Task Progress:
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In this year of funding (March 2024 - March 2025), we focused on completing screening and data collection on the candidate genes from our RNA sequencing (RNA-seq) contrast list using T-DNA insertional mutants from the Salk collection. In previous work, we screened approximately 90 T-DNA lines for mutant phenotypes, finding 11 mutant lines with putative gravity-involved phenotypes for further analysis. To extend this work, we completed necessary phenotyping and genotyping experiments on all lines received to date. The grant funded 16 undergraduate research students in total over the current period, including 9 full-time summer research positions. Students performed all aspects of the project, including preparing sterile growth media and sowing seeds, imaging experiment setup and image analysis, DNA and RNA isolations, and polymerase chain reaction (PCR) or reverse transcription-polymerase chain reaction (RT-PCR) experiments.
Thus far, we have 96 T-DNA mutant lines on hand and have successfully completed genotyping 65. Of the lines screened thus far, 7 have been confirmed heterozygous for the T-DNA allele, and of those, 2 show a gravity related phenotype; 56 lines have been confirmed homozygous for the T-DNA carrying allele; the remainder of the lines genotyped have shown ambiguous results and we are in the process of redesigning primers. Some lines without a positive confirmation PCR result may be due to a later transposition event with the T-DNA. We are in the process of amplifying and sequencing the region surrounding the location of the T-DNA insertion to detect possible footprint deletions. Some of the lines also showed a lack of positive product for the positive control primer pair as well, indicating bad primer design or PCR conditions. Sequencing in the region of the purported T-DNA will also shed light on these lines.
In addition to genotyping, we are also testing for transcript knock-down in the T-DNA lines to be able to correlate any phenotypes observed with lack of transcript abundance. To date we have carried out RT-PCR on 55 lines and confirmed the lack of mRNA transcript for the gene of interest in 37 of our lines, with 2 lines showing no difference in transcript abundance compared to the wild-type. The RT-PCR experiments required for this assay are more demanding than the genotyping PCR experiments, leading to an overall slower rate of completion. We carried out this assay along with many others as part of my Plant Physiology lab experience for 16 students in Spring 2024. I have redesigned the lab experience around this NASA-funded screening project to provide students hands-on experience with real research. Since so many of the assays and screens of these mutant lines is routine in the lab, this will provide students the opportunity to contribute to the project while learning valuable skills in bioinformatics, DNA and RNA isolation, real-time RT-PCR, and various plant growth analyses. I incorporated this project into the lab portion of the class in the previous two years and it was moderately successful, with about half of the data generated by student groups of sufficient quality to be useful. Last spring, I structured the work a bit more and provided templates for the students to collect and interpret results, which mitigate some of the errors I saw in previous years.
In addition to the molecular characterization of mutants, we have made good progress on the growth experiments designed to test the mutants for any gravity-related phenotypes. We have developed a novel assay to detect differences in the regulation of differential growth. The assay is based on a previous technique used heavily in my lab, called ROTATO, which uses real-time image analysis to constrain the root tip at a constant angle over time by rotating the plate. This technique is good for measuring single roots, but does not scale well to large numbers of roots on a plate, as required for a medium-scale mutant screening project. I have used the average response rate (rotation) of wild-type roots as an input to control rotation of whole plates of mutant seedlings, reasoning that if the roots have “normal” gravity response, their tip angles will remain relatively unchanged because they are able to maintain the differential growth required to do so. We have now completed analysis of 76 T-DNA mutant lines using this technique and have identified 20 lines that show a statistically significant difference in response compared to wild-type. 16 of the 20 lines show significantly reduced gravity response, while the other 4 lines show greater gravity response.
Other experiments to characterize the mutants include standard reorientation assays to assess gravitropic response and root phototropic assays to try to distinguish gravity perception processes from growth regulation and gravity response elements. We have conducted hundreds of standard root reorientation assays thus far, and have identified 26 mutants having a significantly different gravity response after 3 h. Interestingly, of the 26 mutants showing a free response gravity phenotype, only 8 also show a significant continuous response phenotype. The use of both assays thus may both expand the pool of possible contributors to gravity response and provide useful physiological differences between the two assays for future follow-up experiments. We also began analyzing responses as a function of time, since we have been collecting angle measurements across a 3-h response period. These comparisons indicate differences in kinetics that could also reveal hints at the underlying mechanisms perturbed by the mutation.
For the root phototropism assays, we have done some pilot testing with large-scale experiments, but I am unsatisfied so far with the amount of curvature induced in the positive and negative controls. Last summer, one of the student researchers worked on developing a better assay design and construction that will optimize this response, but we have not yet screened a large number of the mutants yet. The lab also completed the acquisition of a ground-based engineering model of flight hardware designed for the European Space Agency’s European Modular Cultivation System (EMCS) that provides highly repeatable phototropic stimulation, which we have begun adopting for potential use in carrying out these experiments.
This year we continued work designing and cloning Clustered Regularly Interspaced Short Palindromic Repeats (CRISPR) constructs to knock out genes for which there is no T-DNA line available in a stock center. Thus far, we have created guide sequence constructs for a total of 23 genes showing a gravitropic phenotype. We have successfully cloned the guide RNAs into expression vectors and completed floral dip of wild type (wt) plants. We are currently in the process of screening the seeds from these T0 lines for resistance and selfing those. In addition to creating knockouts for those genes lacking a Salk T-DNA insertion, this process will also allow us to generate second alleles for those genes for which we find a phenotype and wish to confirm.
In addition to using CRISPR to knock out genes of interest, we have begun making double-mutants between those mutants that show a promising gravity-related phenotype and the pgm-1 mutant, which lies at the heart of this project. By testing the phenotypes of double mutants in the pgm-1 mutant background, we hope to identify molecular participants in the non-statolith sensing pathway by finding double mutants with a stronger phenotype than either single mutant alone. This year we crossed another 10 lines to pgm, making a total of 33 crosses with our confirmed mutants into the pgm-1 mutant to date, with 23 confirmed F1 lines. In addition, we are in the process of screening 4 F3 lines collected from individual F2 parents to identify double mutants. In addition to crossing into the pgm-1 background, we have also been crossing candidate mutants into the semi-quantitative auxin reporter line R2D2, with 12 lines at the F1 stage to date and 2 lines at the confirmed F3 stage. These will allow us to determine the potential involvement of our new mutants in the regulation of auxin transport during gravitropism.
This year we made significant progress on a rewritten and renewed ROTATO system. I had previously rewritten the core image analyzer in MATLAB and have successfully used this image processing engine to constrain roots at the desired angle for indefinite periods. This system takes images captured from a standard Raspberry Pi HQ camera module, which uploads the images to a server where the computer running MATLAB can access them and control rotation of the vertical stage holding the root. This year we focused on transitioning the core analyzer away from MATLAB and into Python, which would enables us to deploy the software on any Raspberry Pi imaging computer in the lab and also share it widely for those interested in incorporating it into their own projects. One of my summer research students has completed a beta version of the software and we are currently refining it in the lab. We hope to generate a methods-based publication from this work in the near future.
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