![]() On 9 May 2016 there was a transit of the planet Mercury across the Sun. This happens approximately 13 times per century, and always around 8 May or 10 November. The last visible transit of Mercury visible from the Netherlands was on 7 May 2003. The next time that the entire transit will be visible from the Netherlands will be on 7 May 2049. The first part of the transit of 11 November 2019 will visible from the Netherlands as well. After the Venus transit of 8 June 2004 this was my second observation of a transit of a planet across the Sun. Members of our local astronomy society gathered a field close to my
hometown Assen. They brought a variety of telescopes. I took my 'old'
Canon 30D and a zoom + extender effectively giving me a 280mm lens.
This was just sufficient to picture Mercury as a little dot on the Sun.
The transit started at 13:12 local time and lasted 7 1/2 hours. |
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![]() The little dot on the left is planet Mercury. The picture on the left is made at 13:33 local time, the picture at the right as 14:51. It show how much Mercury moves in 1 hour and 18 minutes. In the middle of the picture a Sun spot is visible. The apparent diameter of Mercury is about 1/160 of the apparent diameter of the Sun. |
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![]() Bob brought an Astrophysics 130mm Starfire refractor with solar filter. Through this telescope Mercury appeared as a nice sphere before the Sun. |
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| One way to
observe solar eclipses and planetary transits is to project the image
of the Sun on a screen. No filter is required. The dot on the upper
left planet Mercury.
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![]() At the end of the afternoon I went home, and observed the transit with my Coronado PST solar telescope. With this telescope you can see the chomosphere of the Sun. The colour red is the hydrogen-alpha line with a wave lenght of 6563 ångström (656.3 nanometer). The chomosphere is the layer on the Sun just above the photosphere that we usually see. |
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![]() With a compact camera I took a picture through the eyepiece of the PST telescope. |
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![]() The diagram above shows the path of Mercury across the Sun. Due to the actual orientations of telescopes and camera, many pictures of the transit show Mercury at 'other' positions. |
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Mercury Transits 1901-2050
Date Universal Separation*
Time (Sun and Mercury)
1907 Nov 14 12:06 759"
1914 Nov 07 12:02 631"
1924 May 08 01:41 85"
1927 Nov 10 05:44 129"
1937 May 11 09:00 955"
1940 Nov 11 23:20 368"
1953 Nov 14 16:54 862"
1957 May 06 01:14 907"
1960 Nov 07 16:53 528"
1970 May 09 08:16 114"
1973 Nov 10 10:32 26"
1986 Nov 13 04:07 471"
1993 Nov 06 03:57 927"
1999 Nov 15 21:41 963" (graze)
2003 May 07 07:52 708"
2006 Nov 08 21:41 423"
2016 May 09 14:57 319"
2019 Nov 11 15:20 76"
2032 Nov 13 08:54 572"
2039 Nov 07 08:46 822"
2049 May 07 14:24 512"
* distance (arc-seconds) between the centers of the Sun and Mercury
Source: http://eclipse.gsfc.nasa.gov/transit/transit.html