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Etat : New. 423 pp., hardcover, new. - If you are reading this, this item is actually (physically) in our stock and ready for shipment once ordered. We are not bookjackers. Buyer is responsible for any additional duties, taxes, or fees required by recipient's country.

Hardcover. Etat : new. Hardcover. Studying the evolution of the surfaces and atmospheres of planetary bodies in the solar system is fundamental to our understanding of the present state of the solar system. Exospheres are the interfaces between the planetary body and the open space, so that, studying the exospheric filling and loss processes is the way to expand knowledge of the bodys evolution. Surface and atmospheric changes are caused predominantly by the continuous bombardment of the bodies by photons, energetic ions, and micrometeoroids. Eventually, the ongoing processes are functions of the space environment, in other words, the planets are subjected to space weather.This book focuses on the large subset of planetary objects (planets, moons, and small bodies) that are not protected by either strong magnetic fields or thick atmospheres in the inner solar system where the solar influence is stronger. The main exponents class regarding this class of objects are Mercury and the Moon. In these cases, the exosphere is directly connected to the surface, thus, it is called a surface-bounded exosphere. This is due to the surface release processes that are also the exospheric filling ones, where atoms and molecules collide with the surface far more frequently than collisions with each other.During the last decade, several space missions provided important new findings for many airless bodies. Furthermore, new ground-based imaging techniques offered the possibility of improved exosphere observations. In the next decade, the ESA-JAXA BepiColombo mission will explore Mercury utilizing two spacecraft. And on a global scale, almost all space agencies will foresee orbiters and landers to the Moon as part of their space programs.This collection of articles summarizes the current state of knowledge on surface-bounded exospheres, as a support for the interpretation of data that will be received from the forthcoming missions, for the next-generation of scientists that will be involved in the exploration of Mercury, the Moon and other airless bodies, including exoplanets. Reprinted from the Space Science Reviews Topical Collection Surface-Bounded Exospheres and Interactions in the Inner Solar System This book is the printed edition of the Space Science Reviews Topical Collection Surface-Bounded Exospheres and Interactions in the Inner Solar System.Studying the evolution of the surfaces and atmospheres of planetary bodies in the solar system is fundamental to our understanding of the present state of the solar system. Shipping may be from multiple locations in the US or from the UK, depending on stock availability. …

Buch. Etat : Neu. Neuware -Studying the evolution of the surfaces and atmospheres of planetary bodies in the solar system is fundamental to our understanding of the present state of the solar system. Exospheres are the interfaces between the planetary body and the open space, so that, studying the exospheric filling and loss processes is the way to expand knowledge of the body's evolution. Surface and atmospheric changes are caused predominantly by the continuous bombardment of the bodies by photons, energetic ions, and micrometeoroids. Eventually, the ongoing processes are functions of the space environment, in other words, the planets are subjected to space weather.This book focuses on the large subset of planetary objects (planets, moons, and small bodies) that are not protected by either strong magnetic fields or thick atmospheres in the inner solar system where the solar influence is stronger. The main exponents class regarding this class of objects are Mercury and the Moon. In these cases, the exosphere is directly connected to the surface, thus, it is called a surface-bounded exosphere. This is due to the surface release processes that are also the exospheric filling ones, where atoms and molecules collide with the surface far more frequently than collisions with each other.Duringthe last decade, several space missions provided important new findings for many airless bodies. Furthermore, new ground-based imaging techniques offered thepossibility of improved exosphere observations. In the next decade, the ESA-JAXA BepiColombo missionwillexplore Mercury utilizing two spacecraft. And on a global scale, almost all space agencies willforeseeorbiters and landers to the Moon as part of their spaceprograms.This collection of articles summarizes the current state of knowledge on surface-bounded exospheres, as a support for the interpretationof datathat will be received from the forthcomingmissions, for the next-generation of scientists that will be involved in the exploration of Mercury, the Moon and other airless bodies, including exoplanets.Reprinted from theSpace Science Reviews Topical Collection Surface-Bounded Exospheres and Interactions in the Inner Solar System 424 pp. Englisch.…

Buch. Etat : Neu. Neuware -Studying the evolution of the surfaces and atmospheres of planetary bodies in the solar system is fundamental to our understanding of the present state of the solar system. Exospheres are the interfaces between the planetary body and the open space, so that, studying the exospheric filling and loss processes is the way to expand knowledge of the body's evolution. Surface and atmospheric changes are caused predominantly by the continuous bombardment of the bodies by photons, energetic ions, and micrometeoroids. Eventually, the ongoing processes are functions of the space environment, in other words, the planets are subjected to space weather.This book focuses on the large subset of planetary objects (planets, moons, and small bodies) that are not protected by either strong magnetic fields or thick atmospheres in the inner solar system where the solar influence is stronger. The main exponents class regarding this class of objects are Mercury and the Moon. In these cases, the exosphere is directly connected to the surface, thus, it is called a surface-bounded exosphere. This is due to the surface release processes that are also the exospheric filling ones, where atoms and molecules collide with the surface far more frequently than collisions with each other.Duringthe last decade, several space missions provided important new findings for many airless bodies. Furthermore, new ground-based imaging techniques offered thepossibility of improved exosphere observations. In the next decade, the ESA-JAXA BepiColombo missionwillexplore Mercury utilizing two spacecraft. And on a global scale, almost all space agencies willforeseeorbiters and landers to the Moon as part of their spaceprograms.This collection of articles summarizes the current state of knowledge on surface-bounded exospheres, as a support for the interpretationof datathat will be received from the forthcomingmissions, for the next-generation of scientists that will be involved in the exploration of Mercury, the Moon and other airless bodies, including exoplanets.Reprinted from theSpace Science Reviews Topical Collection Surface-Bounded Exospheres and Interactions in the Inner Solar System 424 pp. Englisch.…

Buch. Etat : Neu. Neuware - Studying the evolution of the surfaces and atmospheres of planetary bodies in the solar system is fundamental to our understanding of the present state of the solar system. Exospheres are the interfaces between the planetary body and the open space, so that, studying the exospheric filling and loss processes is the way to expand knowledge of the body's evolution. Surface and atmospheric changes are caused predominantly by the continuous bombardment of the bodies by photons, energetic ions, and micrometeoroids. Eventually, the ongoing processes are functions of the space environment, in other words, the planets are subjected to space weather.This book focuses on the large subset of planetary objects (planets, moons, and small bodies) that are not protected by either strong magnetic fields or thick atmospheres in the inner solar system where the solar influence is stronger. The main exponents class regarding this class of objects are Mercury and the Moon. In these cases, the exosphere is directly connected to the surface, thus, it is called a surface-bounded exosphere. This is due to the surface release processes that are also the exospheric filling ones, where atoms and molecules collide with the surface far more frequently than collisions with each other.Duringthe last decade, several space missions provided important new findings for many airless bodies. Furthermore, new ground-based imaging techniques offered thepossibility of improved exosphere observations. In the next decade, the ESA-JAXA BepiColombo missionwillexplore Mercury utilizing two spacecraft. And on a global scale, almost all space agencies willforeseeorbiters and landers to the Moon as part of their spaceprograms.This collection of articles summarizes the current state of knowledge on surface-bounded exospheres, as a support for the interpretationof datathat will be received from the forthcomingmissions, for the next-generation of scientists that will be involved in the exploration of Mercury, the Moon and other airless bodies, including exoplanets.Reprinted from theSpace Science Reviews Topical Collection Surface-Bounded Exospheres and Interactions in the Inner Solar System.…

Hardcover. Etat : Brand New. 423 pages. 9.25x6.10x9.49 inches. In Stock.

Etat : New.

Buch. Etat : Neu. Surface-Bounded Exospheres and Interactions in the Inner Solar System | Anna Milillo (u. a.) | Buch | Space Sciences Series of ISSI | vi | Englisch | 2025 | Springer | EAN 9789402422917 | Verantwortliche Person für die EU: Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg, juergen[dot]hartmann[at]springer[dot]com | Anbieter: preigu. …

Etat : new. Questo è un articolo print on demand.

Buch. Etat : Neu. This item is printed on demand - Print on Demand Titel. Neuware -Studying the evolution of the surfaces and atmospheres of planetary bodies in the solar system is fundamental to our understanding of the present state of the solar system. Exospheres are the interfaces between the planetary body and the open space, so that, studying the exospheric filling and loss processes is the way to expand knowledge of the body's evolution. Surface and atmospheric changes are caused predominantly by the continuous bombardment of the bodies by photons, energetic ions, and micrometeoroids. Eventually, the ongoing processes are functions of the space environment, in other words, the planets are subjected to space weather.Springer Verlag GmbH, Tiergartenstr. 17, 69121 Heidelberg 424 pp. Englisch.…