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- Binocular Universe
Binocular Universe: Orion's Arm
Voice your opinion about this subject in our forums
favorite constellation, Orion the Hunter, stands tall in the January sky.
He's like an old friend who returns every year just to check in and say
"hello." We have visited
him before in this e-column, enjoying the treasure of the Orion Nebula, M42, as
well as some other sights, including M78 and his "Belt Cluster,"
Collinder 70. All are worth
revisiting on every clear winter's night. But
this time around, we are going to pay a call on some new targets that often go
Above: Winter 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)
begin our visit to the Hunter with his “Alpha” star, brilliant Betelgeuse.
While many of Orion's stars are happily fusing hydrogen into helium
within their cores, Betelgeuse has been there, done that.
Though estimated to be less than 10 million years old, Betelgeuse has
lived life fast and furious. The
hydrogen supply in its core was exhausted long ago, causing the star to swell
into an enormous red supergiant. Today,
heavier elements are undergoing fusion in its core.
In the process, internal pressures have bloated its outer diameter.
Were it centered in our solar system, Betelgeuse would extend beyond the
four inner planets and continue halfway out to Jupiter.
Eventually, its central process will end and Betelgeuse will go out in a
burst of glory as a supernova. When
will that happen? Experts tell us
sometime in the next million years or so. For
now, enjoy its brilliant ruby red color.
Betelgeuse’s designation as the Alpha star in Orion makes a fun footnote in an
astronomical trivia contest. When
Johann Bayer originally conceived his star-designation system based on the Greek
alphabet in his 1603 star atlas Uranometria Omnium Asterismorum, he
sorted the prominent stars in each constellation in order of descending
magnitude. Alpha was reserved for
the brightest in each constellation, followed by Beta, Gamma, Delta, and so on.
But he messed up in Orion as well as a couple of other constellations.
Betelgeuse, it turns out, is not the brightest star in Orion; Rigel is.
Betelgeuse varies between magnitudes +0.3 and +1.2, while Rigel is rated
magnitude +0.1. Perhaps Bayer was
victim to what’s called the Purkinje Effect. This
optical illusion causes red stars to grow in brightness the longer you stare at
arm is usually shown on star maps as raised high above Betelgeuse and holding a
club to do battle with Taurus, the Bull. Let’s
trace his arm northward from Betelgeuse, stopping at a few interesting spots
along the way. First, some 7 degrees
north of Betelgeuse, we come to open cluster NGC 2169. Look for it to
the southeast of the midpoint between Nu Orionis and Xi Orionis.
This small, bright open cluster is made up of about 30 stars ranging from
magnitudes 8 to 10. Binoculars reveal the four brightest cluster members buried
in a small, misty glow. In addition,
there are two small asterisms just to the southeast of NGC 2169 that make a fun
addition to the scene.
Left: NGC 2169 and surroundings as seen through the author's 10x50 binoculars.
open cluster, NGC 2194, is plotted to
the southeast of NGC 2169 on the chart above, but poses a much tougher
challenge. The best I can muster in
my 10x50 binoculars is a faint suggestion of its existence, and only then under
clear, dark skies. How about you?
trace out Orion’s raised right arm northward, you’ll pass many neat little
patterns of stars dotting the way. Although
they are not true star clusters, each certainly adds to the beauty of this rich
region of the winter sky.
pause at the top of Orion’s arm, marked by Chi-1 and Chi-2 Orionis.
Scan just 2 degrees to their east and you will find NGC
2175, an often-ignored open cluster. I
bumped into it again not long ago through my 10x50s and saw it as a small tuft
of celestial fuzz. An arrow-shaped
asterism to its southeast points the way.
large, but little known open clusters from the Collinder catalog also reside in
this part of Orion. First, there is Collinder
69, which includes Lambda Orionis, the star at the top of the Hunter's tiny,
triangular head, as well as with several dozen fainter suns within about 1
degree. Most binoculars reveal
between 15 and 20 stars ranging in brightness from 5th to 9th magnitude.
Studies also show that, like Betelgeuse, Collinder 69 is probably no more
than 10 million years old.
second Collinder cluster, Collinder 65,
is north of Orion’s head and spills into adjacent Taurus. By adding a few
non-cluster stars to the east and north, I imagine this cluster as a spear that
Orion is about to heave at the Bull. "Orion's
Spear" measures about 8° tip to tip, which makes it perfect for 7x and 8x
find our final target this month, you'll need to head east from Betelgeuse and
cross the border into Monoceros. A
unicorn by design, Monoceros contains several noteworthy open clusters for
binoculars. We will visit several
next month, but for now, we pause at NGC
2251, 10 degrees due east of Betelgeuse.
Listed among the targets that make up the Astronomical League Deep-Sky
Binocular Club's observing list, NGC 2251 shows a tiny knot of unresolved
starlight in my 10x50s, nestled in a grand field of view that includes NGC 2244
about half a field of view to the south. Revisit
my February 2010 e-column for more information on that pretty open cluster as
well as the huge wreath of nebulosity -- the Rosette Nebula -- that surrounds
2244 is just one of the many other objects awaiting you in this month’s
Binocular Universe. Here is a list
of many more.
I hope that 2013 bring
us all many clear nights to get out and enjoy our universe.
And of course, in the new year as in the past, remember that for
stargazing, two eyes are better than one.
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 2013 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.|