The Cosmic Carousel Spawns Hot Jupiters ✛ ✦

Original: "Stellar Multiplicity of M Dwarfs with Short-period Giant Planets, and the Characterization of TOI-5628Ab"
arXiv:2607.10177 · 2026-07-11 · CC BY 4.0 · 1 min
Around dim red dwarfs with a distant partner, scorching giant planets are six times more common — like a carousel where a neighbor rocks the orbit.

A new study of 38 systems with hot Jupiters around red dwarfs has shown: every third one has a distant stellar companion. Among ordinary red dwarfs, pairs are found in only one out of twenty — a difference of 6.5 times. A typical example is TOI-5628Ab: a gas giant with a four-day year and a white dwarf neighbor. This is the cooled core of a star that swelled into a red giant only 530 million years ago; the planet survived the cataclysm.

The mechanism resembles a carousel: the distant companion, as if tugging on a rope, stretches the orbit into an ellipse. As the planet approaches the star, tidal forces slow it down, and it settles into a tight orbit — this is planetary migration, spurred by the neighbor's evolution. Calculations (spectroscopy and photometry) confirm: the process fits within 10 billion years. The star's composition doesn't matter.

Hot Jupiters were discovered in 1995 by Michel Mayor and Didier Queloz; the transit method, refined by David Charbonneau, helped find thousands of such planets.

The white dwarf in TOI-5628 cooled down only 530 million years ago, while its progenitor star lived for billions of years — the planet held on as its neighbor swelled into a red giant.

The TOI-5628 system is like Tatooine from Star Wars, but one of its two suns has already gone dark.

\frac{P(HJ|Comp)}{P(HJ)} = \frac{P(Comp|HJ)}{P(Comp)}
Odds ratio of finding a hot Jupiter given a distant companion versus without one. In this work, the ratio reaches 6.5—a real windfall for planetologists.
t_{\rm KL} \approx \frac{2}{3\pi} \frac{P_{\rm out}^2}{P_{\rm in}} \frac{M_*+M_p}{M_{\rm comp}} (1-e_{\rm out}^2)^{3/2}
Characteristic time for orbital rocking via the Kozai-Lidov mechanism: the farther and more massive the companion, the faster a planet turns its circle into a stretched ellipse and plunges toward the star.
Scientists
Christian DopplerD. B. McLaughlinDidier QuelozMichel MayorR. A. RossiterDavid Charbonneau
Concepts
exoplanets around red dwarfs red dwarf planets multi planet systems jupiter mass brown dwarf desert donor star hot jupiter atmospheres binary star dynamics binary stellar evolution asteroid belt planetary embryo trappist 1 stellar wobble starburst mass transfer mercury terrestrial exoplanet tidal migration interstellar object ejection pulsar companion