Compact Ultradense Objects in the Solar System
J. Rafelski (Arizona), Ch. Dietl, and L. Labun
TL;DR
This paper explores the properties and gravitational interactions of ultra-dense objects in the solar system, proposing that they may be enclosed in comets and influence impact phenomena.
Contribution
It introduces the hypothesis that compact ultra dense objects (CUDOs) can be embedded in comets, affecting impact stability and resolving certain cometary impact issues.
Findings
CUDOs can be enclosed in comets.
CUDO cores may stabilize comet impacts.
Hypothesis explains some comet impact anomalies.
Abstract
We describe properties and gravitational interactions of meteor-mass and greater compact ultra dense objects with nuclear density or greater (CUDO s). We discuss possible enclosure of CUDO s in comets, stability of these objects on impact with the Earth and Sun and show that the hypothesis of a CUDO core helps resolve issues challenging the understanding of a few selected cometary impacts.
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