The brilliant stars that make up Orion, Taurus,
Gemini, Canis Major, and Auriga dominate the winter sky, but there are many less
showy constellations that nevertheless contain some fine binocular targets that
often go unnoticed. This month, we are going to pay a visit to two of those
constellations, both found south of the mighty Hunter.
Above: Winter star map from Star
by Phil Harrington.
Finder chart for this month's Binocular Universe.
adapted from Touring
Binoculars Atlas (TUBA)
Let's start with Lepus, the Hare. While the Hare does
not play a specific role in any particular myth, its location so close to
Orion's large dog, Canis Major, suggests it is taunting the dog into action. The
Greek poet Aratus wrote that Canis Major is "close behind he rises and as
he sets he eyes the setting hare."
The four brightest stars in Lepus form a trapezoid
immediately south of Orion. But with the brightest, Arneb (Alpha Leporis), only
shining at magnitude 2.6, the Hare holds little to grab naked-eye attention. For
those willing to delve a little deeper with binoculars, however, Lepus holds
some fine deep-sky "carrots" that are worth fleshing out.
First, we pay a call on Gamma Leporis, the
southernmost star in the Lepus trapezoid. Gamma is a superb double star awash in
vivid color. Separated by a wide 97" of arc, they constitute one of the
finest binary stars in the entire binocular sky. The system's 3rd magnitude
primary sun is a striking yellow orb while the 6th magnitude secondary star
appears as an orangish point of light. Interestingly, some visual astronomers
refer to the companion's color as pale green, but that is merely a byproduct of
the human eye's color receptors, not the star itself. In reality, the yellowish
primary star is spectral type F, making it a little hotter than our type G Sun,
while the companion is spectral type K, meaning it is a little cooler. Estimates
place at least 870 Astronomical Units between the stars, resulting in an
excruciating long orbital period of some 18,000 years. Together, they reside a
little more than 29 light years from Earth.
Next, we have another colorful character, the classic
long-period variable star R Leporis. Across a 432 day cycle, R pulses
between magnitudes 5.5 and 11.7. When it's near peak performance, R puts on a
real show through binoculars radiating a magnificent red hue. This appearance,
first noted in 1845 by the English astronomer J.R. Hind, led to the star's
better known nickname Hind's Crimson Star. Hind described it "blood-drop on
the black background of the sky."
Spectral analysis indicates that R Leporis is a rare
carbon star. Carbon stars are low temperature red giants engulfed in atmospheres
that are unusually rich in carbon compounds. Other noted carbon stars visible in
binoculars include V Hydrae and S Cephei.
Lastly, we find M79, Messier's only winter
globular cluster. Pierre Méchain was first to spot this 8th-magnitude object in
October 1780. He recorded it as simply a nebulous object, which certainly
describes its appearance through binoculars. M79 may be most easily found by
drawing an imaginary line from Alpha Leporis to Beta Leporis and continuing it
an equal distance to the latter's south. Look for a soft, circular glow.
Resolving any of its myriad stars is out of the question for binoculars. They
lie in the realm of moderately large telescopes.
Continuing southward, we find Columba, the Dove, a faint
southern constellation wedged between the far more brilliant regions of Canis
Major and Puppis. Its origin dates back to the 17th century, when it was first
depicted on Bayer's 1603 star charts as a dove near the mighty ship Argo Navis.
While the monstrous constellation Argo has since been sliced into separate
constellations, little Columba remains untouched.
NGC 1851 is the only non stellar deep sky object
within Columba that is bright enough to crack the binocular barrier. Finding it
can be a bear from mid-northern latitudes, since it lies so far south of the
celestial equator. At declination -40 degrees, it culminates no more than 10
degrees above my Long Island horizon. Add to the fact that there are no bright
stars anywhere in its immediate vicinity, and NGC 1851 can prove very
challenging. Be prepared to search for awhile. Once spotted, however, this
7th-magnitude globular cluster will look like a small, circular patch of fuzzy
light. In fact, given a good vantage point, it easily outclasses M79. It would
undoubtedly have been in the Messier catalog were it not so far south. But as it
was, NGC 1851 went undiscovered until James Dunlop bumped into it on May 29,
1826. Recent studies suggest that it's a runaway from the Canis Major Dwarf
galaxy, which was only discovered in 2003.
As you can see from the listing below, there are plenty
of binocular targets awaiting you in this month's Binocular Universe. Be sure to
take the time and brave the cold to enjoy all that this season has to offer.
And until we meet again
next month, remember that, in 2014 as in the past, for
stargazing, two eyes are better than one!
About the Author:
Harrington has written 9 books on astronomy, including Star Ware,
Watch, and his latest, Cosmic Challenge. Visit his
web site, www.philharrington.net,
copyright 2014 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