Ancient texts contain statements about the change of the year length in days, requiring adjustments of the calendars, and the change of the location where the Sun rises and sets, implying a change of the direction of the rotational momentum of the Earth, more precisely a reversal if the positions of sunrise and sunset would exactly interchange. Mechanisms that may change the axis direction have been recently considered. Changes due to impact with a sufficiently large asteroid or comet have been studied by Barbiero [1]; changes due to the torque by a sufficiently large body passing near the Earth have been considered by Woelfli and Baltensperger [2]. Changes of the orbital parameters, hence of the length of the year, have been considered by Brunini [3] for the case of an impact. To our knowledge changes in both the rotation and revolution parameters, that are expected after this type of interaction, have never been modelled mathematically. Here we provide under simplifying assumptions such an analysis.
On the reversal of the rotational momentum of Earth : a derivation and analysis of the Herodotus equation
SPEDICATO, Emilio Giuseppe
2006-01-01
Abstract
Ancient texts contain statements about the change of the year length in days, requiring adjustments of the calendars, and the change of the location where the Sun rises and sets, implying a change of the direction of the rotational momentum of the Earth, more precisely a reversal if the positions of sunrise and sunset would exactly interchange. Mechanisms that may change the axis direction have been recently considered. Changes due to impact with a sufficiently large asteroid or comet have been studied by Barbiero [1]; changes due to the torque by a sufficiently large body passing near the Earth have been considered by Woelfli and Baltensperger [2]. Changes of the orbital parameters, hence of the length of the year, have been considered by Brunini [3] for the case of an impact. To our knowledge changes in both the rotation and revolution parameters, that are expected after this type of interaction, have never been modelled mathematically. Here we provide under simplifying assumptions such an analysis.File | Dimensione del file | Formato | |
---|---|---|---|
WPMateRi01(2006)Spedicato.pdf
accesso aperto
Versione:
publisher's version - versione editoriale
Licenza:
Licenza default Aisberg
Dimensione del file
333.64 kB
Formato
Adobe PDF
|
333.64 kB | Adobe PDF | Visualizza/Apri |
Pubblicazioni consigliate
Aisberg ©2008 Servizi bibliotecari, Università degli studi di Bergamo | Terms of use/Condizioni di utilizzo