| New Task Description (Ed., 12/01/24)
Background.
Studies of bone loss in ISS astronauts, using quantitative computed tomography (QCT) of the hip and spine and high-resolution-peripheral QCT (HRpQCT) of the lower leg, describe losses of trabecular bone mineral density (Trb vBMD) that are not detectable by the clinical test for age-related osteoporosis (Op), i.e., areal bone mineral density (aBMD) measured by dual-energy X-ray absorptiometry (DXA). Both QCT and HRpQCT revealed losses in Trb vBMD immediately following long duration (LD) spaceflight and continuing in some individuals even after recovery periods of a year or more. We reported rapid loss rates of spaceflight hip QCT Trb vBMD, relative to rates with terrestrial aging. In a pilot study, hip QCT showed lack of recovery of hip Trb vBMD to baseline in 4 of 10 astronauts evaluated 2 years after return to Earth. Analyses of serum and urine collected during spaceflight showed significant in-flight elevation of bone resorption (BR) markers in the 4 astronauts who did not recover Trb vBMD vs. the 6 astronauts who did; a biomarker for bone formation (BF) remained stable until ~120 days into the flight. Biochemical assays consistently show BR exceeding BF during spaceflight accounting for a rapid loss of Trb vBMD which could also increase the risk for disrupted trabecular connectivity. While the efficacy of an oral bisphosphonate to mitigate spaceflight bone loss has been substantiated in an astronaut flight study, there is reduced willingness in some stakeholders to use a pharmaceutical countermeasure. Hence, there is a concern for the risk of irreversible losses in trabecular connectivity in the absence of an anti-resorptive countermeasure. Such trabecular disruptions are associated with skeletal fragility and fractures in other populations undergoing bone loss but have not been characterized in astronaut hips because of prohibitive radiation exposures needed for high-resolution imaging of deeply embedded bone. HRpQCT has low radiation and sufficient resolution to study microarchitecture, but only for peripheral sites such as the lower leg and wrist. Hence, it is critical to apply a technology to the deeply embedded hip bone with no ionizing radiation, such as MRI, to safely define the effect size of rapid bone loss during spaceflight on trabecular microarchitecture, particularly with the reported observations of delayed or no recovery in hip Trb vBMD.
Hypothesis.
We hypothesize that 1) LD astronauts will have an increased risk for bone fractures because of disruptions in Trb uArch of the hip and 2) a 3-Tesla (3T) MRI scanning protocol can detect disruptive changes in Trb uArch, some of which could be irreversible.
Specific Aims:
We will investigate this hypothesis by addressing the following Specific Aims (SA):
SA 1) Use spinal cord injury (SCI) to model the skeletal effects of LD spaceflight on hip trabecular bone microarchitecture (Trb uArch).
SA 2) Apply a previously validated 3T MRI protocol to assess serial changes in hip Trb uArch (over a 12-mth time period) following spinal cord injury (SCI) in consented subjects.
SA 3) Verify that 3T MRI data can discriminate disrupted hip Trb connectivity in subjects with SCI relative to age- and sex-matched ambulatory controls.
SA 4) Validate that an 3T MRI protocol can detect disruptions in the connectivity of Trb bone uArch in the distal tibia (ankle region) in subjects with SCI as compared to detection by HRpQCT.
SA 5) Compare estimates of trabecular bone strength (as a surrogate for fracture risk) at hip and the ankle by Finite Element modeling of Trb uArch data, including verification and validation processes informed by data. Data of Trb uArch are derived from serial testing (12-mth apart) of hip and ankle in study subjects (able-bodied controls and SCI) by 3T MRI and HRpQCT.
--------------------------- New Task Description (Ed., 9/30/23)
Background.
Studies of bone loss in ISS astronauts, using quantitative computed tomography (QCT) of the hip and spine and high-resolution-peripheral QCT (HRpQCT) of the lower leg, describe losses of trabecular bone mineral density (Trb vBMD) that are not detectable by the clinical test for age-related osteoporosis (Op), i.e., areal bone mineral density (aBMD) measured by dual-energy X-ray absorptiometry (DXA). Both QCT and HRpQCT revealed losses in Trb vBMD immediately following long duration (LD) spaceflight and continuing in some individuals even after recovery periods of a year or more. We reported rapid rates of spaceflight hip QCT Trb vBMD loss, relative to terrestrial aging rates. In a pilot study, hip QCT showed lack of recovery of hip Trb vBMD to baseline in 4 of 10 astronauts evaluated 2 years after return to Earth. Analyses of serum and urine collected during spaceflight showed significant in-flight elevation of bone resorption (BR) markers in the 4 astronauts who did not recover Trb vBMD vs. the 6 astronauts who did; a biomarker for bone formation (BF) remained stable until ~120 days into the flight. Biochemical assays consistently show BR exceeding BF during spaceflight accounting for a rapid loss of Trb vBMD which could also increase the risk for disrupted trabecular connectivity. While the efficacy of an oral bisphosphonate to mitigate spaceflight bone loss has been substantiated in an astronaut flight study, there is reduced willingness in some stakeholders to use a pharmaceutical countermeasure. Hence, there is a concern for the risk of irreversible losses in trabecular connectivity in the absence of an anti-resorptive countermeasure. Such trabecular disruptions are associated with skeletal fragility and fractures in other populations undergoing bone loss but have not been characterized in astronaut hips because of prohibitive radiation exposures needed for high-resolution imaging of deeply embedded bone. HRpQCT has low radiation and sufficient resolution to study microarchitecture, but only for peripheral sites such as the lower leg and wrist. Hence, it is critical to apply a technology with no ionizing radiation such as MRI to safely define the effect size of spaceflight on hip trabecular microarchitecture, particularly with the observation of delayed or no recovery in hip Trb vBMD.
Hypothesis.
We hypothesize that 1) LD astronauts will have an increased risk for bone fractures because of disruptions in Trb uArch of the hip and 2) a 3-Tesla (3T) MRI scanning protocol can detect disruptive changes in Trb uArch, some of which could be irreversible.
Specific Aims:
We will investigate this hypothesis by addressing the following Specific Aims (SA):
Specific Aims: 1) Identify and consent individuals with SCI to assess the effects of prolonged unloading to the hip; 2) Apply a previously-validated 3T MRI protocol to characterize serial changes in hip trabecular microarchitecture of SCI subjects at 0 and 12-mo following injury; 3) Compare the ability of 3T MRI to discriminate loss of trabecular connectivity between subjects with SCI (Aim 1) and age- and sex-matched ambulatory controls for the hip and ankle; 4) Evaluate the ability of MRI to discriminate changes in trabecular connectivity at the hip and ankle (by MRI serial testing 12 months apart) and the subsequent effects on trabecular bone strength (by the analysis of Finite Element models of serially acquired trabecular microarchitecture data). |