by Ann » Tue Nov 29, 2022 7:28 am
APOD Robot wrote:
The Gum Nebula is so close that we are much nearer the front edge than the back edge, each measuring 450 and 1500 light years respectively.
That's certainly fascinating!
Anyway. The Gum Nebula is faint, which is why we don't often see it being photographed. The nebulas at upper left in this APOD, the Carina Nebula and also the Running Chicken Nebula, are bright, and they are also much more distant, at an approximate distance of 7,500 light-years.
It is interesting that the upper to upper left part of the Gum Nebula (as seen in this APOD) is quite dark.
Wikipedia wrote:
The Gum Nebula (Gum 12) is an emission nebula that extends across 36° in the southern constellations Vela and Puppis. It lies approximately 450 parsecs from the Earth. Hard to distinguish, it was widely believed to be the greatly expanded (and still expanding) remains of a supernova that took place about a million years ago. More recent research suggests it may be an evolved H II region. It contains the 11,000-year-old Vela Supernova Remnant, along with the Vela Pulsar.
More recent research suggests that the Gum Nebula may be an evolved H II region? Really?
The Gum Nebula contains about 32 cometary globules. These dense cloud cores are subject to such strong radiation from O-type stars γ2 Vel and ζ Pup and formerly the progenitor of the Vela Supernova Remnant that the cloud cores evaporate away from the hot stars into comet-like shapes. Like ordinary Bok globules, cometary globules are believed to be associated with star formation.
So hot O-type stars Gamma Velorum and Zeta Puppis affect the Gum nebula. They shape cometary globulas in the Gum Nebula, but they also inject energy into the large nebula and certainly help ionize parts of it.
Perhaps the dark part of the Gum Nebula is shielded from the harsh ultraviolet light from Gamma Velorum and Zeta Puppis?
Ann
[float=right][attachment=0]APOD 29 November 2022 annotated.png[/attachment][/float][img3="The Gum Nebula Supernova Remnant
Image Credit & Copyright: Victor Lima"]https://apod.nasa.gov/apod/image/2211/Gum_Lima_960_annotated.jpg[/img3]
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[quote]APOD Robot wrote:
The Gum Nebula is so close that we are much nearer the front edge than the back edge, each measuring 450 and 1500 light years respectively. [/quote]
That's certainly fascinating! :shock:
Anyway. The Gum Nebula is faint, which is why we don't often see it being photographed. The nebulas at upper left in this APOD, the Carina Nebula and also the Running Chicken Nebula, are bright, and they are also much more distant, at an approximate distance of 7,500 light-years.
It is interesting that the upper to upper left part of the Gum Nebula (as seen in this APOD) is quite dark.
[quote][url=https://en.wikipedia.org/wiki/Gum_Nebula]Wikipedia[/url] wrote:
The Gum Nebula (Gum 12) is an emission nebula that extends across 36° in the southern constellations Vela and Puppis. It lies approximately 450 parsecs from the Earth. Hard to distinguish, it was widely believed to be the greatly expanded (and still expanding) remains of a supernova that took place about a million years ago. More recent research suggests it may be an evolved H II region. It contains the 11,000-year-old Vela Supernova Remnant, along with the Vela Pulsar.[/quote]
More recent research suggests that the Gum Nebula may be an evolved H II region? Really?
[float=right][img3="Image simulation of the Gum Nebula. Author: Roberto Mura."]https://upload.wikimedia.org/wikipedia/commons/1/13/GumNebula.png[/img3][/float][quote]The Gum Nebula contains about 32 cometary globules. These dense cloud cores are subject to such strong radiation from O-type stars γ2 Vel and ζ Pup and formerly the progenitor of the Vela Supernova Remnant that the cloud cores evaporate away from the hot stars into comet-like shapes. Like ordinary Bok globules, cometary globules are believed to be associated with star formation.[/quote]
So hot O-type stars Gamma Velorum and Zeta Puppis affect the Gum nebula. They shape cometary globulas in the Gum Nebula, but they also inject energy into the large nebula and certainly help ionize parts of it.
Perhaps the dark part of the Gum Nebula is shielded from the harsh ultraviolet light from Gamma Velorum and Zeta Puppis?
Ann