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Astronomy Picture of the Day 8-21-03
NASA ^ | 8-21-03 | Robert Nemiroff and Jerry Bonnell

Posted on 08/20/2003 10:37:09 PM PDT by petuniasevan

Astronomy Picture of the Day

Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.

2003 August 21
See Explanation.  Clicking on the picture will download
 the highest resolution version available.

X-Rays from M17
Credit: L. Townsley (PSU) et al., CXC, NASA

Explanation: About 5,000 light-years away, toward the constellation Sagittarius and the center of our galaxy, lies the bright star forming region cataloged as M17. In visible light, M17's bowed and hollowed-out appearance has resulted in many popular names like the Horseshoe, Swan, Omega, and Lobster nebula. But what has sculpted this glowing gas cloud? This Chandra Observatory image of x-rays from M17 provides a clue. Many massive young stars are responsible for the pink central region of the false-color x-ray picture, their colliding stellar winds producing the multimillion degree gas cloud which extends ten or so light-years to the left. When compared with visible light images, this x-ray hot cloud is partly surrounded by the nebula's cooler gas. In fact, having carved out a central cavity the hot gas seems to be flowing out of the horseshoe shape like champagne from an uncorked bottle ... suggesting yet another name for star forming region M17.


TOPICS: Astronomy; Astronomy Picture of the Day; Science
KEYWORDS: chandra; m17; stars; xray

Smoothed Chandra Image of M17 without Point Sources

This version of Chandra's observation of M17 has been processed to emphasize
the diffuse emission in the cluster. In this image, the point sources have been
removed and then the pixels have been slightly blurred, or smoothed, together.
Red represents lower energy X-rays (0.5-2 keV) and blue shows a higher range of
X-rays (2-7 keV).

Scale:
Image is approx. 17 arcmin per side
(Credit: NASA/CXC/PSU/L.Townsley et al.)


Chandra & Hubble Comparison of M17

The image on the right shows M17 in visible light as
observed by the Hubble Space Telescope compared with
Chandra's larger field of view on the left. Using the
Advanced Camera for Survey instrument (ACS), Hubble
observed M17 for 2.6 hours on April 1-2, 2002.

Scale: Left: 17 arcmin per side; Right: 2.5 arcmin per side
(Credit: X-ray: NASA/CXC/PSU/L.Townsley et al.; Optical: NASA/STScI/ESA)


2MASS Infrared Image of M17

This infrared image of M17 from the 2MASS project
penetrates the the dust in this nebular to reveal
the otherwise invisible dark molecular cloud.
This giant molecular cloud (a cold, dense interstellar cloud which
contains a high fraction of molecules) is one of the most luminous and
active star-forming regions in the Milky Way. Although the gas in the
molecular cloud is too cold to emit visible or near-infrared light, traces of
the densest portions of the cloud can still be seen as dark, cloudy structures.

Scale: Left: 17 arcmin per side; Right: 60 arcmin per side
(Credit: 2MASS/UMass/IPAC-Caltech/NASA/NSF)

Note: 2MASS refers the 2 Micron All Sky Survey.


DSS Optical Image of M17

The Digital Sky Survey (DSS) image reveals an irregular
shaped cloud of illuminated gas, with darker superimposed regions.
The obscured areas are due to dust grains located in the foreground of the nebula.
Even the obscured regions are not completely dark, suggesting that the stars are either in the foreground
or are in the outer fringes of the dusty regions and are bright enough to be seen through the haze.
This optical image covers the same region of sky as the Chandra data.

Scale: Image is approx. 17 arcmin per side
(Credit: Palomar Observatory DSS)


VLA Radio Image of M17

The radio image of M17 depicts the distribution of ionized hydrogen
(hydrogen atoms with their electrons stripped away) in what astronomers refer to as "H II regions".
The missing electrons are the result of collisions with other atoms and/or radiation from nearby stars.
H II regions are the signposts for active star formation.
The radio image covers the same region of sky as the Chandra data.

Scale: 17 arcmin per side
(Credit: NRAO/AUI)



M17 in Sagittarius

Right Ascension 18 : 20.8 (h:m)
Declination -16 : 11 (deg:m)
Distance 5.0 (kly)
Visual Brightness 6.0 (mag)
Apparent Dimension 11.0 (arc min)

Here's a nice amateur photo of M17.

Finder chart:


1 posted on 08/20/2003 10:37:10 PM PDT by petuniasevan
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To: MozartLover; Joan912; NovemberCharlie; snowfox; Dawgsquat; viligantcitizen; theDentist; ...

2 posted on 08/20/2003 10:44:07 PM PDT by petuniasevan (Beer nuts are $1.39. Deer nuts are under a buck.)
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To: petuniasevan
A wealth of information! Thank you.
3 posted on 08/21/2003 6:57:59 AM PDT by foolish-one
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