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Nova in Binary Star System HM Sagittae (Artist’s Concept)
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 DateJune 10, 2024
- Science ReleaseNASA’s Hubble Finds Surprises Around a Star That Erupted 40 Years Ago
- CreditsNASA, ESA, Leah Hustak (STScI)
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Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov
NASA, ESA, Leah Hustak (STScI)