
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 white dwarf is the dense, hot remnant core left behind after a star like the Sun has exhausted its nuclear fuel and shed its outer layers.
12,000 kmDiameterSun has about 116 times the diameter of White dwarf.
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 chosen 12,000 km, 0.6 solar-mass white dwarf. These remnants have roughly planetary dimensions but stellar masses.
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 chosen 12,000 km, 0.6 solar-mass white dwarf. These remnants have roughly planetary dimensions but stellar masses.
The labelled spans and stored measurements determine the scale; unmeasured illustration details do not.
There’s always another scale
Side by side







