Venus
Venus is a rocky planet orbiting the Sun, covered by thick clouds of carbon dioxide and sulphuric acid.
How big is it?
12,100 km across
Mean diameter · approximate
A little perspective
About the same scale as White dwarf.
White dwarf: 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.
Measurements, assumptions & sources +
Venus
Mean-radius spherical model for Venus; actual shape is not perfectly spherical.
NASA JPL — planetary physical parameters
The marked mean diameter is calibrated. Unmeasured illustration details are representative.
White dwarf
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 your perspective
Put it next to…
Choose a suggestion to redraw the comparison, or open its page to learn what it is.
Why this measurement?
Why we use 12,100 km
For comparison, this page uses mean diameter. This is labelled approximate; the central value is useful for comparison, while real values or measurement solutions can vary.
Mean-radius spherical model for Venus; actual shape is not perfectly spherical.
The marked horizontal span follows the named feature; transparent margins and unmeasured details do not alter it. How calibrated comparisons work →
Recorded properties
Venus dimensions and measurements
| Property | Selected value | Recorded range | Basis |
|---|---|---|---|
| 12,100 km | Not recorded | approximate | |
| 6,052 km | Not recorded | approximate | |
| 38,020 km | Not recorded | derived | |
| 460,200,000 km² | Not recorded | derived | |
| 9.284 × 10¹¹ km³ | Not recorded | derived | |
| 4.867 × 10²¹ t | Not recorded | approximate | |
| 8.87 m/s² | Not recorded | approximate | |
| 0.7233 AU | Not recorded | rounded orbital anchor | |
| 126,100 km/h | Not recorded | rounded orbital anchor |
Around this scale
Go smaller. Go bigger.
These links use compatible length records, ordered around the selected value.
Nearest lower value · SpaceWhite dwarf12,000 kmA 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.
Around the same scale · SpaceMars6,779 kmMars is a rocky planet orbiting the Sun, with a reddish surface due to iron oxide.
Nearest higher value · SpaceEarth12,740 kmEarth is the rocky planet on which we live and the third planet from the Sun.Sources and method
Want to check the number?
The source records and measurement method remain available for inspection.
- NASA JPL — planetary physical parametersMean radii and masses. Spherical area and volume here are derived from mean radius. This atlas rounds for scale comparison.
- NASA — Planet CompareConventional surface gravities; giant-planet values refer to an atmospheric reference level. Earth uses standard gravity, 9.80665 m/s².
- Defined examples — our methodology
More ways to see it
Curated comparisons
There’s always another scale
Follow your curiosity.
SpaceEarth12,740 kmEarth is the rocky planet on which we live and the third planet from the Sun.
SpaceMoon3,475 kmThe Moon is Earth’s natural satellite and the brightest large object in Earth’s night sky.
SpaceJupiter139,800 kmJupiter is a giant planet composed mainly of hydrogen and helium, orbiting the Sun beyond the asteroid belt.
SpaceSun1,391,000 kmThe Sun is the star at the centre of the Solar System.SpaceWhite dwarf12,000 kmA 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.SpaceMars6,779 kmMars is a rocky planet orbiting the Sun, with a reddish surface due to iron oxide.
SpaceGanymede5,262 kmGanymede is a natural satellite of Jupiter and contains a magnetic field generated by its partially liquid core.
SpaceTitan5,150 kmTitan is a natural satellite of Saturn, with a thick nitrogen-rich atmosphere and surface lakes of hydrocarbons.