Universe

The universe (Latinuniversus) is all of space and time[a] and their contents,[10] including planetsstarsgalaxies, and all other forms of matter and energy. While the spatial size of the entire universe is unknown,[3] it is possible to measure the size of the observable universe, which is currently estimated to be 93 billion light-years in diameter. In various multiverse hypotheses, a universe is one of many causally disconnected[11] constituent parts of a larger multiverse, which itself comprises all of space and time and its contents;[12] as a consequence, ‘the universe’ and ‘the multiverse’ are synonymous in such theories.UniverseThe Hubble Ultra-Deep Field image shows some of the most remote galaxies visible with present technology, each consisting of billions of stars. (Apparent image area about 1/79 that of a full moon)[1]Age (within Lambda-CDM model)13.799 ± 0.021 billion years[2]DiameterUnknown.[3] Diameter of the observable universe: 8.8×1026 m (28.5 Gpc or 93 Gly)[4]Mass (ordinary matter)At least 1053 kg[5]Average density (including the contribution from energy)9.9 x 10−30 g/cm3[6]Average temperature2.72548 K (-270.4 °C or -454.8 °F)[7]Main contentsOrdinary (baryonic)matter (4.9%)
Dark matter (26.8%)
Dark energy (68.3%)[8]ShapeFlat with a 0.4% margin of error[9]

The earliest cosmological models of the universe were developed by ancient Greek and Indian philosophers and were geocentric, placing Earth at the center.[13][14] Over the centuries, more precise astronomical observations led Nicolaus Copernicus to develop the heliocentric model with the Sun at the center of the Solar System. In developing the law of universal gravitationIsaac Newton built upon Copernicus’ work as well as Johannes Kepler‘s laws of planetary motion and observations by Tycho Brahe.

Further observational improvements led to the realization that the Sun is one of hundreds of billions of stars in the Milky Way, which is one of at least two trillion galaxies in the universe. Many of the stars in our galaxy have planetsAt the largest scale, galaxies are distributed uniformly and the same in all directions, meaning that the universe has neither an edge nor a center. At smaller scales, galaxies are distributed in clusters and superclusters which form immense filaments and voids in space, creating a vast foam-like structure.[15] Discoveries in the early 20th century have suggested that the universe had a beginning and that space has been expanding since then,[16] and is currently still expanding at an increasing rate.[17]

The Big Bang theory is the prevailing cosmological description of the development of the universe. According to estimation of this theory, space and time emerged together 13.799±0.021 billion years ago[2] and the energy and matter initially present have become less dense as the universe expanded. After an initial accelerated expansion called the inflationary epoch at around 10−32 seconds, and the separation of the four known fundamental forces, the universe gradually cooled and continued to expand, allowing the first subatomic particles and simple atoms to form. Dark matter gradually gathered, forming a foam-like structure of filaments and voids under the influence of gravity. Giant clouds of hydrogen and helium were gradually drawn to the places where dark matter was most dense, forming the first galaxies, stars, and everything else seen today. It is possible to see objects that are now further away than 13.799 billion light-years because space itself has expanded, and it is still expanding today. This means that objects which are now up to 46.5 billion light-years away can still be seen in their distant past, because in the past, when their light was emitted, they were much closer to Earth.

From studying the movement of galaxies, it has been discovered that the universe contains much more matter than is accounted for by visible objects; stars, galaxies, nebulas and interstellar gas. This unseen matter is known as dark matter[18] (dark means that there is a wide range of strong indirect evidence that it exists, but we have not yet detected it directly). The ΛCDM model is the most widely accepted model of our universe. It suggests that about 69.2%±1.2% [2015] of the mass and energy in the universe is a cosmological constant (or, in extensions to ΛCDM, other forms of dark energy, such as a scalar field) which is responsible for the current expansion of space, and about 25.8%±1.1% [2015] is dark matter.[19] Ordinary (‘baryonic‘) matter is therefore only 4.84%±0.1% [2015] of the physical universe.[19] Stars, planets, and visible gas clouds only form about 6% of ordinary matter, or about 0.29% of the entire universe.[20]

There are many competing hypotheses about the ultimate fate of the universe and about what, if anything, preceded the Big Bang, while other physicists and philosophers refuse to speculate, doubting that information about prior states will ever be accessible. Some physicists have suggested various multiverse hypotheses, in which our universe might be one among many universes that likewise exist.[3][21][22]

Definition

File:NASA-HubbleLegacyFieldZoomOut-20190502.webm

Play mediaHubble Space Telescope – Ultra deep field galaxies to Legacy field zoom out
(video 00:50; May 2, 2019)

The physical universe is defined as all of space and time[a] (collectively referred to as spacetime) and their contents.[10] Such contents comprise all of energy in its various forms, including electromagnetic radiation and matter, and therefore planets, moons, stars, galaxies, and the contents of intergalactic space.[23][24][25] The universe also includes the physical laws that influence energy and matter, such as conservation lawsclassical mechanics, and relativity.[26]

The universe is often defined as “the totality of existence”, or everything that exists, everything that has existed, and everything that will exist.[26] In fact, some philosophers and scientists support the inclusion of ideas and abstract concepts—such as mathematics and logic—in the definition of the universe.[28][29][30] The word universe may also refer to concepts such as the cosmosthe world, and nature.[31][32]

Universe

The universe (Latinuniversus) is all of space and time[a] and their contents,[10] including planetsstarsgalaxies, and all other forms of matter and energy. While the spatial size of the entire universe is unknown,[3] it is possible to measure the size of the observable universe, which is currently estimated to be 93 billion light-years in diameter. In various multiverse hypotheses, a universe is one of many causally disconnected[11] constituent parts of a larger multiverse, which itself comprises all of space and time and its contents;[12] as a consequence, ‘the universe’ and ‘the multiverse’ are synonymous in such theories.UniverseThe Hubble Ultra-Deep Field image shows some of the most remote galaxies visible with present technology, each consisting of billions of stars. (Apparent image area about 1/79 that of a full moon)[1]Age (within Lambda-CDM model)13.799 ± 0.021 billion years[2]DiameterUnknown.[3] Diameter of the observable universe: 8.8×1026 m (28.5 Gpc or 93 Gly)[4]Mass (ordinary matter)At least 1053 kg[5]Average density (including the contribution from energy)9.9 x 10−30 g/cm3[6]Average temperature2.72548 K (-270.4 °C or -454.8 °F)[7]Main contentsOrdinary (baryonic)matter (4.9%)
Dark matter (26.8%)
Dark energy (68.3%)[8]ShapeFlat with a 0.4% margin of error[9]

The earliest cosmological models of the universe were developed by ancient Greek and Indian philosophers and were geocentric, placing Earth at the center.[13][14] Over the centuries, more precise astronomical observations led Nicolaus Copernicus to develop the heliocentric model with the Sun at the center of the Solar System. In developing the law of universal gravitationIsaac Newton built upon Copernicus’ work as well as Johannes Kepler‘s laws of planetary motion and observations by Tycho Brahe.

Further observational improvements led to the realization that the Sun is one of hundreds of billions of stars in the Milky Way, which is one of at least two trillion galaxies in the universe. Many of the stars in our galaxy have planetsAt the largest scale, galaxies are distributed uniformly and the same in all directions, meaning that the universe has neither an edge nor a center. At smaller scales, galaxies are distributed in clusters and superclusters which form immense filaments and voids in space, creating a vast foam-like structure.[15] Discoveries in the early 20th century have suggested that the universe had a beginning and that space has been expanding since then,[16] and is currently still expanding at an increasing rate.[17]

The Big Bang theory is the prevailing cosmological description of the development of the universe. According to estimation of this theory, space and time emerged together 13.799±0.021 billion years ago[2] and the energy and matter initially present have become less dense as the universe expanded. After an initial accelerated expansion called the inflationary epoch at around 10−32 seconds, and the separation of the four known fundamental forces, the universe gradually cooled and continued to expand, allowing the first subatomic particles and simple atoms to form. Dark matter gradually gathered, forming a foam-like structure of filaments and voids under the influence of gravity. Giant clouds of hydrogen and helium were gradually drawn to the places where dark matter was most dense, forming the first galaxies, stars, and everything else seen today. It is possible to see objects that are now further away than 13.799 billion light-years because space itself has expanded, and it is still expanding today. This means that objects which are now up to 46.5 billion light-years away can still be seen in their distant past, because in the past, when their light was emitted, they were much closer to Earth.

From studying the movement of galaxies, it has been discovered that the universe contains much more matter than is accounted for by visible objects; stars, galaxies, nebulas and interstellar gas. This unseen matter is known as dark matter[18] (dark means that there is a wide range of strong indirect evidence that it exists, but we have not yet detected it directly). The ΛCDM model is the most widely accepted model of our universe. It suggests that about 69.2%±1.2% [2015] of the mass and energy in the universe is a cosmological constant (or, in extensions to ΛCDM, other forms of dark energy, such as a scalar field) which is responsible for the current expansion of space, and about 25.8%±1.1% [2015] is dark matter.[19] Ordinary (‘baryonic‘) matter is therefore only 4.84%±0.1% [2015] of the physical universe.[19] Stars, planets, and visible gas clouds only form about 6% of ordinary matter, or about 0.29% of the entire universe.[20]

There are many competing hypotheses about the ultimate fate of the universe and about what, if anything, preceded the Big Bang, while other physicists and philosophers refuse to speculate, doubting that information about prior states will ever be accessible. Some physicists have suggested various multiverse hypotheses, in which our universe might be one among many universes that likewise exist.[3][21][22]

Definition

File:NASA-HubbleLegacyFieldZoomOut-20190502.webm

Play mediaHubble Space Telescope – Ultra deep field galaxies to Legacy field zoom out
(video 00:50; May 2, 2019)

The physical universe is defined as all of space and time[a] (collectively referred to as spacetime) and their contents.[10] Such contents comprise all of energy in its various forms, including electromagnetic radiation and matter, and therefore planets, moons, stars, galaxies, and the contents of intergalactic space.[23][24][25] The universe also includes the physical laws that influence energy and matter, such as conservation lawsclassical mechanics, and relativity.[26]

The universe is often defined as “the totality of existence”, or everything that exists, everything that has existed, and everything that will exist.[26] In fact, some philosophers and scientists support the inclusion of ideas and abstract concepts—such as mathematics and logic—in the definition of the universe.[28][29][30] The word universe may also refer to concepts such as the cosmosthe world, and nature.[31][32]

GBA Games

The Game Boy Advance[a] (GBA) is a 32-bit handheld game console developed, manufactured and marketed by Nintendo as the successor to the Game Boy Color. It was released in Japan on March 21, 2001, in North America on June 11, 2001, in Australia and Europe on June 22, 2001, and in mainland China on June 8, 2004 as iQue Game Boy Advance. The GBA is part of the sixth generation of video game consoles. The original model does not have an illuminated screen; Nintendo addressed that with the release of a redesigned model with a frontlit screen, the Game Boy Advance SP, in 2003. A newer revision of the redesign was released in 2005, with a backlit screen. The final redesign, the Game Boy Micro, was released in 2005.Game Boy AdvanceThe indigo version of the original Game Boy AdvanceAlso known asiQue Game Boy Advance (China)DeveloperNintendo R&EManufacturerNintendoProduct familyGame Boy Advance familyTypeHandheld game consoleGenerationSixth generationRelease date

Lifespan2001–2010Introductory priceUS$99.99[4]Discontinued

  • JP: Q4 2006
  • NA: May 15, 2010
  • PAL: Q4 2008

Units sold81.51 million (as of June 30, 2010)[5]MediaGame Boy Advance Game PakCPUARM7TDMI @ 16.78 MHz, Sharp LR35902 (8080-derived) @ 8.388 or 4.194 MHzMemory32 KB internal, 256 KB external, 96 KB VRAMDisplayTFT LCD, 240×160 pixels, 40.8×61.2 mm[6]Power2 × AA batteriesDimensions82 x 144.5 x 24.5 mmBest-selling gamePokémon Ruby and Sapphire, 16 million units[7]Backward
compatibility
Game BoyGame Boy ColorPredecessorGame Boy Color[8]SuccessorNintendo DSRelated articlesGame Boy Advance SP

As of June 30, 2010, 81.51 million units of the Game Boy Advance series have been sold worldwide.[5] Its successor, the Nintendo DS, was released in November 2004[9] and is also compatible with Game Boy Advance software.

History

Hardware

GamesEdit

See also: List of Game Boy Advance games

Clockwise from left: A Game BoyGame Pak, a Game Boy Advance Game Pak, and a Nintendo DSGame Card. On the far right is a US nickel shown for scale.

With hardware performance comparable to the Super Nintendo Entertainment System, the Game Boy Advance represents progress for sprite-based technology. The system’s library includes platformers, SNES-like role-playing video games, and games ported from various 8-bit and 16-bit systems of the previous generations. This includes the Super Mario Advance series, as well as the system’s backward compatibility with all earlier Game Boy titles. While most GBA games employ 2D graphics, developers have ambitiously designed some 3D GBA games that push the limits of the hardware, including first-person shooters like a port of Doom and racing games like GT Advance Championship Racing.

In Japan, the final game to have been released on the system is Final Fantasy VI Advance on November 30, 2006, which is also the final game published by Nintendo on the system.[36] In North America, the last game for the system is Samurai Deeper Kyo, released on February 12, 2008. Lastly, in Europe, 2 Games in 1: Columns Crown & ChuChu Rocket! is the last game for the system (and also the last one released on the system overall), released on November 28, 2008. The Japan-only Rhythm Tengoku, the first game in what would eventually become known outside Japan as the Rhythm Heaven/Rhythm Paradise series, is the final first-party-developed game for the system, released on August 3, 2006.

Compatibility with other systemsEdit

An accessory for the GameCube, known as the Game Boy Player, was released in 2003 as the successor to the Super Game Boy peripheral for the Super Nintendo Entertainment System. The accessory allows Game Boy Advance games, as well as Game Boy and Game Boy Color games, to be played on the GameCube. However, some games may have compatibility issues due to certain features requiring extra hardware. For example, games with built-in motion sensors (such as Yoshi’s Topsy-Turvy) would require players to manipulate the console itself.

The GBA is the last of the three Nintendo handheld systems to bear the Game Boy name, games developed for it are incompatible with older Game Boy systems, and each game’s box carries a label indicating that the game is “not compatible with other Game Boy systems”. However, games designed for older Game Boy systems are conversely compatible with the Game Boy Advance, with options to play such games on either their standard aspect ratios or a stretched fullscreen.

Game Boy Advance games are compatible with Nintendo DS models that support them with a dedicated GBA cartridge slot beneath the touch screen, (specifically the original model and the Nintendo DS Lite), although they cannot support multiplayer or features involving the use of GBA accessories because they do not have the GBA’s external peripheral port that these features require to function. The Nintendo DSi and Nintendo DSi XL do not have backward compatibility with the GBA.

Virtual ConsoleEdit

See also: Virtual Console

As part of an Ambassador Program for early adopters of the Nintendo 3DS system, ten Game Boy Advance games were made available free for players who bought a system before August 2011.[37] Unlike other Virtual Console games for the system, features such as the Home menu or save states are missing, since the games are running natively instead of in emulation. 3DS systems that have custom firmware installed can also install the ten available games available to Ambassador Program members. Many other Game Boy Advance games can also be played via custom firmware by injecting a different game into one of the released Game Boy Advance games.[citation needed] Satoru Iwata stated Game Boy Advance games will be available on the Wii U Virtual Console sometime during April 2014.[38] On April 3, 2014, the first of the announced GBA games, Advance WarsMetroid Fusion, and Mario & Luigi: Superstar Saga, were released for the Wii U Virtual Console.[39] A Virtual Console library of Game Boy Advance games was launched for the Wii U console. All of the Virtual Console releases are single player only, as they do not emulate multiplayer features enabled by Game Link cables.

Pokemon emerald link – https://www-pokemoner-com.cdn.ampproject.org/v/s/www.pokemoner.com/2015/04/pokemon-emerald.html/amp?usqp=mq331AQRKAGYAeb2j-W1p4TEtgGwASA%3D&amp_js_v=a6&amp_gsa=1

Breakfast at my House

During the week we’re often walking out the door with a coffee in one hand and slice of toast in the other, but on weekends breakfast is never rushed. It’s a late affair, sometimes spilling over to lunch, with lots of reading and chatter in between courses of fruits, poached eggs, honey and toast. One of our favorite things we like to serve when friends are visiting are buckwheat blueberry pancakes.