Lacaille 9352

Lacaille 9352

Star

Lacaille 9352 — one of the closest and brightest red dwarfs, 10.7 light-years away in Piscis Austrinus. An M1V star about half the Sun's mass, it is unusually magnetically QUIET for a red dwarf, and it hosts a compact family of four confirmed planets found from its radial-velocity wobble.

Open in 3D viewSee Lacaille 9352 in the live, interactive 3D map

Key facts

Mass
9.85 × 10²⁹ kg
0.495 M☉
Radius
325,588 km
47% of the Sun's radius
Surface temperature
3,688 K (3,415 °C)
Luminosity
1.41 × 10²⁵ W
Spectral type
M1V (red dwarf)

Science

Physical

Mass
9.85 × 10²⁹ kg · 0.495 M☉
Radius
325,588 km · 47% of the Sun's radius
Density
6,810 kg/m³ · 6.8× water
Computed from mass and radius
Spectral type
M1V (red dwarf)

Motion through space

Proper motion
6.9 arcseconds per year · its drift across our sky
SIMBAD — 2020yCat.1350....0G, 2018A&A...616A...7S
Radial velocity
+8.8 km/s · moving away from the Sun
SIMBAD — 2020yCat.1350....0G, 2018A&A...616A...7S
Speed across our line of sight
107 km/s
Computed from proper motion and parallax
Speed through space, relative to the Sun
108 km/s
Computed from proper motion, parallax and radial velocity

Rotation

Note
Rotates slowly (tens of days) and flares little — quiet for a red dwarf.

Composition

By mass
A red dwarf about half the Sun's mass — one of the brightest and closest of its type. It is notably quiet magnetically, which helped make its four small planets detectable in the star's radial velocity.

Temperature

Surface
3,688 K (3,415 °C)

Radiation & temperature

Luminosity
1.41 × 10²⁵ W · 0.0368 L☉
Surface temperature
3,688 K (3,415 °C)
Peak wavelength
786 nm · near-infrared (mostly invisible to the eye)
Computed (Wien's law) from the surface temperature

Discovery & history

Discovered
1763
By
Nicolas-Louis de Lacaille
Method
Telescope
Name
Named for the French astronomer Nicolas-Louis de Lacaille and its number in his 1763 southern-sky catalogue. It is also GJ 887.

Recorded by Nicolas-Louis de Lacaille in his catalogue of southern stars (published 1763), as entry 9352. It has the sixth-largest proper motion of any star. In 2020 the RedDots/HARPS team announced two planets (b, c); two more (d, e) were confirmed in 2026 by Hartogh et al.

Images

Images from open archives · credit shown per image