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Four Proplyds in the Orion Nebula (Hubble)

Four telescope images, at the center of each is a bright circular or oval-shaped object surrounded by a dark halo.

These are Hubble Space Telescope images of four protoplanetary disks around young stars in the Orion Nebula, approximately 1,300 light-years away. The disks range in size from two to eight times the diameter of our solar system. Astronomers spotted the disks in large-scale survey images of the Orion nebula taken with Hubble between January 1994 and March 1995.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    05h 35m 17.29s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    -5° 23' 27.99"
  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    The distance to the Orion Nebula is 1,500 light-years (460 parsecs).

About the Data

  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC2
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Orion Nebula, M42, NGC 1976
  • Object Description
    Object DescriptionThe type of astronomical object.
    Protoplanetary disks in the Orion Nebula
  • Release Date
    April 30, 2020
  • Science Release
    NASA’s Webb Telescope to Unravel Riddles of a Stellar Nursery
  • Credit
    Image: NASA, Mark McCaughrean (MPIA), C. O'Dell (Rice University)

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Four telescope images, at the center of each is a bright circular or oval-shaped object surrounded by a dark halo.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

Each picture is a composite of three images taken with Hubble's Wide Field and Planetary Camera 2, through narrow-band filters which admit the light of emission lines of ionized oxygen (represented here by blue), hydrogen (green), and nitrogen (red).

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Details

Last Updated
Aug 28, 2025
Contact
Media

Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov

Image Credit

NASA, Mark McCaughrean (MPIA), C. O’Dell (Rice University)