| Steve Bodin | ||||
| Star:
Struve 1937, eta Corona Borealis
Date & Time: 6 May 2003 11 pm to 1 am Seeing: 4-5 <1-10 Seeing Scale (10 best)>. Transparency: poor Location of site: Silverdale WA, USA 47N 123W Site classification: suburb-rural Conditions: temp 40F, damp Sky darkness: 4.5 due moon <Limiting magnitude> Telescope: Celestron C8 Eyepieces: not used Additional: DX-8263SL video camera at prime focus and 3x, 6x Magnification: app. 333x, 1000x and 2000x Star: Struve 1930
Star: Struve 1930
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One
of those stars that I have been following for many years. Definite orbital
motion seen over the last 30 years, but have made measurements for only
part of that time. The color is definitely yellow for both stars, but they
are joined in a C8 at this time. this needed a stacked 2x and 3x , 6x total,
teleconverter to get sufficient image size. Measured,
0.55 sec at 91.7 deg PA, which is near the WDS prediction of 0.548 sec
at 91.7 sec. Just lucky that this measure is this close as the poor image
could be almost anything!
Had
a second look trying to split it cleanly, the seeing looked like a 7, but
degraded to 5 by the time I got all the barlows connected to make 6x magnification.
Still joined at an equivalant 2000x, measurement
0.563 sec at 091.2 deg PA.
Viewed
and reported twice before, but never fully split. This time is about as
close as a C8 can get to a star a the limit. Both yellow as close. WDS
6th Orbit elements solve to 0.542 sec at 093.2 on 24 June.
Measurements from two separate images, 0.574 sec at 093.0 deg PA, close
enough for me.
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| Bob Hogeveen | ||||
| Star:
Struve 1937, eta Corona Borealis
Date & Time: 28 May 2003 Seeing: 7 <1-10 Seeing Scale (10 best)> Transparency: fair degrading to poor in lower sky Location of site: Annen, The Netherlands 53ºN, 6ºE Site classification: Rural with some light domes Sky darkness: 5 <Limiting magnitude> Transparency: <1 worst - 10 best> Conditions: temp 10 C, damp Telescope: C11 on G11 Eyepieces: Pentax SMC XL 40mm, Ultima 30mm, TV plossl 20mm, plossl 10mm, LV 5mm Magnification: 560x, 400x, 280x
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I have observed Eta a few
times before, last year and this year, and it strikes me how easy it is
to split with the C11 when seeing is reasonable. With the predicted separation
of 0.55" confirmed by Steve's measurments I am always pleased to see the
obvious dark gap between the small airy disks at 560x, although the two
disks are surrounded by (parts of) several diffraction rings. This time
it was already with 280x that I had a positive indication of the two components,
where before I needed 400x. The color of both stars is white.
Another sub-arcsecond double in CrB is Gamma. After the succes on Eta I had a (first ever) look at Gamma. The separation of Gamma is
somewhat larger (0.7"), but the difference in brightness is also larger
(3.8 - 5.4). I suppose a DI of these doubles would be about the same. And
indeed at 560x Gamma was as nicely split as Eta. The bright primary creating
a larger image and the small, more faint secondary sitting close to it,
but not touching and showing a yellowish color.
Ambience: The promise of
a clear night before Ascension day was reason to arrange an observingsession
in the field with two fellow-observers. On clear, moonless nights I now
and then go to a nearby location with a very low and reasonably dark southern
horizon. There I try to find all sorts of low objects that are invisible
from my home-location.
This night the sky was somewhat disappointing. Besides the fact that we have already entered the grey summer skies at our latitude, it remained hazy in the lower regions and there was a lot of moisture in the air. I had to discard many of the low faint fuzzies on my list. I had hoped to support Steve Bodin with his quest for Double Galaxies but the situation was not good enough for serious observing of the double galaxies that were on my list. We started the night at 22.00,
still early twilight, but a good time to setup comfortably and to admire
the new C8 + Vixen GP that one of my fellow-observers recently obtained.
This time of evening the calls of a Quail (Coturnix coturnix), nearby in
the field, competed with the noise of passing trucks on the provincial
road a few miles away and the "roaring" of the motors of a 10" LX200.
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| John M. Ryan | ||||
| Star:
Struve 1937, eta Corona Borealis
Date & Time: 18:O6:03 12:00 local time Seeing: 6 <1-10 Seeing Scale (10 best)> Transparency: Fair to good Location of site: Barreras, Salamanca, Spain Site classification: Rural Sky darkness: 7 <Limiting magnitude> Transparency: <1 worst - 10 best> Conditions: Temp. 25ºC, Light wind Telescope: Celestron 9.25" SCT Eyepieces: none Magnification: Stella Cam Ex video camera, 4X Telemate with 2X Zoom for overall of 8X |
The video camera is black and white so no color can be noted. This double consists of two components almost equal in magnitude. This double being very close with a separation of under 1 arcsecond was boiling like mad on the laptop screen. I could see the separation at times but the video clip did not give me enough good frames to arrive at an accetable image for measuring. No measurements. I would need a night with better seeing and this shows that my limit for average seeing would be a separation of about 1.25" with the Steve Bodin method and my equipment. | |||