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Download : International Space Station
NASA’s
International Space Station (ISS) celebrated 15 years of operations
in November 2013 and
is living up to expectations as a leading space laboratory, hosting
state-of-the-art science facilities, and providing researchers with a
continuous microgravity environment to conduct investigations across
many disciplines.
From
the first ISS element, launched in November 1998, the ISS has
supported investigations and technology demonstrations that will
advance NASA’s human exploration capabilities beyond low Earth
Orbit (LEO), and improve the daily lives of people on Earth well
beyond its operational lifetime. The first 15 years of utilization on
ISS has helped answer scientific questions ranging from “How do
fluids flow in space?” to “What are the origins of the universe?”
The science and technology returns have grown at a steady pace. Even
before the assembly of ISS was completed in 2011, the on-orbit crew
were busy performing experiments, and with the full complement of a 6
person crew, more than 1 600 investigations have been conducted to
date across the international partnership.
This
report is intended to provide an archival record of the
internationally-sponsored ISS research results collected for
investigations performed from 2000-2011 on ISS (Expedition 0 through
30), including scientific publications from studies based on
operational data. These investigations represent the research of
thousands of scientists around the globe, and have impacts beyond the
field of space research into traditional areas of science in
multidisciplinary ways that no Earth-based laboratory has done. Yet
much like a typical laboratory on Earth, the logistics of the ISS
allows for many investigations to be carried forward over several ISS
crew expeditions, enabling repeated experimentation and data
collection that traditional science calls for. One example of this is
the Seedling Growth-1 (SG-1) joint NASA-ESA experiment that was
implemented as an extension of the earlier Tropi-1 and Tropi-2 plant
growth experiments that first confirmed the existence red-light based
phototropism in roots and hypocotyls of seedlings. Researchers were
able to capitalize on Tropi results in the SG-1 design by improving
different lighting conditions, decreasing seed storage time, and
adding real-time seedling observation through improved image downlink
[4] .
The
results from ISS have so far yielded updated new insights into how to
better live and work in space, such as addressing radiation effects
on crew health [4] , combating bone and muscle loss [1, 7] ,
improving designs of systems that handle fluids in microgravity [12]
, and how to most efficiently maintain environmental control [15] .
Latest examples of the ISS utilization applications relevant to our
life on Earth is published in the second edition of the ISS Benefits
for Humanity, which documents several tangible benefits that have
resulted from ISS utilization in areas of Earth Observation and
Disaster Response, Human Health, Global Education, Innovative
Technology, and Economic Development of Space [2] . These benefits
include such examples of how space-based research leads to
improvements in therapies for balance disorders [2, 16] and
contributions to improvements in smart fluids for advanced braking
systems and earthquake dampening devices [2, 6] . ISS results also
show promise in diverse applications such as medicine [2, 10] and
global maritime tracking [11] and have advanced our knowledge of our
planet’s health while also contributing to disaster response
efforts [2, 13, 9, 8] . With all its diversity, the ISS continues to
inspire millions of students in ways that only space can [14, 5, 3] .
The
ISS offers a unique platform for science with critical capabilities
not available anywhere else. It provides long-duration microgravity
exposure, thermosphere exposure, and external environment exposure
for material observations at high inclination, altitude, and
velocity. The microgravity environment of the ISS allows scientists
to observe unique behaviors that are otherwise masked by gravity on
Earth, such as thermocapillary and fluid flows, protein crystal
growth, flame structures, and the structure of living cells. The ISS
platform also provides access to extreme heat and cold cycles, ultra
vacuum, atomic oxygen, and high-energy radiation.
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