Day J, McPherson A
Department of Biochemistry, University of California, Riverside 92521.
Protein Sci. 1992 Oct;1(10):1254-68. doi: 10.1002/pro.5560011004.
Macromolecular crystal growth experiments, using satellite tobacco mosaic virus (STMV) and canavalin from jack beans as samples, were conducted on a US Space Shuttle mission designated International Microgravity Laboratory--1 (IML-1), flown January 22-29, 1992. Parallel experiments using identical samples were carried out in both a vapor diffusion-based device (PCG) and a liquid-liquid diffusion-based instrument (CRYOSTAT). The experiments in each device were run at 20-22 degrees C and at colder temperatures. Crystals were grown in virtually every trial, but the characteristics of the crystals were highly dependent on the crystallization technique employed and the temperature experience of the sample. In general, very good results, based on visual inspection of the crystals, were obtained in both PCG and CRYOSTAT. Unusually impressive results were, however, achieved for STMV in the CRYOSTAT instrument. STMV crystals grown in microgravity by liquid-liquid diffusion were more than 10-fold greater in total volume than any STMV crystals previously grown in the laboratory. X-ray diffraction data collected from eight STMV crystals grown in CRYOSTAT demonstrated a substantial improvement in diffraction quality over the entire resolution range when compared to data from crystals grown on Earth. In addition, the extent of the diffraction pattern for the STMV crystals grown in space extended to 1.8 A resolution, whereas the best crystals that were ever grown under conditions of Earth's gravity produced data limited to 2.3 A resolution. Other observations indicate that the growth of macromolecular crystals is indeed influenced by the presence or absence of gravity. These observations further suggest, consistent with earlier results, that the elimination of gravity provides a more favorable environment for such processes.
利用烟草花叶卫星病毒(STMV)和刀豆中的伴刀豆球蛋白作为样本,在1992年1月22日至29日飞行的名为国际微重力实验室-1(IML-1)的美国航天飞机任务中进行了大分子晶体生长实验。使用相同样本在基于气相扩散的装置(PCG)和基于液-液扩散的仪器(低温恒温器)中进行了平行实验。每个装置中的实验在20-22摄氏度以及更低温度下进行。几乎在每次试验中都生长出了晶体,但晶体的特性高度依赖于所采用的结晶技术以及样本经历的温度。总体而言,基于对晶体的目视检查,在PCG和低温恒温器中都获得了非常好的结果。然而,在低温恒温器仪器中,STMV取得了异常令人印象深刻的结果。通过液-液扩散在微重力条件下生长的STMV晶体总体积比之前在实验室中生长的任何STMV晶体大10倍以上。从在低温恒温器中生长的8个STMV晶体收集的X射线衍射数据表明,与在地球上生长的晶体数据相比,在整个分辨率范围内衍射质量有了显著提高。此外,在太空中生长的STMV晶体的衍射图案范围扩展到了1.8埃分辨率,而在地球重力条件下生长的最佳晶体产生的数据仅限于2.3埃分辨率。其他观察结果表明,大分子晶体的生长确实受到重力存在与否的影响。这些观察结果进一步表明,与早期结果一致,消除重力为这些过程提供了更有利的环境。