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  2. Red-giant branch - Wikipedia

    en.wikipedia.org/wiki/Red-giant_branch

    For stars with a degenerate helium core, there is a limit to this growth in size and luminosity, known as the tip of the red-giant branch, where the core reaches sufficient temperature to begin fusion. All stars that reach this point have an identical helium core mass of almost 0.5 M ☉, and very similar stellar luminosity and temperature ...

  3. Dengeki Bunko: Fighting Climax - Wikipedia

    en.wikipedia.org/wiki/Dengeki_Bunko:_Fighting_Climax

    An updated version of the game, titled Dengeki Bunko: Fighting Climax Ignition (電撃文庫 FIGHTING CLIMAX IGNITION, Dengeki Bunko Faitingu Kuraimakkusu Igunishion), was released in July 2015. [7] The update contains additional characters and more balanced gameplay.

  4. List of Sony Interactive Entertainment video games - Wikipedia

    en.wikipedia.org/wiki/List_of_Sony_Interactive...

    Wild Arms Alter Code: F: PlayStation 2: November 27, 2003: Media.Vision / Japan Studio: Japan only Gran Turismo 4 Prologue: PlayStation 2: December 4, 2003: Polyphony Digital: Ghosthunter: PlayStation 2: December 5, 2003: Guerrilla Cambridge: PAL only Gacharoku 2: Kondo wa Sekai Isshuu yo!! PlayStation 2: December 18, 2003: Agenda / Japan ...

  5. National Ignition Facility - Wikipedia

    en.wikipedia.org/wiki/National_Ignition_Facility

    The National Ignition Facility, located at Lawrence Livermore National Laboratory The target assembly for NIF's first integrated ignition experiment is mounted in the cryogenic target positioning system, or cryoTARPOS. The two triangle-shaped arms form a shroud around the cold target to protect it until they open five seconds before a shot.

  6. Helium flash - Wikipedia

    en.wikipedia.org/wiki/Helium_flash

    A helium flash is a very brief thermal runaway nuclear fusion of large quantities of helium into carbon through the triple-alpha process in the core of low-mass stars (between 0.8 solar masses (M ☉) and 2.0 M ☉ [1]) during their red giant phase. The Sun is predicted to experience a flash 1.2 billion years after it leaves the main sequence.

  7. Triple-alpha process - Wikipedia

    en.wikipedia.org/wiki/Triple-alpha_process

    As a side effect of the process, some carbon nuclei fuse with additional helium to produce a stable isotope of oxygen and energy: 12 6 C + 4 2 He → 16 8 O + γ (+7.162 MeV) Nuclear fusion reactions of helium with hydrogen produces lithium-5, which also is highly unstable, and decays back into smaller nuclei with a half-life of 3.7 × 10 −22 s.

  8. Hypergolic propellant - Wikipedia

    en.wikipedia.org/wiki/Hypergolic_propellant

    A gas, usually helium, is fed to the propellant tanks under pressure through a series of check and safety valves. The propellants in turn flow through control valves into the combustion chamber; there, their instant contact ignition prevents a mixture of unreacted propellants from accumulating and then igniting in a potentially catastrophic ...

  9. Liquid helium - Wikipedia

    en.wikipedia.org/wiki/Liquid_helium

    Liquid helium is a physical state of helium at very low temperatures at standard atmospheric pressures.Liquid helium may show superfluidity.. At standard pressure, the chemical element helium exists in a liquid form only at the extremely low temperature of −269 °C (−452.20 °F; 4.15 K).