PDS_VERSION_ID = PDS3 RECORD_TYPE = UNDEFINED ^ASCII_DOCUMENT = "NIS.ASC" ^ADOBE_PDF_DOCUMENT = "NIS.PDF" OBJECT = ASCII_DOCUMENT DOCUMENT_NAME = "THE NEAR INFRARED SPECTROMETER" DOCUMENT_TOPIC_TYPE = "INSTRUMENT DESCRIPTION" INTERCHANGE_FORMAT = ASCII DOCUMENT_FORMAT = TEXT PUBLICATION_DATE = 1998 DESCRIPTION = "This provides an overview of the Near Infrared Spectrometer" END_OBJECT = ASCII_DOCUMENT OBJECT = ADOBE_PDF_DOCUMENT DOCUMENT_NAME = "THE NEAR INFRARED SPECTROMETER" DOCUMENT_TOPIC_TYPE = "INSTRUMENT DESCRIPTION" INTERCHANGE_FORMAT = BINARY DOCUMENT_FORMAT = ADOBE_PDF PUBLICATION_DATE = 1998 DESCRIPTION = "This provides and overview of the Near Infrared Spectrometer" ABSTRACT_TEXT = " The Near Infrared Spectrometer (NIS) instrument will map the spectral prop- erties of asteroid 433 Eros in the range 800-2600 nm to determine its mineral content. Optically, NIS uses a scan mirror and an imaging mirror to project an image at a field stop. A grating spectrometer disperses the energy, and a dichroic beamsplitter separates two spectral orders, reflecting the short wavelengths (816-1500 nm) to a 32-element Ge detector, and transmitting the long wavelengths (1500-2600 nm) to a 32-element InGaAs detector. The spectral resolutions are 22 and 44 nm for the second and first spectral orders, respectively. A scan mirror rotates the field of view over a 140 degree range that includes a solar-illuminated calibration target. Spectra are measured at 1 Hz using a selection of data acquisition macros. The properties of the instrument were extensively measured during on-ground calibration, and in-flight calibration was begun shortly after launch. The NIS will observe Eros during approach to the asteroid and will produce composition maps of the entire illuminated surface at spatial resolutions as high as 300 m. " END_OBJECT = ADOBE_PDF_DOCUMENT END