Human Research Program
Improving Kidney Stone Detection in Space Analogs
Project Description
POSTDOCTORAL FELLOWSHIP 1. Project Aims The twinkling artifact (TA) is a rapid color-shift that selectively highlights hard objects such as kidney stones in color-Doppler ultrasound images; however, its inconsistent appearance has limited its clinical use. Our objective is to develop an ultrasound imaging protocol to enhance kidney stone detection in space, addressing ExMC Gap 4.13. In the 3rd year renewal proposal, the aims are: AIM 1: Develop, refine, and test in space analogs improved ultrasound imaging protocols to enhance kidney stone detection. AIM 2: Determine the effect of breathing gas composition on twinkling in swine. AIM 3: Determine the role of bacteria in twinkling. 2. Key Findings Twinkling was reduced when 9 swine were exposed to elevated carbon dioxide (CO2) levels (similar to what is found on the International Space Station (ISS)) with the degree of reduction in twinkling correlating with the concentration of CO2; twinkling increased when swine were exposed to 100% oxygen. When 4 swine were exposed to elevated CO2 levels versus normal air, there was an unrecoverable decrease in twinkling over the course of the study. Concentrations of gases in the blood and urine suggest both O2 and CO2 contribute to twinkling. Imaged 7 human subjects in the hyperbaric chamber and found a statistically significant increase in twinkling when subjects breathe 100% O2 at 1.6 ATA (the decompression stop) compared to initial twinkling levels. Growing several different species of bacteria on sterilized stones did not induce or increase twinkling; bacteria grown on agar plates also did not twinkle. Found evidence suggesting the contribution of internal micro-cracks to twinkling in addition to the surface crevice bubbles. Low frequency ultrasound was found to enhance twinkling if already present on stones, but did not cause non-twinkling stones to twinkle. Published 2 papers in peer-reviewed scientific journals; 4 additional papers are in preparation. Presented at 5 scientific conferences including an invited talk at the Acoustical Society of America Meeting in Honolulu, HI. Mentored a Pacific Science Center summer high school student and a summer undergraduate student. Organized a Wide World of Sound Booth at Engineering Discovery Days as Chair of the Outreach Committee, Cascadia Regional Chapter, Acoustical Society of America. Was interviewed for 2 National Space Biomedical Research Institute (NSBRI)/University of Washington promotional videos and a book on women in science. Accepted a tenure-track assistant professor position in the Graduate Program in Acoustics, Department of Aerospace Engineering at the Pennsylvania State University. 3. Impact We have discovered that breathing CO2 significantly reduces twinkling in swine and have shown that breathing normal air (0.04% CO2) is insufficient to restore twinkling. The results also suggest that breathing elevated O2 may restore or enhance twinkling, which is supported in our human hyperbaric study. Bacteria grown on sterile stones or agar plates was found to be insufficient to induce or enhance twinkling; bacteria may need to be present in the stone formation process to contribute to twinkling. While increasing the energy delivered to the stone or lowering the transmitted frequency has been found to enhance twinkling, there remains some stones that do not twinkle. Further investigation into the stone formation process and/or the presence or absence of internal micro-cracks, which have been shown to play a role in twinkling in addition to the surface crevice bubbles, may help elucidate why some stones are resistant to twinkling so new techniques can be developed. 4. Proposed research While this project is ended with NSBRI, we plan to finish recruiting and imaging the last subject for the human hyperbaric study and plan to submit 3 more journal publications. We are also looking to investigate in humans the effect of either an elevated CO2 or O2 environment on kidney stone twinkling.
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Anticipated Benefits
Kidney stones currently affect approximately 1 in 11 Americans and the prevalence is increasing worldwide. In the US alone, more than 3 million diagnoses and treatments are made annually at an estimated annual cost of over $10 billion. Further, more than 50% of stone-formers have a repeat stone event within 5 years. The risk of renal stone formation (Exploration Medical Capabilities--ExMC 4.13) is considered a "shall" for all missions beyond the International Space Station. Specific in-flight conditions including bone demineralization, dehydration, stasis, and increased alkalinity of the urine contribute to an increased risk of renal stone formation in space. US astronauts have reported more than 30 symptomatic stone events that have occurred pre- or post-flight; one noteable in-flight stone incident has been described by the Russian space program where a crewmate was found "writhing in pain." While no US astronaut has experienced an in-flight kidney stone event, the incidence of kidney stones in space is expected to rise as missions become longer, astronauts are exposed to gravitational changes, and immediate transport to Earth becomes more problematic. Stone size is a significant predictor for the severity of a stone incident, as small stones may pass on their own causing relatively little pain. The Integrated Medical Model team defines two renal stone scenarios; the best case scenario (i.e., where stones pass safely and spontaneously) is predicted to occur in 70% of cases where stones are small (<6 mm diameter). However, as stones increase to >6 mm, only 20% of stones are predicted to pass safely and spontaneously. These data show the need for a diagnostic tool that allows for routine monitoring of people at risk for developing kidney stones both on Earth and in space. On Earth, computed tomography (CT) is considered the gold standard for kidney stone detection; plane film, kidney-ureter-bladder x-ray is also used to detect kidney stones. Both of these technologies expose patients to ionizing radiation. Our goal is to make ultrasound a more robust tool to detect small kidney stones, thereby reducing patient exposure to ionizing radiation and reducing the costs associated with kidney stones. Improving ultrasound for kidney stone detection would allow emergency rooms to diagnose kidney stones immediately rather than sending the patient to radiology for an x-ray or CT. Ultrasound could also be used for more routine monitoring of kidney stones so that steps could be taken to avoid emergency surgery. While we have not found a way for ultrasound to predict stone composition, significant improvements have been made in kidney stone imaging and sizing. We have shown that surface crevice bubbles and internal micro-cracks contribute to the ultrasound twinkling artifact and we continue to increase our understanding of kidney stone formation. Furthermore, we have found that breathing elevated levels of oxygen may enhance twinkling, which could help make kidney stones even easier to diagnose, particularly for non-expert sonographers. In space, ultrasound is one of the few imaging technologies that can be safely flown, and our improved kidney stone detection protocols will make ultrasound a more robust tool for early stone detection, which is critical for minimizing mission disruption and reducing the risk of an unpredictable and life-threatening renal stone incident.
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Primary U.S. Work Locations and Key Partners
| Organizations Performing Work | Role | Type | Location |
|---|---|---|---|
| National Space Biomedical Research Institute (NSBRI) | Lead Organization | Industry | Houston, Texas |
| University of Washington | Supporting Organization | Academia | Seattle, Washington |
Primary U.S. Work Locations
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Washington
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