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Gap in Stellar Dust Disk May Be Swept Out By Planet

Gap in Stellar Dust Disk May Be Swept Out By Planet
A striking NASA Hubble Space Telescope near-infrared picture of a disk around the star HD 141569, located about 320 light-years away in the constellation Libra. Hubble shows that the 75 billion-mile wide disk seems to come in two parts: a dark band separates a bright inner region from a fainter outer region. The structure superficially looks much like the largest gap in Saturn's rings - but on a vastly larger scale. The Hubble image, taken at a wavelength of 1.1 microns, was made using the coronagraph in the Near Infrared and Multi-Object Spectrometer (NICMOS) to reduce the glare of the star. The observed radiation from the disk is caused by dust particles which reflect the light of the central star. The dark spikes in the image are regions where there are no useful data due to diffraction artifacts introduced by the optical systems of the telescope and camera. The central portion of the disk remains unseen because of residual glare from the bright star.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    15h 49m 57.74s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -3° 55' 16.35"
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    HD 141569
  • Release Date
    January 8, 1999
  • Science Release
    Hubble Views of Dust Disks and Rings Surrounding Young Stars Yield Clues
  • Credit
    Credit: Alycia Weinberger, Eric Becklin (UCLA), Glenn Schneider (University of Arizona) and NASA

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Details

Last Updated
Mar 28, 2025
Contact
Media

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