THE SOUTHWORTH PLANETARIUM
70 Falmouth Street      Portland,Maine 04103
(207) 780-4249      usm.maine.edu/planet
43.6667° N    70.2667° W  Altitude:  10 feet below sea level Founded
January 1970
2021-2022: XXIX
"I have loved the stars too fondly to ever be fearful of the night."
-Sarah Williams

THE DAILY ASTRONOMER Thursday, October 14, 2021
The Cassiopeia Clock


Aliens, black holes, galaxy clusters, eclipses, and parallel Universes are
all very well and intensely exciting. However, at times, one feels in the
mood for more homespun astronomy, you know, the kitchen made Boysenberry
jam astronomy stored in a mason jar and wrapped in cellophane with a frayed
bow and quaint card bordered by hydrangeas and featuring a rabbit in a
gingham pinafore standing by an oven in the corner.* In other words, simple
night sky astronomy.

So, today, we turn to the Cassiopeia Clock, a celestial device that will
enable observers to keep track of the time. Yes, we know you don't need
anything else to tell you the time as you already have smart watches,
smarter phones, impatient relatives, and google speakers that will tell you
the time, date, weather forecast, the first derivative of the hyperbolic
secant and the thread count of Charlemagne's bedding. However, we're
reverting back to the pre-digital age of turf fires, forest sorcery and
skies unobscured by light pollution.

One can see that the w-shaped Cassiopeia and the Big Dipper are
diametrically opposed relative to Polaris, the north star. At our latitude,
these are all circumpolar, meaning that they'll never set, at least not in
our lifetime. Consequently, we can always find them in a clear sky anytime
of night and anytime of year.

[image: constsp.gif]

As Earth rotates, the stars appear to revolve around Polaris, or, more
correctly, the North Celestial Pole which is less than a degree away from
it. Throughout a 23 hours, 56 minute period**, Cassiopeia and the other
circumpolar constellations complete a circuit around the NCP. As this
revolutionary period is slightly less than the day length, the position of
circumpolar constellations shifts gradually over many weeks.

The above image shows the positions of Cassiopeia and Ursa Major in the
early evening spring sky. Notice that Cassiopeia is descending toward the
horizon while Ursa Major is ascending toward its apex. However, after
midnight, Cassiopeia begins its ascent in the northeastern sky and Ursa
Major begins to move toward the horizon.

In the summer early evening sky, Cassiopeia begins the night low in the
northeast and ascends throughout the night. Cassiopeia is at its highest
position by the pre-dawn.

Cassiopeia begins the night high in the northeastern sky in early autumn
and begins a descent toward the horizon after midnight

One will see Cassiopeia in the northwestern sky in the early winter evening
sky. The ancient queen descends toward the horizon throughout most of the
night and by early morning appears along the horizon.

Ursa Major will always appear opposite Cassiopeia. At times, Ursa Major
will be easier to see than Cassiopeia because the latter will be low along
the horizon. At other times, the situation will be reversed.

We can watch these constellations quite easily in our lovely little
stardome because the northern sky is toward the back of the theatre, the
same location as the console. The true north, the north of the real world,
is actually to the left of the dome's center and, of course, is duly
marked.***

Even if you don't have a quaint star dome at your disposal, you can always
find Cassiopeia in the northern star and, if you can dazzle your loved ones
by using the celestial queen to tell the time. And, yes, being in a house
littered with phone-worshipping teenagers, I am well aware that if it
doesn't beep, flash or explode, it can't possibly dazzle. Give it a go,
anyway.







*Yes, that is what is known as the tidal spaghettification of a metaphor.

**If Earth would only stay still and not revolve around the Sun, life would
be so much simpler. However, the stars rise four minutes earlier each day
as a consequence of Earth's revolutionary motion. For this reason, the
circumpolar stars complete an orbit around the NCP every 23 hours and 56
minutes instead of 24 hours.

***This directional marking was necessitated by recently implemented
University of Maine system consolidation protocol that requires us to
genuflect three times a day in the direction of Orono.


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