from the city sell their famous glass and
lace products to tourists. Trade, shipbuilding,
fishing, and manufacturing
also bring money to Venice.
History
People settled the islands of Venice in
the 500s. They moved there to escape
invaders on the Italian mainland.
A series of dukes, called doges, ruled
Venice from the 700s until 1797. It
developed into an independent power
called a city-state. Venice controlled
important trade routes and grew wealthy
from sea trade. In the 1200s it began
taking over other territories in the
region. Venice achieved its greatest
power and wealth in the 1400s.
Venice began to decline in the 1500s. It
gradually lost the lands of its empire in
wars with other powers. Austria took
control of Venice in 1797. The city has
been part of Italy since 1866.
In modern times air pollution and
regular flooding have damaged Venice’s
great buildings. Also, the islands have
Boats called gondolas gather for a special
event on the Grand Canal of Venice, Italy.
BRITANNICA STUDENT ENCYCLOPEDIA Venice 65
been sinking into the lagoon at an
alarming rate. In the 20th century the
city began projects to try to control
these problems.
#More to explore
Canal • Italy
Venus
Venus is one of the planets that orbit,
or travel around, the sun in the solar
system. Venus is the brightest planet in
the sky when viewed from Earth. It is
Earth’s nearest neighbor, coming closer
to Earth than any other planet. Venus is
the second planet from the sun. Its
distance from the sun averages about 67
million miles (108 million kilometers).
It is the hottest planet in the solar
system.
Physical Features
Venus is about the same size and weight
as Earth. Its diameter, or distance
through its center, is about 7,500 miles
(12,100 kilometers). It is solid and
rocky. Scientists believe that Venus also
has layers like Earth’s. These layers consist
of a metal core, a thick rocky
middle, and a crust.
In the past lava from erupting volcanoes
shaped the surface of Venus. Most of the
landscape is gently rolling plains. Venus
also has tall mountains.
The atmosphere, or layer of gases, surrounding
Venus is thick and heavy. Also,
thick clouds always cover the planet.
The gases and clouds trap heat. The
temperature near Venus’ surface is about
867° F (464° C). Its surface is hot
enough to melt lead.
Orbit and Spin
Like all planets, Venus has two types of
motion: orbit and spin. The orbit is the
path it takes as it travels around the sun.
Venus orbits the sun in a nearly perfect
circle. Venus takes 225 Earth days to
complete one orbit. In other words, one
year on Venus lasts 225 Earth days.
Venus also spins, or rotates about its
center. A planet’s orbit and spin combine
in a complex way to determine the
length of a day on that planet. For most
planets a day is almost equal to the time
it takes to complete one rotation. Venus
is unusual in that the length of its day is
very different than the time it takes to
complete one rotation. The planet takes
243 Earth days to complete one rota-
A view of Venus taken by the Magellan
spacecraft shows the planet’s highest mountain
range. It appears as a bright spot near
the center of the photograph.
66 Venus BRITANNICA STUDENT ENCYCLOPEDIA
tion, but a day on Venus lasts only about
117 Earth days. A day on a planet is the
time it takes for the sun to appear
straight overhead, to set, and then to rise
straight overhead again.
Observation and Exploration
People have observed Venus from Earth
since ancient times. In addition, more
than 20 unmanned spacecraft have visited
the planet. The U.S. Mariner 2
spacecraft passed by Venus in 1962. It
was the first spacecraft to fly near
another planet. In 1970 the Soviet
Union’s Venera 7 landed on Venus. It
was the first spacecraft to successfully
land on another planet. In the 1990s the
U.S. Magellan spacecraft mapped Venus’
surface in great detail. The European
Space Agency sent a craft to study
Venus’ atmosphere in 2005.
#More to explore
Earth • Planets • Solar System • Space
Exploration
Venus, goddess
#see Aphrodite.
Venus’s-flytrap
The Venus’s-flytrap is a plant that traps
and eats insects. It belongs to a group of
carnivorous, or meat-eating, plants. This
group also includes sundews and pitcher
plants. The scientific name of the
Venus’s-flytrap is Dionaea muscipula.
In the wild the Venus’s-flytrap grows
only in parts of North and South Carolina,
in the United States. It grows best
in soil that is damp.
The Venus’s-flytrap grows from a bulblike
root. It reaches heights of between 8
and 12 inches (20 to 30 centimeters)
and produces small, white flowers. The
leaves of the plant grow in rounded
halves. The halves are hinged together
on one side like jaws. Each half has long
spikes along its edge and three hairs on
top that are sensitive to touch. The leaf
oozes a sticky substance that attracts flies
and other insects.
When an insect crawls between the two
halves of a leaf, the hairs detect its presence.
In less than a second, the leaf
snaps shut and the long spikes lock
together. The leaf then releases digestive
juices that break down the insect into
nutrients. The leaf absorbs the nutrients