Hitchcock Haunts a Nebula

Article written: 1 Feb , 2012
Updated: 24 Dec , 2015
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First impression after seeing this new image of NGC 3324? It’s Alfred Hitchcock, bulbous nose and all (see image below for comparison). The right edge of the wall of gas and dust in this star-forming region really bears a strong resemblance to the famous profile of the British film director and producer, notorious for his thriller movies from the 1940’s through the 1970’s.

NGC 3324 is located in the southern constellation of Carina, roughly 7500 light-years from Earth. It is on the northern outskirts of the chaotic environment of the Carina Nebula. All the gas and dust here fueled a burst of star birth several millions of years ago and led to the creation of several hefty and very hot stars that are prominent in the new picture.

Alfred Hitchcock. Via iwatchstuff.com

A nickname for the NGC 3324 region is the ‘Gabriela Mistral Nebula,’ after the Nobel Prize-winning Chilean poet but I think I’ll start a petition to call it the Hitchcock Nebula. Hitchcock liked to make cameo appearances in his own movies, and perhaps he is making a pareidoliaic guest appearance here.

The new image of NGC 3324 was taken with the Wide Field Imager on the the European Southern Observatory’s 2.2-metre telescope at the La Silla Observatory in Chile. Read more about it on the ESO website.

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4 Responses

  1. Edward Morbius says

    I’ll sign your petition. It definitely looks like Hitchcock’s profile. For Miss Mistral’s sake I sure hope it wasn’t named after her because it looks like her.

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  3. Anonymous says

    Alfred Hitchcock was such an Icon of weird that I am surprised after the publication of this view, anyone would object to the naming of this nebula for him. Now for the Music from the Show! Too droll! 🙂

    you have my vote

  4. Nirmalendu Das says

    NGC 3324 is located in the southern constellation of Carina, roughly 7500 light-years from Earth.
    I calculate the distance of it as 6.52169×10^21 cm, where 7500 light years = 7.09537×10^21 cm.

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