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ROSES-24 Amendment 29: New Opportunity D.20 Exoplanet Mass Measurement Program

D.20 Exoplanet Mass Measurement Program (EMMP) solicits investigations that will identify and mitigate systematics that currently limit the precision of radial velocity or astrometry observations from measuring the masses of temperate terrestrial planets orbiting Sun-like stars. Proposed investigations should advance tools, techniques, and understanding to extract small Keplerian signals buried in complex time-series stellar spectra or astrometric measurements. Proposed investigations may involve theory, observation, analysis of archival data, or a combination of these approaches

ROSES-2024 Amendment 29 releases final text and due dates for D.20 EMMP. Mandatory NOIs are due January 23, 2025, and proposals are due February 26, 2025.

On or about July 12, 2024, this Amendment to the NASA Research Announcement "Research Opportunities in Space and Earth Sciences (ROSES) 2024" (NNH24ZDA001N) will be posted on the NASA research opportunity homepage and will appear on SARA's ROSES blog.

Questions concerning D.20 EMMP may be directed to Hannah Jang-Condell at hannah.jang-condell@nasa.gov.

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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.