Jumat, 17 Juni 2011

Gerhana bulan

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Gerhana Bulan
Diagram gerhana bulan: Bayangan bumi yang menutupi bulan
Gerhana bulan terjadi saat sebagian atau keseluruhan penampang bulan tertutup oleh bayangan bumi. Itu terjadi bila bumi berada di antara matahari dan bulan pada satu garis lurus yang sama, sehingga sinar matahari tidak dapat mencapai bulan karena terhalangi oleh bumi.
Dengan penjelasan lain, gerhana bulan muncul bila bulan sedang beroposisi dengan matahari. Tetapi karena kemiringan bidang orbit bulan terhadap bidang ekliptika, maka tidak setiap oposisi bulan dengan matahari akan mengakibatkan terjadinya gerhana bulan. Perpotongan bidang orbit bulan dengan bidang ekliptika akan memunculkan 2 buah titik potong yang disebut node, yaitu titik di mana bulan memotong bidang ekliptika. Gerhana bulan ini akan terjadi saat bulan beroposisi pada node tersebut. Bulan membutuhkan waktu 29,53 hari untuk bergerak dari satu titik oposisi ke titik oposisi lainnya. Maka seharusnya, jika terjadi gerhana bulan, akan diikuti dengan gerhana matahari karena kedua node tersebut terletak pada garis yang menghubungkan antara matahari dengan bumi.
Sebenarnya, pada peristiwa gerhana bulan, seringkali bulan masih dapat terlihat. Ini dikarenakan masih adanya sinar matahari yang dibelokkan ke arah bulan oleh atmosfer bumi. Dan kebanyakan sinar yang dibelokkan ini memiliki spektrum cahaya merah. Itulah sebabnya pada saat gerhana bulan, bulan akan tampak berwarna gelap, bisa berwarna merah tembaga, jingga, ataupun coklat.
Gerhana bulan dapat diamati dengan mata telanjang dan tidak berbahaya sama sekali.

[sunting] Jenis-jenis gerhana bulan

  • Gerhana bulan total
Pada gerhana ini, bulan akan tepat berada pada daerah umbra.
  • Gerhana bulan sebagian
Pada gerhana ini, tidak seluruh bagian bulan terhalangi dari matahari oleh bumi. Sedangkan sebagian permukaan bulan yang lain berada di daerah penumbra. Sehingga masih ada sebagian sinar matahari yang sampai ke permukaan bulan.
  • Gerhana bulan penumbra
Pada gerhana ini, seluruh bagian bulan berada di bagian penumbra. Sehingga bulan masih dapat terlihat dengan warna yang suram.

[sunting] Galeri


Sabtu, 28 Mei 2011

 
 
 
 
 
     

jalak bali

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?Jalak Bali
Jalak Bali di Kebun Binatang Brookfield
Jalak Bali di Kebun Binatang Brookfield
Status konservasi
Klasifikasi ilmiah
Kerajaan: Animalia
Filum: Chordata
Kelas: Aves
Ordo: Passeriformes
Famili: Sturnidae
Genus: Leucopsar
Stresemann, 1912
Spesies: L. rothschildi
Nama binomial
Leucopsar rothschildi
Stresemann, 1912
Jalak Bali
Jalak Bali di Kebung Binatang Houston
Jalak Bali (Leucopsar rothschildi) adalah sejenis burung pengicau berukuran sedang, dengan panjang lebih kurang 25cm, dari suku Sturnidae. Jalak Bali memiliki ciri-ciri khusus, di antaranya memiliki bulu yang putih di seluruh tubuhnya kecuali pada ujung ekor dan sayapnya yang berwarna hitam. Bagian pipi yang tidak ditumbuhi bulu, berwarna biru cerah dan kaki yang berwarna keabu-abuan. Burung jantan dan betina serupa.
Endemik Indonesia, Jalak Bali hanya ditemukan di hutan bagian barat Pulau Bali. Burung ini juga merupakan satu-satunya spesies endemik Bali dan pada tahun 1991 dinobatkan sebagai lambang fauna Provinsi Bali. Keberadaan hewan endemik ini dilindungi undang-undang.
Jalak Bali ditemukan pertama kali pada tahun 1910. Nama ilmiah Jalak Bali dinamakan menurut pakar hewan berkebangsaan Inggris, Walter Rothschild, sebagai orang pertama yang mendeskripsikan spesies ini ke dunia pengetahuan pada tahun 1912.
Karena penampilannya yang indah dan elok, jalak Bali menjadi salah satu burung yang paling diminati oleh para kolektor dan pemelihara burung. Penangkapan liar, hilangnya habitat hutan, serta daerah burung ini ditemukan sangat terbatas menyebabkan populasi burung ini cepat menyusut dan terancam punah dalam waktu singkat. Untuk mencegah hal ini sampai terjadi, sebagian besar kebun binatang di seluruh dunia menjalankan program penangkaran jalak Bali.
Jalak Bali dinilai statusnya sebagai kritis di dalam IUCN Red List serta didaftarkan dalam CITES Appendix I.

[sunting] Lihat pula

[sunting] Referensi

[sunting] Pranala luar

andes

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Andes (Quechua: Anti(s/kuna))
Range
Aerial photo of a portion of the Andes between Argentina and Chile
Countries Argentina, Bolivia, Chile, Colombia, Ecuador, Peru, Venezuela

Cities Bogotá, Santiago, Medellín, La Paz, Cali, Quito, Pasto, Bucaramanga, Arequipa, Mendoza, Cuenca, Cochabamba, Pereira, Ibagué, Salta, Manizales

Highest point Mt. Aconcagua
 - location Las Heras Department, Mendoza, Argentina
 - elevation 6,962 m (22,841 ft)
 - coordinates 32°39′10″S 70°0′40″W / 32.65278°S 70.01111°W / -32.65278; -70.01111

Length 7,000 km (4,350 mi)
Width 500 km (311 mi)

Composite satellite image of the southern Andes
The Andes is the world's longest continental mountain range. It is a continual range of highlands along the western coast of South America. This range is about 7,000 km (4,300 mi) long, about 200 km (120 mi) to 700 km (430 mi) wide (widest between 18 degrees South and 20 degrees South latitude), and of an average height of about 4,000 m (13,000 ft).
Along its length, the Andes is split into several ranges, which are separated by intermediate depressions. The Andes is the location of several high plateaux – some of which host major cities such as Quito, Bogotá, Arequipa, Medellín, Sucre, and La Paz.
The so-called Altiplano plateau is the world's second-highest plateau following the Tibetan plateau. The Andes extends to seven countries, in alphabetical order: Argentina, Bolivia, Chile, Colombia, Ecuador, Peru, and Venezuela, some of which are known as the Andean States.
The Andes range is the world's highest mountain range outside of the continent of Asia. The highest peak, Mt. Aconcagua, rises to an elevation of about 6,962 m (22,841 ft) above sea level. The peak of Mt. Chimborazo in the Ecuadorean Andes is located at the point on the surface of the Earth that is the most distant one from its centre. This is because of the Earth's equatorial bulge that results from its rotation. The world's highest volcanos are in the Andes, including Ojos del Salado on the Chile-Argentina frontier which rises to 6,893 m (22,615 ft), and over 50 other volcanos that rise above 6,000 m.

Contents

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[edit] Name

The etymology of the word Andes has been debated. The major consensus is that it derives from the Quechua word anti, which means "high crest". Others believe that Andes comes from Anti Suyu, one of the four regions of the Inca empire. It is more likely however that the word Antisuyo derives from the use of Anti to designate mountain chains. Derivation from the Spanish andén (in the sense of cultivation terrace) has also been proposed, yet considered very unlikely.

[edit] Geography

Aerial view of Aconcagua.
The Andes can be divided into three sections:
I. The Southern Andes in Argentina and Chile;
II. The Central Andes, including the Chilean and Peruvian cordilleras and parts of Bolivia;
III. The Northern Andes in Venezuela, Colombia, and Ecuador that consists of two parallel ranges, the Cordillera Occidental and the Cordillera Oriental. In Colombia, north its the border with Ecuador, the Andes split in three parallel ranges, the western, central, and eastern ranges. (The cordillera occidental, central, and oriental).
In the northern part of the Andes, the isolated Sierra Nevada de Santa Marta range is often considered to be part of the Andes. The eastern range of Colombia is the only one that extends to Venezuela.[1] The term cordillera comes from the Spanish word meaning "cuerda", meaning "rope". The Andes range is about 200 km (124 mi) wide throughout its length, except in the Bolivian flexure where it is about 640 kilometres (398 mi) wide. The islands of the Dutch Caribbean Aruba, Bonaire, and Curaçao, which lie in the Caribbean Sea off the coast of Venezuela, were thought to represent the submerged peaks of the extreme northern edge of the Andes range, but ongoing geological studies indicate that such a simplification does not do justice to the complex tectonic boundary between the South-American and Caribbean plates. [2]

[edit] Geology

Geology of the Andes
The Andes
Orogenies
Pampean orogeny
Famatinian orogeny
Gondwanide orogeny
Andean orogeny
Fold-thrust belts
Central Andean | Patagonian
Batholiths
Peruvian Coastal | North Patagonian | South Patagonian
Subducted structures
Antarctic Plate | Carnegie Ridge | Chile Rise | Farallon Plate (formerly) | Juan Fernández Ridge | Nazca Plate | Nazca Ridge
Faults
Gastre | Liquiñe-Ofqui | Magallanes-Fagnano
Andean Volcanic Belt
Northern Zone| Peruvian flat-slab | Central Zone | Pampean flat-slab | Southern Zone | Patagonian Gap | Austral Zone
Paleogeographic terminology
Arequipa-Antofalla Terrane | Chilenia | Chiloé Block | Cuyania | Iapetus Ocean | Madre de Dios Terrane | Mejillonia | Pampia
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The Andes are a MesozoicTertiary orogenic belt of mountains along the Pacific Ring of Fire, a zone of volcanic activity that encompasses the Pacific rim of the Americas as well as the Asia-Pacific region. The Andes are the result of plate tectonics processes, caused by the subduction of oceanic crust beneath the South American plate. The main cause of the rise of the Andes is the compression of western rim of the South American Plate due to the subduction of the Nazca Plate and the Antarctic Plate. To the east, the Andes range is bounded by several sedimentary basins such as Orinoco, Amazon Basin, Madre de Dios and Gran Chaco which separates the Andes from the ancient cratons in eastern South America. In the south the Andes shares a long boundary with the former Patagonia Terrane. To the west the Andes ends at the Pacific Ocean, although the Peru-Chile trench can be considerated its ultimate western limit. From a geographical approach the Andes are considered to have their western boundaries marked by the appearance of coastal lowlands and a less rugged topography.

[edit] Orogeny

The western rim of the South American Plate has been the place of several pre-Andean orogenies since at least the of the late Proterozoic and early Paleozoic when several terranes and microcontinents collided and amalgamated with the ancient cratons of eastern South America, by then the South American part of Gondwana.
The formation of the modern Andes began with the events of the Triassic when Pangea begun to break up and several rifts developed. It continued through the Jurassic Period. It was during the Cretaceous Period that the Andes began to take its present form, by the uplifting, faulting and folding of sedimentary and metamorphic rocks of the ancient cratons to the east. The rise of the Andes has not been constant and different regions have had different degrees of tectonic stress, uplift, and erosion.
Tectonic forces above the subduction zone along the entire west coast of South America where the Nazca Plate and a part of the Antarctic Plate are sliding beneath the South American Plate continue to produce an ongoing orogenic event resulting in minor to major earthquakes and volcanic eruptions to this day. In the extreme south a major transform fault separates Tierra del Fuego from the small Scotia Plate. Across the 1,000 km (620 mi) wide Drake Passage lie the mountains of the Antarctic Peninsula south of the Scotia Plate which appear to be a continuation of the Andes chain.[citation needed]

[edit] Volcanism