March 2013 Constellation
of the Month – Ursa Major
The constellation Ursa Major, the
Great Bear, includes the group of stars (an "asterism") called the "Big Dipper." The Big Dipper comprises less than half the
area covered by Ursa Major; the remainder consists of 3 appendages extending
from the back and bottom of the bowl.
That would be to the South in the early night time sky tonight.
Ursa Major is a circumpolar
constellation. This is explained in the
blog post for our December 2012 constellation of the month, Cassiopeia,
the "W" . Basically,
circumpolar constellations never set below the horizon. They are visible all night every night of the
year. The W and the Ursa Major are
always on opposite sides of the North Star, around which they seem to revolve every
24 hours and every 12 months. Soon after
sunset, Ursa Major is visible to the North and slightly East, relatively high
in the sky, while Cassiopeia is to lower in the sky, to the North and slightly
West. At midnight, Cassiopeia will be at
its lowest point near the northern horizon, and Ursa Major will be at its
highest point.
As is well known, the last two stars
in the bowl of the dipper point to the North Star. The second star, in the middle of the handle
of the dipper, is a double star, which can be made out with the naked eye – if you
have good eyesight. Otherwise,
binoculars or a telescope will make it visible.
The brighter of the two stars, called Mizar, is itself a double star, which
can be seen in a small telescope.
Ursa Major has a number of prominent
deep-sky objects -- objects outside our Solar System – which can be seen with
small telescopes such as those used at Discovery Center astronomy events. The Owl Nebula, M 97, is a planetary nebula
(explained in last month's blog post) with two dark round patches that give the
appearance of an Owl's eyes. It is
located below the middle of the bowl of the dipper. The Owl Nebula is in our Milky Way galaxy,
about 2,600 light years away. M81,
Bode's Galaxy and M82, the Cigar galaxy are about 5,000 times as far away. Some tens of millions of years ago, these two
galaxies nearly collided. Each of their
gravitational fields affected the other, causing some disruption in their shapes,
and facilitating the formation of new stars.
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