Венера мен Галлей кометине арналған "Вега-1" ғарыш миссиясы

1984 Soviet uncrewed space mission to study Venus and Halley's Comet

Vega 1 (along with its twin Vega 2) was a Soviet space probe, part of the Vega program. The spacecraft was a development of the earlier Venera craft. They were designed by Babakin Space Centre and constructed as 5VK by Lavochkin at Khimki. The name VeGa (ВеГа) combines the first two letters from the Russian words for Venus (Венера: "Venera") and Halley (Галлея: "Galleya"). The craft was powered by twin large solar panels and instruments included an antenna dish, cameras, spectrometer, infrared sounder, magnetometers (MISCHA), and plasma probes. The craft was launched by a Proton 8K82K rocket from Baikonur Cosmodrome, Tyuratam, Kazakh SSR. Both Vega 1 and 2 were three axis stabilized spacecraft. The spacecraft were equipped with a dual bumper shield for dust protection from Halley's comet.

The descent module arrived at Venus on 11 June 1985, two days after being released from the Vega 1 flyby probe. The module, a sphere with a diameter of , contained a surface lander and a balloon explorer. The flyby probe performed a gravitational assist maneuver using Venus, and continued its mission to intercept the comet.

The Vega 1 Lander/Balloon capsule entered the Venus atmosphere ( altitude) at 2:06:10 UT (Earth received time; Moscow time 5:06:10 a. m.) on 11 June 1985 at roughly At approximately 2:06:25 UT the parachute attached to the landing craft cap opened at an altitude of The cap and parachute were released 15 seconds later at altitude. The balloon package was pulled out of its compartment by parachute 40 seconds later at altitude, at 8.1 degrees N, 176.9 degrees east. A second parachute opened at an altitude of , 200 seconds after entry, extracting the furled balloon. The balloon was inflated 100 seconds later at and the parachute and inflation system were jettisoned. The ballast was jettisoned when the balloon reached roughly and the balloon floated back to a stable height between some 15 to 25 minutes after entry. The mean stable height was , with a pressure of and a temperature of in the middle, most active layer of the Venus three tiered cloud system. The balloon drifted westward in the zonal wind flow with an average speed of about at nearly constant latitude. The probe crossed the terminator from night to day at 12:20 UT on 12 June after traversing The probe continued to operate in the daytime until the final transmission was received at 00:38 UT on 13 June from 8.1 N, 68.8 E after a total traverse distance of or about 30% of the circumference of the planet. It is not known how much farther the balloon traveled after the final communication.

After their encounters, the Vegas' motherships used the gravity of Venus, also known as a gravity assist, to intercept Halley's Comet. Images started to be returned on 4 March 1986, and were used to help pinpoint Giotto's close flyby of the comet. The early images from Vega showed two bright areas on the comet, which were initially interpreted as a double nucleus. The bright areas would later turn out to be two jets emitting from the comet. The images also showed the nucleus to be dark, and the infrared spectrometer readings measured a nucleus temperature of , much warmer than expected for an ice body. The conclusion was that the comet had a thin layer on its surface covering an icy body. Vega 1 made its closest approach on 6 March at around (at 07:20:06 UT) of the nucleus. It took more than 500 pictures via different filters as it flew through the gas cloud around the coma. Although the spacecraft was battered by dust, none of the instruments were disabled during the encounter. The data intensive examination of the comet covered only the three hours around closest approach. They were intended to measure the physical parameters of the nucleus, such as dimensions, shape, temperature and surface properties, as well as to study the structure and dynamics of the coma, the gas composition close to the nucleus, the dust particles' composition and mass distribution as functions of distance to the nucleus and the cometary solar wind interaction. The Vega images showed the nucleus to be about long with a rotation period of about 53 hours. The dust mass spectrometer detected material similar to the composition of carbonaceous chondrites meteorites and also detected clathrate ice. After subsequent imaging sessions on 7 and 8 March 1986, Vega 1 headed out to deep space. In total Vega 1 and Vega 2 returned about 1500 images of Comet Halley. Vega 1 ran out of attitude control propellant on 30 January 1987, and contact with Vega 2 continued until 24 March 1987. Vega 1 is currently in heliocentric orbit, with perihelion of 0.70 AU, aphelion of 0.98 AU, eccentricity of 0.17, inclination of 2.3 degrees and orbital period of 281 days.