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Contamination Control and Assessment Strategy for Martian Moons Exploration (MMX)Martian Moons eXploration (MMX) is a sample return mission from the Martian moon Phobos. The MMX spacecraft is scheduled for launch in 2026 and return to Earth in 2031. The primary science objective of MMX is to reveal the origin of the Martian moons, thereby advancing the understanding of planetary system formation and material transport in the solar system, as well as to observe processes affecting the circumplanetary and surface environments of Mars. The returned sample will be transported to the curation facility at ISAS/JAXA, and the subsequent curation and sample analysis activity will be conducted. As a sample return mission, MMX requires strict contamination control to prevent the intrusion of terrestrial materials.
Document ID
20260003948
Acquisition Source
Johnson Space Center
Document Type
Extended Abstract
Authors
H Sugahara ORCID
(Institute of Space and Astronautical Science Tokyo, Japan)
W Fujiya ORCID
(Ibaraki University Ibaraki, Japan)
K Sakamoto ORCID
(Institute of Space and Astronautical Science Tokyo, Japan)
R Fukai ORCID
(Institute of Space and Astronautical Science Tokyo, Japan)
T Usui ORCID
(Institute of Space and Astronautical Science Tokyo, Japan)
M Abe ORCID
(Institute of Space and Astronautical Science Tokyo, Japan)
K Nagashima ORCID
(Institute of Space and Astronautical Science Tokyo, Japan)
A Nakano
(Institute of Space and Astronautical Science Tokyo, Japan)
S Kimura
(Institute of Space and Astronautical Science Tokyo, Japan)
T Ozawa
(Japan Aerospace Exploration Agency Tokyo, Japan)
H Sawada
(Institute of Space and Astronautical Science Tokyo, Japan)
H Kato
(Japan Aerospace Exploration Agency Tokyo, Japan)
Y Sato
(Institute of Space and Astronautical Science Tokyo, Japan)
K Yoshikawa ORCID
(Japan Aerospace Exploration Agency Tokyo, Japan)
Y Takano ORCID
(Japan Agency for Marine-Earth Science and Technology Yokosuka, Japan)
K Bajo ORCID
(Hokkaido University Sapporo, Japan)
S Tachibana ORCID
(The University of Tokyo Tokyo, Japan)
Y N Miura ORCID
(The University of Tokyo Tokyo, Japan)
M Zolensky ORCID
(Johnson Space Center Houston, United States)
C Gonzalez
(Amentum (United States) Chantilly, France)
M Rodriguez
(Amentum (United States) Chantilly, France)
C Calva
(Amentum (United States) Chantilly, France)
E P Seto ORCID
(Honeybee Robotics (United States) Brooklyn, United States)
N Bouey
(Honeybee Robotics (United States) Brooklyn, United States)
L Troung
(Honeybee Robotics (United States) Brooklyn, United States)
K Zacny
(Honeybee Robotics (United States) Brooklyn, United States)
Y Matsuyama
(Honeybee Robotics (United States) Brooklyn, United States)
D Van Dyne
(Honeybee Robotics (United States) Brooklyn, United States)
K Bywaters
(Honeybee Robotics (United States) Brooklyn, United States)
S Lam
(Honeybee Robotics (United States) Brooklyn, United States)
A Zapata
(Honeybee Robotics (United States) Brooklyn, United States)
R Espadas
(Honeybee Robotics (United States) Brooklyn, United States)
Date Acquired
May 6, 2026
Publication Date
August 9, 2026
Publication Information
Publisher: The Meteoritical Society
Subject Category
Ground Support Systems and Facilities (Space)
Exobiology
Meeting Information
Meeting: 88th Annual Meteoritical Society Meeting (MetSoc)
Location: Frankfort
Country: DE
Start Date: August 9, 2026
End Date: August 14, 2026
Sponsors: The Meteoritical Society
Funding Number(s)
CONTRACT_GRANT: 80GSFC19C0022
WBS: 048292
CONTRACT_GRANT: NNN12AA01C
CONTRACT_GRANT: 80JSC022DA035
Distribution Limits
Public
Copyright
Portions of document may include copyright protected material.
Technical Review
Single Expert
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