2012 transit of Venus
{{short description|Transit of Venus across the Sun visible from Earth on 5–6 June 2012}}
{{Use dmy dates|date=September 2019}}
File:SDO's Ultra-high Definition View of 2012 Venus Transit (304 Angstrom Full Disc 02).jpg spacecraft. Venus is in the upper right quadrant]]
The 2012 transit of Venus, when the planet Venus appeared as a small, dark spot passing across the face of the Sun, began at 22:09 UTC on 5 June 2012, and finished at 04:49 UTC on 6 June.{{cite web |url=http://eclipse.gsfc.nasa.gov/OH/transit12.html |title=2012 Transit of Venus |last=Espenak |first=Fred |publisher=NASA |access-date=6 June 2012}} Depending on the position of the observer, the exact times varied by up to ±7 minutes. Transits of Venus are among the rarest of predictable celestial phenomena and occur in pairs. Consecutive transits per pair are spaced 8 years apart, and consecutive pairs occur more than a century apart:{{cite news |title=Venus-sun event rarer than Halley's Comet |first=Jay |last=Withrow |url=http://www.omaha.com/article/20120602/NEWS01/706029927 |newspaper=Omaha World-Herald |date=2 June 2012 |access-date=6 June 2012 |url-status=dead |archive-url=https://archive.today/20120907010023/http://www.omaha.com/article/20120602/NEWS01/706029927 |archive-date=7 September 2012 }} The previous transit of Venus took place on 8 June 2004 (preceded by transits on 9 December 1874 and 6 December 1882); the next pair of transits will occur on 10–11 December 2117 and December 2125 within the 22nd century.{{cite news |first=Irene |last=Klotz |title=Venus transit offers opportunity to study planet's atmosphere (+video) |url=http://www.csmonitor.com/Science/2012/0606/Venus-transit-offers-opportunity-to-study-planet-s-atmosphere-video |publisher=Christian Science Monitor |date=6 June 2012|access-date=6 June 2012}}
Observations of the event
File:2012 Transit of Venus, path across Sun and associated data.png
File:Visibility of 2012 Transit of Venus.png
The entire transit was visible from the western Pacific Ocean, northwesternmost North America, northeastern Asia, Japan, the Philippines, eastern Australia, New Zealand, and high Arctic locations including northernmost Scandinavia, and Greenland.{{cite journal |title=The Transit of Venus |journal=Astronomy Now |publisher=Pole Star Publications |first1=Peter |last1=Grego |first2=Andrea |last2=Wulf |first3=Keith |last3=Cooper |pages=58–61 |date=June 2012 |issn=0951-9726}} In North America, the Caribbean, and northwestern South America, the beginning of the transit was visible on 5 June until sunset. From sunrise on 6 June, the end of the transit was visible from South Asia, the Middle East, east Africa, and most of Europe. The phenomenon was not visible from most of South America, nor from western Africa. There were a number of live online video streams with footage from telescopes around the world. Midway through the transit one of the NASA streams had nearly 2 million total views and was getting roughly 90,000 viewers at any given moment.
In Los Angeles, crowds jammed Mount Hollywood where the Griffith Observatory set up telescopes for the public to view the transit. In Hawaii, hundreds of tourists watched the event on Waikiki Beach where the University of Hawaii set up eight telescopes and two large screens showing webcasts of the transit.{{cite news |title=Last transit of Venus this century draws stargazers around the world |url=https://www.theguardian.com/science/2012/jun/06/transit-of-venus-century-stargazers |newspaper=The Guardian |date=6 June 2012 |access-date=6 June 2012}} The transit was also observed and historically photographed by NASA astronaut Don Pettit aboard the International Space Station.{{cite news |title=Stargazers watch rare Venus transit |url=http://www.aljazeera.com/news/americas/2012/06/20126505956548854.html |newspaper=Al Jazeera |date=6 June 2012 |access-date=6 June 2012}}
NASA's Solar and Heliospheric Observatory could not see the transit as it was not in between the Earth and the Sun at the time of the event, but high-definition images of the event were obtained by Solar Dynamics Observatory, from {{convert|36000|km|mi|abbr=on}} above the Earth. Agency astrophysicist Dr. Lika Guhathakurta said, "We get to see Venus in exquisite detail because of SDO's spatial resolution, SDO is a very special observatory. It takes images that are about 10 times better than a high-definition TV and those images are acquired at a temporal cadence of one every 10 seconds. This is something we've never had before".{{cite news |title=Venus makes rare trek across Sun |first=Jonathan |last=Amos |url=https://www.bbc.co.uk/news/science-environment-17745366 |work=BBC News |date=6 June 2012 |access-date=6 June 2012}}
Research
File:Transit of Venus observations in TL.jpg observing the transit of Venus]]
The 2012 transit gave scientists a number of research opportunities. These included:{{cite news |title=Venus Transit On June 5 May Bring New Alien Planet Discoveries |first=Mike |last=Wall |url=http://www.huffingtonpost.com/2012/05/16/venus-transit-june-5-new-alien-planet_n_1522342.html |newspaper=The Huffington Post |date=16 May 2012 |access-date=6 June 2012}}{{cite news |title=Counting down to the Transit of Venus – our nearest exoplanet test-lab |url=http://phys.org/news/2012-03-transit-venus-nearest-exoplanet.html |work=Phys.Org |date=5 March 2012 |access-date=6 June 2012}}{{cite web |url=https://venustex.oca.eu/foswiki/ |title=The Venus Twilight Experiment: Refraction and scattering phenomena during the transit of Venus on June 5–6, 2012 |work=venustex.oca.eu |access-date=6 June 2012 |archive-url=https://web.archive.org/web/20161023145933/https://venustex.oca.eu/foswiki |archive-date=23 October 2016 |url-status=dead }}
- Measurement of dips in a star's brightness caused by a known planet transiting a known star (the Sun). This will help astronomers when searching for exoplanets. Unlike the 2004 Venus transit, the 2012 transit occurred during an active phase of the 11-year activity cycle of the Sun, and would have provided practice in detecting a planet's signal around a "spotty" variable star.
- Measurement of the apparent diameter of Venus during the transit, and comparison with its known diameter. This will have given information on how to estimate exoplanet sizes.
- The number of locations documenting the event will provide much data via parallax that will generate more accurate measurements.
- Observation of the atmosphere of Venus simultaneously from Earth-based telescopes and from the Venus Express spacecraft. This gave a better opportunity to understand the intermediate level of Venus's atmosphere than is possible from either viewpoint alone, and should provide new information about the climate of the planet.
- Spectrographic study of the atmosphere of Venus. The results of analysis of the well-understood atmosphere of Venus will be compared with studies of exoplanets with atmospheres that are unknown.
- The Hubble Space Telescope used the Moon as a mirror to study the light reflected from Venus to determine the makeup of its atmosphere. This may provide another technique to study exoplanets.
- Experimental reconstruction of Lomonosov's discovery of Venusian atmosphere (1761) with antique refractors.{{cite journal |title=Experimental Reconstruction of Lomonosov's Discovery of Venus's Atmosphere with Antique Refractors During the 2012 Transit of Venus |journal=Solar System Research |publisher=Springer |first1=Alexandre |last1=Koukarine |first2=Igor |last2=Nesterenko |first3=Yuri |last3=Petrunin |first4=Vladimir |last4=Shiltsev |volume=47 |issue=6 |pages=487–490 |date=November 2013 |doi=10.1134/S0038094613060038 |arxiv=1208.5286|bibcode = 2013SoSyR..47..487K }} The researchers observed the "Lomonosov's arc" and other aureole effects due to Venus's atmosphere and concluded that Lomonosov's telescope was fully adequate to the task of detecting the arc of light around Venus off the Sun's disc during ingress or egress if proper experimental techniques as described by Lomonosov in his 1761 paper are employed.
{{Clear}}
Gallery
North America:
File:Transit of Airplane during Transit of Venus across the Sun - June 05, 2012 02.jpg|San Francisco, California, United States
Transit of airliner with Venus
File:Venus Transit from Tempe, AZ June 5, 2012.jpg|Tempe, Arizona, USA
01:54 UTC
File:2012 Transit Of Venus Wichita Falls Texas.JPG|Wichita Falls, Texas, USA
File:Fennell Observatory, Oakland, TN 35.2597°N, 89.5125°W.png|Fennell Observatory
Oakland, Tennessee, USA
File:VenusTransit20120605Toronto.JPG|Toronto, Ontario, Canada
23:06 UTC
Europe:
File:Transit of Venus 2012 Ragusa.jpg|Ragusa, Sicily, Italy
04:11 UTC
File:Transit of Venus 2012 from Moscow.jpg|Moscow, Russia
03:47 UTC
File:Venus Transit Helsingborg Sweden.jpg|Helsingborg, Sweden
04:20 UTC
File:Transit of Venus 06-06-2012.jpg|Úvaly, Czech Republic
04:26 UTC
File:2012venustransit.jpg|Kecskemét, Hungary
03:41 UTC
Asia:
File:Venus Kuwait 2012.jpg|Kuwait City, Kuwait
File:2012 Transit of Venus from Amman, Jordan.jpg|Amman, Jordan
Combination of 3 exposures
File:Beauty Spot on Sun Transit of Venus on June 06, 2012.jpg|Delhi, India
File:The 2012 transit of Venus in Guangzhou.jpg|Guangzhou, China
00:41 UTC
File:Transit of Venus for filter sequence.jpg|Photo sequence from Taichung, Taiwan
File:Анимация прохождения Венеры по Солнцу 06.06.2012.gif|Video from Ussuriysk, Russia
00:08–04:43 UTC
File:Transit of venus 2012 Handa Aichi movie.gif|Video from Handa, Aichi, Japan
23:36–04:50 UTC
Australasia:
File:IMG 2111Venus.JPG|Sydney
23:25 UTC
File:Transit of Venus viewed in Wagga Wagga (2).jpg|Wagga Wagga
00:49 UTC
File:Transit of Venus.jpeg|Clayton
01:06 UTC
Others:
File:SDO%27s Ultra-high Definition View of 2012 Venus Transit.ogv|Solar Dynamics Observatory Ultra-high Definition View
File:Transit of Venus, 2012 Orbital Paths.ogv|This visualization shows the orbital paths of Venus and Earth that led to this rare alignment on 5–6 June 2012
File:ISS-31 Venus passes across the face of the sun.jpg|Venus transit, seen from the International Space Station.
File:Hinode Views the 2012 Venus Transit.jpg|Close-up of Venus by the Japanese Hinode spacecraft on the Sun-synchronous orbit.
File:Venus Transit 2012.ogv|Visualization generated by compositing the small field-of-view, high-cadence closeups of Venus with the full-disk, low-cadence imagery from SDO.
References
{{Reflist}}
Further reading
{{refbegin}}
- {{cite book
| author = Anderson, Mark
| author-link = Mark Anderson (writer)
| title = The Day the World Discovered the Sun: An Extraordinary Story of Scientific Adventure and the Race to Track the Transit of Venus
| year = 2012
| publisher = Da Capo Press
| location = Boston
| isbn = 978-0-306-82038-0}}
- {{cite book
| last = Lomb
| first = Nick
| title = Transit of Venus: 1631 to the Present
| year = 2011
| publisher = NewSouth Publishing
| location = Sydney, Australia
| isbn = 978-1-74223-269-0
| oclc = 717231977}}
- {{cite book
| author = Sellers, David
| title = The Transit of Venus: the Quest to Find the True distance of the Sun
| year = 2001
| publisher = Magavelda Press
| location = Leeds
| isbn = 0-9541013-0-8}}
- {{cite book
| author = Sheehan, William
| author2 = Westfall, John
| title = The Transits of Venus
| year = 2004
| publisher = Prometheus Books
| location = Amherst, New York
| isbn = 1-59102-175-8
| url = https://archive.org/details/transitsofvenus0000shee
}}
- {{cite book
| author = Wulf, Andrea
| author-link = Andrea Wulf
| title = Chasing Venus: The Race to Measure the Heavens
| year = 2012
| publisher = Knopf
| location = New York
| isbn = 978-0-307-70017-9
| url = https://archive.org/details/chasingvenusrace00wulf
}}
{{refend}}
External links
{{commons category}}
- [https://web.archive.org/web/20120518015045/http://venustransit.nso.edu/ Venus Transit of 2012] by the National Solar Observatory
- [http://www.skyandtelescope.com/astronomy-news/observing-news/transits-of-venus-explained/ "Transits of Venus Explained"] by Sky & Telescope
- [http://www.pcworld.com/article/257056/missed_the_venus_transit_in_2012_watch_it_online_until_2115.html "Missed the Venus Transit in 2012? Watch It Online Until 2117"] by PC World
- {{APOD |date=5 June 2012 |title=Watching for Venus to Cross the Sun}}
{{Venus}}