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Gaussian gravitational constant and Specific relative angular momentum

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

Difference between Gaussian gravitational constant and Specific relative angular momentum

Gaussian gravitational constant vs. Specific relative angular momentum

The Gaussian gravitational constant (symbol) is a parameter used in the orbital mechanics of the solar system. In celestial mechanics the specific relative angular momentum \vec plays a pivotal role in the analysis of the two-body problem.

Similarities between Gaussian gravitational constant and Specific relative angular momentum

Gaussian gravitational constant and Specific relative angular momentum have 10 things in common (in Unionpedia): Conic section, International System of Units, Johannes Kepler, Kepler's laws of planetary motion, Newton's law of universal gravitation, Orbital period, Perturbation (astronomy), Second, Standard gravitational parameter, Two-body problem.

Conic section

In mathematics, a conic section (or simply conic) is a curve obtained as the intersection of the surface of a cone with a plane.

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International System of Units

The International System of Units (SI, abbreviated from the French Système international (d'unités)) is the modern form of the metric system, and is the most widely used system of measurement.

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Johannes Kepler

Johannes Kepler (December 27, 1571 – November 15, 1630) was a German mathematician, astronomer, and astrologer.

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Kepler's laws of planetary motion

In astronomy, Kepler's laws of planetary motion are three scientific laws describing the motion of planets around the Sun.

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Newton's law of universal gravitation

Newton's law of universal gravitation states that a particle attracts every other particle in the universe with a force which is directly proportional to the product of their masses and inversely proportional to the square of the distance between their centers.

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Orbital period

The orbital period is the time a given astronomical object takes to complete one orbit around another object, and applies in astronomy usually to planets or asteroids orbiting the Sun, moons orbiting planets, exoplanets orbiting other stars, or binary stars.

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Perturbation (astronomy)

In astronomy, perturbation is the complex motion of a massive body subject to forces other than the gravitational attraction of a single other massive body.

Gaussian gravitational constant and Perturbation (astronomy) · Perturbation (astronomy) and Specific relative angular momentum · See more »

Second

The second is the SI base unit of time, commonly understood and historically defined as 1/86,400 of a day – this factor derived from the division of the day first into 24 hours, then to 60 minutes and finally to 60 seconds each.

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Standard gravitational parameter

In celestial mechanics, the standard gravitational parameter μ of a celestial body is the product of the gravitational constant G and the mass M of the body.

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Two-body problem

In classical mechanics, the two-body problem is to determine the motion of two point particles that interact only with each other.

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The list above answers the following questions

Gaussian gravitational constant and Specific relative angular momentum Comparison

Gaussian gravitational constant has 53 relations, while Specific relative angular momentum has 25. As they have in common 10, the Jaccard index is 12.82% = 10 / (53 + 25).

References

This article shows the relationship between Gaussian gravitational constant and Specific relative angular momentum. To access each article from which the information was extracted, please visit:

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