The March Sky
By Paul Curtin
Saturn is the planet to watch this month.
The rings are especially well placed for observation. Price
(1) and Alexander (see Moore in (2)) cover the basics of observing
disk and ring features. Those wishing to draw Saturn may wish
to consult these texts for templates displaying the range
of ring inclinations. Dobbins et al. (3) and Price (1) have
excellent sections on observing and identifying the components
of the rings.
The March Sky
Northern March is a month of open clusters
and an introduction to the season of galaxies. The south enjoys
warm nights and fantastic Milky Way objects.
Let us begin by forming a triangle with Polaris
at the apex, the western side is the seventh hour line to
southern Camelopardalis (this line, continued south, would
divide Gemini into roughly equal portions), and the western
stars of the Big Dipper form the eastern side. In this region
one finds dozens of faint nebulae, all of which are galaxies
far removed from our Milky Way. These galaxies belong primarily
to the Coma-Virgo Super cluster to which our Local Group belongs.
The brightest of these are M81 and M82. Wide field telescopes
and binoculars will show them both in one field. The contrast
in shape is quite striking. Due to the lack of bright signposts,
locating these objects is a real challenge. But those interested
in deep-sky objects should take this opportunity to hone their
star-hopping skills and compare the great range of galactic
morphologies.
For observers interested in easier finds,
we turn now to M44, east of Gemini. M44, also known as the
Praesepe, is the heart of Cancer. This is a delightful open
cluster best observed with binoculars. In early March one
can still compare the Pleiades, the Hyades and M44 with respect
to color, density and overall brightness. In addition to M44,
Cancer boasts a number of interesting stars. Using a telescope,
try to split Iota Cancri, a green-orange pair due north of
M44.
To the south of Cancer is a rough circle
of stars that constitutes the head of Hydra. West of this
is the bright star Procyon in Canis Minor. Scan the area southward
for the open clusters M46 and M47 in Puppis. M48 can be found
by scanning north and east of M46, but it can be hard to find
due to the lack of guide stars.
In the south the Milky Way in Puppis and
Pyxis provides us with many objects of interest. M93, due
east of the feet of Canis Major, is a fine open cluster. Scan
southwards from here, following the dense star fields on the
eastern edge of the Milky Way. NGC 245 is a large open cluster
in Puppis. Moving south note the star clouds of Vela and Carina.
Beyond the western edge of the Milky Way in Carina is NGC
2516, a very wide open cluster. Use binoculars or a wide field
telescope to catch the entire cluster.
The Planets in March
Mercury is in the evening sky after sunset. The first half
of March will present northerners with their best view of
Mercury this year.
Venus is not visible this month.
Mars rises a few hours before the sun. It continues to brighten
although its disk is still a fourth of what it will be at
opposition.
Jupiter, in Virgo, rises after dark and outshines everything
in the sky including Sirius.
Saturn is still in Gemini rising before dusk and setting
early in the morning. The rings are still well placed for
viewing.
References
1. F. Price, "The Planet Observer's Handbook,"
Cambridge: Cambridge University Press, 1994.
2. P. Moore (ed.), "Practical Amateur Astronomy,"
London: Lutterworth Press, 1975.
3. T. Dobbins, D. Parker and C. Capen, "Introduction
to Observing and Photographing the Solar System," Richmond:
Willmann-Bell, 1988.
Bibliography
Robert Burnham, Jr., "Burnham's Celestial Handbook,"
New York: Dover, 1978.
R. Gupta (ed.), "Observers Handbook 2005," Toronto:
University of Toronto Press, 2004.
G. R. Kepple and G. W. Sanner, "The Night Sky Observers
Guide," Richmond, VA: Willmann-Bell, 1999.
W. Tirion, B. Rappaport and W. Remaklus, "Uranometria
Deep Sky Atlas," Richmond, VA: Willmann-Bell, 2000.
T. W. Webb, "Celestial Objects for Common Telescopes,"
New York: Dover, 1962. 
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