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71.
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Paul AL Levine HG McLamb W Norwood KL Reed D Stutte GW Wells HW Ferl RJ 《Acta Astronautica》2005,56(6):623-628
Spaceflight experiments involving biological specimens face unique challenges with regard to the on orbit harvest and preservation of material for later ground-based analyses. Preserving plant material for gene expression analyses requires that the tissue be prepared and stored in a manner that maintains the integrity of RNA. The liquid preservative RNAlater (Ambion) provides an effective alternative to conventional freezing strategies, which are limited or unavailable in current spaceflight experiment scenarios. The spaceflight use of RNAlater is enabled by the Kennedy space center fixation tube (KFT), hardware designed to provide the necessary containment of fixatives during the harvest and stowage of biological samples in space. Pairing RNAlater with the KFT system provides a safe and effective strategy for preserving plant material for subsequent molecular analyses, a strategy that has proven effective in several spaceflight experiments. Possible spaceflight scenarios for the use of RNAlater and KFTs are explored and discussed. 相似文献
74.
We consider four aspects of interstellar chemistry for comparison with comets: molecular abundances in general, relative abundances
of isomers (specifically, HCN and HNC), ortho/para ratios for molecules, and isotopic fractionation, particularly for the
ratio hydrogen/deuterium. Since the environment in which the solar system formed is not well constrained, we consider both
isolated dark clouds where low mass stars may form and the "hot cores" that are the sites of high mass star formation. Attention
is concentrated on the gas phase, since the grains are considered elsewhere in this volume.
This revised version was published online in June 2006 with corrections to the Cover Date. 相似文献
75.
英国伊顿公学被外界誉为制造精英的流水线,风靡一时的哈利波特黑色礼服和神秘古堡,让人不得不相信魔力依存的伊顿,迄今已有19名英国首相从那座古堡中走了出来。伦敦以西20多英里的温莎小镇,浸润着英王室数百年的恩泽。567个年头的漫漫岁月,侵蚀了伊顿古旧的砖墙,让伊顿显得有些老气横秋,但是,伊顿依然坚守着传统的价值,锤炼着过去,现在和未来恒久的伊顿教育的哲学。伊顿的教育不只在于成功,而是在于孩子们一个完整的人生,为此,成绩和专业仅仅只是他们的一个基本点。 相似文献
76.
Ralph L. McNutt Jr. Stefano A. Livi Reid S. Gurnee Matthew E. Hill Kim A. Cooper G. Bruce Andrews Edwin P. Keath Stamatios M. Krimigis Donald G. Mitchell Barry Tossman Fran Bagenal John D. Boldt Walter Bradley William S. Devereux George C. Ho Stephen E. Jaskulek Thomas W. LeFevere Horace Malcom Geoffrey A. Marcus John R. Hayes G. Ty Moore Mark E. Perry Bruce D. Williams Paul Wilson IV Lawrence E. Brown Martha B. Kusterer Jon D. Vandegriff 《Space Science Reviews》2008,140(1-4):315-385
The Pluto Energetic Particle Spectrometer Science Investigation (PEPSSI) comprises the hardware and accompanying science investigation on the New Horizons spacecraft to measure pick-up ions from Pluto’s outgassing atmosphere. To the extent that Pluto retains its characteristics similar to those of a “heavy comet” as detected in stellar occultations since the early 1980s, these measurements will characterize the neutral atmosphere of Pluto while providing a consistency check on the atmospheric escape rate at the encounter epoch with that deduced from the atmospheric structure at lower altitudes by the ALICE, REX, and SWAP experiments on New Horizons. In addition, PEPSSI will characterize any extended ionosphere and solar wind interaction while also characterizing the energetic particle environment of Pluto, Charon, and their associated system. First proposed for development for the Pluto Express mission in September 1993, what became the PEPSSI instrument went through a number of development stages to meet the requirements of such an instrument for a mission to Pluto while minimizing the required spacecraft resources. The PEPSSI instrument provides for measurements of ions (with compositional information) and electrons from 10 s of keV to ~1 MeV in a 160°×12° fan-shaped beam in six sectors for 1.5 kg and ~2.5 W. 相似文献
77.
Antonella A. Albuja Daniel J. Scheeres Rita L. Cognion William Ryan Eileen V. Ryan 《Advances in Space Research (includes Cospar's Information Bulletin, Space Research Today)》2018,61(1):122-144
The Yarkovsky-O’Keefe-Radzievskii-Paddack (YORP) effect is a proposed explanation for the observed rotation behavior of inactive satellites in Earth orbit. This paper further explores the YORP effect for highly asymmetric inactive satellites. Satellite models are developed to represent the GOES 8 and GOES 10 satellites, both of which are currently inactive in geosynchronous Earth orbit (GEO). A simple satellite model for the GOES 8 satellite is used to analyze the short period variations of the angular velocity and obliquity as a result of the YORP effect. A more complex model for the rotational dynamics of the GOES 8 and GOES 10 satellites are developed to probe their sensitivity and to match observed spin periods and states of these satellites. The simulated rotation periods are compared to observations for both satellites. The comparison between YORP theory and observed rotation rates for both satellites show that the YORP effect could be the cause for the observed rotational behavior. The YORP model also predicts a novel state for the GOES 8 satellite, namely that it could periodically fall into a tumbling rotation state. Recent observations of this satellite are consistent with this prediction. 相似文献
78.
79.
Paul AL Zupanska AK Ostrow DT Zhang Y Sun Y Li JL Shanker S Farmerie WG Amalfitano CE Ferl RJ 《Astrobiology》2012,12(1):40-56
80.
Gerstenmaier W 《Acta Astronautica》2004,54(11-12):777-778
This introductory address provides a brief overview and a timeline for construction of the International Space Station, beginning with the July 2000 launch of the Russian Service Module, Zvezda, and ending with the Mission STS-112. 相似文献