Descrizione: D:\backup disco E\04_II_SESTANTE_SITO\en\ASTRONOMIA\i_grandi_astronomi\Colombo\kirkwood_gaps\indietro.gif  The main asteroid belt within the orbits of Mars and Jupiter

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Histogram of the distribution of the asteroid semi-major axes

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"Gaps" in the distribution of the asteroid semi-major axes

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«... Already 100 years passed by from the discovery of the Kirkwood gaps in the distribution of the asteroid semi major axes and, still [1981], a theory able to explain their origin has not been found. [...] (1) » 
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i        These are the most popular hypotheses:  
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Gaps are only a statistical occurrence

Gaps are formed by gravitational forces alone

Gaps form, because near to resonance asteroids tend to assume a large eccentricity and due to collisions with other asteroids can be ejected

Asteroids never occupy the gaps

 

Revision of the hypotheses

The statistical assumption led to the conclusion that asteroids near to resonance never cross it

The gravitational hypothesis was studied analytically with the planar model of the restricted three bodies problem. In such a hypothesis asteroids located in the “gap”, never leave it

The collision hypothesis was studied following a procedure related with the plane-elliptical problem, to test asteroids very close to resonance. Eccentricity showed no evidence it could increase much. Furthermore, the study of the collision probabilities showed very small values

The dynamic hypotheses, necessary to explore the possibility that asteroids may never be found within the “gaps”, were not yet thoroughly examined

 

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1981: studies and simulations on gap 3:1 – unstable resonance with Jupiter

How to explain the formation of the “gap” concerning the 3:1 resonance of the asteroids with Jupiter was analytically taken into consideration and developed with the help of the computer of Jack Wisdom (1), a contemporary of Bepi Colombo on this topic. 
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The problem was gradually examined, starting from the most simple planar models.  
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The negative answers given by the simplified models led to take into consideration a 3D model in place of a planar one; to consider the inclination of Jupiter’s orbit; Jupiter’s orbit is not static, but is subject to age-old perturbations and, from a strict mathematical point of view, in the processing of the equations also the terms of higher order [up to least 4th level] in the eccentricity were included; also included were the long period resonance terms and the high frequency perturbations. 
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Additionally, it was observed that the time requested for a gap is longer than what was estimated till now. 
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So, this more flexible model, after a suitable period of time, discovered that the eccentricity of the orbit of the asteroid near to the 3:1 resonance, suddenly sharply raised, from low values, [less than 0,10] to higher values [more than 0,3], sufficient to cross the orbit of Mars. 
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A gap shape is obtained, quite similar to the one measured in the distribution of the semi major axes, assuming that within time Mars may remove through a “slingshot effect” ["fly-by"] the asteroids within the 3:1 resonance band, with an eccentricity more than 0.3. 
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Lifetime of a “Mars crosser” [eccentricity more than 0,3] has been estimated in 200 million years. 
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Gap 3:1 is completed in a period of time of 18 million years. 
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Results of the study are summarised as follows:

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(1) Jack Widsom - "The Origin of the Kirkwood Gaps: a Mapping for Asteroidal Motion near the 3/1 Commensurability 
      The Astronomical Journal - 1981