Name: how gravity acts between objects
Uploaded: 2025-05-22T09:06:17.000Z
Duration: 1 min 16 s
Channel: JoVE

La revolución de la luna alrededor de la Tierra indica la presencia de una fuerza que la atrae hacia el centro de la órbita.
Issac Newton propuso que esta fuerza de atracción es la misma que tira de una manzana hacia el suelo.
Fue una idea revolucionaria, ya que se creía que los objetos celestes y los objetos en la Tierra seguían reglas diferentes.
La luna tarda 27,3 días en orbitar la Tierra. Teniendo en cuenta la distancia media a la Luna, se puede estimar su aceleración. 
La relación entre la aceleración lunar y la aceleración de un objeto que cae sobre la Tierra indica que la aceleración es inversamente proporcional a la distancia al cuadrado.
Dado que la fuerza es la masa por la aceleración, la fuerza gravitacional es directamente proporcional a la masa e inversamente proporcional a la distancia al cuadrado.
Al observar que la aceleración de los planetas disminuye inversamente con su distancia al Sol, Newton predijo que la fuerza gravitacional actúa entre el Sol, los planetas y sus lunas.
Extendiendo este argumento a todos los objetos del universo, Newton formuló la ley de la gravitación universal.

<ol>
	<li>Verma, H.C. (2008). Conceptos de Física. Volumen 1, Bharati Bhawan Pub. & Dis.: secciones 11.1 y 11.2; páginas 203-204.</li>
</ol>

fuerza gravitacional

En los años anteriores a Newton, prevalecía una creencia general de que diferentes leyes gobernaban los objetos en el cielo que los objetos en la Tierra. Cuando Kepler escribió las tres leyes del movimiento planetario, explicando en detalle las propiedades geométricas de las órbitas planetarias alrededor del Sol, no hubo una idea inmediata para discernir su conexión con leyes más fundamentales. Fue Isaac Newton quien, en 1665-66, descubrió la conexión entre el movimiento planetario, el movimiento de la luna alrededor de la Tierra y el fenómeno cotidiano de los objetos que caen sobre la superficie de la Tierra. Este fenómeno universal se conoce hoy como gravitación. Aunque suene común hoy en día, la afirmación de que el mismo fenómeno gobierna el movimiento de los objetos en la Tierra y el movimiento de la luna alrededor de la Tierra fue revolucionaria en tiempos de Newton. Descubrió que la aceleración de la luna centrífuga alrededor de la Tierra y la aceleración debido a la gravedad tienen una relación inversamente proporcional al cuadrado de la distancia respectiva del objeto a la Tierra. Dado que la aceleración es independiente de la masa, según sus leyes del movimiento, la fuerza debe ser proporcional a la masa. Esta idea lo llevó a formular la ley de la gravitación que lleva su nombre. Otra información necesaria para completar la ley de gravitación de Newton era la constante gravitacional, que se derivó experimentalmente. El primer experimento exitoso para medir la constante fue llevado a cabo por Henry Cavendish. Una vez que se conocía el valor de esta constante, junto con las leyes del movimiento de Newton, se podían derivar las leyes del movimiento planetario de Kepler.

Fuerza gravitacional

En los años anteriores a Newton, prevalecía la creencia general de que leyes diferentes gobernaban los objetos en el cielo que los objetos en la Tierra. Cuando Kepler escribió el ...

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Education

Educación

JoVE Core

Mechanical Engineering

Ingeniería Mecánica

Unit 1

Unidad 1

Physics Basics

Conceptos básicos de física

KEY TERMS AND CONCEPTS

TÉRMINOS Y CONCEPTOS CLAVE

Gravitational Force

how gravity acts between objects

Gravity is a force that pulls objects toward one another. On Earth, this force gives objects weight and keeps people, water, and other materials from drifting away. It also helps explain why planets and moons stay in motion around larger bodies.

The strength of gravitational force depends on the masses of the objects involved. Larger masses create a stronger pull, while smaller masses create a weaker one. The distance between objects also matters, because gravity becomes weaker as objects move farther apart.

Students can use this relationship to understand motion in space and on Earth. Gravity acts between all objects with mass, even when the effect is hard to notice. That makes it an important force in both everyday life and the study of the solar system.

How Gravity Acts Between Objects

introduction to scalers

Scalar Quantities in Physics

Scalar quantities in physics have size only. They do not include direction. This makes them different from vector quantities. Common scalar examples include mass, temperature, time, and energy. Each one can be described with a number and a unit. Because direction is not part of the value, scalars are often easier to compare and measure.

vector or cross product

Cross Product of Two Vectors

The cross product of two vectors gives a new vector that is related to both original vectors. It is also called the vector product. In many physics problems, this operation helps describe quantities that depend on direction as well as size. The result of a cross product has a direction set by the two input vectors. It is not the same as ordinary multiplication. The transcript focuses on the vector or cross product as a core vector operation students use when working with vectors in science.

introduction to vectors

Vectors in Motion and Direction

Vectors describe quantities that have both size and direction. They are used in physics to show how motion, force, and other quantities act in space. A vector can be represented with an arrow. The length of the arrow shows the size, and the arrowhead shows the direction. This makes vectors useful for comparing how one quantity points relative to another. Scalars are different because they have size only and no direction. Understanding the difference between vectors and scalars is an important...

units and standards of measurement

Measurement Units, Standards, and SI Basics

Measurement units, standards, and SI basics help scientists describe physical quantities clearly. A unit gives a number meaning, while a standard provides a fixed reference for that measurement. Together, they make results easier to compare and understand. The International System of Units, or SI, is the most common measurement system in science. It uses agreed-upon base units for common quantities. These standards reduce confusion when measurements are shared across labs, classrooms, and...

accuracy and precision

Measurement Errors, Accuracy, and Precision

Measurement errors can affect how close a result is to the true value and how consistent repeated results are. Accuracy describes how close a measurement is to the accepted or true value. Precision describes how close repeated measurements are to one another. A result can be accurate, precise, both, or neither. A set of measurements may cluster tightly together and still be far from the true value. Another set may include values spread out from one another, even if one of them is close to the...

rules of significant figures

Counting Significant Figures in Measurements

Significant figures help students record measurements with the correct level of precision. They show which digits in a number are meaningful and which only help place the decimal point. In science class, this idea matters when writing and comparing measured values. The rules for significant figures explain how to count these digits in different numbers. Some digits are always counted, while others depend on where they appear in the number. Learning the rules makes it easier to report answers...

random and systematic errors

Measuring Error in Scientific Data

Random and systematic errors affect scientific measurements. Random errors cause values to spread around the true value. They make repeated measurements less consistent. Systematic errors shift measurements in the same direction each time. Understanding both kinds of error helps students judge data quality. Random error can come from small changes during measurement. Systematic error can come from a biased tool or method. Scientists look for these patterns so they can improve results and...

position and displacement

Tracking Motion with Position and Displacement

Position and displacement are key ideas in straight-line motion. Position tells where an object is located compared with a chosen starting point, called the origin. Displacement describes how far and in what direction the object has moved from its starting position. These ideas help describe motion clearly. Position can change as an object moves. Displacement focuses on the change in position, not just the path taken. That makes it useful for comparing motion in a simple and precise way.

position and displacement vectors

Using Vectors to Describe Motion

Position and displacement vectors describe motion in physics. A position vector shows where an object is located relative to a chosen origin. A displacement vector shows how far and in what direction the object moves from one point to another. These vectors are useful because they give a clear way to track movement in space. The video connects position and displacement to the idea of a reference point and shows how direction matters as much as distance. That makes them important for describing...

mass and weight

How Mass Differs from Weight

Mass and weight are related, but they are not the same. Mass is the amount of matter in an object. Weight is the force of gravity acting on that object. This difference matters because mass stays the same even when gravity changes. Weight can change if the gravitational pull changes. A person or object therefore has the same mass, but not always the same weight. The terms are often used in everyday speech as if they mean the same thing. In physics, they describe two different ideas.

acceleration due to gravity on earth

Free-Fall Acceleration on Earth

Free-fall acceleration on Earth describes how fast an object speeds up when gravity is the only force acting on it. Near Earth’s surface, this acceleration is nearly constant for many everyday situations. Gravity pulls objects toward Earth and gives them downward acceleration. This motion is often written as g, and it helps explain why falling objects gain speed as they move downward. The value of g is commonly used in physics to predict the motion of objects dropped or released near the...

tension

Tension in Ropes and Strings

Tension is the pulling force carried by a rope, string, or cable when it is stretched by a load. In physics, this force acts along the length of the object and pulls away from the objects at each end. A stretched rope can support a hanging mass because the tension in the rope balances the weight of the load. The same idea appears in many everyday situations, such as a cable holding a sign or a string lifting an object. Understanding tension helps students connect force diagrams to real motion.

gravitational force

Gravity is a force that pulls objects toward one another. On Earth, this force gives objects weight and keeps people, water, and other materials from drifting away. It also helps explain why planets and moons stay in motion around larger bodies. The strength of gravitational force depends on the masses of the objects involved. Larger masses create a stronger pull, while smaller masses create a weaker one. The distance between objects also matters, because gravity becomes weaker as objects move...

key terms and concepts

Learn how gravitational force depends on mass and distance, and how gravity affects weight, motion on Earth, and the movement of planets and moons.

How Gravity Acts Between Objects | JoVE K12

JoVE Core Mechanical Engineering offers concise, easy-to-understand animated videos covering key topics such as equilibrium, forces, truss analysis, and structural mechanics. Explore their real-world applications, and witness these concepts in action through scientist-led experiments.

mechanical engineering

How Gravity Acts Between Objects

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