alarm-clock.org/solar

Venus

Earth's twin in size and mass, and in nothing else at all. Where it is right now, how big and how heavy, and what is still unexplained.

Jump to

Distances from the sun are in AU — one AU is the Earth’s average distance, 149,597,870 km — and the angle is where the body sits around its orbit, measured from the March equinox direction.

Venus by the numbers

Width12,104 km — 0.95× Earth
Mass4.867 × 10^24 kg — 0.815× Earth
Surface gravity8.87 m/s² — 0.91× Earth
Day243.0 Earth days (backwards)
Year224.7 Earth days
Distance from the sun0.723 AU on average — 0.72 to 0.73 AU
Sunlight takes6.0 minutes
Axial tilt177.4° — it is upside down
Temperature464 °C, and almost the same everywhere, day and night, poles and equator
MoonsNone
Atmosphere96.5% carbon dioxide at 92 times Earth's pressure, under permanent clouds of sulfuric acid

The mass is worked out from Venus’s gravitational parameter and the gravity from that and its radius; the year comes from Kepler’s third law and the width is the same figure the simulator draws with. None of them is typed in beside the picture, so none of them can disagree with it.

When Earth and Venus are next closest

Both planets are moving, so the gap between them swings enormously — and the closest approaches are not all equal, because the orbits are ellipses rather than circles. These are the next four, solved from the orbits rather than looked up.

October 25, 20260.273 AU — light takes 2.3 minutes
June 1, 20280.288 AU — light takes 2.4 minutes
January 5, 20300.265 AU — light takes 2.2 minutes
August 11, 20310.289 AU — light takes 2.4 minutes

Click a date to take the simulator there. These are minimum-distance moments, which fall near — but not exactly on — opposition.

Venus: things worth knowing

What we still don’t know about Venus

Every one of these is genuinely unsettled — not simplified for the page, not waiting on a textbook update.

Why does it spin backwards, and so slowly?

Either a giant impact flipped it, or the thick atmosphere did it: solar tides in an atmosphere that heavy, working against friction between core and mantle, can in principle turn a planet over and stall its spin without hitting it. The two histories are hard to tell apart from the outside, and the answer decides whether Venus was violently rearranged or just slowly wound down.

Did Venus ever have oceans?

Its deuterium-to-hydrogen ratio is about 150 times Earth's, which is the signature of a planet that has lost an enormous amount of ordinary water to space. How much, and when the last of it went — early, or as recently as a billion years ago — is unresolved, and the answer changes whether Venus was ever habitable.

Is anything happening in the clouds?

A 2020 claim of phosphine in the cloud deck, where the temperature is mild even though the surface is not, has been argued about ever since; later observations have both supported and failed to reproduce it, and there is no accepted abiotic or biological explanation. Treat it as an open measurement question, not as a discovery.

Recently learned about Venus

2023A reanalysis of Magellan radar images from 1990–92 found a volcanic vent that changed shape between two passes — the first direct evidence that Venus is volcanically active now, rather than in the past. Further flow features were identified in the same archive in 2024.
2020sThree missions have been approved to go back — DAVINCI (an atmospheric probe), VERITAS (radar mapping) and ESA's EnVision — after more than thirty years in which no dedicated mission was sent. Their launch dates have slipped repeatedly with budget cycles.

Findings reviewed August 2026. Space science moves; a date on a finding is part of the finding.

The rest of the system

Inward: Mercury. Outward: Earth. Or go back to the whole system, where every planet is on screen at once.

Make a link to a particular view

The date, the zoom, the span, the speed, the layers and any flight path are all in the address bar, so copying the URL shares exactly what is on screen. Set it up above, then take the link — it is the quickest way to hand a class one specific thing to look at.

The other simulator

This one is about the whole system. If the question is where the sun and the moon are from where you are standing — what time the sun comes up, why tonight's moon is the shape it is — that is the Sun, Earth & Moon movement simulator, which has a page for every city and a slider over a day, a week or a month.

Also: the classroom guide · sunrise & sunset by city · moon phase & moonrise · lunar eclipses · how the positions are worked out

Venus: questions without settled answers

Why does it spin backwards, and so slowly? Either a giant impact flipped it, or the thick atmosphere did it: solar tides in an atmosphere that heavy, working against friction between core and mantle, can in principle turn a planet over and stall its spin without hitting it. The two histories are hard to tell apart from the outside, and the answer decides whether Venus was violently rearranged or just slowly wound down.

Did Venus ever have oceans? Its deuterium-to-hydrogen ratio is about 150 times Earth's, which is the signature of a planet that has lost an enormous amount of ordinary water to space. How much, and when the last of it went — early, or as recently as a billion years ago — is unresolved, and the answer changes whether Venus was ever habitable.

Is anything happening in the clouds? A 2020 claim of phosphine in the cloud deck, where the temperature is mild even though the surface is not, has been argued about ever since; later observations have both supported and failed to reproduce it, and there is no accepted abiotic or biological explanation. Treat it as an open measurement question, not as a discovery.

💡 Question, problem or idea? Tell us →

Ask us anything about the tools, tell us what's broken or confusing, or suggest something we're missing. Every message is read by a person.

If you leave an email we'll reply to questions. We can't promise to build every suggestion, but they directly shape what we work on next.