Planetary
Cartography
Astronomers have developed various methods of distinguishing features
on the surface of a planet. Each hemisphere is divided into a number of
provinces, tropical and non-tropical, with each province generally acquiring
a number and a name. Each hemisphere also has a "polar cap".
The planetary surface features are usually classified in the following
way:
| anguis | meandering fissures | mons | mountains | ||
| catena | chains of cratersv | patera | an irregular crater with jagged sides | ||
| chasma | canyons or gulfs | planitia | a large flat expanse i.e. a plain | ||
| craters | craters | planum | plateau's | ||
| dorsa | ridges | terrae | continents | ||
| fossa | gorges, or long narrow valleys | tholus | a hill | ||
| labyrinthus | a network of valleys cutting though a flat region | vallis | a valley | ||
| mensa | flat-topped protuberance ringed by cliffs | vastitas | vast low-lying plains |
Very often mountains, valleys, craters and other features are named
after famous scientists, astronomers and pioneers who have contributed
to the advancement of astronomical knowledge.
The Moon
The average distance of the moon from earth is 384,400 km (238,906 miles).
This is an average because the moon's orbit is elliptical. The moon's
apparent size varies by as much as 10 percent during the lunar cycle,
because of it's distance from the Earth.
The moon is thought to be round, but there is a slight flattening in the
visible face, i.e. the lunar hemisphere that faces Earth, while the far
side of the moon is slightly raised. Despite being raised, the far hemisphere
has at it's center a large depression about 1400 km in diameter and 5
km in depth. Conversely, the near side, despite being flattened, has at
it's center the Appenine Mountain chain, which reaches an elevation of
3 km.
The orbit of the moon is mainly determined by the attraction of Earth,
but the gravitational forces of the Sun and the other planets introduce
perturbations. This makes the precise calculation of the moon's orbit
somewhat tricky.
The moon's rotation about it's own axis has one noticeble characteristic
- it coincides with that of the earth, so that the same side of the moon
always faces the earth. However, because of slight variations in the rotational
speed at perigee and apogee, people on Earth get to see about 59% of the
surface of the moon at one time or another.
The moon's geographical features were orginally named in the 17th century.
The craters visible from Earth bear the names of scholars, poets, artists
and philosophers of the past, such as Newton, Plato and Descartes.
Depressions on the lunar surface were originally thought to be seas or
oceans, and are called maria (latin for sea). There are two main
groups of seas, the "favorable" seas, Sea of Nectar,
Sea of Tranquility, Sea of Fertility, etc, and the "dangerous"
seas, Sea of Storms, Sea of Cold, Ocean of Tempests,
etc. The most pictureseque name on the moon is probably that of the mare,
the Lake of Dreams.
The mountain ranges are named after their similarity to their earthly
counterparts, Alps, Appenines, Carpathians, Pyrenees,
etc.
See the Map of the Near Side of the Moon.
(800 KB)
Lunar rock samples have indicated that the moon's
surface has less volatile elements, compared to Earth, such as carbon
and oxygen, but is richer in other elements, such as titanium, iron, calcium,
magnesium and other rare earths. So far, two minerals found on the moon
have never been observed before, tranquillite, found near the Sea
of Tranquility, and pyroxyferroite, a silicate of iron and calcium.
Tectonically, the moon is relatively calm. Although there are about 3000
earthquakes per year, they are of very low intensity, occur at depths
of approximately 1000 km, and are barely detectable on the surface of
the moon. The most active epicenter for quakes is under a small mountain
range between the Sea of Humors and the Sea of Clouds.
The temperature on the moon ranges from a maximum of 117 degrees Centigrade
in daytime to a minimum of -170 degrees Centigrade at night.
Venus
The orbit of Venus around the sun is almost precisely
circular, so the planet is always about 108 million kilometers from the
sun. Seen from Earth, Venus seems to shift from one side of the sun to
the other, sometimes rising before the sun as a "morning star"
and sometimes setting after the sun as an "evening star". For
this reason, people of ancient times believed that Venus was actually
two different celestial bodies, known as Phosphoros and Hesperus to the
Greeks, and Lucifer and Vesper to the Romans. Venus is also known as the
shepherd star.
Venus is similar in size and mass to earth, but the crust of Venus is
thicker and appears to consist of a single basaltic tectonic plate which
supports the plains and mountainous regions. The atmosphere of Venus is
composed almost entirely of carbon dioxide. It has a permanent cloudy
mantle, and layers of mist, and the clouds contain droplets of suphuric
acid. There are strong upwards and downwards drafts. Temperatures on the
ground are about 450 degrees centigrade, owing to the greenhouse effect
of the atmosphere.
Venus has large amounts of heavy metals such as lead and bismuth. It is
believed that metals melt in the high temperatures at ground level and
condense at higher altitudes, coating the mountain ranges in a bright
metallic layer or skin, and contributing to the reflective sheen of Venus.
Metallic mountains of Venus
Sixty percent of the surface of Venus consists of
a vast plain with altitudes not exceeding 1000 meters. There are two large
mountainous regions on the surface of Venus known as Terra Ishtar
and Terra Aphrodite. Terra Ishtar is the size of the United
States and it's central region is a large plateau called Lakshmi Planum
with an altitude of about 3 kilometers.
See the Map of Venus. (400 KB)
Mars
It is now believed by astronomers that the surface of Mars consisted in ancient times of one-third water, owing to an ocean-like depression in the northern hemisphere of Mars. Scientists have named the two features suspected of being ancient shorelines Arabia and Deuteronilus. The long lines on the Martian surface rise and fall in a way resembling a landscape with a rising elevation etched by sea waves.
This raises the possibility
of Mars having once had a civilization. Researchers
have recently discovered seven deep caves on the slopes of the Arsia Mons
volcano. They have been nicknamed the "seven sisters" and have been given
the names: Dena, Chloe, Wendy, Annie, Abbey, Nicki and Jeanne. A manned
expedition to Mars is planned for around 2020.
See
the Map of Mars 1. (850 KB)
See the Map
of Mars 2. (800 KB)