Selection of the Mars Science Laboratory Landing Site

The selection of Gale crater as the Mars Science Laboratory landing site took over five years, involved broad participation of the science community via five open workshops, and narrowed an initial >50 sites (25 by 20?km) to four finalists (Eberswalde, Gale, Holden and Mawrth) based on science and safety. Engineering constraints important to the selection included: (1)?latitude (±30°) for thermal management of the rover and instruments, (2)?elevation (<?1?km) for sufficient atmosphere to slow the spacecraft, (3)?relief of <100–130?m at baselines of 1–1000?m for control authority and sufficient fuel during powered descent, (4)?slopes of <30° at baselines of 2–5?m for rover stability at touchdown, (5)?moderate rock abundance to avoid impacting the belly pan during touchdown, and (6)?a?radar-reflective, load-bearing, and trafficable surface that is safe for landing and roving and not dominated by fine-grained dust. Science criteria important for the selection include the ability to assess past habitable environments, which include diversity, context, and biosignature (including organics) preservation. Sites were evaluated in detail using targeted data from instruments on all active orbiters, and especially Mars Reconnaissance Orbiter. All of the final four sites have layered sedimentary rocks with spectral evidence for phyllosilicates that clearly address the science objectives of the mission. Sophisticated entry, descent and landing simulations that include detailed information on all of the engineering constraints indicate all of the final four sites are safe for landing. Evaluation of the traversabilty of the landing sites and target “go to” areas outside of the ellipse using slope and material properties information indicates that all are trafficable and “go to” sites can be accessed within the lifetime of the mission. In the final selection, Gale crater was favored over Eberswalde based on its greater diversity and potential habitability.     

The Dawn Framing Camera

The Framing Camera (FC) is the German contribution to the Dawn mission. The camera will map 4 Vesta and 1 Ceres through a clear filter and 7 band-pass filters covering the wavelengths from the visible to the near-IR. The camera will allow the determination of the physical parameters of the asteroids, the reconstruction of their global shape as well as local topography and surface geomorphology, and provide information on composition via surface reflectance characteristics. The camera will also serve for orbit navigation. The resolution of the Framing Camera will be up to 12 m per pixel in low altitude mapping orbit at Vesta (62 m per pixel at Ceres), at an angular resolution of 93.7 ??rad?px^?1. The instrument uses a reclosable front door to protect the optical system and a filter-wheel mechanism to select the band-pass for observation. The detector data is read out and processed by a data processing unit. A power converter unit supplies all required power rails for operation and thermal maintenance. For redundancy reasons, two identical cameras were provided, both located side by side on the +Z-deck of the spacecraft. Each camera has a mass of 5.5 kg.     

多载波DS—CDMA在数字微波通信系统中的应用

基于数字微波通信系统的特点，介绍了多载波SD-CDMA（Multicarrier-DS-CDMA,即MC-DS-CDMA）调制技术的基本原理及其应用于数字微波通信系统中的具体实现方法。从理论上详细地分析了MC-CDMA工作方式的性能，并将其与传统的数字微波通信系统进行了比较，阐明了将MC-DS-CDMA工作方式应用于数字微波通信系统的必要性。     

带着全家去出海

这个夏天,有没有筹划一次全家人都可以参与的旅行呢?带着爱人或者家里的小朋友与大自然进行一次深入的交流,想必对于彼此之前感情的沟通能起到不错的作用。如果可以,带着全家去出海吧!     

Numerical modelling of radiance of the presumed dust torus around Mars in the 0.350–1 μm spectral range

With the use of high performance liquid chromatography the products of abiogenic synthesis of adenine nucleotides in solid films were indentified and estimated quantitatively. The main products of photosynthesis appeared to be adenosine and deoxyadenosine monophosphates. Maximal yield of these products in case of adenosine has been 0.36 for 5′AMP, 0.41% for 2′(3′)AMP, 0.20 for 2′3′cAMP; in case of deoxyadenosine 0.13% for 5′dAMP, 0.15% for 3′dAMP, 0.24% for 3′5′cdAMP. The destruction of initial adenosine and deoxyadenosine by the end of the experiment was 10 and 15%, respectively. By the increasing of irradiation dose, 5′AMP and 5′dAMP synthesized in the cource of VUV photolysis were destructed up to adenine, its yield being 15% in both cases.     

Women''s place in space exploration

A Mars manned space mission would be characterized by long-lasting psycho-social stress for its human participants. Based on the results of our and other authors' experiments with small human groups under simulated space stress conditions, and bearing in mind historical evidence of the changing role of women in human society, the differences of feminine and masculine cognitive patterns should be taken into greater account. Participation of women in astronautics should be reconsidered from the point of view of the roles of women as members of a space ship crew, as members of a space control centre and in relation to the family life of male astronauts on long-term space missions.     

小卫星星座自主定轨的论证与仿真

在建立星座自主定轨条件方程的基础上,对其求解的可行性进行了分析、论证和仿真计算。结果表明：在仅考虑一阶摄动理论的情况下,升交点赤经总是秩亏的,即使考虑更精密的摄动模型,其条件方程也近似病态。其它根数在很多情况下也有相关性。因此,为了最大限度地满足自主定轨的要求,在星座结构设计时应尽量考虑不同类型轨道的卫星。     

Graviperception in ciliates: steps in the transduction chain.

Ciliates represent suitable model systems to study the mechanisms of graviperception and signal transduction as they show clear gravity-induced behavioural responses (gravitaxis and gravikinesis). The cytoplasm seems to act as a "statolith" stimulating mechanosensitive ion channels in the cell membrane. In order to test this hypothesis, electrophysiological studies with Stylonychia mytilus were performed, revealing the proposed changes (de- or hyperpolarization) depending on the cell's spatial orientation. The behaviour of Paramecium and Stylonychia was also analyzed during variable acceleration conditions of parabolic flights (5th German Parabolic Flight Campaign, 2003). The corresponding data confirm the relaxation of the graviresponses in microgravity as well as the existence of thresholds of graviresponses, which are found to be in the range of 0.4xg (gravikinesis) and 0.6xg (gravitaxis).     

DNA structures and radiation injury.

In the present paper experimental results from radiobiological investigations of the sedimentation behaviour of damaged and restored DNA-subunits attached to the nuclear membrane have been summarized. The studies were carried out preferably with Chinese Hamster cells V79-4 irradiated with different kinds of radiation (gamma-rays, neutrons and carbon ions) using the nucleoid sedimentation technique. Single-strand breaks relax the supercoiled DNA in the subunits resulting in a decreased sedimentation velocity. Rejoining leads to a correct restoration of the structure as can be studied by means of postincubation irradiation. Double-strand breaks release DNA fragments, again leading to an increased sedimentation velocity. If the average number of the induced double-strand breaks per subunit increases to a number higher than one, the measured results suggest that the structures should not be restored completely. The results are compatible with a new repair model developed in our laboratory on the assumption that, firstly, the single DNA subunits are the sensitive target rather than the whole DNA and, secondly, the repair of DNA damage takes place independently in each subunit.