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“It’s estimated that 95 percent of the livable space on our planet is in the ocean, yet only a fraction of that space has been explored,” said study lead author Carole Baldwin of the NMNH. Endangered Waves can empower and incentivize surfers (there are 24 million worldwide) to monitor the health of their coastlines through crowdsourced data. Surfers can use this app to create crowdsourced data to identify and then reduce hazards in their local surf breaks. In the US, tourism and recreation comprise 72% of employment in the ocean economy and 31% of its gross value. Creating apps that cater to this market isn’t indulgent, it’s good business sense. Supercritical fluids, although not liquids, do share various properties with liquids. Underneath the thick atmospheres of the planets Uranus and Neptune, it is expected that these planets are composed of oceans of hot high-density fluid mixtures of water, ammonia and other volatiles.[86] The gaseous outer layers of Jupiter and Saturn transition smoothly into oceans of supercritical hydrogen.[87][88] The atmosphere of Venus is 96.5% carbon dioxide, which is a supercritical fluid at its surface. Plastic is everywhere – even the deepest parts of the ocean are now awash with it. The motions of the ocean surface, known as undulations or waves, are the partial and alternate rising and falling of the ocean surface. The series of mechanical waves that propagate along the interface between water and air is called swell.[citation needed] The goal of the Big Ocean Button Challenge is to advance development of and investment in ocean data products and services. Many sectors can benefit from solutions for organizing and standardizing ocean data. Some applications that are in need of ocean services include: Ta rozmowa jest jak życie, raz płynie jak wartka rzeka, innym razem powolutku – delikatnie zaczepiając o problematyczne skałki a czasem zupełnie jak wzburzony ocean. Jestem naprawdę zauroczona osobowością, pozytywnym nastawieniem i otwartością Pani Julii 🙂 Fantastyczna książka. Gorąco polecam! W skład oceanów (układów oceanicznych) wchodzą także mniejsze obszary wodne, jak: morza, zatoki, kanały, zalewy i cieśniny, które od pełnych wód oceanicznych mogą być oddzielone półwyspami, wyspami bądź archipelagami. Wszystkie te zasoby wodne Ziemi określa się łącznie mianem wszechoceanu. The benthic zones are aphotic and correspond to the three deepest zones of the deep-sea. The bathyal zone covers the continental slope down to about 4,000 meters (13,000 ft). The abyssal zone covers the abyssal plains between 4,000 and 6,000 m. Lastly, the hadal zone corresponds to the hadalpelagic zone, which is found in oceanic trenches. Large bodies of liquid hydrocarbons are thought to be present on the surface of Titan, although they are not large enough to be considered oceans and are sometimes referred to as lakes or seas. The Cassini–Huygens space mission initially discovered only what appeared to be dry lakebeds and empty river channels, suggesting that Titan had lost what surface liquids it might have had. Cassini’s more recent fly-by of Titan offers radar images that strongly suggest hydrocarbon lakes exist near the colder polar regions. Titan is thought to have a subsurface liquid-water ocean under the ice and hydrocarbon mix that forms its outer crust. Oceanographers divide the ocean into different vertical zones defined by physical and biological conditions. The pelagic zone includes all open ocean regions, and can be divided into further regions categorized by depth and light abundance. The photic zone includes the oceans from the surface to a depth of 200 m; it is the region where photosynthesis can occur and is, therefore, the most biodiverse. Because plants require photosynthesis, life found deeper than the photic zone must either rely on material sinking from above (see marine snow) or find another energy source. Hydrothermal vents are the primary source of energy in what is known as the aphotic zone (depths exceeding 200 m). The pelagic part of the photic zone is known as the epipelagic. Sarah Cooley, a marine scientist at the Ocean Conservancy, explains the environmental group’s strategy for reaching out to both sides of the aisle on legislation to address ocean challenges in a divisive political environment.20 days ago Ocean’s design is influenced by its coastal setting. Blues, whites and beiges create a modern classic look, while delightful hand-crafted furniture and specially commissioned artwork emphasise the feeling of luxury. White American shutters frame stunning views over the gardens to the ocean beyond. +44 (0)20 7292 6161 info@oceanoutdoor.com Terms & Conditions The deepest point in the ocean is the Mariana Trench, located in the Pacific Ocean near the Northern Mariana Islands. Its maximum depth has been estimated to be 10,971 meters (35,994 ft) (plus or minus 11 meters; see the Mariana Trench article for discussion of the various estimates of the maximum depth.) The British naval vessel Challenger II surveyed the trench in 1951 and named the deepest part of the trench the “Challenger Deep”. In 1960, the Trieste successfully reached the bottom of the trench, manned by a crew of two men. Please reach out to UNESCO’s IOC via oceandecade@unesco.org Exploring the extreme environment of the deep sea requires special technology. Enter a research habitat based on real ocean laboratories. Climb into an actual submarine, learn how sonar works, and “fly” a remote operated vehicle (ROV) as you explore the wonders of the undersea world. Nautilus Minerals forecasts that in copper alone an emerging undersea industry in oceans around the world could be worth $30bn a year by 2030. And it claims that by mining a small area of seabed, the venture will be friendlier to the environment. It contrasts its work with mines on land where trees and topsoil are swept away across vast areas. Pośród odkrytych planet pozasłonecznych znajdują się ciała krążące w obrębie tzw. ekosfery, czyli w obszarze wokół gwiazdy, w którym takie zbiorniki mogą istnieć. Współczesne modele powstawania planet wskazują na możliwość istnienia planet oceanicznych, pokrytych całkowicie wodami oceanu. Na niektórych ciałach położonych poza klasycznie definiowaną ekosferą mogą istnieć podpowierzchniowe zbiorniki ciekłej wody. Niektóre z nich tworzą płynną warstwę wody otaczającą cały glob, pokrytą skorupą lodową o wielokilometrowej grubości. Taki podpowierzchniowy ocean posiadają niektóre księżyce planet, w szczególności Europa, a także prawdopodobnie Ganimedes i Kallisto, dwa inne galileuszowe księżyce Jowisza oraz Tytan i Enceladus, krążące wokół Saturna[6]. Ocean na Europie przypuszczalnie ma kontakt ze skalistym wnętrzem księżyca i na jego dnie może mieć miejsce aktywność wulkaniczna lub hydrotermalna; także ocean na Enceladusie rozciąga się między lodową skorupą a skałami[7]. Prawdopodobne oceany na trzech największych księżycach lodowych są uwięzione pomiędzy dwiema warstwami lodu o różnej strukturze krystalicznej i gęstości[8]. Modele ewolucji termicznej wskazują także na możliwość powstania takich zbiorników na niektórych większych obiektach transneptunowych[9] (plutoidach). For the time being, SoFi is remote-controlled. But the idea is that future versions would use machine vision to lock onto individual fish and follow them around, all without raising suspicion. That could help scientists study schooling dynamics, or monitor the health of fish populations in increasingly unhealthy oceans. “It could help us with the problems of fish avoidance and fish attraction that are associated with other forms of monitoring with robots and divers,” says Northeastern’s Hanumant Singh, who develops autonomous underwater vehicles but was not involved in the research. Scientists have just defined the newly named rariphotic zone, a layer of ocean between depths of 130 and 300 metres (400 and 1,000 feet) – a low-light or “twilight zone” in deeper reef regions. Extraterrestrial oceans may be composed of water or other elements and compounds. The only confirmed large stable bodies of extraterrestrial surface liquids are the lakes of Titan, although there is evidence for the existence of oceans elsewhere in the Solar System. Early in their geologic histories, Mars and Venus are theorized to have had large water oceans. The Mars ocean hypothesis suggests that nearly a third of the surface of Mars was once covered by water, and a runaway greenhouse effect may have boiled away the global ocean of Venus. Compounds such as salts and ammonia dissolved in water lower its freezing point so that water might exist in large quantities in extraterrestrial environments as brine or convecting ice. Unconfirmed oceans are speculated beneath the surface of many dwarf planets and natural satellites; notably, the ocean of Europa is estimated to have over twice the water volume of Earth. The Solar System’s giant planets are also thought to have liquid atmospheric layers of yet to be confirmed compositions. Oceans may also exist on exoplanets and exomoons, including surface oceans of liquid water within a circumstellar habitable zone. 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