Difference between revisions of "Horsehead Nebula"

From Traveller Wiki - Science-Fiction Adventure in the Far future
Jump to navigation Jump to search
(3 intermediate revisions by one other user not shown)
Line 1: Line 1:
 
[[File:Horsehead Nebula.jpg|400px|thumb|right|Horsehead Nebula (Barnard 33)]]
 
[[File:Horsehead Nebula.jpg|400px|thumb|right|Horsehead Nebula (Barnard 33)]]
 
 
The [[Horsehead Nebula]] (also known as '''Barnard 33''') is a dark nebula, or absorption nebula, in the constellation Orion as seen from the night sky of [[Terra]].  
 
The [[Horsehead Nebula]] (also known as '''Barnard 33''') is a dark nebula, or absorption nebula, in the constellation Orion as seen from the night sky of [[Terra]].  
 +
* It is an [[astrographic feature]] and a [[nebula]].
  
 
== Description ([[Specifications]]) ==
 
== Description ([[Specifications]]) ==
 
The nebula is part of the much larger ''Orion Molecular Cloud Complex'' (where star formation is taking place), and lies at a distance of ~460pc from [[Sol (star)|Sol]] along a Rimward by Rimtrailing bearing at 207.0<sup>o</sup> galactic longitude and -16.8<sup>o</sup> south galactic latitude.  
 
The nebula is part of the much larger ''Orion Molecular Cloud Complex'' (where star formation is taking place), and lies at a distance of ~460pc from [[Sol (star)|Sol]] along a Rimward by Rimtrailing bearing at 207.0<sup>o</sup> galactic longitude and -16.8<sup>o</sup> south galactic latitude.  
* The pinkish-red glow emanating from the nebula is caused by hydrogen gas (predominantly behind the nebula) that has been ionized by the nearby bright star ''Sigma Orionis''. The darkness of the Horsehead is the result of thick dust blocking the light of the stars behind it, and the visible dark nebula emerging from the gaseous complex is a region of low-mass star formation. Bright spots at the base of the Horsehead Nebula are young stars in the process of forming.
+
*The ''Orion Molecular Cloud Complex'' extends throughout the [[Terra]]n-sky constellation of [[Orion]] and includes [[Barnard's Loop]], the [[Orion Nebula]], [[M43]], [[M78]], and the [[Flame Nebula]].
 +
* The pinkish-red glow emanating from the [[Horsehead Nebula]] is caused by hydrogen gas (predominantly behind the nebula) that has been ionized by the nearby bright star [[Sigma Orionis (star)|Sigma Orionis]]. The darkness of the Horsehead is the result of thick dust blocking the light of the stars behind it, and the visible dark nebula emerging from the gaseous complex is a region of low-mass star formation. Bright spots at the base of the Horsehead Nebula are young stars in the process of forming.  
  
 
== History & Background ([[Dossier]]) ==
 
== History & Background ([[Dossier]]) ==
Line 11: Line 12:
  
 
=== Image Repository ===
 
=== Image Repository ===
No information yet available.
+
[[TravellerMap]]: <br>
 +
[https://travellermap.com/?options=58367&x=141.163&y=-404.872&scale=24.25]
  
 
== [[World]]s & [[Sector]]s ([[Astrography]]) ==
 
== [[World]]s & [[Sector]]s ([[Astrography]]) ==
 
This [[astrographic feature]] is primarily found in the following areas: <br>
 
This [[astrographic feature]] is primarily found in the following areas: <br>
 
''[[Charted Space]]:''
 
''[[Charted Space]]:''
* [[TBD Sector]]
+
* [[Sigma Orionis Sector]]
 
** [[TBD Subsector]]
 
** [[TBD Subsector]]
  
Line 24: Line 26:
  
 
== References & Contributors (Sources) ==
 
== References & Contributors (Sources) ==
{{metadata}}
+
{{Metadata}}
 
{{Intermediate}}
 
{{Intermediate}}
 
{{Detail}}
 
{{Detail}}

Revision as of 02:12, 20 January 2019

Horsehead Nebula (Barnard 33)

The Horsehead Nebula (also known as Barnard 33) is a dark nebula, or absorption nebula, in the constellation Orion as seen from the night sky of Terra.

Description (Specifications)

The nebula is part of the much larger Orion Molecular Cloud Complex (where star formation is taking place), and lies at a distance of ~460pc from Sol along a Rimward by Rimtrailing bearing at 207.0o galactic longitude and -16.8o south galactic latitude.

  • The Orion Molecular Cloud Complex extends throughout the Terran-sky constellation of Orion and includes Barnard's Loop, the Orion Nebula, M43, M78, and the Flame Nebula.
  • The pinkish-red glow emanating from the Horsehead Nebula is caused by hydrogen gas (predominantly behind the nebula) that has been ionized by the nearby bright star Sigma Orionis. The darkness of the Horsehead is the result of thick dust blocking the light of the stars behind it, and the visible dark nebula emerging from the gaseous complex is a region of low-mass star formation. Bright spots at the base of the Horsehead Nebula are young stars in the process of forming.

History & Background (Dossier)

No information yet available.

Image Repository

TravellerMap:
[1]

Worlds & Sectors (Astrography)

This astrographic feature is primarily found in the following areas:
Charted Space:

World Listing: 1105

The following systems and worlds are associated with this astrographic feature:

No world articles for Horsehead Nebula


References & Contributors (Sources)

This article has metadata.
62px-Information icon.svg.png This article is missing content for one or more detailed sections. Additional details are required to complete the article. You can help the Traveller Wiki by expanding it.
Smallwikipedialogo.png This page uses content from Wikipedia. The original article was at Horsehead_nebula. The list of authors can be seen in the page history. The text of Wikipedia is available under the Commons Attribution-ShareAlike 3.0 Unported License.
This list of sources was used by the Traveller Wiki Editorial Team and individual contributors to compose this article. Copyrighted material is used under license from Far Future Enterprises or by permission of the author. The page history lists all of the contributions.