Planetary Formation: A Field-Based Framework
The standard model of planetary formation, solar nebula collapse, planetesimal aggregation, runaway accretion, has served science well as a descriptive framework. It accounts for the broad strokes: a rotating cloud of gas and dust flattens into a disk, clumps form, gravity takes over, and planets emerge. What it doesn't account for, at least not satisfyingly, is the precision. Why are planetary orbits spaced the way they are? Why do planets in the same disk end up with such dramatically different compositions and interior architectures? Why do magnetic fields emerge with the geometry they do, and why does tectonic activity persist billions of years into a planet's life? These questions get waved at, but they don't get answered at the structural level. This paper proposes that the missing layer is field geometry, specifically, the organized electromagnetic and gravitational field environment generated by the star itself, which acts as a structural template for everything that follows. This work is part of a larger collection of UST documents. The other versions available in the DOI record are not revisions of this document. They are separate papers written for different purposes. Some versions present the full mathematical proofs behind the update rules, others provide a technical physical description of substrate behavior, and others are formal proof papers built around the Universal Balance Laws. Together, these documents form a complete set: a plain‑language booklet, a physical description paper, and full mathematical proof papers, each offering a different perspective on the same underlying theory. If you have questions or want to discuss the work, you can contact me directly at [email protected] Don't be shy. I want to discuss science. It is fun and should be. Reachout and lets get started on new discoveries.
Authors
- Dustin Lee
Publication Details
- Journal
- Zenodo (CERN European Organization for Nuclear Research)
- Published
- 2026-08-28
- DOI
- https://doi.org/10.5281/zenodo.22137385
- Primary Topic
- Astrophysics and Star Formation Studies
- Type
- preprint