Mount Canicula
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Mount Canicula
Mount Canicula () is a mountain formed of two rock peaks, high. It stands east of Sirius Knoll on the divide separating Russell East Glacier and Russell West Glacier in central Trinity Peninsula, and is linked to Louis-Philippe Plateau to the north by Verdikal Gap, and to Trakiya Heights to southwest by Srem Gap.Verdikal Gap.
SCAR Composite Antarctic Gazetteer. It was charted in 1946 by the
Falkland Islands Dependencies Survey The British Antarctic Survey (BAS) is the United Kingdom's national polar research institute. It has a dual purpose, to conduct polar science, enabling better understanding of global issues, and to provide an ...
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Sirius Knoll
Sirius Knoll () is a conspicuous ice-covered knoll, 1,010 m, situated 2.28 km north-northeast of Mount Schuyler and marking the northeast end of Detroit Plateau in the central part of Trinity Peninsula in Antarctica. Surmounting Russell West Glacier to the north. Charted in 1946 by the Falkland Islands Dependencies Survey (FIDS) and named after Sirius, the dog star. Map Trinity Peninsula.Scale 1:250000 topographic map No. 5697. Institut für Angewandte Geodäsie and British Antarctic Survey, 1996. References SCAR Composite Antarctic Gazetteer
Hills of Trinity Peninsula {{TrinityPeninsula-geo-stub ...
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Russell East Glacier
Russell East Glacier () is a glacier, 6 nautical miles (11 km) long and 3 nautical miles (6 km) wide, which lies at the north end of Detroit Plateau and flows from Mount Canicula and Verdikal Gap along the south slopes of Erul Heights eastward into Smokinya Cove in Prince Gustav Channel on the south side of Trinity Peninsula. This glacier together with Russell West Glacier, which flows westward into Bone Bay on the north side of Trinity Peninsula, form a through glacier across the north part of Antarctic Peninsula. It was first surveyed in 1946 by the Falkland Islands Dependencies Survey (FIDS). Named by the United Kingdom Antarctic Place-Names Committee (UK-APC) for V.I. Russell, surveyor and leader of the FIDS base at Hope Bay in 1946. See also * List of glaciers in the Antarctic * Glaciology Glaciology (; ) is the scientific study of glaciers, or more generally ice and natural phenomena that involve ice. Glaciology is an interdisciplinary Earth science ...
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Russell West Glacier
Russell West Glacier () is a glacier, 11 nautical miles (20 km) long and 4 nautical miles (7 km) wide, which lies immediately north of Detroit Plateau and flows from Mount Canicula, Verdikal Gap and Trajan Gate westward into Bone Bay on the north side of Trinity Peninsula. This glacier together with Russell East Glacier, which flows eastward into Prince Gustav Channel on the south side of Trinity Peninsula, form a through glacier across the north part of Antarctic Peninsula. It was first surveyed in 1946 by the Falkland Islands Dependencies Survey (FIDS). Named by the United Kingdom Antarctic Place-Names Committee (UK-APC) for V.I. Russell, surveyor and leader of the FIDS base at Hope Bay in 1946. See also * Allen Knoll * List of glaciers in the Antarctic * Glaciology Glaciology (; ) is the scientific study of glaciers, or more generally ice and natural phenomena that involve ice. Glaciology is an interdisciplinary Earth science that integrates geophysics, geolo ...
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Trinity Peninsula
Trinity Peninsula is the northernmost part of the Antarctic Peninsula. It extends northeastward for about 130 km (80 mi) to Cape Dubouzet from an imaginary line connecting Cape Kater on the north-west coast and Cape Longing on the south-east coast. Prime Head is the northernmost point of this peninsula. Some 20 kilometers southeast of Prime Head is Hope Bay with the year-round Argentinian Esperanza Base. History It was first sighted on 30 January 1820 by Edward Bransfield, Master, Royal Navy, immediately after his charting of the newly discovered South Shetland Islands nearby. In the century following the peninsula's discovery, chartmakers used various names (Trinity Land, Palmer Land, and Land of Louis Philippe) for this portion of it, each name having some historical merit. The recommended name derives from "Trinity Land", given by Bransfield during 1820 in likely recognition of the Corporation of Trinity House, Britain's historical maritime pilotage authority, altho ...
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Louis-Philippe Plateau
Louis Philippe Plateau () is a plateau, about long and wide, which rises to and occupies the central part of Trinity Peninsula, Antarctica, between Russell West Glacier and Windy Gap. This application of the name, recommended by the UK Antarctic Place-Names Committee in 1948, commemorates Captain Jules Dumont d'Urville's 1838 exploration of the Trinity Peninsula area, which he had named "Terre Louis Philippe," after Louis Philippe I, the King of France at the time. Central plateaus of Graham Land North to south: * Laclavère Plateau * Louis Philippe Plateau * Detroit Plateau * Herbert Plateau * Foster Plateau * Forbidden Plateau * Bruce Plateau * Avery Plateau * Hemimont Plateau Hemimont Plateau ( bg, плато Хемимонт, plato Hemimont, ) is the long and narrow ice-covered plateau of elevation about 1600 m in southern Graham Land, Antarctica bordering Avery Plateau on the north. It is situated midway between Lo ... References Plateaus of Antarctica Landfo ...
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Verdikal Gap
Verdikal Gap ( bg, Вердикалска седловина, ‘Verdikalska Sedlovina’ \ver-di-'kal-ska se-dlo-vi-'na\) is the flat ice-covered saddle with an elevation of 801 mReference Elevation Model of Antarctica.
Polar Geospatial Center. University of Minnesota, 2019
located on in , . It is part of the ice divide between

Trakiya Heights
The Trakiya Heights ( bg, Тракийски възвишения, ‘Trakiyski Vazvisheniya’ \tra-'kiy-ski v&z-vi-'she-ni-ya\) are the heights rising to ( Irakli Peak) on Trinity Peninsula, Antarctic Peninsula. The heights are bounded by Russell West Glacier to the north, Srem Gap and Russell East Glacier to the northeast, Victory Glacier to the southwest and Zlidol Gate to the northwest. The heights surmount Prince Gustav Channel, Weddell Sea The Weddell Sea is part of the Southern Ocean and contains the Weddell Gyre. Its land boundaries are defined by the bay formed from the coasts of Coats Land and the Antarctic Peninsula. The easternmost point is Cape Norvegia at Princess Martha ... to the southeast. The heights extend in northwest-southeast direction and in northeast-southwest direction. The heights are named after the historical region of Trakiya (Thrace). Location The Trakiya Heights are centred at . German-British mapping in 1996. Maps Trinity Peni ...
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Srem Gap
Srem Gap ( bg, Сремска седловина, ‘Sremska Sedlovina’ \'srem-ska se-dlo-vi-'na\) is the flat saddle of elevation 813 mReference Elevation Model of Antarctica.
Polar Geospatial Center. University of Minnesota, 2019
extending 1.35 km on , , which is situated between to the northwest and a tributary glacier to

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Falkland Islands Dependencies Survey
The British Antarctic Survey (BAS) is the United Kingdom's national polar research institute. It has a dual purpose, to conduct polar science, enabling better understanding of global issues, and to provide an active presence in the Antarctic on behalf of the UK. It is part of the Natural Environment Research Council (NERC). With over 400 staff, BAS takes an active role in Antarctic affairs, operating five research stations, one ship and five aircraft in both polar regions, as well as addressing key global and regional issues. This involves joint research projects with over 40 UK universities and more than 120 national and international collaborations. Having taken shape from activities during World War II, it was known as the Falkland Islands Dependencies Survey until 1962. History Operation Tabarin was a small British expedition in 1943 to establish permanently occupied bases in the Antarctic. It was a joint undertaking by the Admiralty and the Colonial Office. At the end of t ...
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Canicula
Sirius is the brightest star in the night sky. Its name is derived from the Ancient Greek language, Greek word , or , meaning 'glowing' or 'scorching'. The star is designated α Canis Majoris, Latinisation of names, Latinized to Alpha Canis Majoris, and abbreviated Alpha CMa or α CMa. With a visual apparent magnitude of −1.46, Sirius is almost twice as bright as Canopus, the next brightest star. Sirius is a binary star consisting of a main-sequence star of spectral type A-type main-sequence star, A0 or A1, termed Sirius A, and a faint white dwarf companion of spectral type DA2, termed Sirius B. The distance between the two varies between 8.2 and 31.5 astronomical units as they orbit every 50 years. Sirius appears bright because of its intrinsic luminosity and its proximity to the Solar System. At a distance of , the Sirius system is one of Earth's List of nearest stars, nearest neighbours. Sirius is gradually moving closer to the Solar System, so it is expected ...
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