The surface of Venus is obscured by thick clouds of sulfuric acid which are opaque to visible light and cause acid rain to fall in the upper atmosphere. Below around 25 km above the surface, this acid rain evaporates, leaving a dense but transparent layer consisting mainly of carbon dioxide beneath.
The atmosphere on Venus is so thick that the pressure at the surface is equivalent to the pressure found half a mile under the sea on Earth. Venus is closer to the Sun than the Earth and carbon dioxide is a greenhouse gas, which traps the Sun’s heat, resulting in an average surface temperature of around 460 °C. The first probes sent to Venus were quickly destroyed by the high atmospheric pressure and heat.
- Type: Terrestrial
- Diameter: 12,104 km (0.95 Earths)
- Mass: 4.868×1024 kg (0.815 Earths)
- Distance from Sun: 0.728 AU to 0.718 AU
- Sidereal period (day length): 243 Earth days (retrograde)
- Orbital period (year length): 224.7 Earth days or 0.615 years
- Number of Moons: 0
- Symbol: ♀ (HTML code: ♀)
The Magellan probe, launched in 1989, produced a highly accurately radar map of the surface, from orbit above the clouds, which showed evidence of extensive volcanic activity.
Magellan also discovered a reflective substance on the peaks of high mountains, which is speculated to be metallic “snow” consisting possibly of tellurium or lead sulfide (galena).
Seen from Earth, Venus is the second brightest object in the night sky, after the Moon, and is so bright that it is often responsible for reported UFO sightings.
Depending on its position relative to the Sun, Venus is often know as the “morning star”, when visible in the early hours of morning, and the “evening star”, when visible in the early evening (personified by the half brothers Phosphorus and Hesperus, respectively, in Greek mythology).