A planetary nebula forms when Sun - like stars gently eject their outer gaseous layers that
form bright nebulae with amazing and confounding shapes.
Not exact matches
This huge, dusky object
forms a conspicuous silhouette against the
bright, starry band of the Milky Way and for this reason the
nebula has been known to people in the southern hemisphere for as long as our species has existed.
Four stars collectively called the Trapezium
form the center of the
nebula, which to our eye looks like the
brightest star in the sword of Orion.
It is actively
forming new stars in regions that are so
bright that some can even be seen from Earth with the naked eye, such as the Tarantula
Nebula.
Of particular interest is a star at the center of the
nebula, just below the
brightest region, whose intense light and furious winds appear to have driven out the local gas,
forming a spherical void perhaps only 30,000 years agoquite recent, by astronomical standards.
While the
bright part of the
nebula is of about 65 arc seconds in diameter (more accurately, the «cork» is about 42x87», the «wings» 157x87»), this
nebula is surrounded by a faint halo covering a region of 290 arc seconds in diameter (Millikan, 1974); this material was probably ejected in the
form of stellar winds from the central star when it was still in the Red Giant phase of evolution.
Bright nebulae are usually vast concentrations of gas and dust in which stars have been or are being
formed.
NGC 6910 and M29 (NGC 6913) are the two
brightest star clusters in this region, and both of these star clusters
formed in this
nebula.
The second method is to plot the giant HII regions (
bright nebulae of ionised hydrogen) which are usually
formed in the spiral arms.
The structure of the
bright central region is a result of the fast stellar wind from the central star interacting with the material expelled when the
nebula was
formed.