| David
Jenkins |
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| Star: Struve 1964 Date: 12 June 2006 Time: 5:00-7:30 UTC Seeing: <1-10 Seeing Scale (10 best)>: 5 Transparency: <1-10 Scale (10 best)>: 8 Location of site:Orem, Utah USA Latitude, 40.29694. Longitude, -111.69389 Site classification: Utah Valley urban area of 500,000 with strong light pollution due to acorn glass street lights which shoot light up and out – The bane of all local observers. Salt Lake City metro light dome to the northwest at 40 miles. Conditions: Clear, breezy (as can be seen in some of the images), warm Moon: Full moon raising late in observing session Sky darkness: <Limiting magnitude>: 3.5 Telescope: Celestron GPS 11" on APT Wedge Mount: Standard Celestron fork and tripod Eyepieces: Meade Super Plossl – 32mm Diagonal: Yes, Meade 1.25" flip mirror diagonal Magnification: Approximately 350X using Nikon Coolpix 4500 and 4X zoom Software: Reduc version 3.62 – Great software from Florent Losse. S33 group member. |
Distance:
14.7, PA: 87![]() |
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| Richard Jepeal | ||||
| Star: Struve 1964 Date: June 17, 2006 UT Seeing: Vary, from 5/10 to 8/10 (Zenith) Transparency: --- Location of site: New Britain, Connecticut, USA Site classification: Urban Conditions: Sky darkness: Telescope: 8in Celestron Nexstar Eyepieces: Magnification: |
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| William
Schart |
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| Star: Struve 1964 Date: 6/19/06 Time: 10:36 PM Seeing: 4 out of 5 Transparency: Location of site: Columbia, USA Site classification: Suburban Conditions: warm Sky darkness: around mag 5 (LM) Telescope: C8 Eyepieces: 25 and 10 mm Magnification: |
Easy split almost 90. White. | |||
| Brian
McInnerny |
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| Star: Struve 1964 Date: 2006 June 30/ July 1 Time: 0030UT Seeing: 5/10 (10 best) Transparency: Hazy Location of site: SW England Site Site classification: Suburban Sky Conditions: Moon: Sky darkness: Naked eye Limiting mag: Zeta Boo=3.8 Telescope: ETX 90EC (90mm) Eyepieces: Magnification: |
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| Steve
Bodin |
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| Star: Struve 1964 Date: 25 June 2006 Time: 11pm to midnight Seeing: 5-6/10 Transparency: good Location of site: Mattawa Wa, USA 46.7N,119.9W Site classification: Rural Conditions: 79F, no wind, dry Sky darkness: limiting mag 6.5 Telescope: Meade 16 inch LX200GPS UHTC Eyepieces: not used maging: DX8263SL video camera at f30 Magnification: app. 1800x |
I know this
is not a 'nut' as
listed in out project, but there are two close components and one
impossible
companion making this pair actually a fivesome. Obvious, even at prime
focus is
that the eastern star is double, C and D. The main star has a B
component,
cataloged as Hu 1167, that is very difficult due to separation and
magnitude
difference. Finally the C star is an impossible 0.1 sec pair cataloged
as WAK
1. Measured, AC 15.19 sec at
087.4 deg PA, CD 1.64 sec at 022.3 deg PA, AB 1.27
sec at 080.7 deg PA, AD 15.9 sec at 081.9 deg PA.
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| Wolfgang
Vollmann |
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| Star: Struve 1964 Date: 2006 July 6 Time: 21:00-23:00 UT Seeing: 5 <1-10 Seeing Scale (10 best)> Transparency: clear Location of site: Vienna, Austria Site classification: Suburban Sky Conditions: Moon: Sky darkness: Naked eye limiting mag. 4.5 Telescope: 130/1040mm refractor Eyepieces: n/a Camera: SBIG ST237A CCD Exposures: 6x10 seconds for astrometry and 6x1 seconds for distance/PA measurement. Image measurement: astrometry with Astrometrica software and UCAC2 catalog (see http://www.astrometrica.at); with exact focal length and image orientation I measured distance and PA with AIP4WIN software. I took means of measuring all my images for a star. There is a scatter of 0.2 arcsec in separation and 0.2 deg in PA. Scatter in PA is much larger if the stars are very close. Note: All images have north up and an image size of approximately 16x12 arc minutes |
WDS 15382+3615 This
pretty double star is 1/2 degree
southwest of Zeta CrB which is a remarkable double itself. The image
shows the
two almost equally bright components A and C. Each one has a close
companion B
and D which are not resolved with my telescope at prime focus. ![]() |
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| Wolfgang
Vollmann |
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| Star: Struve 1964 Date: 2006 July 26 Time: 21:00-24:00 UT Seeing: 5 <1-10 Seeing Scale (10 best)> Transparency: clear Location of site: Vienna, Austria Site classification: Suburban Conditions: Moon: Sky darkness: 4.5 <Limiting magnitude> Telescope: 130/1040mm refractor Camera: SBIG ST237A CCD Exposures: 6 or 12 x 10 seconds for astrometry. Distance/PA measurement was done with these images also except where noted (bright stars need shorter exposure times of 1 sec or less) Image measurement: astrometry with Astrometrica software and UCAC2 or USNO B1.0 catalog (see http://www.astrometrica.at); with exact focal length and image orientation I measured distance and PA with AIP4WIN software. I took means of measuring all my images for a star. There is a scatter of 0.2 arcsec in separation and 0.2 deg in PA. Scatter in PA is much larger if the stars are very close. Note: All images have north up Eyepieces: n/a Magnification: n/a |
I already
measured AC for the
project but only from 2 frames. Now I took the opportunity to take 12
more with
exposure times of 1 and 0.1 seconds and remeasured the stars. Measure:
STF1964AC: year 2006.57 / distance 15.0 arcsec / PA 84.3 deg Weighted
average
of 2 nights: STF1964AC: year 2006.56 / distance 15.0 arcsec / PA 84.3
deg
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