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Hayabusa Mission

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Journal Article
Journal: Elements
Published: 01 February 2014
Elements (2014) 10 (1): 45-50.
... processes on the airless surface of Itokawa, such as the impact of small objects, grain motion, and irradiation by solar wind. © 2014 by the Mineralogical Society of America 2014 Hayabusa mission regolith space weathering solar wind impact S-type asteroids Launched on May 9, 2003...
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Journal Article
Journal: Geology
Published: 10 July 2017
Geology (2017) 45 (9): 819-822.
... goals of the Hayabusa mission of the Japan Aerospace Exploration Agency was to recover samples from asteroid 25143 Itokawa, a 535 × 295 × 209 m body, and return them to Earth ( Abe et al., 2006 ; Nakamura et al., 2011 ). In June 2010, the sample catcher was recovered, revealing at least 1500 regolith...
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Journal Article
Published: 01 January 2008
Reviews in Mineralogy and Geochemistry (2008) 68 (1): 273-343.
... differences and degree of heating. However, dynamical processes have significantly affected these trends. Close observation of asteroids by spacecraft, such as NEAR-Shoemaker to 433 Eros and Hayabusa to 25143 Itokawa, are currently the best way to discern the mineralogies of individual asteroids...
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Image
Logos of <b>missions</b> scheduled to visit asteroids in the near future: Dawn (NA...
in > Elements
Published: 01 February 2014
F igure 7 Logos of missions scheduled to visit asteroids in the near future: Dawn (NASA), OSIRIS-REx (NASA), Hayabusa-2 (JAXA), and MarcoPolo-R (ESA)
Series: Geological Society, London, Special Publications
Published: 01 January 2006
DOI: 10.1144/GSL.SP.2006.256.01.19
EISBN: 9781862395046
..., and the future potential of matching asteroid types to meteorite samples was to have been realized with the first successful sample return mission. Japan's Hayabusa (MUSES-C) spacecraft successfully made its rendezvous with the near-Earth asteroid (25143) Itokawa on 12 September 2005. Itokawa is an S-type...
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Series: AAPG Memoir
Published: 01 January 2013
DOI: 10.1306/13361574M1013543
EISBN: 9781629810027
.... Near–Earth asteroid discovery statistics as of January 19, 2011 ( Spahr, 2011 ). LINEAR = Lincoln Near–Earth Asteroid Research program; NEAT = Near–Earth Asteroid Tracking;LONEOS = Lowell Observatory Near–Earth Object Search. Missions such as Japan’s Hayabusa ( Fujiwara et al.,2006 ) Sample...
Journal Article
Journal: Elements
Published: 01 February 2014
Elements (2014) 10 (1): 19-24.
... of particles from the S-type asteroid Itokawa, successfully returned by the Japanese Hayabusa mission in 2010, shows that the particles came from materials like those in thermally metamorphosed LL-group ordinary chondrites and that the spectrum of Itokawa has been reddened by space weathering as a result...
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Journal Article
Journal: Elements
Published: 01 February 2014
Elements (2014) 10 (1): 25-30.
... of known provenance in hand. Recently we directly sampled the near-Earth asteroid Itokawa ( Tsuchiyama 2014 ). Asteroid sample-return missions are also scheduled for later in this decade (OSIRIS-REx, Hayabusa-2). Compositional studies of meteorites indicate that they originated from at least many tens...
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Journal Article
Journal: Elements
Published: 01 February 2014
Elements (2014) 10 (1): 11-17.
...F igure 7 Logos of missions scheduled to visit asteroids in the near future: Dawn (NASA), OSIRIS-REx (NASA), Hayabusa-2 (JAXA), and MarcoPolo-R (ESA) ...
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Journal Article
Published: 01 August 2011
Clays and Clay Minerals (2011) 59 (4): 416-432.
.... Undifferentiated meteorites are important sources of information about asteroids. Other than small returned samples ( e.g. comet dust returned by NASA’s Stardust mission; Brownlee et al. , 2006 ; Zolensky et al. , 2006 ; mineral fragments recently returned from asteroid Itokawa by the ISAS Hayabusa mission...
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Series: SEPM Special Publication
Published: 01 January 2012
DOI: 10.2110/pec.12.102.0097
EISBN: 9781565763135
... Itokawa recently returned by the Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA) Hayabusa mission ( Yano et al. 2006 ) sample only a few specific solar-system bodies (the Moon, one comet, and one asteroid). On Earth, coarse clastic detritus is dominated...
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Image
( A ) Close-up image of the very rough surface of Itokawa (mean diameter 32...
in > Elements
Published: 01 February 2014
F igure 3 ( A ) Close-up image of the very rough surface of Itokawa (mean diameter 320 m), taken by Hayabusa (a 1-meter scale is indicated on the image); the surface is composed mainly of a thin layer of gravel and pebbles. ( B ) Close-up image of the surface of 17 km Eros, taken by the NEAR
Image
( A ) Close-up image of the very rough surface of Itokawa (mean diameter 32...
in > Elements
Published: 01 February 2014
F igure 3 ( A ) Close-up image of the very rough surface of Itokawa (mean diameter 320 m), taken by Hayabusa (a 1-meter scale is indicated on the image); the surface is composed mainly of a thin layer of gravel and pebbles. ( B ) Close-up image of the surface of 17 km Eros, taken by the NEAR
Journal Article
Published: 01 April 2018
Geochemical Perspectives (2018) 7 (1): 97-99.
... with the Hayabusa mission give us some idea of the problems we are facing with such asteroid missions. If we want to better understand the formation of our solar system and the evolution of other planetary systems we need strong cosmochemical research groups. REFERENCES SECTION 18 Palme , H...
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Journal Article
Published: 01 November 2007
Geological Magazine (2007) 144 (6): 1030-1031.
... rewritten second edition of a 1997 conference volume. Since the publication of the original work, there have been theoretical and practical advances in this fast-moving field. For example, several cometary and asteroid sampling missions are either, like Rosetta and Hayabusa , in progress or, like...
Journal Article
Journal: Elements
Published: 01 June 2016
Elements (2016) 12 (3): 197-202.
... micrometeorites orbited in space for up to several million years as small bodies. Nishiizumi et al. ( 2015 ) reported the concentrations of 10 Be and 26 Al in particles that the Hayabusa mission brought back from the LL-chondritic asteroid Itokawa; one of the particles analyzed had a mass of only 0.5 μg...
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Journal Article
Journal: Elements
Published: 01 October 2019
Elements (2019) 15 (5): 348.
... of these experiences, he has been investigating fine-grained samples returned from a comet, an asteroid, the Moon, and the international space station. In the Hayabusa 1 mission, he worked as a member of the JAXA/Institute of Space and Astronautical Science curation team and found that the surface of the returned fine...
Journal Article
Journal: Elements
Published: 01 August 2019
Elements (2019) 15 (4): 286-287.
... are distributed for scientific study in a fair, timely, and responsible manner. This maximizes the scientific return on each sample. The JSC curation currently houses all, or part of, nine different astromaterial sample collections, with two more sample-return missions underway: (1) Apollo program samples (1969...
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Journal Article
Journal: Elements
Published: 01 April 2018
Elements (2018) 14 (2): 113-118.
... Hayabusa return mission to the “S-type” asteroid Itokawa, and NASA's Dawn mission to asteroids Vesta and Ceres) can provide additional data about samples that date from the very earliest times in our solar system. These missions can either provide remote data (such as Rosetta ) or could be sample...
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Series: Geological Society, London, Special Publications
Published: 01 January 2014
DOI: 10.1144/SP378.6
EISBN: 9781862396623
... ( Fujimaki et al. 1992 ). If one or more recent events could be identified in the LL chondrites, it might be possible to tie them to the evolution of the one asteroid definitively known to contain ordinary chondrite material. The Hayabusa mission studied the S asteroid 25143 Itokawa extensively...
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