The Spheroid Classification: Small Formed Baryonic Spheres
Abstract
This paper introduces the Spheroid classification for small baryonic objects that formed in the SMDS extrusion disc but were removed before reaching planetary mass. Spheroids originate in the same condensation environment as planets—the galactic foundry extrusion zone—but are pulled away with departing stellar systems before completing their growth. This distinguishes them from asteroids, which result from collapse or collision events, and from planets, which completed their formation. Spheroids are proto-planets frozen at an early developmental stage, transported throughout the galaxy with their host stellar systems.
Fields of Study & Subjects
Astronomy and Astrophysical Research
Stellar
planetary
and galactic studies
Astrophysics and Star Formation Studies
Publication details
- Journal / source
- Zenodo (CERN European Organization for Nuclear Research)
- Publication date
- 4 January 2026
- Document type
- Preprint