MONTHLY OBSERVER’S CHALLENGE
Compiled by:
Roger Ivester, North Carolina
&
Sue French, New York
February 2020
Report #133
NGC 1931 Bright Nebula and Cluster in Auriga
Sharing Observations and Bringing Amateur Astronomers Together
Introduction
The purpose of the Observer’s Challenge is to encourage the pursuit of visual observing. It’s open to everyone who’s interested, and if you’re able to contribute notes, and/or drawings, we’ll be happy to include them in our monthly summary. Visual astronomy depends on what’s seen through the eyepiece. Not only does it satisfy an innate curiosity, but it allows the visual observer to discover the beauty and the wonderment of the night sky. Before photography, all observations depended on what astronomers saw in the eyepiece, and how they recorded their observations. This was done through notes and drawings, and that’s the tradition we’re stressing in the Observer’s Challenge. And for folks with an interest in astrophotography, your digital images and notes are just as welcome. The hope is that you’ll read through these reports and become inspired to take more time at the eyepiece, study each object, and look for those subtle details that you might never have noticed before.
February: NGC 1931 – Bright Nebula and Cluster – Auriga; Mag. V= 10.1; Size 6′
RA: 05h 31m Dec. +34º 14′
The embedded Stars in NGC 1931 by Sue French:
Don’t be surprised about not seeing the stars in NGC 1931. Folks get very mixed results. Go to http://www.deepsky-archive.com/ and type NGC 1931 in the Designation box, then look at everyone’s sketches.
Here’s a long-ago Amastro post from Brian Skiff that gives the magnitudes of the trapezium system embedded in the brightest part of the nebula. I see one of these stars, or a blend of them, in the 105mm scope. The 10-inch at 213× gives me six stars in the brightest part of the nebulosity plus several mag 11-13½ stars scattered to the south. I’ve pasted an image below Brian’s data and labeled the stars on it. The image is in infrared so that the nebulosity doesn’t blot out the stars. Below the Aladin image is a WEBDA chart showing which stars I saw in the main group through the 10-inch..
While cleaning up some star-lists, I collected data for stars in the nebulous open cluster NGC 1931 in Auriga. The group contains a faint trapezium system, ADS 4112, that might be of interest to ‘amastro’ folks. The specs for the group are shown below. The V magnitudes for the stars come from modern photoelectric or CCD studies. The separations derive from positions in the 2MASS catalogue, which should be better than the 100-year-old visual micrometry, but which in any case match the old data to within a few tenths of an arcsecond. The brighter trio is straightforward in a small telescope; in 1989 I was able to make out the fourth ‘E’ component very faintly in my 6-inch refractor at 200x. The very faint, close ‘D’ companion to star ‘B’ doubtless requires a very large aperture. The data quoted for it is from S. W. Burnham’s work; the magnitude is possibly too bright. The 2MASS coordinates are listed at the bottom. Star ‘D’ does not appear in any astrometric catalogue. The spectral types for the three brightest stars, by the way, are B0V, B0.5V, and B1V. Thus the object should contain some emission, although there must be a substantial reflection component, since filters do not provide much contrast enhancement.
\Brian
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ADS 4112 = BD+34 1074: 5 31 27 +34 14.9 (2000)
V mags sep pa
AB 11.5,12.3 8″.1 239
AC 13.0 10″.5 310
AE 14.0 14″.6 17
BD (15.8) 2″.3 322
RA (2000) Dec
A 5 31 27.08 +34 14 49.6
B 5 31 26.54 +34 14 45.0
C 5 31 26.43 +34 14 56.3
E 5 31 27.50 +34 15 03.2
Mario Motta: Observer from Massachusetts
See attached image of NGC 1931, for the February 2020 Observer’s Challenge report.
Taken with my 32-inch telescope, and SBIG STL 1001E camera. One hour of H alpha, one hour of Sulfur S2 filters, and only 20 minutes of O3 filter as there was essentially no Oxygen signal.
Processed in PixInsight.
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