Sample Return Science by Hayabusa Near-Earth Asteroid Mission

A Fujiwara; M Abe; M Kato; I Kushiro; T Mukai; T Okada; J Saito; S Sasaki; H Yano; D Yeomans

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NASA NTRS · 20040059594

Sample Return Science by Hayabusa Near-Earth Asteroid Mission

A Fujiwara·M Abe·M Kato·I Kushiro·T Mukai·T Okada·J Saito·S Sasaki·H Yano·D Yeomans

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Abstract

Assigning the material species to each asteroid spectral type and finding out the corresponding meteorite category is crucial to make the global material map in the whole asteroid belt and to understand the evolution of the asteroid belt. Recent direct observations by spacecrafts are revealing new intriguing aspects of asteroids which cannot be obtained solely from ground-based observations or meteorite studies. However identification of the real material species constituting asteroids and their corresponding meteorite analogs are still ambiguous. Space weathering makes difficult to identify the true material, and there is still a great gap between the remote sensing data on the global surface and the local microscopic data from meteorites. Sample return from asteroids are inevitable to solve these problems. For this purpose sample return missions to asteroids belonging to various spectral classes are required. The HAYABUSA spacecraft (prelaunch name is MUSESC) launched last year is the first attempt on this concept. This report presents outline of the mission with special stress on its science.

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BibTeX RIS

A Fujiwara, M Abe, M Kato, I Kushiro, T Mukai, T Okada, J Saito, S Sasaki, H Yano, D Yeomans. 2004-03-16. Sample Return Science by Hayabusa Near-Earth Asteroid Mission. https://ntrs.nasa.gov/citations/20040059594

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