Mission Summary


Interstellar Probe science objectives are shown at various distances along the trajectory. The yellow-orange color bar indicates the radial region where measurements are possible; the deepest orange is the prime region of interest. Among the objectives that are also possible are measurement of the cosmic infrared radiation background free from the zodiacal light, a survey >1 km size Kuiper Belt objects, a survey of organic matter in the outer solar system and the interstellar medium, and the identification of interstellar antiprotons arising from dark matter or primordial black holes.

NASA's Interstellar Probe will be the first spacecraft designed to explore the nearby interstellar medium and its interaction with our solar system. Its unique trajectory from Earth to 200 AU in 15 years will enable the first comprehensive measurements of plasma, neutral atoms, magnetic fields, dust, energetic particles, cosmic rays and infrared emission from the outer solar system, through the boundaries of the heliosphere, and on into the interstellar medium. Although the success of the mission requires crossing the heliopause, a wide range of interdisciplinary studies can be addressed throughout the mission.

In view of the fundamental contributions that Interstellar Probe would make to studies that include space plasma physics, planetary science, astrophysics, stellar and galactic evolution, and cosmology, it is important that NASA begin developing the technology required to carry out this truly exploratory mission.


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Introduction
Interstellar Medium
Interaction Between the Interstellar Medium and the Solar Wind
The Outer Solar System
Scientific Instruments and Mission Requirements
Acknowledgments
Table of Contents


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For more information regarding this website
and the Interstellar Probe Project,
please contact Dr. Paulett Liewer

This site was last updated:
February 8, 2000.