Does space radiation alter floral scent? Building and testing the question in Brassica rapa

RNA-seq analysis code and data for a Brassica rapa (Wisconsin Fast Plant) project asking whether galactic-cosmic-ray (GCR) radiation changes floral scent — part of the Lunar LEAF (Life sciences & Engineering for lunar Agriculture and Flight) effort.

CC0-1.0Lunar LEAF RNA-seqNASA OSDR / GeneLab-style 🚧 in development

🚧 Status — work in progress. This repository is an analytical framework and a preliminary, testable signal — not a finished study or a claimed discovery. The two RNA-seq datasets are still being reconciled, the manuscript is a draft outline with open placeholders, and the low-dose radiation effect described below is small and awaits higher-power counts from collaborators to confirm. Treat everything here as provisional.

Overview

Lunar and Martian agriculture will need to know which plant traits change under galactic cosmic radiation. Floral scent underlies pollination and is one of the most biochemically well-mapped plant traits, yet its response to radiation is essentially untested. This project builds a reusable transcriptomic framework to ask the question in Brassica rapa (Wisconsin Fast Plant), a fast-cycling model crop, and reports a first, deliberately modest test. The aim is a resource + method + a specific, falsifiable prediction — a foundation for a properly powered follow-up, not a definitive answer.


What's in this repository

The repo brings together two separate RNA-seq experiments in the same species. They use different samples and different genome annotations, so their gene-ID namespaces (Bra… Chiifu/Ensembl vs BRA… FPsc/RefSeq) do not join directly — reconciling them is the first analytical step.

Preliminary signal — no significant effect at 40 cGy

Stated as a hypothesis to test, not a finding. At this low dose the result is a non-significant trend; it needs the collaborators' higher-power counts to confirm or refute.

Working from a curated, tiered floral-volatile gene set (~363 genes across the terpenoid, benzenoid/phenylpropanoid, fatty-acid/green-leaf-volatile and apocarotenoid routes), the core volatile synthase enzymes are unaffected by 40 cGy. A correlation-aware permutation test (5,000 sample-label shuffles, stratified by genotype and preservative) with Benjamini–Hochberg correction finds no route significant at FDR<0.10 — the naïve competitive test (p ≈ 0.004) was inflated roughly ten-fold by inter-gene correlation. The strongest remaining trend is a mild relative down-shift of the ester/methyltransferase "tailoring" route (permutation p ≈ 0.07, BH q ≈ 0.16 — not significant). That is enough to motivate a specific, falsifiable prediction: if radiation alters scent, it should act on the tailoring methyltransferases, not the core synthases — the same gene family that is lineage-specifically expanded and scent-defining across flowering plants (see Fig 3–4 and the tables). Confirming or refuting this needs higher-powered radiation counts.

Data & code

Sequencing data trace to SRA/NASA OSDR (accessions/DOI to be linked); OSDR data remain subject to the NASA Open Data policy. Part of the Lunar LEAF effort.