|True color picture of Saturn,
assembled from Voyager 2 images obtained Aug. 4, 1981
On August 25, 1981, American space probe Voyager 2 passed Saturn and transmitted stunning pictures of the ring planet. The space probe had been launched by NASA on August 20, 1977 to study the outer Solar System and eventually to push forward into interstellar space. Until today, operating for more than 30 years the spacecraft still receives routine commands and transmits data back to the Deep Space Network, a world-wide network of large antennas and communication facilities. Besides its passage of the Saturnian System, Voyager had already passed the Jovian system including Jupiter’s moons, and continued its journey encountering also the Uranian system in 1986, and the Neptunian system in 1989, after which the primary mission of Voyager 2 ended December 31, 1989. We already have dedicated an article to Voyager’s passage of Jupiter and the Jupiter moons. But, today’s article will focus on Saturn, the most extraordinary planet of our solar system.
Saturn is the sixth planet from the Sun and the second largest planet in the Solar System, after Jupiter, and is named after the Roman God of agriculture. Saturn is a gas giant with an average radius about nine times that of Earth. While only one-eighth the average density of Earth, with its larger volume Saturn is just over 95 times more massive than Earth.
Two weeks after the launch of Voyager 2, the twin Voyager 1 probe was launched on September 5, 1977. However, Voyager 1 would reach both Jupiter and Saturn sooner, as Voyager 2 had been launched into a longer, more circular trajectory through the Solar System. Saturn has a prominent ring system that consists of nine continuous main rings and three discontinuous arcs, composed mostly of ice particles with a smaller amount of rocky debris and dust. Known since prehistoric times, Saturn was the most distant of the five known planets in the solar system in ancient time. To discover Saturn’s rings it requires at least a 15-mm-diameter telescope and thus they were not known to exist until Galileo Galilei first saw them in 1610, when he directed his new telescope to the ring planet. But, Galileo first thought of the Ring to be two moons on Saturn’s sides. It was not until Christian Huygens used greater telescopic magnification that Saturn’s presumed moons were identified as a ring. Huygens furthermore discovered Saturn’s moon Titan. Italian astronomer Giovanni Domenico Cassini later discovered four other moons: Iapetus, Rhea, Tethys and Dione. In 1675, Cassini discovered the gap now known as the Cassini Division.
|Trajectory of Voyager 2 primary mission|
The first human built spaceprobe that pushed forward to Saturn was the Pioneer 11 flyby in September 1979. Pioneer 11 passed within 20,000 km of the planet’s cloud tops. Images were taken of the planet and a few of its moons, although their resolution was too low to recognize any surface detail. In November 1980, the Voyager 1 probe visited the Saturn system. It sent back the first high-resolution images of the planet, its rings and satellites. Voyager 1 also performed a close flyby of Titan, increasing knowledge of the atmosphere of the moon. Almost a year later, in August 1981, Voyager 2 continued the study of the Saturn system. More close-up images of Saturn’s moons were acquired, as well as evidence of changes in the atmosphere and the rings. Unfortunately, during the flyby, the probe’s turnable camera platform stuck for a couple of days and some planned imaging was lost. Actually, this put plans to officially extend the mission to Uranus and Neptune in jeopardy, but fortunately the mission’s engineers were able to fix the problem.
Voyager 2 found that at the uppermost pressure levels (seven kilopascals of pressure), Saturn’s temperature was 70 kelvins (?203 °C), while at the deepest levels measured (120 kilopascals) the temperature increased to 143 K (?130 °C). The north pole was found to be 10 kelvins cooler, although this may be seasonal. Moreover, The Voyager discovered and confirmed several new satellites orbiting near or within the planet’s rings, and also discovered the small Maxwell and Keeler gaps in the rings. Funally, Saturn’s gravity was used to direct the spacecraft’s trajectory towards Uranus.
The exploration of the Saturnian system did not end with Voyager 2. On July 1, 2004, the Cassini–Huygens spacecraft performed the SOI (Saturn Orbit Insertion) maneuver and entered into orbit around Saturn. Besides more in depth data about Saturn and its satellites, Huygens descended onto the surface of the Saturn moon Titan on January 14, 2005, sending a flood of data during the atmospheric descent and after the landing, while the Cassini part remained in orbit and gathered further data on Saturn, its rings and its satellites.
At yovisto you might learn more about the Voyager space program and the discovery of ouer outer solar system in a NASA special space science presentation on ‘Voyager – Humanity’s Farthest Journey‘.
References and Further Reading:
- Saturn profile at NASA’s Solar System Exploration site
- NASA Voyager website
- Voyager 2 Mission Profile
- Voyager 2 on Twitter
Related Articles in Yovisto Blog:
- To Boldly Go Where no Man has Gone Before – Voyager 2
- And yet it moves – Galileo Galilei and his major achievements
- Christian Huygens and the Discovery of Saturn Moon Titan
- Giovanni Cassini and the Saturn Moon Rhea
- The Arecibo Radio Telescope – Looking for Extraterrestrial Signals
- Eris – The Planet of Discord
- The Sputnik Shock
- A4 – The First Human Vessel To Touch Outer Space
- James van Allen and the Weather in Space
- The First Image from Abroad – Earth Rising and Lunar Orbiter 1
- Shoemaker-Levy 9 hits Jupiter
- The Eagle has Landed – The First Man on the Moon