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Phase II Final Report - NASA's Institute for Advanced Concepts

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Chapter 1.0 Introduction<br />

1.3 Mission<br />

craters’ magnetic signatures, can lead to a greater understanding of the early history of magnetism<br />

on Mars. Also, by identify young craters in older terrain and mapping the magnetic fields<br />

around these craters, in<strong>for</strong>mation relevant to the thermal evolution of the planet can be obtained.<br />

The history of Mars’ magnetic field may be an important link <strong>for</strong> understanding the radiation<br />

environment due to the early sun's solar wind.<br />

From previous scientific investigation, it is know that the magnetism of Mars varies greatly over<br />

the planet’s surface. It is very highly magnetized at certain locations (an order of magnitude<br />

greater than the magnetic field strength on Earth, and at altitudes an order of magnitude higher<br />

than on Earth, greater than 1,500 nT at 100 km altitude, and greater than 250 nT at 400 km altitude),<br />

and weakly magnetized at others. The locations of the strong magnetic fields correspond<br />

with some of the older and highly cratered areas of Mars.<br />

Presently there is no active mechanism <strong>for</strong> <strong>for</strong>ming a uni<strong>for</strong>m magnetic field (as on Earth).<br />

Because of this lack of a planetary magnetic field, it is much easier to measure the crustal magnetization<br />

directly. This crustal magnetization can exceed several Gauss (200,000 nT). The magnetic<br />

landscape of Mars was first discovered by the Mars Global Surveyor spacecraft. This<br />

spacecraft measured many large scale, highly magnetic locations on the surface of Mars, many<br />

extending over hundreds of kilometers. However, due to the distance from the surface, small<br />

scale variations in the magnetic fields, which are believed to exist could not be discerned. The<br />

Entomopter can be used to investigate these magnetic field regions and provide high resolution<br />

data on the magnetic field strength variations within these regions. An example of the differences<br />

between the magnetic fields on Mars and Earth are shown in Figure 1-14.<br />

Earth Magnetic Field<br />

Mars Magnetic Field<br />

Figure 1-14: Magnetic Field Shape on Earth and Mars<br />

The magnetic field mapping done by the Entomopter would enable a greater understanding of<br />

the crustal magnetism on Mars. For this to be accomplished, it would require that measurements<br />

of the magnetic field be per<strong>for</strong>med with enough spatial resolution to relate magnetism to specific<br />

geologic features and structures. With the Entomopter, the spatial resolution on these measurements<br />

would be less than 1 m, orders of magnitude greater than what is achievable from orbit.<br />

19

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