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Space radiation measured during first-ever commercial suborbital mission on Virgin Galactic SpaceShipTwo Unity on 29 June 2023
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.09.003
Tsvetan Dachev , Pantaleone Carlucci , Francesco Cairo , Borislav Tomov , Yuri Matviichuk , Plamen Dimitrov , Mityo Mitev , Malina Jordanova , Lucia Paciucci
The paper presents the variations of space radiation (primary and secondary galactic cosmic rays (GCR) absorbed dose rate in silicon and flux) measured during the first-ever commercial suborbital flight of the Virgin Galactic (VG) SpaceShipTwo Unity on 29 June 2023. A Portable Dosimeter-Spectrometer Liulin-CNR-VG is used. It is developed in the Space Research and Technology Institute, Bulgarian Academy of Sciences (SRTI-BAS) under a scientific contract with National Research Council of Italy (CNR), Italy. Liulin-CNR-VG size is 63х54 × 23 mm. Its weight is 0.092 kg. During the first part of the SpaceShipTwo flight, up to 14.4 km, the dose rate rises from 0.058 μGy h-1 up to 2.5 μGy h-1. Above the altitude of 30 km, the dose rate falls to 2.2 μGy h-1, while the dose to flux ratio increases to values about 1.0 nGy cm2 particle-1. The latter confirms the outcomes of previous balloon experiments, i.e. the change of the composition of the radiation field of the GCR and secondary radiation source from predominantly light particles as electrons, pions and muons towards heavier particles as protons and neutrons. On the descending part of the flight, one maximum in the flux and dose rate curves is obtained as Regener-Pfotzer maximum (R-PM). The flux calculated by the moving avervage is equal to 1.2 cm-2 s-1 and the dose rate is equal to 2.9 μGy h-1 at an altitude of 13 km. These values are well in line with those expected in conditions of relatively high solar activity, such as during the flight. The dose rates measured by Liulin-CNR-VG are in good agreement with other Liulin data, such as those recorded during balloon flights in 2005 and 2015 and civil aviation flights. The calculated total equivalent dose rate during the VG SpaceShipTwo flight is 7.46 μSv for 1.22 h. This reveals that there is a very small radiation risk for the pilots and astronauts flying at the VG SpaceShipTwo up to 85.1 1 km altitude.
{"title":"Space radiation measured during first-ever commercial suborbital mission on Virgin Galactic SpaceShipTwo Unity on 29 June 2023","authors":"Tsvetan Dachev ,&nbsp;Pantaleone Carlucci ,&nbsp;Francesco Cairo ,&nbsp;Borislav Tomov ,&nbsp;Yuri Matviichuk ,&nbsp;Plamen Dimitrov ,&nbsp;Mityo Mitev ,&nbsp;Malina Jordanova ,&nbsp;Lucia Paciucci","doi":"10.1016/j.lssr.2024.09.003","DOIUrl":"10.1016/j.lssr.2024.09.003","url":null,"abstract":"<div><div>The paper presents the variations of space radiation (primary and secondary galactic cosmic rays (GCR) absorbed dose rate in silicon and flux) measured during the first-ever commercial suborbital flight of the Virgin Galactic (VG) SpaceShipTwo Unity on 29 June 2023. A Portable Dosimeter-Spectrometer Liulin-CNR-VG is used. It is developed in the Space Research and Technology Institute, Bulgarian Academy of Sciences (SRTI-BAS) under a scientific contract with National Research Council of Italy (CNR), Italy. Liulin-CNR-VG size is 63х54 × 23 mm. Its weight is 0.092 kg. During the first part of the SpaceShipTwo flight, up to 14.4 km, the dose rate rises from 0.058 μGy h<sup>-1</sup> up to 2.5 μGy h<sup>-1</sup>. Above the altitude of 30 km, the dose rate falls to 2.2 μGy h<sup>-1</sup>, while the dose to flux ratio increases to values about 1.0 nGy cm<sup>2</sup> particle<sup>-1</sup>. The latter confirms the outcomes of previous balloon experiments, i.e. the change of the composition of the radiation field of the GCR and secondary radiation source from predominantly light particles as electrons, pions and muons towards heavier particles as protons and neutrons. On the descending part of the flight, one maximum in the flux and dose rate curves is obtained as Regener-Pfotzer maximum (R-PM). The flux calculated by the moving avervage is equal to 1.2 cm<sup>-2</sup> s<sup>-1</sup> and the dose rate is equal to 2.9 μGy h<sup>-1</sup> at an altitude of 13 km. These values are well in line with those expected in conditions of relatively high solar activity, such as during the flight. The dose rates measured by Liulin-CNR-VG are in good agreement with other Liulin data, such as those recorded during balloon flights in 2005 and 2015 and civil aviation flights. The calculated total equivalent dose rate during the VG SpaceShipTwo flight is 7.46 μSv for 1.22 h. This reveals that there is a very small radiation risk for the pilots and astronauts flying at the VG SpaceShipTwo up to 85.1 1 km altitude.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 126-133"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047204","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Moxifloxacin plus Cordyceps polysaccharide ameliorate intestinal barrier damage due to abdominal infection via anti-inflammation and immune regulation under simulated microgravity 在模拟微重力环境下,莫西沙星加冬虫夏草多糖可通过抗炎和免疫调节改善腹腔感染导致的肠屏障损伤。
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.11.005
Hong-Yun Nie , Jun Ge , Kai-Ge Liu , Yuan Yue , Hao Li , Hai-Guan Lin , Tao Zhang , Hong-Feng Yan , Bing-Xin Xu , Hong-Wei Sun , Jian-Wu Yang , Shao-Yan Si , Jin-Lian Zhou , Yan Cui
<div><h3>Background</h3><div>Currently, there is limited research on the impact of abdominal infection on intestinal damage under microgravity conditions. Cordyceps polysaccharide (CPS), the main active ingredient of Cordyceps, has demonstrated various pharmacological effects, including anti-inflammatory, antioxidant, and immunomodulatory properties. Moxifloxacin (MXF) is a fourth-generation quinolone antibiotic that is believed to have a dual regulatory effect on immune system activation and suppression. Our objective was to investigate the effects of MXF plus CPS on the intestinal barrier damage due to abdominal infection under microgravity.</div></div><div><h3>Methods</h3><div>The hindlimb unloading model in rats was employed to simulate microgravity. The rat model of abdominal infection was established by cecal ligation and puncture (CLP). MXF, CPS and the combination of the two drugs were used to treat CLP-rats in simulated microgravity. We assessed histopathological changes of ileum by hematoxylin and eosin staining. The intestinal ultrastructure was observed under transmission electron microscopy. Additionally, the expression of intestinal barrier proteins RegIII α/γ and MUC2 was detected by Western blot analysis, while the localization of these proteins within the ileum was examined using immunohistochemistry. Cytometric bead array (CBA) was employed to detect cytokine including IL-6, TNF-α, IL-1β, IL-1α, CXCL-1, MCP-1, IL-17A, IL-18, and IL-33. Flow cytometry analysis was conducted to determine the percentages of Treg cells, M1 macrophages, M2 macrophages, T cells and CD8<sup>+</sup><em>T</em> cells.</div></div><div><h3>Results</h3><div>The results showed that compared with the normal gravity groups, the simulated microgravity groups exhibited a significant decrease in RegIII α/γ protein expression, an increase in M1 macrophage frequency, and elevated levels of TNF-α, IL-1α, MCP-1 and IL-6. Notably, the combined application of MXF and CPS effectively mitigated intestinal barrier damage in CLP-rats exposed to microgravity, as evidenced by alleviated ultrastructural and pathological impairments in ileum, along with increased expression of key intestinal barrier proteins MUC2 and RegIII α/γ. Furthermore, the combination therapy enhances the proportion of T cells, CD8<sup>+</sup> <em>T</em> cells, and M2 macrophages in septic rats exposed to simulated microgravity while reducing the frequency of Treg cells and M1 macrophages. MXF plus CPS also led to a reduction of proinflammatory cytokines and chemokines, including IL-6, TNF-α, IL-1β, IL-1α, CXCL-1, MCP-1, IL18, and IL33.</div></div><div><h3>Conclusion</h3><div>Our study showed that MXF plus CPS exhibited a protective effect on intestinal barrier damage due to abdominal infection under microgravity, potentially attributed to its anti-inflammatory properties and immune regulatory mechanisms. These findings may provide insights into the development of drugs targeting abdominal infections in t
{"title":"Moxifloxacin plus Cordyceps polysaccharide ameliorate intestinal barrier damage due to abdominal infection via anti-inflammation and immune regulation under simulated microgravity","authors":"Hong-Yun Nie ,&nbsp;Jun Ge ,&nbsp;Kai-Ge Liu ,&nbsp;Yuan Yue ,&nbsp;Hao Li ,&nbsp;Hai-Guan Lin ,&nbsp;Tao Zhang ,&nbsp;Hong-Feng Yan ,&nbsp;Bing-Xin Xu ,&nbsp;Hong-Wei Sun ,&nbsp;Jian-Wu Yang ,&nbsp;Shao-Yan Si ,&nbsp;Jin-Lian Zhou ,&nbsp;Yan Cui","doi":"10.1016/j.lssr.2024.11.005","DOIUrl":"10.1016/j.lssr.2024.11.005","url":null,"abstract":"&lt;div&gt;&lt;h3&gt;Background&lt;/h3&gt;&lt;div&gt;Currently, there is limited research on the impact of abdominal infection on intestinal damage under microgravity conditions. Cordyceps polysaccharide (CPS), the main active ingredient of Cordyceps, has demonstrated various pharmacological effects, including anti-inflammatory, antioxidant, and immunomodulatory properties. Moxifloxacin (MXF) is a fourth-generation quinolone antibiotic that is believed to have a dual regulatory effect on immune system activation and suppression. Our objective was to investigate the effects of MXF plus CPS on the intestinal barrier damage due to abdominal infection under microgravity.&lt;/div&gt;&lt;/div&gt;&lt;div&gt;&lt;h3&gt;Methods&lt;/h3&gt;&lt;div&gt;The hindlimb unloading model in rats was employed to simulate microgravity. The rat model of abdominal infection was established by cecal ligation and puncture (CLP). MXF, CPS and the combination of the two drugs were used to treat CLP-rats in simulated microgravity. We assessed histopathological changes of ileum by hematoxylin and eosin staining. The intestinal ultrastructure was observed under transmission electron microscopy. Additionally, the expression of intestinal barrier proteins RegIII α/γ and MUC2 was detected by Western blot analysis, while the localization of these proteins within the ileum was examined using immunohistochemistry. Cytometric bead array (CBA) was employed to detect cytokine including IL-6, TNF-α, IL-1β, IL-1α, CXCL-1, MCP-1, IL-17A, IL-18, and IL-33. Flow cytometry analysis was conducted to determine the percentages of Treg cells, M1 macrophages, M2 macrophages, T cells and CD8&lt;sup&gt;+&lt;/sup&gt;&lt;em&gt;T&lt;/em&gt; cells.&lt;/div&gt;&lt;/div&gt;&lt;div&gt;&lt;h3&gt;Results&lt;/h3&gt;&lt;div&gt;The results showed that compared with the normal gravity groups, the simulated microgravity groups exhibited a significant decrease in RegIII α/γ protein expression, an increase in M1 macrophage frequency, and elevated levels of TNF-α, IL-1α, MCP-1 and IL-6. Notably, the combined application of MXF and CPS effectively mitigated intestinal barrier damage in CLP-rats exposed to microgravity, as evidenced by alleviated ultrastructural and pathological impairments in ileum, along with increased expression of key intestinal barrier proteins MUC2 and RegIII α/γ. Furthermore, the combination therapy enhances the proportion of T cells, CD8&lt;sup&gt;+&lt;/sup&gt; &lt;em&gt;T&lt;/em&gt; cells, and M2 macrophages in septic rats exposed to simulated microgravity while reducing the frequency of Treg cells and M1 macrophages. MXF plus CPS also led to a reduction of proinflammatory cytokines and chemokines, including IL-6, TNF-α, IL-1β, IL-1α, CXCL-1, MCP-1, IL18, and IL33.&lt;/div&gt;&lt;/div&gt;&lt;div&gt;&lt;h3&gt;Conclusion&lt;/h3&gt;&lt;div&gt;Our study showed that MXF plus CPS exhibited a protective effect on intestinal barrier damage due to abdominal infection under microgravity, potentially attributed to its anti-inflammatory properties and immune regulatory mechanisms. These findings may provide insights into the development of drugs targeting abdominal infections in t","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 23-37"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047191","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Sex-specific effects on the heart from combined exposure to simulated galactic cosmic radiation and hindlimb unloading
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.12.001
A.S. Nemec-Bakk , V. Sridharan , J.S. Willey , I. Koturbash , D.K. Williams , M. Chesal , C.M. Patel , A.M. Borg , K. Reno , G. Gifford , W. Newhauser , J. Williams , J.C. Chancellor , M. Boerma
Future long duration space missions will expose astronauts to higher doses of galactic cosmic radiation (GCR) than those experienced on the international space station. Recent studies have demonstrated astronauts may be at risk for cardiovascular complications due to increased radiation exposure and fluid shift from microgravity. However, there is a lack of direct evidence on how the cardiovascular system is affected by GCR and microgravity since no astronauts have been exposed to exploratory mission relevant GCR doses. Therefore, we utilized a ground-based mouse model to determine the cardiovascular risks for space radiation exposure while the mice were simultaneously hindlimb suspended to mimic microgravity. 6-month-old male and female C57BL/6 mice were exposed to an absorbed dose of 0 Gy, 0.5 Gy, or 1.5 Gy simulated GCR (GCRsim) that comprised beams of 5 ions at NASA's Space Radiation Laboratory. Subcohorts of mice were hindlimb unloaded (HLU), starting 5 days before GCRsim until the completion of radiation exposure. GCRsim + HLU was performed over 8 hours (0.5 Gy) or 24 hours (1.5 Gy). After completion of GCRsim and HLU, mice were shipped to UAMS for long-term observation. Cardiac function was measured using high resolution ultrasound at 6 and 9 months after exposure. Tissues were collected after the final ultrasound and prepared for further analysis. Female mice exposed to 1.5 Gy + HLU demonstrated a significant increase in body weight compared to ground controls months after GCR exposure; however, there was no change in male body weights. Cardiac ultrasound revealed 0.5 Gy GCRsim decreased left ventricular (LV) mass, LV posterior wall thickness in diastole, and systole in males 6 months after exposure. In females, 1.5 Gy + HLU significantly increased LV posterior wall thickness in diastole and systole at 6 months. These changes in ultrasound measurements were no longer seen at 9 months. Moreover, at 9 months there was no change in total collagen content or density of the capillary network in the heart. Lastly, the combination of GCRsim and HLU influenced immune cell markers in the heart of female mice. These data suggest that combined simulated GCR and microgravity result in minor, yet statistically significant sex-dependent changes to body weight and cardiac structure.
{"title":"Sex-specific effects on the heart from combined exposure to simulated galactic cosmic radiation and hindlimb unloading","authors":"A.S. Nemec-Bakk ,&nbsp;V. Sridharan ,&nbsp;J.S. Willey ,&nbsp;I. Koturbash ,&nbsp;D.K. Williams ,&nbsp;M. Chesal ,&nbsp;C.M. Patel ,&nbsp;A.M. Borg ,&nbsp;K. Reno ,&nbsp;G. Gifford ,&nbsp;W. Newhauser ,&nbsp;J. Williams ,&nbsp;J.C. Chancellor ,&nbsp;M. Boerma","doi":"10.1016/j.lssr.2024.12.001","DOIUrl":"10.1016/j.lssr.2024.12.001","url":null,"abstract":"<div><div>Future long duration space missions will expose astronauts to higher doses of galactic cosmic radiation (GCR) than those experienced on the international space station. Recent studies have demonstrated astronauts may be at risk for cardiovascular complications due to increased radiation exposure and fluid shift from microgravity. However, there is a lack of direct evidence on how the cardiovascular system is affected by GCR and microgravity since no astronauts have been exposed to exploratory mission relevant GCR doses. Therefore, we utilized a ground-based mouse model to determine the cardiovascular risks for space radiation exposure while the mice were simultaneously hindlimb suspended to mimic microgravity. 6-month-old male and female C57BL/6 mice were exposed to an absorbed dose of 0 Gy, 0.5 Gy, or 1.5 Gy simulated GCR (GCRsim) that comprised beams of 5 ions at NASA's Space Radiation Laboratory. Subcohorts of mice were hindlimb unloaded (HLU), starting 5 days before GCRsim until the completion of radiation exposure. GCRsim + HLU was performed over 8 hours (0.5 Gy) or 24 hours (1.5 Gy). After completion of GCRsim and HLU, mice were shipped to UAMS for long-term observation. Cardiac function was measured using high resolution ultrasound at 6 and 9 months after exposure. Tissues were collected after the final ultrasound and prepared for further analysis. Female mice exposed to 1.5 Gy + HLU demonstrated a significant increase in body weight compared to ground controls months after GCR exposure; however, there was no change in male body weights. Cardiac ultrasound revealed 0.5 Gy GCRsim decreased left ventricular (LV) mass, LV posterior wall thickness in diastole, and systole in males 6 months after exposure. In females, 1.5 Gy + HLU significantly increased LV posterior wall thickness in diastole and systole at 6 months. These changes in ultrasound measurements were no longer seen at 9 months. Moreover, at 9 months there was no change in total collagen content or density of the capillary network in the heart. Lastly, the combination of GCRsim and HLU influenced immune cell markers in the heart of female mice. These data suggest that combined simulated GCR and microgravity result in minor, yet statistically significant sex-dependent changes to body weight and cardiac structure.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 38-46"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047200","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Biofilm dynamics in space and their potential for sustainable space exploration – A comprehensive review 空间生物膜动力学及其在可持续空间探索中的潜力--综合评述
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.08.006
V G Sowmeya, Mythili Sathiavelu
Microbial biofilms are universal. The intricate tapestry of biofilms has remarkable implications for the environment, health, and industrial processes. The field of space microbiology is actively investigating the effects of microgravity on microbes, and discoveries are constantly being made. Recent evidence suggests that extraterrestrial environments also fuel the biofilm formation. Understanding the biofilm mechanics under microgravitational conditions is crucial at this stage and could have an astounding impact on inter-planetary missions. This review systematically examines the existing understanding of biofilm development in space and provides insight into how molecules, physiology, or environmental factors influence biofilm formation during microgravitational conditions. In addition, biocontrol strategies targeting the formation and dispersal of biofilms in space environments are explored. In particular, the article highlights the potential benefits of using microbial biofilms in space for bioremediation, life support systems, and biomass production applications.
微生物生物膜具有普遍性。错综复杂的生物膜对环境、健康和工业流程有着显著的影响。太空微生物学领域正在积极研究微重力对微生物的影响,并不断有新的发现。最近的证据表明,地外环境也会促进生物膜的形成。在现阶段,了解微重力条件下的生物膜力学至关重要,可能会对星际飞行任务产生惊人的影响。本综述系统地研究了对太空生物膜发展的现有认识,并深入探讨了分子、生理或环境因素如何影响微重力条件下生物膜的形成。此外,还探讨了针对太空环境中生物膜的形成和扩散的生物控制策略。文章特别强调了在太空中利用微生物生物膜进行生物修复、生命支持系统和生物质生产应用的潜在益处。
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引用次数: 0
Integrated spaceflight transcriptomic analyses and simulated space experiments reveal key molecular features and functional changes driven by space stressors in space-flown C. elegans 综合太空飞行转录组分析和模拟太空实验揭示了在太空飞行的秀丽隐杆线虫的关键分子特征和由太空压力驱动的功能变化。
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.11.004
Ge Zhang, Lei Zhao, Zejun Li, Yeqing Sun
The space environment presents unique stressors, such as microgravity and space radiation, which can induce molecular and physiological changes in living organisms. To identify key reproducible transcriptomic features and explore potential biological roles in space-flown C. elegans, we integrated transcriptomic data from C. elegans subjected to four spaceflights aboard the International Space Station (ISS) and identified 32 reproducibly differentially expressed genes (DEGs). These DEGs were enriched in pathways related to the structural constituent of cuticle, defense response, unfolded protein response, longevity regulation, extracellular structural organization, and signal receptor regulation. Among these 32 DEGs, 13 genes were consistently downregulated across four spaceflight conditions, primarily associated with the structural constituent of the cuticle. The remaining genes, involved in defense response, unfolded protein response, and longevity regulation pathway, exhibited distinct patterns depending on spaceflight duration: they were downregulated during short-term spaceflights but upregulated during long-term spaceflights. To explore the potential space stressors responsible for these transcriptomic changes, we performed qRT-PCR experiments on C. elegans exposed to simulated microgravity and low-dose radiation. Our results demonstrated that cuticle-related gene expression was significantly downregulated under both simulated microgravity and low-dose radiation conditions. In contrast, almost all genes involved in defense response, unfolded protein response, and longevity regulation pathway were downregulated under simulated microgravity but upregulated under low-dose radiation exposure. These findings suggest that both microgravity and space radiation inhibit cuticle formation; microgravity as the primary stressor inhibit defense response, unfolded protein response, and longevity regulation pathway during short-term spaceflights, while space radiation may promote these processes during long-term spaceflights. In summary, through integrated spaceflight transcriptomic analyses and simulated space experiments, we identified key transcriptomic features and potential biological functions in space-flown C. elegans, shedding light on the space stressors responsible for these changes. This study provides new insights into the molecular and physiological adaptations of C. elegans to spaceflight, highlighting the distinct impacts of microgravity and space radiation.
{"title":"Integrated spaceflight transcriptomic analyses and simulated space experiments reveal key molecular features and functional changes driven by space stressors in space-flown C. elegans","authors":"Ge Zhang,&nbsp;Lei Zhao,&nbsp;Zejun Li,&nbsp;Yeqing Sun","doi":"10.1016/j.lssr.2024.11.004","DOIUrl":"10.1016/j.lssr.2024.11.004","url":null,"abstract":"<div><div>The space environment presents unique stressors, such as microgravity and space radiation, which can induce molecular and physiological changes in living organisms. To identify key reproducible transcriptomic features and explore potential biological roles in space-flown <em>C. elegans</em>, we integrated transcriptomic data from <em>C. elegans</em> subjected to four spaceflights aboard the International Space Station (ISS) and identified 32 reproducibly differentially expressed genes (DEGs). These DEGs were enriched in pathways related to the structural constituent of cuticle, defense response, unfolded protein response, longevity regulation, extracellular structural organization, and signal receptor regulation. Among these 32 DEGs, 13 genes were consistently downregulated across four spaceflight conditions, primarily associated with the structural constituent of the cuticle. The remaining genes, involved in defense response, unfolded protein response, and longevity regulation pathway, exhibited distinct patterns depending on spaceflight duration: they were downregulated during short-term spaceflights but upregulated during long-term spaceflights. To explore the potential space stressors responsible for these transcriptomic changes, we performed qRT-PCR experiments on <em>C. elegans</em> exposed to simulated microgravity and low-dose radiation. Our results demonstrated that cuticle-related gene expression was significantly downregulated under both simulated microgravity and low-dose radiation conditions. In contrast, almost all genes involved in defense response, unfolded protein response, and longevity regulation pathway were downregulated under simulated microgravity but upregulated under low-dose radiation exposure. These findings suggest that both microgravity and space radiation inhibit cuticle formation; microgravity as the primary stressor inhibit defense response, unfolded protein response, and longevity regulation pathway during short-term spaceflights, while space radiation may promote these processes during long-term spaceflights. In summary, through integrated spaceflight transcriptomic analyses and simulated space experiments, we identified key transcriptomic features and potential biological functions in space-flown <em>C. elegans</em>, shedding light on the space stressors responsible for these changes. This study provides new insights into the molecular and physiological adaptations of <em>C. elegans</em> to spaceflight, highlighting the distinct impacts of microgravity and space radiation.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 10-22"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047187","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Space biological and human survival: Investigations into plants, animals, microorganisms and their components and bioregenerative life support systems
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.10.007
Lin Cheng , Yitong Li , Jing Yan
Space life science has been a frontier discipline in the life sciences, aiming to study the life phenomena of earth organisms and their activity patterns under the special environment of space. This review summarizes studies in various key topics in space life science, namely, how microbiome changes in humans and plants, the development of space agriculture and the use of animal, plant and cell models to study the effect of space environments on physiology. We highlight the new possibilities of using high-quality protein crystals uniquely available when grown under space conditions to aid drug development on earth, and the state-of-the-art Bioregenerative Life Support Systems (BLSS) to achieve long term human survival in space.
{"title":"Space biological and human survival: Investigations into plants, animals, microorganisms and their components and bioregenerative life support systems","authors":"Lin Cheng ,&nbsp;Yitong Li ,&nbsp;Jing Yan","doi":"10.1016/j.lssr.2024.10.007","DOIUrl":"10.1016/j.lssr.2024.10.007","url":null,"abstract":"<div><div>Space life science has been a frontier discipline in the life sciences, aiming to study the life phenomena of earth organisms and their activity patterns under the special environment of space. This review summarizes studies in various key topics in space life science, namely, how microbiome changes in humans and plants, the development of space agriculture and the use of animal, plant and cell models to study the effect of space environments on physiology. We highlight the new possibilities of using high-quality protein crystals uniquely available when grown under space conditions to aid drug development on earth, and the state-of-the-art Bioregenerative Life Support Systems (BLSS) to achieve long term human survival in space.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 143-153"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047201","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
The Effects of Cosmic Radiation Exposure on Pregnancy During a Probable Manned Mission to Mars
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.10.008
Abdurrahman Engin Demir , Elif Nur Sevinc , Mustafa Ulubay
Space missions have revealed certain disincentive factors of this unique environment, such as microgravity, cosmic radiation, etc., as the aerospace industry has made substantial progress in exploring deep space and its impacts on human body. Galactic cosmic radiation (GCR), a form of ionizing radiation, is one of those environmental factors that has potential health implications and, as a result, may limit the duration – and possibly the occurrence – of deep-space missions. High doses of cosmic radiation exposure during spaceflight, particularly during exploration class missions, may have teratogenic effects on a developing fetus, if an unintended pregnancy occurs shortly before or during the flight. This study aimed to discuss whether the cumulative dosage for a pregnant woman during a probable manned mission to Mars may exceed the terrestrial teratogenic radiation limit. A variety of studies, technical documents, and publications that provided flight duration data and the absorbed cosmic radiation dosage equivalents between Earth and Mars were analyzed. A literature-based hypothetical model of a pregnancy simulation over a 6-month spaceflight was also designed to estimate the cumulative absorbed GCR dose. The estimated dose rates ranged from 90 to 324 mSv. Assuming that a pregnant crew member is exposed to this dosage range, the total teratogenic dose equivalent to the embryo/fetus appear to be significantly higher than that of the National Council on Radiation Protection (NCRP)’s and United States Nuclear Regulatory Commission (USNRC)’s recommendations, which state a maximum radiation dose of 5 mSv for the duration of the pregnancy, and thus such an exceeded dose may likely result in teratogenesis. Current protective strategies may not be sufficient to protect the human genome from the detrimental effects of cosmic radiation, and they need be improved for long-term interplanetary travels during human colonization of Mars.
{"title":"The Effects of Cosmic Radiation Exposure on Pregnancy During a Probable Manned Mission to Mars","authors":"Abdurrahman Engin Demir ,&nbsp;Elif Nur Sevinc ,&nbsp;Mustafa Ulubay","doi":"10.1016/j.lssr.2024.10.008","DOIUrl":"10.1016/j.lssr.2024.10.008","url":null,"abstract":"<div><div>Space missions have revealed certain disincentive factors of this unique environment, such as microgravity, cosmic radiation, etc., as the aerospace industry has made substantial progress in exploring deep space and its impacts on human body. Galactic cosmic radiation (GCR), a form of ionizing radiation, is one of those environmental factors that has potential health implications and, as a result, may limit the duration – and possibly the occurrence – of deep-space missions. High doses of cosmic radiation exposure during spaceflight, particularly during exploration class missions, may have teratogenic effects on a developing fetus, if an unintended pregnancy occurs shortly before or during the flight. This study aimed to discuss whether the cumulative dosage for a pregnant woman during a probable manned mission to Mars may exceed the terrestrial teratogenic radiation limit. A variety of studies, technical documents, and publications that provided flight duration data and the absorbed cosmic radiation dosage equivalents between Earth and Mars were analyzed. A literature-based hypothetical model of a pregnancy simulation over a 6-month spaceflight was also designed to estimate the cumulative absorbed GCR dose. The estimated dose rates ranged from 90 to 324 mSv. Assuming that a pregnant crew member is exposed to this dosage range, the total teratogenic dose equivalent to the embryo/fetus appear to be significantly higher than that of the National Council on Radiation Protection (NCRP)’s and United States Nuclear Regulatory Commission (USNRC)’s recommendations, which state a maximum radiation dose of 5 mSv for the duration of the pregnancy, and thus such an exceeded dose may likely result in teratogenesis. Current protective strategies may not be sufficient to protect the human genome from the detrimental effects of cosmic radiation, and they need be improved for long-term interplanetary travels during human colonization of Mars.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 154-162"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047223","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Anthocyanin can improve the survival of rice seeds from solar light outside the international space station
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.10.010
Manabu Sugimoto , Masahiko Maekawa , Hajime Mita , Shin-ichi Yokobori
A purple-pigmented (purple) rice seeds containing an anthocyanin, a major class of flavonoids, and their isogenic non-pigmented (white) seeds were exposed outside of the international space station (ISS) to evaluate the impact of anthocyanin on seed viability in space. The rice seeds were placed in sample plates at the exposed facility of ISS for 440 days, with the bottom layer seeds exposed to space radiation and the top layer seeds exposed to both solar light and space radiation. Though the seed weight of both purple and white seeds decreased after exposure to outer space, growth percentages after germination of purple and white seeds in the top layer were 55 and 15 %, respectively, compared to those in the bottom layer 100 and 70 %, respectively. RNA analysis revealed that 1,590 and 1,546 seed-stored mRNAs (long-lived mRNAs) were degraded in the white seeds of the top and the bottom layers, respectively, whereas those of the purple seeds in the top and bottom layers were 548 and 303, respectively. These results suggest that anthocyanin protected seeds and safeguarded long-lived mRNAs from solar light and space radiation to increase the seed viability.
{"title":"Anthocyanin can improve the survival of rice seeds from solar light outside the international space station","authors":"Manabu Sugimoto ,&nbsp;Masahiko Maekawa ,&nbsp;Hajime Mita ,&nbsp;Shin-ichi Yokobori","doi":"10.1016/j.lssr.2024.10.010","DOIUrl":"10.1016/j.lssr.2024.10.010","url":null,"abstract":"<div><div>A purple-pigmented (purple) rice seeds containing an anthocyanin, a major class of flavonoids, and their isogenic non-pigmented (white) seeds were exposed outside of the international space station (ISS) to evaluate the impact of anthocyanin on seed viability in space. The rice seeds were placed in sample plates at the exposed facility of ISS for 440 days, with the bottom layer seeds exposed to space radiation and the top layer seeds exposed to both solar light and space radiation. Though the seed weight of both purple and white seeds decreased after exposure to outer space, growth percentages after germination of purple and white seeds in the top layer were 55 and 15 %, respectively, compared to those in the bottom layer 100 and 70 %, respectively. RNA analysis revealed that 1,590 and 1,546 seed-stored mRNAs (long-lived mRNAs) were degraded in the white seeds of the top and the bottom layers, respectively, whereas those of the purple seeds in the top and bottom layers were 548 and 303, respectively. These results suggest that anthocyanin protected seeds and safeguarded long-lived mRNAs from solar light and space radiation to increase the seed viability.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 79-85"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047164","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Galactic cosmic ray environment predictions for the NASA BioSentinel Mission, part 2:Post-mission validation NASA 生物哨兵任务的银河宇宙射线环境预测,第 2 部分:任务后验证。
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.10.006
Shirin Rahmanian , Tony C. Slaba , Stuart George , Leslie A. Braby , Sharmila Bhattacharya , Tore Straume , Sergio R. Santa Maria
The BioSentinel CubeSat was deployed on the Artemis-I mission in November 2022 and has been continuously transmitting physical measurements of the space radiation environment since that time. Just before mission launch, we published computational model predictions of the galactic cosmic ray exposure expected inside BioSentinel for multiple locations and configurations. The predictions utilized models for the ambient galactic cosmic ray environment, radiation physics and transport, and BioSentinel geometry. Now that the nominal six-month BioSentinel mission has completed and some additional time has passed, those pre-launch predictions and additional model components can be validated. Dose-rate and linear energy transfer (LET) spectral measurements from the on-board dosimeter are presented along with a summary of the computational models used to calculate exposure quantities of interest. Sensitivity tests are performed to gauge the impact of various model choices on these quantities. Satellite data collected during the BioSentinel mission are used to provide some measure of independent validation for the galactic cosmic ray model used in the present calculations. It is shown that the combined models are in excellent agreement with the measured dose-rate. Model calculations agree well with measurement below ∼10 keV/µm and underpredict at higher LET. It is argued that the underprediction is likely due to detector response or low energy anomalous cosmic ray contributions able to reach the thinly shielded side of the on-board dosimeter.
{"title":"Galactic cosmic ray environment predictions for the NASA BioSentinel Mission, part 2:Post-mission validation","authors":"Shirin Rahmanian ,&nbsp;Tony C. Slaba ,&nbsp;Stuart George ,&nbsp;Leslie A. Braby ,&nbsp;Sharmila Bhattacharya ,&nbsp;Tore Straume ,&nbsp;Sergio R. Santa Maria","doi":"10.1016/j.lssr.2024.10.006","DOIUrl":"10.1016/j.lssr.2024.10.006","url":null,"abstract":"<div><div>The BioSentinel CubeSat was deployed on the Artemis-I mission in November 2022 and has been continuously transmitting physical measurements of the space radiation environment since that time. Just before mission launch, we published computational model predictions of the galactic cosmic ray exposure expected inside BioSentinel for multiple locations and configurations. The predictions utilized models for the ambient galactic cosmic ray environment, radiation physics and transport, and BioSentinel geometry. Now that the nominal six-month BioSentinel mission has completed and some additional time has passed, those pre-launch predictions and additional model components can be validated. Dose-rate and linear energy transfer (LET) spectral measurements from the on-board dosimeter are presented along with a summary of the computational models used to calculate exposure quantities of interest. Sensitivity tests are performed to gauge the impact of various model choices on these quantities. Satellite data collected during the BioSentinel mission are used to provide some measure of independent validation for the galactic cosmic ray model used in the present calculations. It is shown that the combined models are in excellent agreement with the measured dose-rate. Model calculations agree well with measurement below ∼10 keV/µm and underpredict at higher LET. It is argued that the underprediction is likely due to detector response or low energy anomalous cosmic ray contributions able to reach the thinly shielded side of the on-board dosimeter.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 134-142"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047169","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
Dose measurements with the Pille-ISS thermoluminescent dosimeter system during extravehicular activities (2004-2022)
IF 2.9 3区 生物学 Q2 ASTRONOMY & ASTROPHYSICS Pub Date : 2025-02-01 DOI: 10.1016/j.lssr.2024.12.005
Patrik Pinczés , Attila Hirn , István Apáthy , Sándor Deme , Konstantin O. Inozemtsev , Olga A. Ivanova , Vyacheslav A. Shurshakov
One of the most problematic goals for radiation safety during spaceflight is an assessment of additional doses received by astronauts during extravehicular activity (EVA). The Pille-ISS thermoluminescent dosimeter developed by the predecessor of the Hungarian Research Network (HUN-REN) Centre for Energy Research (Budapest, Hungary) is designed for the routine dose measurements not only inside the spacecraft compartments, but also for personal dosimetric control for EVA. During almost two decades of the International Space Station (ISS) operation, the unique set of 131 EVA doses were recorded in different conditions, such as: solar activity, ISS trajectory along the South Atlantic Anomaly (SAA), and shielding conditions provided by two kinds of spacesuits: the Extravehicular Mobility Unit (EMU) and Orlan.
The EVA dose rates during the normal scenario (without SAA crossing during EVA) are: 26 μGy/h on average, with maximum value of 118 μGy/h for the EMU spacesuit; and 103 μGy/h on average, with maximum value of 255 μGy/h for the Orlan spacesuit. However, the corresponding EVA dose can increase by about 33% on average regardless the spacesuit type, depending on time spent in SAA. The worst case mean EVA dose is equivalent to 7 days inside the ISS with 2.423 mGy. In general, the possible additional radiation risk due to the EVA is small in comparison with typical half-year mission onboard the ISS.
The long-term experience of EVA dose assessments with Pille-ISS dosimeter shows that in some cases the skin dose can be underestimated due to the excessive shielding of the standard Pille-ISS dosimeter. To solve this problem, the modified Pille-ISS dosimeters with significantly reduced shielding are developed and involved onboard the ISS for the dose measurements starting from 2023.
{"title":"Dose measurements with the Pille-ISS thermoluminescent dosimeter system during extravehicular activities (2004-2022)","authors":"Patrik Pinczés ,&nbsp;Attila Hirn ,&nbsp;István Apáthy ,&nbsp;Sándor Deme ,&nbsp;Konstantin O. Inozemtsev ,&nbsp;Olga A. Ivanova ,&nbsp;Vyacheslav A. Shurshakov","doi":"10.1016/j.lssr.2024.12.005","DOIUrl":"10.1016/j.lssr.2024.12.005","url":null,"abstract":"<div><div>One of the most problematic goals for radiation safety during spaceflight is an assessment of additional doses received by astronauts during extravehicular activity (EVA). The Pille-ISS thermoluminescent dosimeter developed by the predecessor of the Hungarian Research Network (HUN-REN) Centre for Energy Research (Budapest, Hungary) is designed for the routine dose measurements not only inside the spacecraft compartments, but also for personal dosimetric control for EVA. During almost two decades of the International Space Station (ISS) operation, the unique set of 131 EVA doses were recorded in different conditions, such as: solar activity, ISS trajectory along the South Atlantic Anomaly (SAA), and shielding conditions provided by two kinds of spacesuits: the Extravehicular Mobility Unit (EMU) and Orlan.</div><div>The EVA dose rates during the normal scenario (without SAA crossing during EVA) are: 26 <span><math><mi>μ</mi></math></span>Gy/h on average, with maximum value of 118 <span><math><mi>μ</mi></math></span>Gy/h for the EMU spacesuit; and 103 <span><math><mi>μ</mi></math></span>Gy/h on average, with maximum value of 255 <span><math><mi>μ</mi></math></span>Gy/h for the Orlan spacesuit. However, the corresponding EVA dose can increase by about 33% on average regardless the spacesuit type, depending on time spent in SAA. The worst case mean EVA dose is equivalent to <span><math><mo>∼</mo></math></span> 7 days inside the ISS with 2.423 mGy. In general, the possible additional radiation risk due to the EVA is small in comparison with typical half-year mission onboard the ISS.</div><div>The long-term experience of EVA dose assessments with Pille-ISS dosimeter shows that in some cases the skin dose can be underestimated due to the excessive shielding of the standard Pille-ISS dosimeter. To solve this problem, the modified Pille-ISS dosimeters with significantly reduced shielding are developed and involved onboard the ISS for the dose measurements starting from 2023.</div></div>","PeriodicalId":18029,"journal":{"name":"Life Sciences in Space Research","volume":"44 ","pages":"Pages 58-63"},"PeriodicalIF":2.9,"publicationDate":"2025-02-01","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":null,"resultStr":null,"platform":"Semanticscholar","paperid":"143047166","PeriodicalName":null,"FirstCategoryId":null,"ListUrlMain":null,"RegionNum":3,"RegionCategory":"生物学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":"OA","EPubDate":null,"PubModel":null,"JCR":null,"JCRName":null,"Score":null,"Total":0}
引用次数: 0
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Life Sciences in Space Research
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