Venus
Venus — its permanent sulphuric-acid cloud deck shows almost no detail in visible light. Procedural illustration.
When to See It
Dates for your saved location. Venus spends about nine months on one side of the Sun, vanishes into its glare, then reappears on the other side.
The Evening & Morning Star
Diameter
12,104 km
Earth’s near-twin
One rotation
243 days
Longer than its year
Year
225 days
Spins backwards
Venus is the brightest object in the night sky after the Moon — dazzling enough to cast faint shadows and to be mistaken for a UFO. Beneath its serene glow hides a hellish world: a runaway greenhouse atmosphere of carbon dioxide crushes the surface at 90 times Earth’s pressure and holds it at 465°C, hot enough to melt lead.
Finding It
When Venus is in view it is unmistakable — the brilliant “star” blazing in the west after sunset or the east before dawn. Through a telescope it shows no surface markings, but it runs through phases like the Moon, from a small bright disc to a large thin crescent as it swings between us and the Sun.