SearcharxivSearch

arXiv · 2507.08251

Non-Propulsive Payload Deployment for Efficient On-Orbit Servicing of Mega-Constellations

Abstract

The prevailing assumption holds that on-orbit servicing (OOS) of mega-constellations is infeasible due to prohibitive fuel consumption incurred by multiple rendezvous maneuvers across vast and dispersed satellite populations. To address this challenge, a novel OOS architecture termed Non-Propulsive Payload Deployment (NPD) is proposed in this paper. Within this framework, a service spacecraft (SSc) ejects micro-payload spacecraft (PSc) into transfer orbits, after which the PSc autonomously rendezvous with target spacecraft (TSc). Since propulsion is required only for the minimal mass of the PSc, maneuvering fuel consumption is significantly reduced. This paper develops a phase-based approximation algorithm to resolve the scheduling problems arising from cumulative recoil-induced orbital perturbations. Numerical simulations for a constellation of over 100 satellites demonstrate that this algorithm reduces computation time by over 90% while maintaining ejection velocity errors below 1%. Further analysis yields an analytical formula for evaluating the deployment capability of the NPD system, providing planning estimates with less than 2% error within low Earth orbit (LEO) regimes. Finally, a case study of the Starlink Gen2 constellation confirms that the NPD system consumes less than 1/50 of the propellant required by conventional methods, enabling efficient multi-plane servicing via J2 perturbation.

Explore related subjects

Keep this discovery

BibTeXRIS

Li Zhengrui, Feng Guanhua, Wu Xiaokun, Li Wenhao, Yue Yuxian. 2025-07-11. Non-Propulsive Payload Deployment for Efficient On-Orbit Servicing of Mega-Constellations. https://arxiv.org/abs/2507.08251

Cite the original work for its findings. Save a collection to share your selection of sources.

KEEP EXPLORING

Related papers

Projection Angles of Projectiles in Sports: Qualitative Assessment of the Effects of Aerodynamic Forces or Run-Up

We examine two major factors that influence the optimum projection angle: aerodynamic forces and the effect of run-up. With respect to aerodynamics, we consider not only the drag but also the lift generated by spin during flight. By linearizing the equations of motion that include these forces, we derive perturbation solutions with respect to drag and lift coefficients and clarify their qualitative effects. The results show that both drag and lift reduce the optimum projection angle, with the latter exerting a stronger influence. To investigate the effect of run-up, we use an extended projection model in which the initial speed depends on the initial angle. Analysis of this model reveals that a stronger run-up increases the relative projection angle but decreases the launch angle observed from the ground. These findings provide a mechanical explanation for the release angle in shot put and the takeoff angle in long jump. The present study establishes a simple theoretical framework for clarifying the respective roles of aerodynamic and run-up effects in determining the optimum projection angles in sports.

physics.class-ph

Dunkl-Based Modeling of Vibrational Modes in Lightweight Elastic Beams

Optimizing slender elastic structures for renewable energy applications requires non-classical continuum formulations capable of accounting for spatial micro-interactions without sacrificing analytical tractability. Here, we extend beam vibration mechanics by replacing standard spatial derivatives with the Dunkl differential operator. This modification introduces a reflection-coupled mathematical structure that accounts for spatial parity effects across the beam domain. We formulate the governing dynamic equations into a generalized eigenvalue problem and derive exact analytical expressions for modal characteristics under standard boundary conditions. The classical limit confirms exact convergence to classical Euler-Bernoulli formulations. Parametric analyses reveal that the Dunkl parameter acts as a reflection-induced modulation parameter, significantly shifting natural frequencies and altering the modal characteristics of higher modes. These results provide an analytical baseline for dynamic optimization in lightweight structural components.

physics.class-ph

A purely mechanical system realizing a Coulomb-like interaction

We solve in closed form a one-dimensional relativistic system: two masses interacting only through elastic collisions with a massless mediator bouncing between them. Momenta, times, and positions are hyperbolic functions of the collision index. The mediator energy, interpreted as the pair's effective potential, obeys an exact discrete Coulomb law, $V\propto 1/r$, with a Lorentz-invariant action as coupling. A massive Newtonian mediator instead transmits a $1/r^{3}$ force; one adiabatic invariant traces both laws to the mediator's dispersion relation. Continued to negative mediator energy, the closed forms turn trigonometric, binding a one-dimensional mechanical analog of the Coulomb atom.

physics.class-ph