The Astronomy Book

(National Geographic (Little) Kids) #1

305


See also: Radio astronomy 179 ■ Space telescopes 188–95 ■ A digital view of the skies 296 ■
Gravitational waves 328–31 ■ Lagrange (Directory) 336


THE TRIUMPH OF TECHNOLOGY


L2 is a place in space where the
gravity of the sun and Earth work
together to pull an orbiting object
around the sun at the same rate as
Earth, making one orbit every year.
This means the JWST will be largely
in the shadow of Earth, blocking
out any heat pollution from the
sun and allowing the telescope
to detect very faint infrared sources
in deep space. NASA claims that
the telescope could detect the heat
of a bumblebee on the moon.


Heat seeker
The JWST’s vast primary mirror
is seven times the area of Hubble’s
and, instead of polished glass, the
mirror contains 18 hexagonal units
made from beryllium for maximum
reflection. The 270-sq-ft (25-m^2 )
mirror is too large to be launched
flat, so it is designed to unfold
once in orbit.
To pick up the faint heat
signatures of the most distant stars,
the telescope’s detectors must
always be extremely cold—never
more than –370°F (–223°C). To
accomplish this, the JWST has
a heat shield the size of a tennis
court. Again, this is folded away
for launch. The shield is made from
five layers of shiny plastic that reflect
most of the light and heat. Any heat


that penetrates the top layer is then
radiated sideways by successive
inner layers so that almost nothing
reaches the telescope itself.

First light
The light waves from the first stars
to form have been stretched as
they shine through the expanding
universe, changing them from
visible light to infrared, so they

The light from the first stars has been
shining through expanding space.

Infrared is mostly
invisible from
Earth’s surface.

The expansion has
stretched the light into
infrared wavelengths.

are a prime target of observation
for the JWST. At the same time,
this ultra-sensitive eye on the
infrared sky has three other main
goals. It will investigate how
galaxies have been built over
billions of years, study the birth of
stars and planets, and provide data
about extrasolar planets. NASA
hopes that the telescope will be
in operation for at least 10 years. ■

JSWT will not be exactly at the L2 point, but will circle around it in
a halo orbit. Lagrange points are positions in the orbit of two large bodies
where a smaller object can keep a stable position relative to those two large
bodies. There are five L points in the orbital plane of Earth and the sun.

To see the first stars,
a giant infrared
telescope must be
sent into space.

L1


L4


L2


L5


L3


Earth’s orbit

Moon’s orbit

JWST’s orbit
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