Archive for January 23, 2020

NGC 1931 – Bright Nebula and Cluster in Auriga: February 2020 Observer’s Challenge Report

January 23, 2020

 

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

 ————————————————

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

 

Sue French: Observer from New York

254/1494mm (10-inch f/5.8) Newtonian. Seeing: fair. Transparency: a little better than average.

43×: NGC 1931 is just a short hop westward from starfish-like M36. It presents a small hazy spot surrounding a star.

115×: The nebula spans about 3 arcminutes, and the star now appears triple. Several additional stars straggle south through west-southwest of the nebulous mass.

213×: Six stars are now buried in the nebulosity, three brightest members arranged in a little triangle.

The WEBDA cluster plot below marks the four trapezium-system stars viewed as well as two additional stars spotted within the nebula.

Visual magnitudes of the trapezium stars according to WEBDA:

A=11.4, B=12.3, C=13.0, E=14.0. There is a component D in the trapezium system very close to B, but it’s thought to be magnitude 15.8 or dimmer and was not seen. The two arrowed stars were visible: the northern one shining at magnitude 14.1, and the southern one at magnitude 14.5.

fullsizeoutput_1235

fullsizeoutput_1236

Mario Motta: Observer from Massachusetts

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.

NGC1931

 

Roger Ivester: Observer from North Carolina 

On the night of January 28, 2020, the transparency and seeing were very good.  Using my 10-inch, f/4.5 reflector, NGC 1931 was very easy to locate and see at 57×, appearing as a star with a mostly round halo of nebulosity. 

When increasing the magnification to 267×, using a 12mm eyepiece and a 2.8× Barlow, the bright nucleus revealed a tiny trio of faint stars, with a fourth, much fainter star, toward the WSW.  This fourth star was extremely difficult, and could not be held constantly, but intermittently at best.  The nebula was elongated, with a NE-SW orientation.  

The first time I observed NGC 1931 was with poor seeing, on January 8, 1994, and could not see the trio of stars.  My second attempt to see the trio of stars was in January, 2020, but again with poor seeing and transparency, and was unable to see any of the faint stars.   

Pencil sketch, with the colors inverted:   

 

image001

 

 

Uwe Glahn: Observer from Germany

Telescope: 27-inch f/4.2Newtonian @ 293×.

Seeing: IV, NELM 7.0+

NGC 1931 and Parsamian 1 (a cometary nebula in southern part of NGC 1931)

 

http://www.deepsky-visuell.de/Zeichnungen/NGC1931.htm

 

NGC1931

 

Gus Johnson: Observer from Maryland

Could not see NGC 1931 on a clear night with a 5-inch at 24×. I also attempted with an H-beta filter at 30× and a UHC filter, however to no avail.  On another night in February 1985, I saw it with an 8-inch reflector @ 40×. Small, fairly bright mostly round nebulosity. Could not see the small trapezium of stars.

 

 

 

 

NGC 1999 – Reflection Nebula With Hole: January 2020 – Observer’s Challenge Report

January 23, 2020

rogerivester

MONTHLY OBSERVER’S CHALLENGE

Compiled by:

Roger Ivester, North Carolina

&

Sue French, New York

January 2020

Report #132

NGC 1999 Reflection Nebula in Orion

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…

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