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IC 5148/5150 - a planetary nebula in the constellation Crane
(Grus) |
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Object description:
IC 5148 is a
beautiful planetary ring nebula at a distance of 4200 light years (GAIA
distance for the most central one). It is located in a relatively star-poor
region in the constellation Grus (the Crane). The nebula has a diameter of
several light-years and is expanding at over 50 kilometers per second, making
it one of the fastest growing planetary nebulae in the Milky Way.
In the
background lies a large field of very faint galaxies with magnitudes around the
18th and 19th magnitudes and distances ranging from 500 million to 2 billion
light-years, identifiable by a yellowish color.
The nebula, which
appears in almost monochromatic blue light, has 2 small reddish spots in the
northeast and in the southwest. The inner part is not completely dark, but
glows faintly in a diffuse light. Clearly visible in our image is the blue
central star with a magnitude 16.2 brightness. A high resolution image of IC
5148
shows an image of the ESO. |
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About the double naming 5148/5150
The nebula was
discovered on June 4, 1894 by the Australian amateur astronomer
W. F. Gale. Gale was actually a successful comet
observer, having discovered 7 comets himself. Gale first thought the nebulous
object was also an unknown comet, but after a few nights of observation it was
clear to him that this object must not be a comet, but - much rarer - a
planetary ring nebula. The Danish astronomer Johan Ludvig Emil Dreyer included
the object in 1908 with the catalog number IC 5150 in the 2nd index catalog.
3 years after Gale's discovery - on July 23, 1897 - the nebula was
independently observed by Lewis Swift from
California. Dreyer cataloged "Swift's object" as IC 5148. The reason for the
double entry in the IC catalog was the inaccurate position information of both
observers.
IC 5148/5150 has additionally the popular names Ghost Ring
Nebula and Spare Tire Nebula. A recent scientific study
can be found
here. |
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Click here or the thumbnail to load a large annoted image
and a size comparison to the full moon. |
The
comparison below shows to scale the apparent sizes of the planetary nebulae,
left: NGC 7293 (12.8 arcminutes), center: Messier 27 (5.8 arcminutes) and
right: IC 5148 (2.0 arcminutes). Total exposure time NGC 7293: 240 min, Messier
27: 130 min and IC 5148: 180 min. |
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