Because comets and asteroids are relatively unchanged leftovers from the solar system
formation process, it is important to discern their structures and chemical makeup. These
objects formed under the same conditions as did the planets, but unlike the planets, they
remained relatively unchanged since their formation. Thus, knowledge of the chemical
composition and structure of these objects should offer clues as to the chemical mix and
conditions under which the solar system's planets formed 4.6 billion years ago. In
addition, information on their compositions and structures will be important should one
of them be discovered to be on an Earth threatening trajectory. Knowledge of their
compositions and structures will also be important in order to make intelligent choices as
to which objects would offer the richest sources of raw materials.
Spacecraft missions are required to understand the detailed chemical compositions and
structures of comets and asteroids. There are wide differences between comets and
asteroids and even wide differences between different types of asteroids. Some asteroids
are likely to be fragile and rich in carbon-based molecules while others are thought to be
solid iron. Whether looking for the richest source of raw materials or trying to nudge an
Earth threatening object out of harms way, it makes a big difference whether we're dealing
with a 50-meter sized fluff ball or a one-mile slab of solid iron. Because comets and
asteroids differ so widely in their characteristics, missions have been planned to visit a
widely diverse group of objects. After a brief summary of various spacecraft
instruments, the seven current missions to comets and asteroids are briefly described.
Typical Spacecraft Instruments:
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