Special issue “Science of solar system materials examined from Hayabusa and future missions (II)”

Six years have passed since the first asteroid sample was returned from the S-type near-Earth asteroid 25143 Itokawa by the JAXA’s Hayabusa mission in 2010 (Yada et al. 2014). Considerable progress has been made in the study of surface regolith materials and the understanding of planetary surface pr...

Full description

Bibliographic Details
Main Authors: Okada, Tatsuaki, Connolly, Harold C, Yada, Toru, Ohtsuki, Keiji, Connolly, Harold C., Binzel, Richard P
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Language:English
Published: Springer Berlin Heidelberg 2017
Online Access:http://hdl.handle.net/1721.1/107459
_version_ 1826202925828931584
author Okada, Tatsuaki
Connolly, Harold C
Yada, Toru
Ohtsuki, Keiji
Connolly, Harold C.
Binzel, Richard P
author2 Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
author_facet Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Okada, Tatsuaki
Connolly, Harold C
Yada, Toru
Ohtsuki, Keiji
Connolly, Harold C.
Binzel, Richard P
author_sort Okada, Tatsuaki
collection MIT
description Six years have passed since the first asteroid sample was returned from the S-type near-Earth asteroid 25143 Itokawa by the JAXA’s Hayabusa mission in 2010 (Yada et al. 2014). Considerable progress has been made in the study of surface regolith materials and the understanding of planetary surface processes such as space weathering (Noguchi et al. 2011), the chronology of Itokawa and its dynamic evolution processes (Nagao et al. 2011; Park et al. 2015), and the thermal alteration undergone in parent bodies (Nakamura T et al. 2011). Discussions of new findings from the Hayabusa-returned samples and from a large collection of meteorites, micrometeorites, and interplanetary dust particles have continued, especially at the annual international Hayabusa symposia of solar system materials (Okada et al. 2015). Progress in sample return science has driven the next stage of exploration. Now, two new sample return missions to primitive, volatile-rich asteroids, JAXA’s Hayabusa2 (Tsuda et al. 2013) and NASA’s OSIRIS-REx (Lauretta et al. 2012), are en route to their target bodies, C-type 162173 Ryugu and B-type 101955 Bennu, respectively. It is our great pleasure to present our second special issue of the journal Earth, Planets and Space, “Science of solar system materials examined from Hayabusa and future missions (II).” This special issue is based on discussions during the Hayabusa 2014 symposium, which featured new results from Hayabusa-returned samples and related studies, but was also open to any scientific results regarding primitive bodies and the early solar system, the results of laboratory experiments and ground-based observations, and reports of new instruments and methods. We will begin with a brief introduction to the missions of the Hayabusa and its successor Hayabusa2. In addition, all six manuscripts published in this special issue are reviewed below.
first_indexed 2024-09-23T12:25:42Z
format Article
id mit-1721.1/107459
institution Massachusetts Institute of Technology
language English
last_indexed 2024-09-23T12:25:42Z
publishDate 2017
publisher Springer Berlin Heidelberg
record_format dspace
spelling mit-1721.1/1074592022-10-01T09:12:02Z Special issue “Science of solar system materials examined from Hayabusa and future missions (II)” Okada, Tatsuaki Connolly, Harold C Yada, Toru Ohtsuki, Keiji Connolly, Harold C. Binzel, Richard P Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Binzel, Richard P Six years have passed since the first asteroid sample was returned from the S-type near-Earth asteroid 25143 Itokawa by the JAXA’s Hayabusa mission in 2010 (Yada et al. 2014). Considerable progress has been made in the study of surface regolith materials and the understanding of planetary surface processes such as space weathering (Noguchi et al. 2011), the chronology of Itokawa and its dynamic evolution processes (Nagao et al. 2011; Park et al. 2015), and the thermal alteration undergone in parent bodies (Nakamura T et al. 2011). Discussions of new findings from the Hayabusa-returned samples and from a large collection of meteorites, micrometeorites, and interplanetary dust particles have continued, especially at the annual international Hayabusa symposia of solar system materials (Okada et al. 2015). Progress in sample return science has driven the next stage of exploration. Now, two new sample return missions to primitive, volatile-rich asteroids, JAXA’s Hayabusa2 (Tsuda et al. 2013) and NASA’s OSIRIS-REx (Lauretta et al. 2012), are en route to their target bodies, C-type 162173 Ryugu and B-type 101955 Bennu, respectively. It is our great pleasure to present our second special issue of the journal Earth, Planets and Space, “Science of solar system materials examined from Hayabusa and future missions (II).” This special issue is based on discussions during the Hayabusa 2014 symposium, which featured new results from Hayabusa-returned samples and related studies, but was also open to any scientific results regarding primitive bodies and the early solar system, the results of laboratory experiments and ground-based observations, and reports of new instruments and methods. We will begin with a brief introduction to the missions of the Hayabusa and its successor Hayabusa2. In addition, all six manuscripts published in this special issue are reviewed below. 2017-03-17T14:12:10Z 2017-03-17T14:12:10Z 2017-02 2017-02 2017-03-10T05:02:11Z Article http://purl.org/eprint/type/JournalArticle 1880-5981 1343-8832 http://hdl.handle.net/1721.1/107459 Okada, Tatsuaki et al. “Special Issue ‘Science of Solar System Materials Examined from Hayabusa and Future Missions (II).’” Earth, Planets and Space 69.1 (2017): n. pag. en http://dx.doi.org/10.1186/s40623-017-0617-3 Earth, Planets and Space Creative Commons Attribution http://creativecommons.org/licenses/by/4.0/ The Author(s) application/pdf Springer Berlin Heidelberg Springer Berlin Heidelberg
spellingShingle Okada, Tatsuaki
Connolly, Harold C
Yada, Toru
Ohtsuki, Keiji
Connolly, Harold C.
Binzel, Richard P
Special issue “Science of solar system materials examined from Hayabusa and future missions (II)”
title Special issue “Science of solar system materials examined from Hayabusa and future missions (II)”
title_full Special issue “Science of solar system materials examined from Hayabusa and future missions (II)”
title_fullStr Special issue “Science of solar system materials examined from Hayabusa and future missions (II)”
title_full_unstemmed Special issue “Science of solar system materials examined from Hayabusa and future missions (II)”
title_short Special issue “Science of solar system materials examined from Hayabusa and future missions (II)”
title_sort special issue science of solar system materials examined from hayabusa and future missions ii
url http://hdl.handle.net/1721.1/107459
work_keys_str_mv AT okadatatsuaki specialissuescienceofsolarsystemmaterialsexaminedfromhayabusaandfuturemissionsii
AT connollyharoldc specialissuescienceofsolarsystemmaterialsexaminedfromhayabusaandfuturemissionsii
AT yadatoru specialissuescienceofsolarsystemmaterialsexaminedfromhayabusaandfuturemissionsii
AT ohtsukikeiji specialissuescienceofsolarsystemmaterialsexaminedfromhayabusaandfuturemissionsii
AT connollyharoldc specialissuescienceofsolarsystemmaterialsexaminedfromhayabusaandfuturemissionsii
AT binzelrichardp specialissuescienceofsolarsystemmaterialsexaminedfromhayabusaandfuturemissionsii