1. The James Webb Space Telescope

2. Introduction
 The James Webb Space Telescope
 The James Webb Space Telescope, also called Webb or JWST, is
a large, space-based observatory, optimized for infrared
wavelengths, which will complement and extend the discoveries
of the Hubble Space Telescope. It will have longer wavelength
coverage and greatly improved sensitivity. The longer
wavelengths enable Webb to look further back in time to find the
first galaxies that formed in the early Universe, and to peer inside
dust clouds where stars and planetary systems are forming today.
It is scheduled for launch in 2013.

3. James E .Webb
 This space-based observatory is named after James E. Webb (1906- 1992),
NASA's second administrator. Webb is best known for leading Apollo, a
series of lunar exploration programs that landed the first humans on the
Moon. However, he also initiated a vigorous space science program that was
responsible for more than 75 launches during his tenure, including America's
first interplanetary explorers.

4. How will Webb be better?
 Webb is designed to look deeper into space to see the earliest stars and
galaxies that formed in the Universe and to look deep into nearby dust
clouds to study the formation of stars and planets. In order to do this, Webb
will have a much larger primary mirror than Hubble (2.5 times larger in
diameter, or about 6 times larger in area), giving it more light-gathering
power. It also will have infrared instruments with longer wavelength
coverage and greatly improved sensitivity than Hubble. Finally, Webb will
operate much farther from Earth, maintaining its extremely cold operating
temperature, stable pointing and higher observing efficiency than with the
Earth-orbiting Hubble.

5. How long will the mission last?
 Webb will have a mission lifetime of not less than 5-1/2 years after launch,
with the goal of having a lifetime greater than 10 years. The lifetime is
limited by the amount of fuel used for maintaining the orbit, and by the
testing and redundancy that ensures that everything on the spacecraft will
work. Webb will carry fuel for a 10-year lifetime; the project will do mission
assurance testing to guarantee 5 years of scientific operations starting at the
end of the commissioning period 6 months after launch.

6. Servicing Webb
 Hubble is in low-Earth orbit, located approximately 600 kilometers away
from the Earth, and is therefore readily accessible for servicing using the
Space Shuttle. Webb will be operated at the second Sun-Earth Lagrange
point, located approximately 1.5 million kilometers away from the Earth,
and will therefore be beyond the reach of any manned vehicle currently
being planned for the next decade. In the early days of the Webb project,
studies were conducted to evaluate the benefits, practicality and cost of
servicing Webb either by human space flight, by robotic missions, or by
some combination such as retrieval to low-Earth orbit. Those studies
concluded that the potential benefits of servicing do not offset the increases
in mission complexity, mass and cost that would be required to make Webb
serviceable, or to conduct the servicing mission itself.

7. Size of the Webb
 The diameter of the primary mirror, will be about 6.5 meters (21 feet) for
Webb. This is about 2.7 times larger than the diameter of Hubble, or about 6
times larger in area. The Webb will have a mass of approximately 6,500 kg,
with a weight of 14,300 lbs on Earth (in orbit, everything is weightless), a
little more than half the mass of Hubble. The largest structure of Webb will
be its sunshade, which must be able to shield the deployed primary mirror
and the tower that holds the secondary mirror. The sunshade is
approximately the size of a tennis court.

8. Communication
 The Webb will send science and engineering data to Earth using a high
frequency radio transmitter. Large radio antennas that are part of the NASA
Deep Space Network will receive the signals and forward them to the Webb
Science and Operation Center at the Space Telescope Science Institute in
Baltimore, Maryland, USA.

9. Orbit
 Webb is going to the second Lagrange (L2) point, which is 1 million miles (1.5
million km) away from Earth, and it just takes a while to travel such a distance.
During the trip to L2, Webb will be fully deployed, will cool down to its operating
temperature, and its systems will begin to be checked out and adjusted. These
commissioning procedures will continue until 6 months after launch, at which point
routine scientific operations will begin.
 Webb will observe primarily the infrared light from faint and very distant objects. To
avoid swamping the very faint astronomical signals with radiation from the
telescope, the telescope and its instruments must be very cold.
 Webb's operating temperature is less than 50 degrees above absolute zero: 50 Kelvin,
(-225 Celcius, or -370 deg F). Therefore, Webb has a large shield that blocks the
light from the Sun, Earth, and Moon, which otherwise would heat up the telescope,
and interfere with the observations. To have this work, Webb will be in an orbit
where all three of these objects are in about the same direction; the second Lagrange
point (L2) of the Sun-Earth system has this property.

10. How far will Webb look?
 One of the main goals of Webb is to detect some of the very first star formation in
the Universe. This is thought to happen somewhere between redshift 15 and 30. At
those redshifts, the Universe was only one or two percent of its current age. The
Universe is now 13.7 billion years old, and these redshifts correspond to 100 to 250
million years after the Big Bang. The light from the first galaxies has traveled for
about 13.5 billion years, over a distance of 13.5 billion light-years.

11. Resources
 http://www.jwst.nasa.gov/