△: Sixsterne86

Udah lama ga nge-post mwehehehe. Ok kali ini gue bakal nge-post tentang ~~abegeabege labil jaman sekarang~~ nama baru DELAPAN ENAM.

Jadiiiiiii, asal lo-lo-lo-lo dan lo semua tau sebenernya nama kelas gue tadinya itu Octavo-Grado-Seis atau Ocho-Seis. Tapii, karena ~~ada kepengurusan admin baru~~ nama itu udah biasa dan kalo ga salah udah dipake sama 8-6 tahun lalu jadi nama itu diganti jadi SIXSTERNE86.

Asshole. sebenernya gue gatau sih ini artinya apaan tapi setau gue dari wawancara ke sang pembuat dan penemu ini nama a.k.a Nabila Sarah Pradila yang bisa ditemuin di tuiter dengan username @nablsp, katanya arti dari 'sterne' itu adalah STAR dan bagi yang gatau star itu apaan bisa cari di gugel translet aja atau mau gue kasi tau disini nih? STAR itu adalah....

A star is a massive, luminous sphere of plasma held together by gravity. At the end of its lifetime, a star can also contain a proportion of degenerate matter. The nearest star to Earth is the Sun, which is the source of most of the energy on Earth. Other stars are visible from Earth during the night, when they are not obscured by atmospheric phenomena, appearing as a multitude of fixed luminous points because of their immense distance. Historically, the most prominent stars on the celestial sphere were grouped together into constellations and asterisms, and the brightest stars gained proper names. Extensive catalogues of starshave 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 in its core releasing energy that traverses the star's interior and then radiates into outer space. Almost all naturally occurring elements heavier than helium were created by stars, either via stellar nucleosynthesis during their lifetimes or by supernova nucleosynthesis when stars explode. Astronomerscan determine the mass, age, chemical composition and many other properties of a star by observing its spectrum, luminosity and motion through space. The total mass of a star is the principal determinant in its evolution and eventual fate. Other characteristics of a star are determined by its evolutionary history, including diameter, rotation, movement and temperature. 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.

A star begins as a collapsing cloud of material composed primarily of hydrogen, along with helium and trace amounts of heavier elements. Once the stellar core is sufficiently dense, some of the hydrogen is steadily converted into helium through the process of nuclear fusion. The remainder of the star's interior carries energy away from the core through a combination of radiative and convective processes. The star's internal pressure prevents it from collapsing further under its own gravity. Once the hydrogen fuel at the core is exhausted, a star with at least 0.4 times the mass of the Sun expands to become a red giant, in some cases fusing heavier elements at the core or in shells around the core. The star then evolves into a degenerate form, recycling a portion of the matter into the interstellar environment, where it will form a new generation of stars with a higher proportion of heavy elements.

Binary and multi-star systems consist of two or more stars that are gravitationally bound, and generally move around each other in stable orbits. When two such stars have a relatively close orbit, their gravitational interaction can have a significant impact on their evolution. Stars can form part of a much larger gravitationally bound structure, such as a cluster or agalaxy.

Okeh itu artikel gue dapetin dari Wikipedia dan langsung gue copas gapake ngedit so, kalo ada yang tulisan warnanye biru2 begitu itu mah darisononye soalnya ga gue edit. Bagi elo-elo yang ga ngarti itu apaan bisa translate di gugel atau dimane serah lo dah. Dan buat elo-elo yang ga ngerti cara translate atau ga tau google itu apa... kelaut aje daaahhhhh.