This page is a real-time composition built from four live data streams. Nothing here is decorative—every visual element is driven by data pulled from NASA and weather APIs right now.
The central mass is today's Astronomy Picture of the Day. The photograph has been decomposed: each pixel is sampled for its color and brightness, then re-rendered as an individual light particle. Bright regions of the image produce denser particle clusters. The photograph's structure—spiral arms, nebula filaments, star fields—is preserved in the particle distribution, but the image itself is gone. You're looking at its data, not its surface.
The orbiting particle clusters represent asteroids currently approaching Earth, pulled from NASA's NEO (Near Earth Object) API. Each asteroid becomes a cluster of particles. Larger asteroids produce larger clusters. Their orbital speed maps to their actual approach velocity. When an asteroid's closest approach distance is small, its cluster drifts closer to the central APOD body—the two masses begin to entangle. Hazardous asteroids glow red.
The background turbulence and grain intensity are driven by solar flare activity from NASA's DONKI (Space Weather Database). Recent solar flares increase the visual noise, color volatility, and particle drift chaos across the entire canvas. A quiet sun produces a smooth, stable image. An active sun makes everything jitter. Solar flares are classified from B (weakest) through C, M, to X (strongest).
The color palette and volumetric fog are shaped by live weather in Charleston, SC via Open-Meteo. Temperature shifts the color from cyan (cold) to magenta (warm). Cloud cover controls fog density and grain intensity. Wind speed drifts particles laterally.
Move your mouse to push particles and shift the fog center. The composition regenerates continuously. Tomorrow, a new APOD image resets the primary body, and the asteroid field updates with new approach data.
Data: NASA APOD, NEO, DONKI APIs & Open-Meteo • Built by Wayne Intelligence
Sampling light...