mean distance

Thân thiện

The mean distance of the Moon from Earth is about 384,400 kilometers.

Definition

Noun: - Mean Distance: In astronomy, this term refers specifically to the arithmetic mean (average) of the greatest (maximum) and least (minimum) distances between a celestial body, such as a satellite or a secondary star, and the primary body it orbits.

Usage

• This is a technical term used primarily in the fields of astronomy, astrophysics, and orbital mechanics to describe a standard, averaged orbital parameter.
• It is often used when discussing the orbits of moons around planets, planets around stars, or in binary star systems.

Examples

• Noun:
  • The mean distance of the Moon from Earth is approximately 384,400 kilometers.
  • Astronomers calculated the planet's mean distance from its sun to determine its orbital period.

Advanced Usage

• "Semi-major axis": In many orbital calculations, the "mean distance" is effectively equivalent to the semi-major axis of an elliptical orbit. This is a more precise term used in Kepler's laws of planetary motion.
  • For a perfectly circular orbit, the mean distance is constant and equal to the radius.

Variants and Related Words

• Orbital Radius: Often used interchangeably in contexts of circular orbits, though "mean distance" is more general for elliptical paths.
• Average Distance: A less technical synonym, though it lacks the specific astronomical definition of averaging only the extreme points.

Synonyms

• Average Distance (in a general, non-technical sense)
• Semi-major Axis (in the context of orbital mechanics for elliptical orbits)

Notes on Meaning

• This term has a single, specific technical meaning in its primary context. It should not be confused with a simple statistical average of many distance measurements over time. It is defined specifically as (Maximum Distance + Minimum Distance) / 2.
• It provides a single, representative figure for the separation between two orbiting bodies, which is useful for calculations involving orbital period and gravitational force.

Học thuật

Noun

1. the arithmetic mean of the maximum and minimum distances of a celestial body (satellite or secondary star) from its primary