This first group with a 6-inch f/15 refractor (with a 60mm f/16 Tasco strapped to it):
JC 6 AB: 6-inch; 250x: ! Light orange A, grey B lies on A's
diffraction ring, faint, 3 Dm. Very pretty diamond ring effect. No Gaia parallax data for the secondary. There hasn't been much change in PA or
separation since discovery, but an orbit could be tried all the same. JC = W.S. Jacob, "Captain, Bombay
Engineers" who observed with a Dolland telescope of 5-feet focal length --
probably a 4-inch refractor -- from "Poonah" = Pune, India. Wikipedia: "While in England in 1855
Jacob wrote "A few more words on the Plurality of Worlds" in which he
suggested life on other planets ("probably that some of the known planets
are inhabited, not very improbable that all of them are"), and described
his computation of stellar orbits for the Royal Astronomical Society. Jacob
posited that apparent orbital anomalies in the binary star 70 Ophiuchi might be
caused by an exoplanet. While these anomalies are now thought to have other
causes, this was the first serious claim by an astronomer to have detected an
exoplanet using scientific methods: 100 years before the first exoplanet was
conclusively detected and well before the science of exoplanets was even in its
infancy. Professor David Kipping states that the ‘claim is so remarkable
because Jacob was making tiny measurements (80 milliarc seconds or 22
millionths of a degree) with the naked eye, at a time when he wasn’t even sure
whether Newton’s law of gravity held sway in distant parts of the galaxy. While
Jacob... was ultimately proved wrong, he had the audacity to try.'"
18h 25m 21.02s -20° 32' 29.9" P.A. 280.00 sep 1.7 mag
5.03,7.43 Sp K1III+A1V dist. 125.79 pc (410.33 l.y.)
STF2315 AB: 6-inch; 250x: ! White A, very extremely faint B
resolves with foveal coaxing and I can then hold it direct, very closely split
clean. No Gaia parallax data for either star.
Sixth Orbit Catalog grade 4 orbit, 2094-year period.
18h 24m 58.46s +27° 23' 41.3" P.A. 117.00 sep 0.6 mag
6.57,7.77 Sp A0V+A4V dist. 117.51 pc (383.32 l.y.)
STT 350 AB: 6-inch; 250x: !! Incredible pair, super delicate,
pure white faint stars, 1 Dm, in a star field of bright white stars (open
cluster NGC 6633, which is gorgeous, large loose stars in an E-W arc).
Disappointingly, Gaia DR3 shows -32% parallax range overlap, it is not likely binary.
18h 26m 52.89s +06° 25' 23.9" P.A. 166.00 sep 1.9 mag
7.79,9.39 Sp A0III
STF2320 AB: 6-inch; 250x: ! Super fine white A and 2 Dm B,
hairline split. 58% parallax range overlap, 334 AU weighted separation,
3.2+2.1 Msol, it is likely binary and needs an orbit.
18h 27m 45.89s +24° 41' 50.8" P.A. 1.00 sep 0.9 mag
7.14,8.90 Sp B9V dist. 256.41 pc (836.41 l.y.)
STT 368 AB: 6-inch; 250x: ! Close white A and blue B in perfect
seeing, 1 Dm, just past hairline split.
4% parallax range overlap, 221 AU weighted separation, 1.9+2.4 Msol, it might be binary and needs an orbit.
19h 16m 01.84s +16° 09' 39.5" P.A. 218.00 sep 1.1 mag
7.53,8.49 Sp A9IV dist. 240.96 pc (786.01 l.y.)
STF2579 AB: 152; 200x: ! Excellent close pair,
very bright A and faint B resolves outside A's first diffraction ring at 200x
& 250x. I also see it in the 60mm scope at 90x, but only with foveal
coaxing and because I already knew where to look after seeing it in the
6-inch. The refractor and small aperture suppress the bright star's
diffraction and provides the contrast needed to see the companion. No
Gaia data for the secondary. SOC grade 4 orbit, 657-year period.
19h 44m 58.44s +45° 07' 50.5" P.A. 213.00 sep 2.7 mag
2.89,6.27 Sp B9.5IV dist. 50.58 pc (164.99 l.y.)
Using a 7-inch aperture mask on my 20-inch f/5 dob:
AC 7 BC: 7-inch; 200x: ! Component of
STF220, which is a 3.5 magnitude light orange star with a 10th magnitude wide
companion. This is BC, which while faint was resolved at 1"
separation to an close unequal pair. Brightens slightly with averted vision,
the star images were cleaner with the 7-inch than full aperture. PA to
the NE, it's faint white pair near equal but nice close split. SOC grade
1 orbit, 43.46-year period, it will be due east by 2040. 4% PRO,
only 29 AU WS, 0.3+0.3 Msol, very interesting pair.
17h 46m 25.07s +27° 43' 01.4" P.A. 27.00 sep 1.0 mag
10.20,10.70 Sp M2.2V+M4V
With my 20-inch f/5 dob:
JEF1 AB: 20-inch; 1270x: Nusakan, 3 CrB. With
apodising mask and blue filter, I can detect the position angle of the
elongation as SSE. Currently 0.15", it will widen quickly in the
next couple of years reaching apastron in 2028 at 0.314". SOC grade
1 orbit, 10.54-years period, and probably the shortest period binary I've observed.
15h 27m 49.85s +29° 06' 19.8" P.A. 140.00 sep 0.15" mag
3.68,5.20 Sp A5+F2 dist. 34.28 pc (111.82 l.y.)
STT 535 AB: 20-inch; 1270x: Using an apodising mask
and blue filter, at >500x the elongation was obvious, and bumping the
magnification up to 1270x I had a clean split, slightly unequal stars with PA
to the NE. Spurious disks were fairly steady but there was a fair amount
of dancing diffraction at this magnification. I observed it in October
2020 with the 20-inch, when it was at 0.165", and it appeared
single. So this makes a handful of pairs in which I've been able to trace
movement over the last few years. We have another four years or so before
the secondary makes its dive back toward the primary and will be undetectable
visually. What a fun observation, 5.71-year period! SOC grade 1
orbit.
21h 14m 28.81s +10° 00' 25.1" P.A. 7.00 sep 0.33"
mag 5.19,5.52 Sp F6V+F6V dist. 18.49 pc (60.31 l.y.)
BR,
Mark
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