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Results for “Long-duration spaceflight”

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PubMed2026

Using Organoids to Unlock the Potential of Human Torpor for Spaceflight.

PURPOSE OF REVIEW: This paper reviews the current understanding of the potential for humans to enter a state of torpor/hibernation, and discusses the possibility of inducing torpor in astronauts for long-duration space travel, including some of the physiological, technological, and ethical considerations associated with its implementation. By exploring means to induce torpor in various human organoid systems, we hope such research can provides insights to comprehensive solutions to overcome some of the major hurdles that limit the potential for human to enter a state of torpor during long-duration deep-space missions, and contribute to the ongoing efforts to make such missions more feasible and safer for astronauts. RECENT FINDINGS: On future deep space missions such as NASA's planned missions to the Moon, Mars, and near-Earth asteroids, astronauts will be continuously exposed to environments that are radically different from those on Earth, each presenting multiple logistical and physiological challenges. Beyond the well-documented physiological effects of microgravity, space travelers will encounter a complex radiation environment that may contribute to significant short- and long-term adverse effects on human physiology and increase the risk of cancer and other diseases. Besides these physical challenges, life support systems must also be designed to mitigate psychological impacts of long-term isolation and confinement - all of which collectively pose formidable engineering problems. Hibernation/torpor is a state of prolonged inactivity and metabolic depression used by a wide variety of mammals to survive periods of cold temperatures and food scarcity, including some primates and perhaps even an extinct early line of hominins that lived nearly half a million years ago. Since modern humans share common ancestry with these hominins and hibernating primates, it is likely the human genome encodes the necessary genetic information to hibernate, or at least enter the similar, more transient state of torpor. The reduced body activity, lowered metabolism, and decreased energy requirements that characterize torpor suggest that developing means of inducing such a state in astronauts could address these challenges, including providing a degree of radioprotection. SUMMARY: This review explores the potential application of human torpor as a countermeasure to address the many challenges posed by long-duration spaceflight beyond low-Earth orbit (LEO), discusses various natural hibernating model systems for studying means of inducing a torpor-like state in humans, and highlights the vast potential of using human organoids to test and validate mechanisms that govern induction and maintenance of torpor to identify the means to one day safely induce this state in astronauts to provide additional protection from the myriad stressors of spaceflight.

Astronaut Health↗

PubMed2025

Nanobioreactor detection of space-associated hematopoietic stem and progenitor cell aging.

Human hematopoietic stem and progenitor cell (HSPC) fitness declines following exposure to stressors that reduce survival, dormancy, telomere maintenance, and self-renewal, thereby accelerating aging. While previous National Aeronautics and Space Administration (NASA) research revealed immune dysfunction in low-earth orbit (LEO), the impact of spaceflight on human HSPC aging had not been studied. To study HSPC aging, our NASA-supported Integrated Space Stem Cell Orbital Research (ISSCOR) team developed bone marrow niche nanobioreactors with lentiviral bicistronic fluorescent, ubiquitination-based cell-cycle indicator (FUCCI2BL) reporter for real-time HSPC tracking in artificial intelligence (AI)-driven CubeLabs. In month-long International Space Station (ISS) missions (SpX-24, SpX-25, SpX-26, and SpX-27) compared with ground controls, FUCCI2BL reporter, whole-genome and transcriptome sequencing, and cytokine arrays demonstrated cell-cycle, inflammatory cytokine, mitochondrial gene, human repetitive element, and apolipoprotein B mRNA editing enzyme, catalytic polypeptide-like 3 (APOBEC3) deregulation together with clonal hematopoietic mutations. Furthermore, HSPC functionally organized multi-omics aging (HSPC-FOMA) analyses revealed reduced telomere maintenance, adenosine deaminase acting on RNA1 (ADAR1) p150 self-renewal gene expression, and replating capacity indicative of space-associated HSPC aging that may limit long-duration spaceflight.

Humans↗

PubMed2026

Leveraging bioinformatics approaches for drug repositioning in space radiation protection.

The health effects of space radiation, primarily Galactic Cosmic Rays (GCRs), on humans remain largely unknown, with potential cardiovascular consequences posing a significant threat to astronauts on long-duration spaceflight missions. Currently, there are no established pharmacological countermeasures for GCR exposure. Drug repositioning offers a promising strategy to accelerate pharmaceutical research in space medicine. This study leverages existing bioinformatics techniques to identify and prioritize potential drug candidates associated with proteomic perturbations following simulated GCR exposure using previously published murine cardiac proteomic data. A protein-protein interaction (PPI) network was constructed using the top differentially expressed proteins (DEPs) from murine heart tissue following exposure to 5-ion GCRs as seed nodes, focusing on experimentally supported interactions. Network topology, Markov clustering, and functional enrichment analyses were used to characterize biologically relevant proteins and pathways. Drug-protein interactions were predicted using Drugst.One and mapped to PPI clusters of interest to identify candidate drugs. Selected drug-macromolecule interactions were further explored using CB-Dock2 molecular docking and short-duration molecular dynamics simulations as hypothesis-generating structural assessments. Analysis of a key PPI network cluster consisting of several ATP synthase proteins identified 23 unique drug candidates. These analyses demonstrate a systematic approach for leveraging bioinformatics techniques to identify candidate molecular targets and generate pharmacological hypotheses in the context of space radiation countermeasures. Ultimately, this strategy introduces a hypothesis-generating framework for the prioritization of potential drug candidates for future computational characterization and experimental investigation against spaceflight stressors.

Animals↗

PubMed1991

Protein composition in human plasma after long-term orbital missions and in rodent plasma after spaceflights on biosatellites "Cosmos-1887" and "Cosmos-2044".

The two-dimensional plasma protein map of crewmembers of long-duration "Mir" expeditions obtained the day after the recovery shows a manifold increase in the content of several proteins normally seen in trace amounts. The emergence of several unusual protein spots occurs as well, some of them probably due to charge shifts provided by the events influencing posttranslational modification processes. By the 8 postflight day these phenomena were disappeared. In the "Cosmos-1887" biosatellite experiment, the plasma samples obtained two days after the landing as well as plasma of synchronous animals exhibited the higher fibrinogen levels when compared to those of vivarium animals. The protein consisting of a number of fractions with molecular weight of 50 to 60 kD and pI 5 to 6 had protein spots of similar size in flight and synchronous animals while in vivarium rats one of the spots was larger in size as opposed to the others. The plasma protein spectrum of flight and synchronous groups of animals in "Cosmos-1887" experiment where plasma samples were prepared in the period of time from 5 to 10 hours after spaceflight coincided with the pattern of vivarium animals. The data suggest that the protein changes described above develop during postflight period and accelerations, vibrations, readaptation to 1 G gravity, emotional stress could be the cause of these alterations.

Animals↗

PubMed2026

Selective saccular plasticity under microgravity links peripheral transcriptomic remodeling to postflight vestibular dysfunction.

Long-duration exposure to microgravity disrupts human balance and spatial orientation, yet the molecular mechanisms underlying vestibular adaptation to spaceflight remain poorly understood. Here, we tested the hypothesis that the saccule, the primary gravity-sensing otolith organ, undergoes selective remodeling during spaceflight and contributes to transient postflight postural instability. Using a cross-species approach, we combined transcriptomic analysis of mouse otolith organs with physiological assessments in astronauts. Laser microdissection-based RNA sequencing of mouse otolith sensory epithelia after a 35-d spaceflight revealed pronounced, organ-specific transcriptomic remodeling in the saccule, whereas the utricle remained stable. Principal component and clustering analyses demonstrated that the saccular transcriptome shifted toward an utricle-like profile under microgravity, accompanied by changes in genes related to synaptic and neuronal function. Promoter motif analysis identified NFAT-associated transcriptional networks, suggesting Ca2+-dependent regulation of synaptic plasticity as a potential molecular substrate of gravity-dependent adaptation. In parallel, vestibular testing in astronauts following long-duration missions (157 to 328 d) revealed selective attenuation of saccule-mediated cervical vestibular-evoked myogenic potentials and increased postural sway immediately after return to Earth, while utricle-mediated responses and semicircular canal function were preserved. Both saccular function and postural stability recovered within approximately 10 d. Notably, early postflight postural instability was partially mitigated by noisy galvanic vestibular stimulation, consistent with stochastic resonance-mediated sensory enhancement. Together, these findings identify the saccule as a plastic gravity sensor and establish a mechanistic link between peripheral molecular remodeling and functional balance deficits after spaceflight, providing a framework for developing countermeasures to facilitate vestibular readaptation during human space exploration.

Animals↗

PubMed1991

Neuromuscular aspects in development of exercise countermeasures.

Based on the results generated from experiments conducted by our investigators, it is clear that prolonged exposure to microgravity environments can induce ultrastructural abnormalities and atrophy of muscle and impair muscle function, especially upon return to terrestrial gravity. It is also apparent that ground-base models can be effectively used to study these changes. This provides a less expensive and more controlled laboratory condition in order to conduct experiments. The use of animal models must be more closely examined. In the case of muscle adaptations to microgravity, the data from flight experiments which have used rodents might suggest the use of exercise with characteristics contrary to those which would be most appropriate to defend against atrophy and dysfunction in human muscle. Although many spaceflight experiments may be limited to the use of animal models, the results of the studies reviewed in this paper emphasize the importance of using human models in order to provide the most accurate interpretation of data for the development of exercise countermeasures for spaceflight. If maintenance of muscle structure, size and function is perceived as operationally necessary, the results from the studies conducted by our investigators indicate that the use of more resistive exercise must be given greater consideration as part of the development of future exercise countermeasure programs for spaceflight. The advantages of incorporating resistive exercise with a strong emphasis on the use of eccentric muscle actions in addition to concentric actions may prove most effective as a countermeasure against the muscle atrophy and dysfunction caused by long-duration exposure to microgravity environments.

Adult↗

PubMed1990

Influence of static head position on the horizontal nystagmus evoked by caloric, rotational and optokinetic stimulation in the squirrel monkey.

We studied the influence of static head position on the horizontal nystagmus produced by caloric, rotational and optokinetic stimulation in alert squirrel monkeys. Caloric nystagmus is stronger for nose up (NU) than for nose down (ND) pitches; so, for example, slow-phase eye velocity is four times larger in supine than in prone positions. A similarly directed asymmetry occurs in the horizontal vestibulo-ocular (HVOR) responses to long-duration, constant angular-head accelerations, but not to midband (0.1 Hz) sinusoidal head rotations. Consistent with a first-order model of the HVOR, the low-frequency or acceleration gain of the reflex (GA) is equal to the product of the midband velocity gain (GV) and a time constant (TVOR). GV is proportional to the cosine of the angle between the horizontal-canal plane and the plane of rotation, from which it is concluded that signals from the horizontal, but not from the vertical canals contribute to the HVOR. TVOR can be as much as twice as large in NU than in ND positions. GA is proportional to TVOR and it, too, shows a NU-ND asymmetry. The time constant of optokinetic after nystagmus (TOKAN) was also studied. Since TVOR and TOKAN are modified in similar ways by static tilts, it is concluded that head position affects the time constants by way of velocity-storage mechanisms. Evidence is presented that the position-dependent modification of velocity storage is otolith-mediated. The results are used to analyze the mechanisms of caloric nystagmus. The caloric response consists of a convective component (CC), as originally envisioned by Bárány (1906), and a nonconvective component (NC). CC accounts for 75% of the caloric response in the conventional supine testing position. Both components can be affected by the position-dependent modification of TVOR or, equivalently, of GA. It has been suggested that two mechanisms might contribute to NC: 1) a direct thermal effect on hair cells or afferents; or 2) a thermal expansion of labyrinthine fluids that results in a cupular displacement. Both theoretical and experimental evidence indicates that only the first of these mechanisms could result in the steady-state caloric response that is observed in the absence of convection (e.g., in spaceflight and after canal plugging) and that contributes to the prone-supine asymmetry seen in caloric testing.

Animals↗