A Low Albedo, Thin, Resistant Unit in Oxia Planum, Mars: Evidence for an Airfall Deposit and Late-Stage Groundwater Activity at the ExoMars Rover Landing Site [0.03%]
火星奥克西亚平原低反照率、薄而抗风化的地层单元：ExoMars rover着陆区空气降落沉积和晚期地下水活动的证据
E Harris,J M Davis,P M Grindrod et al.
E Harris et al.
Oxia Planum, Mars, is the future landing site of the ExoMars Rosalind Franklin rover mission, which will search for preserved biosignatures in a phyllosilicate-bearing unit. Overlying the mission-important phyllosilicate-bearing rocks is a ...
Investigating the Role of Amazonian Mesoscale Wind Patterns and Strength on the Spatial Distribution of Martian Bedrock Exposures [0.03%]
探究亚马逊平原中尺度风格局及其强度对火星露头岩石空间分布的作用
C E Gary-Bicas,T I Michaels,A D Rogers et al.
C E Gary-Bicas et al.
The Martian highlands contain Noachian-aged areally-extensive (>225 km2) bedrock exposures that have been mapped using thermal and visible imaging datasets. Given their age, crater density and impact gardening should have led to the formati...
Episodic Plate Tectonics on Europa: Evidence for Widespread Patches of Mobile-Lid Behavior in the Antijovian Hemisphere [0.03%]
欧罗巴反 jovian 半球移动地幔板块构造的证据
Geoffrey C Collins,G Wesley Patterson,Charlene E Detelich et al.
Geoffrey C Collins et al.
A nearly pole-to-pole survey near 140°E longitude on Europa revealed many areas that exhibit past lateral surface motions, and these areas were examined to determine whether the motions can be described by systems of rigid plates moving ac...
A Reevaluation of Cryolava Flow Evolution: Assumptions, Physical Properties, and Conceptualization [0.03%]
cryolava流演化再评估：假设、物理性质和概念模型
Aaron A Morrison,Alan G Whittington,Karl L Mitchell
Aaron A Morrison
Cryovolcanism has been invoked to explain numerous features observed on icy bodies. Many of these features show similar morphologies to volcanic features observed on Earth suggesting similar physics involved in their formation. Cryovolcanis...
The Curiosity Rover's Exploration of Glen Torridon, Gale Crater, Mars: An Overview of the Campaign and Scientific Results [0.03%]
火星盖尔陨石坑 Glen Torridon区域的祝融号探测 rover探索概览与科学成果总结
Kristen A Bennett,Valerie K Fox,Alex Bryk et al.
Kristen A Bennett et al.
The Mars Science Laboratory rover, Curiosity, explored the clay mineral-bearing Glen Torridon region for 1 Martian year between January 2019 and January 2021, including a short campaign onto the Greenheugh pediment. The Glen Torridon campai...
Compositions and Interior Structures of the Large Moons of Uranus and Implications for Future Spacecraft Observations [0.03%]
天王星大型卫星的组成及内部结构和对未来航天器观测的启示
Julie Castillo-Rogez,Benjamin Weiss,Chloe Beddingfield et al.
Julie Castillo-Rogez et al.
The five large moons of Uranus are important targets for future spacecraft missions. To motivate and inform the exploration of these moons, we model their internal evolution, present-day physical structures, and geochemical and geophysical ...
Mars 2020 Perseverance Rover Studies of the Martian Atmosphere Over Jezero From Pressure Measurements [0.03%]
火星2020年毅力号探测器的杰泽罗陨石坑地区大气压力测量研究
A Sánchez-Lavega,T Del Rio-Gaztelurrutia,R Hueso et al.
A Sánchez-Lavega et al.
The pressure sensors on Mars rover Perseverance measure the pressure field in the Jezero crater on regular hourly basis starting in sol 15 after landing. The present study extends up to sol 460 encompassing the range of solar longitudes fro...
Lifting and Transport of Martian Dust by the Ingenuity Helicopter Rotor Downwash as Observed by High-Speed Imaging From the Perseverance Rover [0.03%]
毅力号探测车高速成像观测到的机智号直升机旋翼下洗流引起的火星扬沙现象
M T Lemmon,R D Lorenz,J Rabinovitch et al.
M T Lemmon et al.
Martian atmospheric dust is a major driver of weather, with feedback between atmospheric dust distribution, circulation changes from radiative heating and cooling driven by this dust, and winds that mobilize surface dust and distribute it i...
A Positive Feedback Between Crustal Thickness and Melt Extraction for the Origin of the Martian Dichotomy [0.03%]
关于火星二元论地壳厚度与熔岩提取之间的正向反馈机制的起源
Valentin Bonnet Gibet,Chloé Michaut,Mark Wieczorek et al.
Valentin Bonnet Gibet et al.
A North/South difference in crustal thickness is likely at the origin of the Martian dichotomy in topography. Recent crustal thickness maps were obtained by inversion of topography and gravity data seismically anchored at the InSight statio...
Winds at the Mars 2020 Landing Site. 2. Wind Variability and Turbulence [0.03%]
火星2020着陆点的风。第二部分：风的变化和湍流
D Viúdez-Moreiras,M de la Torre,J Gómez-Elvira et al.
D Viúdez-Moreiras et al.
Wind speeds measured by the Mars 2020 Perseverance rover in Jezero crater were fitted as a Weibull distribution. InSight wind data acquired in Elysium Planitia were also used to contextualize observations. Jezero winds were found to be much...