Neutron Star: Difference between revisions

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A '''Neutron Star''' is a relatively small [[Star|star]] with a significantly high density. This high density is due to the tightly packed neutrons within it, hence the name. Neutron stars are formed when a [[Super Nova|super nova]] collapses but is not sufficiently massive to form a [[Black Hole|black holes]]. Certain neutron stars, known as [[Magnetar|magnetars]], possess a powerful magnetic field. These types of stars were used as the power sources of the [[Voidgate|voidgates]] and their defensive [[Aegisphere|aegispheres]].
A '''Neutron Star''' is a relatively small [[Star|star]] with a significantly high density. This high density is due to the tightly packed neutrons within it, hence the name. Neutron stars are formed when a supernova collapses but is not sufficiently massive to form a [[Black Hole|black holes]]. Certain neutron stars, known as [[Magnetar|magnetars]], possess a powerful magnetic field. These types of stars were used as the power sources of the [[Voidgate|voidgates]] and their defensive [[Aegisphere|aegispheres]].
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Latest revision as of 15:21, 21 January 2018

A Neutron Star is a relatively small star with a significantly high density. This high density is due to the tightly packed neutrons within it, hence the name. Neutron stars are formed when a supernova collapses but is not sufficiently massive to form a black holes. Certain neutron stars, known as magnetars, possess a powerful magnetic field. These types of stars were used as the power sources of the voidgates and their defensive aegispheres.