| Mike Sutherland | ||||
| Star: Struve 3055 Date: 21 October 2006 Time: 9:20pm PDT Seeing: about 5/10 Transparency: average Location: Beaverton Oregon, USA Site classification: Suburban Conditions: 56F, dry Sky darkness: limiting mag 3 Telescope: Takahashi FS128 Eyepieces: 9mm ortho Magnification: 116x |
Very
wide, uninteresting pair.
Perhaps more exciting in binoculars. |
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| Steve Bodin | ||||
| Star: Struve 3055 Date: 22 Oct 2006 Time: 9 to 11pm Seeing: 4-5/10 Transparency: fair Location: Mattawa Wa, USA, 46.7N,119.9W Site classification: Rural Conditions: 48F, no wind, dry Sky darkness: limiting mag 6.5 Telescope: Meade 16 inch LX200GPS UHTC Eyepieces: not used Imaging: DX8263SL video camera at f10 and f30 Magnification: app.600x and 1800x |
Another star that is
multiple, but the project star is
the AC pair. The AB pair is again an old friend, measured 5.66 sec at 359.8 deg.
PA, The AC pair 121.6 sec at 031.7 deg PA. ![]() |
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| Wolfgang
Vollmann |
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| Star: Struve 3055 Date: 22 Oct 2006 Time: Seeing: 5/10 (10 best) Transparency: clear Location: Vienna, Austria Site classification: Suburban Conditions: Sky darkness: Naked eye limiting mag. 4.5 Telescope: 130/1040mm refractor Eyepieces: Imaging: SBIG ST237A CCD Magnification: Note: All images have north up Please follow the links to see the images! |
This nice
unequal triple
system was imaged with 10s exposures: http://static.flickr.com/97/280761953_fb3a5e576b_o.jpg The bright and close AB pair is in the middle, B sits immediately above (north) of A. C is the fainter star towards upper left of the two. I did astrometry on my images with Astrometrica (see http://www.astrometrica.at) and determined separation and PA of A-C on these images. In addition I took 1 and 3 second exposures and measured the AB pair on them (C is also visible towards upper left): http://static.flickr.com/120/280761955_a3a94956ed_o.jpg Measures: year 2006.81 STF3055 AB: distance 5.5 +- 0.2 arcsec / PA 359.1 +- 0.9 deg / 24 images STF3055 AC: distance 122.7 arcsec / PA 31.5 deg / 8 images All 3 stars appear relatively unchanged since the first measures in the WDS and seem to share common proper motion. |
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