do not follow here
News
Article

Magnetic field and potential planet candidates of the nearby Red dwarf Gliese 729

publication date1. 8. 2026

      
Magnetic field and potential planet candidates of the nearby Red dwarf Gliese 729
Star system: Ross 154 | Distance from the Sun: 9.7 light years
Gliese 729 (Ross 154) is the seventh closest Red dwarf to the Sun and serves as a significant subject for exoplanet research. Because Red dwarfs are typically very active, their magnetic fields can create noise that masks the subtle signals of orbiting planets. By analyzing a decade of data, the magnetic field of Gliese 729 has been mapped, revealing how its activity affects the search for small, rocky worlds in its vicinity.

The research utilized spectropolarimetric data—a technique that measures the polarization of light to reveal magnetic field structures—spanning four different time periods over 10 years. This allowed for the reconstruction of the star's large-scale magnetic field. The findings indicate that the magnetic field is relatively weak, ranging from 50 to 145 Gauss, and changes its shape over time, fluctuating between different geometric configurations.

To search for planets, the team analyzed radial velocity data, which tracks the tiny wobbles a star makes when tugged by the gravity of an orbiting planet. They used statistical modeling to account for stellar activity. While the models could not definitively confirm a planet, a repeating signal with a 7-day period and an amplitude of 1.9 meters per second was consistently identified. This signal might represent an Earth-mass or Super-Earth planet, though it could also be an artifact of the star's internal magnetic activity.

Key findings
- Gliese 729 exhibits a weak, evolving large-scale magnetic field ranging from 50 to 145 Gauss.
- Magnetic field geometry shifts between poloidal (north-south) and complex toroidal configurations.
- A 7-day period signal was detected in radial velocity data, which could indicate a low-mass planet or stellar noise.
- The results highlight the difficulty of distinguishing between planetary gravitational signals and magnetic activity in active Red dwarfs.
Generated by LLM, corrected by human

Share this discovery

Related themes

Stars mentioned

M3.5 V, Red dwarf
mass: 0.17 M☉
radius: 0.3 R☉
distance: 9.7 ly
stars in the system: 1
exoplanets: 0
Advertisement
Advertisement

study iconResearch with similar tags

line
Advertisement
Get your next news from nearby stars
Stellar Catalog brings the stars from our galaxy to you. Discover their position, physical properties and whether there are any exoplanets or disks orbiting them. The data in Stellar Catalog come from respectable sources like Gaia space telescope, or SIMBAD database.

Advertisement