Pick a date and see where Pluto, Eris, Sedna and their neighbours really are.

What's included

• Jupiter to Neptune plus Ceres, Pluto, Haumea, Makemake, Eris, Gonggong, Quaoar, Sedna and comet 1P/Halley, each at its real position for the chosen date (JPL orbital elements).
• Perihelion, aphelion, period and inclination of every body, stored in the object properties.
• A Kuiper belt and scattered disc drawn from the real structure (3:2 and 2:1 resonances, cold and hot populations).
• A schematic Oort cloud (2,000–100,000 AU), clearly labelled as theoretical.
• Halley with a tail that grows toward the Sun (set the date to 1986-02-09 for its perihelion).
• 19 cameras: overview, inner system, Kuiper belt, top view, Sedna's whole orbit, the Oort cloud and one per body.
• Studio or physical lighting, adaptive scale, labels, optional 50-year animation.
• A ready-to-render .blend (Cycles) with the script embedded, plus the script itself so you can change any setting and rebuild.
• README with what is real and what is not, CREDITS with all references.

What is illustrative (we say it up front)

• The Kuiper-belt rocks are random draws from the real structure, NOT real objects. The Oort cloud has never been observed and is a schematic.
• Surfaces are procedural and illustrative; rotation of the dwarf planets is not animated; moons and rings are not included.
• Orbits are two-body Kepler orbits from JPL osculating elements; Halley's real orbit is perturbed by the planets, so its date can be off by months.
• The JPL record gives a diameter only for Ceres and Halley; the other sizes are published values that you should verify if you quote them.

Who it is for: science communicators, teachers, planetarium and YouTube creators, and anyone who wants to show how far the Solar System really extends.

Data: NASA/JPL Small-Body Database; JPL (Standish). Not affiliated with or endorsed by NASA.