Courtesy of the Jet Propulsion Laboratory and NASA's National Space Science Data Center
The spacecraft carried a sophisticated imaging radar, which was used to make the most highly detailed map of Venus ever captured during its four years in orbit around Venus from 1990 to 1994. After concluding its radar mapping, Magellan also made global maps of Venus's gravity field. Flight controllers then tested a new maneuvering technique called aerobraking, which uses a planet's atmosphere to slow or steer a spacecraft. The spacecraft made a dramatic plunge into the thick, hot Venusian atmosphere on October 12, 1994, and was crushed by the pressure of Venus's atmosphere. Magellan's signal was lost at 10:02 Universal Time (3:02 a.m. Pacific Daylight Time) that day.
The Magellan mission was divided up into "cycles" with each cycle lasting 243 days (the time necessary for Venus to rotate once under the Magellan orbit). The mission proceeded as follows:
04 May 1989 - Launch 10 Aug 1990 - Venus orbit insertion and spacecraft checkout 15 Sep 1990 - Cycle 1: Radar mapping (left-looking) 15 May 1991 - Cycle 2: Radar mapping (right-looking) 15 Jan 1992 - Cycle 3: Radar mapping (left-looking) 14 Sep 1992 - Cycle 4: Gravity data acquisition 24 May 1993 - Aerobraking to circular orbit 03 Aug 1993 - Cycle 5: Gravity data acquisition 30 Aug 1994 - Windmill experiment 12 Oct 1994 - Loss of radio signal 13 Oct 1994 - Loss of spacecraft
In all, the highly successful imaging radar mapped more than 98 percent of the planet's surface and collected high-resolution gravity data of Venus. The lessons learned from Magellan's aerodynamic dive into the Venusian atmosphere will be applied to future planetary missions.
On May 4, 1989, the Magellan spacecraft was deployed from the shuttle. The spacecraft is topped by a 3.7-meter (12-foot) diameter dish-shaped antenna that was a spare part left over from the Voyager program. The long, white, horn-shaped antenna, attached just to the left of the dish antenna, is the altimeter antenna that gathers data concerning the surface height of features on Venus. Most of the spacecraft is wrapped in reflective white thermal blankets that protect its sensitive instruments from solar radiation. (Courtesy NASA/JPL)
The Magellan spacecraft's deployment from the shuttle Atlantis' cargo bay was captured by an astronaut with a hand-held camera pointed through the shuttle's aft flight deck windows. Deployment occurred in the early evening of May 4, 1989, after Atlantis had carried Magellan and its Inertial Upper Stage (IUS) booster rocket, into low Earth orbit. Once the shuttle was safely away from the spacecraft, the IUS ignited and placed Magellan on course for its 15-month journey to Venus. (Courtesy NASA/JPL)
Magellan Orbiting Venus
On August 10, 1990, Magellan entered into orbit about Venus, as depicted in this artist's view. During its 243-day primary mission, referred to as Cycle 1, the spacecraft mapped well over 80 percent of the planet with its high-resolution Synthetic Aperture Radar (SAR). The spacecraft returned more digital data in the first cycle than all previous U.S. planetary missions combined. (Courtesy NASA/JPL)
Magellan Mapping Venus
The sequence of events that comprise a Magellan mapping orbit are shown in this artist's conception. For the first 37.2 minutes of each orbit, the Synthetic Aperture Radar measures and records a 20-kilometer (12-mile) wide swath of the planet's surface. When Magellan reaches the high point of its orbit, the spacecraft turns its antenna toward Earth and transmits the data. After 113.8 minutes of transmitting, the antenna is repositioned for another orbit about Venus. (Courtesy NASA/JPL)