Hubble Reveals V445 Puppis Fires 20 Million MPH Bullets as White Dwarf Feeds Again
Updated
Updated · Space.com · Jul 24
Hubble Reveals V445 Puppis Fires 20 Million MPH Bullets as White Dwarf Feeds Again
3 articles · Updated · Space.com · Jul 24
Summary
20 million mph gas clumps are blasting from V445 Puppis, Hubble observations showed after a dust cloud that hid the system for more than two decades finally cleared.
The new view identified the Milky Way’s only known helium nova as a white dwarf accreting helium-rich material from a rare stripped helium star companion.
Astronomers said the oxygen-rich “bullets” have not been seen in any other nova, making their origin a fresh mystery even after the system’s structure was pinned down.
The white dwarf is now feeding again, raising the prospect of another helium nova and offering a rare test case for how repeated eruptions might lead to a Type Ia supernova.
Could a rare star's strange 'bullets' rewrite our understanding of the universe's expansion?
What mysterious force is launching 20-million-mph oxygen bullets from an exploding star?
After 20 years of silence, is the Milky Way's rarest nova preparing to erupt again?
V445 Puppis: The Milky Way’s Only Helium Nova and Its Impact on Supernova Science
Overview
V445 Puppis is a unique helium nova in our galaxy, formed when helium-rich gas builds up on a white dwarf in a binary system. This accumulation leads to runaway helium burning and a powerful nova eruption, as seen in its dramatic 2000 outburst. Although once thought to be a possible precursor to a Type Ia supernova, recent research shows that V445 Puppis and similar helium novae do not become these supernovae, refining our understanding of stellar explosions. The eruption caused major changes in the system’s dynamics, drawing significant attention and offering new insights into rare cosmic events.