M42 und Running Man-Nebel (Giovanni)

Celestial hemisphere: Southern · Constellation: Orion (Ori) · Contains: Great Orion Nebula · Lower Sword · M 42 · M 43 · Mairan's Nebula · NGC 1973 · NGC 1975 · NGC 1976 · NGC 1977 · NGC 1980 · NGC 1981 · NGC 1982 · Orion Nebula · The star 42Ori · The star 45Ori · The star θ1Ori · The star θ2Ori · The star ιOri · Upper Sword · the Running Man Nebula

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M42 und Running Man-Nebel

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M42 und Running Man-Nebel

M42 and Running Man-Nebula

Der Orionnebel (Katalogbezeichnung M 42 oder NGC 1976) ist ein Emissionsnebel im Sternbild Orion. Durch die relativ große scheinbare Helligkeit von rund 4 mag ist der Nebel mit bloßem Auge als Teil des Schwertes des Orion unter den drei Sternen des Oriongürtels sichtbar.[2]

Der überwiegend aus Wasserstoff bestehende Orionnebel entwickelte sich aus Teilen einer interstellaren Molekülwolke. Aufgrund der ionisierenden Strahlung darin entstehender junger Sterne, insbesondere des Trapeziums, leuchtet der Nebel im sichtbaren Bereich und wird daher auch als H-II-Gebiet klassifiziert.[3] Etwa 414 Parsec[4] (1350 Lichtjahre) entfernt, ist er eines der aktivsten Sternentstehungsgebiete in der galaktischen Nachbarschaft der Sonne.

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Imagers of Italy

Messier

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M42 und Running Man-Nebel

M42 und Running Man-Nebel

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M42 und Running Man-Nebel

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