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: http://star.arm.ac.uk/press/2012/Venus_transit_aac_pr.html
Дата изменения: Fri Jun 8 12:45:40 2012 Дата индексирования: Tue Oct 2 06:38:41 2012 Кодировка: IBM-866 Поисковые слова: sts-64 |
An image obtained by Tolis Christou from Greece
during the 6th June 2012 transit of Venus.
One of a series of images obtained by Tolis Christou
from Lavrion, Greece, during the 6th June 2012 transit
of Venus. The large black circle is the planet Venus,
the smaller dark patches are groups of sunspots on the
SunтАЩs surface (photosphere). The equipment used was a
digital SLR Canon EOS 350D camera with a telephoto lens
mounted on a tripod. The Sun was imaged through a Baader
AstroSolar film with exposures ranging from 1/200 to 1/4000
of a second. The exposure times decreased for the series of
images as the Sun climbed higher in the sky.
Apostolos (Tolis) Christou, an astronomer at the Armagh Observatory, successfully observed the recent transit of Venus from the town of Lavrion, about 30 kilometres south–east of Athens. The next opportunity to observe this rare phenomenon will not occur until 2117.
Historically, observations of transits of Venus were used to calculate the distance from the Earth to the Sun – the Astronomical Unit (AU) – by triangulation, thereby obtaining the dimensions of the Solar System. The AU is the fundamental yardstick used for measuring the size of the Universe.
Nowadays, astronomers use accurate observations of the same phenomenon, that is the transit of an extra–solar planet (exoplanet) in front of a distant star, to infer the size and distance of such planets orbiting other stars. The technique depends on very precise measurements of the decrease in light of the distant star when the planet passes exactly between the Earth and the star.
In October 1995, Michel Mayor and Didier Queloz of the University of Geneva observed what is believed to have been the first confirmed exoplanet orbiting a sun-like star, 51 Pegasi. Currently, there are now almost 800 confirmed exoplanets – including a few then-unconfirmed cases from the 1980s. By February of this year, the Kepler spacecraft had discovered over 2,300 unconfirmed candidate planets orbiting almost 1,800 host stars.
Armagh Observatory is presently running a Transit of Venus Exhibition, from 10am – 11am and 3pm – 4pm during week-days, until Tuesday 12th June where some images of the June 2012 transit are on show. Please book your place by telephoning John McFarland on 028-3752-2928 or emailing jmfarm.ac.uk.
FOR FURTHER INFORMATION CONTACT: John McFarland at the Armagh Observatory, College Hill, Armagh, BT61 9DG. Tel.: 028-3752-2928; 028-3751-2962; Email: jmfarm.ac.uk.
Last Revised: 2012 June 8th |