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6235 Burney and Hiroshi Kaneda

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

Difference between 6235 Burney and Hiroshi Kaneda

6235 Burney vs. Hiroshi Kaneda

6235 Burney, provisional designation, is a Florian or background asteroid from the inner regions of the asteroid belt, approximately in diameter. is a Japanese astronomer and discoverer of minor planets from Sapporo, in the northernmost prefecture of Japan.

Similarities between 6235 Burney and Hiroshi Kaneda

6235 Burney and Hiroshi Kaneda have 4 things in common (in Unionpedia): List of minor planet discoverers, Minor planet, Minor Planet Center, Seiji Ueda.

List of minor planet discoverers

This is a list of all astronomers who are credited by the Minor Planet Center (MPC) with the discovery of one or several minor planets.

6235 Burney and List of minor planet discoverers · Hiroshi Kaneda and List of minor planet discoverers · See more »

Minor planet

A minor planet is an astronomical object in direct orbit around the Sun (or more broadly, any star with a planetary system) that is neither a planet nor exclusively classified as a comet.

6235 Burney and Minor planet · Hiroshi Kaneda and Minor planet · See more »

Minor Planet Center

The Minor Planet Center (MPC) is the official worldwide organization in charge of collecting observational data for minor planets (such as asteroids and comets), calculating their orbits and publishing this information via the Minor Planet Circulars.

6235 Burney and Minor Planet Center · Hiroshi Kaneda and Minor Planet Center · See more »

Seiji Ueda

is a Japanese astronomer.

6235 Burney and Seiji Ueda · Hiroshi Kaneda and Seiji Ueda · See more »

The list above answers the following questions

6235 Burney and Hiroshi Kaneda Comparison

6235 Burney has 38 relations, while Hiroshi Kaneda has 24. As they have in common 4, the Jaccard index is 6.45% = 4 / (38 + 24).

References

This article shows the relationship between 6235 Burney and Hiroshi Kaneda. To access each article from which the information was extracted, please visit:

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