D/H ratios of water and organics in meteorites, comets, and the Saturnian system

This is a collection of D/H isotopic ratios for meteorites, interplanetary dust particles, comets, Jupiter, and the Saturnian system (Saturn, Rhea, Titan, Hyperion, Iapetus, Saturn's B ring, and Enceladus). D/H ratios were distinguished based on the source molecule (H2, ammonia, water, methane, organic, or bulk measurements). Most of the data is from organic, water, and bulk measurements. Values reported as δD (‰) in the original publication were converted to D/H using VSMOW standard (D/H = 0.00015576) and are identified in the spreadsheet. This data was used to generate Fig. 2 in a manuscript under revision at JGR Planets: "A Roadmap for the Exploration of Enceladus" by Laura E. Rodriguez, Jessica M. Weber, Morgan L. Cable, Laura M. Barge, Julie C. Castillo-Rogez, Mark Chodas, Sierra N. Ferguson, Paul M. Schenk, Steven D. Vance, Kalind Carpenter, Michel D. Ingham, Corey J. Cochrane, Catherine M. Elder, Bryana L. Henderson, Sona Hosseini, Angela G. Marusiak, Aaron C. Noell, Scott M. Perl, and Masahiro Ono.