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Elliptic orbit and Orbital mechanics

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

Difference between Elliptic orbit and Orbital mechanics

Elliptic orbit vs. Orbital mechanics

In astrodynamics or celestial mechanics, an elliptic orbit or elliptical orbit is a Kepler orbit with an eccentricity of less than 1; this includes the special case of a circular orbit, with eccentricity equal to 0. Orbital mechanics or astrodynamics is the application of ballistics and celestial mechanics to the practical problems concerning the motion of rockets and other spacecraft.

Similarities between Elliptic orbit and Orbital mechanics

Elliptic orbit and Orbital mechanics have 26 things in common (in Unionpedia): Apsis, Celestial mechanics, Circular orbit, Comet, Dwarf planet, Ellipse, Hohmann transfer orbit, Hyperbolic trajectory, Isaac Newton, Johannes Kepler, Kepler orbit, Kepler's laws of planetary motion, Newton's law of universal gravitation, Orbital eccentricity, Orbital elements, Orbital period, Orbital speed, Planet, Primary (astronomy), Semi-major and semi-minor axes, Solar System, Specific orbital energy, Specific relative angular momentum, Standard gravitational parameter, Virial theorem, Vis-viva equation.

Apsis

An apsis (ἁψίς; plural apsides, Greek: ἁψῖδες) is an extreme point in the orbit of an object.

Apsis and Elliptic orbit · Apsis and Orbital mechanics · See more »

Celestial mechanics

Celestial mechanics is the branch of astronomy that deals with the motions of celestial objects.

Celestial mechanics and Elliptic orbit · Celestial mechanics and Orbital mechanics · See more »

Circular orbit

A circular orbit is the orbit with a fixed distance around the barycenter, that is, in the shape of a circle.

Circular orbit and Elliptic orbit · Circular orbit and Orbital mechanics · See more »

Comet

A comet is an icy small Solar System body that, when passing close to the Sun, warms and begins to release gases, a process called outgassing.

Comet and Elliptic orbit · Comet and Orbital mechanics · See more »

Dwarf planet

A dwarf planet is a planetary-mass object that is neither a planet nor a natural satellite.

Dwarf planet and Elliptic orbit · Dwarf planet and Orbital mechanics · See more »

Ellipse

In mathematics, an ellipse is a curve in a plane surrounding two focal points such that the sum of the distances to the two focal points is constant for every point on the curve.

Ellipse and Elliptic orbit · Ellipse and Orbital mechanics · See more »

Hohmann transfer orbit

In orbital mechanics, the Hohmann transfer orbit is an elliptical orbit used to transfer between two circular orbits of different radii in the same plane.

Elliptic orbit and Hohmann transfer orbit · Hohmann transfer orbit and Orbital mechanics · See more »

Hyperbolic trajectory

In astrodynamics or celestial mechanics, a hyperbolic trajectory is the trajectory of any object around a central body with more than enough speed to escape the central object's gravitational pull.

Elliptic orbit and Hyperbolic trajectory · Hyperbolic trajectory and Orbital mechanics · See more »

Isaac Newton

Sir Isaac Newton (25 December 1642 – 20 March 1726/27) was an English mathematician, astronomer, theologian, author and physicist (described in his own day as a "natural philosopher") who is widely recognised as one of the most influential scientists of all time, and a key figure in the scientific revolution.

Elliptic orbit and Isaac Newton · Isaac Newton and Orbital mechanics · See more »

Johannes Kepler

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

Elliptic orbit and Johannes Kepler · Johannes Kepler and Orbital mechanics · See more »

Kepler orbit

In celestial mechanics, a Kepler orbit (or Keplerian orbit) is the motion of one body relative to another, as an ellipse, parabola, or hyperbola, which forms a two-dimensional orbital plane in three-dimensional space.

Elliptic orbit and Kepler orbit · Kepler orbit and Orbital mechanics · See more »

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.

Elliptic orbit and Kepler's laws of planetary motion · Kepler's laws of planetary motion and Orbital mechanics · See more »

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.

Elliptic orbit and Newton's law of universal gravitation · Newton's law of universal gravitation and Orbital mechanics · 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.

Elliptic orbit and Orbital eccentricity · Orbital eccentricity and Orbital mechanics · See more »

Orbital elements

Orbital elements are the parameters required to uniquely identify a specific orbit.

Elliptic orbit and Orbital elements · Orbital elements and Orbital mechanics · See more »

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.

Elliptic orbit and Orbital period · Orbital mechanics and Orbital period · See more »

Orbital speed

In gravitationally bound systems, the orbital speed of an astronomical body or object (e.g. planet, moon, artificial satellite, spacecraft, or star) is the speed at which it orbits around either the barycenter or, if the object is much less massive than the largest body in the system, its speed relative to that largest body.

Elliptic orbit and Orbital speed · Orbital mechanics and Orbital speed · See more »

Planet

A planet is an astronomical body orbiting a star or stellar remnant that is massive enough to be rounded by its own gravity, is not massive enough to cause thermonuclear fusion, and has cleared its neighbouring region of planetesimals.

Elliptic orbit and Planet · Orbital mechanics and Planet · See more »

Primary (astronomy)

A primary (also called a gravitational primary, primary body, or central body) is the main physical body of a gravitationally bound, multi-object system.

Elliptic orbit and Primary (astronomy) · Orbital mechanics and Primary (astronomy) · 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.

Elliptic orbit and Semi-major and semi-minor axes · Orbital mechanics and Semi-major and semi-minor axes · See more »

Solar System

The Solar SystemCapitalization of the name varies.

Elliptic orbit and Solar System · Orbital mechanics and Solar System · See more »

Specific orbital energy

In the gravitational two-body problem, the specific orbital energy \epsilon\,\! (or vis-viva energy) of two orbiting bodies is the constant sum of their mutual potential energy (\epsilon_p\,\!) and their total kinetic energy (\epsilon_k\,\!), divided by the reduced mass.

Elliptic orbit and Specific orbital energy · Orbital mechanics and Specific orbital energy · See more »

Specific relative angular momentum

In celestial mechanics the specific relative angular momentum \vec plays a pivotal role in the analysis of the two-body problem.

Elliptic orbit and Specific relative angular momentum · Orbital mechanics and Specific relative angular momentum · See more »

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.

Elliptic orbit and Standard gravitational parameter · Orbital mechanics and Standard gravitational parameter · See more »

Virial theorem

In mechanics, the virial theorem provides a general equation that relates the average over time of the total kinetic energy, \left\langle T \right\rangle, of a stable system consisting of N particles, bound by potential forces, with that of the total potential energy, \left\langle V_\text \right\rangle, where angle brackets represent the average over time of the enclosed quantity.

Elliptic orbit and Virial theorem · Orbital mechanics and Virial theorem · See more »

Vis-viva equation

In astrodynamics, the vis-viva equation, also referred to as orbital-energy-invariance law, is one of the equations that model the motion of orbiting bodies.

Elliptic orbit and Vis-viva equation · Orbital mechanics and Vis-viva equation · See more »

The list above answers the following questions

Elliptic orbit and Orbital mechanics Comparison

Elliptic orbit has 49 relations, while Orbital mechanics has 114. As they have in common 26, the Jaccard index is 15.95% = 26 / (49 + 114).

References

This article shows the relationship between Elliptic orbit and Orbital mechanics. To access each article from which the information was extracted, please visit:

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