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Other literature type . 2026
License: CC BY
Data sources: ZENODO
ZENODO
Other literature type . 2026
License: CC BY
Data sources: Datacite
ZENODO
Other literature type . 2026
License: CC BY
Data sources: Datacite
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The equation for Planetary Mass from any Accretion Disc

Authors: Braben, Peter;

The equation for Planetary Mass from any Accretion Disc

Abstract

Abstract : This is the 2nd of 4 papers describing a new planet and star formation theory. Currently there is no explanation for why planets form with particular masses. A number of models have been suggested, (for example the Nice[1] model and others), but these conflict both with conservation of momentum, and Kepler’s equations. This paper solves those problems, deriving a mass-equation mathematically, and then verifying with observed data. The paper will then go on to explain the formation of “Hot Jupiter” retrograde exoplanets[2], explain the formation of giant planets like Jupiter and Saturn in our own Solar System, and also put forward a hypothetical new class of Astronomical objects, “Dark Stars”[3], which can potentially revolutionise Astronomy. This paper will additionally identify 32 exosystems where life as we know it is likely to develop, and offer a potential explanation which removes the need for “Dark Matter” to exist. [1] Explained and challenged in this paper – see section 1.5 in this paper [2] Some 200 of these have been observed, and are currently substantially unexplained. [3] If this theory is correct, and these are observed, then it will avoid the need for “Dark Matter”.

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average