Introducing the Night Sky
Part 4
by John Harper
There is one more celestial object which I should describe before we
return to the
stars, and that is the moon, which waxes and wanes from crescent to
full and back
to a crescent again within the period of a month. Actually, the average
time between
two consecutive full moons is 29 days, 12 hours, 44 mins, 2.9 secs. The
various
appearances of the moon, the shape it appears to be in the night sky,
are called
phases. The phases of the moon are caused by the angle at which
sunlight falls on
the moon, and also where the moon happens to be in relation to the
earth at the
time.
Earth and Moon
(Painting by John Harper)
At new moon, both moon and sun are in the same part of the sky, and as
a result,
the night side of the moon is facing us. At this time, the moon cannot
be seen at
all - it is lost in the sun's glare. Within the week following new
moon, the thin
crescent begins to appear in the western twilight and after sunset. At
this time
it is possible to see a most beautiful phenomenon called 'Earthshine',
faintly illuminating
the rest of the moon's disc. What we are seeing is the light of ourown
planet reflected
from the lunar night surface, rather like the full moonilluminating the
landscape
on earth at night. In days gone by, this beautiful sight was often
referred to as
'The old moon in the new moon's arms.'
Earthshine
"The old moon in the new moon's arms"
Seven days or so after new moon, the moon looks like a capital letter
'D' in the
sky - it is now at first quarter, and it has covered a quarter of its
orbit of the
earth. This is an ideal time to see the craters through binoculars.
Notice how they
are best seen near the straight edge, or Terminator, as it is properly
called. The
Terminator is the line of lunar sunrise at this time, and the craters
are easy to
see because they are filled with deep shadows cast by the low rising
sun.
Most lunar craters
are believed to have been produced when the moon was bombarded
by thousands of lumps of rock in the early days of the solar system,
some 4 000
million years ago. They are the circular depressions covering much of
the lunar
surface. The largest crater on the earth-facing hemisphere of the moon
lies near
the southern edge or 'limb' of the moon, and is called Bailley, a
crater over 180
miles (300km) in diameter.
Craters on the Moon
(Photograph by J. Harper)
During the next week, the moon becomes gibbous or three quarter in
shape, until,
a fortnight after new moon, the moon becomes full. Our satellite is now
opposite
the sun in the sky, and has accomplished half of its orbit around the
earth. Full
moon is the best time to see the lunar Maria, or seas. These are the
relatively
dark smooth planes once thought to contain water, but which are in
reality, vast
lava flows filling huge impact basins of the distant past. It is these
dark areas
that in our mind's eye we see as the 'man in the moon' and other
fanciful figures,
such as the Lady, the Crab, the Hare, and even the Poodle, in the moon!
The Full Moon
A week later, the moon has waned to last quarter, when it is about to
start the
last quarter of its orbit of earth. It now looks like a reversed
capital D. Seven
days after this, the moon is new again, and lost once more in sunlight,
ready to
recommence its cycle of phases all over again.
Occasionally at new
moon, when the earth, moon and sun line up exactly in that order,
we can witness the awe-inspiring spectacle of a total eclipse of the
sun. At this
time, the moon's shadow falls on the earth, and in the cone of the
shadow everything
becomes cold and dark as the moon covers the sun's disc, cutting off
the light and
heat for several minutes.
A total eclipse of the sun
When the sun, earth and moon line up exactly at the time of full moon,
we can observe
an eclipse of the moon. On this occasion we watch the moon pass into
the earth's
shadow. The moon often becomes dim and russet coloured, and can look
most strange
during a lunar eclipse. The colour effect is due to sunlight being
refracted (bent)
through earth's atmosphere onto the moon.
Total eclipse of
the moon
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to Part 3
Written by John Harper for Diarmid's
Observatory
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