hertzsprung–russell diagram wikipedia - EAS

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    https://en.wikipedia.org/wiki/Hertzsprung–Russell_diagram

    The Hertzsprung–Russell diagram, abbreviated as H–R diagram, HR diagram or HRD, is a scatter plot of stars showing the relationship between the stars' absolute magnitudes or luminosities versus their stellar classifications or effective temperatures. The diagram was created … See more

    In the nineteenth century large-scale photographic spectroscopic surveys of stars were performed at Harvard College Observatory, producing spectral classifications for tens of thousands of stars, culminating … See more

    There are several forms of the Hertzsprung–Russell diagram, and the nomenclature is not very well defined. All forms share the same general layout: stars of greater luminosity … See more

    Contemplation of the diagram led astronomers to speculate that it might demonstrate stellar evolution, the main suggestion being that stars collapsed from red giants to dwarf stars, then moving down along the line of the main sequence in the course of … See more

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    Interpretation image

    Most of the stars occupy the region in the diagram along the line called the main sequence. During the stage of their lives in which stars are found on the main sequence line, they … See more

    Asymptotic giant branch – Stars powered by fusion of hydrogen and helium in shell with an inactive core of carbon and oxygen
    Galaxy color–magnitude diagram – Chart depicting the … See more

    Omega Cen H-R animation of a Hertzsprung–Russell diagram created from real Hubble data
    JavaHRD an interactive Hertzsprung–Russell diagram as a Java applet See more

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  2. https://simple.wikipedia.org/wiki/Hertzsprung–Russell_diagram

    The Hertzsprung-Russell diagram is a graph of many stars. It shows the relation between stars' luminosity (how bright they are) and their temperature (how hot they are). These diagrams are …

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      When was the Hertzsprung–Russell diagram developed?In 1911 Hertzsprung developed the Hertzsprung–Russell diagram, independently developed in 1913 by Henry Norris Russell . In 1913 Hertzsprung determined the distances to several Cepheid variable stars by parallax, [3] and was thus able to calibrate the relationship, discovered by Henrietta Leavitt, between Cepheid period and luminosity.
      en.wikipedia.org/wiki/Ejnar_Hertzsprung
      What do All Stars in a Hertzsprung Russell diagram have in common?All stars in a given area of a Hertzsprung-Russell diagram share similar luminosities and temperatures. The main region where stars appear is the diagonal curved line, going from the upper-left (hot and bright) to the lower-right (cooler and less bright). This is called the Main Sequence.
      simple.wikipedia.org/wiki/Hertzsprung%E2%80%93Russell…
      What does the vertical axis of a Hertzsprung-Russell diagram show?The vertical axis of a Hertzsprung-Russell diagram shows the luminosity or brightness of the stars, as if they were all measured from the same distance. Another term for this is absolute magnitude.
      simple.wikipedia.org/wiki/Hertzsprung%E2%80%93Russell…
      What did Ejnar Hertzsprung do?Ejnar Hertzsprung (Danish: [ˈɑjnɐ ˈhɛɐ̯tsˌpʁɔŋ]; 8 October 1873 – 21 October 1967) was a Danish chemist and astronomer born in Copenhagen. In the period 1911–1913, together with Henry Norris Russell, he developed the Hertzsprung–Russell diagram.
      en.wikipedia.org/wiki/Ejnar_Hertzsprung
    • https://de.wikipedia.org/wiki/Hertzsprung-Russell-Diagramm

      Das Hertzsprung-Russell-Diagramm, kurz HRD, zeigt grob die Entwicklungsverteilung der Sterne. Es wurde 1913 von Henry Norris Russell entwickelt und baut auf Arbeiten von Ejnar Hertzsprung auf. Wird dazu der Spektraltyp gegen die absolute Helligkeit aufgetragen, ergeben sich bei einer genügenden Anzahl von Eintragungen charakteristische linienartige Häufungen.

      • Estimated Reading Time: 3 mins
      • https://hu.wikipedia.org/wiki/Hertzsprung–Russell-diagram
        Image
        Vízszintes tengelyre a csillagok felszíni hőmérsékletét, az úgynevezett színindexet(BV), vagy a színképosztályt viszik fel, a forró kék csillagoktól a hideg vörösekig, balról jobbra. A függőleges tengelyen a csillagok fényességét tüntetik fel valamely mértékegység szerint, például abszolút fényességet vagy a …
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        • Published: May 03, 2022
      • https://sv.wikipedia.org/wiki/Hertzsprung–Russell-diagram
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        Strax efter stjärnbildningen följer en protostjärna det nästan vertikala så kallade Hayashispåretlängst till höger i diagrammet (ej i bild). Diagonalt i diagrammet från hög ljusstyrka och hög temperatur till låg ljusstyrka och låg temperatur sträcker sig huvudserien. Den representerar de stjärnor som omvandl…
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        • https://cs.wikipedia.org/wiki/Hertzsprungův–Russellův_diagram

          HR diagram Hertzsprungův–Russellův diagram vyjadřuje závislost povrchové teploty ( spektrální typ) hvězd na jejích svítivosti ( zářivý výkon) nebo absolutní magnitudě v různých fázích …

        • https://da.wikipedia.org/wiki/Hertzsprung-Russell-diagrammet

          et hertzsprung-russell-diagram (ofte forkortet til hr-diagram eller hrd) er et koordinatsystem , hvori alle stjerner kan indplaceres på grundlag af to af deres egenskaber, der kan observeres …

        • https://en.wikipedia.org/wiki/Hertzsprung_gap

          The Hertzsprung Gap is a feature of the Hertzsprung–Russell diagram for a star cluster. It is named after Ejnar Hertzsprung , who first noticed the absence of stars in the region of the

        • https://en.wikipedia.org/wiki/Ejnar_Hertzsprung

          In 1911 Hertzsprung developed the Hertzsprung–Russell diagram, independently developed in 1913 by Henry Norris Russell. In 1913 Hertzsprung determined the distances to several …

        • https://en.wikipedia.org/wiki/Stellar_classification

          The Hertzsprung–Russell diagram, which the MK system is based on, is observational in nature so these remnants cannot easily be plotted on the diagram, or cannot be placed at all. Old neutron stars are relatively small and …



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