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APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 4:07 am
by APOD Robot
The Red Spider Planetary Nebula
Explanation: Oh what a
tangled web a
planetary nebula can weave. The
Red Spider Planetary Nebula shows the complex structure that can result when a
normal star ejects its outer gases and becomes a
white dwarf star. Officially tagged
NGC 6537, this two-lobed symmetric
planetary nebula houses one of the
hottest white dwarfs ever observed, probably as part of a
binary star system. Internal
winds emanating from the central stars, visible in the center, have been measured in excess of 1000 kilometers per second. These
winds expand the nebula, flow along the nebula's walls, and cause waves of hot
gas and
dust to collide.
Atoms caught in these colliding shocks radiate light shown in the above representative-color picture by the
Hubble Space Telescope. The
Red Spider Nebula lies toward the
constellation of the Archer (
Sagittarius). Its distance is not well known but has been
estimated by some to be about 4,000
light-years.
[/b]
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 4:55 am
by Boomer12k
Reminds me of the "X red Square nebula"...
and the larger image reminds me of the "Running Man Nebula"...
Why is there a dark patch in the center...is that a relative void or something???
:---[===] *
- X red Square Nebula...
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 7:06 am
by Ann
If the central star of this nebula is one of the hottest known, then it is interesting that the nebula is so red. I would have expected more blue-green OIII emission in the presence of such a very hot star.
Ann
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 9:03 am
by tannaberton
You are looking at an hourglass figure at an angle. These things always do that.
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 11:56 am
by biddie67
Awesome but so frustrating! I'd love to be able to rotate a view of this nebula in 3-D so the complete shape could be seen.
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 12:12 pm
by royalpalms6@msn.com
What is a 1000 meters a second mean in laimans term. ( = to ? miles an hour).
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 12:53 pm
by rstevenson
royalpalms6@msn.com wrote:What is a 1000 meters a second mean in laimans term. ( = to ? miles an hour).
Your browser probably has a small search field in the top area, with a drop-down for selecting which search engine to use. Select Google. (Others will also work, I'm sure, but I used Google.) Enter this into that search field (or in Google's home page search field if you wish)...
"convert 1000 meters a second to mph"
The answer is in the search results: 2236.94 mph.
You can use the same technique to calculate any reasonable -- and some unreasonable -- conversions.
Rob
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 1:05 pm
by neufer
rstevenson wrote:royalpalms6@msn.com wrote:
What is a 1000 meters a second mean in laimans term. ( = to ? miles an hour).
Your browser probably has a small search field in the top area, with a drop-down for selecting which search engine to use. Select Google. (Others will also work, I'm sure, but I used Google.) Enter this into that search field (or in Google's home page search field if you wish)...
"convert 1000 meters a second to mph"
The answer is in the search results: 2236.94 mph.
And don't forget we are talking 1000
kilometers per second here.
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 1:29 pm
by neufer
Ann wrote:
If the central star of this nebula is one of the hottest known, then it is interesting that the nebula is so red. I would have expected more blue-green OIII emission in the presence of such a very hot star.
Most of the oxygen is probably
much more highly ionized than just
doubly ionized .
And you are assuming that any doubly ionized oxygen there
would last for a long enough period of time for a
forbidden blue-green OIII photon to be emitted before being knocked about by an ultraviolet photon from the white dwarf.
Most of the hydrogen is fully ionized but an isolated proton & electron at least have the time to connect up and
rapidly radiate non-forbidden Lyman & Balmer photons before an ultraviolet photon from the white dwarf comes along to re-ionize it.
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Mon Oct 29, 2012 10:56 pm
by owlice
Oh, I should have mentioned this earlier; my apologies. This APOD is mirrored
here as well as on the other
APOD mirrors.
Goddard's servers were shut down earlier today as a precaution against a power outage due to Hurricane Sandy.
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Fri Nov 23, 2012 2:20 pm
by 500pesos
emanating from the central stars, visible in the center
I don't see any stars. Only a weird whiteish thing with a black centre.
Re: APOD: The Red Spider Planetary Nebula (2012 Oct 29)
Posted: Fri Nov 23, 2012 2:32 pm
by neufer
500pesos wrote: emanating from the central stars, visible in the center
I don't see any stars. Only a weird whiteish thing with a black centre.
http://pintester.com/2012/08/honey-and- ... d-removal/
http://asterisk.apod.com/viewtopic.php?f=23&t=30183