Browsing by Author "Grott, Matthias"

The InSight mission to Mars will launch in March of 2016, landing six months later in Elysium Planitia. In contrast to the 43 previous missions to Mars, which have thoroughly explored its surface features and chemistry, atmosphere, and searched for past or present life, InSight will focus on the deep interior of the planet. InSight will investigate the fundamental processes of terrestrial planet formation and evolution by performing the first comprehensive surfacebased geophysical measurements on Mars. It will provide key information on the composition and structure of an Earthlike planet that has gone through most of the evolutionary stages of the Earth up to plate tectonics. The planet Mars can play a key role in understanding early terrestrial planet formation and evolution. Unlike the Earth, its overall structure appears to be relatively unchanged since the first few hundred million years after formation; unlike the Moon, it is large enough that the PT conditions within the planet span an appreciable fraction of the terrestrial planet range. Thus the largescale chemical and structural evidence preserved in Mars’ interior should tell us a great deal about the processes of planetary differentiation and heat transport. InSight will undertake this investigation using the “traditional” geophysical techniques of seismology, precision tracking (for rotational dynamics), and heat flow measurement. The predominant challenge, in addition to the technical problems of the remote installation and operation of instruments on a distant and harsh planetary surface, comes from the practical limitation of working with data acquired from a single station. We will discuss how we overcome these limitations through the application of singlestation seismic analysis techniques, which take advantage of some of the specific attributes of Mars, and global heat flow modeling, which allows the interpretation of a single measurement of a spatially inhomogeneous surface distribution.

The InSight mission will illuminate the processes of terrestrial planet formation and evolution through a surface-based geophysical investigation of Mars.