
Sun
The Sun is the star at the centre of the Solar System.
1,391,000 kmDiameterWorlds apart
What are they, and what does the difference actually look like?
Two things. One honest scale.
Meet the pair

The Sun is the star at the centre of the Solar System.
1,391,000 kmDiameter
A neutron star is the dense remnant core left after a massive star explodes as a supernova, composed mostly of neutrons.
20 kmDiameterSun has about 69,600 times the diameter of Neutron star.
Our star, modelled with the IAU nominal solar radius. “Surface” means the visible photosphere. The core is much hotter; this is not a solid surface.
IAU — nominal solar and planetary conversion constants
The marked diameter is calibrated. Unmeasured illustration details are representative.
A 20 km, 1.4 solar-mass teaching model. The precise radius depends on stellar mass and the uncertain behaviour of dense matter.
The marked diameter is calibrated. Unmeasured illustration details are representative.
Change the comparison
Measurement details
The visual compares diameter with diameter. The records below preserve each value’s basis and caveats.
Diameter · approximate
Our star, modelled with the IAU nominal solar radius. “Surface” means the visible photosphere. The core is much hotter; this is not a solid surface.
Diameter · representative
A 20 km, 1.4 solar-mass teaching model. The precise radius depends on stellar mass and the uncertain behaviour of dense matter.
The labelled spans and stored measurements determine the scale; unmeasured illustration details do not.
There’s always another scale
Side by side







