Cool Space Pics

Oct 28, 2005
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Hails!! \m/

Post some of yarr cool space pics, here's one came in about 30 minutes ago, just released....
from http://scm.x.am :headbang:
Mountains_spitzer_f20.jpg

http://antwrp.gsfc.nasa.gov/apod/ap051111.html
Mountains of Creation
Credit: Lori Allen (Harvard-Smithsonian CfA) et al., JPL-Caltech, NASA
Explanation: This fantastic skyscape lies at the eastern edge of giant stellar nursery W5, about 7,000 light-years away in the constellation Cassiopeia. An infrared view from the Spitzer Space Telescope, it features interstellar clouds of cold gas and dust sculpted by winds and radiation from a hot, massive star outside the picture (just above and to the right). Still swaddled within the cosmic clouds, newborn stars are revealed by Spitzer's penetrating gaze, their formation also triggered by the massive star. Fittingly dubbed "Mountains of Creation", these interstellar clouds are about 10 times the size of the analogous Pillars of Creation in M16, made famous in a 1995 Hubble Space Telescope view. W5 is also known as IC 1848 and together with IC 1805 it is part of a complex region popularly dubbed the Heart and Soul Nebulae. The Spitzer image spans about 70 light-years at the distance of W5.


And here's the two best ones, so far, from the other metal forum threads:
This is the galaxy that our Milky Way Galaxy is colliding with, which is estimated to consume Earth and our solar system in about 5 000 000 000 years or so, released today from NASA & @ http://scm.x.am:
R1D1 said:
Three Faces of Andromeda
http://www.spitzer.caltech.edu/Media/releases/ssc2005-20/ssc2005-20a.shtml
ssc2005-20a_medium.jpg

Credit: NASA/JPL-Caltech/K. Gordon (University of Arizona)

NASA's Spitzer Space Telescope has captured stunning infrared views of the famous Andromeda galaxy to reveal insights that were only hinted at in visible light.

Spitzer's 24-micron mosaic (top panel) is the sharpest image ever taken of the dust in another spiral galaxy. This is possible because Andromeda is a close neighbor to the Milky Way at a mere 2.5 million light-years away.

The Spitzer multiband imaging photometer's 24-micron detector recorded 11,000 separate snapshots to create this new comprehensive picture. Asymmetrical features are seen in the prominent ring of star formation. The ring appears to be split into two pieces, forming the hole to the lower right. These features may have been caused by interactions with satellite galaxies around Andromeda as they plunge through its disk.

Spitzer also reveals delicate tracings of spiral arms within this ring that reach into the very center of the galaxy. One sees a scattering of stars within Andromeda, but only select stars that are wrapped in envelopes of dust light up at infrared wavelengths.

This is a dramatic contrast to the traditional view at visible wavelengths (lower left panel), which shows the starlight instead of the dust. The center of the galaxy in this view is dominated by a large bulge that overwhelms the inner spirals seen in dust. The dust lanes are faintly visible in places, but only where they can be seen in silhouette against background stars.

The multi-wavelength view of Andromeda (lower right panel) combines images taken at 24 microns (blue), 70 microns (green), and 160 microns (red). Using all three bands from the multiband imaging photometer allows astronomers to measure the temperature of the dust by its color. The warmest dust is brightest at 24 microns while the coolest is most evident at 160 microns. The blue/white areas have the hottest dust, as seen in the bulge and in the star-forming areas along the arms. The cooler dust floating further out in the ring and arms are in the redder regions.

The data were taken on August 25, 2004, the one-year anniversary of the launch of the space telescope. The observations have been transformed into this remarkable gift from Spitzer -- the most detailed infrared image of the spectacular galaxy to date.

About the Object Object Name: Andromeda Galaxy (M31)
Object Type: spiral galaxy
Position (J2000): RA: 00h42m44.3s Dec: +41d16m09s
Distance: 780,000 pc; 2.5 million light-years
Constellation: Andromeda
About the Data Image Credit:
NASA/JPL-Caltech/K. Gordon (University of Arizona)
Instrument: MIPS
Wavelength:
24 microns (pseudocolor); also 24 microns (blue), 70 microns (green), and 160 microns (red)
Exposure Date:
2004 August 25
Exposure Time:
100 sec/pixel (24 microns), 40 sec/pixel (70 microns), 9 sec/pixel (160 microns)
Image Scale: 2.8 x 0.8 degrees
Orientation: North is 53 deg CCW from up
Release Date: October 13, 2005
Observers Karl D. Gordon (University of Arizona)
Jeremy Bailin (Swinburne University of Technology, Australia)
Charles W. Engelbracht (University of Arizona)
George H. Rieke (University of Arizona)
Karl A. Misselt (University of Arizona)
William B. Latter (SSC/Caltech)
E. T. Young (University of Arizona)
Deborah A. Levine (SSC/Caltech)
M. W. Werner (JPL)
Pauline Barmby (Harvard-Smithsonian Center for Astrophysics)
Brad K. Gibson (Swinburne University of Technology, Australia)
Joannah Hinz (University of Arizona)
Susan Stolovy (SSC/Caltech)


LINK TO ULTRA MASSIVE VERSION:
http://ipac.jpl.nasa.gov/media_images/ssc2005-20a.jpg

LINK TO ULTRA MASSIVE VERSION TOP IMAGE:
http://ipac.jpl.nasa.gov/media_images/ssc2005-20a1.jpg

LINK TO ULTRA MASSIVE VERSION BOTTOM LEFT IMAGE:
http://ipac.jpl.nasa.gov/media_images/ssc2005-20a3.jpg

LINK TO ULTRA MASSIVE VERSION BOTTOM RIGHT:
http://ipac.jpl.nasa.gov/media_images/ssc2005-20a2.jpg

Click here for more information & interviews:
http://www.spitzer.caltech.edu/Media/releases/ssc2005-20/moreinfo.shtml

Click here for SCM full NASA Jet Propulsion Laboratory Official Press Release:
http://scm.11.forumer.com/viewtopic.php?p=5187#5187

&

Another dousy!! \m/
From The Space Colonization Movement http://scm.x.am
PIC: First Galactic Look ~ Galaxy 891
051027_iod_firstlight_04.jpg

http://www.space.com/imageoftheday/image_of_day_051027.html
First Galactic Look

The Large Binocular Telescope (LBT) opened its eyes on this galaxy, NGC 891, during its “first light” operations this month.

NGC 891 sits about 24 million light-years from Earth towards the constellation Andromeda.

“We admit that we picked NGC 891 because we find it to be a very attractive galaxy,” LBT astronomers said. “However, NGC891 is of particular scientific interest because the galaxy-wide burst of star formation inferred from X-ray emission is stirring up the gas and dust in its disk, resulting in filaments of obscuring dust extending vertically for hundreds of light-years.”

The $120 million LBT instrument consists of two, 27.6-foot (8.4 meter) mirrors, set inside an observatory atop Mount Graham in southeastern Arizona.

Astronomers used the telescope to capture this view of NGC 891 on Oct. 12, 2005 using a blue filter and 10, 30-second exposures. The telescope should begin full-up operations in 2006.

-- SPACE.com Staff

Credit: Large Binocular Telescope Observatory.


Post your thoughts!! Add some too!! Slay on.... \m/
 
Glad yous dig em :headbang:
BasilisK 3 7 77 said:
Good stuff. Too bad no good space pics work as 100x100 avatars (or whatever the limit is here).
Actually, if you get a free photobucket at www.photobucket.com you can use that to host and resize it to fit. I been with them for a year or two, and have found no better free image hoster anywheres...
I host my avatars with em too, and smileys, picks, banners, and whatever else. Check it out \m/
 
Yea, I use Photobucket to host my avatar and sig banner too. Resizing images though always makes them come out totally fucked up and no longer worth using... If it's like 150x150 or maybe even 200x200 it might be usable, but anything bigger or not near-perfectly square always get too distorted.
 
BasilisK 3 7 77 said:
Yea, I use Photobucket to host my avatar and sig banner too. Resizing images though always makes them come out totally fucked up and no longer worth using... If it's like 150x150 or maybe even 200x200 it might be usable, but anything bigger or not near-perfectly square always get too distorted.
That's funny, I was thinking the exact opposite thing!
 
Thor's Helmet Nebula!!!!!!!
from http://scm.x.am moving over to http://megaweb.x.am
\m/
ngc2359_smith.jpg

http://antwrp.gsfc.nasa.gov/apod/ap051119.html
NGC 2359: Thor's Helmet
Credit: Christine and David Smith, Steve Mandel, Adam Block (KPNO Visitor Program), NOAO, AURA, NSF
Explanation: NGC 2359 is a striking emission nebula with an impressive popular name - Thor's Helmet. Sure, its suggestive winged appearance might lead some to refer to it as the "duck nebula", but if you were a nebula which name would you choose? By any name NGC 2359 is a bubble-like nebula some 30 light-years across, blown by energetic winds from an extremely hot star seen near the center and classified as a Wolf-Rayet star. Wolf-Rayet stars are rare massive blue giants which develop stellar winds with speeds of millions of kilometers per hour. Interactions with a nearby large molecular cloud are thought to have contributed to this nebula's more complex shape and curved bow-shock structures. NGC 2359 is about 15,000 light-years distant toward the constellation Canis Major.

:Smokedev:
 
I can see the helmet shap and eyes.......butI keep seeing a giant clown nose and smile to lol
 
It should either be a clown or that Disney elephant. Norse helmets didn't have horns, or wings. You'd figure people who base their research around pure fact would factor that in. Just a little pet-peev of mine.
 
The Bringer said:
Those are fucking incredible. I love looking at space. If I could afford it, I'd buy a high-powered telescope too.


it would be so cool to get a high-powered telescope,it gets dark here at 16.00 so i would have time to look:Spin:
 
These two are both METAL!!!!!!!
icon_twisted.gif
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Erebus = The Amenta song
Sirius B = Therion song & CD
They can be found @ the new Megaweb, with the Space Colonization Movement, Metal Mega, and more....
http://megaweb.x.am
Both released in the last week or so...
\m/

PIA03622.jpg

http://www.jpl.nasa.gov/missions/mer/images.cfm?id=1835
Rim of 'Erebus'
12/5/05
The center upper portion of this image shows a portion of the rim of "Erebus Crater" in the Meridiani Planum region of Mars. This approximately true-color view from the panoramic camera on NASA's Mars Exploration Rover Opportunity is a composite of frames acquired on the rover's 657th Martian day, or sol, (Nov. 28, 2005). This is a small portion of a large panorama. Other portions of the panorama were still being shot three sols later. This view is a composite of separate images taken through the camera's 750-nanometer, 530-nanometer and 430-nanometer filters.

Image Credit: NASA/JPL-Caltech/Cornell


web_print.jpg

http://hubblesite.org/newscenter/newsdesk/archive/releases/2005/36/image/a
The Dog Star, Sirius, and its Tiny Companion


STScI-PRC2005-36a


This Hubble Space Telescope image shows Sirius A, the brightest star in our nighttime sky, along with its faint, tiny stellar companion, Sirius B. Astronomers overexposed the image of Sirius A [at center] so that the dim Sirius B [tiny dot at lower left] could be seen. The cross-shaped diffraction spikes and concentric rings around Sirius A, and the small ring around Sirius B, are artifacts produced within the telescope's imaging system. The two stars revolve around each other every 50 years. Sirius A, only 8.6 light-years from Earth, is the fifth closest star system known.

Sirius B, a white dwarf, is very faint because of its tiny size, only 7,500 miles in diameter. White dwarfs are the leftover remnants of stars similar to our Sun. They have exhausted their nuclear fuel sources and have collapsed down to a very small size. Sirius B is about 10,000 times fainter than Sirius A. The white dwarf's feeble light makes it a challenge to study, because its light is swamped in the glare of its brighter companion as seen from telescopes on Earth. However, using the keen eye of Hubble's Space Telescope Imaging Spectrograph (STIS), astronomers have now been able to isolate the light from Sirius B and disperse it into a spectrum. STIS measured light from Sirius B being stretched to longer, redder wavelengths due to the white dwarf's powerful gravitational pull. Based on those measurements, astronomers have calculated Sirius B's mass at 98 percent that of our Sun. Analysis of the white dwarf's spectrum also has allowed astronomers to refine the estimate for its surface temperature to about 44,900 degrees Fahrenheit (25,200 degrees Kelvin).

Accurately determining the masses of white dwarfs is fundamentally important to understanding stellar evolution. Our Sun will eventually become a white dwarf. White dwarfs are also the source of Type Ia supernova explosions, which are used to measure cosmological distances and the expansion rate of the universe. Measurements based on Type Ia supernovae are fundamental to understanding "dark energy," a dominant repulsive force stretching the universe apart. Also, the method used to determine the white dwarf's mass relies on one of the key predictions of Einstein's theory of General Relativity: that light loses energy when it attempts to escape the gravity of a compact star.

This image was taken Oct. 15, 2003, with Hubble's Wide Field Planetary Camera 2. Based on detailed measurements of the position of Sirius B in this image, astronomers were then able to point the STIS instrument exactly on the white dwarf and make the measurements to determine its gravitational redshift and mass.

Credit: NASA, H.E. Bond and E. Nelan (Space Telescope Science Institute, Baltimore, Md.); M. Barstow and M. Burleigh (University of Leicester, U.K.); and J.B. Holberg (University of Arizona)

Image Type: Astronomical
STScI-PRC2005-36a

SEE FULL RELEASE: http://megaweb.10.forumer.com/viewtopic.php?t=3215
 
Here's a real cool one just out today, new version of the Helix Nebula.. Looks like a grim eye... hehehe
From the Space Colonization Movement @ http://megaweb.x.am where Metal Mega is too now...
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060109_iod_helix_04.jpg

http://www.space.com/imageoftheday/image_of_day_060109.html
The Helix Nebula's New Look



The Helix Nebula gets a new look in this Spitzer Space Telescope view released today.



This image, released today at the 207th meeting of the American Astronomical Society in Washington D.C., offers a new portrait of the Helix Nebula.



While named after its apparent coil structure, previous studies have shown it consists of two vast disks of gas arranged almost perpendicular to each other. The Helix Nebula sits about 650 light-years from Earth toward the constellation Aquarius.



The space-based Spitzer telescope shows phenomena known as “cometary knots,” thousands of lumpy blobs which – like comets – appear to have heads and long tails. Each knot, however, is much larger than an actual comet, with masses comparable to Earth and sizes about twice that of the Solar System.



In Spitzer’s new view, the cometary knots appear with blue-green heads and reddish tails. The blue hue is due to molecular hydrogen excited by ultraviolet radiation from stellar wind or the nebula’s central star, while the reddish tails indicate they have been relatively shielded due to their position behind the main body of knots



The image also details a trend for the Helix Nebula to become redder the farther out from its central star. The entire arrangement is constantly changing due to its hot stellar core, which will eventually destroy the eye-pleasing nebula.



-- SPACE.com Staff



Credit: NASA/JPL/CfA