universal gravitational constant
Học thuậtThân thiện
A student calculates the universal gravitational constant in a physics textbook.
Definition
- Noun:
- A fundamental physical constant: The "universal gravitational constant" is a fixed numerical value that appears in Newton's law of universal gravitation. It quantifies the strength of the gravitational force between two objects.
- The proportionality constant in Newton's law: It is the constant 'G' that relates the gravitational force between two bodies to the product of their masses and the inverse square of the distance between their centers.
Usage Examples
- Noun:
- The value of the universal gravitational constant is extremely small.
- Calculating the force between planets requires the use of the universal gravitational constant.
- Scientists have worked to measure the universal gravitational constant with great precision.
Advanced Usage
- "To determine the universal gravitational constant": Refers to the experimental process of measuring its value.
- The Cavendish experiment was designed to determine the universal gravitational constant.
- In equations: It is almost exclusively represented by the symbol 'G'.
- The formula F = G * (m1m2)/r² contains the universal gravitational constant.*
Variants and Related Words
- Gravitational constant (n): A common shortened form for "universal gravitational constant".
- The gravitational constant is a key part of Einstein's field equations.
- Constant of gravitation (n): Another synonymous term.
- Newton's constant (n): A name reflecting its origin in Newton's law.
Synonyms
- G: The standard symbol used in physics.
- Cavendish's constant: A historical name referencing Henry Cavendish, who performed an early measurement.
Related Phrases
- Law of universal gravitation: The physical law in which the constant is used.
- Big G: An informal name used to distinguish it from 'g' (acceleration due to gravity).
A student calculates the universal gravitational constant in a physics textbook.
Noun
- (physics) the universal constant relating force to mass and distance in Newton's law of gravitation