- Astrotrac 360 tracking platform – first impression
- FIELD TEST: CARL ZEISS APOCHROMATIC & SHARPEST (CZAS) BINOVIEWER
- Omegon 32mm 70º SWA eyepiece review
- Review of iPolar hardware and software for polar alignment
- Review of the Hubble Optics 14 inch, f/4.6 Premium Ultra Light Dobsonian Tele...
- My experience with the Starizona Landing Pad
- A quick Review of the MIGHTY MAX 12V 100AH BATTERY
- Nexus II Review
- New Moon Telescopes 20”F/3.3 Review
- FIELD TEST OF THE BAADER MAXBRIGHT® II BINOVIEWER
- My Experience using SkyWatch for the Alphea All Sky Camera from Alcor Systems
- Astroart 7 - A Review and "How To" (Part 1)
- My experience using two 80-millimeter long-focus refractors
- GSO 8-inch TRUE CASSEGRAIN
- Celestron Regal 65ED M2
CNers have asked about a donation box for Cloudy Nights over the years, so here you go. Donation is not required by any means, so please enjoy your stay.
Binocular Universe: The Swan and the Lizard
Discuss this article in our forums
The Swan and the Lizard
October is probably my favorite month for stargazing. The night air is clearer than the humid nights of July, August, and even September. And the temperatures are still warm enough that all we need is a sweatshirt or light jacket to spend many enjoyable hours under the sky. Overhead, the Summer Triangle rides near the zenith as evening twilight ends, while the autumn Milky Way streams eastward from Cygnus toward Cassiopeia.
Above: Autumn star map adapted from the book Star Watch by Phil Harrington
Last month, I mentioned that we were going to continue my Stellafane scan of the Milky Way up through northern Cygnus and into its faint neighboring constellation, Lacerta, the Lizard. You probably know Cygnus well, but possibly not Lacerta. Lacerta was one of seven faint constellations created by the 17th-century Polish astronomer Johannes Hevelius. His atlas of the sky, which introduced those constellations, was published posthumously in 1690, three years after his death.
Above: Finder chart for this month's Binocular Universe. Chart adapted from Touring the Universe through Binoculars Atlas (TUBA), www.philharrington.net/tuba.htm
Since the brightest Lacertan stars shine at only 4th magnitude, the constellation's faint, zigzag pattern is tough to make out from any but the darkest observing sites. Binoculars, however, reveal unexpected riches hidden among them, even under moderate light pollution. As you can see from the TUBA chart here, it's a mighty crowded area.
Before we cross into Lacerta, let's pause at M39, one of my favorite late-summer open clusters. M39 lies about 9°, or about 1.5 binocular fields, from Deneb. To find it, scan from Deneb to a small arrowhead of stars just to the northeast. Follow the arrowhead’s aim to a string of six faint stars that continues to the east-northeast. M39 is east of the easternmost star in that line. Look for a tiny, triangular grouping of about two-dozen faint points. Whenever I view it from a dark location, M39 strikes me as looking almost three dimensional, as if it were suspended in front of a blanket of faint stardust.
The sketch below by CN member Rony De Laet also shows a small smudge to the south of M39. That's NGC 7082, a comparatively dim open cluster. As the drawing so clearly portrays, NGC 7082 appears as an oval blur of light with two faint points poking through, one on either end. It's hard to believe that M39 and NGC 7082 each contain about 180 stars, but they do. Their distances explain the difference. M39 is "just" 2,600 light years from Earth, while NGC 7082 is 4,300 light years away.
Left: M39 (above center)
and NGC 7082 (below center) as portrayed by Rony
De Laet through 8x56 binoculars. This
remarkably realistic sketch was made on July 1,
2008 from Bütgenbach, Belgium.
Be sure to visit Rony's web site for more amazing sketches.
North is up.
Working our way slowly toward Lacerta, let's next try for one of the binocular challenges profiled in my new book Cosmic Challenge (available next month "at better bookstores everywhere" from Cambridge University Press). Actually, this isn't just one challenge, but rather, a pair. Here's an excerpt from the book describing them.
IC 5146, known to many by its nickname, the Cocoon Nebula, is a taxing patch of glowing gas, while Barnard 168 is a thin, sinuous lane of darkness that seems to start at the bright nebula and extend far to its northwest.
To spot this celestial odd couple for yourself, begin at the bright open cluster M39 to the northeast of Deneb [Alpha Cygni]. Famous as a bright, loose congregation of stars and covering an area of sky as large as the Full Moon, M39 is best appreciated at very low powers. Be sure to take a moment to enjoy the view.
From M39, steer your telescope 2½° east-northeast to 4th-magnitude Pi-2 Cygni, and then slowly scan southward, watching for the starry background to drop off abruptly. That will be Barnard 168. Because of its length -- more than a degree tip-to-tip -- Barnard 168 is best appreciated with binoculars. My 16x70 binoculars reveal a winding stream of black ink flowing through a valley in the stars.
By following the dark cloud to its eastern end, you will come to a pair of 9.5-magnitude stars. Both are engulfed in the subtle clouds of the Cocoon. Armed with a 22-mm Tele Vue Panoptic eyepiece (46x), my 4-inch refractor, used to make the sketch here, can only muster the slightest hint of the nebula itself, looking like an oval glow surrounding those stars.
The opaque silhouette of Barnard 168 was obvious in my 16x70s from Stellafane in August, but I still couldn't see any hint of IC 5146, the Cocoon Nebula, despite the clear skies. One of my observing projects this month is to try again through my new 25x100 binoculars. From a dark-sky site, both should be evident…hopefully. I'll post an update on my success (or failure) in this column's discussion forum. I'd encourage all readers to do the same and share their experiences with this challenging pair.
Hopping across the border into Lacerta, let's stop at a cluster that's visible in most binoculars. NGC 7209 borders 6th-magnitude HT Lacertae to the south. HT Lacertae is a semi-regular variable that fluctuates between magnitudes 6.1 and 6.4. That variability is far too subtle to be detected by most eyes, but the star's yellowish tint should be evident.
Through my 10x50s, NGC 7209 looks like a soft glow spanning perhaps 20'. The brightest of the 98 stars that call the cluster home shine at 9th magnitude. Although that's below the visibility threshold for 50-mm binoculars, a few faint points are visible in my 16x70s.
You will probably find that NGC 7243 is more satisfying through binoculars. Here, we find some 40 stars gathered into an area about 20' across. Most of the cluster stars shine between 9th and 11th magnitudes, although a few appear a little brighter. Of these, eight are bright enough to be seen through my 10x50s. The remaining stars blend into a circular glow. NGC 7243 is a little less than 3° west of Alpha Lacertae, the constellation's brightest star and one of four that mark the Lizard's diamond-shaped body.
Here is a list of all binocular objects that are plotted on the TUBA chart. That should keep even the most industrious binocularist busy for a while!
Next month, we'll wrap up my Stellafane 2010 experience with a royal visit to the queen of the autumn sky. Meanwhile, if you have comments or suggestions for future columns, I'd love to hear them. E-mail me at firstname.lastname@example.org.
Until November, remember that when it comes to stargazing, two eyes are better than one!
About the Author:
Phil Harrington is the author of Touring the Universe through Binoculars. Visit his web site at www.philharrington.net for a preview of his next book, Cosmic Challenge, coming next month from Cambridge University Press.
Phil Harrington's Binocular Universe is copyright 2010 by Philip S. Harrington. All rights reserved. No reproduction, in whole or in part, beyond single copies for use by an individual, is permitted without written permission of the copyright holder.