Transit of Venus on Tuesday Is Rarer Than Halley's Comet
This still from a NASA video shows the position of Venus on the sun's disk in Pacific Daylight Time on June 5, 2012 during the last transit of Venus for 105 years.
The last chance most of us will ever have to see the planet Venus pass in front of the sun is coming up this Tuesday (June 5).
On that day, more than half the world will get to see an exceedingly rare event: a transit of Venus crossing the face of the sun at inferior conjunction. A transit of Venus is among the rarest of astronomical events, rarer even than the return of Halley's Comet every 76 years. Only six transits of Venus are known to have been observed by humans before: in 1639, 1761, 1769, 1874, 1882 and most recently in 2004.
When Venus is in transit across the solar disk, the planet appears as a distinct, albeit tiny, round black spot with a diameter just 1/32 that of the sun. This size is large enough to readily perceive with the naked eye; however, prospective observers are warned to take safety precautions (as with a solar eclipse) in attempting to view the silhouette of Venus against the blindingly brilliant face of the sun. Special glasses or telescope filters must be used at all times.
Prior to local sunset, observers who are located over much of North America and the northwestern part of South America will be able to observe at least the opening stages of this most unusual celestial phenomenon. [Venus Transit of the Sun: A 2012 Observer's Guide (Infographic)]
The entire transit will be a west-to-east passage (right to left) taking six hours and 40 minutes. The sun will be above the horizon for the whole transit for much of Greenland and far-northern portions of Canada, all of Alaska and Hawaii, central and eastern Asia, New Zealand and the eastern half of Australia. For these last three regions, the transit will occur on June 6.
The sun rises with Venus already on its disk for western Asia, the eastern half of Africa and virtually all of Europe on the morning of June 6. Interestingly, as seen from Iceland, the beginning and end of the transit will be visible, but the sun will set prior to, then rise after, the middle of the transit.
One region that will miss the transit is a large portion of South America. From places south and east of an imaginary line drawn between Morawhanna, Guyana, southwest to Tacna, Peru, the sun will unfortunately set before the transit begins. In addition, a large part of western Africa as well as Portugal and the western half of Spain will also miss out, because from there the transit will end before the sun rises.
If you wish to generate predictions for the transit for where you live, the Astronomical Applications Department of the U.S. Naval Observatory has produced an online Transit Computer at: http://www.usno.navy.mil/USNO/astronomical-applications/data-services/transit-us
For the United States and Canada, the transit will begin when the dark disk of Venus first touches the outer limb of the sun, known as Contact I. From the Eastern United States and Eastern Canada, Contact I should occur within about a minute of 6:03 p.m. EDT. From the Western United States and Western Canada, Contact I should occur within about a minute of 3:06 p.m. PDT.
It will take about 18 minutes for the black disk of Venus to move completely onto the sun's face, ultimately bringing its black disk just inside the sun's upper left edge. This will be an especially interesting time.
The moment when the two disks become internally tangent — that is, when Venus moves completely onto the sun's disk — is known as Contact II. And just moments before interior contact actually takes place, assiduous viewers might see the silhouette of Venus become suddenly connected to the sun's limb by a dark ligament — like a drop of water just before separating from a faucet. [Last Venus Transit In Your Lifetime | Video Show]
Another way to describe the sight is that the planet will seem attached to the sun's limb by a thin black column or thread. This optical illusion is known as the "black drop effect." Its cause is believed to be the combination of local atmospheric seeing and telescope diffraction, in conjunction with the dark disk of Venus interacting with the limb darkening of the sun's outer edge.
Venus will then take more than six hours to traverse the disk of the sun, although for most Americans (except in Alaska and Hawaii), sunset will intervene before Venus moves off of the sun.
The circumstances of the transits of Venus repeat themselves with great exactness over a period of 243 years. The intervals between individual transits (in years) currently go as follows: 8 + 121½ + 8 + 105½ = 243. In other words, a pair of transits may occur over a time span of just eight years, but following the second transit, the next will not occur again for over a century. The upcoming Venus transit is the second of a pair, the first having occurred on June 8, 2004.
But take heed: should clouds prevent you from getting a view of this year's event, it will be most unfortunate, since the next opportunity to observe a transit of Venus will not occur until December 10-11, 2117! We can expect that very few people who witness this year's transit will still be alive to catch the next one in 105½ years.
Editor's note: If you snap a great photo of the Venus transit and would like to share it with SPACE.com for a story or gallery, please send images and comments to SPACE.com managing editor Tariq Malik at email@example.com.
Joe Rao serves as an instructor and guest lecturer at New York's Hayden Planetarium. He writes about astronomy for The New York Times and other publications, and he is also an on-camera meteorologist for News 12 Westchester, N.Y.
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