Henrik Hargitai – författare

This encyclopedia provides a snapshot of our current geological knowledge on solid-surface Solar System bodies. Each entry contains information about the features’ morphology, its interpretation, proposed formation models, distribution and occurrence, planetary or terrestrial analogs, and research history. The entries are fully referenced. All image captions include original image IDs. More than 600 named planetary feature types are discussed in the encyclopedia, covering a wide range of scales--from micrometers to global scale--and also include landform types (structural or topographic features), parts of landforms, terrain types or surface textures, surface patterns, and features identified at wavelengths extending from visible to radio waves (e.g., albedo, thermal infrared, and radar features). The book covers features formed by impact, aeolian, magmatic, volcanic, tectonic, fluvial, lacustrine, marine and coastal, mass movement, sedimentary, desiccation, liquefaction, periglacial, glacial, nival, sublimation, collapse, weathering, and selective erosion or other, including complex processes.Depending on the information and formation models available, the entries have different approaches. Some of them discuss their subject from the point of view of the inferred process or origin, others are morphology or description-based. As a default, entries focus on extraterrestrial landforms, while also mentioning their proposed terrestrial analogs. Most planetary landforms are not body-specific, but some have no known terrestrial counterparts. Named historic (obsolete) landform types are also included to provide reference for previous key research papers. To make it easier to find features with related origins, the encyclopedia contains entries that list landforms based on their formative processes. It also lists body-specific features on Mercury (5 feature types), Venus (40), the Earth (13), the Moon (15), Mars (87), Io (7), Europa (17), Callisto (7), Titan (9), Triton (2), mid-sized satellites (8), and small bodies (3). Also included are entries on the 51 planetary feature descriptor terms approved by IAU.

This encyclopedia provides a snapshot of our current geological knowledge on solid-surface Solar System bodies. Each entry contains information about the features’ morphology, its interpretation, proposed formation models, distribution and occurrence, planetary or terrestrial analogs, and research history. The entries are fully referenced. All image captions include original image IDs. More than 600 named planetary feature types are discussed in the encyclopedia, covering a wide range of scales--from micrometers to global scale--and also include landform types (structural or topographic features), parts of landforms, terrain types or surface textures, surface patterns, and features identified at wavelengths extending from visible to radio waves (e.g., albedo, thermal infrared, and radar features). The book covers features formed by impact, aeolian, magmatic, volcanic, tectonic, fluvial, lacustrine, marine and coastal, mass movement, sedimentary, desiccation, liquefaction, periglacial, glacial, nival, sublimation, collapse, weathering, and selective erosion or other, including complex processes.Depending on the information and formation models available, the entries have different approaches. Some of them discuss their subject from the point of view of the inferred process or origin, others are morphology or description-based. As a default, entries focus on extraterrestrial landforms, while also mentioning their proposed terrestrial analogs. Most planetary landforms are not body-specific, but some have no known terrestrial counterparts. Named historic (obsolete) landform types are also included to provide reference for previous key research papers. To make it easier to find features with related origins, the encyclopedia contains entries that list landforms based on their formative processes. It also lists body-specific features on Mercury (5 feature types), Venus (40), the Earth (13), the Moon (15), Mars (87), Io (7), Europa (17), Callisto (7), Titan (9), Triton (2), mid-sized satellites (8), and small bodies (3). Also included are entries on the 51 planetary feature descriptor terms approved by IAU.

This revised and updated second edition provides a complete snapshot of our current knowledge on the geological features on solid-surface Solar System bodies. They extend over a wide range of scales, from micrometers to global scales, and include landform types (structural or topographic features), parts of landforms, terrain types and surface textures, surface patterns, and features identified at wavelengths extending from visible to radio waves, including albedo features, thermal infrared features, and radar features. The extensive new content addresses findings from the Messenger, Cassini, New Horizons, Curiosity and Maven missions and provides information on at least ten new landform types, as well as articles on exoplanet landforms. Refinements in methods and formations theories are also covered. Today scientists have a huge set of images and other physical data which makes it possible to create models on the inner structure and thermal history of planetary bodies. Combined data sets lead to better supported models on the formation of surface features. These models give reliable explanations for the origin of planetary landforms. New, higher resolution images reveal new sets of meso- and microscale landforms, while images from previously not imaged dwarf planets, satellites, asteroids and cometary nuclei show landforms never seen before. In the future exoplanets are expected to continue to provide brand new types of relief features not predictable by our Earth-and Solar System bound imagination.There are so many different landforms on planetary surfaces that it is nearly impossible for anybody to overview all of them who does not work exactly with that certain feature type. The Encyclopedia helps with presenting the landforms in searchable, alphabetical order. The book contains more than a simple list of various features: it provides context and connections between them and point to their origin. For example sand dunes were found on Venus, Mars and Titan, fluvial valleys and shorelines are present on Mars and Titan, impact craters have many different types - all are presented and explained here. Beyond the texts, references, schematic figures, images and planetary maps accompany the description of landforms, providing a wide background for detailed analyses even for geomorphologists working in planetary science. This book helps the reader discover the great variety of planetary landforms. Its continual updating makes it the go-to reference in the field.

This book approaches geological, geomorphological and topographical mapping from the point in the workflow at which science-ready datasets are available. Though there have been many individual projects on dynamic maps and online GISs, in which coding and data processing are given precedence over cartographic principles, cartography is more than “just” processing and displaying spatial data. However, there are currently no textbooks on this rapidly changing field, and methods tend to be shared informally.  Addressing this gap in the literature, the respective chapters outline many topics pertaining to cartography and mapping such as the role and definition of planetary cartography and (vs?) Geographic Information Science; theoretical background and practical methodologies in geological mapping; science-ready versus public-ready products; a goal/procedure-focused practical manual of the most commonly used software in planetary mapping, which includes generic (ArcGISand its extensions, JMARS) and specific tools (HiView, Cratertools etc.); extracting topographic information from images; thematic mapping: climate; geophysics; surface modeling; change detection; landing site selection; shared maps; dynamic maps on the web; planetary GIS interfaces; crowdsourcing; crater counting techniques; irregular bodies; geological unit symbology; mapping center activities; and web services.All chapters were prepared by authors who have actually produced geological maps or GISs for NASA / the USGS, DLR, ESA or MIIGAIK. Taken together, they offer an excellent resource for all planetary scientists whose research depends on mapping, and for students of astrogeology.