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The main benefit of an interstellar mission is to carry out in-situ measurements within a target star system. To allow for extended in-situ measurements, the spacecraft needs to be decelerated. One of the currently most promising…

Space Physics · Physics 2016-08-24 Nikolaos Perakis , Andreas M. Hein

The fission thrust sail as booster for nuclear fusion-based rocket propulsion for future starships is studied. Some required aspects of these systems such as neutron moderation and sail regeneration are discussed. First order calculations…

Instrumentation and Detectors · Physics 2014-08-28 Frederik Ceyssens , Kristof Wouters , Maarten Driesen

Observations suggest that the large-scale convective velocities obtained by solar convection simulations might be over-estimated (convective conundrum). One plausible solution to this could be the small-scale dynamo which cannot be fully…

Solar and Stellar Astrophysics · Physics 2018-05-01 Bidya Binay Karak , Mark Miesch , Yuto Bekki

Background: A solar sail presents a large sheet of low areal density membrane and is the most elegant propellant-less propulsion system for the future exploration of the Solar System and beyond. By today the study on sail membrane…

Popular Physics · Physics 2022-03-01 Vladimir Ya. Kezerashvili , Roman Ya. Kezerashvili

Propellantless propulsion refers to methods of space travel that do not require onboard propellant, instead relying on natural forces or external energy sources. In this paper, I review different approaches that have been explored and…

Popular Physics · Physics 2026-01-21 Roman Ya. Kezerashvili

Kinetic exospheric models revealed that the solar wind is accelerated by an ambipolar electric field up to supersonic velocities. The presence of suprathermal Strahl electrons at the exobase can further increase the velocity to higher…

Solar and Stellar Astrophysics · Physics 2024-01-25 Viviane Pierrard , Maximilien Peters de Bonhome

The electric solar wind sail is a novel propellantless space propulsion concept. According to numerical estimates, the electric solar wind sail can produce a large total impulse per propulsion system mass. Here we consider using a 0.5 N…

Instrumentation and Methods for Astrophysics · Physics 2014-08-28 Pekka Janhunen , Jean-Pierre Lebreton , Sini Merikallio , Mark Paton , Giovanni Mengali , Alessandro A. Quarta

The electric solar wind sail (E-sail) is a novel, efficient propellantless propulsion concept which utilises the natural solar wind for spacecraft propulsion with the help of long centrifugally stretched charged tethers. The E-sail requires…

Instrumentation and Methods for Astrophysics · Physics 2013-01-11 P. Janhunen

The current preferred envisioned method for transmitting power to a space elevator climber is a laser/photovoltaic (PV) system. In this, a ground-based laser beam would transmit megawatts of optical power through the atmosphere to an…

Popular Physics · Physics 2018-02-22 Mark A. Wessels

Theoretical aspects of a solar sail material degradation are presented when the solar electromagnetic and corpuscular forms of radiation were considered as sources of degradation. The analysis of the interaction of two components of solar…

Space Physics · Physics 2024-10-29 Roman Ya. Kezerashvili

A solar sail is one of the most promising space exploration system because of its theoretically infinite specific impulse using solar radiation pressure (SRP). Recently, some researchers proposed "transformable spacecrafts" that can…

Machine Learning · Computer Science 2024-12-19 Yuki Kubo , Toshihiro Chujo

Achieving relativistic flight to enable extrasolar exploration is one of the dreams of humanity and the long term goal of our NASA Starlight program. We derive a fully relativistic solution for the motion of a spacecraft propelled by…

Instrumentation and Methods for Astrophysics · Physics 2018-04-04 Neeraj Kulkarni , Philip Lubin , Qicheng Zhang

The transverse radiation pressure force and acceleration is compared for two parametrically optimized designs: prismatic and two-pillar metasurface gratings. The numerical results were cross-verified with both Maxwell stress tensor and…

Optics · Physics 2023-06-27 Prateek R. Srivastava , Ryan M. Crum , Grover A. Swartzlander

Several lines of evidence suggest that the velocity amplitude in global simulations of solar convection, U, may be systematically over-estimated. Motivated by these recent results, we explore the factors that determine U and we consider how…

Solar and Stellar Astrophysics · Physics 2016-09-21 Bridget O'Mara , Mark S. Miesch , Nicholas A. Featherstone , K. C. Augustson

The radiation pressure exerted by incoherent light on diverse surfaces is examined. The thermodynamic rule, first given by Carnot in 1824, describes the limitation to the amount of free energy that can be obtained from a source of thermal…

Space Physics · Physics 2016-09-08 Thomas Gold

In the solar convection zone, rotation couples with intensely turbulent convection to drive a strong differential rotation and achieve complex magnetic dynamo action. Our sun must have rotated more rapidly in its past, as is suggested by…

The use of ultrathin solid foils offers optimal conditions for accelerating protons from laser-matter interactions. When the target is thin enough that relativistic self-induced transparency (RSIT) sets in, all of the target electrons get…

Plasma Physics · Physics 2020-10-07 Julien Ferri , Evangelos Siminos , Laurent Gremillet , Tünde Fülöp

The Solar System Odyssey mission uses modern-day high-precision experimental techniques to test the laws of fundamental physics which determine dynamics in the solar system. It could lead to major discoveries by using demonstrated…

Asteroids, planets, stars in some open clusters, as well as molecular clouds appear to possess a preferential spin-orbit alignment, pointing to shared processes that tie their rotation at birth to larger parent structures. We present a new…

Earth and Planetary Astrophysics · Physics 2022-08-03 Rico G. Visser , Marc G. Brouwers

In the corona, plasma is accelerated to hundreds of kilometers per second, and heated to temperatures hundreds of times hotter than the Sun's surface, before it escapes to form the solar wind. Decades of space-based experiments have shown…