Unit 1:  Our place in the Universe                                          1   2   3   4  

 

 

2. The origin of the Universe

 

2.1. First ideas about the Universe

Human being has felt always the necessity of explain the observed phenomena.

 

The early astronomers scrutinised the sky month after month as part of a religious ritual and observed that some stars seems to appear just before the sun and they set immediately after it.

 

They repeated their observations year after year and made measurements and annotations of the moments and positions in which these phenomena occur. Scientifics concluded that they repeated cyclically with each season. They realized that there was a big calendar written in the sky which allowed them to predict the favorable seasons to seed, hunt or navigate.

 

Babylonians sat the basis of the modern Astronomy. They described with precision the movement of the Sun, the Moon and the planets, they invented the sexagesimal system (the 3600 of the circumference) and established the Zodiac and the first calendars.

 

a) Geocentric model

    It is the simplest hypothesis to explain the movement of the celestial bodies

    and it considers our planet as the centre of the Universe.

    The observations which led to that conclusion were:

 

                     - The “fixed stars” and the Milky Way seems to move during the night

          like if they were joined to an invisible vault that was turning around

          a fixed point in the sky. First astronomers deduced that this celestial

          vault was similar to a huge sphere that surrounded the Earth.

 

                     - Other ones, however, did not behave like the stars. During part of the year

          they seemed to move forward and during other part backward.

          These celestial bodies were called planets.

 

    So that, according to the Geocentric model, the Earth, fixed and immobile,

    occupies the centre of the celestial sphere where are located the firmament,

    the Sun, the Moon, the planets and the fixed stars.

 

    Aristotle (384-322 B.C.) divided the Universe into two parts: the celestial

    and the terrestrial world. The terrestrial world was imperfect and it was

    formed by four elements: air, water, fire and earth. The celestial world,

    by contrast, was perfect and immutable. It was formed by the fifth element

    or quintessence, the ether (that means eternal) and its only movement

    has to be circular, because the circle is the perfect figure: it does not have end

    or beginning and it is equal in all its points.

 

    The Sun, the Moon, Venus, Mars and Jupiter were located in different

    transparent glass spheres, included ones in others and the Earth was in the centre.

    The stars were fixed and occupied the outermost sphere.

 

 

Animation: Aristotle's universe

 

In the II century A.C., Claudius Ptolemy (Egypt, 100-170 A.D.) published

the Almagesto. In it he stated that the Sun, The Moon and the five visible planets from the Earth (Mercury, Venus, Mars, Jupiter and Saturn) moved in their own transparent spheres describing circular movements.

 

Ptolemy solved the discrepancies between observations and the aristotelian model establishing the hypothesis that the planets describe small circular movements (epicycles) which centres move in a circular orbit around the Earth.

 

This model persisted until the XVI century and it became in the essence

of the Church’s dogma about the nature of the Universe. According to this, by divine design, the Earth was the immobile center of everything and the sky was the absolute perfection.

 


 

Animation: Ptolomy's universe


The astronomer Tycho Brahe (Denmark, 1546-1601) refused the idea of the existence of glass spheres that transport the planets after study the trajectories of comets and check that they moved out of them.

 

Besides, he concluded that the skies were no immutable after observe in 1572, the emergence of a supernova.

 

To explain the planetary movement, he proposed a geocentric model in which the planets turn around the Sun and this one and the Moon turn around the Earth. This was the last attempt to maintain the geocentrism.

Video: Tycho Brahe

 

b) Heliocentric model

The first heliocentric model was proposed in the 2nd century B.C

by Aristarcus of Samos (Greece, 310-230 B.C.).

 

In this model the Earth and the rest of the planets revolved around the Sun

and the Moon revolved around the Earth. In addition, he defended that the Earth rotated around itself each 24 hours and it revolved around the Sun once a year. However, his theories found an unbridgeable opposition among the Greek philosophers and they never were accepted.

 

Most part of the early Grecian scientists’ works was lost during the fire of the Alexandria’s library and its knowledge was vanished. Only a small part of them

arrived to Occident through the Arabian culture.

 

During all the Middle Age the geocentric theory was supported, because it was

very well accepted by the ecclesiastical power. It was coherent that the creatures created by God inhabited the planet Earth that was located in the Centre of the Universe. What was no more than a mathematic instrument became in faith dogma. Others hypothesis were considered heresies and their authors condemned to the fire.

 

A cover of darkness and ignorance was extended by the world, and the ideas of many wisdom men and women were refused and set aside, being substituted by absurd and inconsistent models that however were according to the Sacred Scriptures.

 

 

Nicolaus Copernicus (Poland, 1473-1543),

polish astronomer, collected his observations

in his book “About the celestial spheres revolutions”.

In this work, Copernicus, stated that the Earth

rotates around its own axis once a day.

Basing in this idea, he discovered that the

complex orbits described by Ptolemy can be

simplify if the sun was considered the centre

of the universe instead of the Earth.

That is to say, the Earth and the rest of

the planets revolved around the Sun.

 

However, although the Copernican model was simpler and more systematic than the Ptolemy one,

he still held the idea than the planets described a circular orbit and the existence of the epicycles.

 

Fearing the ecclesiastical reprisals, Copernicus kept his discovery in secret and he only publish it when he was next to die.

 


Giordano Bruno (Italy, 1548-1600) was one of the first to accept and spread the heliocentric model of Copernicus. Following the logical thought that there must be an infinite number of worlds, he also proposed that there must be life in other parts of the Universe. These ideas, counter to Church’s ones, cost him his life. He was burned in the stake after pass 8 year imprisoned.

 

Video: Giordano Bruno

 

 

In 1610, the mathematician Joannes Kepler (Germany, 1571 – 1630) used the Tycho Brahe’s exhaustive data and adapted the Copernicus’ theory to a planetary system with elliptical orbits.

 

He discarded the idea of the uniform movement and supposed that the velocity of the planets varied with their distance to the Sun. His theories, true for every object in orbit around a star were established in the three laws of the planetary movement or Laws of Kepler. But again the scientific knowledge crashed with the religious fanaticism and the Kepler’s work was prohibited by the Catholic Church.

 


Galileo Galilei (Italy, 1564-1642) discovered the phases of Venus using a telescope made by himself in 1610, demonstrating that it revolved around the Sun and that the Copernicus’ theory was true. He also discovered the four main satellites of Jupiter. Besides, he studied the sunspots and the Milky Way. 

 

In 1632 his book “Dialogue between the two great systems of the world” was published. In it he defended the heliocentric theory of Copernicus. The reaction of the Catholic Church was again immediate and Galileo was obliged to retract.

 


From the discoveries of Copernicus, Galileo and Kepler, Isaac Newtons (England, 1643-1727) write his work “Mathematic principles of natural philosophy”.

 

In it he formulated the theory of the universal gravitation, a set of scientific laws that explain the movement of the celestial bodies, the fall and weight of bodies, the movement of satellites, the movement and periodicity of the tides

and the trajectory of the comets.

 

Since this moment the heliocentrism was universally accepted.

Video: Isaac Newton

Animation: Astronomy timeline (NASA)

READING ACTIVITIES

                                                                                          

After reading the text, copy and answer the following questions into your notebook:

2.1. Relate each concept or discovery with the scientist who proposed it or made it:

    

a. Epicycles

b. Phases of Venus

c. First calendars

d. The planets move faster when they are near the Sun.

e. The existence of life beyond the Earth

f. The Earth rotates on its axis each 24 h.

g. The Sun is the center of the Universe.

h. The skies are neither immutable nor static.

i. The way celestial bodies move.

j. The Universe of transparent glass spheres.




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2.1. First ideas about the Universe CMC
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