| Morgan
Spangle |
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| Star: Struve 2098 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 14.3 145.2
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| David
Jenkins |
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| Star: Struve 2098 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. |
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| Richard Jepeal | ||||
| Star: Struve 2098 Date: July, 14th, 2006 Time:--- Seeing: 6-7/10 Transparency: --- Location of site: New Britain, Connecticut USA Site classification: Urban Conditions: ---- Sky darkness: --- Telescope: 8in Celestron Nexstar Eyepieces: --- Magnification: 53x to 228x |
Another
good-looking triple.
All are yellowish to different intensities.![]() |
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| Axel
Tute |
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| Star: Struve 2098 Date: 17.07.2006 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 21.3°C 43% humidity Moon: no moon Sky darkness: Bortle 4 Telescope: Celestron 8 Eyepieces: Magnification: |
I
tried to make a good drawing from this one |
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| Wolfgang
Vollmann |
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| Star: Struve 2098 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 |
STF2098 = WDS 16457+3000 This is a very unequal
pretty quintuple system! A and
B are quite close with my focal length of 1040mm, C and D are widely
separated.
D has a faint companion a to the west which is only 13.7mag according
to the
current WDS. This pair Da was not measurable since the star images are
merged
but the companion clearly shows up in my image! All other pairs were
easily
measurable on my images. Judging from the proper motion data in the WDS
components A and B have common proper motion and seem to be related
They have
different proper motion from C and D but these two widely separated
stars seem
to be a common proper motion pair! ![]() |
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| Ian
Coster |
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| Star: Struve 2098 Date: 29/08/06 Time: 22:00 UT Seeing: 3/5 Transparency: 4/5 Location of site: London Lat: 51:27:54N, Lon: 0:16:36W Site classification: Suburban Conditions: Clear Moon: Not risen Sky darkness: Mag4 Sky (ZLM) Telescope: Orion Optics 200mm F6 Eyepieces: 18mm Ortho Barlow: No Magnification: x67 |
Comments:
Moderately rich
field Primary Colour: White Secondary Colour: Orange General Notes:
Easy split
in 18mm and a clear colour contrast Measurements: PA: 147 Sep: 14.3 (3x
Barlow
& 12.5mm MG. scale constant 5.3" per division)
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