Suggested Searches

 

ROSES-25 Amendment 40: Exoplanets Research Program Step-2 Due Date Deferred to February 2, 2026

23 January 2026

The Exoplanets Research Program (XRP), element F.3 of ROSES-25, solicits basic research proposals to conduct scientific investigations that significantly improve our understanding of exoplanets and exoplanet formation. This program element is cross-divisional and jointly managed by three of the Divisions within NASA’s Science Mission Directorate: Astrophysics, Planetary Science, and Heliophysics. Proposed investigations that combine multiple scientific disciplines or cross traditional Divisional science boundaries, for example, by including topics or analysis techniques from Heliophysics, are highly encouraged.

ROSES-2025 Amendment 40 defers the Step-2 due date for F.3 XRP to February 2, 2026.

On or about January 22, 2026, this Amendment to the NASA Research Announcement "Research Opportunities in Space and Earth Sciences (ROSES) 2025" (NNH25ZDA001N) will be posted on the NASA research opportunity homepage at https://solicitation.nasaprs.com/ROSES2025 and will appear on SARA's ROSES blog at: https://science.nasa.gov/researchers/solicitations/roses-2025/

Questions concerning F.3 XRP may be directed to the XRP program officers at hq-xrp@mail.nasa.gov.

News Straight to Your Inbox

Subscribe to your community email news list

We will never share your email address.

Privacy Policy

Sign Up
Angled from the upper left corner to the lower right corner is a cone-shaped orange-red cloud known as Herbig-Haro 49/50. This feature takes up about three-fourths of the length of this angle. The upper left end of this feature has a translucent, rounded end. The conical feature widens slightly from the rounded end at the upper right down to the lower right. Along the cone there are additional rounded edges, like edges of a wave, and intricate foamy-like details, as well as a clearer view of the black background of space. In the upper left, overlapping with the rounded end of Herbig-Haro 49/50, is a background spiral galaxy with a concentrated blue center that fades outward to blend with red spiral arms. The background of space is speckled with some white stars and smaller, more numerous, fainter white galaxies throughout.