Distribution of Hydrogen in the Near Surface of Mars: Evidence for Subsurface Ice Deposits

@article{Boynton2002DistributionOH,  title={Distribution of Hydrogen in the Near Surface of Mars: Evidence for Subsurface Ice Deposits},  author={William V. Boynton and William Charles Feldman and Steven W. Squyres and Thomas H. Prettyman and Johannes Br{\"u}ckner and Larry G. Evans and R. C. Reedy and Richard D. Starr and James R. Arnold and Darrell M. Drake and Peter A. J. Englert and Albert E. Metzger and Igor G. Mitrofanov and Jack I. Trombka and C. d'Uston and Heinrich W{\"a}nke and Olivier Gasnault and David K. Hamara and Daniel M. Janes and Roberto Marcialis and Sylvestre Maurice and I. Mikheeva and G. Jeffrey Taylor and Robert L. Tokar and C. Shinohara},  journal={Science},  year={2002},  volume={297},  pages={81 - 85},  url={https://api.semanticscholar.org/CorpusID:16788398}}
The Gamma-Ray Spectrometer on the Mars Odyssey has identified two regions near the poles that are enriched in hydrogen, and it is suggested that the host of the hydrogen in the subsurface layer is ice, which constitutes 35 ± 15% of the layer by weight.

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24 References

Global Distribution of Neutrons from Mars: Results from Mars Odyssey

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