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4962 Vecherka and Asteroid spectral types

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

Difference between 4962 Vecherka and Asteroid spectral types

4962 Vecherka vs. Asteroid spectral types

4962 Vecherka, provisional designation, is a Eunomian asteroid and slow rotator from the central regions of the asteroid belt, approximately 10 kilometers in diameter. An asteroid spectral type is assigned to asteroids based on their emission spectrum, color, and sometimes albedo (reflectivity).

Similarities between 4962 Vecherka and Asteroid spectral types

4962 Vecherka and Asteroid spectral types have 4 things in common (in Unionpedia): Albedo, Asteroid, Asteroid spectral types, S-type asteroid.

Albedo

Albedo (albedo, meaning "whiteness") is the measure of the diffuse reflection of solar radiation out of the total solar radiation received by an astronomical body (e.g. a planet like Earth).

4962 Vecherka and Albedo · Albedo and Asteroid spectral types · See more »

Asteroid

Asteroids are minor planets, especially those of the inner Solar System.

4962 Vecherka and Asteroid · Asteroid and Asteroid spectral types · See more »

Asteroid spectral types

An asteroid spectral type is assigned to asteroids based on their emission spectrum, color, and sometimes albedo (reflectivity).

4962 Vecherka and Asteroid spectral types · Asteroid spectral types and Asteroid spectral types · See more »

S-type asteroid

S-type asteroids are asteroids with a spectral type that is indicative of a silicaceous (i.e. stony) mineralogical composition, hence the name.

4962 Vecherka and S-type asteroid · Asteroid spectral types and S-type asteroid · See more »

The list above answers the following questions

4962 Vecherka and Asteroid spectral types Comparison

4962 Vecherka has 31 relations, while Asteroid spectral types has 80. As they have in common 4, the Jaccard index is 3.60% = 4 / (31 + 80).

References

This article shows the relationship between 4962 Vecherka and Asteroid spectral types. To access each article from which the information was extracted, please visit:

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