Large SPEs, especially when the shielding is inadequate, not only increase the risk of cancer, but also the possibility of occurrence of acute radiation syndrome (ARS). As physical shielding alone cannot solve current space radiation problems, in 2003 we introduced the adaptive response as an efficient model of biological protection. The development of this model is discussed in our recent publications. A recently published paper, authored by 30 scientists from countries such as US, UK, Russia, and Belgium has confirmed the need for selection of astronauts based on their adaptive response (this paper cites our reports on how AR helps choosing the astronauts for a deep space mission). Moreover, A NASA report published in 2016 has cited our early report on the importance of radioadaptive response in space missions and states that cells can be expected to be exposed to multiple hits of protons before being traversed by an HZE particle. However, substantial evidence showing that SPEs are a real concern, indicate that our proposed model is more applicable and evidence-based. Regarding the risk of infection, change of the virulence (ability to cause disease) of microorganisms and astronauts’ dysregulated immune system, significantly increases the infection risk in deep space missions.
Strategies for reducing the risk of radiation for astronauts in space mission...SMJ Mortazavi
Exposure to high levels of space radiation and microgravity are two important concerns which need to be addressed before any long-term manned space mission. There are also reports showing that microgravity, through a synergistic effect, increases the radiation susceptibility of living organisms. Other researchers as well as our team have conducted some experiments on design and fabrication of appropriate radiation shields for spacecrafts. However, due to some cardinal barriers such as weight limitations and extreme inadequacy of current physical shields during extravehicular activity, we strongly believe that the physical shielding alone cannot solve the problem of potential exposure to high levels of radiation in a long-term space mission.
Therefore, over the past several years, we focused on two solutions; radioadaptive response and other biological-based radiation protection methods. Adaptive response, that is the increased radioresistance in cells or living organisms pre-exposed to a low adapting dose and then exposed to a high challenging dose, was firstly proposed by our team in 2003 as an effective method. This novel idea later formed the basis of many space radiation biology projects around the world.
Furthermore, conventional radioprotectors cannot efficiently be used in space due to limitations such as their considerable toxicity and the very narrow time window for their effective use (radioprotectors should be used before or at the time of exposure, while astronauts cannot estimate their doses before a solar particle event). Therefore, we focused on introducing natural radiation mitigators which could be efficiently used several hours after exposure (e.g. when a solar particle event subsides and astronauts are able to estimate their doses). In these experiments, radiation mitigators were introduced by our team which could be used even 24 hours after exposure to high levels of radiation caused by unpredictable sources such as SPEs.
Finally, some of our recent experiments were aimed at finding methods which could lead to boosting the immune system of astronauts during long-term missions. We investigated the effect of RF-EMFs-induced adaptive responses on immune system modulation in a mouse model of hindlimb unloading (HU). Hindlimb unloading rodent model is widely accepted by the scientific community as the model of choice for simulating spaceflight. In this study, serum levels of T helper cytokines were determined in HU mice, RF-EMF treated mice and HU mice pre-exposed to RF-EMF compared to those of untreated controls. The findings of this study will be published soon.
LEO Commercialization: Space-based Research and Development and Manufacturing ISSRDC
By the end of 2017, NASA plans to purchase both crew and cargo delivery services to the International Space Station from commercial suppliers. Near the planned end-of-life for ISS, NASA intends to transition low Earth orbit (LEO) operations from government-led to commercially-driven as a result of greater involvement from the private sector. CASIS has seen increasing demand for use of the ISS National Lab to support research and development in numerous fields. This session will highlight the R&D opportunities in low Earth orbit ranging from LEO commercialization efforts related to advancing protein crystal growth studies for drug discovery and delivery; stem cell, organs-on-chips, and vascularized tissue research for organ bioengineering; and use of 3D printing capabilities and superior optical fiber manufacturing for on-orbit production.
Anatomy of a Megathrust Earthquake Rupture - The 2010 M8.8 Chile QuakeStephen Hicks
Presented for an IRIS (Incorporated Research Institutions for Seismology) webinar on 9 April 2014.
Webinar can be viewed here: https://www.youtube.com/watch?v=MNcl5AZlX3k
Abstract: In February 2010, a magnitude 8.8 megathrust earthquake struck the Maule region of Central Chile - the sixth largest earthquake ever recorded. It is fast becoming one of the best-studied megathrust ruptures, allowing us a unique insight into the inner workings of subduction zone earthquakes. In the earthquake’s immediate aftermath, an international group of research institutions deployed geophysical instruments in the rupture area. A network of ~160 seismic stations on the forearc recorded over 50,000 aftershocks in the first 10 months following the earthquake.
I have used observations of P- and S-waves from aftershocks to derive a high-resolution seismic travel-time tomography of the rupture zone. Observations from ocean-bottom seismometers further improve image sharpness in the offshore portion of the seismogenic zone, where most slip occurred during the earthquake. The tomographic images reveal the distribution of P-wave velocity and Poisson’s Ratio within the earthquake rupture zone. Based on accurate aftershock locations and moment tensors, I have defined a new 3-D plate interface geometry to infer the physical structure and composition along the plate interface. I compare these velocities with the mainly geodetically observed behaviour of the fault throughout a cycle of seismic behaviour (preseismic locking, coseismic slip, postseismic deformation). This comparison allows us to understand some of the physical properties that may govern seismogenesis along the megathrust. I will reveal how both the long-lived geological structure of the forearc and the composition of the subducting oceanic plate may influence the rupture behaviour of large megathrust earthquakes. An understanding of seismic velocities along the megathrust may therefore be used to constrain the seismogenic potential of subduction zones worldwide.
Strategies for reducing the risk of radiation for astronauts in space mission...SMJ Mortazavi
Exposure to high levels of space radiation and microgravity are two important concerns which need to be addressed before any long-term manned space mission. There are also reports showing that microgravity, through a synergistic effect, increases the radiation susceptibility of living organisms. Other researchers as well as our team have conducted some experiments on design and fabrication of appropriate radiation shields for spacecrafts. However, due to some cardinal barriers such as weight limitations and extreme inadequacy of current physical shields during extravehicular activity, we strongly believe that the physical shielding alone cannot solve the problem of potential exposure to high levels of radiation in a long-term space mission.
Therefore, over the past several years, we focused on two solutions; radioadaptive response and other biological-based radiation protection methods. Adaptive response, that is the increased radioresistance in cells or living organisms pre-exposed to a low adapting dose and then exposed to a high challenging dose, was firstly proposed by our team in 2003 as an effective method. This novel idea later formed the basis of many space radiation biology projects around the world.
Furthermore, conventional radioprotectors cannot efficiently be used in space due to limitations such as their considerable toxicity and the very narrow time window for their effective use (radioprotectors should be used before or at the time of exposure, while astronauts cannot estimate their doses before a solar particle event). Therefore, we focused on introducing natural radiation mitigators which could be efficiently used several hours after exposure (e.g. when a solar particle event subsides and astronauts are able to estimate their doses). In these experiments, radiation mitigators were introduced by our team which could be used even 24 hours after exposure to high levels of radiation caused by unpredictable sources such as SPEs.
Finally, some of our recent experiments were aimed at finding methods which could lead to boosting the immune system of astronauts during long-term missions. We investigated the effect of RF-EMFs-induced adaptive responses on immune system modulation in a mouse model of hindlimb unloading (HU). Hindlimb unloading rodent model is widely accepted by the scientific community as the model of choice for simulating spaceflight. In this study, serum levels of T helper cytokines were determined in HU mice, RF-EMF treated mice and HU mice pre-exposed to RF-EMF compared to those of untreated controls. The findings of this study will be published soon.
LEO Commercialization: Space-based Research and Development and Manufacturing ISSRDC
By the end of 2017, NASA plans to purchase both crew and cargo delivery services to the International Space Station from commercial suppliers. Near the planned end-of-life for ISS, NASA intends to transition low Earth orbit (LEO) operations from government-led to commercially-driven as a result of greater involvement from the private sector. CASIS has seen increasing demand for use of the ISS National Lab to support research and development in numerous fields. This session will highlight the R&D opportunities in low Earth orbit ranging from LEO commercialization efforts related to advancing protein crystal growth studies for drug discovery and delivery; stem cell, organs-on-chips, and vascularized tissue research for organ bioengineering; and use of 3D printing capabilities and superior optical fiber manufacturing for on-orbit production.
Anatomy of a Megathrust Earthquake Rupture - The 2010 M8.8 Chile QuakeStephen Hicks
Presented for an IRIS (Incorporated Research Institutions for Seismology) webinar on 9 April 2014.
Webinar can be viewed here: https://www.youtube.com/watch?v=MNcl5AZlX3k
Abstract: In February 2010, a magnitude 8.8 megathrust earthquake struck the Maule region of Central Chile - the sixth largest earthquake ever recorded. It is fast becoming one of the best-studied megathrust ruptures, allowing us a unique insight into the inner workings of subduction zone earthquakes. In the earthquake’s immediate aftermath, an international group of research institutions deployed geophysical instruments in the rupture area. A network of ~160 seismic stations on the forearc recorded over 50,000 aftershocks in the first 10 months following the earthquake.
I have used observations of P- and S-waves from aftershocks to derive a high-resolution seismic travel-time tomography of the rupture zone. Observations from ocean-bottom seismometers further improve image sharpness in the offshore portion of the seismogenic zone, where most slip occurred during the earthquake. The tomographic images reveal the distribution of P-wave velocity and Poisson’s Ratio within the earthquake rupture zone. Based on accurate aftershock locations and moment tensors, I have defined a new 3-D plate interface geometry to infer the physical structure and composition along the plate interface. I compare these velocities with the mainly geodetically observed behaviour of the fault throughout a cycle of seismic behaviour (preseismic locking, coseismic slip, postseismic deformation). This comparison allows us to understand some of the physical properties that may govern seismogenesis along the megathrust. I will reveal how both the long-lived geological structure of the forearc and the composition of the subducting oceanic plate may influence the rupture behaviour of large megathrust earthquakes. An understanding of seismic velocities along the megathrust may therefore be used to constrain the seismogenic potential of subduction zones worldwide.
How does biological protection help astronauts tolerate high levels of radiationSMJ Mortazavi
Abstract:
Exposure to high levels of space radiation and microgravity are two important concerns which need to be addressed before any long-term manned space mission. There are also reports showing that microgravity, through a synergistic effect, increases the radiation susceptibility of living organisms. Other researchers as well as our team have conducted some experiments on design and fabrication of appropriate radiation shields for spacecrafts. However, due to some cardinal barriers such as weight limitations and extreme inadequacy of current physical shields during extravehicular activity, we strongly believe that the physical shielding alone cannot solve the problem of potential exposure to high levels of radiation in a long-term space mission.
Therefore, over the past several years, we focused on two solutions; radioadaptive response and other biological-based radiation protection methods. Adaptive response, that is the increased radioresistance in cells or living organisms pre-exposed to a low adapting dose and then exposed to a high challenging dose, was firstly proposed by our team in 2003 as an effective method. This novel idea later formed the basis of many space radiation biology projects around the world.
Furthermore, conventional radioprotectors cannot efficiently be used in space due to limitations such as their considerable toxicity and the very narrow time window for their effective use (radioprotectors should be used before or at the time of exposure, while astronauts cannot estimate their doses before a solar particle event). Therefore, we focused on introducing natural radiation mitigators which could be efficiently used several hours after exposure (e.g. when a solar particle event subsides and astronauts are able to estimate their doses). In these experiments, radiation mitigators were introduced by our team which could be used even 24 hours after exposure to high levels of radiation caused by unpredictable sources such as SPEs.
Finally, some of our recent experiments were aimed at finding methods which could lead to boosting the immune system of astronauts during long-term missions. We investigated the effect of RF-EMFs-induced adaptive responses on immune system modulation in a mouse model of hindlimb unloading (HU). Hindlimb unloading rodent model is widely accepted by the scientific community as the model of choice for simulating spaceflight. In this study, serum levels of T helper cytokines were determined in HU mice, RF-EMF treated mice and HU mice pre-exposed to RF-EMF compared to those of untreated controls. The findings of this study will be published soon.
Final-How Some INIRPRC’s Studies Can Re-Route the Direction of Global Science...SMJ Mortazavi
In this presentation some of the game changer achievements of the Ionizing and Non-Ionizing Radiation Protection Research Center (INIRPRC) in the following fields are discussed: 1. Space Biology 2. COVID-19 Management 3. Ramsar high background radiation areas (HBRAs) Studies 4. Health Effects of Radiofrequency Radiation
Space habitats for bioengineering and surgical repair: addressing the require...Sérgio Sacani
Numerous technical scenarios have been developed to facilitate a human return to the Moon, and as a testbed for a subsequent
mission to Mars. Crews appointed with constructing and establishing planetary bases will require a superior level of physical ability
to cope with the operational demands. However, the challenging environments of nearby planets (e.g. geological, atmospheric,
gravitational conditions) as well as the lengthy journeys through microgravity, will lead to progressive tissue degradation and an
increased susceptibility to injury. The isolation, distance and inability to evacuate in an emergency will require autonomous medical
support, as well as a range of facilities and specialised equipment to repair tissue damage on-site. Here, we discuss the design
requirements of such a facility, in the form of a habitat that would concomitantly allow tissue substitute production, maintenance
and surgical implantation, with an emphasis on connective tissues. The requirements for the individual modules and their operation
are identified. Several concepts are assessed, including the presence of adjacent wet lab and medical modules supporting the
gradual implementation of regenerative biomaterials and acellular tissue substitutes, leading to eventual tissue grafts and, in
subsequent decades, potential tissues/organ-like structures. The latter, currently in early phases of development, are assessed
particularly for researching the effects of extreme conditions on representative analogues for astronaut health support. Technical
solutions are discussed for bioengineering in an isolated planetary environment with hypogravity, from fluid-gel bath suspended
manufacture to cryostorage, cell sourcing and on-site resource utilisation for laboratory infrastructure. Surgical considerations are
also discussed.
The Challenges of J-shaped Dose Response Models for Ionizing and Non-ionizing...SMJ Mortazavi
An accumulating body of evidence indicates that living organisms exposed to specific windows of doses/dose rates of both ionizing and non-ionizing radiation demonstrate J-shaped dose response curves. Evaluation of these dose-response curves is of great importance in radiation biology as well as radiation protection. Studies conducted by my colleagues and I show that the general patterns of induction of phenomena such as adaptive response are similar for ionizing and non-ionizing radiations. Given this consideration, we have previously reported that the so called “dose window theory” that is well discussed for adaptive responses induced by ionizing radiation, is valid for non-ionizing radiation. Recently, after reviewing the current literature, we provided data indicating that in a similar pattern with ionizing radiation, the carcinogenesis of non-ionizing radiofrequency electromagnetic fields (RF-EMF) may have a nonlinear dose-response relationship. In particular, we introduced data that support the validity of a J-shaped dose-response relationship. Considering the pattern of J-shaped dose response models, ignoring the key issue of the exposure level (low levels vs. high-level exposures) can be introduced as a main root of current controversial reports regarding the carcinogenesis of RF-EMF. In this light, some studies show an association between mobile phone use and brain tumors, especially in people who used their mobile phones for long durations (e.g. ≥10 years). In summary, better understanding of the J-shaped dose response models for both ionizing and non-ionizing radiations can shed some light on the dark corners of current controversies about the adverse health effects of low-level exposures.
In vitro simulation of spaceflight environment to elucidate combined effect o...Advanced-Concepts-Team
Long-term exposure to microgravity, ionizing radiation and increased levels of psychological stress can cause changes in the astronauts’ skin, resulting in skin rashes, itches and delayed wound healing during space missions. There is still a lack of understanding how the complex spaceflight environment induces these defects. This PhD project aims to investigate how exposure to a combination of spaceflight stressors can affect the structure and function of the skin, and how they can hamper wound healing. For this we have developed in vitro simulation models and are exposing primary human dermal fibroblasts to hydrocortisone, ionizing radiation and simulated microgravity. Results indicate a significant negative effect of hydrocortisone as well as simulated microgravity on wound healing capability of dermal fibroblasts. Furthermore, a project has been initiated with the support of the European Space Agency Academy “Spin Your Thesis!” Campaign, aiming to investigate the effects of an increased gravitational force on fibroblast function related to wound healing. Altogether the results of this PhD project will give more insights into the effects of combined spaceflight stressors on dermal skin cells, and improve risk assessment for human deep space exploration.
Tissue Engineering and Human Regenerative Therapies in Space: Benefits for Ea...CrimsonpublishersITERM
Living and working in space presents many challenges for maintenance of optimal human physiology and psychology. The physical effects of microgravity and increased radiation exposure together with the psychological effects of isolation on human beings pose problems which are under intense investigation by global space agencies, corporate and academic research institutions. An unsurmountable challenge, at least today, for deep space exploration and colonisation (DSEC) is the longevity of human lifespan and the potential for organ system dysfunction which may lead to premature death and mission termination in the absence of bio-reparative capabilities. The unique nature of microgravity encountered in space provides both a challenge and an opportunity for regenerative medicine that cannot be fully replicated on Earth. This minireview describes some recent advances in the use of stem cells, tissue engineering and the potential for 3D bioprinting in space as future concepts for consideration in the design of missions supporting longer term space exploration and colonisation.
REVIEW Open AccessRadiations and female fertilityRoberto.docxhealdkathaleen
REVIEW Open Access
Radiations and female fertility
Roberto Marci1,2,3* , Maddalena Mallozzi4, Luisa Di Benedetto4, Mauro Schimberni4, Stefano Mossa5, Ilaria Soave4,
Stefano Palomba6 and Donatella Caserta4
Abstract
Hundreds of thousands of young women are diagnosed with cancer each year, and due to recent advances in
screening programs, diagnostic methods and treatment options, survival rates have significantly improved.
Radiation therapy plays an important role in cancer treatment and in some cases it constitutes the first therapy
proposed to the patient. However, ionizing radiations have a gonadotoxic action with long-term effects that
include ovarian insufficiency, pubertal arrest and subsequent infertility. Cranial irradiation may lead to disruption of
the hypothalamic-pituitary-gonadal axis, with consequent dysregulation of the normal hormonal secretion. The
uterus might be damaged by radiotherapy, as well. In fact, exposure to radiation during childhood leads to altered
uterine vascularization, decreased uterine volume and elasticity, myometrial fibrosis and necrosis, endometrial atrophy
and insufficiency. As radiations have a relevant impact on reproductive potential, fertility preservation procedures
should be carried out before and/or during anticancer treatments. Fertility preservation strategies have been employed
for some years now and have recently been diversified thanks to advances in reproductive biology. Aim of this paper is
to give an overview of the various effects of radiotherapy on female reproductive function and to describe the current
fertility preservation options.
Keywords: Radiotherapy, Radiation, Infertility, Fertility preservation
Introduction
In modern society people are frequently exposed to differ-
ent types of radiations and this exposure comes form
different sources. It could be either related to everyday life
(e.g. televisions, mobile phones, computer devices, occupa-
tional equipment) or to the necessity of medical care (e.g.
diagnostic imaging, interventional radiology procedures,
anticancer therapy). Usually radiations are divided into two
big subgroups, ionizing and non-ionizing, depending on
the energy of the radiated particles.
Non-ionizing radiations
These type of radiations are basically electromagnetic fields
(EMFs) that do not have enough energy to release elec-
trons (non–ionizing), but are able to excite the movement
of an electron to a higher energy state. Several classification
of EMFs have been proposed, but generally 4 big
subgroups are recognized [1, 2]:
(i) extremely low frequency EMFs that have
frequencies below 300 Hz (military equipment,
railroads)
(ii) intermediate frequency EMFs characterized by
frequencies ranging from 300 Hz to 10 MHz
(televisions, computer monitors, industrial cables)
(iii)hyper frequency EMFs characterized by frequencies
ranging from 10 MHz to 3000 GHz (mobile
phones, radio)
(iv)static EMFs that have zero frequency (MRI,
geomagnetism)
The biological react ...
PHARMACOKINETIC CHANGES AND PHARMACOTHERAPEUTIC APPROACHES IN SPACE ASTRONAUTPARUL UNIVERSITY
Space Pharmacology is the study of use of pharmaceutical drugs during spaceflights Space flight can alter administered drug act on the body. Space medicine is fundamental to the human exploration of space. It supports survival, function and performance in this challenging and potentially lethal environment. It is international, intercultural and interdisciplinary, operating at the boundaries of exploration, science, technology and medicine. This review introduces the field of space pharmacology and describes the different types of environmental challenges, associated medical and physiological effects, and medical considerations. It will describe the varied roles of the space pharmacist. Astronauts are not the only ones who benefit from space medicine research. Space pharmacology research will benefit health care on Earth. Several medical products have been developed that are space spinoffs, that is practical applications for the field of medicine arising out of the space program. It is difficult to conclude the optimal drug regimens in microgravity to ensure safe, effective, and definitive treatment of space travellers. This study is mainly focused on the health issues in space, space medicine for astronauts, pharmacokinetic, pharmacodynamics and pharmacotherapeutics in space and medicine spinoffs.
Mercury Released from Dental Amalgam Fillings in Response to Different Physic...SMJ Mortazavi
Approximately 50% of dental amalgam is elemental mercury by weight. Accumulating body of evidence now shows that not only static magnetic fields (SMF) but both ionizing and non-ionizing electromagnetic radiations can increase the rate of mercury release from dental amalgam fillings. Iranian scientists firstly addressed this issue in 2008 but more than 10 years later, it became viral worldwide after BBC released a report on this issue.
Low-Dose Radiation Therapy for COVID-19 -Time reveals the truth.pptxSMJ Mortazavi
More than two years ago, we warned about the dangers of treatment methods that are based on the use of antivirals, but it took a long time for the issue of selective pressure caused by antivirals to be widely discussed in scientific societies. Now the Science report published on June 29, 2022 clearly points to this issue
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How does biological protection help astronauts tolerate high levels of radiationSMJ Mortazavi
Abstract:
Exposure to high levels of space radiation and microgravity are two important concerns which need to be addressed before any long-term manned space mission. There are also reports showing that microgravity, through a synergistic effect, increases the radiation susceptibility of living organisms. Other researchers as well as our team have conducted some experiments on design and fabrication of appropriate radiation shields for spacecrafts. However, due to some cardinal barriers such as weight limitations and extreme inadequacy of current physical shields during extravehicular activity, we strongly believe that the physical shielding alone cannot solve the problem of potential exposure to high levels of radiation in a long-term space mission.
Therefore, over the past several years, we focused on two solutions; radioadaptive response and other biological-based radiation protection methods. Adaptive response, that is the increased radioresistance in cells or living organisms pre-exposed to a low adapting dose and then exposed to a high challenging dose, was firstly proposed by our team in 2003 as an effective method. This novel idea later formed the basis of many space radiation biology projects around the world.
Furthermore, conventional radioprotectors cannot efficiently be used in space due to limitations such as their considerable toxicity and the very narrow time window for their effective use (radioprotectors should be used before or at the time of exposure, while astronauts cannot estimate their doses before a solar particle event). Therefore, we focused on introducing natural radiation mitigators which could be efficiently used several hours after exposure (e.g. when a solar particle event subsides and astronauts are able to estimate their doses). In these experiments, radiation mitigators were introduced by our team which could be used even 24 hours after exposure to high levels of radiation caused by unpredictable sources such as SPEs.
Finally, some of our recent experiments were aimed at finding methods which could lead to boosting the immune system of astronauts during long-term missions. We investigated the effect of RF-EMFs-induced adaptive responses on immune system modulation in a mouse model of hindlimb unloading (HU). Hindlimb unloading rodent model is widely accepted by the scientific community as the model of choice for simulating spaceflight. In this study, serum levels of T helper cytokines were determined in HU mice, RF-EMF treated mice and HU mice pre-exposed to RF-EMF compared to those of untreated controls. The findings of this study will be published soon.
Final-How Some INIRPRC’s Studies Can Re-Route the Direction of Global Science...SMJ Mortazavi
In this presentation some of the game changer achievements of the Ionizing and Non-Ionizing Radiation Protection Research Center (INIRPRC) in the following fields are discussed: 1. Space Biology 2. COVID-19 Management 3. Ramsar high background radiation areas (HBRAs) Studies 4. Health Effects of Radiofrequency Radiation
Space habitats for bioengineering and surgical repair: addressing the require...Sérgio Sacani
Numerous technical scenarios have been developed to facilitate a human return to the Moon, and as a testbed for a subsequent
mission to Mars. Crews appointed with constructing and establishing planetary bases will require a superior level of physical ability
to cope with the operational demands. However, the challenging environments of nearby planets (e.g. geological, atmospheric,
gravitational conditions) as well as the lengthy journeys through microgravity, will lead to progressive tissue degradation and an
increased susceptibility to injury. The isolation, distance and inability to evacuate in an emergency will require autonomous medical
support, as well as a range of facilities and specialised equipment to repair tissue damage on-site. Here, we discuss the design
requirements of such a facility, in the form of a habitat that would concomitantly allow tissue substitute production, maintenance
and surgical implantation, with an emphasis on connective tissues. The requirements for the individual modules and their operation
are identified. Several concepts are assessed, including the presence of adjacent wet lab and medical modules supporting the
gradual implementation of regenerative biomaterials and acellular tissue substitutes, leading to eventual tissue grafts and, in
subsequent decades, potential tissues/organ-like structures. The latter, currently in early phases of development, are assessed
particularly for researching the effects of extreme conditions on representative analogues for astronaut health support. Technical
solutions are discussed for bioengineering in an isolated planetary environment with hypogravity, from fluid-gel bath suspended
manufacture to cryostorage, cell sourcing and on-site resource utilisation for laboratory infrastructure. Surgical considerations are
also discussed.
The Challenges of J-shaped Dose Response Models for Ionizing and Non-ionizing...SMJ Mortazavi
An accumulating body of evidence indicates that living organisms exposed to specific windows of doses/dose rates of both ionizing and non-ionizing radiation demonstrate J-shaped dose response curves. Evaluation of these dose-response curves is of great importance in radiation biology as well as radiation protection. Studies conducted by my colleagues and I show that the general patterns of induction of phenomena such as adaptive response are similar for ionizing and non-ionizing radiations. Given this consideration, we have previously reported that the so called “dose window theory” that is well discussed for adaptive responses induced by ionizing radiation, is valid for non-ionizing radiation. Recently, after reviewing the current literature, we provided data indicating that in a similar pattern with ionizing radiation, the carcinogenesis of non-ionizing radiofrequency electromagnetic fields (RF-EMF) may have a nonlinear dose-response relationship. In particular, we introduced data that support the validity of a J-shaped dose-response relationship. Considering the pattern of J-shaped dose response models, ignoring the key issue of the exposure level (low levels vs. high-level exposures) can be introduced as a main root of current controversial reports regarding the carcinogenesis of RF-EMF. In this light, some studies show an association between mobile phone use and brain tumors, especially in people who used their mobile phones for long durations (e.g. ≥10 years). In summary, better understanding of the J-shaped dose response models for both ionizing and non-ionizing radiations can shed some light on the dark corners of current controversies about the adverse health effects of low-level exposures.
In vitro simulation of spaceflight environment to elucidate combined effect o...Advanced-Concepts-Team
Long-term exposure to microgravity, ionizing radiation and increased levels of psychological stress can cause changes in the astronauts’ skin, resulting in skin rashes, itches and delayed wound healing during space missions. There is still a lack of understanding how the complex spaceflight environment induces these defects. This PhD project aims to investigate how exposure to a combination of spaceflight stressors can affect the structure and function of the skin, and how they can hamper wound healing. For this we have developed in vitro simulation models and are exposing primary human dermal fibroblasts to hydrocortisone, ionizing radiation and simulated microgravity. Results indicate a significant negative effect of hydrocortisone as well as simulated microgravity on wound healing capability of dermal fibroblasts. Furthermore, a project has been initiated with the support of the European Space Agency Academy “Spin Your Thesis!” Campaign, aiming to investigate the effects of an increased gravitational force on fibroblast function related to wound healing. Altogether the results of this PhD project will give more insights into the effects of combined spaceflight stressors on dermal skin cells, and improve risk assessment for human deep space exploration.
Tissue Engineering and Human Regenerative Therapies in Space: Benefits for Ea...CrimsonpublishersITERM
Living and working in space presents many challenges for maintenance of optimal human physiology and psychology. The physical effects of microgravity and increased radiation exposure together with the psychological effects of isolation on human beings pose problems which are under intense investigation by global space agencies, corporate and academic research institutions. An unsurmountable challenge, at least today, for deep space exploration and colonisation (DSEC) is the longevity of human lifespan and the potential for organ system dysfunction which may lead to premature death and mission termination in the absence of bio-reparative capabilities. The unique nature of microgravity encountered in space provides both a challenge and an opportunity for regenerative medicine that cannot be fully replicated on Earth. This minireview describes some recent advances in the use of stem cells, tissue engineering and the potential for 3D bioprinting in space as future concepts for consideration in the design of missions supporting longer term space exploration and colonisation.
REVIEW Open AccessRadiations and female fertilityRoberto.docxhealdkathaleen
REVIEW Open Access
Radiations and female fertility
Roberto Marci1,2,3* , Maddalena Mallozzi4, Luisa Di Benedetto4, Mauro Schimberni4, Stefano Mossa5, Ilaria Soave4,
Stefano Palomba6 and Donatella Caserta4
Abstract
Hundreds of thousands of young women are diagnosed with cancer each year, and due to recent advances in
screening programs, diagnostic methods and treatment options, survival rates have significantly improved.
Radiation therapy plays an important role in cancer treatment and in some cases it constitutes the first therapy
proposed to the patient. However, ionizing radiations have a gonadotoxic action with long-term effects that
include ovarian insufficiency, pubertal arrest and subsequent infertility. Cranial irradiation may lead to disruption of
the hypothalamic-pituitary-gonadal axis, with consequent dysregulation of the normal hormonal secretion. The
uterus might be damaged by radiotherapy, as well. In fact, exposure to radiation during childhood leads to altered
uterine vascularization, decreased uterine volume and elasticity, myometrial fibrosis and necrosis, endometrial atrophy
and insufficiency. As radiations have a relevant impact on reproductive potential, fertility preservation procedures
should be carried out before and/or during anticancer treatments. Fertility preservation strategies have been employed
for some years now and have recently been diversified thanks to advances in reproductive biology. Aim of this paper is
to give an overview of the various effects of radiotherapy on female reproductive function and to describe the current
fertility preservation options.
Keywords: Radiotherapy, Radiation, Infertility, Fertility preservation
Introduction
In modern society people are frequently exposed to differ-
ent types of radiations and this exposure comes form
different sources. It could be either related to everyday life
(e.g. televisions, mobile phones, computer devices, occupa-
tional equipment) or to the necessity of medical care (e.g.
diagnostic imaging, interventional radiology procedures,
anticancer therapy). Usually radiations are divided into two
big subgroups, ionizing and non-ionizing, depending on
the energy of the radiated particles.
Non-ionizing radiations
These type of radiations are basically electromagnetic fields
(EMFs) that do not have enough energy to release elec-
trons (non–ionizing), but are able to excite the movement
of an electron to a higher energy state. Several classification
of EMFs have been proposed, but generally 4 big
subgroups are recognized [1, 2]:
(i) extremely low frequency EMFs that have
frequencies below 300 Hz (military equipment,
railroads)
(ii) intermediate frequency EMFs characterized by
frequencies ranging from 300 Hz to 10 MHz
(televisions, computer monitors, industrial cables)
(iii)hyper frequency EMFs characterized by frequencies
ranging from 10 MHz to 3000 GHz (mobile
phones, radio)
(iv)static EMFs that have zero frequency (MRI,
geomagnetism)
The biological react ...
PHARMACOKINETIC CHANGES AND PHARMACOTHERAPEUTIC APPROACHES IN SPACE ASTRONAUTPARUL UNIVERSITY
Space Pharmacology is the study of use of pharmaceutical drugs during spaceflights Space flight can alter administered drug act on the body. Space medicine is fundamental to the human exploration of space. It supports survival, function and performance in this challenging and potentially lethal environment. It is international, intercultural and interdisciplinary, operating at the boundaries of exploration, science, technology and medicine. This review introduces the field of space pharmacology and describes the different types of environmental challenges, associated medical and physiological effects, and medical considerations. It will describe the varied roles of the space pharmacist. Astronauts are not the only ones who benefit from space medicine research. Space pharmacology research will benefit health care on Earth. Several medical products have been developed that are space spinoffs, that is practical applications for the field of medicine arising out of the space program. It is difficult to conclude the optimal drug regimens in microgravity to ensure safe, effective, and definitive treatment of space travellers. This study is mainly focused on the health issues in space, space medicine for astronauts, pharmacokinetic, pharmacodynamics and pharmacotherapeutics in space and medicine spinoffs.
Mercury Released from Dental Amalgam Fillings in Response to Different Physic...SMJ Mortazavi
Approximately 50% of dental amalgam is elemental mercury by weight. Accumulating body of evidence now shows that not only static magnetic fields (SMF) but both ionizing and non-ionizing electromagnetic radiations can increase the rate of mercury release from dental amalgam fillings. Iranian scientists firstly addressed this issue in 2008 but more than 10 years later, it became viral worldwide after BBC released a report on this issue.
Low-Dose Radiation Therapy for COVID-19 -Time reveals the truth.pptxSMJ Mortazavi
More than two years ago, we warned about the dangers of treatment methods that are based on the use of antivirals, but it took a long time for the issue of selective pressure caused by antivirals to be widely discussed in scientific societies. Now the Science report published on June 29, 2022 clearly points to this issue
More than two years ago, we warned about the dangers of treatment methods that are based on the use of antivirals, but it took a long time for the issue of selective pressure caused by antivirals to be widely discussed in scientific societies. Now the Science report published on June 29, 2022 clearly points to this issue.
How Crucial is the Importance of COVID-19 in Long-Term Space Missions?SMJ Mortazavi
How Crucial is the Importance of COVID-19 in Long-Term Space Missions?
The higher fatality of COVID-19 infections in space is due to:
1) impossibility to use the so-called “social distancing” due to microgravity
2) immune system dysregulation
3) possibly higher mutation rates of the SARS-CoV-2 as an RNA virus
4) higher risk of reactivation of the virus
5) existence of strong selective pressure and
6) decreased maximum oxygen uptake.
How did we trigger scientists around the globe to uncover the low dose radiat...SMJ Mortazavi
Any attempt to inactivate a virus exerts strong selective pressure on the virus. Given this consideration, antiviral drugs can exert strong selective pressure on SARS-COV-2. In March 2020, we proposed the concept of Low Dose Radiation Therapy (LDRT) for COVID-19 associated pneumonia. This treatment was a 100% "selective pressure-free" therapeutic approach. After our paper, tens of papers published on this issue, and now LDRT for COVID-19 is receiving rapidly increasing global attention.
Low-dose radiation therapy (LDRT) for COVID-19 associated pneumoniaSMJ Mortazavi
The efficiency of low dose radiation therapy as a potential treatment of pneumonia in COVID-19 patients has been addressed by many scientists from different parts of the world. For further reading please see the first report of Ghadimi-Moghadam et al. (COVID-19 Tragic Pandemic: Concerns over Unintentional “Directed Accelerated Evolution” of Novel Coronavirus (SARS-CoV-2) and Introducing a Modified Treatment Method for ARDS https://lnkd.in/dzXtqkc) and later reports by Canadian (Is low dose radiation therapy a potential treatment for COVID-19 pneumonia? https://lnkd.in/d7TQKcS), Spanish (Low Dose Lung Radiotherapy for COVID-19 Pneumonia. The Rationale for a Cost-Effective Anti-Inflammatory Treatment https://lnkd.in/dStMJKr), American (Low dose radiation therapy as a potential life saving treatment for COVID-19-induced acute respiratory distress syndrome (ARDS) https://lnkd.in/dnR8kyJ), German (Low-dose radiation therapy for COVID-19 pneumopathy: what is the evidence? https://lnkd.in/dWGCQBb) and French (Irradiation pulmonaire à faible dose pour l’orage de cytokines du COVID-19 : pourquoi pas ? https://lnkd.in/dsW65ew) scientists.
Basavarajeeyam is an important text for ayurvedic physician belonging to andhra pradehs. It is a popular compendium in various parts of our country as well as in andhra pradesh. The content of the text was presented in sanskrit and telugu language (Bilingual). One of the most famous book in ayurvedic pharmaceutics and therapeutics. This book contains 25 chapters called as prakaranas. Many rasaoushadis were explained, pioneer of dhatu druti, nadi pareeksha, mutra pareeksha etc. Belongs to the period of 15-16 century. New diseases like upadamsha, phiranga rogas are explained.
Adv. biopharm. APPLICATION OF PHARMACOKINETICS : TARGETED DRUG DELIVERY SYSTEMSAkankshaAshtankar
MIP 201T & MPH 202T
ADVANCED BIOPHARMACEUTICS & PHARMACOKINETICS : UNIT 5
APPLICATION OF PHARMACOKINETICS : TARGETED DRUG DELIVERY SYSTEMS By - AKANKSHA ASHTANKAR
Title: Sense of Smell
Presenter: Dr. Faiza, Assistant Professor of Physiology
Qualifications:
MBBS (Best Graduate, AIMC Lahore)
FCPS Physiology
ICMT, CHPE, DHPE (STMU)
MPH (GC University, Faisalabad)
MBA (Virtual University of Pakistan)
Learning Objectives:
Describe the primary categories of smells and the concept of odor blindness.
Explain the structure and location of the olfactory membrane and mucosa, including the types and roles of cells involved in olfaction.
Describe the pathway and mechanisms of olfactory signal transmission from the olfactory receptors to the brain.
Illustrate the biochemical cascade triggered by odorant binding to olfactory receptors, including the role of G-proteins and second messengers in generating an action potential.
Identify different types of olfactory disorders such as anosmia, hyposmia, hyperosmia, and dysosmia, including their potential causes.
Key Topics:
Olfactory Genes:
3% of the human genome accounts for olfactory genes.
400 genes for odorant receptors.
Olfactory Membrane:
Located in the superior part of the nasal cavity.
Medially: Folds downward along the superior septum.
Laterally: Folds over the superior turbinate and upper surface of the middle turbinate.
Total surface area: 5-10 square centimeters.
Olfactory Mucosa:
Olfactory Cells: Bipolar nerve cells derived from the CNS (100 million), with 4-25 olfactory cilia per cell.
Sustentacular Cells: Produce mucus and maintain ionic and molecular environment.
Basal Cells: Replace worn-out olfactory cells with an average lifespan of 1-2 months.
Bowman’s Gland: Secretes mucus.
Stimulation of Olfactory Cells:
Odorant dissolves in mucus and attaches to receptors on olfactory cilia.
Involves a cascade effect through G-proteins and second messengers, leading to depolarization and action potential generation in the olfactory nerve.
Quality of a Good Odorant:
Small (3-20 Carbon atoms), volatile, water-soluble, and lipid-soluble.
Facilitated by odorant-binding proteins in mucus.
Membrane Potential and Action Potential:
Resting membrane potential: -55mV.
Action potential frequency in the olfactory nerve increases with odorant strength.
Adaptation Towards the Sense of Smell:
Rapid adaptation within the first second, with further slow adaptation.
Psychological adaptation greater than receptor adaptation, involving feedback inhibition from the central nervous system.
Primary Sensations of Smell:
Camphoraceous, Musky, Floral, Pepperminty, Ethereal, Pungent, Putrid.
Odor Detection Threshold:
Examples: Hydrogen sulfide (0.0005 ppm), Methyl-mercaptan (0.002 ppm).
Some toxic substances are odorless at lethal concentrations.
Characteristics of Smell:
Odor blindness for single substances due to lack of appropriate receptor protein.
Behavioral and emotional influences of smell.
Transmission of Olfactory Signals:
From olfactory cells to glomeruli in the olfactory bulb, involving lateral inhibition.
Primitive, less old, and new olfactory systems with different path
Tom Selleck Health: A Comprehensive Look at the Iconic Actor’s Wellness Journeygreendigital
Tom Selleck, an enduring figure in Hollywood. has captivated audiences for decades with his rugged charm, iconic moustache. and memorable roles in television and film. From his breakout role as Thomas Magnum in Magnum P.I. to his current portrayal of Frank Reagan in Blue Bloods. Selleck's career has spanned over 50 years. But beyond his professional achievements. fans have often been curious about Tom Selleck Health. especially as he has aged in the public eye.
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Introduction
Many have been interested in Tom Selleck health. not only because of his enduring presence on screen but also because of the challenges. and lifestyle choices he has faced and made over the years. This article delves into the various aspects of Tom Selleck health. exploring his fitness regimen, diet, mental health. and the challenges he has encountered as he ages. We'll look at how he maintains his well-being. the health issues he has faced, and his approach to ageing .
Early Life and Career
Childhood and Athletic Beginnings
Tom Selleck was born on January 29, 1945, in Detroit, Michigan, and grew up in Sherman Oaks, California. From an early age, he was involved in sports, particularly basketball. which played a significant role in his physical development. His athletic pursuits continued into college. where he attended the University of Southern California (USC) on a basketball scholarship. This early involvement in sports laid a strong foundation for his physical health and disciplined lifestyle.
Transition to Acting
Selleck's transition from an athlete to an actor came with its physical demands. His first significant role in "Magnum P.I." required him to perform various stunts and maintain a fit appearance. This role, which he played from 1980 to 1988. necessitated a rigorous fitness routine to meet the show's demands. setting the stage for his long-term commitment to health and wellness.
Fitness Regimen
Workout Routine
Tom Selleck health and fitness regimen has evolved. adapting to his changing roles and age. During his "Magnum, P.I." days. Selleck's workouts were intense and focused on building and maintaining muscle mass. His routine included weightlifting, cardiovascular exercises. and specific training for the stunts he performed on the show.
Selleck adjusted his fitness routine as he aged to suit his body's needs. Today, his workouts focus on maintaining flexibility, strength, and cardiovascular health. He incorporates low-impact exercises such as swimming, walking, and light weightlifting. This balanced approach helps him stay fit without putting undue strain on his joints and muscles.
Importance of Flexibility and Mobility
In recent years, Selleck has emphasized the importance of flexibility and mobility in his fitness regimen. Understanding the natural decline in muscle mass and joint flexibility with age. he includes stretching and yoga in his routine. These practices help prevent injuries, improve posture, and maintain mobilit
micro teaching on communication m.sc nursing.pdfAnurag Sharma
Microteaching is a unique model of practice teaching. It is a viable instrument for the. desired change in the teaching behavior or the behavior potential which, in specified types of real. classroom situations, tends to facilitate the achievement of specified types of objectives.
Local Advanced Lung Cancer: Artificial Intelligence, Synergetics, Complex Sys...Oleg Kshivets
Overall life span (LS) was 1671.7±1721.6 days and cumulative 5YS reached 62.4%, 10 years – 50.4%, 20 years – 44.6%. 94 LCP lived more than 5 years without cancer (LS=2958.6±1723.6 days), 22 – more than 10 years (LS=5571±1841.8 days). 67 LCP died because of LC (LS=471.9±344 days). AT significantly improved 5YS (68% vs. 53.7%) (P=0.028 by log-rank test). Cox modeling displayed that 5YS of LCP significantly depended on: N0-N12, T3-4, blood cell circuit, cell ratio factors (ratio between cancer cells-CC and blood cells subpopulations), LC cell dynamics, recalcification time, heparin tolerance, prothrombin index, protein, AT, procedure type (P=0.000-0.031). Neural networks, genetic algorithm selection and bootstrap simulation revealed relationships between 5YS and N0-12 (rank=1), thrombocytes/CC (rank=2), segmented neutrophils/CC (3), eosinophils/CC (4), erythrocytes/CC (5), healthy cells/CC (6), lymphocytes/CC (7), stick neutrophils/CC (8), leucocytes/CC (9), monocytes/CC (10). Correct prediction of 5YS was 100% by neural networks computing (error=0.000; area under ROC curve=1.0).
Title: Sense of Taste
Presenter: Dr. Faiza, Assistant Professor of Physiology
Qualifications:
MBBS (Best Graduate, AIMC Lahore)
FCPS Physiology
ICMT, CHPE, DHPE (STMU)
MPH (GC University, Faisalabad)
MBA (Virtual University of Pakistan)
Learning Objectives:
Describe the structure and function of taste buds.
Describe the relationship between the taste threshold and taste index of common substances.
Explain the chemical basis and signal transduction of taste perception for each type of primary taste sensation.
Recognize different abnormalities of taste perception and their causes.
Key Topics:
Significance of Taste Sensation:
Differentiation between pleasant and harmful food
Influence on behavior
Selection of food based on metabolic needs
Receptors of Taste:
Taste buds on the tongue
Influence of sense of smell, texture of food, and pain stimulation (e.g., by pepper)
Primary and Secondary Taste Sensations:
Primary taste sensations: Sweet, Sour, Salty, Bitter, Umami
Chemical basis and signal transduction mechanisms for each taste
Taste Threshold and Index:
Taste threshold values for Sweet (sucrose), Salty (NaCl), Sour (HCl), and Bitter (Quinine)
Taste index relationship: Inversely proportional to taste threshold
Taste Blindness:
Inability to taste certain substances, particularly thiourea compounds
Example: Phenylthiocarbamide
Structure and Function of Taste Buds:
Composition: Epithelial cells, Sustentacular/Supporting cells, Taste cells, Basal cells
Features: Taste pores, Taste hairs/microvilli, and Taste nerve fibers
Location of Taste Buds:
Found in papillae of the tongue (Fungiform, Circumvallate, Foliate)
Also present on the palate, tonsillar pillars, epiglottis, and proximal esophagus
Mechanism of Taste Stimulation:
Interaction of taste substances with receptors on microvilli
Signal transduction pathways for Umami, Sweet, Bitter, Sour, and Salty tastes
Taste Sensitivity and Adaptation:
Decrease in sensitivity with age
Rapid adaptation of taste sensation
Role of Saliva in Taste:
Dissolution of tastants to reach receptors
Washing away the stimulus
Taste Preferences and Aversions:
Mechanisms behind taste preference and aversion
Influence of receptors and neural pathways
Impact of Sensory Nerve Damage:
Degeneration of taste buds if the sensory nerve fiber is cut
Abnormalities of Taste Detection:
Conditions: Ageusia, Hypogeusia, Dysgeusia (parageusia)
Causes: Nerve damage, neurological disorders, infections, poor oral hygiene, adverse drug effects, deficiencies, aging, tobacco use, altered neurotransmitter levels
Neurotransmitters and Taste Threshold:
Effects of serotonin (5-HT) and norepinephrine (NE) on taste sensitivity
Supertasters:
25% of the population with heightened sensitivity to taste, especially bitterness
Increased number of fungiform papillae
- Video recording of this lecture in English language: https://youtu.be/kqbnxVAZs-0
- Video recording of this lecture in Arabic language: https://youtu.be/SINlygW1Mpc
- Link to download the book free: https://nephrotube.blogspot.com/p/nephrotube-nephrology-books.html
- Link to NephroTube website: www.NephroTube.com
- Link to NephroTube social media accounts: https://nephrotube.blogspot.com/p/join-nephrotube-on-social-media.html
Muktapishti is a traditional Ayurvedic preparation made from Shoditha Mukta (Purified Pearl), is believed to help regulate thyroid function and reduce symptoms of hyperthyroidism due to its cooling and balancing properties. Clinical evidence on its efficacy remains limited, necessitating further research to validate its therapeutic benefits.
2. Adaptive Response in NASA Report
• A NASA report entitled “Evidence
Report: Risk of Radiation
Carcinogenesis”(Huff et al., 2016)
that is approved for public release
on April 7, 2016 has cited our 2003
report as well as other reports on
the importance of adaptive
response studies in deep space
missions.
Mortazavi SMJ, Ph.D
2
4. • “There have been several studies performed
that indicate an adaptive response to low-dose
ionizing radiation can provide a level of
protection against future exposures
(Bhattacharjee and Ito 2001; Mortazavi et al.
2003; Elmore et al. 2008; Rithidech et al.
2012). This may be particularly important for
understanding risks in the space environment
because the GCR environment is comprised
predominantly of protons, and it is realistic to
expect that cells will be exposed to multiple hits
of protons prior to being traversed by an HZE
particle”.
Mortazavi SMJ, Ph.D
4
Adaptive Response in NASA Report
5. Mortazavi SMJ, Ph.D
5
A recently published
paper (Oncotarget
Journal), authored by
30 scientists from US,
UK, Russia, Belgium,…
confirms the need for
selection of astronauts
based on their adaptive
response (as we
proposed it in 2003)
6. Mortazavi SMJ, Ph.D
6
"There is a strong evidence of a wide range of adaptive
response among different individuals, suggesting that
medical selection of the candidates based on the in
vitro adaptive response studies is very promising
[108, 186, 188, 189]"
"Countries actively engaged in development of the spaceflight
missions, such as United States and Russia, have well-
established protocols for selection of the potential candidates.
While these selection pipelines differ substantially from one to
another 184, 185], in vitro adaptive response studies is the only
approach widely implemented for the medical selection of the
radioresistant individuals [186, 187]. "
8. Mortazavi SMJ, Ph.D
8
Prof SMJ Mortazavi Prof A Niroomand-Rad Prof J R Cameron
So, what’s the model proposed by
our team?
Our early projects date back to 2003!
Univ W MadisonShiraz Univ Med Sci,
Shiraz, Iran
Georgetown Univ,
Univ W Madison
9. Mortazavi SMJ, Ph.D
9
Radiation Protection Challenges
in Space
Three General Guidelines:
•Time (Generally Not Applicable in Space,
Needs New Technologies for Propulsion
System)
•Distance (Not Applicable in Space,
Inverse Square Law Doesn’t help!)
•Shield (Not Easily Applicable in Space due
to Weight Limitations)
10. Mars Mission as a New Challenge
• “Typical missions to the
International Space Station
last six months.
• A round-trip mission to
Mars could last three years.
Key question:
• Do the effects of being in
space change over time?”
Mortazavi SMJ, Ph.D
10
NASA is taking the first steps on its
Journey to Mars. Artist’s concept,
looking toward Mars.
Credits: NASA
Source:
https://www.nasa.gov/feature/bridging-the-gap-nasa-studies-the-
human-body-in-space-for-one-year-to-extrapolate-for
13. Mortazavi SMJ, Ph.D
13
Other researchers as well as our
team have conducted some
experiments on design and
fabrication of appropriate
radiation shields for spacecrafts.
In spite of some advances in this
field, it will be discussed here
that improving the physical
shielding alone cannot solve the
problem of exposure to high
levels of radiation in a long term
space mission.
Our previous and current experiences:
15. Mortazavi SMJ, Ph.D
15
“For space applications, however,
every kilogram of mass has a
significant impact upon the
mission cost and feasibility.”
http://large.stanford.edu/courses/20
15/ph241/clark1/
16. Mortazavi SMJ, Ph.D
16
“ In fact, shielding is very
difficult in space: the very high
energy of the cosmic rays and the
severe mass constraints in
spaceflight represent a serious
hindrance to effective shielding.”
Marco Durante and Francis A. Cucinotta
Physical basis of radiation protection in space travel
Rev. Mod. Phys. 83, 1245 – Published 8 November 2011
REVIEWS OF
MODERN
PHYSICS
17. Mortazavi SMJ, Ph.D
17
“For space applications, however,
every kilogram of mass has a
significant impact upon the
mission cost and feasibility.”
http://large.stanford.edu/courses/20
15/ph241/clark1/
19. Mortazavi SMJ, Ph.D
19
“Examining the different methods
of space radiation shielding, it is
clear that no single good solution
currently exists to adequately
protect astronauts from the
radiation environment of space.”
http://large.stanford.edu/courses/20
15/ph241/clark1/
20. Mortazavi SMJ, Ph.D
20
Therefore, as physical
shielding alone cannot
solve current space
radiation problems, we
focused on:
• Adaptive Response
• Other Biological
Protection Methods
21. NASA’s Twin Study: Genomic Era of Space Travel
• Let’s take a look at NASA’s Twin Study
• “NASA was interested to see what happened to astronaut
Scott Kelly, in space, compared to his identical twin brother,
Mark, who remained on Earth.
• This study propelled NASA into the genomics era of space
travel.
• The Twins Study brought ten research teams from around
the country together to accomplish one goal:
discover what happens to the human body after spending one year in
space. “
Mortazavi SMJ, Ph.D
21
22. Mortazavi SMJ, Ph.D
22
Incorrect News
Spread By Media
In contrast with lots
of incorrect news, Scott
Kelly's DNA was not
changed after spending
a year in space
Image Credit: NASA
23. Mortazavi SMJ, Ph.D
23
“NASA has a grasp on what
happens to the body after the
standard-duration six-month
missions aboard the
International Space Station, but
Scott Kelly’s one-year mission
is a stepping stone to a three-
year mission to Mars.”
Source:
https://www.nasa.gov/feature/nasa-twins-study-confirms-preliminary-
findings
NASA/Robert Markowitz
24. Mortazavi SMJ, Ph.D
24
NASA reports that "Scott’s
telomeres …actually became
significantly longer in space.
Additionally, a new finding is
that the majority of those
telomeres shortened within two
days of Scott’s return to Earth".
Source: NASA
https://www.nasa.gov/feature/nasa-twins-
study-confirms-preliminary-findings
25. Mortazavi SMJ, Ph.D
25
• It can be postulated that Scott only
needed this protective mechanism
when he was in space, maybe a
natural response to high levels of
space radiation.
• This experiment can support the
theory that at least for long-term
space missions (e.g. Mars missions),
physical shielding alone cannot be
adequate for controlling radiation-
induced stresses.
https://www.ncbi.nlm.nih.gov/pubmed/29358
922
Image Credit: NASA/SOHO
26. Mortazavi SMJ, Ph.D
26
In this light, in a Mars
mission, we need screening
for measuring the
magnitude of
radioadaptation and
selection of the best
candidates.
As discussed in our recent papers
(https://www.ncbi.nlm.nih.gov/pubmed/12971409), adaptive
response not only increases the resistance against high levels
of space radiation but also it can limit factors such as
inflammation which affect gene expression.
27. Mortazavi SMJ, Ph.D
27
Mars vs. ISS Missions
A deep space mission such as a
journey to Mars would be
completely different from ISS
missions!
• No shielding effects of
magnetosphere
• Much longer mission duration
• Urgent EVAs are more likely, so
higher radiation doses are
expected!
• More biological effects?
29. Mortazavi SMJ, Ph.D
29
Adaptive response, that is
an increased
radioresistance in cells or
organisms exposed to a
high challenging dose after
pre-exposure to a low
adapting dose, can
considerably reduce the
radiation susceptibility of
humans (Olivieri et al.,
1984).
Mortazavi et al. 2003
Adaptive response
30. Mortazavi SMJ, Ph.D
30
• In any irradiated biological
systems, immediate
molecular damage may
increase linearly with the
absorbed dose.
• However, the response to
radiation damage of the
whole biological system is
not linear.
Feinendegen LE
Quantification of Adaptive Protection Following Low-dose
Irradiation.
Health Phys. 2016 Mar;110(3):276-80.
doi: 10.1097/HP.0000000000000431.
31. Mortazavi SMJ, Ph.D
31
What does it mean?
Our bodies are not passive
observers of the damages
physical and chemical
stressors induce!
Repair mechanisms!
Adaptation?
Feinendegen LE
Quantification of Adaptive Protection Following Low-dose
Irradiation.
Health Phys. 2016 Mar;110(3):276-80.
doi: 10.1097/HP.0000000000000431.
32. Mortazavi SMJ, Ph.D
32
“Brief exposure of a major
part of the body to more than
1 Sv may cause acute
radiation syndrome….”
Source: Radiation Injury
Arthur C. Upton, in Goldman's Cecil Medicine
(Twenty Fourth Edition), 2012
Adaptive response can
prevent ARS.
ARS can threaten the
success of space mission
33. Mortazavi SMJ, Ph.D
33
The Galactic Cosmic Radiation (GCR) ions originate from
outside our solar system and contain mostly highly energetic
protons and alpha particles, with a small component of high
charge and energy (HZE) nuclei moving at relativistic speeds
and energies.
About 88% of all GCR particles are hydrogen (protons), 10%
are helium (alpha particles), and the remaining percentage
(~2%) consists of heavier ions.
In addition to GCR, unpredictable and intermittent solar
particle events (SPEs) can produce large plasma clouds
containing highly energetic protons and some heavy ions that
may cause a rapid surge of radiation both outside and within
a spacecraft.
Space Environment
34. Mortazavi SMJ, Ph.D
34
Radiation risk from high level cosmic
rays exposure and microgravity are
two important concerns that need to
be addressed prior to a long-term
space mission.
It has been reported that microgravity
increases the radiation susceptibility
of living organisms by a synergistic
effect.
Mortazavi et al. 2003
Radiation and Microgravity as
Two Main Barriers
40. Mortazavi SMJ, Ph.D
Two survey meters show dose rates
of 142 and 143 µSv/h on contact
with a bedroom wall
40
Our proposed theory was
based on the findings of the
1st report on the induction of
adaptive response in the
residents of High Background
Radiation Areas (HBRAs)
Background of our Theory
42. Mortazavi SMJ, Ph.D
365 citations recorded by
GoogleScholasr
Adaptive response in the
residents of High
Background Radiation
Areas (HBRAs)
42
202 citations recorded by
Scopus
43. Mortazavi SMJ, Ph.D
43
We have previously shown that
chronic exposure of humans to
ionizing radiation can lead to
induction of adaptive response
in the majority of participants.
However, some of the
participants did not show this
phenomenon and even their
lymphocytes became more
sensitive to subsequent high
dose exposures (Synergistic
Effect).
Mortazavi et al. 2003
Inter-individual variabilities!
44. Mortazavi SMJ, Ph.D
44
o Astronauts are chronically exposed to
different levels of galactic cosmic
radiation (GCR).
o If a solar particle event (SPE) occurs,
astronauts may receive doses as high
as 1 Gy in a short time.
o In this light selection of astronauts
with high magnitude of adaptive
response would be critical.
o In this case, astronauts will be
adapted by GCR and when SPE
occurs, they will show a significant
radioresistance.
Mortazavi et al. 2003: GCR vs SPE!
45. Mortazavi SMJ, Ph.D
45
Although NASA report cites our paper,
it looks at AR from a different point of
view:
“…. Cells will be exposed to multiple
hits of protons prior to being traversed
by an HZE particle”
NASA 2016 reprt
Source: Huff, J., Carnell, L., Blattnig, S., Chappell, L., Kerry, G., Lumpkins, S., et al.
(2016). Evidence Report: Risk of Radiation Carcinogenesis. National Aeronautics and
Space Administration (NASA).
46. Mortazavi SMJ, Ph.D
46
NASA 2016 report
Our 2013 report
Substantial evidence shows
that our proposed
mechanism is more
applicable and evidence-
based!
49. Mortazavi SMJ, Ph.D
49
SPEs are a real concern!
“NASA has funded several projects that have provided
evidence for the radiation risk in space. One radiation
concern arises from solar particle event (SPE) radiation,
which is composed of energetic electrons, protons, alpha
particles and heavier particles. SPEs are unpredictable
and the accompanying SPE radiation can place astronauts
at risk of blood cell death, contributing to a weakened
immune system and increased susceptibility to infection”.
Sanzari JK1, Cengel KA1, Wan XS1, Rusek A2, Kennedy AR1.Acute Hematological Effects in Mice Exposed to the Expected Doses,
Dose-rates, and Energies of Solar Particle Event-like Proton Radiation.Life Sci Space Res (Amst). 2014 Jul 1;2:86-91.
PMID: 25202654 PMCID: PMC4155507 DOI: 10.1016/j.lssr.2014.01.003
50. Mortazavi SMJ, Ph.D
50
SPEs are a real concern!
"For future space missions outside of the Earth's
magnetic field, the risk of radiation exposure from
solar particle events (SPEs) during extra-vehicular
activities (EVAs) or in lightly shielded vehicles is a
major concern when designing radiation protection
including determining sufficient shielding
requirements for astronauts and hardware.".
Kim MH1, Hayat MJ, Feiveson AH, Cucinotta FA.Prediction of frequency and exposure level of solar
particle events.Health Phys. 2009 Jul;97(1):68-81. doi: 10.1097/01.HP.0000346799.65001.9c.
51. Mortazavi SMJ, Ph.D
51
"Ancedotal reports suggest Amifostine may have
been carried by US astronauts on their trips to the
moon (Hall, 2012), to be used in case of a solar
flare event where astronauts could be exposed to
an estimated total body dose of several Gy".
Kleiman et al. 2017
Doses in SPE!
52. Mortazavi SMJ, Ph.D
52
o “The likelihood that SPE will
produce doses that are above 1
Gy is small, while the occurrence
of doses that can induce
prodromal risks are quite
possible”.
o Wu et al.
Doses in SPE!
53. Mortazavi SMJ, Ph.D
53
High doses of radiation can induce
profound radiation sickness and death.
Lower doses of radiation induce
symptoms that are much milder
physiologically, but that pose
operational risks that are equally
serious.
Both scenarios have the potential to
seriously affect crew health and/or
prevent the completion of mission
objectives”
o Wu et al.
54. Mortazavi SMJ, Ph.D
54
“Complicating matters is the additional ~
20% probability of short-term solar particle
events (SPEs) during the roughly 400- day
round trip to and from Mars
This could conceivably impart a relatively
high acute dose of predominantly protons and
light ions within 1 hour or less, significantly
increasing mission total dose equivalent
(TDE)”. Rodman et al., Leukemia, 2016
The Probability of a Solar Particle
Event in Mars Missions
http://www.nature.com/leu/journal/vaop/ncurrent/full/leu2016344a.html
20%
55. Mortazavi SMJ, Ph.D
55
The average Effective dose for 6-
month ISS missions of 80 mSv
(Cucinotta et al., 2008).
Transcontinental pilots receive
annual exposures of about 1 to 5
mSv
F. Cucinotta et al. Space Radiation Risk Limits and
Earth-Moon-Mars Environmental Models, NASA
Lyndon B. Johnson Space Center 2101 NASA
Parkway, Houston, Texas 77058
Mars mission potential dose:
Up to several Gy?
57. Mortazavi SMJ, Ph.D
57
NASA standards limit the additional risk of cancer
death by radiation exposure, not the total lifetime
risk of dying from cancer
• Baseline lifetime risk of death from cancer (non-
smokers) – 16% males, 12% females.
• After Mars Mission (solar max), Astronauts
lifetime risk of death from cancer ~20%.
https://www.nasa.gov/sites/default/files/files/1_NAC_HEO_SMD_Committee_Mars_Radiation_Intro_201
5April7_Final_TAGGED.pdf
58. Mortazavi SMJ, Ph.D
58
Is 4-8% increase in lifetime risk of death from cancer so
high? Comparing the risk with what LNT wrongly
predicts for a chest x-ray!
59. Mortazavi SMJ, Ph.D
59
“Low doses of ionizing radiation to cells and animals may
induce adaptive responses that reduce the risk of cancer.
However, there are upper dose thresholds above which
these protective adaptive responses do not occur.”
Mitchel RE1, Burchart P, Wyatt H. Radiat Res. 2008
Dec;170(6):765-75. doi: 10.1667/RR1414.1.
Adaptive response can reduce the risk
of cancer
60. Mortazavi SMJ, Ph.D
60
In a study on adaptive response in high background radiation
area (HBRA) of Yangjiang, China, gene and protein
expression of receptor for advanced glycation end products
(RAGE) and S100A6 in peripheral blood and sputum in the
inhabitants were determined.
RAGE and S100A6 expression were significantly reduced in
both gene and protein level in HBRA residents compared to
those of control area.
Authors concluded that the low expression of RAGE and
S100A6 in HBRA group might be correlated with the adaptive
response and the low mortality of cancer in HBRA.
Adaptive response can reduce the risk
of cancer (cont.)
Zhang SP1, Wu ZZ, Wu YW, Su SB, Tong J.Mechanism study of adaptive response in high
background radiation area of Yangjiang in China.2010 Zhonghua Yu Fang Yi Xue Za Zhi,
Sep;44(9):815-9.
61. • The development of our early model of radioadaptation
as well as the importance of SPEs are discussed in detail
in our recent publications:
1. Bevelacqua JJ, Welsh J, Mortazavi SMJ. Response to ‘An overview
of space medicine’. British Journal of Anaesthesia. 2018
2018/02/01/.
2. 4. Bevelacqua JJ, Mortazavi SMJ. Commentary: Human
Pathophysiological Adaptations to the Space Environment.
Frontiers in Physiology. 2018 2018-January-08;8(1116). English.
3. 5. Mortazavi SMJ, Bevelacqua JJ, Fornalski KW, Welsh J, Doss
M. Comments on "Space: The Final Frontier-Research Relevant to
Mars". Health Phys. 2018 Mar;114(3):344-5. PubMed PMID:
29360711. Pubmed Central PMCID: PMC5784783. Epub
2018/01/24. eng.
Mortazavi SMJ, Ph.D
61
65. Mortazavi SMJ, Ph.D
65
Figure 1. (A) An in vitro adaptive response study
help choosing good candidates for deep manned
space missions. (B) During space mission, the
selected astronauts will be adapted to radiation by
exposure to chronic galactic cosmic radiation
(GCR) and will better tolerate sudden high doses
due to solar particle events (SPE).
66. Mortazavi SMJ, Ph.D
66
A. Different individuals show different
levels of radioadaptation (and some
show no radioadaptation and even
show some kind of synergism; more
adverse biological effects).
B. Candidates for deep space missions
should be screened.
C. The level of the radioadaptation of
each individual can be measured by
ground-based tests (e.g. by exposing
blood samples to a low dose and then
to a high dose radiation and measuring
parameters such as chromosome
aberrations, etc.).
Summary of the hypothesis proposed by our team:
Joseph J. Bevelacqua1 and S.M.J. Mortazavi2*
Front. Physiol., 08 January 2018 |
https://doi.org/10.3389/fphys.2017.01116
67. Measuring the magnitude of
adaptive response
• For measuring the
magnitude of adaptive
response, blood sample of
each candidate should be
divided into 4 aliquots; one
aliquot will only be exposed
to low dose, one only to high
dose, one to both adapting
and challenge doses and one
will be remained unexposed.
Mortazavi SMJ, Ph.D
67
Joseph J. Bevelacqua1 and S.M.J. Mortazavi2*
Front. Physiol., 08 January 2018 |
https://doi.org/10.3389/fphys.2017.01116
68. Measuring the magnitude of
adaptive response
• Therefore, the third aliquots
will be firstly exposed to an
adapting or conditioning low
dose (e.g. a few cGy) and then
they will be irradiated with a
challenging high dose (e.g. 1
Gy). In the next step, the
frequency of dicentrics and
rings will be determined.
Mortazavi SMJ, Ph.D
68
Joseph J. Bevelacqua1 and S.M.J. Mortazavi2*
Front. Physiol., 08 January 2018 |
https://doi.org/10.3389/fphys.2017.01116
69. Measuring the magnitude of adaptive
response
• Then the magnitude of adaptive response (MAR) will be
calculated using this equation:
• MAR = Observed frequency/Expected frequency
While expected frequency can be calculated as:
• Expected frequency =
Freq of Dic/Ring in samples only exposed to low dose +
Freq of Dic/Ring in samples only exposed to high dose –
Freq of Dic/Ring in non-exposed control samples.
Mortazavi SMJ, Ph.D
69
70. Mortazavi SMJ, Ph.D
70
D. The magnitude of radioadaptation of
the candidate can be compared now.
E. Candidates with a high magnitude of
radioadaptation will be good choices for a
deep space mission.
F. During space mission, the selected
astronauts will be adapted to radiation by
chronic galactic cosmic radiation (GCR).
It’s worth noting that the
magnitude and duration of
solar particle event (SPE) is
currently unpredictable.
Summary of the hypothesis proposed by our team (cont.):
Joseph J. Bevelacqua1 and S.M.J. Mortazavi2*
Front. Physiol., 08 January 2018 |
https://doi.org/10.3389/fphys.2017.01116
71. Mortazavi SMJ, Ph.D
71
G. If a solar particle event occurs it can
deliver potentially large doses of energetic
particles even behind modest spacecraft
shielding.
H. Adaptive response can help the selected
astronauts tolerate these relatively high
levels of radiation.
Summary of the hypothesis proposed by our team (cont.):
Joseph J. Bevelacqua1 and S.M.J. Mortazavi2*
Front. Physiol., 08 January 2018 |
https://doi.org/10.3389/fphys.2017.01116
72. AR & Risk of Infection in Deep
Space Missions
Change of virulence (ability to cause
disease)
Dysregulated Immune System
Increased Risk of Infection
AR can Stimulate the Immune System
and Control the Risk of Infection
Mortazavi SMJ, Ph.D
72
73. Two years after Mortazavi et al. 2003 report, cancer
scientists firstly agreed that adaptive response is a
puzzling issue in space radiobiology
• 2005-Cancer specialist Dr. John
Dicello
• “Cells often react in unexpected ways to radiation, notes Dicello.
For example, there's a puzzling phenomenon known as adaptive
response. Sometimes, when tissue is exposed to damaging
radiation, it not only repairs itself, but also learns to repair itself
better next time. How that works is still being investigated”
• “The damage could be less than the two kinds added together -- or
it could be more! There could, perhaps, be an adaptive response in
which lightweight solar protons stimulate repair processes to help
reduce the effects of the heavy cosmic ray ions. Or something
totally unexpected could happen”.
• Mysterious Cancer http://science.nasa.gov/
Mortazavi SMJ, Ph.D
73
74. Mortazavi SMJ, Ph.D
74
George et al. 2007:
“This study of adaptive response is very interesting and it is important
that the phenomenon be investigated further.
in 2007:
75. • Durante and Manti 2008:
• “Another possibility is that an adaptive response to the space environment takes
place after the first exposure, which may confer the exposed individual an increased
radioresistance. Such a response would be similar to that hypothesized to explain
the apparent lack of adverse health effects in VHBRA and HBRA residents. As
pointed out by Mortazavi et al. (2003), radiobiological studies on these areas may
lead to the identification of the cellular and molecular mechanisms by which
susceptibility to genetic damage and cancer is decreased by chronic radiation
exposure, hence helping the astronaut selection process.”
Mortazavi SMJ, Ph.D
75
77. Mortazavi SMJ, Ph.D
77
In 2011, without citing the early idea:
o Low dose (10 cGy)
of protons followed
after either 5-15 min
(immediate) or 16-24
h (delayed) by 1 Gy
of iron ions
o Low dose (10 cGy) of
iron ions followed
after either 5-15 min
or 16-24 h by 1 Gy of
protons
78. Mortazavi SMJ, Ph.D
78
• “Moreover, a second spaceflight apparently does not proportionately increase the
yield of aberrations, suggesting a non-additive or even an infra-additive effect,
raising the possibility of a radio-adaptive response in crewmembers (i.e.,
“radiation hormesis”).”
• “Notwithstanding this finding, knowledge of the basic mechanisms specific to
low-dose radiation, to sequential doses of low-dose radiation and to adaptive
responses is still at a rudimentary stage.”
In 2014, without citing the
early idea:
1st Mission
2nd Mission
Methodological
Error?
The Time
Interval Between
AD and CD?
79. Mortazavi SMJ, Ph.D
79
In 2016, without citing the
early idea:
• Effects of mixed-field proton/iron ion irradiations on cellular
adaptive responses were examined by Elmore et al. using an in vitro
HeLa X human fibroblast hybrid cell transformation assay, but
interestingly was only shown to be radioprotective when 10 cGy 1
GeV/n iron ions was delivered prior to 1 Gy of 1 GeV protons, (that
is, the reverse order of our irradiations).
Protons
Iron Ions
80. Mortazavi SMJ, Ph.D
80
In 2016, without citing the
early idea:
• More recently, Buonanno et al. reported significant radioprotection
for chromosomal damage (micronuclei) induction in primary
human fibroblasts exposed to 20 cGy of 50 MeV or 1 GeV protons
followed by 50 cGy of 1 GeV/n iron ions, with the radioprotective
effect persisting for 24 h.
81. Mortazavi SMJ, Ph.D
81
Space particles have an inevitable impact
on organisms during space missions
Radio-adaptive response (RAR) is a
critical radiation effect due to both low-
dose background and sudden high-dose
radiation exposure during solar storms.
Chenguang Deng et al. Effect of modeled microgravity on radiation-induced adaptive
response of root growth in Arabidopsis thaliana, Mutation Research/Fundamental and
Molecular Mechanisms of Mutagenesis 2017
And in 2017:
82. Mortazavi SMJ, Ph.D
82
Concluding Remarks:
• Even lower doses of radiation which induce
mild symptoms may cause operational risks
which can affect crew health and/or prevent
the completion of mission goals.
• Physical protection alone cannot solve the key
problem of high levels of space radiation.
• We need effective biological protection
methods.
• Screening can solve the existing problems
(choosing astronauts with a high magnitude of
adaptive response after Ground-based in vitro
examinations)!
• In this case, adaptive Response can reduce
ARS and infection risk during long term
manned space missions and decreases cancer
risk post mission
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