Astronomical Observations of Volatiles on Asteroids
arXiv:1502.06442 · doi:10.2458/azu_uapress_9780816532131-ch004
Abstract
We have long known that water and hydroxyl are important components in meteorites and asteroids. However, in the time since the publication of Asteroids III, evolution of astronomical instrumentation, laboratory capabilities, and theoretical models have led to great advances in our understanding of H2O/OH on small bodies, and spacecraft observations of the Moon and Vesta have important implications for our interpretations of the asteroidal population. We begin this chapter with the importance of water/OH in asteroids, after which we will discuss their spectral features throughout the visible and near-infrared. We continue with an overview of the findings in meteorites and asteroids, closing with a discussion of future opportunities, the results from which we can anticipate finding in Asteroids V. Because this topic is of broad importance to asteroids, we also point to relevant in-depth discussions elsewhere in this volume.
Chapter to appear in the (University of Arizona Press) Space Science Series Book: Asteroids IV
References in corpus (7)
- Solar System evolution from compositional mapping of the asteroid belt
- The Compositional Structure of the Asteroid Belt
- ALICE: The Ultraviolet Imaging Spectrograph aboard the New Horizons Pluto-Kuiper Belt Mission
- Visible spectroscopic and photometric survey of Jupiter Trojans: final results on dynamical families
- Comet 17P/Holmes in Outburst: The Near Infrared Spectrum
- Spectroscopic Survey of X-type Asteroids
- The 3 m Spectrum of Jupiter's Irregular Satellite Himalia
Cited by in corpus (17)
- Ammonium salts are a reservoir of nitrogen on a cometary nucleus and possibly on some asteroids
- The Main Belt Comets and Ice in the Solar System
- Connecting Asteroids and Meteorites with visible and near-infrared spectroscopy
- Asteroid Families: properties, recent advances and future opportunities
- Dynamical Evolution and Thermal History of Asteroids (3200) Phaethon and (155140) 2005 UD
- Infrared Spectroscopy of Large, Low-Albedo Asteroids: Are Ceres and Themis Archetypes or Outliers?
- Style and intensity of hydration among C-complex asteroids: a comparison to dessicated carbonaceous chondrites
- Expected spectral characteristics of (101955) Bennu and (162173) Ryugu, targets of the OSIRIS-REx and Hayabusa2 missions
- PRIMASS visits Hilda and Cybele groups
- Water abundance at the surface of C-complex main-belt asteroids
- CASTAway: An Asteroid Main Belt Tour and Survey
- Distant formation and differentiation of outer main belt asteroids and carbonaceous chondrite parent bodies
- How Many Hydrated NEOs Are There?
- Fates of hydrous materials during planetesimal collisions
- Bennu's global surface and two candidate sample sites characterized by spectral clustering of OSIRIS-REx multispectral images
- Spectroscopic and dynamical properties of comet C/2018 F4, likely a true average former member of the Oort cloud
- Spectral clustering tools applied to Ceres in preparation for OSIRIS-REx color imaging of asteroid (101955) Bennu