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SILVIA: Ultra-precision formation flying demonstration for space-based interferometry

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arxiv 2504.05001 v2 pith:IT3G352X submitted 2025-04-07 astro-ph.IM cs.SYeess.SYgr-qcphysics.ins-det

SILVIA: Ultra-precision formation flying demonstration for space-based interferometry

classification astro-ph.IM cs.SYeess.SYgr-qcphysics.ins-det
keywords missionsilviadesignedgravitationalinterferometerrelativespacecraftwave
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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We propose SILVIA (Space Interferometer Laboratory Voyaging towards Innovative Applications), a mission concept designed to demonstrate ultra-precision formation flying between three spacecraft separated by 100 m. SILVIA aims to achieve sub-micrometer precision in relative distance control by integrating spacecraft sensors, laser interferometry, low-thrust and low-noise micro-propulsion for real-time measurement and control of distances and relative orientations between spacecraft. A 100-meter-scale mission in a near-circular low Earth orbit has been identified as an ideal, cost-effective setting for demonstrating SILVIA, as this configuration maintains a good balance between small relative perturbations and low risk for collision. This mission will fill the current technology gap towards future missions, including gravitational wave observatories such as DECIGO (DECihertz Interferometer Gravitational wave Observatory), designed to detect the primordial gravitational wave background, and high-contrast nulling infrared interferometers like LIFE (Large Interferometer for Exoplanets), designed for direct imaging of thermal emissions from nearby terrestrial planet candidates. The mission concept and its key technologies are outlined, paving the way for the next generation of high-precision space-based observatories.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. Space and Lunar Interferometry: Emerging Concepts and Pathways

    astro-ph.IM 2026-07 accept novelty 3.5

    Science targets set wavelength and resolution, which fix baseline and architecture for free-flying and lunar interferometers, with shared technologies and a decade of pathfinder decisions determining which become missions.