Динамика - Ньютон заңдары

<p>F = G * (m1 * m2) / R^2 (C)</p> Signup and view all the answers

<p>Модулі жағынан тең, бағыты жағынан қарама-қарсы (C)</p> Signup and view all the answers

<p>Қозғалысқа кедергі көрсетуінен (D)</p> Signup and view all the answers

<p>Жердің массасы мен радиусына байланысты (B)</p> Signup and view all the answers

<p>≈ 7,9 км/с (C)</p> Signup and view all the answers

<p>≈ 11,2 км/с (A)</p> Signup and view all the answers

<p>6,67∙10^-11 Н∙м²/кг² (A)</p> Signup and view all the answers

An object at rest stays at rest and an object in motion stays in motion with the same speed and in the same direction unless acted upon by an unbalanced force.

The acceleration of an object is directly proportional to the net force acting on it and inversely proportional to its mass.

For every action, there is an equal and opposite reaction.

The resistance of any physical object to any change in its state of motion.

A measure of an object's inertia.

Any interaction that, when unopposed, will change the motion of an object.

The force of attraction between all masses in the universe.

The more massive the objects, and the closer they are, the stronger the gravitational force.

The acceleration of an object falling freely near Earth's surface.

The speed needed to maintain a stable orbit around a planet or star.

The speed needed to escape a planet's gravitational pull.

The speed needed to escape the Solar System.