Sun

Sun

Star

The Sun is the star at the centre of the Solar System — a nearly perfect sphere of hot plasma that holds 99.86% of the system's mass and supplies, through nuclear fusion in its core, essentially all the energy that drives the planets, weather and life.

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Key facts

Mass
1.99 × 10³⁰ kg
1 M☉
Radius
695,700 km
109× wider than Earth
Surface temperature
5,772 K (5499 °C)
Luminosity
3.83 × 10²⁶ W
Spectral type
G2V (yellow dwarf)

Science

Physical

Mass
1.99 × 10³⁰ kg · 1 M☉
Radius
695,700 km · 109× wider than Earth
Density
1,410 kg/m³ · 1.4× water
Spectral type
G2V (yellow dwarf)

Rotation

Equatorial period
25.0 days
Note
Differential rotation: ~25 days at the equator, ~35 days near the poles

Composition

By mass
~73.5% hydrogen, 24.9% helium and 1.6% heavier elements, by mass

Magnetism & activity

Surface field
1 gauss
Activity cycle
11 years

Temperature

Surface
5,772 K (5499 °C)
Core
15,700,000 K (15699727 °C)

Radiation & temperature

Luminosity
3.83 × 10²⁶ W · 1 L☉
Absolute bolometric magnitude
4.74
Surface temperature
5,772 K (5499 °C)
Peak wavelength
502 nm · green-yellow visible light
Surface magnetic field
100 µT

Discovery & history

First known
Known since antiquity
Name
Old English 'sunne'; Latin 'Sol', Greek 'Helios' — names as old as language itself.

The Sun has been known and worshipped for as long as humans have existed; it needed no discovery. Ancient cultures tracked its yearly path to build calendars and aligned monuments such as Stonehenge to its solstices. Only in recent centuries did we learn what it is: Galileo's telescope revealed sunspots in 1610, spectroscopy in the 19th century showed it is made of hydrogen and helium, and in the 1920s–30s physicists realised it shines by nuclear fusion in its core.

  1. 1994UlyssesObserved from afar

    First spacecraft to fly over the Sun's poles, sampling the solar wind out of the ecliptic plane.

Images

Images from open archives · credit shown per image