Friday, September 28, 2012

Venus Transit Movie Shows Perspective In Viewing Our Solar System

Beginning of Venus transit, on 6 June 2012, 00:13:28 CEST. White light image from Svalbard Islands
Credit: Pérez Ayúcar/Breitfellner

New movies of the transit of Venus on 6 June 2012, viewed from two different locations on Earth, clearly show the parallax effects that have made Venus transits so important historically. The results were presented at the European Planetary Science Congress in Madrid, Spain.
Credit: Pérez Ayúcar/Breitfellner/Lightcurve Films

In this short animation, you will see the Transit of Venus 2012, as seen from Svalbard (78ºN) and Canberra (Australia, 35ºS). The sites are 11600km separated from each other.

The images used in the animation were obtained by members of the European Space Astronomy Centre, which is located outside Madrid.

The Venus Transit as seen through an H-alpha solar telescope. This wavelength band shows more details of the solar disk surface. Image taken from Svalbard Islands on 6 June 2012. 
Credit: Pérez Ayúcar/Breitfellner

The movies compress 6 hours of observations and 5000 individual images taken by optical and solar telescopes into a 40 second video. Data gaps due to cloudy conditions produce jumps in the otherwise smooth Venus motion across the Sun disk. The observations were taken from Svalbard in Norway and Canberra in Australia, which are separated by 11600km.

Combined images taken simultaneously from Svalbard and Cannberra, showing the VEnus parallax effect from two different locations on Earth, separated by 11600km.
 Credit: Pérez Ayúcar/Breitfellner

When the images from the two locations are superimposed, the parallax effect (which first allowed astronomers to measure the distance between the Earth to the Sun) becomes clear. Parallax means that when the transit is viewed from widely separated points on the Earth’s surface, Venus appears to follow a different path in front of the Sun’s disc. Precise observations of the duration of the transit – together with an accurate measurement of the distance between the observation points – means that the distance to Venus and to the Sun can be calculated via triangulation.

Combined images taken simultaneously from Svalbard and Canberra, showing the Venus parallax effect from two different locations on Earth, separated by 11600km. The red line represents the apparent path of Venus across the solar disk during the 6 hour duration of the Venus Transit. 
Credit: Pérez Ayúcar/Breitfellner

The images used in the movies were obtained by members of the European Space Astronomy Centre, which is located outside Madrid. Two of the observers, Miguel Pérez Ayúcar and Michel Breitfellner are on the science operations planning team for the Venus Express satellite, which has been orbiting Venus since 2006.

Pérez Ayúcar said, “During the hours of the transit we were delighted by the slow, delicate, gracious passage of Venus in front of the Sun. A perfect black circle, containing a world in it, moving in front of its looming parent star. How thankful we were to witness it. Now with these movies, we can share a sense of that experience.”

Combined images taken simultaneously from Svalbard and Cannberra, showing the VEnus parallax effect from two different locations on Earth, separated by 11600km. 
Credit: Pérez Ayúcar/Breitfellner

Breitfellner said, “In the 18th century people realised that transits of Venus could be used to measure the distance from the Earth to the Sun. Teams of astronomers were sent all across the world to measure this effect. The 2012 transit has its own historical importance - it is the first that has occurred when a spacecraft is in orbit at Venus. Science teams are now working to compare observations of the Venus transit from Earth with simultaneous observations from Venus Express.”

In this short animation, you will see part of the Transit of Venus 2012, as seen from Svalbard (78ºN) and Canberra (Australia, 35ºS). The sites are 11600km separated from each other. The images have been superposed, so that the parallax of Venus (Venus appearing in a slightly different place in front of the Sun's disk as seen from both locations) is clear. The "upper" Venus is as seen from Canberra, the "lower" Venus is as seen from Svalbard.
Credit: Pérez Ayúcar/Breitfellner/Lightcurve Films

The images used in the animation were obtained by members of the European Space Astronomy Centre, which is located outside Madrid

Colin Wilson, Operations Scientist for Venus Express, said, “Planetary transits are not just of historical interest, they have acquired a new importance in the study of newly discovered planets around other stars. Because we cannot image exoplanets directly, it is only by studying their transits that we can discover whether they harbour liquid water or other potential ‘biomarker’ molecules like methane or ozone. 

The Venus transit is an example much closer to home, offering us a chance to test our understanding of how to interpret transit data. This certainly added extra interest as we watched the Venus transit in June - particularly knowing it was our last chance that we’d have to wait until 2117 to see the next one!”

Our last Transit of Venus is a film project about the Transit of Venus of 5/6 of June 2012. It will be the last of our century. In Episode 1 (of a series of short films that will cover this unique event) Thomas Widemann, planetary scientist at the Paris Observatory, explains the Venus Twilight Experiment. This film project is supported by the European Planetology Network (Europlanet, www.europlanet-eu.org).
our last ToV: it is happening now! from Lightcurve Films on Vimeo.

Contacts and sources:
Europlanet Media Centre

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