Star Fox (video game)

Star Fox (スターフォックス, Sutā Fokkusu), released as Starwing in Europe (to avoid confusion with an association named "StarVox" in Germany), is the first game in the Star Fox series of video games, released on February 21, 1993 in Japan, on March 26, 1993 in North America, and on June 3, 1993 in Europe for the Super Famicom/Super Nintendo Entertainment System.

It was the second three-dimensional Nintendo-developed game (behind 1992's X, also developed by Nintendo EAD together with Argonaut Software) but it is Nintendo's first game to use 3D polygon graphics. It accomplished this by being the first ever game to use the Super FX graphics acceleration coprocessor powered GSU-1. The complex display of three-dimensional models with polygons was still new and uncommon in console video games, and the game was much-hyped as a result.

Star Fox featured arcade rail shooting and obstacle course style gameplay by Shigeru Miyamoto, anthropomorphic character designs by Nintendo artist Takaya Imamura, then music composed by Hajime Hirasawa. Star Fox was developed by Nintendo EAD with assistance by Argonaut Software, and was published by Nintendo. The game was a critical and commercial success, which established Star Fox as one of Nintendo's flagship franchises.

Star Fox

Star Fox may refer to:

Super Smash Bros.

Super Smash Bros., known in Japan as Dairantō Smash Brothers (Japanese: 大乱闘スマッシュブラザーズ, Hepburn: Dairantō Sumasshu Burazāzu, lit. "Great Melee Smash Brothers"), is a series of crossover fighting games published by Nintendo, that primarily featuring characters from franchises established on its systems. All five games have been directed by Masahiro Sakurai.

The gameplay objective differs from that of traditional fighters by aiming to knock opponents out of the stage instead of depleting life bars. The original Super Smash Bros., released in 1999 for the Nintendo 64, had a small budget and was originally a Japan-only release, but its domestic success led to a worldwide release. The series achieved even greater success with the release of Super Smash Bros. Melee, which was released in 2001 for the GameCube and became the best-selling game on that system. A third installment, Super Smash Bros. Brawl, was released in 2008 for the Wii. Although HAL Laboratory has been the developer of the first two titles, the third game was developed through the collaboration of several companies. The fourth and fifth installments,Super Smash Bros. for Nintendo 3DS and Wii U, were released in 2014 for the Nintendo 3DS and Wii U, respectively. The 3DS installment was the first series title to be released on a handheld platform.

Super Smash Bros. Brawl

Super Smash Bros. Brawl, known in Japan as Dairantō Smash Brothers X (大乱闘(だいらんとう)スマッシュブラザーズX(エックス)^?, lit. "Great Melee Smash Brothers X") , is the third installment in the Super Smash Bros. series of crossover fighting games, developed by an ad hoc development team consisting of Sora, Game Arts, and staff from other developers, and published by Nintendo for the Wii video game console.Brawl was announced at a pre-E3 2005 press conference by Nintendo president and Chief Executive Officer Satoru Iwata.Masahiro Sakurai, director of the previous two games in the series, assumed the role of director for the third installment at the request of Iwata. Game development began in October 2005 with a creative team that included members from several Nintendo and third-party development teams. After delays due to development problems, the game was finally released on January 31, 2008, in Japan; March 9, 2008, in North America; June 26, 2008, in Australia; and June 27, 2008, in Europe. Twenty-seven months after its original Japanese release, the game was released in Korea, on April 29, 2010.

Star

A star is a luminous sphere of plasma held together by its own gravity. The nearest star to Earth is the Sun. Other stars are visible to the naked eye from Earth during the night, appearing as a multitude of fixed luminous points in the sky due to their immense distance from Earth. Historically, the most prominent stars were grouped into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of stars have been assembled by astronomers, which provide standardized star designations.

For at least a portion of its life, a star shines due to thermonuclear fusion of hydrogen into helium in its core, releasing energy that traverses the star's interior and then radiates into outer space. Once the hydrogen in the core of a star is nearly exhausted, almost all naturally occurring elements heavier than helium are created by stellar nucleosynthesis during the star's lifetime and, for some stars, by supernova nucleosynthesis when it explodes. Near the end of its life, a star can also contain degenerate matter. Astronomers can determine the mass, age, metallicity (chemical composition), and many other properties of a star by observing its motion through space, luminosity, and spectrum respectively. The total mass of a star is the principal determinant of its evolution and eventual fate. Other characteristics of a star, including diameter and temperature, change over its life, while the star's environment affects its rotation and movement. A plot of the temperature of many stars against their luminosities, known as a Hertzsprung–Russell diagram (H–R diagram), allows the age and evolutionary state of a star to be determined.