C-3PO and R2-D2 Pop! Vinyl Bobble-Head Figure Set by Funko – Star Wars

Bobble may refer to:

• Bobble, another name for stasis (fiction) in Vernor Vinge's Peace Authority science fiction series
• Bobble (knitting), a form of stitching in knitting
• Bobble (textile), small round pieces of fabric that form on natural fabrics through use
• Bobble hat, a knit beanie hat with a "bobble" (pom pom) at the top
• Bobblehead, a doll that moves or "bobbles" its head
• A hair tie, particularly in English

C, or c, is the third letter of the Latin alphabet, used in the modern English alphabet, the alphabets of other western European languages and others worldwide. Its name in English is cee (pronounced ), plural cees.

D2, D02, D.II, D II or D-2 may refer to:

Funko Inc. is an American company that manufactures licensed and limited pop culture collectibles, known for its licensed vinyl figurines and bobbleheads. In addition, the company produces licensed plush, action figures, apparel, accessories and games. Founded in 1998 by Mike Becker and Claudia Becker, Funko was originally conceived as a small project to create various low-tech, nostalgia-themed toys. The company's first manufactured bobblehead was of the Big Boy restaurant mascot.

First sold in 2005, Funko, Inc. is now headed by CEO Cynthia Williams. Since then, the company has increased the scope of its toy lines and signed licensing deals with major companies such as Warner Bros., Nickelodeon, MTV, NBCUniversal, Disney, Marvel Entertainment, and Major League Baseball.

A head is the part of an organism which usually includes the ears, brain, forehead, cheeks, chin, eyes, nose, and mouth, each of which aid in various sensory functions such as sight, hearing, smell, and taste. Some very simple animals may not have a head, but many bilaterally symmetric forms do, regardless of size.

Heads develop in animals by an evolutionary trend known as cephalization. In bilaterally symmetrical animals, nervous tissue concentrate at the anterior region, forming structures responsible for information processing. Through biological evolution, sense organs and feeding structures also concentrate into the anterior region; these collectively form the head.

A star is a luminous spheroid of plasma held together by self-gravity. The nearest star to Earth is the Sun. Many other stars are visible to the naked eye at night; their immense distances from Earth make them appear as fixed points of light. The most prominent stars have been categorised into constellations and asterisms, and many of the brightest stars have proper names. Astronomers have assembled star catalogues that identify the known stars and provide standardized stellar designations. The observable universe contains an estimated 10²² to 10²⁴ stars. Only about 4,000 of these stars are visible to the naked eye—all within the Milky Way galaxy.

A star's life begins with the gravitational collapse of a gaseous nebula of material largely comprising hydrogen, helium, and trace heavier elements. Its total mass mainly determines its evolution and eventual fate. A star shines for most of its active life due to the thermonuclear fusion of hydrogen into helium in its core. This process releases energy that traverses the star's interior and radiates into outer space. At the end of a star's lifetime as a fusor, its core becomes a stellar remnant: a white dwarf, a neutron star, or—if it is sufficiently massive—a black hole.

Stellar nucleosynthesis in stars or their remnants creates almost all naturally occurring chemical elements heavier than lithium. Stellar mass loss or supernova explosions return chemically enriched material to the interstellar medium. These elements are then recycled into new stars. Astronomers can determine stellar properties—including mass, age, metallicity (chemical composition), variability, distance, and motion through space—by carrying out observations of a star's apparent brightness, spectrum, and changes in its position in the sky over time.

Stars can form orbital systems with other astronomical objects, as in planetary systems and star systems with two or more stars. When two such stars orbit closely, their gravitational interaction can significantly impact their evolution. Stars can form part of a much larger gravitationally bound structure, such as a star cluster or a galaxy.