Why hasn’t the ‘Blaze Star’ exploded yet? Astronomers weigh in on what to expect
AI-summarised brief · reviewed before publication
Astronomers predict that the binary system T Coronae Borealis, a white dwarf accreting from a red giant, will erupt in a nova explosion within the next few years. The white dwarf has been gathering material for about 80 years, reaching a critical mass that triggers a dramatic flare. Experts note the difficulty of precise timing due to uncertain accretion rates and trigger mass, but observations suggest the event is imminent. The eruption will brighten the system from magnitude +10 to +1.7, visible to the naked eye for a brief period.
💡 Why It Matters
- · The impending nova offers a rare chance to study the physics of stellar explosions in real time, providing insights into mass transfer and accretion processes that shape binary evolution.