NASA/JPL
Venus is almost the same size, mass and density as the Earth. Thus, it must generate heat within itself (due to the decay of radioactive elements) at almost the same rate as the Earth. On Earth, one of the main ways this heat escapes is through volcanic eruptions. On average, at least 50 volcanoes erupt annually.
But despite decades of searching, we haven’t seen clear signs of volcanic eruptions on Venus – until now. New research geophysics Robert Herrick University of Alaska Fairbanks, which he reported this week at the Lunar and Planetary Science Conference in Houston and published in the journal Sciencefinally caught one of the planet’s volcanoes in action.
It is not easy to study the surface of Venus because it has a dense atmosphere, including a continuous cloud layer at an altitude of 45-65 km, which is opaque to most wavelengths of radiation, including visible light. The only way to get a detailed view of the ground above the clouds is to use a radar pointing down from an orbiting spacecraft.
ISAS/JAXA
A technique known as aperture synthesis is used to create an image of a surface. This combines the varying strengths of ground-reflected radar echoes, including the time delay between transmission and reception, as well as small frequency shifts corresponding to whether the spacecraft is approaching or moving away from the source of a particular echo. The resulting image looks like a black and white photograph, except that the brighter areas generally correspond to rougher surfaces, and the darker areas generally correspond to smoother surfaces.

NASA/JPL
NASA’s Magellan probe orbited Venus from August 1990 to October 1994 and used such radar techniques to map the planet’s surface with a spatial resolution of about a hundred meters at best. It showed that more than 80 percent of the surface is covered in lava flows, but how the youngest of them erupted recently, and whether any eruptions are still ongoing today, remained a mystery for the next three decades.