SWAN M4 was the brightest comet of the year 2006. For a long time it was announced with a luminous intensity of max. mag * 8-9, and would have been an object for larger telescopes. Around the 24th of October however the brightness arose to mag 4.2 whereby the luminous intensity on the 25th of Oct. was seen with the naked eye. The comet became estimated by me up to mag 3,8. This constant brightness was observed since the 26th of Oct. afterwards bad weather was dominating in Southern Germany. It is remarkable that the comet tail showed a noticeable brightness in the comparison to the coma.
Further detail maps under Winnies homepage
26th of October 2006
tb mr mr
TB/ MR; Auerberg/ Bavaria: Nikon 480mm (dig)/2.8; 90 seconds; ASA 800 Canon 20D
Swan M4 shows a very bright comet tail in the ' Corkscrew form '. This suggests a strong rotation of the comet nucleus.
25th of October
TB; Moorenweis, Fuerstenfeldbruck, Bavaria: Nikon 480mm (dig)/2.8; 80 seconds; ASA 800 Canon 20D
The comet appears with a very broad and bright tail, which suggests a larger material loss. Possibly an explosion in or on the comet nucleus was the consequence.
19th of October
TB; Nikon 3040mm (dig) Newtonian; 90 seconds, Canon 20D
17th of October
TB; Nikon 480mm (dig)/2.8; 105 seconds, Canon 20D
Comet SwanM4 close to the star Seginus of Bootes. The comet with apprx. mag 6-7 could hardly be recognized with the naked eye.
Small astro collection from Martin on the 25th of October 06
North America -, Andromeda- and Veil nebula.
*mag = > light magnitude: Up to mag +3-4 stars are visible nearby cities with the naked eye, in very dark areas the seeing limit can reach up to mag +6-7.
The more higher numerical value is given, the more weaker are the objects. E.g. - 4,7 mag, Venus glittering; - 1,0 Sirius, brightest star; +3,5 M31 Andromeda, pale shiny oval)
All comet observations from 2001 up to now ..
Etna Stromboli Volcano world Cinema
From Etna to Stromboli Planets & Space
©2006 photos& text by Thorsten Boeckel (tb), ©2006 photos by Martin Rietze (mr)