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. |
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