File:The Eagle Nebula M16 Peering Into the Pillars Of Creation.jpg

From Wikipedia, the free encyclopedia

Original file(2,400 × 2,361 pixels, file size: 582 KB, MIME type: image/jpeg)

Summary[edit]

File information
Description

A new look at the famous "Pillars of Creation" with NASA's Chandra X-ray Observatory has allowed astronomers to peer inside the dark columns of gas and dust. This penetrating view of the central region of the Eagle Nebula reveals how much star formation is happening inside these iconic structures.


Different Views of the Eagle Nebula (M16) The Chandra data shows bright X-ray sources in this field, most of which are young stars. In this image, red, green, and blue represent low, medium, and high energy X-rays. The Chandra data have been overlaid on the Hubble Space Telescope image to show the context of these X-ray data.

Very few X-ray sources are found in the pillars themselves. This suggests that the Eagle Nebula may be past its star-forming prime, since young stars are usually bright X-ray sources. However, there are two X-ray objects found near the tips of the pillars. One is a young star about 4 or 5 times as massive as the Sun, visible as the blue source near the tip of the pillar on the left. The other is a lower mass star near the top of the other pillar that is so faint it is not visible in the composite image.

Source

X-ray: NASA/CXC/U.Colorado/Linsky et al.; Optical: NASA/ESA/STScI/ASU/J.Hester & P.Scowen.

Date
Author
Permission
(Reusing this file)

See below.



Licensing[edit]


File history

Click on a date/time to view the file as it appeared at that time.

Date/TimeThumbnailDimensionsUserComment
current17:18, 18 December 2007Thumbnail for version as of 17:18, 18 December 20072,400 × 2,361 (582 KB)Mpozzan (talk | contribs)X-ray: NASA/CXC/U.Colorado/Linsky et al.; Optical: NASA/ESA/STScI/ASU/J.Hester & P.Scowen.
No pages on the English Wikipedia use this file (pages on other projects are not listed).

Metadata