- 107 Views
- Uploaded on
- Presentation posted in: General

Lecture 2 The Solar System The Universal Gravitation

Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author.While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server.

- - - - - - - - - - - - - - - - - - - - - - - - - - E N D - - - - - - - - - - - - - - - - - - - - - - - - - -

Chapter 1.3 1.11

Homework: On-line quiz for Chapter 1 (due August 27th)

Outline

- What we see in the sky
- The Ptolemaic system
- The Copernican system, Kepler’s laws
- Universal gravitation

Patterns of stars seen in the sky

There are 88 constellations

About 50 of them were named by ancient Greeks and Romans

Relations of celestial objects to weather and agriculture

Observations of the Sun and Moon

Observations of stars and planets

Developed by Claudius Ptolemy (A.D. 100-170)

The Earth is in the center

The Sun is at the third orbit from Earth after Mercury and Venus

Epicycles are added to circular orbits of planets to explain retrograde motion

The Ptolemaic model along with a catalog of positions of 1028 stars were published in his book Almagest

Copernicus is said to be the founder of modern astronomy

- Planets move on elliptical orbits
- 2. The planet’s radius-vector sweeps out the same areas in equal times
- 3. The squares of the periods of the planets are proportional to the cubes of their semi-major axes

Demonstration of Kepler's laws

Content:

Sun (the only star)

9 planets

Nearly 100 moons

Asteroids

Comets

Free-flying gas and ``dusty’’ particles

http://solarviews.com/eng/homepage.htm

Every mass attracts every other mass through the force called gravity

The force of attraction is directly proportional to the product of their masses

The force of attraction is inversely proportional to the distance between the objects

Fg = G x M1x M2 / d2

gravity

Newton found that Kepler’s first two laws apply not only to planets, but to any object going around another one under the force of gravity

The orbits do not have to be elliptical

They can also be parabolic or hyperbolic

Tides are due to gravitational attraction between the Earth and the Moon

The tidal bulges try to stay on the Earth – Moon line

The Earth’s rotation tries to pull the bulges around

The tidal friction slows down the Earth’s rotation

The length of a day gets longer

It makes the Moon move further away from Earth

The Moon is in synchronous rotation with the Earth

(always showing the same face)

In 1781, the planet Uranus was discovered telescopically

from Britain by William Herschel.

In 1845, a Cambridge mathematician, John Couch Adams, based on the law of gravitation, predicted the existence of an unseen planet, to account for the fact that Uranus was being pulled slightly out of position in its orbit.

He sent the calculations to test to England’s Royal Astronomer, who set them aside.

Shortly after that, a French mathematician, Urbain Leverrier,published a similar prediction and contacted astronomers at Berlin Observatory, who found the new planet on the night of 23 September 1846.

Astronomy is a science

It describes the real world, sets new problems and solves them, using methods of itself and other sciences (such as physics and mathematics)

Astrology is interpreting apparent positions of the Sun, planets, and stars to predict human life.

It does not set and solve any problem

The Earth is not the center of the universe but instead is a planet orbiting a rather ordinary star in the Milky Way Galaxy.

- Celestial bodies in the gravitational field of each other move according to Kepler’s laws.

- Newton’s discoveries showed that the same physical laws we observe on Earth apply throughout the Universe.