Jeffree Star

Jeffree Star (born Jeffrey Lynn Steininger on November 15, 1985) is an American singer-songwriter, make-up artist, fashion designer and model from Orange County, California. He started his music career on MySpace with over 25 million plays on his self-released music. After releasing two extended plays, Star released his debut album, Beauty Killer (2009), under Popsicle Records. In 2014, he launched his own cosmetics brand called Jeffree Star Cosmetics. Star is also known for his fashion line, Beauty Forever, and transgressive, gender-bending appearance and persona.

Early life

Jeffree Star was born in Los Angeles County, California. His father died when Star was 6 years old; subsequently he was raised solely by his mother, a model who frequently went on assignments. As a child, Star regularly began experimenting with his mother's makeup and convinced her to let him wear it to school when he was in junior high. He moved to Los Angeles following his graduation from high school, supporting himself with various makeup, modeling, and music jobs. He later recalled spending his time on weekends "using a fake ID to attend Hollywood clubs dressed in mini dresses and nine inch high heels where celebrities would contract [Star] for makeup work at their homes", or "hiring [Star] as a model." Star reports that his weekend socializing at clubs and the makeup advice he offered eventually led to his modeling career.

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.