Faster access than browser!Similarities between Apsis and Orbital eccentricity
Apsis and Orbital eccentricity have 32 things in common (in Unionpedia): Angular momentum, Apsidal precession, Astronomical object, Axial precession, Center of mass, Ceres (dwarf planet), Conic section, Earth, Ellipse, Elliptic orbit, Eris (dwarf planet), Halley's Comet, Haumea, Jupiter, Makemake, Mars, Mercury (planet), Milankovitch cycles, Moon, Neptune, Orbit, Perihelion and aphelion, Pluto, Saturn, Semi-major and semi-minor axes, Solar System, Solstice, Specific orbital energy, Specific relative angular momentum, Standard gravitational parameter, ..., Uranus, Venus. Expand index (2 more) »
Angular momentum
In physics, angular momentum (rarely, moment of momentum or rotational momentum) is the rotational equivalent of linear momentum.
Angular momentum and Apsis · Angular momentum and Orbital eccentricity ·
Apsidal precession
In celestial mechanics, apsidal precession or orbital precession is the precession (rotation) of the orbit of a celestial body.
Apsidal precession and Apsis · Apsidal precession and Orbital eccentricity ·
Astronomical object
An astronomical object or celestial object is a naturally occurring physical entity, association, or structure that exists in the observable universe.
Apsis and Astronomical object · Astronomical object and Orbital eccentricity ·
Axial precession
In astronomy, axial precession is a gravity-induced, slow, and continuous change in the orientation of an astronomical body's rotational axis.
Apsis and Axial precession · Axial precession and Orbital eccentricity ·
Center of mass
In physics, the center of mass of a distribution of mass in space is the unique point where the weighted relative position of the distributed mass sums to zero, or the point where if a force is applied it moves in the direction of the force without rotating.
Apsis and Center of mass · Center of mass and Orbital eccentricity ·
Ceres (dwarf planet)
Ceres (minor-planet designation: 1 Ceres) is the largest object in the asteroid belt that lies between the orbits of Mars and Jupiter, slightly closer to Mars' orbit.
Apsis and Ceres (dwarf planet) · Ceres (dwarf planet) and Orbital eccentricity ·
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.
Apsis and Conic section · Conic section and Orbital eccentricity ·
Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life.
Apsis and Earth · Earth and Orbital eccentricity ·
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.
Apsis and Ellipse · Ellipse and Orbital eccentricity ·
Elliptic orbit
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.
Apsis and Elliptic orbit · Elliptic orbit and Orbital eccentricity ·
Eris (dwarf planet)
Eris (minor-planet designation 136199 Eris) is the most massive and second-largest (by volume) dwarf planet in the known Solar System.
Apsis and Eris (dwarf planet) · Eris (dwarf planet) and Orbital eccentricity ·
Halley's Comet
Halley's Comet or Comet Halley, officially designated 1P/Halley, is a short-period comet visible from Earth every 74–79 years.
Apsis and Halley's Comet · Halley's Comet and Orbital eccentricity ·
Haumea
Haumea, minor-planet designation 136108 Haumea, is a dwarf planet located beyond Neptune's orbit.
Apsis and Haumea · Haumea and Orbital eccentricity ·
Jupiter
Jupiter is the fifth planet from the Sun and the largest in the Solar System.
Apsis and Jupiter · Jupiter and Orbital eccentricity ·
Makemake
Makemake (minor-planet designation 136472 Makemake) is a dwarf planet and perhaps the largest Kuiper belt object in the classical population, with a diameter approximately two thirds that of Pluto.
Apsis and Makemake · Makemake and Orbital eccentricity ·
Mars
Mars is the fourth planet from the Sun and the second-smallest planet in the Solar System after Mercury.
Apsis and Mars · Mars and Orbital eccentricity ·
Mercury (planet)
Mercury is the smallest and innermost planet in the Solar System.
Apsis and Mercury (planet) · Mercury (planet) and Orbital eccentricity ·
Milankovitch cycles
Milankovitch cycles describe the collective effects of changes in the Earth's movements on its climate over thousands of years.
Apsis and Milankovitch cycles · Milankovitch cycles and Orbital eccentricity ·
Moon
The Moon is an astronomical body that orbits planet Earth and is Earth's only permanent natural satellite.
Apsis and Moon · Moon and Orbital eccentricity ·
Neptune
Neptune is the eighth and farthest known planet from the Sun in the Solar System.
Apsis and Neptune · Neptune and Orbital eccentricity ·
Orbit
In physics, an orbit is the gravitationally curved trajectory of an object, such as the trajectory of a planet around a star or a natural satellite around a planet.
Apsis and Orbit · Orbit and Orbital eccentricity ·
Perihelion and aphelion
The perihelion of any orbit of a celestial body about the Sun is the point where the body comes nearest to the Sun.
Apsis and Perihelion and aphelion · Orbital eccentricity and Perihelion and aphelion ·
Pluto
Pluto (minor planet designation: 134340 Pluto) is a dwarf planet in the Kuiper belt, a ring of bodies beyond Neptune.
Apsis and Pluto · Orbital eccentricity and Pluto ·
Saturn
Saturn is the sixth planet from the Sun and the second-largest in the Solar System, after Jupiter.
Apsis and Saturn · Orbital eccentricity and Saturn ·
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.
Apsis and Semi-major and semi-minor axes · Orbital eccentricity and Semi-major and semi-minor axes ·
Solar System
The Solar SystemCapitalization of the name varies.
Apsis and Solar System · Orbital eccentricity and Solar System ·
Solstice
A solstice is an event occurring when the Sun appears to reach its most northerly or southerly excursion relative to the celestial equator on the celestial sphere.
Apsis and Solstice · Orbital eccentricity and Solstice ·
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.
Apsis and Specific orbital energy · Orbital eccentricity and Specific orbital energy ·
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.
Apsis and Specific relative angular momentum · Orbital eccentricity and Specific relative angular momentum ·
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.
Apsis and Standard gravitational parameter · Orbital eccentricity and Standard gravitational parameter ·
Uranus
Uranus is the seventh planet from the Sun.
Apsis and Uranus · Orbital eccentricity and Uranus ·
Venus
Venus is the second planet from the Sun, orbiting it every 224.7 Earth days.
The list above answers the following questions
- What Apsis and Orbital eccentricity have in common
- What are the similarities between Apsis and Orbital eccentricity
Apsis and Orbital eccentricity Comparison
Apsis has 80 relations, while Orbital eccentricity has 92. As they have in common 32, the Jaccard index is 18.60% = 32 / (80 + 92).
References
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