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4 Equulei and Radial velocity

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

Difference between 4 Equulei and Radial velocity

4 Equulei vs. Radial velocity

4 Equulei is a binary star system in the constellation of Equuleus, located about 3° to the east of Alpha Equulei. The radial velocity of an object with respect to a given point is the rate of change of the distance between the object and the point.

Similarities between 4 Equulei and Radial velocity

4 Equulei and Radial velocity have 3 things in common (in Unionpedia): Binary star, Orbital eccentricity, Semi-major and semi-minor axes.

Binary star

A binary star is a star system consisting of two stars orbiting around their common barycenter.

4 Equulei and Binary star · Binary star and Radial velocity · 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.

4 Equulei and Orbital eccentricity · Orbital eccentricity and Radial velocity · See more »

Semi-major and semi-minor axes

In geometry, the major axis of an ellipse is its longest diameter: a line segment that runs through the center and both foci, with ends at the widest points of the perimeter.

4 Equulei and Semi-major and semi-minor axes · Radial velocity and Semi-major and semi-minor axes · See more »

The list above answers the following questions

4 Equulei and Radial velocity Comparison

4 Equulei has 27 relations, while Radial velocity has 35. As they have in common 3, the Jaccard index is 4.84% = 3 / (27 + 35).

References

This article shows the relationship between 4 Equulei and Radial velocity. To access each article from which the information was extracted, please visit:

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