|
Collection:
|
|
NASA Marshall Space Flight Center Collection
Collection
NASA Marshall Space Flight Center Collection
Collection
|
|
Name of Image:
|
|
Chandra X-Ray Observatory Image of Black Hole
Name_of_Image
Chandra X-Ray Observatory Image of Black Hole
Name of Image
|
|
Full Description:
|
|
This Chandra X-Ray Observatory (CXO) image is a spectrum of a black hole, which is similar to the colorful spectrum of sunlight produced by a prism. The x-rays of interest are shown here recorded in bright stripes that run rightward and leftward from the center of the image. These x-rays are sorted precisely according to their energy with the highest-energy x-rays near the center of the image and the lower-energy x-rays farther out. The spectrum was obtained by using the Low Energy Transmission Grating (LETG), which intercepts x-rays and changes their direction by the amounts that depend sensitively on the x-ray energy. The assembly holds 540 gold transmission gratings. When in place behind the mirrors, the gratings intercept the x-rays reflected from the telescope. The bright spot at the center is due to a fraction of the x-ray radiation that is not deflected by the LETG. The spokes that intersect the central spot and the faint diagonal rays that flank the spectrum itself are artifacts due to the structure that supports the LETG grating elements. (Photo credit: NASA Cfa/J. McClintock et al)
Full_Description
This Chandra X-Ray Observatory (CXO) image is a spectrum of a black hole, which is similar to the colorful spectrum of sunlight produced by a prism. The x-rays of interest are shown here recorded in bright stripes that run rightward and leftward from the center of the image. These x-rays are sorted precisely according to their energy with the highest-energy x-rays near the center of the image and the lower-energy x-rays farther out. The spectrum was obtained by using the Low Energy Transmission Grating (LETG), which intercepts x-rays and changes their direction by the amounts that depend sensitively on the x-ray energy. The assembly holds 540 gold transmission gratings. When in place behind the mirrors, the gratings intercept the x-rays reflected from the telescope. The bright spot at the center is due to a fraction of the x-ray radiation that is not deflected by the LETG. The spokes that intersect the central spot and the faint diagonal rays that flank the spectrum itself are artifacts due to the structure that supports the LETG grating elements. (Photo credit: NASA Cfa/J. McClintock et al)
Full Description
|
|
Date of Image:
|
|
2000-04-01
Date_of_Image
2000-04-01
Date of Image
|
|
Category:
|
|
History of Chandra X-Ray Observatory
Category
History of Chandra X-Ray Observatory
Category
|
|
term:
|
|
Chandra X-Ray Observatory
Keywords
Chandra X-Ray Observatory
term
|
|
term:
|
|
CXO
|
|
term:
|
|
Spectrum
|
|
term:
|
|
Black Hole
|
|
facet_what:
|
|
Chandra X-Ray Observatory (CXO)
facet_what
Chandra X-Ray Observatory (CXO)
facet_what
|
|
facet_where:
|
|
Marshall Space Flight Center (MSFC)
facet_where
Marshall Space Flight Center (MSFC)
facet_where
|
|
Reference Number:
|
|
MSFC-75-SA-4105-2C
Reference_Number
MSFC-75-SA-4105-2C
Reference Number
|
|
MIX #:
|
|
0200206
|
|
NIX #:
|
|
MSFC-0200206
|
|
MSFC Negative Number:
|
|
0200206
MSFC_Negative_Number
0200206
MSFC Negative Number
|
|
UID:
|
|
SPD-MARSH-0200206
UID
SPD-MARSH-0200206
UID
|
|
original url:
|
original_url
original url
|