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Hubble Spies Vast Gas Disk around Unique Massive Star

Hubble Spies Vast Gas Disk around Unique Massive Star

This visible-light image taken by NASA's Hubble Space Telescope reveals a pancake-shaped disk of gas around an extremely bright star in our Milky Way galaxy. The disk glows brightly in the light of ionized nitrogen.

The central star is nicknamed "Nasty 1," derived from its catalog name of NaSt1. Nasty 1 is thought to be a Wolf-Rayet star, a massive, rapidly evolving star weighing well over 10 times the mass of our sun. The star is losing its hydrogen-filled outer layers quickly, exposing its super-hot and extremely bright helium-burning core.

Nasty 1 is thought to have a companion, and gravitational interactions between them may have created the gas disk. Both stars are heavily obscured by gas and dust in the disk. Hubble observations suggest that as Nasty 1 sheds its weight, some of the mass is falling onto a companion star and some is leaking into space, forming the disk. The vast structure is nearly 2 trillion miles wide. The disk is clumpy because astronomers think the outbursts occur sporadically. The knot at left of center is an unusually bright clump of gas. The image is tinted blue to bring out details in the disk.

Astronomers were surprised to find the disk-like structure, which has never been seen before around a Wolf-Rayet star in our galaxy. The star may represent a brief transitory stage in the evolution of massive stars.

The Nasty 1 system may be as close as 3,000 light-years from Earth.

The observations were taken in April 2013 with the 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.
    18h 52m 17.55s
  • Dec. Position
    Dec. PositionDeclination – analogous to latitude – is one component of an object's position.
    00° 59' 44.28"
  • Constellation
    ConstellationOne of 88 recognized regions of the celestial sphere in which the object appears.
    Aquila
  • 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.
    Between 3,300 - 9,800 light-years (1 - 3 kpc) away

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.
    Data of WR 122 were obtained from the HST proposal 13034: J. Mauerhan (University of California, Berkeley), N. Smith (Steward Observatory/University of Arizona), and S. Van Dyk (IPAC/Caltech). The science team comprises: J. Mauerhan (University of California, Berkeley), N. Smith (Steward Observatory/University of Arizona), S. Van Dyk (IPAC/Caltech), K. Morzinski, L. Close, P. Hinz, and J. Males (Steward Observatory/University of Arizona), and T. Rodigas (Carnegie Institute of Washington).
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>WFC3/UVIS
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    April 27, 2013
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F645N (Continuum) and F658N ([N II])
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    NaSt1, Wolf-Rayet 122, WR 122
  • Object Description
    Object DescriptionThe type of astronomical object.
    Emission-line Star with Nebula
  • Release Date
    May 21, 2015
  • Science Release
    Hubble Observes One-of-a-Kind Star Nicknamed ‘Nasty’
  • Credit
    NASA, ESA, and J. Mauerhan (University of California, Berkeley)

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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