Astronomy in Antarctica, current projects, future goals and challenges

If you were to ask an astronomer to define the perfect place to locate a telescope, they'd tell you to have it somewhere cold, dark, at high-altitude, with a local climate that contained dry stable air. In short, Antarctica. In New Zealand for example adverse effects, such as the movement air i...

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Main Author: Skinner, Richard
Format: Other/Unknown Material
Language:English
Published: University of Canterbury 2016
Subjects:
Online Access:http://hdl.handle.net/10092/13840
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spelling ftunivcanter:oai:ir.canterbury.ac.nz:10092/13840 2023-05-15T13:55:49+02:00 Astronomy in Antarctica, current projects, future goals and challenges Skinner, Richard 2016 application/pdf http://hdl.handle.net/10092/13840 English en eng University of Canterbury http://hdl.handle.net/10092/13840 All Rights Reserved Theses / Dissertations 2016 ftunivcanter 2022-09-08T13:32:04Z If you were to ask an astronomer to define the perfect place to locate a telescope, they'd tell you to have it somewhere cold, dark, at high-altitude, with a local climate that contained dry stable air. In short, Antarctica. In New Zealand for example adverse effects, such as the movement air in our atmosphere, can cause images to wiggle and warp, such as the observable twinkling of a star in the night sky. Antarctic astronomy, including the operation of the South Pole Telescope, located at Amundsen Station, can largely overcome these problems. In taking advantage of the cold dark skies, these telescopes are able to probe the deep reaches of space, in order to answer some of the fundamental questions related to the universe, including the search for theoretical dark matter and dark energy. Other less conventional astronomy related projects in Antarctica include the 'Ice Cube array'. This uses ultrasensitive light detectors, buried over a mile deep in the Antarctic ice sheet, to detect high-energy neutrinos that were created by the most violent events in the universe, which allow astronomers to visualize distant cosmic events by detecting the neutrinos they create. Other scoping studies have have identified several high altitude sites in East Antarctica such as those at Dome A and 'Dome C' where there is the potential to locate a very large optical or Infra-Red telescope for the search of earth-like planets in other solar systems. Housing such complex equipment in these remote areas, as well as keeping the stations supplied and maintained, is not a simple task and this review will examine the science produced, technical challenges that have to be overcome, potential environmental impacts, as well as examining whether the science produced is worth the costs and resources involved. Other/Unknown Material Antarc* Antarctic Antarctica East Antarctica Ice Sheet South pole South pole University of Canterbury, Christchurch: UC Research Repository Antarctic The Antarctic East Antarctica New Zealand South Pole
institution Open Polar
collection University of Canterbury, Christchurch: UC Research Repository
op_collection_id ftunivcanter
language English
description If you were to ask an astronomer to define the perfect place to locate a telescope, they'd tell you to have it somewhere cold, dark, at high-altitude, with a local climate that contained dry stable air. In short, Antarctica. In New Zealand for example adverse effects, such as the movement air in our atmosphere, can cause images to wiggle and warp, such as the observable twinkling of a star in the night sky. Antarctic astronomy, including the operation of the South Pole Telescope, located at Amundsen Station, can largely overcome these problems. In taking advantage of the cold dark skies, these telescopes are able to probe the deep reaches of space, in order to answer some of the fundamental questions related to the universe, including the search for theoretical dark matter and dark energy. Other less conventional astronomy related projects in Antarctica include the 'Ice Cube array'. This uses ultrasensitive light detectors, buried over a mile deep in the Antarctic ice sheet, to detect high-energy neutrinos that were created by the most violent events in the universe, which allow astronomers to visualize distant cosmic events by detecting the neutrinos they create. Other scoping studies have have identified several high altitude sites in East Antarctica such as those at Dome A and 'Dome C' where there is the potential to locate a very large optical or Infra-Red telescope for the search of earth-like planets in other solar systems. Housing such complex equipment in these remote areas, as well as keeping the stations supplied and maintained, is not a simple task and this review will examine the science produced, technical challenges that have to be overcome, potential environmental impacts, as well as examining whether the science produced is worth the costs and resources involved.
format Other/Unknown Material
author Skinner, Richard
spellingShingle Skinner, Richard
Astronomy in Antarctica, current projects, future goals and challenges
author_facet Skinner, Richard
author_sort Skinner, Richard
title Astronomy in Antarctica, current projects, future goals and challenges
title_short Astronomy in Antarctica, current projects, future goals and challenges
title_full Astronomy in Antarctica, current projects, future goals and challenges
title_fullStr Astronomy in Antarctica, current projects, future goals and challenges
title_full_unstemmed Astronomy in Antarctica, current projects, future goals and challenges
title_sort astronomy in antarctica, current projects, future goals and challenges
publisher University of Canterbury
publishDate 2016
url http://hdl.handle.net/10092/13840
geographic Antarctic
The Antarctic
East Antarctica
New Zealand
South Pole
geographic_facet Antarctic
The Antarctic
East Antarctica
New Zealand
South Pole
genre Antarc*
Antarctic
Antarctica
East Antarctica
Ice Sheet
South pole
South pole
genre_facet Antarc*
Antarctic
Antarctica
East Antarctica
Ice Sheet
South pole
South pole
op_relation http://hdl.handle.net/10092/13840
op_rights All Rights Reserved
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