Jo. Goldsten et al., THE X-RAY GAMMA-RAY SPECTROMETER ON THE NEAR-EARTH ASTEROID RENDEZVOUS MISSION/, Space science reviews, 82(1-2), 1997, pp. 169-216
An X-ray/gamma-ray spectrometer has been developed as part of a rendez
vous mission with the near-Earth asteroid, 433 Eros, in an effort to a
nswer fundamental questions about the nature and origin of asteroids a
nd comets. During about 10 months of orbital operations commencing in
early 1999, the X-ray/Gamma-ray Spectrometer will develop global maps
of the elemental composition of the surface of Eros. The instrument re
motely senses characteristic X-ray and gamma-ray emissions to determin
e composition. Solar excited X-ray fluorescence in the 1 to 10 keV ran
ge will be used to measure the surface abundances of Mg, Al, Si, Ca, T
i, and Fe with spatial resolutions down to 2 km. Gamma-ray emissions i
n the 0.1 to 10 MeV range will be used to measure cosmic-ray excited e
lements O, Si, Fe, H and naturally radioactive elements K, Th, U to su
rface depths on the order of 10 cm. The X-ray spectrometer consists of
three gas filled proportional counters with a collimated field of vie
w of 5 degrees and an energy resolution of 850 eV @ 5.9 keV. Two sunwa
rd looking X-ray detectors monitor the incident solar flux, one of whi
ch is the first flight of a new, miniature solid-state detector which
achieves 600 eV resolution @ 5.9 keV. The gamma-ray spectrometer consi
sts of a NaI(Tl) scintillator situated within a Bismuth Germanate (BGO
) cup, which provides both active and passive shielding to confine the
held of view and eliminate the need for a massive and costly boom. Ne
w coincidence techniques enable recovery of single and double escape e
vents in the central detector. The NaI(Tl) and BGO detectors achieve e
nergy resolutions of 8.7% and 14%, respectively @ 0.662 MeV. A data pr
ocessing unit based on an RTX2010 microprocessor provides the spacecra
ft interface and produces 256-channel spectra for X-ray detectors and
1024-channel spectra for the raw, coincident, and anti-coincident gamm
a-ray modes. This paper presents a detailed overview of the X-ray/Gamm
a-ray Spectrometer and describes the science objectives, measurement o
bjectives, instrument design, and shows some results from early in-fli
ght data.