The opposition of 2003 was special, because it was going to occur while Mars was at its closest point to the Sun. This configuration is known as a perihelic opposition. When Mars is in perihelic opposition it is also much closer to Earth than usual. This means that less fuel and flight time are required to send a spacecraft from Earth to Mars near the time of a perihelic opposition.
Perihelic oppositions only happen every fifteen to seventeen years. During the late 1990s, both the European
FIGURE 7.3
Scientific instruments on the Mars Orbiter
Space Agency and NASA began planning Mars missions to coincide with the perihelic opposition of 2003.
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