But I'm not going out for them tonight. I'll stay inside and watch them from my kitchen.
Ann
Chris Peterson wrote: ↑Wed Jul 29, 2020 7:05 pm
Now that NEOWISE is moving away from the Sun,
the cyanogen glow of the coma is no longer overwhelmed by scattered sunlight.
https://steemit.com/steemstem/@terrylovejoy/comets-a-brief-primer wrote:
<<When distant from the sun a comet looks like an asteroid, however, as it approaches the sun its surface begins to warm which in turns starts to sublimate its constituent ices which include Water, Carbon Dioxide and others. In the vacuum of space most ices sublimate, that is pass from the solid to gas phase without becoming a liquid. Because of outgassing dust and ice grains are also released, and these all combine to form a large cloud around the nucleus which typically extends 100,000 km or more, which is about the size of Jupiter. During the Rosetta mission it was found that Water and Carbon Dioxide liberated from the nucleus of Comet 67P were dissociated from free electrons, creating other products (like Diatomic Carbon and Hydrogen, among others).
Often coma shine a vivid green, something some people can see even by direct observation by eye. Spectroscopic observations of coma reveal the main cause of this to be fluorescing diatomic carbon (C2) and Cyanogen (CN) which are presumably the byproduct of the dissociation of ices containing Carbon (CO2) and Nitrogen (Ammonia) from the nucleus surface. This can be seen in the adjacent (COMET LOVEJOY : 2013) spectra obtained by renown French amateur astronomer Christian Buil.
Surround the nucleus and coma, but not visible in the visual spectrum is a large cloud of Hydrogen atoms, which extends well beyond the normal coma and most likely is derived from the dissociation of water from the nucleus. It can only be detected from outside the earth's atmosphere because of the wavelengths it emits. In the case of Comet Hale-Bopp in 1997 the Hydrogen envelope extended 1 Astronomical Unit!>>
Very interesting, Chris. I like the bright green coma of comet NEOWISE. This green hue is noticeably absent in the portrait in today's APOD of the changing tails of comet NEOWISE.Chris Peterson wrote: ↑Tue Aug 11, 2020 11:56 pm Last night (2020-08-11 UT 03:30) C/2020 F3 (NEOWISE) and C/2017 T2 (PANSTARRS), a couple of the more interesting comets of the last months, passed about 2.7° of each other. Here they are in a single frame that is 3.7° x 1.2°. Two shots mosaiced, with a Canon 7D, 2-min exposure, ISO 1600 on a Stellarvue 102A refractor. NEOWISE on the right, PANSTARRS (much dimmer) in the lower left.
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neo+pan.jpg
Great pictures, Chris. Superb color contrasts particularly in the first image. Here the Moon has a brownish tint too, which I appreciate, since the Moon does indeed have a dark reddish tint.Chris Peterson wrote: ↑Sun Sep 06, 2020 4:46 pm The Moon and Mars, close together but moving apart. The first image was taken shortly after moonrise, 2020-09-06 UT 04:22. The second was taken around sunrise, 2020-09-06 UT 12:11 (so about eight hours later). Both images are at the same scale (but are likely rescaled on the webpage). You'll probably need to scroll the later image to see both objects.
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E7_47077p.jpg
E7_47099p.jpg
I should note that the Moon was low in the sky on the first shot, and very high on the second. Since we have somewhat smoky skies now, that makes the low altitude Moon particularly red in comparison with the high altitude one. The post processing of the two images is identical. In the later shot, you can see that the Moon has waned just a bit, and that it is less reddened by the atmosphere.Ann wrote: ↑Sun Sep 06, 2020 5:52 pmGreat pictures, Chris. Superb color contrasts particularly in the first image. Here the Moon has a brownish tint too, which I appreciate, since the Moon does indeed have a dark reddish tint.Chris Peterson wrote: ↑Sun Sep 06, 2020 4:46 pm The Moon and Mars, close together but moving apart. The first image was taken shortly after moonrise, 2020-09-06 UT 04:22. The second was taken around sunrise, 2020-09-06 UT 12:11 (so about eight hours later). Both images are at the same scale (but are likely rescaled on the webpage). You'll probably need to scroll the later image to see both objects.
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E7_47077p.jpg
E7_47099p.jpg
Ann
That's a great image, Chris. The galaxy looks very fine, and the IFN looks fantastic.Chris Peterson wrote: ↑Mon Sep 14, 2020 11:42 pm Finally had a couple of clear nights, without snow, without clouds, without smoke, without a Moon. So I thought I'd point the scope at something and make sure things were still working. Picked NGC 6951 for no particular reason, except it was high in the sky and looked kind of cool in pictures- a slightly asymmetric barred spiral galaxy. And surprise! Turned out to be a very interesting choice, as it lies behind a nice band of dust in our own galaxy, sometimes called "galactic cirrus" or "integrated flux nebula". Local dust illuminated only by the glow of the Milky Way. I'm amazed how bright it is, showing up in just a few minutes of exposure. Anyway, I collected eight hours of light and ended up with this. Seeing the wisps of foreground clouds gives the scene a very 3D look to my eyes.
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NGC6951_8h.jpg
I started out with this little project mainly just to get my observatory tuned up. I wasn't expecting the IFN, so that caught me by surprise. Most galaxies (to me) aren't overly interesting in color, so I just shot luminance data. But this is a pretty active galaxy, which could be fun to get some color info on, as well as color for the IFN. So I may go back and try that.Ann wrote: ↑Tue Sep 15, 2020 5:42 amThat's a great image, Chris. The galaxy looks very fine, and the IFN looks fantastic.Chris Peterson wrote: ↑Mon Sep 14, 2020 11:42 pm Finally had a couple of clear nights, without snow, without clouds, without smoke, without a Moon. So I thought I'd point the scope at something and make sure things were still working. Picked NGC 6951 for no particular reason, except it was high in the sky and looked kind of cool in pictures- a slightly asymmetric barred spiral galaxy. And surprise! Turned out to be a very interesting choice, as it lies behind a nice band of dust in our own galaxy, sometimes called "galactic cirrus" or "integrated flux nebula". Local dust illuminated only by the glow of the Milky Way. I'm amazed how bright it is, showing up in just a few minutes of exposure. Anyway, I collected eight hours of light and ended up with this. Seeing the wisps of foreground clouds gives the scene a very 3D look to my eyes.
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NGC6951_8h.jpg
I checked out some other pictures of NGC 6951. Many of them show galactic cirrus, and most of them show the cirrus to be reddish. This image is an interesting example.
I also checked out NGC 6951 with my software, and I was astonished at this galaxy's red color. Its B-V index is 0.99, which is very red indeed for a spiral galaxy and even redder than our big bully of a neighbor, Andromeda, which is itself really quite red as spiral galaxies go with a B-V index of 0.92.
This makes me ask two questions, maybe even three. Could the light of NGC 6951 be reddened by the IFN that might be located right in front of it from our point of view? Did you, Chris, use red-sensitive equipment for your image?
And why is the IFN so red? How red is our galaxy?
Ann
Glad someone's skies have cleared, and to see the nice galaxy image you captured Chris.Chris Peterson wrote: ↑Mon Sep 14, 2020 11:42 pm Finally had a couple of clear nights, without snow, without clouds, without smoke, without a Moon. So I thought I'd point the scope at something and make sure things were still working. Picked NGC 6951 for no particular reason, except it was high in the sky and looked kind of cool in pictures- a slightly asymmetric barred spiral galaxy. And surprise! Turned out to be a very interesting choice, as it lies behind a nice band of dust in our own galaxy, sometimes called "galactic cirrus" or "integrated flux nebula". Local dust illuminated only by the glow of the Milky Way. I'm amazed how bright it is, showing up in just a few minutes of exposure. Anyway, I collected eight hours of light and ended up with this. Seeing the wisps of foreground clouds gives the scene a very 3D look to my eyes.
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NGC6951_8h.jpg