkedIn group here to further connect with others: NASA Cosmic Pathfinders LinkedIn Group

Follow the link for more information about the program.

Reach out to Dr. Ronald Gamble (ronald.s.gamble@nasa.gov) or the Leadership Council for further inquiries or questions.

NASA Cosmic Pathfinders Program Early-Career Leaders 2024 – 2025

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An illustration of Sun-like star HD 181327 and its surrounding debris disk. The star is at top right. It is surrounded by a far larger debris disk that forms an incomplete ellpitical path and is cut off at right. There’s a huge cavity between the star and the disk. The debris disk is shown in shades of light gray. Toward the top and left, there are finer, more discrete points in a range of sizes. The disk appears hazier and smokier at the bottom. The star is bright white at center, with a hazy blue region around it. The background of space is black. The label Artist's Concept appears at lower left.