Improved physical properties database of trans-Neptunian dwarf planets

TL;DR

This paper introduces a new calculation method for the physical properties of trans-Neptunian dwarf planets, aiming to improve the accuracy and consistency of their database by revealing underlying relationships.

Contribution

It presents a novel calculation procedure that uncovers unknown relationships among physical properties, suggesting a common origin for these celestial bodies.

Findings

Calculated properties align well with observational data.

Proposed relationships support the idea of a uniform group of dwarf planets.

Enhanced database can aid future research and observations.

Abstract

Because of the objectively existing causes, such as an irregular shape of a celestial body, the lack of the satellites, the low values of albedo at moderate sizes, and a large remoteness from the Sun, creating a more exact the physical properties database of trans-Neptunian dwarf planets in comparison with existing that continues to remain a problem. We offer a new calculation procedure of the physical properties of these objects involving earlier unknown the relationships harmonizing these properties. It allows us to conjecture of they are a group of uniform celestial bodies by their origin beyond the Kuiper belt. The calculated physical properties of these dwarf planets are in a good agreement with the estimates received from observational data and can form the basis for support the validity of this improved physical properties database.