The STS-76 (Shuttle-Mir 3) spaceflight provided an opportunity to test two questions about radiation responses in C. elegans. First, does the absence of gravity modify the dose-response relation for mutation and second, what are the features of the mutation spectrum resulting from exposure to cosmic rays? These questions were put to the test in space using the miniaturized biology laboratory "Biorack" which was housed in the Spacehab module aboard shuttle Atlantis. The mission flew in March, 1996 and was a shuttle rendezvous with the Russian space station Mir. To answer question 1 worms of balancer strain JP10 (
dpy-18/3T1(III)III;
unc-46/eT1(V) V)were launched as dauers in S medium. On orbit they were injected into a series of lexan tubes containing a cylindrical shell of agarose-gelled S medium with a central airspace. The agarose media also contained 0 to 1.3 mCi of 45CaCl2 (a Beta particle emitter) such that a dose vs response curve would be generated from each series of tubes. One series of tubes was incubated at 22 deg C at 0 gravity while a matched set was placed on a 1 x g centrifuge. Matched ground controls at 1 x g and 1.4 x g were also performed. Worms were washed and plated onto E. coli-seeded plates immediately after landing to recover the dauers and processed for autosomal recessive lethal mutation. The results showed that viability and fertility of worms were not significantly altered by gravity and that the mutation dose-response from 0 to 100 Gy yielding 0 to 7% mutants was also unmodulated. To answer question 2,
fem-3(
q20gf) dauer larvae (suspended in S buffer) were placed in lexan tubes and transferred on orbit from a storage locker to the Biorack where they were incubated for the duration of the mission at 22C. The cosmic ray environment for these worms was measured using a combination of thermoluminescent detectors and plastic nuclear track detectors included in the tube-holding container. Upon landing these animals were recovered and screened for mutants by a temperature shift to 25C. Twenty-six independent mutants were recovered, giving a mutation frequency of 2x10-5. This is approximately three times that for ground controls. Each strain was analyzed by Southern hybridization. Only one polymorphism was detected. This spectrum will be compared to those obtained using several ground-based radiation sources and to those obtained on a previous spaceflight (STS-42, IML-1).