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

Die Umdrehung des Mondes um die Erde deutet auf das Vorhandensein einer Kraft hin, die ihn in Richtung des Zentrums der Umlaufbahn zieht.
Issac Newton schlug vor, dass diese Anziehungskraft die gleiche ist wie diejenige, die einen Apfel zum Boden zieht.
Es war eine revolutionäre Idee, da man glaubte, dass Himmelsobjekte und Objekte auf der Erde unterschiedlichen Regeln folgen.
Der Mond braucht 27,3 Tage, um die Erde zu umkreisen. Unter Berücksichtigung der durchschnittlichen Entfernung zum Mond kann seine Beschleunigung abgeschätzt werden. 
Das Verhältnis der Mondbeschleunigung zur Beschleunigung eines auf die Erde fallenden Objekts zeigt an, dass die Beschleunigung umgekehrt proportional zur Entfernung zum Quadrat ist.
Da Kraft Masse mal Beschleunigung ist, ist die Gravitationskraft direkt proportional zur Masse und umgekehrt proportional zur Entfernung zum Quadrat.
Newton beobachtete, dass die Beschleunigung von Planeten umgekehrt mit ihrer Entfernung von der Sonne abnimmt, und sagte voraus, dass die Gravitationskraft zwischen der Sonne, den Planeten und ihren Monden wirkt.
Indem er dieses Argument auf alle Objekte im Universum ausdehnte, formulierte Newton das Gesetz der universellen Gravitation.

<ol>
	<li>Verma, H.C. (2008). Konzepte der Physik. Band 1, Bharati Bhawan Pub. & Dis.: Abschnitte 11.1 und 11.2; Seiten 203–204.</li>
</ol>

gravitationskraft

In den Jahren vor Newton herrschte der allgemeine Glaube, dass Objekte am Himmel anderen Gesetzen unterliegen würden als Objekte auf der Erde. Als Kepler die drei Gesetze der planetaren Bewegung aufschrieb und detailliert die geometrischen Eigenschaften der Planetenbahnen um die Sonne erklärte, gab es keine unmittelbare Idee, ihren Zusammenhang mit grundlegenden Gesetzen zu erkennen. Es war Isaac Newton, der in den Jahren 1665-66 den Zusammenhang zwischen der planetaren Bewegung, der Bewegung des Mondes um die Erde und dem alltäglichen Phänomen von Objekten, die auf die Erdoberfläche fallen, herausfand. Dieses universelle Phänomen ist heute als Gravitation bekannt.

Obwohl es heute selbstverständlich klingt, war die Aussage, dass das gleiche Phänomen die Bewegung von Objekten auf der Erde und die Bewegung des Mondes um die Erde regelt, in Newtons Zeiten revolutionär. Er fand heraus, dass die Beschleunigung des zentripetalen Mondes um die Erde und die Beschleunigung aufgrund der Schwerkraft ein Verhältnis haben, das proportional zum Quadrat des jeweiligen Abstands des Objekts von der Erde ist. Da die Beschleunigung unabhängig von der Masse ist, muss nach seinen Bewegungsgesetzen die Kraft proportional zur Masse sein. Diese Erkenntnis führte ihn zur Formulierung des nach ihm benannten Gravitationsgesetzes.

Eine weitere Information, die benötigt wurde, um das Gravitationsgesetz von Newton zu vervollständigen, war die experimentell abgeleitete Gravitationskonstante. Das erste erfolgreiche Experiment zur Messung der Konstante wurde von Henry Cavendish durchgeführt. Sobald der Wert dieser Konstante zusammen mit Newtons Bewegungsgesetzen bekannt war, konnten Keplers Gesetze der planetaren Bewegung abgeleitet werden.

Gravitationskraft

In den Jahren vor Newton herrschte der allgemeine Glaube vor, dass Objekte am Himmel andere Gesetze regeln als Objekte auf der Erde. Als Kepler die ...

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Lehre

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Mechanical Engineering

Maschinenbau

Unit 1

Einheit 1

Physics Basics

Grundlagen der Physik

KEY TERMS AND CONCEPTS

KERNBEGRIFFE UND KONZEPTE

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.

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How Gravity Acts Between Objects

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