# WASP-19 b artistic concept: visual basis

This image is an **artistic conceptual visualization**, not an observation, recovered image, simulation output, or scale diagram. It was generated with OpenAI's built-in image-generation tool on 2026-10-04 for this report.

The art direction uses evidence-informed but deliberately non-quantitative cues:

- a very close orbit and strongly heated hemisphere, reflecting the 0.789-day orbit and roughly 2,100 K equilibrium-temperature regime;
- a golden, visibly active late-G host, consistent with the stellar-activity problem that complicates transmission spectroscopy;
- dark copper circulation bands and a sharp terminator to communicate strong irradiation and day–night transport;
- a thin blue-gray high-altitude limb, representing the blue scattering reported in optical studies without encoding a unique composition.

The colors, band morphology, haze thickness, stellar surface, viewing angle, apparent sizes and orbital separation are interpretive. In particular, the image does **not** depict TiO, Na or H₂O as confirmed spatial structures. Those published inferences depend on instrument, epoch, reduction and model choice and are discussed as conflicting evidence in the report. Quantitative conclusions come only from the cited observations and scientific figures.

## Generation prompt summary

Wide NASA/ESA-style editorial scientific visualization of a nearly spherical, intensely irradiated gas giant near an active late-G star, with charcoal/copper circulation, a restrained blue-gray scattering limb, sparse space background, and no text, rings, moons, solid surface, chemistry icons or exaggerated tail.