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Moon Impact Crater Detection Using Nested Attention Mechanism Based UNet++

open access: yesIEEE Access, 2021
Impact craters are the most prominent topographic feature on the lunar surface, which will play a significant role in constructing lunar bases and lunar surface activities in the future.
Yutong Jia, Lei Liu, Chenyang Zhang
doaj   +1 more source

Microbial Life in Impact Craters [PDF]

open access: yesCurrent Issues in Molecular Biology, 2020
Asteroid and comet impacts are known to have caused profound disruption to multicellular life, yet their influence on habitats for microorganisms, which comprise the majority of Earth's biomass, is less well understood. Of particular interest are geological changes in the target lithology at and near the point of impact that can persist for billions of
Cockell, Charles S.   +4 more
openaire   +3 more sources

Morphometric Analysis of Pluto’s Impact Craters

open access: yesRemote Sensing, 2021
The scope of this work is to carry out a morphometric analysis of Pluto’s impact craters. A global Pluto digital elevation model (DEM) with a resolution of 300 m/px, created from stereoscopic pairs obtained by the New Horizons Mission, was used to ...
Caio Vidaurre Nassif Villaça   +2 more
doaj   +1 more source

Morphological Features-Based Descriptive Index System for Lunar Impact Craters

open access: yesISPRS International Journal of Geo-Information, 2017
Lunar impact craters are important for studying lunar surface morphology because they are the most typical morphological units of the Moon. Impact crater descriptive indices can be used to describe morphological features and thus provide direct evidence ...
Min Chen   +5 more
doaj   +1 more source

Polygonal impact craters on Ganymede

open access: yesMeteoritics & Planetary Science, 2023
AbstractPolygonal impact craters (PICs) are unique geological features observed on various planetary bodies and constitute a small percentage of the impact crater population. This study focuses on PICs on Ganymede, where no such craters have been investigated so far. Here we present the distribution of PICs, examine their morphological characteristics,
Namitha Rose Baby   +3 more
openaire   +6 more sources

A BAYESIAN NETWORK FRAMEWORK FOR AUTOMATIC DETECTION OF LUNAR IMPACT CRATERS BASED ON OPTICAL IMAGES AND DEM DATA [PDF]

open access: yesThe International Archives of the Photogrammetry, Remote Sensing and Spatial Information Sciences, 2017
Impact craters are among the most noticeable geo-morphological features on the planetary surface and yield significant information on terrain evolution and the history of the solar system.
J. Yang, Z. Kang
doaj   +1 more source

A Machine Learning Approach to Crater Classification from Topographic Data

open access: yesRemote Sensing, 2019
Craters contain important information on geological history and have been widely used for dating absolute age and reconstructing impact history. The impact process results in a lot of ejected fragments and these fragments may form secondary craters ...
Qiangyi Liu   +4 more
doaj   +1 more source

Holocene impact craters on Earth

open access: yesMiscellanea Geographica: Regional Studies on Development, 2023
Impact craters are formed by collisions of cosmic bodies moving with hypervelocity. The formation of these features is not restricted to the distant geological past; new structures are constantly being created and at least 13 confirmed impact craters and
Losiak Anna
doaj   +1 more source

Lunar Evolution Analysis Based on Numerical Simulations of Typical Lunar Impact Craters

open access: yesSpace: Science & Technology, 2023
Impact craters are one of the most important landforms on the lunar surface, playing a crucial role in the formation and later evolution of the Moon. For example, as a primary source of remote sensing observations and lunar samples, lunar regolith is ...
Zongyu Yue   +4 more
doaj   +1 more source

Impact cratering and the Oort Cloud [PDF]

open access: yesMonthly Notices of the Royal Astronomical Society, 2008
We calculate the expected flux profile of comets into the planetary system from the Oort cloud arising from Galactic tides and encounters with molecular clouds. We find that both periodic and sporadic bombardment episodes, with amplitudes an order of magnitude above background, occur on characteristic timescales ~25-35 Myr.
Wickramasinghe, J. T., Napier, W. M.
openaire   +2 more sources

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