Starship Asterisk*

[quote=" https://en.wikipedia.org/wiki/Nebulae_in_fiction#Horsehead_Nebula"]

[b]The Stars, Like Dust[/b] (1951) by Isaac Asimov: Asimov conducts a clinic on geocentrism in a galactic setting, having a character state that the literal adjective "horsehead" is meaningless from non-terrestrial vantages, and that the "generally believed" alternate derivation (that the nebula was first breached by the eponymous explorer Horace Hedd) is far more plausible.

[b]The Hitchhiker's Guide to the Galaxy[/b] (1979) by Douglas Adams: Galactic President Zaphod Beeblebrox and his companion Trillian have stolen the Infinite Improbability Drive prototype ship Heart of Gold. Reaching the Horsehead Nebula, and recognizing their location by the sheer impenetrable darkness outside, they discover the ancient planet Magrathea and its twin suns Soulianis and Rahm. Magrathea is a world whose economy was based on the manufacturing of bespoke planets for the wealthiest people in the universe, back in the days of the Galactic Empire (it was Magrathea that created the Earth).[/quote]

I SEE THE GRINCH!!! In red, on the back of the horses head... Maybe a little too much egg nog this weekend... Sorry if I alarmed anyone...

Know what? With this new close up of the Horsehead Nebula, with the shape of the snout, it looks more like a moose head than a horse. Should we start a petition to rename it the Bullwinklehead Nebula?

[float=left][img2]http://old.iaa.es/sites/default/files/u4/orion_sigma_ori_ilustracion_esp_1920x1169.jpg[/img2][c][size=85]Source: http://old.iaa.es/content/characteristics-multiple-star-sigma-orionis-are-determined[/size][/c][/float]I'd like to add a few words about Sigma Orionis, whose ultraviolet light ionizes the red background nebula and sculpts the shape of the Horsehead itself.

Sigma Orionis is a multiple star somewhat comparable to the [url=https://en.wikipedia.org/wiki/Trapezium_Cluster]Trapezium Cluster[/url], even though the most massive member of Sigma Orionis is not comparable to [url=https://en.wikipedia.org/wiki/Theta1_Orionis_C]Theta 1C Orionis[/url] in the Trapezium. The brightest component of Sigma Orionis, Sigma Orionis Aa, is a hot blue star of spectral class O9.5V, which radiates 35,000 times as much energy as the Sun from a 32,000K surface.

Read more [url=http://stars.astro.illinois.edu/sow/sigmaori.html]here[/url].

Ann

have to get the bazillion pixel poster and an ice col one, like pairing up Star War mo vie an 3D glasses.

WOW... that has got to be the most DETAILED image of it, I have seen... differentiation between sections, with some depth...layers of dark grey, and strands... just WOW...

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[url=https://apod.nasa.gov/apod/ap171227.html][img]https://apod.nasa.gov/apod/calendar/S_171227.jpg[/img] [size=150]The Horsehead Nebula[/size][/url]

[b] Explanation: [/b] One of the most identifiable nebulae in the sky, the [url=http://en.wikipedia.org/wiki/Horsehead_Nebula]Horsehead Nebula[/url] in [url=http://www.astro.wisc.edu/~dolan/constellations/constellations/Orion.html]Orion[/url], is part of a large, dark, [url=https://apod.nasa.gov/apod/ap090623.html]molecular cloud[/url]. Also known as [url=http://en.wikipedia.org/wiki/Edward_Emerson_Barnard]Barnard[/url] 33, the unusual shape was first [url=http://www.messier.seds.org/xtra/ngc/b33.html]discovered[/url] on a [url=https://en.wikipedia.org/wiki/Photographic_plate]photographic plate[/url] in the late 1800s. The red glow originates from [url=http://periodic.lanl.gov/1.shtml]hydrogen[/url] gas predominantly behind the nebula, ionized by the nearby bright star [url=http://www.dibonsmith.com/ori_s.htm]Sigma Orionis[/url]. The darkness of the [url=https://apod.nasa.gov/apod/ap061015.html]Horsehead[/url] is caused mostly by thick [url=https://apod.nasa.gov/apod/ap030706.html]dust[/url], although the lower part of the [url=https://apod.nasa.gov/apod/ap081126.html]Horsehead[/url]'s neck casts a shadow to the left. Streams of gas leaving [url=http://www.youtube.com/watch?v=hgTrLozRj40]the nebula[/url] are funneled by a strong [url=https://en.wikipedia.org/wiki/Magnetic_field]magnetic field[/url]. Bright spots in the [url=http://adsabs.harvard.edu/abs/1987AJ.....93.1514Z]Horsehead Nebula[/url]'s base are young stars just in the [url=https://apod.nasa.gov/apod/ap070218.html]process of forming[/url]. Light takes about 1,500 years to reach us from the [url=https://apod.nasa.gov/apod/ap090224.html]Horsehead Nebula[/url]. The [url=http://www.cfht.hawaii.edu/HawaiianStarlight/AIOM/English/CFHT-Coelum-AIOM-Jan2011.html]featured image[/url] was taken with the large 3.6-m [url=http://www.cfht.hawaii.edu/en/about/]Canada-France-Hawaii Telescope[/url] in [url=https://en.wikipedia.org/wiki/Hawaii#/media/File:Hawaii_in_United_States_(zoom)_(US50)_(-grid).svg]Hawaii[/url], [url=https://www.cia.gov/library/publications/the-world-factbook/geos/us.html]USA[/url].

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