Difference between revisions of "Oort Cloud"
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== Description ([[Specifications]]) == | == Description ([[Specifications]]) == | ||
− | A typical Oort cloud | + | A typical Oort cloud lies between 0.5 and 1 [[light-year]]s from its primary [[star]] and has an aggregate [[mass]] about that of [[Terra]]; density is thus extremely low. |
=== Image Repository === | === Image Repository === | ||
− | [[File:Terra System.jpg]] <br>An overview of the [[Terra]] [[system]], representative of the structure of a [[star system]]. | + | [[File:Terra System.jpg]] <br>An overview of the [[Terra]] [[system]], representative of the structure of a [[star system]] and the position of the Oort Cloud. |
== History & Background ([[Dossier]]) == | == History & Background ([[Dossier]]) == |
Revision as of 16:22, 22 March 2019
An Oort Cloud is a very expansive spherical shell, located in the far system, around most stars or star systems, containing numerous small bodies of cometary material.
- It is an astrographic feature.
Description (Specifications)
A typical Oort cloud lies between 0.5 and 1 light-years from its primary star and has an aggregate mass about that of Terra; density is thus extremely low.
Image Repository
An overview of the Terra system, representative of the structure of a star system and the position of the Oort Cloud.
History & Background (Dossier)
The Oort cloud is named after its discoverer, Terran astronomer Jan Oort.
Cometary Bodies
The main constituents of cometary bodies are ice and dust ("dirty snowballs").
Cometary Collisions
Bodies in the Oort cloud are occasionally perturbed by collisions or by the influence of nearby stars into orbits which pass near the star; these form the visible comets.
Meteors
No information yet available.
References & Contributors (Sources)
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. |
- Classic Traveller Beltstrike
- Traveller Wiki Editorial Team
- Author & Contributor: Lord (Marquis) and Master of Sophontology Maksim-Smelchak of the Ministry of Science