The Spheroid Classification: Small Formed Baryonic Spheres

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Authors: Matt Webb
Cited by: 0

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