Understanding plant growth and development on-orbit is central to humankind's space exploration agenda. The effects of microgravity on plants have been explored for several decades (Paul et al., 2013a; Ričkienė, 2012; Wheeler, 2011; Wolverton and Kiss, 2011; Wyatt and Kiss, 2013); however, to fully understand the effects of microgravity, it is ideal to observe differences in plants that have been developed entirely in the microgravity environment without prior exposure to Earth's 1
One challenge in conducting such experiments in space is ensuring that the configuration is compact, lightweight, safe, and uses minimal crew time. Solid nutrient media (such as with agar or Phytagel) contained in Petri plates has been used in plant research for decades in terrestrial (Barrett-Lennard and Dracup, 1988; Lodha and Netravali, 2005) and orbital research (Paul and Ferl, 2002; Stout et al., 2001; Zupanska et al., 2013) by providing the necessary components required for healthy plant growth. Most importantly, this configuration is lightweight, completely contained, and allows easy access to all plant tissues – especially the roots.
Another consideration is the ease of operation for both the investigators and the astronauts on-board. Mounting an experiment to the International Space Station (ISS) can be complicated given the many conditions required for a successful launch. Hence, for the investigator, it is essential that the biological elements can withstand unpredicted changes in the launch schedule before actual lift-off and delays in operations on-orbit, as such events are common due to a myriad of technical requirements. Therefore, the ideal system should allow for a few days of flexibility without completely voiding the experiment. For example, if the investigator is interested in studying three-day-old plants, and germination is scheduled to be initiated on the ground prior to space vehicle launch, there is always a risk that upon reaching the critical time frame the plant may still be on voyage to the ISS and not accessible for any in-flight operations. Thus, the capability to send dormant seeds that can be initiated for growth at a convenient and flexible time is needed in traversing the challenging environment of spaceflight or other remote environments. An additional advantage of designing the experiment configuration with this flexibility is that the process promotes ease of operations by crew members on-board the ISS.
We have used Phytagel media plates made with commercially available 100 mm square Petri dishes and dormant
Two ecotypes were used for the dormancy tests: Colombia-0 (Col-0) and Wassilewskija (WS). One week before sterilization, seeds were stored in a desiccator containing
Two sets of plates with dormant WS or Col-0 seeds were prepared, wrapped in black cloth, and left for two, four, or six weeks at room temperature (Figures 3–4). On the respective day, the plates were unwrapped and inspected for dormancy breakage. After inspection, they were transferred to a growth room and then evaluated for germination to ensure that the seeds remained viable. Plates were scored for the percentage of seed that held dormancy and subsequently germinated (Figure 5).
Two methods of preparing dormant WS plates were used in the illumination test. The first set of plates were planted with the dry sterilized WS seeds and exposed to far-red light (3.2 μmol m−2 s−1) for 10 min (Nakashima et al., 2014), and were then wrapped in Duvetyne cloth and stored at 4°C. In the second set of plates, dry sterilized WS seeds were prepared as described above, wrapped in Duvetyne black out-cloth, and stored at room temperature. After one week, both sets of plates exposed to ambient room lighting (~100 μmol m−2 s−1) for 30 seconds to inspect for contamination and germination, and then re-wrapped and stored at either 4°C, or at room temperature (respectively) for three additional weeks. After 4 total weeks from planting, plates from both preparation methods were scored for dormancy breakage, and then subsequently evaluated for seed viability by transferring to growth chamber (Figure 6).
Arabidopsis ecotypes Col-0 and WS were evaluated for their ability to be kept in a dormant, yet viable state for greater than a month. Both ecotypes held dormancy and remained viable for six weeks (Figures 3, 4, and 5). Virtually all (> 98%) of the WS seeds remained dormant at room temperature for up to six weeks, and had a viability rate of > 95% (Figures 3 and 5). Of the Col-0 plates subjected to the same regimen, > 97% remained dormant, and then had an average viability rate of > 93% (Figures 4–5). However, although the Col-0 seeds had a high viability rate, the seeds that germinated after being dormant for six weeks were somewhat smaller than those that germinated after four weeks of dormancy (Figure 4).
Due to the nature of spaceflight experiments, it is crucial to be able to inspect the quality of the prepared dormant plates before they are committed to an experiment. This step minimizes the possibility of launching plates containing seeds that have broken germination, and that may have picked up contamination during the preparations. Since the preparations of plates for spaceflight and other remote deployment experiments typically include two to three times as many plates as will actually be deployed, imperfect plates can be excluded from the set turned over for launch.
Both approaches for creating dormant arabidopsis plates discussed here can accommodate a brief (less than 30 seconds) inspection in normal room lighting (less than 180 μmoles m−1s−1) prior to deployment. A comparison of plates prepared by dry sterilization and dark, ambient (20–28°C) temperature storage, and those treated with far-red light treatment and 4°C storage (after the method of Nakashima et al., 2014), is shown in Figure 5. The seeds from both methods remained dormant for three additional weeks after being exposed to ambient room light for 30 seconds one week after they were prepared. Further, greater than 95% of seeds germinated normally when they were finally unwrapped and allowed to grow in standard growth room conditions (Figure 6). These results suggest that opening the light-tight packaging and exposing the dormant plated seeds to ambient light for less than a minute does not drastically affect the seed dormancy. Thus, the plates can be examined, scored for dormancy, and assured free of contamination before being turned over for a flight experiment, or other application where they can reside at room temperature for an extended period of time before use.
The Transgenic Arabidopsis Gene Expression System (TAGES) experiment carried out in 2009–2010 (Figure 7) illustrates the successful use of this technique to deliver dormant arabidopsis seeds to the ISS for germination on orbit (Paul et al., 2012; Paul et al., 2013b). Dormant seeds wrapped in Duvetyne cloth and stowed under ambient (20–28°C) conditions were transported to the ISS via the space shuttle STS-129, STS-130, and STS-131. Upon arrival they were unwrapped, installed onto the ABRS/GIS hardware, and activated for growth by light stimulation. Multiple plates were used in this experiment, all of which illustrates the successful maintenance of seed dormancy and the viability of these dormant seeds (Figure 7).
Accurate characterization of plant responses to the spaceflight environment relies heavily on proper sample preparation. In this paper we described a convenient technique used to prepare sterile, dormant, and viable seeds that are well-suited for passive stowage and on-orbit activation. The material of choice for constructing the light-tight packet is Duvetyne Black-Out Fabric (Seattle Fabrics). Duvetyne is also fire retardant, and now vetted for use on the ISS. We were also able to demonstrate that dormant seeds prepared in this manner can tolerate short exposures to light in the middle of their dormancy period, which can accommodate visual inspection of the plates before they are deployed for an experiment. This feature enables investigators to check their dormant experimental plates for contamination or germinated seed, which in turn allows for the removal of compromised plates from the experimental set.