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Supernova Remnant

The structure resulting from the explosion of a star in a supernova. It consists of ejected material expanding from the explosion and the shocked interstellar medium it sweeps up.

Source: apod.nasa.gov

APODs including "Supernova Remnant"

Filaments of the Vela Supernova Remnant

01/10/2013

Filaments of the Vela Supernova Remnant
Image Credit: Angus Lau, Y Van, SS Tong (Jade Scope Observatory) / NASA APOD

The explosion is over but the consequences continue. About eleven thousand years ago a star in the constellation of Vela could be seen to explode, creating a strange point of light briefly visible to humans living near the beginning of recorded history. The outer layers of the star crashed into the interstellar medium, driving a shock wave that is still visible today. A roughly spherical, expanding shock wave is visible in X-rays. The above image captures some of that filamentary and gigantic shock in visible light. As gas flies away from the detonated star, it decays and reacts with the interstellar medium, producing light in many different colors and energy bands. Remaining at the center of the Vela Supernova Remnant is a pulsar, a star as dense as nuclear matter that rotates completely around more than ten times in a single second. Note: How to follow APOD if the US government shuts down