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Phoenix - The First Mars Scout Mission

机译:凤凰号-第一个火星侦察任务

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As the first of the new Mars Scouts missions, the Phoenix project was selected by NASA in August of 2003. Four years later, almost to the day, Phoenix was launched from Cape Canaveral Air Station and successfully injected into an interplanetary trajectory on its way to Mars. On May 25, 2008 Phoenix conducted the first successful powered decent on Mars in over 30 years. This paper will highlight some of the key changes since the 2008 IEEE paper of the same name, as well as performance through cruise, landing at the north pole of Mars and some of the preliminary results of the surface mission.Phoenix "Follows the water" responding directly to the recently published data from Dr. William Boynton, PI (and Phoenix co-I) of the Mars Odyssey Gamma Ray Spectrometer (GRS). GRS data indicate extremely large quantities of water ice (up to 50% by mass) within the upper 50 cm of the northern polar regolith. Phoenix will land within the north polar region at 68.3°N, 124.6°W identified by GRS to harbor near surface water ice and provide in-situ confirmation of this extraordinary find. Our mission has investigated water in all its phases, as well as the history of water as evidenced in the soil and atmospheric characteristics. Access to the critical subsurface region which contains this information was made possible by a third generation robotic arm capable of excavating the expected Martian regolith to a depth of 1m.Phoenix had four primary science objectives:1) Determine the polar climate and weather, interaction with the surface, and composition of the lower atmosphere around 70° N for at least 90 sols focusing on water, ice, dust, noble gases, and CO2. Determine the atmospheric characteristics during descent through the atmosphere.2) Characterize the geomorphology and active processes shaping the northern plains and the physical properties of the near surface regolith focusing on the role of water.3) Determine the aqueous mineralogy and chemistry as well as the adsorbed gases and organic content of the regolith. Verify the Odyssey discovery of near-surface ice.4) Characterize the history of water, ice, and the polar climate. Determine the past and present biological potential of the surface and subsurface environments.
机译:作为新的火星侦察兵任务的第一个任务,凤凰号项目于2003年8月被美国国家航空航天局选中。四年后,直到今天,凤凰号从卡纳维拉尔角航空站发射升空,并成功地进入了星际轨道火星。 2008年5月25日,凤凰城(Phoenix)在火星上进行了30年来首次成功的动力式体面测试。本文将重点介绍自2008年IEEE同名论文以来的一些重要变化,以及巡航,在火星北极降落时的性能以及水面飞行任务的一些初步结果。 凤凰号“跟随水流”直接回应了火星奥德赛伽玛射线光谱仪(GRS)的威廉·博伊顿博士(PI)和菲尼克斯公司的最新数据。 GRS数据表明,在北极碎石岩的上部50 cm内有极大量的水冰(质量百分比最高为50%)。凤凰号将在GRS确定的北纬68.3°,北纬124.6°的区域内着陆,以藏在地表水冰附近,并就这一非凡的发现提供就地证实。我们的任务是调查所有阶段的水以及土壤和大气特征所证明的水历史。第三代机器人手臂能够将包含预期信息的火星重石发掘至1m的深度,从而可以访问包含该信息的关键地下区域。 凤凰城有四个主要的科学目标: 1)确定至少90种溶胶,水,冰,灰尘,稀有气体和CO2的极性气候和天气,与地表的相互作用以及70°N附近的低层大气的成分。确定在通过大气下降过程中的大气特征。 2)表征北部平原的地貌和活跃过程以及集中在水作用下的近地表砾石的物理特性。 3)确定含水矿物学和化学性质,以及重矿物的吸附气体和有机物含量。验证奥德赛发现的近地表冰块。 4)描述水,冰和极地气候的历史。确定地表和地下环境的过去和现在的生物潜力。

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