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Post Info TOPIC: Dome C


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Title: A review of optical sky brightness and extinction at Dome C, Antarctica
Authors: Suzanne L. Kenyon, John W. V. Storey (School of Physics, University of New South Wales)

The recent discovery of exceptional seeing conditions at Dome C, Antarctica, raises the possibility of constructing an optical observatory there with unique capabilities. However, little is known from an astronomer's perspective about the optical sky brightness and extinction at Antarctic sites.
Researchers review the contributions to sky brightness at high-latitude sites, and calculate the amount of usable dark time at Dome C. They also explore the implications of the limited sky coverage of high-latitude sites and review optical extinction data from the South Pole.
They also examine the proposal of Baldry and Bland-Hawthorn (2001) to extend the amount of usable dark time through the use of polarising filters.

Read more (PDF)

Located at 75.6' South, 123.21' East and an altitude of 3250 m, Dome C is the third highest point on the Antarctica Plateau.
The cloud cover is very low with cloud-free skies observed for at least 74% of the time.


Comparison with Mauna Kea

The local topography of Dome C is extremely flat, resulting in a mean ground-level wind speed of 2.9 ms^-1 (Aristidi et al. 2005a), less than half that at most other observatories.
2005). In addition, the site is extremely cold and the atmosphere has very low precipitable water vapour in comparison to other sites.

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Dome C is one of the most barren places in the world. As one visitor said: "Once you've seen the horizon, you've seen everything" .
Looking at the vast white desert, like the ice world Hoth, it is hard to see what Dome C could possibly contribute to our never ending study of the universe and the search for extraterrestrial life.


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Australian Astronomers hope to kick-start their long-running push to build a telescope in Antarctica in the latest 10-year plan for Australian astronomy.

A draft version of the so-called decadal plan will be discussed at the annual scientific meeting of the Astronomical Society of Australia in Sydney next month.

One of the key recommendations is to go forward with what's now being called the PILOT project in Antarctica.

The proposed 2 metre infra-red telescope was originally scheduled to be completed at Antarctica's Dome C this year. But lack of funds have stalled the project and frustrated astronomers.

Dome C is one of the local summits of Antarctica , accessible from McMurdo Sound. Dome C on the high Antarctic plateau, is one of the coldest, flattest and whitest place on earth.

The summer temperature oscillates between -25°C and -50°C, and the winter temperature between -50°C and -80°C!


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Panorama from Dome C, Antarctica, 1997

Astronomer Dr Michael Burton of the University of New South Wales, a member of a working group for the decadal plan, says Australia risks being left behind by the international astronomy community.

He says Australia's strength in astronomy has traditionally been founded on its radio and infra-red capabilities.
But there are concerns it has fallen behind in infra-red astronomy, which studies infra-red radiation emitted by objects in space.

Infra-red is superior to traditional optical or radio astronomy in detecting the most distant objects in the universe, which have a high 'redshift', a change in the wavelength of light where the wavelength is longer than it was at the source.

"Clearly we have fallen behind in the last decade or so from being one of the major players in that field to just another group with a small facility. We haven't become a major part of any of the big projects which have developed over the last decade and that's definitely a worry"- Dr Michael Burton.


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mcMurdo Sound

Burton says Australia is currently a 5% member of the international Gemini Observatory consortium, which gives it access to two of the world's biggest telescopes in Hawaii and Chile.

This compares to a decade ago when it was a 50% member of the Anglo-Australian Observatory, which at the time hosted what was then one of the world's eight biggest telescopes.

"The problem is that we don't have the really good sites for doing (infra-red) in mainland Australia" .

It is hoped that PILOT which will cost about A$10 million, will put Australia in the position where it can eventually build an extra large telescope in Antarctica.

"What we're trying to do in Antarctica at the moment is build the telescopes there that can put us in a position where we can build the big ones. (PILOT) really is a pathfinder for what could be the ultimate ground-based telescope" - Dr Michael Burton.

The French and Italian programs are already planning to open a station that will run all year round, making Dome C the next logical place for a multi million dollar observatory.
The observatory will be an international collaboration, but the real race is in each country persuading their respective governments to fund the observatory.
Whichever government puts forward the largest amount of money will effectively have the controlling interest in the telescope and make most of the decisions.

Antarctica is the driest continent on Earth and its elevated inland plateau, along with its stable clear weather and absence of daylight in winter, make it ideal for watching the stars.

Professor Warrick Couch, head of physics at the University of New South Wales and another decadal plan working group member, disagrees that Australia is falling behind in infra-red astronomy.

He says Australia is capable of doing "very useful", albeit limited, infra-red astronomy from facilities at the Anglo-Australian Observatory at Siding Spring and the Australian National University.

"The argument for a thing like PILOT ... is that we would [have] something that's pretty much solely Australian owned. It's not that we don't have an infra-red astronomy going on because we certainly do. It's really another opportunity to build on what we're doing at the moment" - Professor Warrick Couch

Going ahead with PILOT will increase Australia's ability to study how stars and galaxies form and find previously undetected planets, Couch says.

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