Fomalhaut

Fomalhaut

Star

Fomalhaut - the brightest star in Piscis Austrinus, 25 light-years away, a young white A-type star famous for the sharp, off-centre ring of dust around it, nicknamed the 'Eye of Sauron'. A point of light once thought to be a planet ('Fomalhaut b') turned out to be an expanding cloud of dust from a collision - so no planet is confirmed, but the ring itself is spectacular.

Open in 3D viewSee Fomalhaut in the live, interactive 3D map

Key facts

Mass
3.82 × 10³⁰ kg
1.92 M☉
Radius
1,280,088 km
1.84× wider than the Sun
Surface temperature
8,590 K (8317 °C)
Luminosity
6.37 × 10²⁷ W
Spectral type
A4V (white main-sequence star)

Science

Physical

Mass
3.82 × 10³⁰ kg · 1.92 M☉
Radius
1,280,088 km · 1.84× wider than the Sun
Density
435 kg/m³ · 0.43× water
Spectral type
A4V (white main-sequence star)

Composition

By mass
A young white main-sequence star (~440 million years old) about 1.9 times the Sun's mass and ~17 times its light, still surrounded by the debris of planet formation.

Temperature

Surface
8,590 K (8317 °C)

Radiation & temperature

Luminosity
6.37 × 10²⁷ W · 16.6 L☉
Surface temperature
8,590 K (8317 °C)
Peak wavelength
337 nm · ultraviolet (invisible to the eye)

Discovery & history

Method
Naked-eye star
Name
Its IAU proper name Fomalhaut is from the Arabic fam al-hut, 'the mouth of the fish'. It is Alpha Piscis Austrini, the brightest star of the Southern Fish.

Known since antiquity as a lonely bright star of autumn, Fomalhaut leapt to fame in 2008 when Hubble imaged a candidate planet inside its dust ring - one of the first exoplanets seen in visible light. By 2020 the 'planet' had faded and spread out, revealing it as debris from a smash-up of icy bodies; JWST in 2023 resolved the ring into nested belts.

Images

Images from open archives · credit shown per image