- Wireless Telescope Control for Celestron (and Compatible) Scopes
- 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
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: You're My Hero!
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You're My Hero!
Don't you just love a happy ending? I know I do. Picture this. Princess Andromeda, a helpless damsel in distress, chained to a rock as a ferocious sea monster loomed nearby. Just when all appeared lost, our hero -- Perseus! -- plunges out of the sky, kills the monster, and sweeps up our maiden in his arms. Together, they fly off into the sunset on his winged horse to live happily ever after.
Such is the stuff of myths and legends. That story, the legend of Perseus and Andromeda, was recounted in last month's column when we visited some binocular targets within the constellation Cassiopeia. In mythology, Queen Cassiopeia was Andromeda's mother, and the cause for her peril in the first place.
Above: Autumn star map adapted from the book Star Watch by Phil Harrington
This month, we return to the scene of the rescue, to our hero, Perseus. He stands in our sky to the east of Cassiopeia and Andromeda, should the Queen's bragging get her daughter into hot water again.
The constellation's brightest star, Mirfak (Alpha Persei), lies about two-thirds of the way along a line that stretches from Pegasus to the bright star Capella in Auriga. Shining at magnitude +1.8, Mirfak is classified as a class F5 white supergiant. It radiates some 5,000 times the energy of our Sun and has a diameter 62 times larger. Measurements show it to be about 590 light years away.
Above: Finder chart for this month's Binocular Universe. Chart adapted from Touring the Universe through Binoculars Atlas (TUBA), www.philharrington.net/tuba.htm
Examining Mirfak through binoculars shows that it is surrounded by dozens of fainter stars scattered in small clumps and knots. While most of the stars appear white or blue-white, a few might show subtle hints of yellow or orange. For instance, the star Sigma Persei, one of three suns forming a small triangle south of Mirfak, shines with a distinctly orangish hue.
Together, the stars gathered into this football-shaped area form the Alpha Persei Association. A stellar association contains mostly blue-white and white (spectral types O, B, and A) stars, like most open star clusters. Typically, however, the stars in an association are more loosely gathered than those in open clusters. In the case of the Alpha Persei group, some 50 suns are bound by their mutual, though weak gravitational grip. All are about the same distance away as Mirfak, having formed from a common cloud of interstellar gas and dust an estimated 51 million years ago. Eventually, they will scatter as their gravitational embrace continues to weaken.
The Alpha Persei Association is also known as the Per OB3 Association and Melotte 20. The latter refers to its listing in Philibert Jacques Melotte's catalog of 245 open star clusters. The Melotte catalog is a great resource for binocularists, since it contains many targets that are too large to be easily detectable in the narrow fields of telescopes.
The Alpha Persei Association is a beautiful sight through even with the smallest pocket binoculars, as is our next target, open cluster M34. M34 is located roughly midway between Algol (Beta Persei) and Almach (Gamma Andromedae). Algol and M34 are separated by 5°, so depending on the span of your binocular's field, both may just squeeze into the same view.
Through most binoculars, M34 looks like a hazy patch of light about as large as the Full Moon. Look for the brightest of its hundred or so stars twinkling in the soft glow of fainter, unresolved suns. If distance estimates of 1,400 light years to M34 are correct, then the cluster spans about 14 light years edge to edge.
Interestingly, M34’s discovery predates Messier’s first encounter by more than a century. Giovanni Batista Hodierna, an Italian astronomer in the court of the Duke of Montechiaro, was the first to spot it, probably before 1654. Messier independently rediscovered it in 1764.
|Left: The Alpha Persei Association (Melotte 20) as sketched through the author’s vintage extra-wide field 7x50 binoculars. North is up.|
While we are in the area, be sure to pay a call on Algol, the famous “Demon Star.” Algol is a fun variable star to follow through binoculars, but in the past, it was viewed with fear and dread. In the Iliad, Homer described Algol as “a ghastly sight, deformed and dreadful, and a sight of woe.”
Had Homer looked more carefully, he might have noticed an even more dreadful sight – that Algol was actually winking at him. That’s because every 2 days, 20 hours, 49 minutes, the star’s brightness drops from magnitude 2.1 to magnitude 3.4.
Algol is not actually winking at us, of course. These apparent fluctuations are the result of an unseen companion star passing in front of the binary system’s primary star. Each eclipse lasts about 10 hours. As the companion moves off the primary, Algol returns to peak brightness. A second, minor dip in brightness occurs as the companion passes behind the primary. The apparent brightness of Algol keeps it well within naked eye and binocular range across its entire cycle, making it an ideal star for fledgling variable star observers to follow.
To track Algol, compare it periodically with stars of known brightness in its immediate surroundings. Use Gamma Andromedae to the west of Algol at magnitude 2.1, Epsilon Persei to its east at magnitude 2.9, and Kappa Persei to its north at magnitude 3.8. All are labeled on the chart above, while the table here lists the dates this month when Algol will be at minimum brightness.
Finally, let's close this month with a pair of open clusters that are more challenging than the objects discussed above. Both lie east of the Alpha Persei Association, near a double-triangle asterism formed by Lambda, Mu, 48, and 53 Persei.
The easier of the pair to spot is NGC 1528. Under dark skies, my 10x50 binoculars show a perfectly round smudge of distant starlight just beyond a tiny Y-shaped asterism of stars.
NGC 1545 is a tough catch, even through large binoculars. All I can make out is a very subtle hint of its existence around the faint stars SAO 24556 and SAO 24554. My 25x100 giant binoculars add only a few additional dim points within.
For readers who would like to delve deeper still, here is a list of some additional binocular targets plotted on this month’s finder chart. Try your luck with each and report your results in this column’s discussion forum.
Next month, we will kick off 2011 with one of my favorite winter targets, the Hyades. Until then, let me wish you and yours a very merry Christmas, happy Hanukah, happy holidays, and a cloud-free new year. And if you have any comments or suggestions for future columns, please e-mail me at [email protected].
As always, 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 new book, Cosmic Challenge, 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.