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THE SOLAR SYSTEM

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The sun has a family of nine planets moving around it due to its gravity. Along with these planets the solar system has comets, asteroids, planetoids, and moons orbiting around planets.

HISTORY

Science and our view of the world change only when we are presented with some observation we can't explain. Early Greek philosophers believed that Earth was at the center of the Universe and all other celestial bodies moving around it. Eudoxus, a mathematician who lived in the fourth century B.C., was one of the first people to propose this theory. Eudoxus’ version of the theory was elegantly simple: God is perfect, the only perfect forms are circles, therefore the Sun and planets must move in circles around the Earth. Claudius Ptolemy, a Greek scholar who lived in Alexandria, Egypt, around 140 AD noted that there were some problems with the theory, however. Careful observations showed that the planets did not quite move in perfect circles. Faced with an observation that couldn’t be explained with current theories, Ptolemy modified Eudoxus’ theory and replaced his simple circles with a complicated system of "epicycles", circles that interlock like gears in a complex machine. Ptolemy’s theory could describe and predict the motions of the planets with an accuracy never before achieved. For almost 1,400 years, until the 16th century, Ptolemy’s theory was considered to be the only theory was considered to be the only correct theory of the Universe. The theory was endorsed by the Catholic Church, which declared any other explanation for the planets’ motions to be heresy and punishable by death.

Ptolemy’s theory only had one problem:it was wrong. One hundred years after Eudoxus, the astronomer Aristarchus watched the shadow of the Earth sweep across the surface of the Moon during a lunar eclipse. His observations showed that the Sun had to be much larger than the Earth, and he felt that it was not likely that a large Sun would rotate around the smaller Earth. He proposed instead that the Earth revolves around the Sun. He was condemned for heresy because of his theory and all of his writings were rounded up and destroyed. The only reason we know anything about Aristarchus at all is because he is mentioned inthe writings of great mathematician Archimedes. No other scientist was willing to risk the wrath of the church by mentioning the astronomer's work. In 1953, nearly 2000 years later, however, Aristarchus' theory was taken up by Polish doctor, lawyer and part-time astronomer Nicolaus Copernicus.Copernicus' careful observations could not be explained by Ptolemy's theory. Only if the sun were at the center of the SOLAR SYSTEM could this data make sense. Once again, because of new observations, new science and a new worldview was born.

But Copernicus' theory still could not explain the strange motion of Mars. In 1600 Tycho Brahe had undertaken the careful study of Mars' orbit. Tycho was perhaps the greatest observational astronomer the world has ever known. We can make more accurate observations today only because we have more accurate instruments. Tycho was world famouswho toured the palaces of Kings and other nobility all over Europe. Tycho had given his student, a German mathematician named Johannes Kepler, the task of creating a mathematical description of Mars' orbit. Tycho, however,  was very protective of his data, as are many scientist today. He would throw out an observation over dinner in casual conversation, which Kepler would frantically scrawl down in a notebook that he kept under the table. When Tycho finally died several years later, Kepler broke into tycho's safe and stole all of his data. Tycho's family demanded the documents to be returned, and Kepler did so- but only after he had made exact copies of all the precious data. Kepler, like most of his fellow scientists, felt certain that the planets traveled in perfect circles. After years of struggling with Tycho's observation of Mars, however, he finally reached  the inescapable conclusion that all the work done before him was wrong: the planets move in ellipses, not circles. In addition, he discovered two other laws of planetary motion that he published in 1609. Thanks to Mars, we now understood not only its motion but the motion of the entire SOLAR SYSTEM as well.

SOURCE-JPL(NASA) & ASU.

 

DATA ON PLANETS OF THE SOLAR SYSTEM

 

Mercury

Venus

Earth

Mars

Jupiter

Saturn

Uranus

Neptune

Pluto

Distance from the sun(AU)

0.387

0.723

1

1.524

5.203

9.537

19.191

30.069

39.481

Approximate distance from the sun(103  km)

57,910

108,200

149,600

227,940

778,400

1,429,725

2,870,980

4,498,250

5,906,370

Radius

2,439.7

6,051.58

6,378.14

3,397.2

 

71,492

 

60,268

 

25,559

 

 

24,764

 

1,195

 

Mass (Earth = 1)

 

0.054

 

0.88

 

1

 

0.149

 

1,136

 

755

 

52

44

0.005

Density (gm/cm3)

 

5.43

 

5.24

 

5.515

 

3.94

 

1.33

 

0.70

 

1.30

 

1.76

 

1.1

 

Rotation Pe riod (day length)

 

58.65

 

-2 43.02

 

0.99

 

1.03

 

0.41

 

0.44

 

-0.7 2

 

0.67

 

-6.39

 

Orbital Period (year in days)

 

88

 

225

 

365

 

687

 

4,333

 

10,760

 

30,685

 

60,190

 

90,800

 

Sideral period ( length of years in earth years)

0.24

 

0.62

 

1

 

1.88

 

11.86

 

29.42

 

83 .75

 

163.72

 

248.02

 

Orbital Tilt (degree s)

0

 

177.3

23.45

25.19

3.12

26.73

97.86

29.58

119.61

Satellites

0

0

1

2

16+(15+)

18

15

8

1

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

 

SOURCE-JPL(NASA) & ASU.

Glossary 

AU - astronomical unit, the distance between Earth and Sun (~1.495 x 108 km).

Rotation Period - the length of the day.

Orbital Period - the length of the year in Ea rth days.

Retrograde - when a celestial body rotates in the opposite direction of the Earth or clockwise.

Satellite - another name for a moon.

Sideral Period - the length of a planet’s yea r in Earth years.

Tilt - how a far a planet is tilted sideways on its axis, measured in degrees. 

Related LINKS

Comets

Planets;  

Asteroids, Asteroid belts and NEOs ; Kuiper belt (beyond Pluto) ; Oort cloud objects ; Asteroid belt(Between Mars and Jupiter)

Sun , Solar flares, Sun spots

Moons 

Space missions

Destination Mars ; Mars Researches: Human mission

Venus transit

Pictures

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