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LRLL 54361 Light Echo – Hubble

LRLL 54361 Light Echo – Hubble

This sequence of images from the Hubble Space Telescope shows a pulse of light emanating from the protostellar object LRLL 54361. Most if not all of this light results from scattering off circumstellar dust in the protostellar envelope.

An apparent edge-on disk visible at the center of the object and three separate structures are interpreted as outflow cavities. The extent and shape of the scattered light changes substantially over a 25.34-day period.

This is caused by the propagation of the light pulse through the nebula. Astronomers propose that the flashes are due to material in a circumstellar disk suddenly being dumped onto a binary pair of forming stars. This unleashes a blast of radiation each time the stars get close to each other in their orbit.

These false color, near-infrared-light photos are from Hubble's Wide Field Camera 3.

About the Object

  • R.A. Position
    R.A. PositionRight ascension – analogous to longitude – is one component of an object's position.
    03h 43m 50.99s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    32° 2' 48.0"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Perseus
  • 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.
    950 light-years (290 parsecs)

About the Data

  • Data Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.
    The image was created from Hubble data from proposal 12284: J. Muzerolle (PI; STScI) and collaborators. The science team comprises: J. Muzerolle (STScI), E. Furlan (NOAO and Caltech), K. Flaherty (Steward Obervatory), Z. Balog (Max Planck Institute for Astronomy, Heidelberg), and R. Gutermuth (University of Massachusetts, Amherst).
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>WFC3/IR
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    December 3 - 26, 2010
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F160W (H)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    LRLL 54361, L54361
  • Object Description
    Object DescriptionThe type of astronomical object.
    Protostar
  • Release Date
    February 7, 2013
  • Science Release
    Strobe-Like Flashes Discovered in a Suspected Binary Protostar
  • Credit
    NASA, ESA, J. Muzerolle (STScI), E. Furlan (NOAO and Caltech), K. Flaherty (University of Arizona/Steward Observatory), Z. Balog (Max Planck Institute for Astronomy), and R. Gutermuth (University of Massachusetts, Amherst)

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LRLL 54361 Light Echo – Hubble
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

The Hubble images were originally black and white and recorded only overall brightness. These brightness values were translated into a range of reddish hues. Such color "maps" can be useful in helping to distinguish subtly varying brightness in an image.

Compass and Scale
Compass and ScaleAn astronomical image with a scale that shows how large an object is on the sky, a compass that shows how the object is oriented on the sky, and the filters with which the image was made.

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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