Acquiring Spectra of Solar System Objects with the NIRSpec Instrument on the James Webb Space Telescope

International audienceThe NIRSpec Instrument on the James Webb Space Telescope will allow near-IR spectroscopy in the wavelength range between 0.6 and 5.3 microns with resolving power of ~100, 1000, or 2700. We review strategies for performing spectral observations of solar system objects using each of NIRSpec's available observing modes, including the integral field unit (IFU), multi-Object Spectroscopy (MOS), and fixed slit (FS) templates, and discuss how the choice of mode affects the limiting target brightness as well as the detailed wavelength and spatial coverage obtained. We also discuss the expected pointing accuracy and target acquisition options for moving targets, including the use and limitations of the Wide Aperture Target Acquisition (WATA) capability and of the pre-defined field points that will be available for use with the MOS template to enable the use of custom micro-shutter patterns including ones emulating very long slits