- A Review of Teeter STS18
- MesuMount 200 Review
- First Light with the Prototype 8x42 Space WalkerTM 3D Binoculars
- INTERSTELLARUM DEEP-SKY ATLAS (FIELD EDITION) REVIEW
- THE BAADER BBHS-SITALL SILVER DIAGONAL
- Explore Scientific AR 102
- Review: davejlec's Paralellogram Mount
- Annals of the Deep Sky, Volumes One and Two
- Discovery 17.5” Split Tube Dobsonian Telescope
- REVIEW OF SUMERIAN OPTICS ALKAID 16” TRAVEL SCOPE
- Astrotrac TP3065 Pier Review
- Apo-tmosphere: Gutekunst ADC Review
- Optolong LRGB Filter Testing and Comparison with Baader LRGB Filters
- First Light Review: Teeter Custom TT Planet Killer 16" f/5.4
- The Baader Planetarium Morpheus
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Binocular Universe: Lyre, Lyre
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The brilliant stellar sapphire Vega sparkles high in the west this month. Famous as the fifth brightest star in the entire night sky, Vega is so dazzling that it punches through even the most severe light pollution. You simply can't miss it!
Above: Autumn star map from Star Watch by Phil Harrington.
Above: Finder chart for this month's Binocular Universe.
Chart adapted from Touring the Universe through Binoculars Atlas (TUBA)
The next chance you get, take a look at Vega through your binoculars. As you are enjoying its blue-white luster, consider that the light you are seeing is only 25 years old. Twenty-five light years works out to be 147 trillion miles. That’s just a town or two away on the cosmic distance scale. We're practically neighbors.
Vega's constellation of Lyra symbolizes the lyre, or harp, owned by the mythological musician Orpheus. Vega marks a portion of the harp's handle, while four fainter stars in a parallelogram frame its body. Light pollution may hide those four stars, so if you can't make them out by eye, try using your binoculars instead. Each is well worth a closer look.
For instance, there is more to 3rd-magnitude Sheliak (Beta [ß] Lyrae), at the parallelogram's southwestern corner, than just a faint star. Sheliak is actually an eclipsing binary that is perfect for binocular study. Over the course of just under 13 days, an unseen companion star causes Sheliak to flicker from magnitude 3.3 to 4.3. Use the chart here to monitor the changes in appearance. By comparing Sheliak's brightness to that of nearby stars that do not vary, can you confirm its 13-day cycle?
The most photographed planetary nebula of all, M57, the Ring Nebula, lies along the southern edge of the harp's parallelogram. To spot it, look midway between Sheliak and Sulafat (Gamma [?] Lyrae) for three very faint stars that create a tiny right triangle. The star at the right angle is actually the Ring. Although it takes at least 50x to make out the classic smoke-ring shape, I've seen M57 as a faint star-like point through binoculars as small as 7x35s. Give this challenge a try tonight and let me know if you are successful. I would be interested in finding out just how small a pair of binoculars will uncover M57.
Now scan southeast of Sulafat, toward the star Albireo in Cygnus, and pause about halfway in between. There, you'll find a conspicuous asterism of stars shaped like a number 7. If you look just to the 7's southeast, you should also spot a faint smudge that doesn't quite look like a star. That's the globular cluster M56. Although 100,000 stars make up M56, the cluster is much too far away to be resolved through binoculars. That task requires at least a 6-inch aperture.
Even the smallest pocket binoculars, however, will reveal Delta (d) Lyrae, at the parallelogram's northeastern corner, as two close-set stars. In fact, some sharp-eyed stargazers don't need any optical aid at all to see them. The brighter star in the pair, 4.3-magnitude Delta-2, looks orangish, while 5.6-magnitude Delta-1 is bluish-white.
The two Delta stars belong to a scattered open cluster nicknamed, appropriately, the Delta Lyrae Cluster and cataloged as Stephenson 1. Fifteen stars belong to Stephenson 1, though most are too faint for binoculars. Although both Deltas are members of the cluster, they are not a true binary system. Studies suggest that Delta-1 lies about 1,200 light years away, while Delta-2 is about 200 light years closer to us.
Open cluster Stephenson 1 as portrayed through the author’s 16x70 binoculars.
The next stop on our tour is Epsilon (e) Lyrae. Look for it just to the northeast of Vega. If you have sharp vision, you may also be able to split Epsilon into two stars with eye alone. The stars are separated by 3.5 arc-minutes, which is near the naked eye's resolution limit. Of course, with binoculars, Epsilon is easy to resolve into two points of light. The northernmost of the pair is labeled Epsilon-1, while the southern member is Epsilon-2.
This system is also known as the Double-Double, as Epsilon-1 and Epsilon-2 are each close-set pairs of stars. Unfortunately, it takes at least 80x to see all four Epsilon affiliates. Even though we can see only two stars in binoculars, the added beauty of gleaming Vega to the southwest and Zeta Lyrae to the southeast create a very pretty binocular scene.
But wait, there's more! Zeta (?) Lyrae is actually a challenging double star for binocular viewing. Zeta is composed of 4th- and 6th-magnitude suns separated by about 44 arc-seconds. The fainter companion lies due south of the brighter star. I can just make out both through my 10x50 binoculars, while the added oomph of my 16x70s cleaning resolves them. Both impress me as shining pure white. How about you?
Earlier, we discussed how Sheliak is a fun variable star to monitor through binoculars. If you are a devout variable-star fan, then you may already know about R Lyrae. R is a type-M red semi-regular star that fluctuates between magnitudes 4.0 and 5.0 over the course of 50 days. Look for it in the northern part of the constellation, about 6° northwest of Vega.
We also have RR Lyrae tucked just inside Lyra's northern border. With great precision, this star rises to magnitude 7.1, falls to magnitude 8.1, and then brightens back up again in just 13 hours, 36 minutes. RR Lyrae heads up a class of variable stars that are also known as "cluster variables," since many are found within globular clusters. RR Lyrae stars are well known for their period-luminosity relationship. By studying the magnitude variations of RR Lyrae stars versus their periods of variability, astronomers can calculate the stars' true luminosities. By knowing both the luminosity and apparent magnitude, the distance to the star can be calculated.
All three variables are shown on the finder chart above, along with several suitable comparison stars that can be used to judge each variable's magnitude value. The visual magnitude of each comparison star is shown in italicized green type, with the decimal point omitted to avoid confusing it for a faint star. For instance, the number 43 next to Zeta Lyrae at the parallelogram's northwestern corner indicates that Zeta shines at a constant visual magnitude 4.3.
About the Author:
Phil Harrington has written 9 books on astronomy, including Star Ware, Star Watch, and his latest, Cosmic Challenge. Visit his web site, www.philharrington.net, for more information.
|Phil Harrington's Binocular Universe is copyright 2012 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.|