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Four Proplyds in the Orion Nebula (Hubble)

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. PositionR.A. PositionRight ascension – analogous to longitude – is one component of an object's position.05h 35m 17.29s
- Dec. PositionDec. PositionDeclination – analogous to latitude – is one component of an object's position.-5° 23' 27.99"
- DistanceDistanceThe 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
- InstrumentInstrumentThe science instrument used to produce the data.WFC2
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Orion Nebula, M42, NGC 1976
- Object DescriptionObject DescriptionThe type of astronomical object.Protoplanetary disks in the Orion Nebula
- Release DateApril 30, 2020
- Science ReleaseNASA’s Webb Telescope to Unravel Riddles of a Stellar Nursery
- CreditImage: NASA, Mark McCaughrean (MPIA), C. O'Dell (Rice University)

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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Laura Betz
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
laura.e.betz@nasa.gov
NASA, Mark McCaughrean (MPIA), C. O’Dell (Rice University)