Into Darkness

Into Darkness may refer to:

See also

Star Trek

Star Trek is an American science fiction entertainment franchise created by Gene Roddenberry and owned by CBS (TV series) and Paramount Pictures (Film Rights).Star Trek: The Original Series and its live-action TV spin-off series, Star Trek: The Next Generation, Star Trek: Deep Space Nine, Star Trek: Voyager, and Star Trek: Enterprise as well as the Star Trek film franchise make up the main canon. The canonicity of Star Trek: The Animated Series is debated, and the expansive library of Star Trek novels and comics is generally considered non-canon, although still part of the franchise.

Star Trek Into Darkness

Star Trek Into Darkness is a 2013 American science fiction action film directed by J.J. Abrams and written by Roberto Orci, Alex Kurtzman and Damon Lindelof. It is the 12th installment in the Star Trek film franchise and sequel to the 2009 film Star Trek. The film features Chris Pine reprising his role as Captain James T. Kirk, with Zachary Quinto, Simon Pegg, Zoe Saldana, Karl Urban, John Cho, Anton Yelchin, Bruce Greenwood and Leonard Nimoy reprising their roles from the previous film. Benedict Cumberbatch, Peter Weller and Alice Eve are also credited in the film's principal cast. The film was the last time Nimoy would portray the character of Spock, and his final film appearance before his death in 2015.

Set in the 23rd century, Kirk and the crew of the USS Enterprise are sent to the Klingon homeworld seeking former Starfleet member-turned-terrorist John Harrison. After the release of Star Trek, Abrams, Burk, Lindelof, Kurtzman and Orci agreed to produce its sequel. Filming began in January 2012. Into Darkness's visual effects were primarily created by Industrial Light & Magic.

Darkness

Darkness, the polar opposite to brightness, is understood to be an absence of visible light. It is also the appearance of black in a colored space.

Humans are unable to distinguish color when either light or darkness predominate. In conditions of insufficient light, perception is achromatic and ultimately, black.

The emotional response to darkness has generated metaphorical usages of the term in many cultures.

Scientific

Perception

The perception of darkness differs from the mere absence of light due to the effects of after images on perception. In perceiving, the eye is active, and that part of the retina that is unstimulated produces a complementary afterimage.

Physics

In terms of physics, an object is said to be dark when it absorbs photons, causing it to appear dim compared to other objects. For example, a matte black paint does not reflect much visible light and appears dark, whereas white paint reflects much light and appears bright. For more information see color.

Light cannot be absorbed without limit. According to the principle of the conservation of Energy, energy cannot be created or destroyed; it can only be converted from one type to another. Consequently, most objects that absorb visible light reemit it as heat. So, although an object may appear dark, it is likely bright at a frequency that humans cannot perceive. For more information see thermodynamics.

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.