| Steve Bodin | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: 1 Mar 2003 9 pm to 11pm local Seeing: 6->4 <1-10 Seeing Scale (10 best)>. Transparency: poor Location of site: Silverdale WA, USA 47N 123W Site classification: suburb-rural Conditions: temp 40F, some dew Sky darkness: 5.5 <Limiting magnitude> Telescope: Celestron C8 Eyepieces: not used Additional: DX-8263SL video camera at prime focus and 3x Magnification: app. 333x, 1000x video |
One
of my favorite UMa stars. This star is in conciderable motion and I have
seen 20 deg of PA swing in the last few years. Creamy white primary and
blue-white secondary. Measurement with the
C8 and 3x barlow; 1.81 sec at 253.3 deg PA.
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| William Guyot | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: 10th, March, 2003, 01:00 Seeing: 7 <1-10 Seeing Scale (10 best)>. Transparency: Location of site: Clermont-Ferrand, France Site classification: suburb-rural Temperature : 5°C: Sky darkness: ~5 <Limiting magnitude> Telescope: Vixen 80ED Eyepieces: LVW 17mm, LVW 8mm , barlow ultima X2 Magnification: X42, X90, X84, X180 |
barely
seen with LVW 8mm, clearly splited with LVW 8mm + barlow X2 (X180). It
was for me a nice 8. My better double of the night :)
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| Tom Teague | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: 2003 March 14 (22:30 UT) Seeing: 6-7 (very variable) <1-10 Seeing Scale (10 best)>. Transparency: Location of site: Chester, UK 53º 11' 08"N, 02ºË 51' 39"³W Site classification: Suburban Conditions: Clear, cold, still. Sky darkness: Poor (gibbous Moon) Telescope: 2.5 inch Zeiss Telementor refractor Mount: Zeiss T-mount Eyepieces: Magnification: x34, x84, x140, x210 Harshaw scale: <1-5 Scale (1 best)> |
Single x34. Clearly double
at all powers from x84 upward.
During moments of better seeing, it appears as a figure-of-eight, with two slightly overlapping discs. Estimated PA is about 260º. The current orbital prediction gives a separation of about 1.8", but although this is a pair with a securely established orbit, I find it hard to believe that it isn't rathercloser @ say 1.5". It should be just resolvable
in my Telementor, but I see the two discs as overlapping rather than tangential.
Perhaps the seeing is to blame for my failure to split them cleanly.I could
not detect any colours, although the difference in brightness betweenthe
two components was obvious enough. I found the most pleasing view was at
apower of x140, but in steadier conditions I would expect x210 to be even
better.
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| Luis Balanzino | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: Mar 11-12, 2003, 20h to 22h UT Seeing: 6 <1-10 Seeing Scale (10 best)>. Transparency: 6 <1 worst - 10 best> Location of site: Göteborg, Sweden 57°43' N, 11°58' E Site classification: Urban area with considerable light pollution Moon: In Taurus, illuminated fraction 0,55 Temperature: 2º C Sky darkness: 4.5 <Limiting magnitude> Telescope: Meade ETX-90 MK 90mm f/13.8 on photo tripod Eyepieces: 26mm Meade 4000 and 12,5mm TAL Super Plossl, 2x TAL Barlow Magnification: 48x, 100x, 200x |
Easy to identify but hard
to split in the ETX. In fact, the separation is not far from the Dawes
limit for this scope. At 48x no split at all, but at 100x I can see two
very bright, small dots of light in contact, nice! They look white or slightly
yellowish. Switching to 200x show the stars almost in contact, but the
conditions aren't good to use high power.
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| Tim Leese | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: 22 March 2003, 22:30 UT Seeing: 6-7 <1-10 Seeing Scale (10 best)>. Transparency: Location of site: Northwich, Cheshire. UK. (53° 15' N -2º 33' W). Site classification: Suburban Conditions: Clear sky, light low mist, no Moon visible. Sky darkness: 3.0 ( Umi ) <Limiting magnitude> Telescope: 4inch f/15 Vixen: achromat. Mount: EQ5 Eyepieces: 18mm and 9mm Orthoscopics, X2 barlow. Magnification: X83, X166, X332 |
9mm Or-------A definite
sighting using this magnification. The seeing was wavering, but for odd
moments, I could see a clear split of the two pale yellow stars.
9mm Or +X2 barlow-----When the boiling image settled, a definite split with the companion estimated to be at about the 270degree mark. I enjoyed observing this double as it takes high power well. As I was searching for this
double I chanced upon another double, nearby ( since identified as STF
1524). Another, very faint and delicate, bluish companion, glimpsed
with an orangey/yellow primary.A bonus!!
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| William Guyot | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: 25 mar 2003, 22 to 24h Seeing: 4->6 <1-10 Seeing Scale (10 best)>. Transparency: medium Location of site: La Garandie near Clermont-Ferrand, France Site classification: suburb/rural Temperature: 8°C, now dew Sky darkness: 5.3 <Limiting magnitude> Telescope: AP Traveller EDT Eyepieces: Clavé 12/20/25mm, vixen LVW 8mm, Powermate X5 Magnification: X24, X36, X51, X76, X122, X153, X254 |
Very nice quite equal pair
very white. Barely splited with X122,
splited nicely with X153
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| Tom Campbell | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: April 1, 2003, 8:25pm - 10:00pm CST (02:25-04:00 UT) Seeing: 7 <1-10 Seeing Scale (10 best)>. Transparency: 7 <1 worst - 10 best> Location of site: Iola, Kansas Long: 95°24'W, 37°55'N Site classification: Suburban Temperature: Temperatures in the lower 60s . There was a moderate breeze. Sky darkness: <Limiting magnitude> Telescope: Discovery DHQ 8" dobsonian Eyepieces: 1.25" Plössls - 25mm,, 15mm, 10mm, 6.5mm, 4mm Magnification: 49x, 81x, 122x, 188x, 305x |
Both stars in this pair
are about equal brightness, and both are yellow-white. At 305x, I could
barely split them.
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| William L. Schart | ||||
| Star:
Xi Ursa Majoris (Struve 1523)
Date & Time: Saturday, 25th of April, 2003 Seeing: 8 <1-10 Seeing Scale (10 best)>. Transparency: Location of site: Texas, USA Site classification: Suburban Sky darkness: 4 <Limiting magnitude> Telescope: C8 Eyepieces: Magnification: |
A
tight pair, but rather bright, hence not an overly
high DI of 72.64. There was a slight elongaton at low power, definately elongated and perhaps even notched at mid power and clearly split at high power.
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