Starship Asterisk*

[url=http://eol.jsc.nasa.gov/scripts/sseop/photo.pl?mission=ISS025&roll=E&frame=9858][b]ISS025-E-9858[/b][/url] [i](Credit: NASA/ISS/EO)[/i]

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Y’know, when you looked at maps of Egypt in school, you could see the Nile cutting through the desert, but you didn’t get the real perspective of where the people were, what that river means.

Space travel makes that perspective a bit easier to soak in:

That, my friends, is the Nile delta as seen by the International Space Station on October 28. The station was well south of that area, about 800 km (500 miles) south if I’ve done the math correctly. In this oblique view facing north, you can see Cairo at the neck of the delta, the city lights blaring. The Mediterranean Sea dominates the northern (top) part of the picture, with Cyprus glowing above and to the right of the mighty river. Off to the right you can also see Tel Aviv in Israel and Amman in Jordan. The glowing arc at the top is airglow, caused when molecules disrupted by ultraviolet light from the Sun during the day recombine. It’s a thin layer you’re seeing here edge-on, so it looks like an arc of light.
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Chris Peterson wrote:

rstevenson wrote:But yes, there are ships and drilling rigs within the range of this image, and the rigs especially can be very bright.

The good light pollution images made from space always show oil rigs in the Gulf. Noise is just a single pixel effect, so it shows up as fairly symmetrical spots. Noisy pixels will often look like a saturated color, as well, since each pixel lies under a color filter, and is therefore interpreted as a pure color.

Chris Peterson wrote:

Sam wrote:And real stars, too! The Lyre and the Dolphin on the right, and Fomalhaut and perhaps even Alnair on the right, though that one's too far south for me to be familiar with.

Don't you mean "left"?

Vega is the bright star close to the Earth's limb, near the left edge. The five other bright stars of Lyra are seen below it and to its right, with beta Lyra (Sheliak) almost at the boundary of skyglow. Delphinius is at the center left, just above that ISS structure supporting the solar array. I'm not sure what's on the right- Piscis Austrinus, maybe?

Sam wrote:And real stars, too! The Lyre and the Dolphin on the right, and Fomalhaut and perhaps even Alnair on the right, though that one's too far south for me to be familiar with.

KerschbaumIfAVienna wrote:I like the Subject Distance of 2147483647.000 m in the EXIF header. Seems they lifted the ISS out to 5.6 times the distance to the moon...

Chris Peterson wrote: There are definitely real lights visible in the ocean areas of this image.

"well above the level of the clouds"

rstevenson wrote:But yes, there are ships and drilling rigs within the range of this image, and the rigs especially can be very bright.

Ewoki wrote:Any Idea what these lights on the ocean are? ships or drilling platforms or both and why so bright?

Ewoki wrote:Any Idea what these lights on the ocean are? ships or drilling platforms or both and why so bright?

toddnang wrote:
I am curious what is the dark green band below the Earth's limb in the photo taken from the space station? It appears to be well above the level of the clouds, but I imagine it must be some atmospheric structure?

http://en.wikipedia.org/wiki/Airglow wrote:

Nightglow

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<<Airglow (also called nightglow) is the very weak emission of light by a planetary atmosphere. In the case of Earth's atmosphere, this phenomenon causes the night sky to never be completely dark (even after the effects of starlight and diffused sunlight from the far side are removed).

The airglow phenomenon was first identified in 1868 by Swedish scientist Anders Ångström. Since then it has been studied in the laboratory, and various chemical reactions have been observed to emit electromagnetic energy as part of the process. Scientists have identified some of those processes which would be present in Earth's atmosphere, and astronomers have verified that such emissions are present.

Airglow is caused by various processes in the upper atmosphere, such as the recombination of ions which were photoionized by the sun during the day, luminescence caused by cosmic rays striking the upper atmosphere, and chemiluminescence caused mainly by oxygen and nitrogen reacting with hydroxyl ions at heights of a few hundred kilometers. It is not noticeable during the daytime because of the scattered light from the Sun.

Even at the best ground-based observatories, airglow limits the sensitivity of telescopes at visible wavelengths. Partly for this reason, space-based telescopes such as the Hubble Space Telescope can observe much fainter objects than current ground-based telescopes at visible wavelengths.

The airglow at night may be bright enough to be noticed by an observer, and is generally bluish in color. Although airglow emission is fairly uniform across the atmosphere, to an observer on the ground it appears brightest at about 10 degrees above the horizon, because the lower one looks the greater the depth of atmosphere one is looking through. Very low down, however, atmospheric extinction reduces the apparent brightness of the airglow.

One airglow mechanism is when an atom of nitrogen combines with an atom of oxygen to form a molecule of nitric oxide (NO). In the process a photon is emitted. This photon may have any of several different wavelengths characteristic of nitric oxide molecules. The free atoms are available for this process because molecules of nitrogen (N2) and oxygen (O2) are dissociated by solar energy in the upper reaches of the atmosphere, and may encounter each other to form NO. Other species that can create air glow in the atmosphere are Hydroxyl (OH), molecular Oxygen (O), and Sodium (Na)and Lithium (Li).>>

florid_snow wrote:I hate to be a downer, but all that light is completely wasted,