Gliese 588
Gliese 588 (GJ 588) is a red dwarf star of spectral type M2.5 in the constellation Lupus, about 19.3 light-years from the Sun. It is one of the nearest star systems and has been a target of radial-velocity planet searches, though no planet has been confirmed.
| Key fact | Detail |
|---|---|
| Spectral type | M2.5 V1 |
| Distance | 19.298 light-years (parallax 168.9965 mas)1 • 2 |
| Apparent magnitude (V) | 9.3112 |
| Mass | 0.46 solar masses (RECONS); 0.42 ± 0.20 M☉ from HARPS analysis1 • 3 |
| Effective temperature | about 3,440 K4 |
| Proper motion | −1176.447, −1030.970 mas/yr (RA, Dec)2 |
| Planets | None confirmed; 2019 candidates attributed to stellar activity3 |
Stellar properties
Gliese 588 is a main-sequence M dwarf, the most common type of star in the solar neighborhood. The RECONS census of the 100 nearest star systems lists it as an M2.5 V star with a mass of 0.46 solar masses at a distance of 19.298 light-years1. A homogeneous analysis of HARPS radial velocities describes it as an M2V-type star with a mass of 0.42 ± 0.20 M☉3. Its effective temperature is about 3,440 K4.
The star is a high proper motion star: SIMBAD lists proper motions of −1176.447 mas/yr in right ascension and −1030.970 mas/yr in declination, with a Gaia parallax of 168.9965 ± 0.0270 mas2. Its visual magnitude of 9.311 places it far below naked-eye visibility2.
Name and observation history
The name comes from Wilhelm Gliese, the German astronomer whose Catalogue of Nearby Stars (1957) numbered the nearby stars, a numbering still used for stars such as Gliese 380 and Gliese 7105.
Planet searches
In 2019, two planet candidates detected by the radial velocity (a star's motion toward or away from us, causing spectral shifts) method around Gliese 588 were reported in a preprint among 118 planets orbiting M dwarf stars.
A 2024 re-analysis of the HARPS radial velocities found no evidence for planets. Between 2003 and 2019, observations of the star spanned 64 nights; the measurements reveal a prominent signal at a 48-day period, near the 51.2-day rotation period inferred from the mean activity level, while the chromospheric data show peaks at 11, 27, 63, and 73 days plus longer-term signals around 340 days. The study concluded that the remaining signals, after subtracting a 7.02-day planetary signature, are most likely due to complex stellar activity rather than planets3.
References
- THE 100 NEAREST STAR SYSTEMS, RECONS
- GJ 588, SIMBAD basic data
- Mignon, L., et al. (2024). A&A, 689, A32
- The Nearest and Brightest Stars, activity sheet
- Ask Astro: Why are so many stars named Gliese?, Astronomy.com
Topic: Encyclopedia › Places and geography › Extraterrestrial places › Exoplanets and nearby star systems › Gliese and nearby red dwarf systems › Gliese-numbered systems
Initially written Oct 20, 2026 · Edited: Oct 25, 2026
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