I knew it! Today's APOD sure looks like a circa 20-30 year-old comet picture - and it is, too!
Rhemann799_109P_24_11_92_1100px[1].jpg
Periodic Comet Swift-Tuttle
Image Credit & Copyright: Gerald Rhemann
You can tell the picture is old because of the lovely colors. The comet head is cyan-green, not grass green, and the ion tail is a lovely shade of blue. And ion tails of comets
are blue, really!
Case Western Reserve University wrote:
The ion tail is made up of ions (surprise!) - mostly CO+, N2+, CO2+. As the comet comes into the inner solar system, the Sun's radiation heats up the nucleus, "boiling off" and ionizing these gases.
These ions are electrically charged particles, and interact with the sun's solar wind (charged particles coming from the sun). The interaction between the comet and the solar wind distorts magnetic field lines, causing a cometary magnetotail which points away from the Sun. The charged ions stream along the magnetic field lines in the magnetotail, so the ion tail always points away from the Sun.
CO+ absorbs sunlight and flouresces, emitting energy at a wavelength of 4200 Angstroms, which is
blue light.
Right! Ion tails are blue. But many of today's comet photographers don't seem to know that. Take a look at a sample of Comet Lovejoy images:
Okay, comet photographers of today, I know you like to be creative. But ion tails of comets are blue, can we agree on that?
But even I have to like this last portrait of Lovejoy, where the comet has captured a nice galaxy in its non-blue net!
Actually, I think I have identified the galaxy in the comet's tail. Not only does it look an awful lot like NGC 891, but it
is NGC 891!
Comet Lovejoy on February 4 2015 Paganini et al.png
Oh, and HD 14633 is a lovely rare O-type star, almost 5,000 light-years away! Isn't that nice?
Ann
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