Physics: Gravitation and Planetary Motion

0.0(0)
Studied by 0 people
call kaiCall Kai
Locked
learnLearn
examPractice Test
spaced repetitionSpaced Repetition
heart puzzleMatch
flashcardsFlashcards
GameKnowt Play
Card Sorting

1/14

flashcard set

Earn XP

Description and Tags

A set of vocabulary flashcards covering the concepts of orbital mechanics, Kepler's laws, and Newton's Universal Law of Gravitation based on the provided lecture notes.

Last updated 3:50 PM on 6/28/26
Name
Mastery
Learn
Test
Matching
Spaced
Call with Kai
Chat

No analytics yet

Send a link to your students to track their progress

15 Terms

1
New cards

Centre of mass

The point inside or outside an object at which the total mass of the object can be assumed to be concentrated.

2
New cards

Geometrical centre

The location of the centre of mass for a spherical object having uniform density.

3
New cards

Centroid

The location of the centre of mass for any object having uniform density.

4
New cards

Centripetal force

A force acting on an object moving in a circle that is directed towards the centre of the circle, expressed as F=mv2rF = \frac{m v^2}{r}.

5
New cards

Kepler's first law

The orbit of a planet is an ellipse with the Sun at one of the foci.

6
New cards

Kepler's second law

The line joining the planet and the Sun sweeps equal areas in equal intervals of time.

7
New cards

Kepler's third law

The square of the period of revolution of a planet around the Sun is directly proportional to the cube of the mean distance of the planet from the Sun, such that T2r3=K\frac{T^2}{r^3} = K.

8
New cards

Ellipse

A curve obtained when a cone is cut by an inclined plane; it has two focal points where the sum of the distances from every point on the curve to these points is constant.

9
New cards

Newton's universal law of gravitation

Every object in the Universe attracts every other object with a force directly proportional to the product of their masses and inversely proportional to the square of the distance between them: F=Gm1m2d2F = G \frac{m_1 m_2}{d^2}.

10
New cards

Universal gravitational constant (G)

The constant of proportionality in Newton's law of gravitation; in SI units, its value is 6.673×1011Nm2kg26.673 \times 10^{-11} N m^2 kg^{-2}.

11
New cards

Henry Cavendish

The scientist who first experimentally measured the value of the Universal gravitational constant (GG).

12
New cards

Johannes Kepler

A German astronomer and mathematician (1571-1630) who used the observations of Tycho Brahe to discover the three laws of planetary motion.

13
New cards

Sir Isaac Newton

The English scientist (1642-1727) who formulated the laws of motion, the theory of gravity in his book Principia, invented calculus, and constructed the first reflecting telescope.

14
New cards

Calculus

A new branch of mathematics invented by Newton with wide ranging applications in physics and mathematics.

15
New cards

Centripetal (meaning)

A term meaning 'centre seeking,' indicating that an object moving in a circle tries to go towards the centre of the circle because of this force.