Updated
Updated · Universe Today · Jul 9
New Paper Says Theta Eridani Shone 12 Times Brighter 2,000 Years Ago
Updated
Updated · Universe Today · Jul 9

New Paper Says Theta Eridani Shone 12 Times Brighter 2,000 Years Ago

2 articles · Updated · Universe Today · Jul 9

Summary

  • Theta Eridani was likely about V≈0.2 in antiquity versus V=2.9 today, a 2.7-magnitude gap that made it roughly 12 times brighter than it now appears.
  • Interferometric, spectroscopic and photometric data show the system is a triple star whose inner pair is a tight 0.083-AU binary, giving researchers the parameters needed to explain the anomaly.
  • The paper argues the primary star nearly filled its Roche lobe after core hydrogen burning, driving mass transfer and a long-lived common-envelope phase that extracted orbital energy and sustained centuries of extra brightness.
  • Ancient records from Hipparchus, Ptolemy and al-Sufi had long conflicted with modern observations; the authors say similar short-lived brightening phases may be common in close binaries and detectable in current surveys.

Insights

If a bright star faded over centuries, how many other 'forgotten' stars might be hiding in ancient astronomical records?
Can we now predict which of today's stars will be the next to flare up for a thousand years?
Why is the brief 'common envelope' phase so critical for the life and death of many binary stars?