CAIRO,
June 7 (IslamOnline.net) - On Tuesday, June 8, around five billion
people may be able to watch a celestial alignment that no human alive
today has ever seen.
The
phenomenon is "Venus Transit," where we "earthlings"
will be able to see the planet cross the face of the Sun, a rare
phenomenon that last occurred in 1882, according to Agence France-Presse
(AFP).
The
Venus
Transit Animation begins at the surface of Venus where
heat ripples distort the scene in a shimmering heat bath. As we leave
Venus and move off into space, we arrive at Earth and watch as Venus
falls behind us and finally passes across the face of the Sun.
Unlike
a solar eclipse, no-one will note any perceptible darkening: the Sun's
light will dim by just a tenth of one percent, and Venus will appear as
a small black disc inching its way, from about 0513 to 1126 GMT, across
the star's surface.
People
should view it indirectly by projecting the image through binoculars or
a telescope onto paper, or by watching it on television or the Internet,
AFP said.
Anyone
looking at it directly must wear proper filters. To look at the Sun
without protection can cause blindness.
"During
a little more than six hours, planet Venus will cross the face of the
Sun, offering a wonderful show for everybody to admire," the
European Southern Observatory (http://www.vt-2004.org/) said.
"Nobody
should miss the opportunity to witness this great event. And -- good
luck! -- it appears that the observing condition prospects are rather
favorable in large areas of the world."
Only
six transits have ever been recorded: in 1631, 1639, 1761, 1769, 1874
and 1882. The next will be in 2012, but the one after it will be in
2117.
"It's
an extremely rare event," said Gordon Bromage, a professor of
Astrophysics at the University of Central Lancashire, a focal point for
British observations about the transit
(http://www.transit-of-venus.org.uk/vt-2004/).
The
reason is because Venus, the second planet from the Sun, has an orbital
plane that is slightly tilted to Earth, the third planet.
Until
the advent of the radar and satellites, the big interest in the
alignment was to measure the exact distance between Earth and the Sun.