REF. Ini juga semacam gerhana, ada yang mau salat atau sembayang berhubung dengan gerhana ini dipersilahkan, karena kali berikutnya gerhana ini akan terjadi lagi pada105 atau 121 tahun yang akan datang.
http://www.bbc.co.uk/news/science-environment-17745366 Venus to put on Sun spectacular By Jonathan Amos Science correspondent, BBC News As part of Horizon's Transit of Venus programme, science presenter Liz Bonnin explains what the transit of Venus is and why it is such a rare event Continue reading the main story Related Stories a.. The transit of science b.. First Earth-sized planets spotted c.. Japan probe fails to orbit Venus Planet Venus is set to move across the face of the Sun as viewed from Earth. The more than six-and-a-half-hour transit, which starts just after 22:00 GMT (23:00 BST) on Tuesday is a very rare astronomical phenomenon that will not be witnessed again until 2117. Observers will position themselves in northwest America, the Pacific, and East Asia to catch the whole event. But some part of the spectacle will be visible across a much broader swathe of Earth's surface, weather permitting. Skywatchers in UK, for example, will catch the end of the transit at sunrise on Wednesday. Venus will appear as a tiny black disc against our star, but no-one should look for it without the proper equipment. Venus appears as a tiny black disc against our star Looking directly at the Sun with the naked eye, or worse still through an open telescope or binoculars, can result in serious injury and even blindness. It is recommended people attend an organised viewing event where the transit will be projected on to a screen; or they can visit one of the many institutional internet sites planning to stream pictures. Venus transits occur four times in approximately 243 years; more precisely, they appear in pairs of events separated by about eight years and these pairs are separated by about 105 or 121 years. The reason for the long intervals lies in the fact that the orbits of Venus and Earth do not lie in the same plane and a transit can only occur if both planets and the Sun are situated exactly on one line. This has happened only seven times in the telescopic age: in 1631, 1639, 1761, 1769, 1874, 1882 and 2004. Once the latest transit has passed, the next pair will not occur until 2117 and 2125. Most people alive today will probably be dead by then. The phenomenon has particular historical significance. The 17th- and 18th-Century transits were used by the astronomers of the day to work out fundamental facts about the Solar System. Employing a method of triangulation (parallax), they were able to calculate the distance between the Earth and the Sun - the so-called astronomical unit (AU) - which we know today to be about 149.6 million km (or 93 million miles). This allowed scientists to get their first real handle on the scale of things beyond Earth. The first person to predict a transit of Venus - the 6 December, 1631, event - was Johannes Kepler, but he died before it occurred. Jeremiah Horrocks, the young English astronomer, was probably the first to record the phenomenon when he and his friend, William Crabtree, made separate observations of the passage on 24 November, 1639. By the time the transits of 1761 and 1769 came around, they had become major scientific events. Expeditions were despatched all over the globe to get the data necessary to calculate the AU. One such expedition was undertaken by Captain James Cook, whose epic voyage in the Endeavour took in the "new lands" of New Zealand and Australia. Continue reading the main story Timing of the transit a.. Times for the start of the transit will vary by a few minutes depending on one's location b.. The timings given here are calculated for a viewing position at the Earth's centre c.. Venus is seen to first touch (1) the edge of the Sun's disc at 22:09 GMT (23:09 BST) d.. It is completely on the disc (2) by 22:27 GMT (23:27 BST). The transit lasts over six hours e.. Come Wednesday by 04:31 GMT (05:31 BST), Venus is touching the disc's far side (3) f.. At 04:49 GMT (05:49 BST), Venus has left the disc (4). The next transit is on 11 December 2117 Modern instrumentation now gives us very precise numbers on planetary positions and masses, as well as the distance between the Earth and the Sun. But to the early astronomers, just getting good approximate values represented a huge challenge. This is not to say the 2012 Venus transit will be regarded as just a pretty show with no interest for scientists. Planetary transits have key significance today because they represent one of the best methods for finding worlds orbiting distant stars. Nasa's Kepler telescope, for example, is identifying thousands of candidates by looking for the tell-tale dips in light that accompany a planet moving in front of its host sun. These planets are too far away to ever be visited by spacecraft, but scientists can learn something about them from the way the background star's light is affected as it passes through the planetary atmosphere. And observing a transiting Venus, which has a known atmospheric composition, provides a kind of benchmark to support these far-flung investigations. But Venus itself will come in for scrutiny. Scientists will be using the event to probe the middle layers of the Venusian atmosphere - its mesosphere. They will be looking for a very thin arc of light, called the aureole, which can only be seen when Venus appears to just touch the edge of the Sun's disc. The brightness and thickness of the aureole depends on the density and temperature of the atmospheric layers above Venus's cloud tops. Observations of the aureole will be combined with data from Europe's Venus Express spacecraft in orbit around the planet to provide information on high-altitude winds. The Venusian atmosphere experiences super-rotation. That is - the whole atmosphere circles the planet in four Earth days, on a body that turns around just once in 243 Earth days. Continue reading the main story How to view the Sun safely METHOD 1: Cut two holes in card for binocular eye-pieces. Push card onto binoculars and fix with tape. Block one lens (with lens cap, for example). Holding binoculars at waist height, angle towards Sun - do not look through them. Move binoculars around until card shadow minimised on viewing surface (piece of white card best). During six-hour transit, move set-up to follow path of Sun across sky, for example by mounting it on tripod or chair. METHOD 2: Take piece of stiff card and pierce with pin. Hold it up and, looking away from the Sun, adjust angle of card until shadow minimised. Pinhole will project image of Sun into middle of shadowed area. Place another piece of card under shadow and adjust distance to get best picture - more distance gives larger but fainter image. Hole must be clean and as small as possible. WARNING: Never observe the Sun with the naked eye or telescope, camera or other optical device. Doing so will seriously damage eyesight and may lead to permanent blindness. [email protected] and follow me on Twitter More on This Story Related Stories a.. The transit of science 01 JUNE 2012, SCIENCE & ENVIRONMENT b.. First Earth-sized planets spotted 20 DECEMBER 2011, SCIENCE & ENVIRONMENT c.. Japan probe fails to orbit Venus 08 DECEMBER 2010, ASIA-PACIFIC d.. Venus 'still volcanically active' 09 APRIL 2010, SCI/TECH e.. Probe peers into Venusian secrets 11 OCTOBER 2006, SCI/TECH f.. Planet Venus completes transit 08 JUNE 2004, SCI/TECH g.. Celebrating Horrocks' half hour 05 JUNE 2004, LANCASHIRE Related Internet links a.. RAS - Transits of Venus b.. Royal Observatory Greenwich- 2012 Transit of Venus c.. Watch the transit live d.. SkyandTelescope.com - Transit of Venus e.. transitofvenus.org f.. British Astronomical Association- Transit of Venus 2012 g.. Society for Popular Astronomy - Get Ready for the Transit of Venus h.. Europlanet Outreach- Transit of Venus 2012 i.. Transit of Venus blog - Esa The BBC is not responsible for the content of external Internet sites [Non-text portions of this message have been removed]
