 Crescent
Moon and Venus Observing
the Moon There
are few things in nature more beautiful than the sight of a darkening
twilight sky adorned with an Earthshine- blue-tinted crescent Moon,
surrounded by a sprinkling of stars and one or two bright planets
nearby. When magnified through binoculars the crescent Moon becomes a
gleaming sickle with a dented edge, and through a telescope our
satellite is transformed into a spectacular alien landscape. Even small
binoculars will show a wealth of lunar detail.
During
the
four centuries since the telescope was invented, watchers of the Moon
have discovered that lunar observing is the most visually rewarding
branch of amateur astronomy. The constantly changing vistas of the
Moon’s surface are every bit as stimulating as the greatest
artistic masterpieces. Lots can be learned about the Moon through
careful observation, even using the unaided eye.
Following the Moon The
Moon’s orbit around the Earth is tilted by just 5 degrees to
the
ecliptic
– the path followed by the Sun during the year
–
and the Moon slowly moves from west to east (right to left in the
northern hemisphere), covering the distance of a little more than its
own diameter each hour. The Moon therefore travels just over
13°
each day – about the width of your outstretched
hand.
 The phases of the
Moon, with new Moon at right and full Moon at left
Phases Because
of the changing angle of lighting by the Sun, the Moon goes through a
complete set of phases from new Moon, through full Moon and back
again to new Moon in 29.5 days. This period is called a
synodic month,
or lunation.
Because the Moon’s orbital plane is
so close to the ecliptic, its monthly path among the stars is similar
to that followed by the Sun during a whole year. When
the Moon is increasing in phase or illumination it is said to be
waxing, and when it is decreasing in phase it is waning. The waxing
half Moon is known as first quarter because at this point the Moon is a
quarter of the way round its orbit, while the waning half moon is last
quarter. The phases between the quarters and full Moon are known as
gibbous phases.
The
Moon’s visibility and its height above the horizon change
according to its phase and the time of the year. Full Moon is always
on the opposite side of the sky to the Sun, in the same region of sky
where the Sun will be in six months’ time. From the UK, the
Sun
of the winter solstice is at its most southerly and climbs to its
lowest point above the southern horizon. Around the same time, the
mid winter full Moon rides very high in the early morning
skies.
At summer solstice the Sun reaches its highest point above the
southern horizon, which means that the mid summer full Moon
barely clears the southern horizon.
For
UK-based observers, the range of intervals between successive
Moonrises varies from a quarter of an hour up to as much an hour and
a half because of the varying angle at which the ecliptic (and the
Moon’s orbital plane nearby) intersects the horizon. Around
the
days of full Moon in autumn the ecliptic makes a very shallow angle
with the eastern horizon, causing the Moon to rise just 15 to 20
minutes later each evening. Astronomers
often refer to the age of the Moon in days. This means the number of
days that have elapsed since new Moon. First quarter is about seven
days, and full Moon is about 14 days.Moon lighting
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