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Home > Art, Film & Photography > Main Sequence Stars: Main Sequence, Wasp-16, Ads 16402, HR 4796, AA Tauri, Delta Doradus, V1094 Scorpii, V718 Persei, Nsvs 06507557, HD 93205
Main Sequence Stars: Main Sequence, Wasp-16, Ads 16402, HR 4796, AA Tauri, Delta Doradus, V1094 Scorpii, V718 Persei, Nsvs 06507557, HD 93205

Main Sequence Stars: Main Sequence, Wasp-16, Ads 16402, HR 4796, AA Tauri, Delta Doradus, V1094 Scorpii, V718 Persei, Nsvs 06507557, HD 93205


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Chapters: Main Sequence, Wasp-16, Ads 16402, Hr 4796, Aa Tauri, Delta Doradus, V1094 Scorpii, V718 Persei, Nsvs 06507557, Hd 93205, Hd 111031, Irs 8*. Source: Wikipedia. Pages: 47. Not illustrated. Free updates online. Purchase includes a free trial membership in the publisher's book club where you can select from more than a million books without charge. Excerpt: The main sequence is a continuous and distinctive band of stars that appear on plots of stellar color versus brightness. These color-magnitude plots are known as HertzsprungRussell diagrams after their co-developers, Ejnar Hertzsprung and Henry Norris Russell. Stars on this band are known as main-sequence stars or "dwarf" stars. After a star has formed, it creates energy at the hot, dense core region through the nuclear fusion of hydrogen atoms into helium. During this stage of the star's lifetime, it is located along the main sequence at a position determined primarily by its mass, but also based upon its chemical composition and other factors. All main sequence stars are in hydrostatic equilibrium, where outward thermal pressure from the hot core is balanced by the inward gravitational pressure from the overlying layers. The strong dependence of the rate of energy generation in the core on the temperature and pressure helps to sustain this balance. Energy generated at the core makes its way to the surface and is radiated away at the photosphere. The energy is carried by either radiation or convection, with the latter occurring in regions with steeper temperature gradients, higher opacity or both. The main sequence is sometimes divided into upper and lower parts, based on the dominant process that a star uses to generate energy. Stars below about 1.5 times the mass of the Sun (or 1.5 solar masses) primarily fuse hydrogen atoms together in a series of stages to form helium, a sequence called the proton-proton chain. Above this mass, in the upper main sequence, the n...More: http: //booksllc.net/?id=1960


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Product Details
  • ISBN-13: 9781157608684
  • Publisher: Books LLC
  • Publisher Imprint: Books LLC
  • Height: 152 mm
  • Sub Title: Main Sequence, Wasp-16, Ads 16402, HR 4796, AA Tauri, Delta Doradus, V1094 Scorpii, V718 Persei, Nsvs 06507557, HD 93205
  • Width: 229 mm
  • ISBN-10: 115760868X
  • Publisher Date: 15 Sep 2010
  • Binding: Paperback
  • Spine Width: 3 mm
  • Weight: 82 gr


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Main Sequence Stars: Main Sequence, Wasp-16, Ads 16402, HR 4796, AA Tauri, Delta Doradus, V1094 Scorpii, V718 Persei, Nsvs 06507557, HD 93205
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Main Sequence Stars: Main Sequence, Wasp-16, Ads 16402, HR 4796, AA Tauri, Delta Doradus, V1094 Scorpii, V718 Persei, Nsvs 06507557, HD 93205

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