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    Català: Aquesta gràfica mostra la taxa de generació d'energia nuclear (ε) per a una estrella de seqüència principal en funció de la temperatura (T). La corba verda mostra el cicle protó-protó, el blau és el cicle CNO i el vermell és el procés triple-alfa. La línia vertical marró representa la temperatura central del Sol, demostrant que la cadena P-P és la font principal de generació d'energia. La línia discontínua que uneix la corba P-P al cicle CNO representa la taxa neta de generació d'energia dels cicles combinats de combustió d'hidrogen nuclear. El pendent de les corbes mostra la sensibilitat més gran a la temperatura del cicle CNO i procés triple-alfa.
    English: This plot shows the rate of nuclear energy generation (ε) for a main sequence star as a function of temperature (T). The green curve shows the proton-proton cycle, blue is the CNO cycle and red is the triple-α process. The brown vertical line represents the core temperature of the Sun, demonstrating that the P-P chain is the primary source of energy generation. The dashed line joining the P-P curve to the CNO cycle represents the net energy generation rate of the combined nuclear hydrogen burning cycles. The slope of the curves shows the greater temperature sensitivity of the CNO cycle and triple-α process. It supports automatic language switch betwween en and any among de el fr it ja mk nl pt ru zh.
    Español: Este gráfico muestra la tasa de generación de energía nuclear (ε) para una estrella de secuencia principal en función de la temperatura (T). La curva verde muestra el ciclo protón-protón, el azul es el ciclo CNO y el rojo es el proceso triple-alfa. La línea vertical marrón representa la temperatura central del Sol, demostrando que la cadena P-P es la principal fuente de generación de energía. La línea discontinua que une la curva P-P al ciclo CNO representa la tasa neta de generación de energía de los ciclos combinados de combustión de hidrógeno nuclear. La pendiente de las curvas muestra la mayor sensibilidad a la temperatura del ciclo CNO y proceso triple-alfa.
    Italiano: Questo grafico mostra il tasso di generazione di energia nucleare (ε) per una stella della sequenza principale in funzione della temperatura (T). La linea verde rappresenta la catena protone-protone (PP), quella blu il ciclo carbonio-azoto-ossigeno (CNO), quella rossa il processo tre alfa (3-&alpha). La linea marrone indica la temperatura del nucleo del Sole evidenziando come sia la catena protone-protone la reazione prevalente. La linea tratteggiata che unisce la curva PP a quella CNO rappresenta il l'energia totale prodotat a quelle temperature dai vari processi. La pendenza delle linee evidenza come i processi CNO e 3-&alpha siano più sensibili alle variazioni di temperatura. Il grafico gestisce automaticamente la rappresentazione nelle seguenti lingue: en (default), de el fr it ja mk nl pt ru zh.
    Date
    Source Own work. See reference below.
    Author

    RJHall

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    Reference

    • After: Schwarzschild, Martin (1958) Structure and Evolution of the Stars (Dover edition (1965) ed.), Princeton University Press, pp. 82 ISBN: 0-486-61479-4.

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    Captions

    Stellar nucleosynthesis

    Items portrayed in this file

    depicts

    stellar nucleosynthesis

    inception

    5 December 2008

    media type

    image/svg+xml

    File history

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    Date/TimeThumbnailDimensionsUserComment
    current11:48, 25 August 2024Thumbnail for version as of 11:48, 25 August 2024642 × 525 (12 KB)Bjankuloski06Corrected Macedoinan word
    15:43, 3 July 2024Thumbnail for version as of 15:43, 3 July 2024642 × 525 (12 KB)Manlleusadded es and ca labels
    20:54, 7 March 2021Thumbnail for version as of 20:54, 7 March 2021642 × 525 (11 KB)YsogoChanged text-anchor to smoothly handle the different lenghts of word
    20:21, 7 March 2021Thumbnail for version as of 20:21, 7 March 2021642 × 525 (11 KB)YsogoAdded labels in de el fr ja mk nl pt ru zh
    08:27, 7 March 2021Thumbnail for version as of 08:27, 7 March 2021642 × 525 (8 KB)YsogoAdded language autoswitch English-Italian
    03:44, 6 December 2008Thumbnail for version as of 03:44, 6 December 2008642 × 525 (8 KB)RJHall{{Information |Description=Nucler energy generation versus temperature. |Source=self-made |Date= |Author= RJHall |Permission= |other_versions= }} Category:Astrophysics Category:Nuclear fusion

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