Encyclopedia of the Solar System 2nd ed

(Marvins-Underground-K-12) #1
138 Encyclopedia of the Solar System

TABLE 2 MESSENGERInstruments and
Measurements
Instrument Observation

Duel Imaging System (1.5◦
and 10.5◦field of view)

Surface mapping in stereo
(10 color filters)
Gamma-Ray and Neutron
Spectrometer

Surface composition (O, Si,
Fe, H, K)
X-Ray Spectrometer (1– to
10 kKeV)

Surface composition (Mg,
Al, Fe, Si, S, Ca, Ti)
Atmospheric and Surface
Spectrometer

Surface and Exosphere
composition
Magnetometer Magnetic field
Laser Altimeter Topography of northern
hemisphere
Energetic Particles and
Plasma Spectrometer

Energetic particles and
plasma
Radio Science (X-band
transponder)

Gravity field and physical
liberation

necessary to answer most of the questions raised in this
chapter. The Europeans are also planning a Mercury mis-
sion called BepiColombo in the years immediately following
theMESSENGERinvestigations.


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FIGURE 25 This drawing shows the orbit ofMESSENGERin
its 12-hour period. The elliptical orbit is required to maintain an
acceptable operating temperature, and yet still obtain
high-resolution data at and near closest approach. Hp is the
closest approach, Ha is the farthest point in the orbit, and the
orbit is inclined at an angle of 60◦to the equator.

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