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3122 Florence and Tidal locking

Shortcuts: Differences, Similarities, Jaccard Similarity Coefficient, References.

Difference between 3122 Florence and Tidal locking

3122 Florence vs. Tidal locking

3122 Florence is a stony trinary asteroid of the Amor group. Tidal locking (also called gravitational locking or captured rotation) occurs when the long-term interaction between a pair of co-orbiting astronomical bodies drives the rotation rate of at least one of them into the state where there is no more net transfer of angular momentum between this body (e.g. a planet) and its orbit around the second body (e.g. a star); this condition of "no net transfer" must be satisfied over the course of one orbit around the second body.

Similarities between 3122 Florence and Tidal locking

3122 Florence and Tidal locking have 2 things in common (in Unionpedia): Minor-planet moon, Orbital eccentricity.

Minor-planet moon

A minor-planet moon is an astronomical object that orbits a minor planet as its natural satellite.

3122 Florence and Minor-planet moon · Minor-planet moon and Tidal locking · See more »

Orbital eccentricity

The orbital eccentricity of an astronomical object is a parameter that determines the amount by which its orbit around another body deviates from a perfect circle.

3122 Florence and Orbital eccentricity · Orbital eccentricity and Tidal locking · See more »

The list above answers the following questions

3122 Florence and Tidal locking Comparison

3122 Florence has 33 relations, while Tidal locking has 139. As they have in common 2, the Jaccard index is 1.16% = 2 / (33 + 139).

References

This article shows the relationship between 3122 Florence and Tidal locking. To access each article from which the information was extracted, please visit:

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