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Venus Transit 2012 - Ultra-high Definition View (NASA/ESA)

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Published on Jun 6, 2012

http://www.facebook.com/ScienceReason ... Ultra-high Definition View of the Venus Solar Transit 2012 (NASA SDO, ESA Proba-2).

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The first part of this video shows the transit of Venus on 5-6 June 2012 as seen from SWAP, a solar imager onboard ESA's PROBA2 microsatellite. SWAP, watching the Sun in EUV light, observes Venus as a small, black circle, obscuring the EUV light emitted from the solar outer atmosphere - the corona - from 19:45UT onwards. At 22:16UT - Venus started its transit of the solar disk

The bright dots all over the image ('snow storm') are energetic particles hitting the SWAP detector when PROBA2 crosses the South Atlantic Anomaly, a region where the protection of the Earth magnetic field against space radiation is known to be weaker.

Note also the small flaring activity in the bright active region in the northern solar hemisphere as Venus passes over. Towards the end, you can see a big dim inverted-U-shape moving away from the Sun towards the bottom-right corner. This is a coronal mass ejection taking off.

http://blogs.esa.int/venustransit/ (Credit: ESA/ROB)

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Launched on Feb. 11, 2010, the Solar Dynamics Observatory, or SDO, is the most advanced spacecraft ever designed to study the sun. During its five-year mission, it will examine the sun's atmosphere, magnetic field and also provide a better understanding of the role the sun plays in Earth's atmospheric chemistry and climate. SDO provides images with resolution 8 times better than high-definition television and returns more than a terabyte of data each day.

On June 5 2012, SDO collected images of the rarest predictable solar event--the transit of Venus across the face of the sun. This event happens in pairs eight years apart that are separated from each other by 105 or 121 years. The last transit was in 2004 and the next will not happen until 2117.

The videos and images displayed here are constructed from several wavelengths of extreme ultraviolet light and a portion of the visible spectrum. The red colored sun is the 304 angstrom ultraviolet, the golden colored sun is 171 angstrom, the magenta sun is 1700 angstrom, and the orange sun is filtered visible light. 304 and 171 show the atmosphere of the sun, which does not appear in the visible part of the spectrum.

http://svs.gsfc.nasa.gov/vis/iTunes/f... (Credit: NASA/SDO)

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Keywords: "Venus Transit" "Transit of Venus" 2012 NASA ESA Sun Solar Eclipse SDO Proba-2 Space Agency Astronomy Astrophysics Ultra High Definition View Full HD
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