| Morgan
Spangle |
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| Star: Struve 2070 Date: 11 June 2006 Seeing: <1-10 Seeing Scale (10 best)>: 5 Transparency: <1-10 Scale (10 best)>: 7 Location of site: Larchmont, NY Site classification: Bright suburuban Conditions: Cool, breezy Moon: Full Sky darkness: 3.5 Telescope: 23.5cm SCT Mount: Takahashi NJP Temma 2 Eyepieces: SBIG ST2000XM CCD camera Magnification: n/a |
NAME SEP PA NOTES 28.6 141.8
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| Axel
Tute |
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| Star: Struve 2070 Date: 29.06.2006 Seeing: <1-10 Seeing Scale (10 best)>: 7 Transparency: <1-10 Scale (10 best)>: 9 Location of site: Küssaberg-Dangstetten, Germany Site classification: rural Conditions: no wind, warm low humidity (I forgot to measure) Moon: no moon Sky darkness: Bortle 4 Telescope: Celestron 8 Eyepieces: Magnification: |
Faint companion in the 12mm RKE (167x) at an estimated PA from 140°. 2094: Not a clear split. "Bump" in PA 70° visible in the 12mm RKE. Faint star also visible at PA 310° |
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| Mike
Sutherland |
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| Star: Struve 2070 Date: 30 June 2006 Time: 10:00pm to 12:00pm PDT Seeing: <1-10 Seeing Scale (10 best)>: 7 Transparency: below average Location of site: Beaverton Oregon, USA 45 28N, 122 51W Site classification: Suburban Conditions: 66F, dry Sky darkness: limiting mag 3 Telescope: Takahashi FS128 Eyepieces: 30mm Ultima, 12mm ortho, 9mm ortho, 7mm ortho, 6mm ortho, Barlow. Magnification: 35x, 87x, 116x, 149x, 173x, 327x |
11:05pm PDT 12mm ortho (87x) and 7mm
ortho (149x) |
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| Wolfgang
Vollmann |
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| Star: Struve 2070 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 16377+1933 Located
south and east of Beta and
Gamma Her. The wide pair (WDS catalog magnitude 7.9 and 10.4mag) shows
almost
no change in distance and position angle. It could be a physical double
star
with very long period or an optical double where the line of sight to
the stars
does not change in very long time; perhaps they are very distant? ![]() |
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