Exploring Saturn’s Titan- a moon which may harbour life

Titan's atmosphere makes Saturn's largest moon look like a fuzzy orange ball in this natural color view from the Cassini spacecraft. Titan's north polar hood is visible at the top of the image, and a faint blue haze also can be detected above the south pole at the bottom of this view. This view looks toward the anti-Saturn side of Titan (3,200 miles, or 5,150 kilometers across). North is up. Images taken using red, green and blue spectral filters were combined to create this natural color view. The images were obtained with the Cassini spacecraft wide-angle camera on Jan. 30, 2012 at a distance of approximately 119,000 miles (191,000 kilometers) from Titan. Image scale is 7 miles (11 kilometers) per pixel.

In Brief

Titan is the largest moon of Saturn and the second-largest natural satellite in the Solar System. It is the only moon known to have a dense atmosphere, and the only known body in space, other than Earth, where clear evidence of stable bodies of surface liquid has been found. Interesting, isn’t it?

Discovery of Titan

Dutch astronomer Christiaan Huygens discovered Saturn’s largest moon, Titan, on March 25, 1655. It was over 250 years later, in 1944, when Dutch-American astronomer Gerard Kuiper discovered one of the characteristics that makes Titan exceptional: this distant moon actually has an atmosphere. Kuiper made the discovery by passing sunlight reflected from Titan through a spectrometer and detecting methane. Further telescope observations from Earth showed that Titan’s atmosphere was dense and hazy.

Exploration of Titan

The first spacecraft to explore Titan, Pioneer 11, flew through the Saturn system on Sept. 1, 1979. Astronomers on Earth had previously studied Titan’s temperature, and calculated its mass, and Pioneer 11 confirmed those characteristics. Because of Titan’s extended and opaque atmosphere, scientists at the time thought (incorrectly, it turns out) that Titan might be the largest moon in the solar system. Pioneer 11 also saw hints of a bluish haze in Titan’s upper atmosphere, which scientists predicted the Voyager spacecraft would be able to see.

When the Voyager 1 and 2 spacecraft voyaged through the Saturn system in 1980 and 1981, they couldn’t see Titan’s surface because of its dense atmosphere. However, images from that mission showed a featureless orange world and they did see the blue haze as a seemingly detached layer of Titan’s upper atmosphere. Just before Voyager 1 arrived in the Saturn system, some scientists speculated that the moon’s cold temperatures and methane meant that Titan might be home to oceans of liquid hydrocarbons. But the Voyager spacecrafts’ cameras were unable to penetrate Titan’s hazy atmosphere to get a complete view of the surface. Voyager did, however, reveal that Titan had traces of acetylene, ethane, and propane, along with other organic molecules, and that its atmosphere was primarily nitrogen, just like…..Earth.

Voyager 1 also finally provided a measurement of Titan’s surface temperature and air pressure, as well as the moon’s radius, revealing Titan to be the second largest moon in the solar system, not the largest, which is Jupiter’s Ganymede (both moons are larger than Mercury). The Voyagers also saw a distinct difference in brightness from north to south, which was presumed to be a seasonal effect—a presumption that was later confirmed.

In 1994, NASA’s Hubble Space Telescope recorded pictures of Titan using particular colors of infrared light that could pierce through the haze. The Hubble images showed large bright and dark areas, including bright region the size of Australia. The Hubble results didn’t prove that liquid seas existed, though, and the mystery about what was hidden below Titan’s haze remained until 2004.

The Cassini spacecraft, with the European Space Agency’s Huygens probe attached, became the first human-made object to orbit Saturn in 2004. Almost immediately, Cassini began observing Titan, peering through the haze for the first time. The Huygens probe detached from Cassini and parachuted through Titan’s atmosphere, landing on the surface on Jan. 14, 2005—the first landing of a probe in the outer solar system. Huygens collected images and atmospheric data during its descent as well as from the surface, and transmitted that data to Cassini, which relayed the data to Earth. Cassini performed 127 close flybys of Titan over 13 years, using a suite of tools, including radar and infrared instruments to peer through Titan’s haze and finally give scientists a detailed view of the moon’s surface and complex atmosphere. Cassini-Huygens discovered that Titan has clouds, rain, lakes and rivers of liquid hydrocarbons, as well as a subsurface ocean of salty water.

Source:

  1. NASA’s official website
  2. Oxford English Dictionary
  3. Wikipedia

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