Tuesday, November 20, 2018

Astronomical Instruments in SPS Museum Srinagar


Heritage week is celebrated throughout world to conserve and appreciate ones history and culture. The department of Archives, archeology  and museums is also celebrating heritage week from 19-25 November by public display of rare manuscripts and medieval astronomical instruments like astrolabe and celestial globe. There are four astrolabes and one celestial globe on display in SPS museum during heritage week. Three of  the astrolabes have Sanskrit inscriptions and the only Indo-  Persian astrolabe is most elaborate. It is crafted by Ḍiyā al-Dīn Muḥammad  of prolific Allahdad family of Lahore in the year 1666 CE. All Sanskrit Astrolabes have been crafted by another prolific metallurgist Lala Bullohmal Lahori although they are not signed by him. The only celestial globe on display has also been crafted by  Lala Bullohmal Lahori. All these instruments have been crafted of brass of various compositions. The SPS museum possess few more traditional astronomical instrument like wooden celestial globe, a metallic gazetteer and a  wooden mater of an astrolabe. There are no information about these instruments in the museum such as from where and when they have been accessed. However several International researchers have studied these or similar instruments and catalogued few of them. Three of the instruments in SPS museum's collection are  unique and rare.
The astrolabe is an ancient astronomical instrument/ analogue computer. Astrolabe is a very versatile  instrument. It was first designed by Greeks to measure the altitude of a heavenly body. It was used to ascertain position of celestial bodies like Sun, Moon, planets and stars in the sky. It was also used for measuring height and distances in land surveys. It can also be used to simulate the motion of heavenly bodies at any locality and time. In fact it can also be used to measure time. The design, manufacture and applications of astrolabes were improved by Arabs in middle ages. It was used to calculate the Qibla and to find the times for Salah.
Several types of astrolabes have been made since antiquity. The most popular type is the planispheric astrolabe, on which the celestial sphere is projected onto the plane of the equator. A typical astrolabe was made of brass and was about 6-10 inches in diameter, although much larger and smaller ones were also made. An astrolabe consists of a disk, called the mater (mother), which is deep enough to hold one or more flat plates called tympans, or climates. A tympan is made for a specific latitude and is engraved with a stereographic projection of circles denoting azimuth and altitude and representing the portion of the celestial sphere above the local horizon. The rim of the mater is typically graduated into hours of time, degrees of arc. Above the mater and tympan, the rete or ankabut, a framework bearing a projection of the ecliptic plane and several pointers indicating the positions of the brightest stars, is free to rotate. The rete, representing the sky, functions as a star chart. When it is rotated, the stars and the ecliptic move over the projection of the coordinates on the tympan. One complete rotation corresponds to the passage of a day. On the back of the mater there is often engraved a number of scales that are useful in the astrolabe's various applications; these vary from designer to designer, but might include curves for time conversions, a calendar for converting the day of the month to the sun's position on the ecliptic, trigonometric scales, and a graduation of 360 degrees around the back edge. The alidade is attached to the back face. When the astrolabe is held vertically, the alidade can be rotated and the Sun or a star sighted along its length, so that its altitude in degrees can be read from the graduated edge of the astrolabe. The concept of astrolabe was introduced in India by noted polymath Alberuni through his writings. The medieval rulers Firoz Shah Tughlaq and Humayun patronized astronomy. During Mughal period some finest astrolabes were manufactured in Lahore. The Indo persian astrolabe in SPS museum has been designed and crafted in Lahore. It consists of  body with kursī shackle and ring, rete for 51 stars, 10 plates, alidade, pin and washer. There are ten plates serving the latitudes 11° to 45° at 2° intervals and the ecliptic coordinates and multiple horizons. Of the three Sanskrit astrolabes in the possession of SPS museum one is ordinary in the sense that similar astrolabe is extant in Rampur Raza library also. The two astrolabes which have solid retes are unique. No such sample is extant anywhere except SPS museum. Noted Scholar SR Sarma has attributed these two to Lala Bulhomal Lahori.
A celestial globe is a three dimensional model of the sky. It was mostly used for  pedagogical purpose rather than an observational instrument like astrolabe. The celestial globe has the advantage of simplicity of design and the ability to function at any geographic location. A hollow celestial globe can either be made in two hemispheres and joined or they can be casted seamlessly in single piece using lost wax technique. The earliest confirmed date for the manufacture of a seamless cast globe is 1589-90 CE, when a globe made by 'Ali Kashmirl ibn Luqman' was produced. The technology of  casting of seamless celestial globe was transferred from Kashmir to Lahore and Allahdad family and Lala Bulhomal also practiced the same technology. There are about 20 extant globes in the world crafted using the technique of lost wax. Even present day copper metallurgists of Kashmir use similar wax inside their copper bowls to provide rigidity while carving designs.
There are no constellation figures on the  globe at SPS museum,  the positions of some prominent stars like Suhel are marked with inlaid silver nails. Unlike in other globes by Bulhomal, there are no meridian circles here. The globe is mounted on a three-legged stand. The stand consists of an ornate horizontal ring, a meridian ring and a zenith ring without a crown. Both the horizontal and meridian rings are graduated in 1° and 6° and labelled in Abjad notation. An axis passing through the two celestial poles on the globe is pivoted to the meridian ring in the stand. The curved legs are decorated with a leaf pattern.
SPS museum also possess a unique Safvid qibla indicator. On the two outer and the two inner side of the qibla indicator, the geographic information  is engraved in  annular circles, carrying the names, longitudes and latitudes of many localities arranged according 6, 12, 18, 24, 30 degree lattitudes, the numbers starting from the equator and reaching to the tropics. There is an urgent need to do a scientific study of all these astronomical instruments to know the history of science in this region.

Thursday, August 30, 2018

Longest Lunar Eclipse


An spectacular lunar eclipse will be taking place during the night of 27-28 July.  If weather permits, the entire cosmic event will be visible from Srinagar and other parts of the state. The penumbral eclipse will begin at quarter to eleven in night and end after Fajr, making it longest eclipse of the century.  The total eclipse will begin at quarter past one and end at quarter to three.  In the night of the eclipse, full moon is also at its farthest from the earth (Apogee) so it will look relatively smaller in the sky hence it is called micro moon in contrast to supermoon when it appears largest.
 A lunar eclipse occurs when the Moon passes behind the Earth so that the Earth blocks the Sun's rays from striking the Moon. This can occur only when the Sun, Earth, and Moon are aligned exactly, or very closely so, with the Earth in the middle. Hence, a lunar eclipse can only occur during the night of a full moon. It might be expected that during every full moon  the Earth's shadow will fall on the Moon, causing a lunar eclipse.  Lunar eclipses are not observed every month because the plane of the Moon's orbit around the Earth is tilted by about five degrees with respect to the plane of Earth's orbit around the Sun. Thus, when a full moons occurs, the Moon usually lies to the north or south of a direct line through the Earth and Sun. Although a lunar eclipse can only occur when the Moon is  full, it must also be positioned very near the intersection of Earth's orbital plane about the Sun and the Moon's orbital plane about the Earth that is, at one of its nodes.
The shadow of the Earth can be divided into two distinctive parts: the umbra and penumbra. Within the umbra, there is no direct solar radiation. Due to the Sun’s large angular size, solar light is only partially blocked in the outer portion of the Earth’s shadow or penumbra. A penumbral eclipse occurs when the Moon passes through the Earth’s penumbra. A partial lunar eclipse occurs when only a portion of the Moon enters the umbra. When the Moon travels completely into the Earth’s umbra, one observes a total lunar eclipse.
Unlike a solar eclipse, which can only be viewed from a certain relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of the Earth. A lunar eclipse lasts for a few hours, whereas a total solar eclipse lasts for only a few minutes at any given place, due to the smaller size of the moon's shadow.
Since moon is a non luminous body, lunar eclipses (unlike Solar Eclipses) are completely safe to observe with the naked eye - no special equipment or filters are needed. Sometimes a Total Lunar Eclipse is best viewed without any optical aid, and just lying under the stars watching the change as the Moon first gets slightly darker (penumbral phase), then starts to get eaten away (partial phase), finally turning deep red or copper coloured as it enters totality. During a total lunar eclipse, the sun’s direct light is blocked by the earth and does not reach the moon. A small amount of the sunlight that passes through earth’s atmosphere, however, is refracted or “bent” towards the moon by the atmosphere and is reflected towards us on earth by the moon. Particles in the atmosphere also preferentially scatter away the bluer light of shorter wavelengths and only the redder light that has relatively longer wavelengths gets through, similar to the sunlight we see at sunset and sunrise. This redder light reaches the moon because of the bending (refraction). Therefore the moon appears copper-coloured during a total lunar eclipse. The exact colour will depend on the nature and quantity of the dust particles, water droplets and aerosols present in the earth’s atmosphere at that time. Hence it is an indicator of earths atmospheric pollution!
For sky-watchers there is another treat in the intervening night of 27-28 July. The red planet Mars will be aligned with Earth and Sun. Mars will be on the opposite side of the Sun and Earth and it will be visible throughout night. It can be seen in the vicinity of eclipsed moon. In fact Jupiter and Saturn will also be clearly visible during the night. It is summer time hence night picnics may be organized by all science and nature lovers in their neighbourhood. All astro-photographers, may aim their cameras towards sky. The eclipse is a unique opportunity to appreciate,  admire and celebrate the beauty and inspiration of this celestial experience.





Monday, January 22, 2018

Copper Red Super Moon

An spectacular lunar eclipse will be taking place at moon rise on Wednesday, January 31. The total lunar eclipse of 31 January 2018 will occur during a “supermoon”, i.e., a full moon that coincides with perigee of the moon (the closest distance that the moon comes to earth during its orbit around the earth). The “super-moon” appears about 14% larger than a regular full moon. Another coincidence is that the full moon of 31 January is also talked of as a “blue moon” in the English media - a blue moon is said to occur when two full moons occur in the same calendar month. Also, this supermoon is the third in a trilogy of super moons, following those of 3 December 2017 and 1 January 2018.
 It will be visible in  Jammu and Kashmir between 6:20 pm up to 8 pm.   I am fascinated by moon since my childhood. When I was a youngster my father brought for me a popular science book in Urdu ‘Nau Saiyare Ektis Chand’. Through this book I came to know that moon is a non luminous body and it shines by reflecting the solar light. I was so upset by this fact that I hid the book lest others may know about the truth that moon does not have its own light. I was naïve like any other child of my age.
 A lunar eclipse occurs when the Moon passes behind the Earth so that the Earth blocks the Sun's rays from striking the Moon. This can occur only when the Sun, Earth, and Moon are aligned exactly, or very closely so, with the Earth in the middle. Hence, a lunar eclipse can only occur during the night of a full moon. It might be expected that during every full moon  the Earth's shadow will fall on the Moon, causing a lunar eclipse.  Lunar eclipses are not observed every month because the plane of the Moon's orbit around the Earth is tilted by about five degrees with respect to the plane of Earth's orbit around the Sun. Thus, when a full moons occurs, the Moon usually lies to the north or south of a direct line through the Earth and Sun. Although a lunar eclipse can only occur when the Moon is  full, it must also be positioned very near the intersection of Earth's orbital plane about the Sun and the Moon's orbital plane about the Earth that is, at one of its nodes.
The shadow of the Earth can be divided into two distinctive parts: the umbra and penumbra. Within the umbra, there is no direct solar radiation. Due to the Sun’s large angular size, solar light is only partially blocked in the outer portion of the Earth’s shadow or penumbra. A penumbral eclipse occurs when the Moon passes through the Earth’s penumbra. A partial lunar eclipse occurs when only a portion of the Moon enters the umbra. When the Moon travels completely into the Earth’s umbra, one observes a total lunar eclipse.
Unlike a solar eclipse, which can only be viewed from a certain relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of the Earth. A lunar eclipse lasts for a few hours, whereas a total solar eclipse lasts for only a few minutes at any given place, due to the smaller size of the moon's shadow.
Since moon is a non luminous body, lunar eclipses (unlike Solar Eclipses) are completely safe to observe with the naked eye - no special equipment or filters are needed. Sometimes a Total Lunar Eclipse is best viewed without any optical aid, and just lying under the stars watching the change as the Moon first gets slightly darker (penumbral phase), then starts to get eaten away (partial phase), finally turning deep red or copper coloured as it enters totality. During a total lunar eclipse, the sun’s direct light is blocked by the earth and does not reach the moon. A small amount of the sunlight that passes through earth’s atmosphere, however, is refracted or “bent” towards the moon by the atmosphere and is reflected towards us on earth by the moon. Particles in the atmosphere also preferentially scatter away the bluer light of shorter wavelengths and only the redder light that has relatively longer wavelengths gets through, similar to the sunlight we see at sunset and sunrise. This redder light reaches the moon because of the bending (refraction). Therefore the moon appears copper-coloured during a total lunar eclipse. The exact colour will depend on the nature and quantity of the dust particles, water droplets and aerosols present in the earth’s atmosphere at that time. Hence it is an indicator of earths atmospheric pollution!
The eclipse is a unique opportunity to admire and celebrate the beauty and inspiration of this celestial experience. It is also preferable to offer two rak’aat Salate Khusoof.