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Halo orbits around \(L_{1}\), \(L_{2}\), and \(L_{3}\) in the photogravitational Sun–Mars elliptical restricted three-body problem
In the framework of Elliptical Restricted Three-Body Problem (ERTBP), we consider the equations of motion of an infinitesimal body in dimensionless...
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New Results of Radiation Study on Board TGO ExoMars in 2018–2023
Abstract —The article provides a brief description of the Liulin-MO dosimeter, which is part of the FREND (Fine Resolution Epithermal Neutron...
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Optimal geometry for lunar swing-by maneuvers aided by solar sails in the restricted four-body problem
As the geometry of the swing-by maneuver greatly influences the outcome of the gain of energy and a possible escape trajectory, a study on the...
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Dusty Plasma in the Solar System: Celestial Bodies without Atmosphere
AbstractWe present a brief review of research on dusty plasma in the solar system. Special attention is paid to theoretical studies related to the...
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Introduction
The atmosphere of Mars consists major gases 95% CO2, 2.8% N2, and 1.6% Ar. It has also trace gases like O, CO, H2O, CH4 and other gases along with a...
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Earth=Venus, part II: future Earth?
A review of the Earth’s history; ancient climate records; continents and climate, little ice ages; migrating habitable zones and...
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Manifestations of Anomalous Dissipation in Dusty Plasma in the Solar System: Atmosphereless Cosmic Bodies
Abstract —One of the main features that distinguishes dusty plasma from ordinary (not containing charged dust particles) plasma is anomalous...
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Low-cost Mars transfer from the Earth using solar sails and lunar swing-bys
As the current phase of space exploration is marked by a rapidly growing number of rocket launches and space missions, techniques that would enable...
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Physics of the Solar System Bodies
In this section we briefly bring the most essential results of the exploration of the bodies of the solar system. The sun itself is treated...
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Introducing the Inner Planets
There is a definite divide between the inner and outer Solar System. The four inner planets, Mercury, Venus, Earth, and Mars, are all packed in close...
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Two-Body Problem and the Solar System
The two-body problem is an important application, which is tackled in this chapter using Lagrange’s equations with particular emphasis on the case of...
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Middle Ionosphere of Mars
The middle ionosphere of Mars is formed mainly due to ablation of meteors and charge exchange of metallic ions between altitudes 60 and 110 km...
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The ExoMars Schiaparelli Entry, Descent and Landing Demonstrator Module (EDM) System Design
The Entry, Descent and Landing Demonstrator Module (EDM) named Schiaparelli, was the ESA-led Mars lander element of the ESA-Roscosmos ExoMars 2016...
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Study of Small Bodies of the Solar System: Odyssey-Asteroids Project
AbstractThe paper discusses priority scientific tasks related to the study of small bodies in the Solar System, identifies the most promising objects...
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Orbital Dynamics
The concept of an orbit is fundamental to the way that any object, whether artificial or natural, moves through space. Everyone knows that a...
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Getting To Know The Sun
Since time immemorial, people have stared in wonder at the sky. In addition to the familiar, twinkling stars, observers noted seven objects that...