| The solstices represent the beginning of summer
and winter, causing the daylight hours to be longest on one side of the Equator
and shortest on the other. The extremes of the solstices are experienced
at the poles, which receive nearly continuous daylight or continuous
darkness. Six months later, when the Earth is exactly halfway around its
solar orbit, the opposite conditions are experienced.
Between the June and
December solstices the Earth’s axis is positioned sideways towards the
sun. When halfway between solstices, the sun’s rays strike the Equator
perpendicularly, causing both hemispheres to briefly receive equal
sunlight. Day length is then the same everywhere. These two positions are
known as the equinoxes, marking the beginning of spring and autumn.
The Tropics |
| Tropical
regions experience the least variation in day length between the seasons.
Their position near to the centre of the sun's exposure on Earth, means
that day length here is never far from average.
On the June solstice the sun's rays are
perpendicular to Earth at a certain latitude which is either north or
south of the equator. On this day, the sun appears to reach its midday
height in the exact vertical centre of the sky. These latitudes
are the geographical limits of the tropics-the equatorial regions which
have a consistently warm climate.
The Northern Hemisphere's tropic line is known as
the Tropic of Cancer and lies at 23°27'
North. The corresponding line in the southern hemisphere is the Tropic
of Capricorn, and lies at 23°27' South. Not surprisingly, these
angles represent the exact tilt of Earth in its orbit around the sun. If
there were no tilt, the sun would always be directly above the equator,
and there would be no seasons as we know them.
Star Positions |
| As the Earth moves, so
does its relationship to the stars and other astronomical bodies. Indeed,
the stars and planets appear to move around Earth, although it is actually
Earth that is moving. This perceived movement of the stars at night has
been a major influence in the development of navigation and geography, as
well as in the world’s cultures and religions. The appearance is
complicated by the fact that the planet is both spinning on its own axis
and orbiting the sun on another axis.
A person’s view of the night sky is influenced
by the seasonal progression of daylight and the night-time. For example,
Orion—a winter constellation in the northern hemishphere—is situated
in the daylight sky in midsummer and since the light of the sun is
stronger, it cannot be seen. As the seasons progress, the night side of
the planet turns toward Orion, which is then visible in the night sky. A
slightly different view of the stars is therefore presented each night,
and the skyscape is the opposite at the summer (June in the Northern
hemisphere) and winter (December) solstices. Constellations near the
horizon disappear from view entirely for one season and then gradually
appear again.
Comets and planets have their own complicated
orbits around the sun, so their patterns of movement in the sky do not
correspond to the more predictable wanderings of the stars. The position
of the stars is also affected by two other factors. First, the Earth’s
tilt on its axis moves slightly backwards and forwards over a period of
many years, altering the celestial view. Second, the stars themselves
travel through space on their own trajectories, and the constellations
change their shape over many centuries.
People have been trying to understand the
position of the stars since long before recorded history.
Constellations—visual groups of stars that resemble familiar
objects—were the first attempt to classify the stars. The constellations
recognized by different cultures through time depended on historical
precedent, cultural factors, and geography. To locate certain stars for
study and navigation, astronomers, astrologers, and navigators still use
the constellations familiar to the ancient civilizations of the Mediterranean,
Central America, China,
and elsewhere.
Although the stars have always been important to
religion, navigation and agriculture were the main practical reasons for
organizing them into recognizable and predictable entities. Stars that
appeared to hardly move were particularly valuable in navigation,
especially Polaris, the North Star of the northern hemishphere, and the
constellation Octans of the southern hemisphere. These are the visible
stars most closely aligned with the axis of Earth.
Modern astronomy uses star charts to make star
navigation more accurate. The stars appear to be spread over the inner
surface of a sphere, so star charts have spherical qualities, like a globe
turned inside out. They are usually organized into Northern and Southern
Hemisphere views that are divided into 24 hours or radial sectors with
180-degree increments between the horizons. Charts of the equatorial
skies, up to about 30° north or south of the equatorial horizon, are
often represented by rectangular maps which are also divided lengthwise
into 24 hours. Star charts are not static like Earth maps because they
usually display seasonal views of the sky from a particular point. They
can also show the entire sky irrespective of season but with some
indication of the seasonal change.
Climate |