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Selecting A Place to Watch Transit of Mercury

5/10/2016

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Things to know before you start is what it mean by "Altitude of Sun in sky?"
The solar elevation angle is the altitude of the sun, the angle between the horizon and the centre of the sun's disc.
In simple words it is the position of Sun in height wise in the sky. For example when Sun is rising it is in 0° and  as hour pasts it increases its altitude and gain the highest altitude of 90° at the noon time. After that Sun started decreasing it's altitude to 0°, that is the sun going bellow horizon. 
​
Picture
This is how exactly it will be from Sunrise to Sunset
Starting time of this transit is 11:12 UTC that means 16:42 IST or 4:42 pm on the 9th of may. Clearly by the timing given we can see it is the time when Sun started going down bellow horizon. So as a rule of nature the Eastern part of country like Assam, West Bengal, Odisha, East part of Tamilnadu and Andhra Pradesh will have Sun in low horizon making it hard to observe. Where as the states like J&K, Delhi, Himachal Pradesh , UP, MP, Telengana, Karnataka will be in much better condition than eastern states. But the good news come for the Western Indian state or the states adjacent to west coast of India, Because Sun will be in much better altitude than the rest of India. 
So it's better if you are in western part of India. Now Chose a high roof top or a area where the west horizon is completely clear. It is better if you move out from city area because the SPM Level in the low horizon sky in the city area are much higher. And because the Mercury will appear a tiny dot (.) in the sun disk so you may not resolve Mercury in that condition.
Now that you are completely positioned lest's enjoy the show with a protective eye gear. DO NOT EVER LOOK AT THE SUN WITHOUT ANY PROTECTIVE GALSS / FILETR .  

Point to note.
  • For any place in India the transit will begun on exactly 16:42 IST that is 4:42 pm on May 9th.
  • The altitude of sun will defer from place to place east to west wise. (North to South wise is negligible in this case) 

*This picture intend for India only Timings are given in IST the upper figures indicating the Sun's altitude at starting of transit (16:42 IST) & the lower figure indicating the sun set time for that region.
               **To get exact timing of your place click here.
Picture
This picture intend for India only Timings are given in IST the upper figures indicating the Sun's altitude at starting of transit (16:42 IST) & the lower figure indicating the sun set time for that region.
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Observing Transit of Mercury

5/7/2016

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Picture
SWAN's Solar Projector
The safest way to observe a transit is to project the image of the Sun through a telescope, binoculars, or pinhole onto a screen, but the event can be viewed with the naked eye using filters specifically designed for this purpose, such as an astronomical solar filter with a vacuum-deposited layer of chromium, eclipse viewing glasses, or Grade 14 welder's glass. An earlier method of using exposed black-and-white film as a filter is no longer regarded as safe, as small imperfections or gaps in the film may permit damaging UV rays to pass through. Also, processed color film (unlike black-and-white film) does not contain silver, and is transparent to infra-red. This may result in burns to the retina. Observing the Sun directly without filters can cause a temporary or permanent loss of visual function, as it can damage or destroy retinal cells.

Click the link bellow to see how to make a solar projector.
Making Safe Solar Projector
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What is Angular Diameter

5/3/2016

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Picture
In this image you can find the actual scaled size of Mercury in front of Sun disk. That is marked by Red line. P.C. Wikipedia
To know how large each celestial object will appear in the sky at first you need to have an idea of Angular Diameter.
The angular diameter or apparent size is an angular measurement describing how large a sphere or circle appears from a given point of view.
In astronomy the sizes of objects in the sky are often given in terms of their angular diameter as seen from Earth, rather than their actual sizes. Since these angular diameters are typically small, it is common to present them in arcseconds. An arcsecond is 1/3600th of one degree.

Degrees, therefore, are subdivided as follows:
360 degrees (°) in a full circle
60 arc-minutes (′) in one degree
60 arc-seconds (″) in one arc-minute
In general perception the tip of your little finger will create 1° by holding the hand at right angles to a fully extended arm. And then the size of Sun disk is exactly the half of your finger tip. So you can well imagine how small the Sun appears in our sky. The size of sun then is ~31° means 31 X 60 = 1860" (Arcsecond). The size of Mercury on event day will be 12" so that will appear as  1/300th times of your little finger tip. So you can well imagine the size. For reference look at the picture. If the red line will be the observable size of Sun (By the help of Optical Instruments) then you can find mercury as a dot (.) appearing in the Sun disk.  
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