The OSIRIS-REx Visible and InfraRed Spectrometer (OVIRS): Spectral Maps of the Asteroid Bennu
arXiv:1703.10574 · doi:10.1007/s11214-018-0482-9
Abstract
The OSIRIS-REx Visible and Infrared Spectrometer (OVIRS) is a point spectrometer covering the spectral range of 0.4 to 4.3 microns (25,000-2300 cm-1). Its primary purpose is to map the surface composition of the asteroid Bennu, the target asteroid of the OSIRIS-REx asteroid sample return mission. The information it returns will help guide the selection of the sample site. It will also provide global context for the sample and high spatial resolution spectra that can be related to spatially unresolved terrestrial observations of asteroids. It is a compact, low-mass (17.8 kg), power efficient (8.8 W average), and robust instrument with the sensitivity needed to detect a 5% spectral absorption feature on a very dark surface (3% reflectance) in the inner solar system (0.89-1.35 AU). It, in combination with the other instruments on the OSIRIS-REx Mission, will provide an unprecedented view of an asteroid's surface.
arXiv comment14 figures, 3 tables, Space Science Reviews, submitted
References in corpus (2)
Cited by in corpus (8)
- OSIRIS-REx: Sample Return from Asteroid (101955) Bennu
- OCAMS: The OSIRIS-REx Camera Suite
- Phase reddening on asteroid Bennu from visible and near-infrared spectroscopy
- Grain Size Effects on UV-MIR (0.2-14 micron) Spectra of Carbonaceous Chondrite Groups
- Widely distributed exogenic materials of varying compositions and morphologies on asteroid (101955) Bennu
- Bennu's global surface and two candidate sample sites characterized by spectral clustering of OSIRIS-REx multispectral images
- Characterization of Exogenic Boulders on Near-Earth Asteroid (101955) Bennu from OSIRIS-REx Color Images
- Detection of a 2.85 micrometer Feature on 5 Spinel-rich Asteroids from JWST