Rapidly growing low-Earth-orbit (LEO) constellations increasingly operate in the spectrum shared with radio astronomy services (RAS), creating escalating interference risks for sensitive scientific observations. Existing mitigation mechanisms rely on reactive beam steering, or avoidance near observatories but fail to account for aggregate sidelobe emissions-leading to residual interference and substantial, unnecessary capacity loss. We present SkyShare, a constellation-wide sky-sharing system that enables predictive, interference-aware spot beam scheduling to protect radio astronomy while preserving network coverage. SkyShare integrates high-fidelity orbital prediction with International Telecommunication Union (ITU)-compliant Equivalent Power Flux Density (EPFD) modeling, and real-time observatory data via Operational Data Sharing (ODS) to jointly optimize beam-cell assignments over observation windows. To make constellation-scale coordination tractable, we introduce a concept of EPFD-budgeted Region-of-Interest(RoI) that bounds residual sidelobe interference while confining optimization to a minimal, provably sufficient set of cells. Building on RoI, we formulate LEO-RAS coexistence as a scalable scheduling problem and design SkySched, a flow-based algorithm that is optimal in special cases and yields scalable near-optimal solutions in the general NP-hard setting. SkyShare operates entirely in the control plane and requires no satellite hardware changes. Using real Starlink constellation geometries, we evaluate SkyShare across 25 single-dish, Ku-band RAS sites worldwide. Compared to Starlink boresight avoidance, SkyShare reduces unserved cells by up to 90.68% while remaining within EPFD limits.
Low-earth orbits (LEO) satellites have recently gained wide attention for their potential to provide high-data-rate services in desert, sea, and rural areas. Currently such systems operate in the Ku band on the down-link. However, inter-operator LEO satellites produce frequent In-Line-Events (ILE) creating co-channel i...
With the continued deployment of low Earth orbit (LEO) satellite constellations, spectrum resources are becoming more limited. As a result, satellite-to-ground links face many types of strongly coupled interference in complex electromagnetic environments. This interference includes non-intentional interference caused b...
Jiang-Bo Si, Haoqin Zhao, Zan Li et al.· IEEE Communications Surveys...· 0 citations
Ultra-low-frequency radio astronomy below 10 MHz remains the least explored region of the electromagnetic spectrum. Ground-based observations are fundamentally limited by ionospheric opacity, propagation effects and terrestrial radio-frequency interference. Space-based interferometry offers a pathway to overcome these...
J. Lazendic-Galloway, Maria Rita Eusébio Vale Lima, J. G. Bij de Vaate et al.· Astronomical Telescopes + In...· 0 citations
The rapid proliferation of large-scale Low Earth Orbit (LEO) mega-constellations has intensified co-frequency coexistence challenges, particularly collinear interference, where a victim user is simultaneously illuminated by the high-gain beams of serving and interfering satellites. High satellite mobility and milliseco...
Yi-Fei Chen, Qi-Huai Huang, Ke Wang et al.· 2026 IEEE/CIC International...· 0 citations
The rapid deployment of large-scale non-geostationary orbit (NGSO) constellations, such as Starlink, OneWeb, and Kuiper, is reshaping satellite communications by enabling worldwide low-latency connectivity. This expansion, however, raises coexistence challenges with legacy geostationary orbit (GSO) systems, particularl...
Luciana R. N. Ferreira, H. T. P. Da Silva, Hugerles S. Silva et al.· IEEE Access· 0 citations
Geodetic very long baseline interferometry (VLBI) is a vulnerable application of the radio astronomy service (RAS): it provides the fundamental link between the celestial and terrestrial reference frames, and is the only technique that uniquely determines UT1-UTC. The next-generation geodetic VLBI Global Observing Syst...
Balthasar Indermuehle, Lucia McCallum, E. van der Wateren et al.· 0 citations
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