geocentric parallax

Học thuật
Thân thiện
geocentric parallax

An astronomer measures the geocentric parallax of the Moon from two different observatories.

Definition
  1. Noun:
    • The apparent shift in the position of a celestial object when observed from two different points on Earth's surface, caused by Earth's rotation. This is a specific type of parallax used in astronomy. It measures the angle of displacement for a nearby celestial body (like the Moon or a planet) by observing it from two separate locations on Earth at the same time, or from one location as Earth rotates.
Usage
  • Noun:
    • Astronomers calculated the Moon's distance using geocentric parallax by making simultaneous observations from observatories in different hemispheres.
    • The geocentric parallax of Mars is much smaller than that of the Moon because Mars is farther away.
Advanced Usage
  • "Diurnal parallax": This is another term for geocentric parallax, emphasizing that the measurement is taken over the course of a day (diurnal cycle) due to Earth's rotation.
    • The diurnal parallax of an asteroid can be used to determine its orbit.
Variants and Related Words
  • Parallax (n): The general effect or method of determining distance by observing an object from two different viewpoints.
    • Stellar parallax is used to measure the distance to nearby stars.
  • Horizontal parallax (n): A specific measurement of geocentric parallax when the celestial body is on the observer's horizon.
    • The horizontal parallax is the maximum value of geocentric parallax for a given body.
Synonyms
  • Diurnal parallax: The apparent shift measured over a daily cycle.
Related Concepts
  • Heliocentric parallax: Parallax measured using two points in Earth's orbit around the Sun (annual parallax), used for measuring stellar distances.
  • Triangulation: The geometric method underlying the concept of parallax for distance measurement.
geocentric parallax

An astronomer measures the geocentric parallax of the Moon from two different observatories.

Noun
  1. the parallax of a celestial body using two points on the surface of the earth as the earth rotates

Từ đồng nghĩa