Nebulas
 
Nebulas, one of the most beautiful phenomenom in the universe, are made up of gas left behind by stars forming or exploding.  There are many different classes of nebula, which are: planetary, supernova remnants, diffuse nebula(which includes reflecting, emission, and dark nebulas).  Small, bright nebulas are called Herbig Haro and are probably jets of gas coming from forming stars.  

Planetary nebulas resemble planets, and are actually left over shell material from forming stars during their giant Red Stage.  The shell probably came off before the white dwarf stage of the star.  Several planetary nebulas exist in the Milky Way.  

Supernova remnants are exactly what they say: supernova nebulas are remnants of a star that exploded.  Left over remnants become surrounded by gas, causing a nebula.   One of the most famous supernova nebulas is the crab nebula in the star constellation Taurus.

Crab Nebula
Image: Crab Nebula
 
Orion Nebula Diffuse nebulas are extremely large, and can be light years in width.  They have no definate shape, and are either light or dark.  These stellar bodies often contain some of the most striking and amazing objects in the galaxy, and have gases that run in chaotic currents all throughout it.  

Dark nebulas are nonilluminous or faintly luminous clouds that have never been seen very clearly.   They obscure some of the Milky way, but are too distant for any light(even from stars) to be seen.

Astronomy Home
Click here to go back.

Created by ThinkQuest Team 23830
Last Updated August 28, 1998.
All images, unless otherwise credited, are credit of M. Mathis, 1998.