I wanted to image a double star in need of attention using a different method, a new technique, now that the WDS "neglected" system as been decommissioned.
After filtering for "old" data, I came across the entry 07481+0525 STF1143 with the last entry reported in 1825! Almost 200 year old data.
Luminance only, ½ second subexposures, 12 stacked shots. FITS Liberator, Paint.NET. North is up; east is left.
Struve 1143 is also known as HD 63241 or SAO 115947. Stars visible to magnitude 14 and beyond are visible.
I found some notes in the WDS database: Some error in position. See note in BDS II. Bu_1906; This may be STF1134AB with a larger error than is typical for a FGW Struve measure.
Now Σ1143 is supposed to be a somewhat tight pair of unequal stars. The primary is mag 6.6 with a secondary at mag 11. The separation is purportedly 9.3 seconds of arc. B is supposed to the to the south-east.
I don't see anything...
The equal pair of stars to the north (not noted as a double) are separated by about 22". So 1143 A and B should be visible at half that distance.
Nothing.
Curious.
What did Friedrich Georg Wilhelm see?
Regardless, it is a lovely little pattern of stars...
§
Another curious thing about this is that SkyTools shows a star north-east of the upper pair, of equal brightness. It says it is NSV 3739. I see nothing.
§
Strange. When I went looking for the completed data the morning after, the target showed as pending... Some short of glitch which in the end worked itself out.
Tuesday, March 19, 2019
Subscribe to:
Post Comments (Atom)
No comments:
Post a Comment