Travis Metcalfe

@travis-metcalfe.bsky.social

Astronomy researcher based in Colorado. I run a nonprofit adopt a star program to help fund astronomy research. #firstgen

This summer I spoke with science journalist Zack Savitsky, who wrote this in-depth article for NatGeo about our updated picture of magnetic stellar evolution, and what it means for understanding our own Sun and the chances of life in other solar systems. www.nationalgeographic.com/science/arti...

The Sun’s Magnetic Field is Behaving Oddly. Astronomers Still Don’t Know Why.

Scientists say our star might be in a midlife crisis of sorts. What does that mean for life?

nationalgeographic.com

Why are there so few points on this plot? Because we need: 👉 Stokes V snapshot with S/N~2000 (dipole field) 👉 existing measurement of Lx (mass-loss rate) 👉 existing measurement of rotation period All of this for stars near and below the solar activity level where WMB occurs. Help us add more points!

Observed torque relative to Skumanich-like model predictions versus Rossby number relative to the solar value. The functional form of the fit dotted line (90% confidence interval in gray) is predicted by the idea that the efficiency of the solar dynamo is currently collapsing (Hopf bifurcation; Cameron & Schussler 2017).

SNEAK PREVIEW: after the collapse of the global dynamo stalls main-sequence spin-down for billions of years, physical expansion on the subgiant branch finally allows stars to reach the transition to anti-solar DR (~1.1 Ro_crit), restoring the large-scale field and reviving magnetic braking!

Ratio of the observationally estimated and model wind braking torque as a function of Rossby number normalized to the solar value. The dotted line and gray shaded region illustrates the fit and 95% confidence interval described by Metcalfe+2025b. The revived magnetic braking in 31 Aql at higher Ro is evident, and quadratic growth is illustrated schematically with a dashed line.