the specific relative angular momentum (often denoted h → {\displaystyle {\vec {h}}} or h {\displaystyle \mathbf {h} } ) of a body is the angular momentum...

Angular momentum (sometimes called moment of momentum or rotational momentum) is the rotational analog of linear momentum. It is an important physical...

mechanics, angular momentum coupling is the procedure of constructing eigenstates of total angular momentum out of eigenstates of separate angular momenta...

The angular momentum of light is a vector quantity that expresses the amount of dynamical rotation present in the electromagnetic field of the light. While...

specific angular momentum because it equals the magnitude L of the angular momentum divided by the mass m of the particle. For brevity, the angular speed...

the bodies; h {\displaystyle h} is the specific relative angular momentum in the sense of relative angular momentum divided by the reduced mass; e {\displaystyle...

for an atomic orbital that determines its orbital angular momentum and describes aspects of the angular shape of the orbital. The azimuthal quantum number...

Spin is an intrinsic form of angular momentum carried by elementary particles, and thus by composite particles such as hadrons, atomic nuclei, and atoms...

notably quantum chemistry, angular momentum diagrams, or more accurately from a mathematical viewpoint angular momentum graphs, are a diagrammatic method...

h\,=r\,v\,\cos \phi } where: h {\displaystyle h\,} is the specific relative angular momentum of the orbit, v {\displaystyle v\,} is the orbital speed of...

r={{h^{2}} \over {\mu }}} where: h = r v {\displaystyle h=rv} is specific angular momentum of the orbiting body. This is because μ = r v 2 {\displaystyle...

{\displaystyle \mathbf {v} } ) can be easily used to compute the specific angular momentum vector as h = r × v {\displaystyle \mathbf {h} =\mathbf {r} \times...

point to POI h1 is defined as specific angular momentum of the original orbit h2 is defined as specific angular momentum of the phasing orbit Remember...

orbiting body from the central body, h {\displaystyle h\,} is the specific angular momentum of the orbiting body, ν {\displaystyle \nu \,} is the true anomaly...

motion do not change: the angular momentum and the mechanical energy. The first constant, called specific angular momentum, can be defined as h = 2 d...

the masses of objects 1 and 2, and h {\displaystyle h} is the specific angular momentum of object 2 with respect to object 1. The parameter θ {\displaystyle...

longitude of the ascending node can be calculated from the specific relative angular momentum vector h as follows: n = k × h = ( − h y , h x , 0 ) Ω = {...

perpendicular at apoapsis and periapsis, conservation of angular momentum requires specific angular momentum h = r p v p = r a v a = constant {\displaystyle...

orbital period is the same, disregarding their eccentricity. The specific angular momentum h of a small body orbiting a central body in a circular or elliptical...

conservation of angular momentum. Areal velocity is closely related to angular momentum. Any object has an orbital angular momentum about an origin,...

Celestial mechanics There is a related parameter, known as the specific relative angular momentum, h {\displaystyle h} . It is related to ℓ {\displaystyle \ell...

\!} is velocity vector h {\displaystyle \mathbf {h} \,\!} is specific angular momentum vector (equal to r × v {\displaystyle \mathbf {r} \times \mathbf...

communication satellites use much higher geostationary orbits and move at the same angular velocity as the Earth as to appear stationary above one location on the...

specific angular momentum, h, of the initial and final orbits are equal in magnitude but not in direction. Therefore, the change in specific angular momentum...

Sun's equator or the invariable plane (the plane that represents the angular momentum of the Solar System, approximately the orbital plane of Jupiter). The...

is characterized by specific energy E = 1 2 v 2 + Φ ( r ) {\textstyle E={\frac {1}{2}}v^{2}+\Phi (r)} and specific angular momentum L = | r → × v → | {\displaystyle...

in momentum (impulse), where: Δ p = m Δ v {\displaystyle \Delta \mathbf {p} =m\Delta \mathbf {v} } , where p {\displaystyle \mathbf {p} } is momentum and...

distance to the central body because of the law of conservation of angular momentum, or equivalently, Kepler's second law. This states that as a body moves...

during equal intervals of time). The constant of integration, h, is the angular momentum per unit mass. In order to get an equation for the orbit from equation...

gravitational parameter based on the total mass, and h the specific relative angular momentum (angular momentum divided by the reduced mass).: 12–17  For values...