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St. Mary's Islands ( ), are a set of four small islands in the Arabian Seamarker off the coast of Malpemarker in Udupimarker, Karnatakamarker, Indiamarker. They are known for their distinctive geological formation of columnar basaltic lava (pictured).

Scientific studies indicate that the basalt of the St. Mary’s Islands was formed by sub-aerial subvolcanic activity, because at that time Madagascarmarker was attached to India. The rifting of Madagascar took place around 88 Ma.

The islands form one of the four geological monuments in Karnataka state, out of the 26 ‘‘Geological Monuments of India’’ declared by the Geological Survey of India in 2001. The monument is considered an important site for "Geo Tourism".


According to folk legend, in the year 1498, Vasco da Gama landed at St. Mary's Islands on his voyage from Portugalmarker to India, fixed a cross on the island and named one of these islands, El Padron de Santa Maria, as a dedication to Mother Mary, before he proceeded to Kozhikodemarker in Keralamarker. It is from this name that the islands have got their current name.

Geography and topography

Out of the four islands which form St. Mary’s Islands, the northernmost island has a basaltic rock formation in a hexagonal form, the only one of its type in India. The island covers an area which is about in length with a width of . It has prominent coconut trees, its cover reflecting in an azure south sea colour, and hence the island is also called Coconut Island. There is no habitation on the islands.

The north-south alined islands are in a non continuous chain. The four large islands are Coconut Island, North Island, Daryabahadurgarh Island and South Island..

The type of rock formation seen on Coconut island is also found atn the Giant's Causewaymarker in Northern Irelandmarker. The stretch of sea between the islands and the long curve of the beach at Malpe is serene and calm.

The islands are generally aligned parallel to the coast line, which provide clues to the phenomenon of uplift of the west coast of India. The islands’ terraces and elevated beach deposits along with the tide gauge data at the dead oyster beach in Suratkalmarker beach (further south of the islands) have been deduced as proof of the reported fall in sea level of about 1 mm/per year.

The highest elevation at Coconut Island, which has generated interest among geologists and tourists, is about above msl with surrounding areas in the form of platforms in the elevation range of + , + , + and + 0 m which are stated to have been formed by wave action pointing to an “episodic sea level rise or fall of land”.


A View of basaltic rock formation in St Mary’s Island
The columnar basaltic lava found in these Islands, which is very well developed in the basalts of Deccan Trap, exhibit an imposing range of hexagonal shaped or multi-faced (polygonal) columns split into a horizontal mosaic. In geological idiom these are called “Columnar Joints”. The lava rocks form regular five, six or seven-sided pillars, called “laminar lava”, and are found in varying heights in all the islands; the tallest of the columns is about 6 m. Considering the importance and rarity of such an occurrence, these islands were classified as a National Geological Monument in 2001 by the Geological Survey of India..

The Deccan Trap, of about 60 million years vintage (CretaceousEocene time), emerged from the vast deluge of hot molten basaltic lava in the western part of India which is now seen as flat topped hills and step like terraces..Scientific studies carried out at the Indian Institute of Technology, Bombaymarker on the Petrology, Palaeomagnetism and Volcanics of the rocks of the island has brought out the following facts.
  • Islands comprise fully of igneous rocks. They have acid composition that consist of dacites, rhyodacites, rhyolites and granophyres and carry basic patches.
  • The columnar jointing pattern is well developed on Coconut Island.
  • Minerologically, Plagioclase, K-feldspar, quartz, ortho-and Clinopyroxenes, olivine, magnetite, and ilmenite are recorded in the ground mass phases
  • Magnetic granulometric studies (susceptibility and hysteresis at different temperatures) of island rock samples indicate the presence of a multi domain (MD) state of magnetite. It is inferred that:
    the formation of MD could have affected the stability and consistency of magnetic directions in these rocks.
  • It has also been inferred that:
    This igneous body has been either annealed or could be an intrusive.
An analysis of Palaeomagnetic data from India and Madagascarmarker hypothesizes a new India–Madagascar fit related to the Late Cretaceous, directly prior to and during the early phase of Madagascar–India separation. A scientific study paper on Late Cretaceous India–Madagascar fit and timing of break–up related magmatism by several scholars reported in the Wiley Inter Science Journal states:.
St. Mary magmatismis linked to the initial break–up between India and Madagascar, and magmatism probably resulted from rift–related extensional processes initially induced by the Marion hotspot underlying southern Madagascar during the Late Cretaceous

Geological age of the rock

There are different theories on the age of the St. Mary’s Islands rocks. In the analysis reported in the above section it has been further concluded that the multi domain (MD) state found in these rocks are not as common in the Deccan Trapsmarker and are reported to be non-existent in the Rajmahal Traps. Six selected samples from the Islands were subject to whole rock K-Ar dating. This yielded a mean age of 93.1 + 2.4 (2σ) vis-à-vis the age of the Rajmahal Traps of about 105-100 Ma and about 65-35 Ma of the Deccan Trapsmarker. With this appreciation, the author has concluded that the igneous activity of St. Mary’s Islands may represent Cretaceous-Tertiary igneous activity..

In a further analysis of the age of the break-up of Greater India (India plus Seychellesmarker) and Madagascar carried out by the scientists of the Physical Research Laboratory, Ahmedabadmarker, India reported in a scientific paper in Earth and Planetary Science Letters, it has been inferred to have occurred in the Upper Cretaceous at 88 Ma. The strength of this inference is based on the approach that the Felsic volcanics (rhyolites and Rhyodacites) of the St. Mary’s Islands (SMI), Southern India, were originally interpreted as a distant outlier of the 65 Ma Deccan volcanic province of west–central India, comprising dominantly flood basalts. Later studies had dated it at 93 Ma by the K-Ar dating technique. Since the technique used was a simple use of an average of five out of six widely varying dates and arbitrary data selectivity chosen, the results were not considered reliable. A method of 40Ar–39Ar (Argon argon dating) of the SMI volcanic yields is reportedly more reliable of the plateau and isochron ages. The weighted mean isochron age is reported to be 85.6±0.9 Ma (2σ). The K–Ar (Potassium-argon dating) technique adopted for the southern Indian Precambrian terrain, intruded by numerous mafic–doleritic dyke swarms, the age from Proterozoic to the latest Cretaceous is reported as 69–65 Ma, (Deccan-related). The two regional dykes (a leucograbbro and a felsite) from the Keralamarker region of southwestern India, which were also dated earlier, indicate the age as 85 Ma. Madagascar flood basalt province’s 40Ar–39Ar ages of 89–85 Ma tallies with the Saint Mary’s Islands’ volcanic age. The conclusion drawn by the study is that the Madagascar flood basalt province, the SMI volcanics, and possibly the Kerala dykes may well represent volcanic activity associated with the break-up of Greater India (India plus Seychellesmarker) and Madagascarmarker, in the Upper Cretaceous at 88 Ma.Another scientific study on the biogeographic and tectonic history of India by Briggs reported in the Journal of Biogeography (2003)it is concluded that:
Although real breaks among the lands were indicated by the physical data, faunal links were maintained by vagile animals that were able to surmount minor marine barriers.
India, during its northward journey, remained close to Africa and Madagascarmarker even as it began to contact Eurasia.

General information

The western coasts of the islands are a seashell haven with seashells of various shapes and sizes littered along the coast. There is no sand beach to swim and relax since it is scatted with basaltic rocks. But there are flat slabs to sit and enjoy the serenity of the place. The beach has security guards who ensure that visitors do not venture into danger zones of the islands. Watching Sun set at the Islands is also a special sight.. It is a popular picnic spot with locals and tourists alike. December to March is the best season to visit the Islands.

All links to the island are only through the mainland town of Malpe, which is a major fishing harbor. The beach at this location is enlivening. It is located at a distance of 5 km west of Udupi town, the administrative headquarters for the Islands. Apart from the Islands, Malpe too has tourist attractions such as the Vadabhandeshwara Temple and an image of Sri Balarama consecrated by the saint Madhwacharya the founder of Dvaita Philosophy.

A detailed description of the natural flora and fauna of the Islands and the Deria Bahdur Ghur, have been compiled in a manual by John Sturrocks who was the district collector of Mangalore at that time in 1894.

Flora and fauna
Colonies of Gulls, Scolopacidae (sandpipers) and a few crows have been sighted on the Islands. But on the approach to the Islands from the Malpe beach, Brahminy Kites (Haliastur indus)), Great White Egrets, Grey Egrets (breeding plumage) and groups of large Green Bee-eaters have been recorded.

Visitor Information
The Islands are bereft of buildings, fences, shops. There are no domestic animals either. There are only covered pavilions with park benches on the shore and further inland. Visitors can wander around freely and enjoy the hexagonal formations from vanatge locations. Visitors have to carry drinking water and sun screens since the climate is either very hot or hot. Since the last few yards of the approach to the island involves wading, it may be preferable to avoid wearing sneakers.

Access to the islands

The only way of getting to the islands is by boat. Regular ferry service ply the 6 km distance from the Malpemarker fishing harbor (which has a ship building yard also) to the islands. However, the frequency of these boats may vary depending on the number of tourists visiting. It is to the North of Mangaloremarker, the coastal city of Karnataka, which is also the nearest airport. The famous religious town Udupimarker, is about West North West of Mangaloremarker. Mumbaimarker, Udupimarker and Thiruvananthapurammarker are linked to Malpe, by the West Coast Railway. The Konkan Railway (map pictured) passes close to the Islands, starting from Mangalore passing through Udupi, Kundapuramarker, Goamarker, Ratnagirimarker and Roha close to Mumbai. Malpe is from Udupi town.

Pictures of St. Mary's Islands

Image:St Mary's Island.JPG|A beach on one of the St. Mary's IslandsImage:St Mary's Island rocks.JPG|Rocks at St. Mary's IslandsImage:St Mary's island.JPG|A view from Ferry towards St. Mary's IslandsFile:Q2160048.jpg| Another view of the IslandFile:Calidris-alpina-001 edit.jpg|Sandpipers on the IslandFile:Black-headed Gull - St James's Park, London - Nov 2006.jpg|GullsFile:Brahminy Kite (Haliastur indus) in Kawal, AP W IMG 2248.jpg|Brahminy KiteFile:Great Egret Fish.jpg|Great White Egret

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