
ISS023-E-57948
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Sunset Seen from the International Space Station: This
spectacular image of sunset on the Indian Ocean was taken by
astronauts aboard the International Space Station (ISS). The image
presents an edge-on, or limb view, of the Earth’s atmosphere as seen
from orbit. The Earth’s curvature is visible along the horizon line,
or limb, that extends across the image from center left to lower
right. Above the darkened surface of the Earth, a brilliant sequence
of colors roughly denotes several layers of the atmosphere. Deep
oranges and yellows appear in the troposphere, which extends from the
Earth’s surface to 6–20 km high. This layer contains over 80 percent
of the mass of the atmosphere and almost all of the water vapor,
clouds, and precipitation. Several dark cloud layers are visible
within this layer. Variations in the colors are due mainly to varying
concentrations of either clouds or aerosols (airborne particles or
droplets). The pink to white region above the clouds appears to be
the lower stratosphere; this atmospheric layer generally has few or
no clouds, and it extends up to approximately 50 km above the Earth’s
surface. Above the stratosphere, blue layers likely mark the
transition between the middle and upper atmosphere as it gradually
fades into the blackness of outer space. The ISS was located over
the southern Indian Ocean when this picture was taken, with the
astronaut looking towards the west. Astronauts aboard the ISS see 16
sunrises and sunsets per day due to their high orbital velocity
(greater than 28,000 km per hour). The multiple chances for
photography are fortunate because at that speed, each sunrise or
sunset only lasts a few seconds!
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ISS023-E-58455
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Aurora Australis Observed from the International Space
Station: Among the views of Earth afforded astronauts aboard the
International Space Station (ISS), surely one of the most spectacular
is of the aurora. These ever-shifting displays of colored ribbons,
curtains, rays, and spots are most visible near the North (aurora
borealis) and South (aurora australis) Poles as charged particles
(ions) streaming from the Sun (the solar wind) interact with Earth’s
magnetic field. While aurora are generally only visible close to
the poles, severe magnetic storms impacting the Earth’s magnetic
field can shift them towards the equator. This striking aurora image
was taken during a geomagnetic storm that was most likely caused by a
coronal mass ejection from the Sun on May 24, 2010. The ISS was
located over the Southern Indian Ocean at an altitude of 350
kilometers (220 miles), with the astronaut observer most likely
looking towards Antarctica (not visible) and the South Pole. The
aurora has a sinuous ribbon shape that separates into discrete spots
near the lower right corner of the image. While the dominant
coloration of the aurora is green, there are faint suggestions of red
left of image center. Dense cloud cover is dimly visible below the
aurora. The curvature of the Earth’s horizon (the limb) is clearly
visible, as is the faint blue line of the upper atmosphere directly
above it (at image top center). Several stars appear as bright
pinpoints against the blackness of space at image top
right. Auroras happen when ions in the solar wind collide with
atoms of oxygen and nitrogen in the upper atmosphere. The atoms are
excited by these collisions, and they typically emit light as they
return to their original energy level. The light creates the aurora
that we see. The most commonly observed color of aurora is green,
caused by light emitted by excited oxygen atoms at wavelengths
centered at 0.558 micrometers, or millionths of a meter. (Visible
light is reflected from healthy (green) plant leaves at approximately
the same wavelength.) Red aurora are generated by light emitted at a
longer wavelength (0.630 micrometers), and other colors such as blue
and purple are also sometimes observed.
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ISS023-E-41934
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Southern Paramushir Island, Kuril Chain, Russia: The Kuril
Island chain is built from a line of volcanoes, an island arc, that
extends from Russia’s Kamchatka Peninsula to northern Japan. Island
arcs form along an active boundary between two tectonic plates, with
one being driven beneath the other (subduction). Magma generated by
subduction feeds volcanoes—and eventually volcanic islands—over the
subduction boundary. Paramushir Island in the northern Kurils is an
example of a large island built by several volcanoes over geologic
time. This astronaut photograph shows the southern end of Paramushir
Island after a snowfall. The western slopes of the mountains are
brightly illuminated, while the eastern slopes are in shadow. Four
major volcanic centers create this part of the island. Fuss Peak
(image center left) is an isolated stratovolcano connected to the
main island via an isthmus. Fuss Peak last erupted in 1854. The
southern tip of the island is occupied by the Karpinsky Group of
three volcanic centers. A minor eruption of ash following an
earthquake occurred on this part of the island in 1952. The
Lomonosov Group to the northeast (image center) includes four cinder
cones and a lava dome that produced several lava flows in the past,
but there have been no eruptions from the Lomonosov Group in recorded
history. The most recent volcanic activity on Paramushir Island
occurred in 2008 at the Chikurachki cone located along the northern
coastline of the island at image top center. The summit of this
volcano [1,816 meters (5,958 feet) above sea level] is the highest on
Paramushir Island. Much of the Sea of Okhotsk visible in the image
is covered with low clouds that often form around the islands in the
Kuril chain. The clouds are generated by moisture-laden air passing
over the cool sea/ocean water, and they typically wrap around the
volcanic islands.
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ISS023-E-56842
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Cape Kazantip, Kerch Peninsula, Southern Sea of Azov, Ukraine:
Cape Kazantip is a prominent headland on the Kerch Peninsula, which
defines the southern shore of the Sea of Azov and the east extension
of the Crimean Peninsula. During the Second World War, German and
Soviet forces fought on the Kerch Peninsula, with the line of battle
impinging on areas shown at the bottom of the image. Due to its
relatively low latitude (45° N) the Crimea has been the warm
holidaying destination for generations of Ukrainians and Russians.
Towns in the Kazantip area—Lenine, Shcholkine—offer tourist
attractions, ranging from birdwatching to beaches and music
festivals. This detailed astronaut photograph was taken from the
International Space Station (ISS) when it was located 400 kilometers
(250 miles) to the northeast, but due to the long (800 mm) lens used,
the photo includes detailed field patterns and city blocks. Green and
brown fields show intensive agricultural activity in the area, and
salt ponds are visible at the west end of the shallow Lake
Aktashskoye at image center. The distance from the tip of the Cape to
the largest local city, Lenine (population ~70,000, image lower left)
is only 20 kilometers (12 miles). Shcholkine, named for a Russian
physicist, is a new town built in 1978 to house workers of the
planned Crimean nuclear power plant. The partially completed plant
was inspected following the Chernobyl disaster of 1986, and was found
to be located on a site prone to earthquakes. Further construction
was terminated, and the already built structures and construction
equipment was abandoned in place. Today, Shcholkine is an
increasingly popular tourist destination.
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