Sunday, June 26, 2005

How strange! The sky is blue! by K.A.Cassimally



Look up! Just do it. What do you see? Stupid question, eh? You see the ceiling of course. When you look upwards during a sunny day while picnicking however, you see the blue sky. Ever wondered why the sky is not green nor but blue?

Before answering this question, lets go back to the basic physics of light. Sorry, but here I go

Light is a kind of energy, which travels in waves. In fact, light is a wave of vibrating electric and magnetic fields. Light forms only one small part of a larger range of vibrating electromagnetic fields called the electromagnetic spectrum. Electromagnetic waves travel through space at an amazing 300 00km/s. Therefore this is also the speed of light.

When you see white light from the bulb, you are actually seeing the seven colours of the rainbow! This is because white light consists of a combination of these seven colours.

Each of these colours has a different wavelength, frequency and energy. Wavelength is the distance between the crests of the waves. The frequency is the number of waves that pass by each second. Note that the longer the wavelength, the lower the frequency and the less energy it contains.

Violet: Shortest wavelength, highest frequency and energy
Red: Longest wavelength, lowest frequency and energy

Now back to our main topic. That blue colour of the sky is due to an effect known as the Rayleigh scattering. As light from the sun moves towards Earths atmosphere, not all the colours are actually able to pass through that atmosphere. Most of the longer wavelength colours do pass (red, orange and yellow for sure) but the shorter wavelength ones however are mostly absorbed by gas molecules found in the atmosphere. Absorbed blue light is then bounced back (radiated would be a better word) in all directions. This makes the shy to appear blue!

You would however ask me why its the blue rays, which get scattered, and not the indigo nor the violet rays (the other colours pass through the atmosphere remembertheres also blue that pass through but it then gets scattered). Well in fact, the shorter the wavelength, the more the colour gets scattered. Violet, which has the shortest wavelength of all colours of the rainbow thus gets scattered more than blue rays do. Our eyes however are much more sensitive to blue than to violet and the sky therefore doesnt appear to be violet but blue (in reality the sky is violet-indigo!).

Now do take the time making the following:
Take a look at the horizon (if youre at the seaside) and note the skys colour there. No, its not as blue as the rest of the sky, is it? Its much paler. This is because for the blue light to reach your eye, it has to travel more. Blue light will thus pass through more air consequently getting scattered more. Conclusion: less blue light reaches your eyes than compared to blue light from just above you.
About the Author
K.A.Cassimally is the editor in chief of Astronomy Journal and Astronomy Journal Ezine. He is also the co-founder of the RCPL Astronomy Club. K.A.Cassimally is best known for his article 'Harry Potter and the Moons of Jupiter'.
He is also Senior Columnist at BackWash.com where he writes 'Not Scientific Science'.

NABGG (Nat'l Assoc. of Black Geologists & Geophysicists) 23rd Annual Conference 9/15 9/18, 2004 - Austin, Texas by Robert Johnson



The NABGG (National Association of Black Geologists and Geophysicists) will hold its 23rd annual conference on Wednesday, September 15Saturday, September 18, 2004.

HOUSTON, TX (PRWEB) August 18, 2004 -- Please plan to join us, as we convene our 23rd annual meeting that will be held in Austin, Texas with the University of Texas at Austin serving as the host institution. Heralding excellent research and technology, the University of Texas at Austins Geoscience Department is a world class department that has consistently produced some of the most influential experts in the field of geoscience.

This years conference theme Partnering Our Different Worlds conveys the concept of the connectivity of the different aspects of geoscience in our society, including Oil & Gas, Environmental Sciences, Academia, Professional Societies, and Governmental Agencies.

Some of the highlights include:
Keynote Speakers:

-Dr. Sandra K. Johnson, Manager, IBM Linux Technology Center
-Dr. Jerry Harris, Head of Geophysics Department, Stanford University
-Dr. Edwin Dorn, Dean, Lyndon B. Johnson School of Public Affairs, University of Texas at Austin.
-Dr. William L. Fisher, Director of the Jackson School of Geosciences, University of Texas at Austin.

Technical Presentations, Career Fair, Tours, and Community Service Activities

In addition, many Texas state leaders are expected to attend this national convention. The convention promises to be an exciting one, so please begin planning to join us. We hope to see you in Austin!

About NABGG
NABGG strives to increase minority representation in the geosciences through partnerships with academia and by mentoring undergraduate as well as graduate students. We are committed to the continuous training and development of aspiring and practicing geoscientists.

Visit NABGG online: www.nabgg.org

NABGG
4212 San Felipe, Suite 420
Houston, Texas 77027-2902
nabgg_us@hotmail.com
About the Author
Vice President , NABGG