line of nodes The line of intersection of the Moon's orbit with the ecliptic plane.
lithosphere Earth's crust and a small portion of the upper mantle that make up Earth's plates. This layer of the Earth undergoes tectonic activity.
Line of nodes The imaginary line passing through the ascending and descending nodes of an orbit. It is the line of intersection of the orbital plane with the reference plane.
Line of Nodes
The nodes of the moons orbit are the points where it passes through the plane of the earth's orbit. An eclipse season occurs whenever the line connecting these nodes (line of nodes) points toward the sun.
Line Profile ...
line of nodes: The line across an orbit connecting the nodes; commonly applied to the orbit of the moon.
liquid metallic hydrogen: A form of hydrogen under high pressure that is a good electrical conductor.
Line of Nodes - The line connecting the two nodes of the Moon's orbit around the Earth
Lithosphere - The rigid outer layer of a planet or satellite, composed of the crust and upper mantle ...
line of nodes the intersection of a planet's or the Moon's orbit with the Earth's orbit. local noon when the Sun is on an observer's meridian.
line of nodes The straight line connecting the two points of intersection of the orbit or a planet, planetoid, or comet and the ecliptic, or the line of intersection of the planes of the orbits of a satellite and its primary.
The line connecting the nodes is called line of nodes.
2. A point, line, or surface in a standing wave where some characteristic of the wave field has essentially zero amplitude.
The absolute direction of the line of nodes changes but slowly as the earth and moon revolve; cerse"uently, in the case shown in the figure, ...
The "line of nodes" indicates the points at which 12 Boo B seems to cross the sky's apparent plane.
A line connecting two nodes is called a line of nodes. The lunar nodes are the points where the moon's line of nodes, when extended, strike the celestial sphere.
If the orbit has a non-zero inclination, then the plane that includes the orbit-focus and is perpendictular to our line of sight intersects the plane of the orbit in a line called the line of nodes.
To reconcile the observed rotation (line of nodes) with the distribution (major axis orientation) of the old populations, a transverse motion of the Large Cloud amounting to about 300 km s-1 is required.
1 degree tilt of the Moon's orbit around the Earth compared to the Earth's orbit around the Sun. The intersection of these two orbits is the line of nodes, and solar eclipses occur when this line is pointing towards the centre of the Sun.
 See also: Orbit, Time, Sun, Planet, Solar
  
|
RSS
