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1 posted on 08/21/2006 6:13:31 PM PDT by vikingd00d
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To: vikingd00d

"They said as they looked down their noses and chuckled softly".


2 posted on 08/21/2006 6:18:23 PM PDT by muawiyah
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To: vikingd00d
...but then learned it was only Chocolate City!


3 posted on 08/21/2006 6:19:10 PM PDT by TexasCajun
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To: vikingd00d; SunkenCiv

direct evidence?


4 posted on 08/21/2006 6:19:21 PM PDT by GeronL (flogerloon.blogspot.com -------------> Rise of the Hate Party)
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To: vikingd00d
NASA Finds Direct Proof of Dark Matter

How did they find it? CAT scans of Howard Dean, Al Gore, and Michael More?

5 posted on 08/21/2006 6:23:08 PM PDT by ConservaTexan (February 6, 1911)
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To: vikingd00d

6 posted on 08/21/2006 6:24:31 PM PDT by My2Cents (A pirate's life for me.)
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To: vikingd00d

1E 0657-56: NASA Finds Direct Proof of Dark Matter

1E 0657-56
Credit: X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.; Lensing Map: NASA/STScI; ESO WFI; Magellan/U.Arizona/D.Clowe et al.

JPEG (479 kb) Tiff (9.2 MB) PS (2.8 MB)

This composite image shows the galaxy cluster 1E 0657-56, also known as the "bullet cluster." This cluster was formed after the collision of two large clusters of galaxies, the most energetic event known in the universe since the Big Bang.

Lensing Illustration
Gravitational Lensing Explanation
Hot gas detected by Chandra in X-rays is seen as two pink clumps in the image and contains most of the "normal," or baryonic, matter in the two clusters. The bullet-shaped clump on the right is the hot gas from one cluster, which passed through the hot gas from the other larger cluster during the collision. An optical image from Magellan and the Hubble Space Telescope shows the galaxies in orange and white. The blue areas in this image show where astronomers find most of the mass in the clusters. The concentration of mass is determined using the effect of so-called gravitational lensing, where light from the distant objects is distorted by intervening matter. Most of the matter in the clusters (blue) is clearly separate from the normal matter (pink), giving direct evidence that nearly all of the matter in the clusters is dark.

Animation of Cluster Collision
Animation of Cluster Collision
The hot gas in each cluster was slowed by a drag force, similar to air resistance, during the collision. In contrast, the dark matter was not slowed by the impact because it does not interact directly with itself or the gas except through gravity. Therefore, during the collision the dark matter clumps from the two clusters moved ahead of the hot gas, producing the separation of the dark and normal matter seen in the image. If hot gas was the most massive component in the clusters, as proposed by alternative theories of gravity, such an effect would not be seen. Instead, this result shows that dark matter is required.

Fast Facts for 1E 0657-56:
Credit  X-ray: NASA/CXC/CfA/M.Markevitch et al.; Optical: NASA/STScI; Magellan/U.Arizona/D.Clowe et al.; Lensing Map: NASA/STScI; ESO WFI; Magellan/U.Arizona/D.Clowe et al.
Scale  Image is 7.5 x 5.4 arcmin
Category  Groups & Clusters of Galaxies
Coordinates (J2000)  RA 06h 58m 19.85s | Dec -55' 56" 29.40º
Constellation  Carina
Observation Dates  2004: Aug 10, 11, 14, 15, 17, 19, 24, 25
Observation Time  140 hours
Obs. IDs  5355-58, 5361, 4984-86
Color Code  Energy (X-ray: Pink; Optical: White/Orange; Lensing Map: Blue)
Instrument  ACIS
Also Known As  The Bullet Cluster
Distance Estimate  About 3.4 billion light years
Release Date  August 21, 2006

More Information on 1E 0657-56:
Press Room: 1E 0657-56 Press Release
More Images of 1E 0657-56
1E 0657-56 Animations
1E 0657-56 Handout: html | pdf
Zoom in on 1E 0657-56 (flash)
Chandra Chronicles: Bedeviling Devil's Advocate Cosmology
Q&A: Astrophysicist Maxim Markevitch on Dark Matter
Powerpoint and PDF
Download image for your desktop
Related Chandra Images:
Photo Album: Abell 2029 (11 Jun 03)
Photo Album: NGC 720 (22 Oct 02)
Photo Album: 1E 0657-56 (20 Feb 02)
Photo Album: EMSS 1358+6245 (06 Sep 01)
More Information on Groups & Clusters of Galaxies:
X-ray Astronomy Field Guide: Groups & Clusters of Galaxies
Questions and Answers: Groups & Clusters of Galaxies
Chandra Images: Groups & Clusters of Galaxies


Chandra Images: ' 06 | ' 05 | ' 04 | ' 03 | ' 02 | ' 01 | ' 00 | ' 99 | Images by Category


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  [News by email: Chandra Digest]
[Contact us: cxcpub@cfa.harvard.edu]
NASA's Home Page Smithsonian's Home Page CXC Home Page Image Map for NASA's, Smithsonian and Chandra's Home Pages
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Phone: 617.496.7941 Fax: 617.495.7356


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Operated for NASA by SAO
This site was developed with funding from NASA under Contract NAS8-39073.
Revised: August 21, 2006

7 posted on 08/21/2006 6:27:23 PM PDT by Mark Felton ("Your faith should not be in the wisdom of men, but in the power of God.")
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To: vikingd00d

Good post!


10 posted on 08/21/2006 6:34:04 PM PDT by Coyoteman (I love the sound of beta decay in the morning!)
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To: vikingd00d

"We've closed this loophole about gravity, and we've come closer than ever to seeing this invisible matter," Clowe said.



I would not bet my inheritance on that.


15 posted on 08/21/2006 6:51:05 PM PDT by Brilliant
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To: vikingd00d

If an inch represents the difference in the knowledge of Kepler and Galileo and todays observers, then a miles represents how much more knowledge there must be before we begin to explain it all. We may never travel that mile.


24 posted on 08/21/2006 6:55:15 PM PDT by RobbyS ( CHIRHO)
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To: betty boop; Alamo-Girl; cornelis

Hmmmm... Light matter/energy vs. dark matter/energy...


29 posted on 08/21/2006 7:01:25 PM PDT by hosepipe (CAUTION: This propaganda is laced with hyperbole.)
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To: vikingd00d

BuMpiTy, BuMp, BuMp, ...BOOM!


32 posted on 08/21/2006 7:07:29 PM PDT by spunkets
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To: vikingd00d
collision of two large clusters of galaxies

If the universe is expanding (Big Bang) how could clusters COLLIDE, let alone how could GALAXIES that have been blown apart, collide? Hmmmm...
36 posted on 08/21/2006 7:28:47 PM PDT by true_blue_texican
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To: vikingd00d

All I know is that there is a bin for the dark matter, one for the gray matter and one for the white matter. If I mix 'em up, she won't do the laundry 'til I fix it.


46 posted on 08/21/2006 8:26:35 PM PDT by REDWOOD99
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To: vikingd00d

Watch out for the "Crazy Eddie Probe".....


47 posted on 08/21/2006 8:28:23 PM PDT by Empireoftheatom48 (God bless our troops!! Our President and those who fight against the awful commie, liberal left!!)
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To: vikingd00d

49 posted on 08/21/2006 8:33:30 PM PDT by CurlyBill (Democratic Party Agenda ------> Emasculate America)
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To: vikingd00d
Now if they can only find
"What's the matter?"
when talking to their wife/girlfriend.

Then they would really be on to something.

51 posted on 08/21/2006 8:41:30 PM PDT by Boiler Plate (Mom always said why be difficult, when with just a little more effort you can be impossible.)
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To: vikingd00d

Ping for later


53 posted on 08/21/2006 8:58:51 PM PDT by Bender2 (Gad! The inmates have control... And I'm trying to quit smoking!)
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To: GeronL; Swordmaker; FairOpinion

Ditching Dark Matter
The Guardian | Thursday February 13, 2003 | Marcus Chown
Posted on 02/15/2003 10:40:45 AM EST by Phaedrus
http://www.freerepublic.com/focus/f-news/844020/posts


59 posted on 08/21/2006 10:06:20 PM PDT by SunkenCiv (updated my FR profile on Thursday, August 10, 2006. https://secure.freerepublic.com/donate/)
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ET type IV civilization moves a pulsar from our Galaxy to another
India Daily | Aug. 20, 2006 | India Daily Technology Team
Posted on 08/21/2006 12:12:20 PM EDT by SunkenCiv
http://www.freerepublic.com/focus/f-chat/1687423/posts


60 posted on 08/21/2006 10:12:27 PM PDT by SunkenCiv (updated my FR profile on Thursday, August 10, 2006. https://secure.freerepublic.com/donate/)
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To: vikingd00d
The concentration of mass is determined using the effect of so-called gravitational lensing, where light from the distant objects is distorted by intervening matter.

If dark matter only interacts through gravity, what is the light coming from to determine where the dark matter is located?

Sounds like there are still research opportunities here.

82 posted on 08/22/2006 9:26:34 AM PDT by <1/1,000,000th%
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