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Hubble Space Telescope Images of a Bright Star in the Large Magellanic Cloud

Hubble Space Telescope Images of a Bright Star in the Large Magellanic Cloud

The three panels show images of a very bright (Wolf-Rayet) star, Melnick 34, located in the giant star-forming region called 30 Doradus in the Large Magellanic Cloud. In the background are a number of fainter stars that are comparable in brightness to our Sun.

[Left] Ground Based View

The best available ground-based image of Melnick 34 (Courtesy Dr. Georges Meylan of the European Southern Observatory). This image was taken under ideal atmospheric conditions when the width of a star image was about 0.6 arc seconds.

[Middle] WF/PC-1 Image

The same field, as imaged by the first Wide Field and Planetary Camera (WF/PC-). The advantages of working in space above Earth's distorting atmosphere are immediately apparent. Atmospheric blurring is gone and many more stars are visible. However, the effects of the Hubble Telescope's spherical aberration also are apparent. In particular there is a four arc second diameter "skirt" around the bright star which obscures the view of the sky in its vicinity. It is very hard to do quantitative measurements on such an image because of the way the light from many stars overlaps.

[Right] WFPC-2 Image

An image of the same field, made with the new Wide Field and Planetary Camera's (WFPC-2) improved optics. With an exposure equivalent to the WF/PC-1 image, this WFPC-2 image collects all the light from the central star into sharp focus because the telescope's spherical aberration is corrected by the new camera's optics. A large number of fainter stars also become visible. This is because all of their light is concentrated, and enough is gathered to make them visible above the intrinsic noise from the instrument and sky. In the WF/PC-1 image, enough light is distributed in the image "skirt that background stars become lost in the noise. In WFPC-2, not only are the fainter stars visible, but quantitative measurements of their brightness also are possible.

By facilitating quantitative measurements in faint and crowded star fields, the Wide Field and Planetary Camera-2 and the Hubble Space Telescope will be able to address all the key programs for which the telescope and instrument were originally designed.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    05h 38m 42.39s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -69° 6' 2.81"
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Melnick 34, 30 Doradus
  • Release Date
    January 13, 1994
  • Science Release
    Hubble Space Telescope Images of a Bright Star in the Large Magellanic Cloud
  • Credit
    Science Release Credit: STScI and NASA

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Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov