3D solar system · mistral-nemo
Output generated Cost / run $0.0003 Runtime 39.6s
Prompt for this run
Build a 3D solar-system visualization using the provided Three.js library. Use HTML, CSS, and JavaScript as needed. Write it to `index.html` in the current working directory using your file tools. Inline your own CSS and JavaScript. Do not use external assets, CDNs, or network requests. Use the provided `three.min.js` (global `THREE`) through a plain local script tag; the runner will inline it into the final artifact. Required behavior: - Show the Sun and all eight planets, with distinguishable colors, readable labels, and orbital paths against a procedural starfield. - Animate planets orbiting the Sun at different speeds. Use schematic sizes and distances for visibility; scientific scale accuracy is not required. Inner planets should generally orbit faster than outer planets. - Initially frame the complete system. Dragging orbits the camera around the Sun, and the mouse wheel changes camera distance within usable bounds. - Provide Pause/Resume and Reset view. Pause freezes planetary motion while leaving camera controls usable; Reset view restores the initial camera framing. - Generate materials and geometry procedurally. Only core global THREE is available; do not import additional controls or texture files. Verify: Inspect the initial planet labels and sample orbital motion. Orbit the camera and check that the system stays visible. Pause the simulation while adjusting the camera, then use Reset view and compare the initial framing.
TAKE IT TO CODE
A single self-contained HTML file — copy it and open in any browser, or reuse the prompt with your own pi-agent run.
RUN
METRICS
Transcript · 8 messages
Build a 3D solar-system visualization using the provided Three.js library. Use HTML, CSS, and JavaScript as needed. Write it to `index.html` in the current working directory using your file tools. Inline your own CSS and JavaScript. Do not use external assets, CDNs, or network requests. Use the provided `three.min.js` (global `THREE`) through a plain local script tag; the runner will inline it into the final artifact. Required behavior: - Show the Sun and all eight planets, with distinguishable colors, readable labels, and orbital paths against a procedural starfield. - Animate planets orbiting the Sun at different speeds. Use schematic sizes and distances for visibility; scientific scale accuracy is not required. Inner planets should generally orbit faster than outer planets. - Initially frame the complete system. Dragging orbits the camera around the Sun, and the mouse wheel changes camera distance within usable bounds. - Provide Pause/Resume and Reset view. Pause freezes planetary motion while leaving camera controls usable; Reset view restores the initial camera framing. - Generate materials and geometry procedurally. Only core global THREE is available; do not import additional controls or texture files. Verify: Inspect the initial planet labels and sample orbital motion. Orbit the camera and check that the system stays visible. Pause the simulation while adjusting the camera, then use Reset view and compare the initial framing.
{"command":"ls -la"}total 604 drwx------ 3 node node 4096 Oct 7 00:54 . drwxrwxrwt 6 root root 4096 Oct 7 00:54 .. drwxr-xr-x 3 node node 4096 Oct 7 00:54 .home -rw-r--r-- 1 node node 603445 Oct 7 00:54 three.min.js
Here is the current directory listing: ``` total 604 drwx------ 3 node node 4096 Oct 7 00:54 . drwxrwxrwt 6 root root 4096 Oct 7 00:54 .. drwxr-xr-x 3 node node 4096 Oct 7 00:54 .home -rw-r--r-- 1 node node 603445 Oct 7 00:54 three.min.js ``` The current directory contains the Three.js library file `three.min.js`.
index.html (3709 bytes)Successfully wrote to index.html
The single-page web app has been written to `index.html` in the current directory. It includes CSS in a `<style>` tag and JavaScript in a `<script>` tag, all inline. No external resources, CDNs, or network requests are used. The app is self-contained and runs fully sandboxed with no network access. Now, let's run the application in the browser and inspect the initial output and console. We'll use the available browser tools for a brief pass through the representative checks in the task, focusing on readily accessible behavior and the remaining time budget. We'll fix clear problems we discover and recheck the affected behavior. After that, we'll save the final file and briefly report what we actually checked and which behaviors remain unverified. The original 15-minute deadline still applies.