Category Astronomy

What are the rings of the Saturn?

               Saturn is the second largest planet of the Solar System. On the basis of the distance from the Sun, this is the sixth planet. Its distance from the Sun is 1,427 million km. Its intense brightness is due to its bigger size. It keeps on revolving round the Sun and takes about 291  years to complete one revolution. It has seventeen moons revolving round it. It appears yellow in colour. It is 96 times heavier than the Earth, while its volume is 743.7 times more than that of the Earth.

               Saturn is the most peculiar of all the planets. Its peculiarity lies in the rings surrounding it. These rings are not visible to the naked eyes but can be seen very clearly with the help of telescopes. In July, 1610 when Galileo studied it with the help of his telescope, he saw some unknown materials stuck to this planet on all sides. In 1655, a scientist named Christian Huygen discovered with the help of a powerful telescope that Saturn is surrounded by a ring which does not touch its main body at any point.

               With the help of powerful telescopes, three rings are seen very clearly. In 1969 scientists discovered a fourth ring also. The four rings of Saturn are called A, B, C, and D rings. The total width of these rings is about 274,000 km. which is twice the diameter of Saturn. Scientists are of the view that these rings might have been formed by minute particles of dust and ice.

                The outermost ring A which is somewhat brighter has its outer diameter to be 274,000 km. and its inner diameter to be 2, 38,400 km. Its width is about 16,000 km. The distance between A and B rings is 4,000 km. The B ring is the brightest. Its outer diameter is 2, 30,400 km, and the inner diameter is 1, 79,200 km. Its outer part is brighter than inner part. Its width is about 25,600 km. The distance between B and C rings is about 960 km. The C ring is not bright. Its outer diameter is 1, 77,600 km and whereas the inner diameter is 1, 43,920 km. The fourth is the D ring. This is very dim and hence it is difficult to locate its boundaries.

               All these rings appear elliptical. From the earth, all these rings appear to be connected with each other. Of all the planets Saturn is the only planet which has such rings.

What is Moon – the only satellite of the Earth?

            The Moon is a heavenly body. Any heavenly body that revolves round a planet is called its satellite. The Moon revolves round the Earth. Therefore, it is called a satellite of the Earth.

            The Moon is the only satellite on which man has landed. On July 20, 1969, Neil Armstrong, an American astronaut, succeeded for the first time in landing on the Moon’s surface in Apollo 11 flight and unravelled many mysteries about it. In this very flight, a retro-reflector was mounted on the Moon’s surface. Laser beams sent from the Earth’s surface and reflected back by this retro-reflector enabled scientists to calculate the exact distance of the Moon from the Earth. The distance so calculated has an accuracy of less than 15 cm. The distance has been calculated to be 3, 84,400 km.

            The Moon is a solid spherical body like a football. It completes one revolution round the Earth in an elliptical path in a period of 29 days 12 hours and 43 minutes. We call this period a lunar month. Only one side of the Moon is always visible to us because the period of its rotation on its axis is approximately the same as the period of its revolution round the Earth.

           The Moon does not have its own light but shines due to the Sun-light. Ten percent of the Sun’s light falling on the Moon is reflected by its surface while the rest is absorbed by it. During noon, the surface temperature of the Moon is about 130°C, while, during the night, it is very cold. The Moon’s surface is very uneven. There are mountains, valleys and black plains on the Moon’s surface. These black portions appear as lunar spots. There are heaps of ashes on its surface caused by the fall of meteors. The diameter of the largest crater on the Moon is 232 km which is 365.7 metres deep. Studies on the samples of rocks collected from the Moon’s surface have revealed that they contain metals like aluminium, iron, magnesium etc. The lunar surface contains silicates also. The Moon does not have air and water and, therefore, there are no signs of life there.

             The average distance of the Moon from the Earth keeps on changing slightly because of the Moon’s elliptical orbit. The diameter of the Moon is approximately 3476 km. It rotates on its axis with a speed of 3430 km per hour. The Earth is about 81.3 times heavier than the Moon and 49 times larger in volume. The force of gravity on the Moon is one-sixth that of the Earth. Scientists are making constant efforts to obtain more and more information about the Moon.

 

How distant are stars from us?

            Billions of stars which we see in the sky every night are made up of hot gases. Even the Sun is a star. However, there are stars which are million times more shining than the Sun, but they don’t appear so because of their greater distances from the earth. The stars are of varying sizes.

            We measure the distance of stars in units of light years. A light year is the distance travelled by light (its velocity being 3 x  km or 3 hundred thousand km per second) in one year. The star nearest to the earth (other than the Sun) is Proxima Centauri. Its distance from the earth is 4.28 light years. This star is visible only in the Southern Hemisphere. The nearest star visible in the Northern Hemisphere is Sirius. Its distance from the earth is 8.8 light years. In addition to this, another neighbouring star is Alpha Centauri which is 4.37 light years away from us.

            The farthest star from the earth which is visible with our naked eye is more than eight million light years away from us. If we use powerful telescopes, we can even see stars that are 1000 times more distant than this one. Some stars are so far away from the earth that light from them takes more than 1,000 million years to reach the earth.

            Scientists have developed various kinds of optical and radio telescopes to study stars. They have gained considerable knowledge relating to the heavenly bodies with the help of these telescopes. 

What is the Zodiac?

            In ancient times, when people looked up at the sky in the night, they observed many bright stars arranged in a certain pattern or group. Each group is called a constellation. It means a group of stars. Studies of movements of these constellations led to the discovery that they move in space in fixed directions. The number of constellations visible during the year at different times was found to be 12. The Sun and the Moon were always seen rising and setting in the same directions in which these twelve constellations were located. These 12 constellations were called the signs of the zodiac.

            The hypothetical part of the sky through which the Sun, the Moon and other planets seem to be passing is called the zodiac. Each of the 12 constellations situated at an angle of 30°, is named as a different sign of the zodiac. In this way the 12 signs of the zodiac have come into existence. Each sign is connected with one constellation and the shape of each constellation resembles certain earthly body or substance. The names of these signs and the position of the Sun are as follows:

  1. Aries: The Ram – 21 March to 19 April
  2. Taurus: The Bull – 20 April to 20 May
  3. Gemini: The Twins – 21 May to 21 June
  4. Cancer: The Crab – 22 June to 22 July
  5. Leo: The Lion – 23 July to 22 August
  6. Virgo: The Virgin – 23 August to 22 September
  7. Libra: The Balance – 23 September to 23 October
  8. Scorpio: The Scorpion – 24 October to 21 November
  9. Sagittarius: The Archer – 22 November to 21 December
  10. Capricorn: The Goat – 22 December to 19 January
  11. Aquarius: The Water Bearer – 20 January to 18 February
  12. Pisces: The Fish – 19 February to 20 March

     

Continue reading “What is the Zodiac?”

What is lunar eclipse?

            When we stand in the sunlight, the rays of the Sun fall on us and we can see our shadows. Exactly like this, shadows of the Earth and the Moon are also formed in the space due to the Sun rays falling on them. Since the Earth and the Moon are spherical in shape, their shadows are conical in shape. These shadows are very long. The larger the distance of a body from the Sun, the longer will be its shadow. Lunar eclipse is darkness on the Moon due to the Earth’s shadow over a portion of it.

          While making their revolutions, the Sun, the Earth, and the Moon come in a straight line and the Earth sometimes comes in between the Sun and the Moon, thus the shadow of the Earth falls on the Moon. In other words, the Sunlight does not fall on the Moon when the Earth comes in between the two. The portion over which the shadow falls becomes dark. This is called lunar eclipse. Such a situation occurs only on Purnima (full Moon) days. Therefore, the lunar eclipse takes place only on that day. If the Earth’s shadow covers the entire Moon, it is total lunar eclipse. If the shadow covers only a part of the Moon, it is partial eclipse. Generally, there are three lunar eclipses in a year, out of which one is a total lunar eclipse.

             Now the question arises: when the full Moon comes every month, why does lunar eclipse not take place every month? The reason is that the plane of the Moon’s orbit makes an angle of 5° with the plane of the Earth’s orbit. Consequently, the Moon revolves either above or below the Earth’s shadow. So, it is only twice or thrice a year that all the three – the Sun, the Moon, and the Earth – come in one straight line. Hence the lunar eclipse does not take place every month. Astronomers, using mathematical calculations, easily predict the time and duration of the lunar eclipse.  

Could you ever see an eclipse of the Moon in daylight?

Yes, though only for a few minutes, and only if the eclipse is occurring just as the Moon is rising and the Sun is setting, or the Moon is setting and the Sun rising. A total eclipse occurs when the Earth is between the Moon and Sun, which are directly opposite to each other in the sky.

 Seeing both the Sun and eclipsed Moon at the same time would appear to be a geometrical impossibility, but because the atmosphere has a lensing effect, it raises the images of both the rising Moon and setting Sun above the horizon for a few minutes.

For the same reason, day and night are not exactly equal at the time of the fall equinox, because the day is artificially lengthened a few minutes at each end by the refractive effect of the atmosphere, for a total of seven minutes. It is not until three or four days later that the day equals the night.

It is easier to see the scallop of a partial eclipse above the horizon at sunrise or sunset than it is to see a total eclipse, because the Sun is so much brighter than the Moon.