Lunar sourcebook. A user's guide to the moon

The Dawn spacecraft targeted 4 Vesta, believed to be a remnant intact protoplanet from the earliest epoch of solar system formation, based on analyses of howardite-eucrite-diogenite (HED) meteorites that indicate a differentiated parent body. Dawn observations reveal a giant basin at Vesta's south pole, whose excavation was sufficient to produce Vesta-family asteroids (Vestoids) and HED meteorites. The spatially resolved mineralogy of the surface reflects the composition of the HED meteorites, confirming the formation of Vesta's crust by melting of a chondritic parent body. Vesta's mass, volume, and gravitational field are consistent with a core having an average radius of 107 to 113 kilometers, indicating sufficient internal melting to segregate iron. Dawn's results confirm predictions that Vesta differentiated and support its identification as the parent body of the HEDs.

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Dawn at Vesta: Testing the Protoplanetary Paradigm

In hyperspectral unmixing, the prevalent model used is the linear mixing model, and a large variety of techniques based on this model has been proposed to obtain endmembers and their abundances in hyperspectral imagery. However, it has been known for some time that nonlinear spectral mixing effects can be a crucial component in many real-world scenarios, such as planetary remote sensing, intimate mineral mixtures, vegetation canopies, or urban scenes. While several nonlinear mixing models have been proposed decades ago, only recently there has been a proliferation of nonlinear unmixing models and techniques in the signal processing literature. This paper aims to give an historical overview of the majority of nonlinear mixing models and nonlinear unmixing methods, and to explain some of the more popular techniques in detail. The main models and techniques treated are bilinear models, models for intimate mineral mixtures, radiosity-based approaches, ray tracing, neural networks, kernel methods, support vector machine techniques, manifold learning methods, piece-wise linear techniques, and detection methods for nonlinearity. Furthermore, we provide an overview of several recent developments in the nonlinear unmixing literature that do not belong into any of these categories.

A Review of Nonlinear Hyperspectral Unmixing Methods

In May of 2011, NASA selected the Origins, Spectral Interpretation, Resource Identification, and Security–Regolith Explorer (OSIRIS-REx) asteroid sample return mission as the third mission in the New Frontiers program. The other two New Frontiers missions are New Horizons, which explored Pluto during a flyby in July 2015 and is on its way for a flyby of Kuiper Belt object 2014 MU69 on January 1, 2019, and Juno, an orbiting mission that is studying the origin, evolution, and internal structure of Jupiter. The spacecraft departed for near-Earth asteroid (101955) Bennu aboard an United Launch Alliance Atlas V 411 evolved expendable launch vehicle at 7:05 p.m. EDT on September 8, 2016, on a seven-year journey to return samples from Bennu. The spacecraft is on an outbound-cruise trajectory that will result in a rendezvous with Bennu in November 2018. The science instruments on the spacecraft will survey Bennu to measure its physical, geological, and chemical properties, and the team will use these data to select a site on the surface to collect at least 60 g of asteroid regolith. The team will also analyze the remote-sensing data to perform a detailed study of the sample site for context, assess Bennu’s resource potential, refine estimates of its impact probability with Earth, and provide ground-truth data for the extensive astronomical data set collected on this asteroid. The spacecraft will leave Bennu in 2021 and return the sample to the Utah Test and Training Range (UTTR) on September 24, 2023.

OSIRIS-REx: Sample Return from Asteroid (101955) Bennu

BepiColombo—Comprehensive exploration of Mercury: Mission overview and science goals

Final Calibration and Multispectral Map Products from the Mercury Dual Imaging System Wide-Angle Camera

An Examination of Several Discrete Lunar Nearside Photometric Anomalies Observed in Lyman‐α Maps

Updated Absolute Age Estimates for the Tolstoj and Caloris Basins, Mercury

A New Global Map of Light Plains from the Lunar Reconnaissance Orbiter Camera

WIDESPREAD SMALL-SCALE VOLATILE COLD TRAPS. David A. Paige, Paul. O. Hayne, Matthew A. Siegler, David E. Smith, Maria T. Zuber, Gregory A. Neumann, Erwan M. Mazarico, Brett W. Denevi, Sean C. Solomon. Department of Earth, Planetary and Space Sciences, UCLA, Los Angeles, CA 90095, dap@moon.ucla.edu; Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109; Department of Earth, Atmospheric and Planetary Sciences, MIT, Cambridge, MA 02139; NASA Goddard Space Flight Center, Greenbelt, MD 20771; Johns Hopkins University Applied Physics Laboratory, Laurel, MD 20723; Lamont-Doherty Earth Observatory, Columbia University, Palisades, NY 10964; Department of Terrestrial Magnetism, Carnegie Institution of Washington, Washington, DC 20015.

Brett W. Denevi

Papers

Final Calibration and Multispectral Map Products from the Mercury Dual Imaging System Wide-Angle Camera

An Examination of Several Discrete Lunar Nearside Photometric Anomalies Observed in Lyman‐α Maps

Updated Absolute Age Estimates for the Tolstoj and Caloris Basins, Mercury

A New Global Map of Light Plains from the Lunar Reconnaissance Orbiter Camera

Dark Surface Deposits in the North Polar Region of Mercury: Evidence for Widespread Small-Scale Volatile Cold Traps