Large Eyes to look the
heavens
Debi Prasad Choudhary
Los Angeles, 02/05/2014
God gifted divine vision to
his friend and disciple in a battlefield to enable him see his “cosmic self”. While
listening to this episode in the story of Mahabharat
from my granny, I wished such a vision to see the cosmos. Twenty years later,
the sight of Saturn, Jupiter and Orion Nebula through a moderate telescope,
reminded me of the feelings of God’s friend if he had really seen these objects
all at once!! Telescopes are large eyes to look at the tiny light glows in the
sky situated far away.
Human eye is a sophisticate
camera with a complex lens of about 8 mm size. In broad daylight, we use only a
small part about 2mm of this this lens through which light enters to make an image
inside the eye. As we enter a low light area the iris fully opens up for the
light to enter through entire 8 mm lens. Usually it takes some time for this to
happen, so we cannot clearly see in the first few moments of entering the dark
from bright illuminated area. The 8 mm lens collect enough light to see the
stars of about 6th magnitude and can distinguish two stars separate by about 1
arc minute. The range of color that our eye can see is limited to the colors of
rainbow.
Light is electromagnetic wave
because the electric field and the magnetic field vibrate in planes
perpendicular to the direction of its propagation. The distance between the
maximum vibrations in same direction is called wavelength. The two extreme
color of rainbow are violet and red have wavelengths 400 nanometer and 700
nanometer respectively. The
electromagnetic waves of long wavelength are of lower energy compared to shorter
wavelength. There are electromagnetic waves beyond this visible range. The
electromagnetic waves of wavelength lower then 400 nanometer are x-ray waves
that are used in dentist office, UV waves that cause skin problem if sunscreen
is not used while lying in beach. The waves with larger than 700 nanometer wavelength
are Infrared that we use for pain reliever, radio and microwave that are used
for communication via TV, radio stations and mobile phone technology. All these
electromagnetic waves are exactly same as the light we see with our necked eye,
but have different wavelength. The stars and galaxies in the sky produce light
in a wide range from very short to very long wavelengths.
Light propagates in the form
of waves that prevent the formation of sharp shadow of knife-edges. Infect, if
you closely look at the shadow of a sharp object like a knife-edge, you will
find dark and bright bands that are produced due to diffraction. The same
effect limits us distinguishing two pennies kept side by side beyond about 225
ft. In order to distinguish them, we need to increase the size of our eye (make
it bigger than about 8 mm), which is not possible. The other alternate is to
use a telescope that has a bigger lens.
The wave nature of light has
another consequence. As the light wave front from a distant star passes through
the earth’s atmosphere, different parts move at different speed through packets
of air with different density. By the time it reaches our eye the light wave is
distorted from its original shape before entering the earth. Since the air
pockets with different density move, we see the stars twinkle. The planets do
not twinkle because they are situated relatively nearer and send many light
waves slightly separated in space. These days, we can repair the distortion
using modern image stabilizer technology somewhat similar to the one available
in many cameras (adaptive optics) and prevent the star from twinkling.
Astronomers build telescopes
and detectors to look at them in all wavelengths in minute detail. About 400
years ago, Galileo used the telescope to discover dark spots on the sun and
moons of Jupiter that made great impact in modern science. While working as a
professor in Padua University in Italy, he used to buy lenses in neighboring
town Venice and select the best ones after examining them by looking at the
stars. The stars would look like a point of bright light if the lens were
perfect. But, since the images in blue, yellow and red color are made at
different distances from the lens, they might still look blurred.
The bigger lenses are used to
make telescopes to see faint stars by collecting more light. Large lenses are
supported only at the periphery, so they become bent due to their own weight
making it impossible to make them larger than about one meter size. This
difficulty can be overcome by using reflecting mirrors of spherical shape, since
they can be supported from the back. Mirror based telescopes produce images of
color at same distance from the reflecting surface. But, the light reflected
from the outer part of large spherical mirrors are focused at different
distance that also results in blurred images. So, large reflecting telescopes
are made with mirrors that are not spherical but parabolic.
The thickness of the mirrors
should be about 1/6 of the diameter in order to prevent flexure leading to the distorting
the parabola shape. This requirement creates problem in making mirrors for the
large telescopes of sizes greater than 3 to 4 meter as they become too heavy. Making
segmented mirrors and using an active support overcomes this problem. The
segmented mirrors use smaller parts of a parabolic mirror held by active
supports that maintain the parabolic shape. The active supports continuously
tilt to adjust the orientation of mirrors to keep them in a parabolic form. The
surface of the mirrors or the lens that produce the images of astronomical
objects must be smooth relative to the wavelength of the light.
Since the earth rotates
around north-south axis, special mounts are built to align them along local
latitude and track the stars by moving at a rate of 360 degree in 24 hours.
There are other sophisticate mounts and tracking systems for large telescopes.
Building the enclosure or telescope dome and the location of the observatory is
also an important part of these astronomical facilities. The observatories are
built at high altitudes – on the top of mountains, that are dark and have clear
sky for most of the year. For installing very large telescopes, like the
30-meter telescope being made by Caltech and University of California,
extensive site survey is undertaken. Additional complexity arises for
telescopes built for observing the sun because it heats the surroundings. The
solar observatories are built surrounded by large body of water or in very high
altitudes where the atmosphere is stable in presence of the sun.
A large part of light in
ultraviolet, X-ray, gamma ray and Infrared is blocked by the atmosphere and do
not reach the earth. Satellite based space born telescopes are built to observe
the stars and galaxies in these wavelengths. These great instruments include
Hubble Space Telescope, Chandra X-ray telescope and Spritzer telescope for IR
light.
The light in radio wavelength
similar to FM radio or TV communication is long so the telescope surface need
not be very smooth. At the same time large mirrors are needed for achieving the
images of higher resolution. Many separate telescopes are used to collect light
and combined to get an image from an effectively large telescope. These are
called interferometers, a technique that is also used for optical wavelengths.
Like, we get lots of
information about an object from the amount of light it emits and its color,
telescopes serve the same purpose for astronomical sources. The information
about the nature of the object is embedded in the amount of light it emits or
reflects, the color or wavelength of light and amount of light wave in
different orientation, which is also known as the state of polarization.
Instruments are used at the focal plane of the telescopes to examine these properties
of light from the astronomical sources.
Modern big eyes enable us to
see the objects very faint in the sky and learn about them in all colors that
are visible to our eye and beyond. Often these faint objects are situated far
away, such that light from them takes many many years to reach us. This means
we are able to see a star that may not be there at this time, but what it was
when the light left from it. Today, we have built such large telescopes that we
can see the objects that were born just after the creation of the universe.
Some times, I think the fantastic imaginations of the ancient stories are
taking real shape.