ざひょう座標zahyou
1.

A set of numerical values that specify the location of a point in a defined space, commonly represented in two or three dimensions using a structured system such as Cartesian coordinates.

2.

A framework or reference that determines the positioning of an object or concept, reflecting its placement relative to a predetermined standard or baseline.

3.

A structured arrangement that provides a clear indication of a point's position, often used in mathematical contexts to analyze spatial relationships and movements.

ざひょうじく座標軸zahyoujiku
1.

A system of reference lines used in mathematics to identify the position of points within a two-dimensional or three-dimensional space by establishing a structured framework for measurement.

2.

A set of lines, often intersecting at right angles, that serves as a basis for plotting and interpreting the location of points in relation to a defined origin within a geometric framework.

3.

Lines that provide a systematic way to represent and communicate the relative positioning of objects or points, often in relation to a central reference point or origin.

デカルトdekarutoざひょう座標zahyou
1.

A system for identifying points in a plane using two perpendicular axes, typically labeled as horizontal and vertical, based on numerical values.

2.

A method of representing the position of a point in a two-dimensional space through an ordered pair of numbers showing its distance from the origin along the axes.

3.

A geometric framework that allows for the precise plotting and analysis of points, lines, and shapes by defining their location through numerical coordinates.

ぎんがざひょう銀河座標gingazahyou
1.

A system of coordinates used to describe positions within the Milky Way galaxy, defined with respect to the galactic equator and measured in terms of galactic latitude and longitude.

2.

A specialized method for mapping and analyzing the structure of the Milky Way, where galactic latitude indicates the angle north or south of the galactic equator, and galactic longitude denotes the angle measured in a clockwise direction from a reference point aligned with the center of the galaxy.

3.

A celestial coordinate framework that aids astronomers in studying the distribution and movement of objects within our galaxy, employing a base of the galactic plane to establish angular measurements in both north-south and east-west orientations.

そうたいざひょう相対座標soutaizahyou
1.

A coordinate system where positions are specified in relation to a designated reference point, rather than using fixed global coordinates.

2.

A method of defining locations based on their relationship to other points within the same system, allowing for flexible positioning in various contexts.

3.

A type of coordinate expression that emphasizes the differences in position relative to certain origins or landmarks, rather than absolute measurements.