The Earth Observing System (EOS) is the major element in the National
Aeronautic and Space Administration's Mission to Planet Earth. It will
be a 15-year-long mission, employing space-based instrumentation and
in situ measurements to provide a long-term, contiguous, calibrated, a
nd validated data set that addresses geophysical and biochemical pheno
mena occurring in the Earth system. The EOS suite of satellites includ
es sun-synchronous, polar-orbiting spacecraft with morning or afternoo
n equator-crossing times. The EOS-AM series, the first of which is sla
ted for launch in June 1998, will address geophysical and biogeochemic
al processes occurring at or near the Earth's surface; the EOS-PM plat
forms will address atmospheric phenomena, including the interaction be
tween clouds and radiation. Synergy and complementarity within and bet
ween these and other platforms will play a major role in acquiring hig
h-quality data. We discuss the following instruments: Moderate Resolut
ion Imaging Spectroradiometer (MODIS), Advanced Spaceborne Thermal Emi
ssion and Reflection Radiometer (ASTER), Multifrequency Imaging Microw
ave Radiometer (MIMR), Multiangle Imaging Spectroradiometer (MISR), an
d Atmospheric Infrared Sounder/Advanced Microwave Sounding Unit/Microw
ave Humidity Sounder) (AIRS/AMSU/MHS). Instrument heritage, design, ca
pabilities, and realization are discussed in terms of satisfying scien
tific requirements. We also discuss the synergy resulting from cross-c
alibration of the instruments and validation of their resulting data p
roducts.