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Did You Know?
By chance, a collision of two galaxies has created a visually
recognizable shape on a cosmic scale - The Cartwheel Galaxy.
The Cartwheel is approximately 500 million light-years away
in the constellation Sculptor. The vibrant purple rim around
the galaxy is 100,000 light years in diameter and is composed
of newly formed massive and very bright stars.
-Kirk Borne STScI, NASA
Did You Know?
Around 100 million years ago, NGC 3310 is supposed to have collided
with a smaller galaxy, causing the large spiral galaxy to light
up with a tremendous burst while forming stars. The changing
gravity during the collision created density waves that compressed
existing clouds of gas and triggered the star-forming party.
MGC 3310 is 50 million light-years away and visible with a telescope
in the direction of the constellation "Ursa Major"
.
-G.R. Meurer (JHU) Hubble Heritage Team, NASA
Did You Know?
What evil lurks in the hearts of galaxies? The gas and dust
in this disk are swirling into what is almost certainly a massive
black hole. The disk is probably what remains of a smaller galaxy
that fell in hundreds of millions of years ago. Collisions like
this may be a common way of creating such active galactic nuclei
as quasars. Strangely, the center of this fiery whirlpool is
offset from the exact center of the galaxy - for a reason that
for now remains an astronomical mystery.
-H. Ford and L. Ferrarese, (Johns Hopkins), W.
Jaffe, (Leiden), NASA
Did You Know?
Gamma rays are the most energetic from of light. When the EGRET
instrument on the orbiting Compton Gamma-ray Observatory surveyed
the sky in the 1990s it catalogued 271 celestial sources of
high-energy gamma rays. Researchers identified some with exotic
black holes, neutron stars, and distant flaring galaxies. But
170 of the catalogued sources remain unidentified.
-N. Gehrels, D. Macomb, D. Bertsch, D. Thompson,
R. Hartman (GSFC), Egret, NASA
Did You Know?
Lofted over the Sun on loopin gmagnetic fields, large solar
prominences are composed of relatively cool, dense plasma. When
seen in front of the brilliant solar disk, they appear as dark
filaments, but these structures are bright when viewed against
the blackness of space.
-SOHO-EIT
Consortium, ESA, NASA
Did You Know?
The unusual jet emanating from the center of Galaxy M87 was
first noticed early in the twentieth century. The exact cause
is still debated. M87 is a giant elliptical galaxy residing
only 50 million light-years away in the Virgo cluster of galaxies.
Faint dots surrounding M87's center are large, ancient globular
clusters.
-J. A. Biretta et al., Hubble Heritage Team,
NASA
Did
You Know?
Every day is cloudy on Jupiter, the solar system's reigning
gas giant. And swirling cloud tops are all that is visible from
satellite images. A giant planet, Jupiter's diameter is more
than eleven times that of the Earth; the smallest storms visible
in this portrait are similar in size to large terrestrial hurricanes. -Cassini
Imagins Team, Cassini Project, NASA
Did You Know?
Jupiter's rings were discovered in 1979 but their origin has
always been a mystery. Data from the Galileo spacecraft
confirmed that they were created by meteoroid impacts on small
nearby moons.
-M. Belton (NOAO), NASA
Did You Know?
The unusual jet emanating from the center of Galaxy M87 was
first noticed early in the twentieth century. The exact cause
is still debated. M87 is a giant elliptical galaxy residing
only 50 million light-years away in the Virgo cluster of galaxies.
Faint dots surrounding M87's center are large, ancient globular
clusters.
-J. A. Biretta et al., Hubble Heritage Team,
NASA
The
Whirlpool Galaxy is a classical spiral galaxy. At only 30
million light-years distant and fully 60,000 light-years across,
anyone with a good pair of glasses can see it toward the constellation
Canes Venatici.
-N. Scoville (Caltech), T. Rector (NOAO) et
al., Hubble Heritage Team, NASA
Did You Know?
The Red Spider planetary nebula is a 2-lobed symmetrical planetary
nebula housing one of the hottest white dwarfs ever observed,
probably as part of a binary system. Internal winds emanating
from the central stars expand the nebula, flow along the nebula's
walls, and cause waves of gas dust to collide. Atoms caught
in these colliding shocks radiate light; a spectacular display
of cloud like gases.
-Garrelt Mellema (Leiden University) et al. HST,
ESA, NASA
Did You Know?
The Red Spider planetary nebula is a 2-lobed symmetrical planetary
nebula housing one of the hottest white dwarfs ever observed,
probably as part of a binary system. Internal winds emanating
from the central stars expand the nebula, flow along the nebula's
walls, and cause waves of gas dust to collide. Atoms caught
in these colliding shocks radiate light; a spectacular display
of cloud like gases.
-Garrelt Mellema (Leiden University) et al. HST,
ESA, NASA
Did You Know?
The unusual jet emanating from the center of Galaxy M87 was
first
noticed early in the twentieth century. M87 is a giant elliptical
galaxy residing only 50 million light-years away in the Virgo
cluster
of galaxies. Faint dots surrounding M87's center are large,
ancient
globular clusters.
-J. A. Biretta et al., Hubble Heritage Team,
NASA
Did You Know?
Massive
stars end their lives in supernova explosions; small, low-mass
stars may, too. Instead of cooling off and quietly fading away,
some white dwarfs are thought to draw enough mass from their
companions to become unstable, triggering a nuclear detonation.
-J. Hughes & C. Rakowski (Rutgers University), et al., CXC,
NASA
Did You Know?
The planet Mercury resembles a moon. Dominated by an iron core,
however, it is much denser and more massive than a moon. Because
it rotates exactly three times every two orbits around the Sun,
and because its orbit is so elliptical, a visitor to Mercury
might see the Sun rise, stop in the sky, go back toward the
rising horizon, stop again, and then go quickly over the other
horizon.
-Mariner 10, NASA
Did You Know?
The planet Mercury resembles a moon. Dominated by an iron core,
however, it is much denser and more massive than a moon. Because
it rotates exactly three times every two orbits around the Sun,
and because its orbit is so elliptical, a visitor to Mercury
might see the Sun rise, stop in the sky, go back toward the
rising horizon, stop again, and then go quickly over the other
horizon.
-Mariner 10, NASA
Did You Know?
In order to find out the true ages of stars in neighboring Andromeda
Galaxy's halo, astronomers stared into the galactic giant with
the Hubble Space Telescope's Advanced Camera for Surveys. The
resulting exposure of over three days was the deepest ever taken
in visible light. The final image illuminated not only the Andromeda
but also the distant universe.
-T.M. Brown (STScl) et al., ESA, NASA
Did You Know?
The Martian crater Galle has internal markings reminiscent of
a smiley face symbol. Such markings were originally discovered
in the late 1970s in pictures taken by the orbiter Viking.
A large meteor impacted the Martian surface to form the crater.
Conventional wisdom holds that the markings inside the crater
are placed by chance by natural processes.
-Malin Space Science Systems, MSG, NASA
Did You Know?
Two images of the supernova remnant Cassiopeia A, taken a year
apart in infrared light, appear to show outward motion, Since
the supernova that created the nebula was seen 325 years ago,
the reason is likely light echoes. Light from the supernova
heated up distant ambient dust that is just beginning to show
its glow. As time goes by, more distant dust lights up, giving
the appearance of outward motion.
-O. Krause (Steward Observatory) et al. SSC,
JPL, Caltech, NASA
Did You Know?
The dark rippled dunes of Mars' Proctor Crater likely formed
more recently than lighter rock forms they appear to cover,
and are thought to slowly shift in response to pervasive winds.
The dunes arise from a complex relationship between the sandy
surface and high winds on Mars. Similar dunes were first seen
in Proctor Crater by Mariner 9 more than 35 years ago.
-NASA
Did You Know?
A small cone on the side of one of Mars' giant shield volcanoes
shows some layers of hard rock but most of it is made of relatively
soft material. This appears to be an example of a "cinder"
cone composed of pieces of lava thrown into the air during a
small volcanic eruption.
Typically,
such eruptions produce fountains of molten lava. Most of the
lava would have cooled in this fountain, producing a loose
pile of lava rocks. However, it appears that some pulses of
the eruption allowed the lava to land without cooling much.
These pieces were hot enough to weld together to make hard
layers seen today. The cone is about 2,300 x 3,600 feet, or
700 x 1,100 meters, in size, similar to many cinder cones
on Earth.
-NASA
Did You Know?
Whatever hit Mimas nearly destroyed it. What remains is one
of the largest impact craters on one of Saturn's smallest moons.
The crater, named Herschel after the 1789 discoverer of Mimas,
Sir William Herschel, spans about 130 kilometers and is pictured
above. Mimas' low mass produces a surface gravity just strong
enough to create a spherical body but weak enough to allow such
relatively large surface features. Mimas is made of mostly water
ice with a smattering of rock - so it is accurately described
as a big dirty snowball.
-Cassini Imaging Team, ISS, JPL, ESA, NASA
Did You Know?
The swirling eye of Hurricane Ivan, whose pwoerful winds reached
over 200 km per hour, was seen from the orbiting International
Space Station as it passed over the Caribbean in 2004.
-Expedtion 9 Crew, International Space Station,
NASA
Did You Know?
Scientists first saw somewhat wedge-shaped, transient clouds
of tiny particles known as "spokes" in images from
NASA's Voyager spacecraft. They dubbed these features in Saturn's
B ring "spokes" because they looked like bicycle spokes.
An electrostatic charge, the way static electricity on Earth
can raise the hair on your arms, appears to be levitating tiny
ring particles above the ring plane, but scientists are still
figuring out how the particles get that charge as they analyze
images from NASA's Cassini spacecraft.
-NASA
Single
Pane Glass Front $149
Fixed Bi-Fold Glass Door $149 Operable
Glass Doors $149
4 Pc. Black Trim Kit $89
4 Pc. SS Trim Kit $99
Thermostat $19
3-Stage Remote $85
Plug Kit $30Call
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39"
9200 BTU Insert Shown
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Shown w/ Fixed Single Pane Glass Front
39" Model# BF39DXP
38 3/4"W 32 3/4"H 15 1/3"D
Back: 36"W 26 3/5"H
Viewing Area: 36"W 22 4/5"H
Weight: 83 lbs.
Options: Single
Pane Glass Front $161 Fixed
Bi-Fold Glass Door $161 Operable Glass Doors $196
4 Pc. Black Trim Kit $87 4
Pc. SS Trim Kit
$103
Thermostat $19
3-Stage Remote $85
Plug Kit $30
Single
Pane Glass Front
$161 Fixed
Bi-Fold Glass Door $161 Operable
Glass Doors $196
4 Pc. Black Trim Kit $87 4
Pc. SS Trim Kit
$103
Thermostat $19
3-Stage Remote $85
Plug Kit $30
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45"
9200 BTU Insert
Shown w/ 4 Pc. SS Trim Kit
& Single Pane Glass Door 45"
Model# BF45DX
44 3/4"W 32 3/4"H 15 1/3"D
Back: 42"W 26 3/5"H
Viewing Area: 42"W 22 4/5"H
Weight: 90 lbs.
Single
Pane Glass Front$186 Fixed
Bi-Fold Glass Door $186 4
Pc. Black Trim Kit $103
4 Pc. SS Trim Kit $109
Thermostat $19
3-Stage Remote $85
Plug Kit $30Call
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Insert w/ Options
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Dimplex
Plug In Electric Fireplaces
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26" Dimplex 26"
Model# DF2608 27 3/8"W
23 1/2"H 9"D
Back: 26 1/3" W 22 5/8" H Weight:
55 lbs.