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Nova in Binary Star System HM Sagittae (Artist’s Concept)

An artist's concept of the symbiotic binary star system HM Sge on the black background of space sprinkled with varying sizes of red and white points of light. A white dwarf star (at top left)  is pulling a stream of gas from its dust-producing red giant companion (at bottom right). That gas forms a blazing hot disk around the white dwarf, which can unpredictably undergo a thermonuclear explosion as the infall of hydrogen from the giant grows denser on the surface until it reaches a tipping point.

This artist’s concept shows the nova system HM Sagittae (HM Sge), where a white dwarf star is pulling material from its red giant companion. This forms a blazing hot disk around the dwarf, which can unpredictably undergo a spontaneous thermonuclear explosion as the infall of hydrogen from the red giant grows denser and reaches a tipping point. These fireworks between companion stars are fascinating to astronomers by yielding insights into the physics and dynamics of stellar evolution in binary systems. 

  • Release Date
    June 10, 2024
  • Science Release
    NASA’s Hubble Finds Surprises Around a Star That Erupted 40 Years Ago
  • Credits
    NASA, ESA, Leah Hustak (STScI)

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Details

Last Updated
Mar 06, 2025
Contact
Media

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

Artwork Credit

NASA, ESA, Leah Hustak (STScI)