Sun

1.39 million kmdiameter

Updated

1.39million km
Visual creditSolar Dynamics Observatory 2024 / NASA / SDO / HMI science team / Public domainSource: Wikimedia Commons

Details

The Sun is the star at the center of the Solar System and the source of almost all the energy reaching its planets. It fuses about 600 million metric tons of hydrogen each second, and energy released in the core takes on the order of 100,000 years to work its way out to the visible surface.

The Sun is a self-gravitating sphere of plasma containing more than 99.8% of the Solar System’s mass. Fusion in its core converts about 600 million metric tons of hydrogen into helium each second, with a small fraction of that mass released as energy.

Its visible photosphere is not a solid surface. The plasma rotates faster at the equator than near the poles, while changing magnetic fields produce sunspots, flares and coronal mass ejections that can affect satellites, power systems and auroras at Earth.

Key facts

Category
Stars
Object class
G-type main-sequence star
Mass
~333,000 Earth masses
Temperature
5,772 K surface
Scale fact
1.39 million kmdiameter
Estimated age
~4.6 billion years
Composition
Hydrogen and helium
Embed

Size neighbors

Objects near Sun on the scale

On the logarithmic size axis, Sun falls between 61 Cygni A and Sirius A. The band uses nearby Stars records.

Shared physical scale
7.95million km
Lalande 21185543,000 km
61 Cygni A925,000 km
Sun1.39 million km
Sirius A2.38 million km
Procyon A2.84 million km
Spica A10.4 million km

Sources

References for Sun

Measurements and descriptive context are compiled by the Scale of Space team from the references below. If you find an error, please let us know.

Continue with nearby objects or open the full scale.

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