About

The Virtual Solar Swarm starts from a question with the hard part removed. Assume getting there is solved by someone else, and that a sensor package can arrive anywhere in the solar system. What would you send to each of the two hundred or so moons and planets we know by name, and why? Then what lies beyond them? Here that question becomes working models you can pull on. It is a thing to think with, not a mission plan.

This is an evolving choose-your-own science adventure, made to help open up the solar system for the civic space stewards of Earth and the solar system.

Data and models

Nothing described on this site has been built or launched. The orbital elements, sizes, masses, spin rates, tilts and magnetic axes of all 384 catalogued bodies are real published values; the physics is real but simplified; the satellites, buses, instruments and timelines are design fiction grounded in current public technology, and the cost figures are engineering estimates for comparison, not a budget anyone has raised.

The orbits come from NASA/JPL. The eight planets use JPL's Keplerian element set with its secular rates; the 187 asteroids, comets, centaurs, dwarf planets and trans-Neptunian objects come from the JPL Small-Body Database, each at its own solution epoch; the moons carry ecliptic mean elements fitted to JPL Horizons. Checked against JPL Horizons on 26 August 2026, the heliocentric positions this site computes sit a median of one arcsecond from where Horizons puts them, and no body is further off than 0.02 degrees; moon positions sit a median of 0.7 degrees out. Radii and masses were reconciled against JPL body by body, keeping whichever reference is the newer one. The full source and accuracy note is in the repository.

Approximations

The concepts this leans on

The study assumes only technologies with flying ancestors: multi-satellite formation flying (NASA's MMS and the Starling swarm), swarm self-navigation by camera (Stanford's StarFOX experiment), deep-space laser communication (NASA's DSOC), quantum key distribution from orbit (the Micius satellite), solar observation from multiple vantage points (Solar Orbiter and the HelioSwarm concept), and satellite mass production as proven by Starlink. What has no ancestor yet is the scale, and scale is exactly what these models are for.

Imagery credits

The maps bundled with this site, each shown on its body's dossier and in the orbit lab:

Assemblies marked CC BY 4.0 are by Solar System Scope, built from NASA mission and elevation data, used under the Creative Commons Attribution 4.0 licence. NASA and USGS imagery is public domain. This site's own code and text are under its own licence, below.

Finding your way around

The site map lists every page grouped by what it is for, and Origins records where the question came from. The whole thing is a public repository: corrections to real measured data, and better authoritative maps, can be proposed through its issues. Where the surface maps came from, and where to find the ones still missing, is recorded in MAP-SOURCES.md.

Spacecraft images

The Watching the Sun page carries 44 spacecraft images from Wikimedia Commons, each under public domain or a Creative Commons licence that allows reuse (Public domain: 37, CC BY-SA 4.0: 2, CC BY-SA 3.0 igo: 2, CC0: 1, CC BY 4.0: 1, CC BY-SA 3.0: 1). Every card links to its mission page; the file behind each image is named in assets/watchers/_credits.json with its licence and creator.

The music

The songs on this site are by i C. infinity, from the album A Protopian Gambit: "Heliospheric Lantern" on the Sun's dossier, and both voices of "We Go Beyond" here and on the home page. The album is on Suno, and the wider music universe holds the rest.

Signature

🤝🔷 A Luke × Claude build. Created by Luke Nathan Hayes (auraofintelligence) and Claude (Fable 5), August 2026. Not a Codex build. Part of the wider Aura of Intelligence and Strange But True family of public design studies.

Licence

Released under the Strange But True Public Source Licence: free to read, learn from and adapt for personal, educational, artistic, research and community use with attribution; all commercial and corporate rights reserved to Luke Nathan Hayes. The full text is in LICENCE.md.