— Ch. 1 · Program Origins And Design —
Vega program.
~4 min read · Ch. 1 of 5
The Soviet Union launched the first Vega spacecraft on the 15th of December 1984 from Baikonur Cosmodrome in the Kazakh SSR. This launch marked a strategic pivot for the Venera program after American Halley mission plans collapsed in 1981. Engineers at Babakin Space Center and Lavochkin at Khimki designed the craft as type 5VK vehicles to handle two distinct objectives simultaneously. The dual purpose required a redesignation of the project name to VeGa, combining the Russian words for Venus and Halley. A Proton 8K82K rocket propelled both identical sister ships into space with twin large solar panels powering their systems. Each probe carried an antenna dish, cameras, spectrometers, magnetometers, and plasma probes to gather data across vast distances. Dust protection was critical for the upcoming comet flyby, so engineers installed a dual bumper shield on every vessel. The second spacecraft followed four days later on the 21st of December 1984, creating a pair that would become part of the Halley Armada.
Venus Atmospheric Descent
Vega 1 arrived at Venus on the 11th of June 1985 while its sister ship Vega 2 reached the planet on the 15th of June 1985. Both vessels released spherical descent units some days before arrival without making active inclination changes during entry. These units contained landers and balloon explorers designed to study the atmosphere and surface conditions below. The Vega 1 lander suffered a catastrophic failure when a hard wind jolt activated its surface experiments prematurely from 30 kilometers above ground. It landed at coordinates 7.5°N latitude and 177.7°E longitude but provided no usable results due to the malfunction. The Vega 2 lander touched down successfully at 03:00:50 UT on the 15th of June 1985 in eastern Aphrodite Terra. Its touchdown site sat 600 meters above the planetary mean radius with measured pressure reaching 91 atmospheres. Temperature readings at this location hit 462 degrees Celsius despite the extreme environment. Surface samples revealed an anorthosite-troctolite composition that differed significantly from previous Venera findings. The successful lander transmitted data for exactly 56 minutes before silence fell over the dark side of Venus.